Iraida Iacovleva () a fost o specialistă în anatomie patologică și oncologie din Rusia stabilită în Republica Moldova.

A absolvit Institutul de Medicină nr. 2 din Moscova. În anii 1948–1963 a lucrat în calitate de asistentă și docent la catedra de anatomie patologică a Institutului de Medicină din Chișinău, azi Universitatea de Stat de Medicină și Farmacie "Nicolae Testemițanu" din Republica Moldova. Ulterior, până în 1990, a fost șef de laborator patomorfologie la Institutul de Oncologie din Chișinău. Din 1990 a fost colaborator științific principal la aceeași instituție. În 1965 a devenit doctor habilitat în medicină, iar în 1967 profesor universitar. A fost membră a Societății Oncologilor din Moldova și membră de onoare a Societății de Anatomie Patologică din România.

Iraida Iacovleva a publicat peste 150 de lucrări de profil. A contribuit la cercetarea epiteliului colului uterin în raport cu vârsta, evidențierea de noi forme de neoplazii metaplastice din colul uterin, descrierea deosebirilor metastructurale ale epiteliilor pavimentoase autentice și metaplastice ale colului uterin etc.

A fost distinsă cu distincțiile sovietice Savant Emerit al RSSM (1967) și Ordinul Steagul Roșu (1971). În 2000, a fost decorată cu Ordinul Gloria Muncii de către Președintele Petru Lucinschi, iar în 2016 a fost menționată cu Medalia jubiliară a Academiei de Științe a Moldovei.

Referințe

Bibliografie

Nașteri în 1924
Nașteri pe 5 ianuarie
Decese în 2021
Medici moldoveni
Femei din Republica Moldova
Decorați cu Ordinul Gloria Muncii al Republicii Moldova

Iraida Iacovleva


خافي فينتا  (مواليد 13 ديسمبر 1975 في أوفييدو - إسبانيا) لاعب كرة قدم إسباني يلعب حاليا لصالح نادي الدرجة الأولى فياريال الإسباني منذ 1999 في مركز الظهير الأيمن .

روابط خارجية

مراجع

لاعبو كرة قدم رجالية إسبان مغتربون
أشخاص على قيد الحياة
أشخاص من سييرو (أستورياس)
رياضيون إسبان مغتربون في إنجلترا
لاعبو الأستورية
لاعبو الدوري الإسباني
لاعبو الدوري الإسباني الدرجة الثالثة
لاعبو الدوري الإسباني الدرجة الثانية
لاعبو الدوري الإسباني الدرجة الثانية ب
لاعبو برينتفورد
لاعبو دوري الدرجة الأولى الإنجليزي
لاعبو راسينغ فيرول
لاعبو كرة قدم إسبان
لاعبو كرة قدم إسبان مغتربون
لاعبو كرة قدم رجالية إسبان
لاعبو كرة قدم رجالية مغتربون في إنجلترا
لاعبو كرة قدم مغتربون في إنجلترا
لاعبو مارينو دو لوانكو
لاعبو نادي أوندا
لاعبو نادي تنريفه
لاعبو نادي فياريال
لاعبو نادي ليفانتي
مدافعو كرة قدم رجالية
مواليد 1975
مواليد في أوفييدو

خافي فينتا


Palazzo Marigliano, također poznata kao Palazzo di Capua je palača u renesansnom stilu u središnjem Napulju, Italija. Nalazi se na adresi Via San Biagio dei Librai broj 39.

Povijest

Palaču koju danas vidimo projektirao je Giovanni Donadio, poznat kao il Mormando, a izgrađena je u periodu 1512.-1513. Ova je palača zamijenila prethodnu zgradu koja je pripadala Bartolomeu di Capua, princu od Riccie i grofu od Altaville. Struktura je mijenjana tijekom godina.

Dvije mramorne ploče na ulaznom portalu podsjećaju na povijesne asocijacije palače.

 Constance Chiaramonte bila je kći Manfredija III Chiaramontea, gospodara Palerma. Udala se u Gaeti u dobi od 12 godina, za Ladislava od Durazza, koji je ubrzo postao kralj Ladislav Napuljski. Međutim, sudbina obitelji Chiaramonte se mijenjala: njezin otac je umro 1391., a njezinog brata uhvatile su i pogubile aragonske snage Martina I. od Aragona, koji se proglasio Martinom II. od Sicilije. Ovakvim preokretom sreće, Ladislav je papinim dekretom ishodio poništenje ili razvod, a 1392. je nadbiskup Gaete čak natjerao da crkveno objavi razvod braka i dobije vjenčani prsten. Constance je bila prisiljena udati se za 4. grofa od Altaville, Andrea di Capua, sina Bartolomea, i protonotara Kraljevstva, koji je boravio u ovoj palači. Na javnoj ceremoniji vjenčanja, Costanza je rekla da je proglasila svog mladoženju, da se ponosi što ima kraljevu ženu i kraljicu za konkubinu.
 Ova je palača bila mjesto susreta onih koji su bili uključeni, predvođeni Gaetanom Gambacortom, u neuspješnoj uroti Makija (Congioura di Macchia) 1701. koja se dogodila tijekom Ratova za španjolsko nasljeđe

Sredinom 1750-ih, palaču je obnovio Bartolommeo di Capua. Od Francesca de Mure naručio je freske za plesnu dvoranu, podsjećajući na pothvate svog istoimenog oca u borbama s napuljskim kraljem Karlom VII. (Španjolskim kraljem Karlom III.). U bitci kod Velletrija 1744., Bartolomeo stariji žrtvovao je svoj život dajući kralju konja. Djelo je teško oštećeno bombardiranjem tijekom 1942. Ostale slike unutar su alegorijske scene (1765.) Giovannija Battiste Maffeija.

S krajem obiteljske loze Capua kuća je pripala drugom sinu Sanserverina di Bisognana, grofa od Saponare. U 19. stoljeću prodali su palaču Francescu Saveriju Mariglianu, vojvodi od Montea. U dvorani oklopa zidovi su oslikani heraldičkim simbolima obitelji povezanih s obitelji Marigliano. Privatna kapela ima Maffeijevu fresku.

Danas veći dio palače zauzima Soprintendenza Archivistica della Campania.

Izvori
Posjetite Palazzo Marigliano

Vanjske poveznice

Renesansne palače u Napulju

Palazzo Marigliano


Biblioteca Națională a Republicii Cehe (în ) este biblioteca centrală a Republicii Cehe. Ea este administrată de Ministerul Culturii. Sediul principal al bibliotecii este situat în clădirea istorică Clementinum din Praga, unde sunt păstrate aproximativ jumătate din cărțile sale. Cealaltă jumătate a colecției este depozitată în districtul Hostivař. Biblioteca Națională este cea mai mare bibliotecă din Republica Cehă, având un fond de aproximativ 6 milioane de documente. Biblioteca are în jur de 60.000 de cititori înscriși. În afară de textele în limba cehă, biblioteca mai conține manuscrise mai vechi din Turcia, Iran și India. Biblioteca adăpostește, de asemenea, cărți ale Universității Caroline din Praga.

Biblioteca a dobândit o recunoaștere internațională în 2005, când a obținut Premiul Jikji al UNESCO prin intermediul Programului Memoria Lumii pentru eforturile depuse în digitalizarea textelor vechi. Proiectul, care a început în 1992, a implicat digitalizarea a 1.700 de documente în primii 13 ani.

Colecții
Cele mai prețioase manuscrise medievale păstrate în Biblioteca Națională sunt Codex Vyssegradensis și Viața stareței Cunigunda.

Clădirea nouă propusă

În 2006 Parlamentul Ceh a aprobat finanțarea construirii unei clădiri noi a bibliotecii în câmpia Letna, între stația de metrou Hradčanská și stadionul Letná al echipei de fotbal Sparta Praga. În martie 2007, în urma unei cereri de ofertă, arhitectul ceh Jan Kaplický a fost selectat de un juriu pentru realizarea proiectului, care urma să fie finalizat în anul 2011. Mai târziu, în cursul aceluiași an, proiectul a fost amânat în urma obiecțiilor cu privire la locația propusă pe care le-au formulat unii demnitari de rang guvernamental, inclusiv primarul Pragăi Pavel Bém și președintele Cehiei Václav Klaus. În februarie 2008 a fost sesizat Oficiul pentru Protecția Concurenței, în scopul de a determina dacă oferta lui Kaplický a câștigat în mod corect. Tot în 2008 ministrul culturii Václav Jehlička a anunțat sfârșitul proiectului, ca urmare a deciziei Comisiei Europene că procesul de licitație nu s-a desfășurat în mod legal.

Incidente
Biblioteca a fost afectată de inundațiile din Europa din 2002, iar unele documente au fost mutate la nivelurile superioare pentru a nu intra în contact cu apa în exces. Peste 4.000 de cărți au fost scoase din bibliotecă în iulie 2011, în urma inundării unor părți ale clădirii principale. Acolo a avut loc un incendiu în decembrie 2012, dar nimeni nu a fost rănit în acel incident.

Referințe

Legături externe

Cehia
Praga
Biblioteci din Cehia

Biblioteca Națională a Republicii Cehe


James William "Bill" Grant (born September 21, 1943) is an American banker and former politician from Madison, Florida. From 1987 to 1991, he served two terms in the United States House of Representatives.

Biography
A graduate of Florida State University, he  attended the University of Florida for graduate studies. He is a fifth generation Floridian whose family has lived in North Florida since before statehood. He is a former Member of the Florida State Senate and the United States Congress and his party's nominee to the U.S. Senate. Prior to beginning his political career, he organized and ran several North Florida commercial banks and was twice elected president of the Florida Bankers Association.

Congress
He represented  in the U.S. Congress from 1987 to 1991. After being elected as a Democrat from the Tallahassee-based 2nd District to succeed 12-term Democrat Don Fuqua, he switched parties to become a Republican on February 21, 1989.

He was defeated for reelection in U.S. House election, 1990 by Douglas Peterson, and ran unsuccessfully for the Senate in 1992, losing to incumbent Bob Graham.

Later career
After leaving politics, he organized and is now CEO of MK Meridian, Inc, an international conflict resolution, trade, and diplomatic advisory firm. In that capacity, he has mediated numerous sovereign and commercial conflicts across Eastern Europe, the Middle East and Africa. He helped organize the United Africa Association, a 13-nation effort for promoting pan-African self-help, free-enterprise capitalism, and democracy.

In 1997, with the assistance of the government of Egypt, he negotiated the end to the first Somali civil war and authored a draft constitutional government for that nation. He has been the senior advisor to two sovereign foreign governments and twice served as Special United States Congressional Envoy to international trouble spots. He served as Executive Vice President of Worldwide Chemical, LLC, a multi-faceted chemical production facility in Ukraine  with 11,000 employees and a worldwide market.

Family
Grant is married to the former Janet Krawiec; they have two children; Madison Kathleen and Kinsey Regan. He has two children from a previous marriage: John Alan and Carter Richmond.

See also
 List of American politicians who switched parties in office
 List of United States representatives who switched parties

External links

1943 births
American bankers
Florida State University alumni
Living people
People from Madison, Florida
University of Florida alumni
Florida Democrats
Republican Party members of the United States House of Representatives from Florida
Democratic Party members of the United States House of Representatives from Florida
Florida state senators
People from Lake City, Florida
Members of Congress who became lobbyists

James W. Grant


Gazel, Türkçe Divan edebiyatının en yaygın nazım şeklidir. Gazel sözcüğü sözlük tarifi ile  "kadınlarla sevgi üzerine konuşmak, söyleşmek" anlamina gelir.

Gelişmesi

Gazel Arapça edebiyatta bir nazım şekli değildir bir kasidenin başında bulunan aşktan, sevgiliden söz eden kısımlara verilen addır. Diğer bir adla "nesîb" olarak bilinir. Fakat sonraları bir şairin bahar, aşk, sevgili, şarap vb. coşkulu haller karşısındaki duygularını, kısa veya uzun olarak, ele alan şiirlere gazel denilmiştir. Arap şiirinde nesib anlamında kadın ve aşktan söz eden kaside şeklinde yazılmış şiirlere "tegazzül" denir.

Klasik Arap şiirinde gazel genel olarak üç başlık altında incelenmektedir. Bunlardan en önemlisi saf, temiz ve iffetli duyguların işlenmiş olduğu "'Uzrî Gazel"dir. Diğer ikisi ise "Sarih (Açık) Gazel" ve "Sınaî (Yapay) Gazel"dir. Her ne kadar Cemil b. Ma'mer'in ve Mecnunu Leylâ'nın öncülüğünü üstlendiği "'Uzrî Gazel" 2016 yılında dilimizde detaylı şekilde ele alındıysa da Arap gazelinin diğer iki kolu henüz Türkçede işlenmemiştir.

Islâmiyet'i kabulünden sonra İran'da Arap şiirinin etkisi altında oluşturulan "yeni İran edebiyatı" içinde gazel lirik şiirin en tercih edilen nazim şekillerinden biri olmuştur. Yeni İran şiirinde Arap edebiyatında kasidenin bir bölümü olan gazel Fars edebiyatında nazım şekli haline gelmiştir. Farsça gazel söyleyen ilk "Şehidi Belhi"'dir.

Batı Türkçesi ile ilk gazel 13.yy. ikinci yarısında ve Anadolu'daki ilk  menakıbname olan "Menakıbı Evhaduddini Kirmani" adlı eserdeki gazel ile Mevlana'ya ait gazeldir.

Yapısal terimler

Kafiye örgüsü "aa,ba,ca" şeklinde olur. İlk beyite "matla",  matladan sonraki beyite "hüsn-i matla"; son beyite "makta", maktadan önceki beyite "hüsn-i makta" denir. En güzel beyite "beyt'ül gazel" ya da "şah beyit" denilir. Şairin "mahlas"ının geçtiği beyite "Taç Beyit" ya da "tahallüs" denir. Matla mısrası gazelin sonunda tekrarlanırsa "reddi matla" denir. Matladan başka mısra tekrarlanırsa "reddi mısra" denir.

Bu uygulama Tanzimat döneminde yapılmıştır. "Sebki hint" şairleri iki matla kullanır. Böyle gazellere "zul metali" denir. Gazeldeki beyitler sadece kafiye, vezin değil anlam bakımından da birbirine bağlanmış ise buna yek ahenk denir. Bütün beyitler aynı güzellikte ise yek avaz denir. Mahlas beyitten sonra birkaç beyit eklenerek biri övülürse ona müzeyyel gazel denir. Arapça, Farsça, Türkçe ile karışık söylenmiş gazellere mülemma gazel denir. İki şairin birlikte veya beyit beyit söyledikleri gazele müşterek gazel denir. Matladan sonra gelen beyitlerin ortalarI ilk beyit ile kafiyeli ise musammat gazel denir.

Kafiyesine de iç "kafiye" denir. Musammat gazeller
mefâ'ilün mefâ'ilün mefâ'ilün mefâ'ilün ya da
Müstef'ilün / Müstef'ilün / Müstef'ilün / Müstef'ilün şeklinde yazılır. Her mısrada aks sanatı yapılmış gazellere "mükerrer gazel" denir.

Gazellerde beyit sayısı genellikle 5-15 arası değişir. Ortalama olarak gazel  beyit  5-7-9 arası yazılır. Gazeller her aruzun kalıbıyla yazılır.

Bir şairi aynı vezin ve kafiyeyle gazeline başka gazel yazmaya "tanzir" denir. Gazele de "naziri" denir. Eğer nazire ters anlamda yazılmışsa buna "nakize" denir.

Gazelde en çok aşk konusu işlenir. Rindlik, tasavvuf, şarap zevki diğer konulardır. Aşkla ilgili gazellere "aşıkane"; beşeri aşkı anlatan gazellere "şuhane"; yaşamdan zevk almayı anlatan gazellere "rindane"; gazel öğretici gazellere "hakimane" gazel denir.

Özellikleri

 Gazel, beyit denilen ikili dizelerden oluşur.
 Konusu genellikle liriktir.
 Gazelin beyit sayısı 5-15 arasında değişir. Daha fazla beyitten oluşan gazellere mutavvel gazel denilir.
 Gazeller eskiden bestelenerek okunurdu. Özelikle bestelenmek için yazılmış gazeller de vardır. Gazelleri makamla okuyan kişilere "gazelhan", gazel yazan usta şairlere ise "gazelsera" adı verilir.
 Gazel, Türk müziğinde ise şiirin bir hanende tarafından doğaçtan seslendirilmesidir. Sesle taksim olarak da bilinir.
 En güzel beytine beyt'ül gazel denir.
 Gazelin ilk beytine matla, matladan sonraki beytine hüsn-i matla; son beytine makta, maktadan önceki beytine hüsn-i makta, denir.<ref>"Dilbilimi.net" websitesinde  Divan Edebiyatı Nazım Biçimleri ve Türleri Online:  , Erişim tarihi: 31 Mayıs 2016</ref>

 Klasik Arap Edebiyatında Gazel
Klasik Arap edebiyatında gazel, şiirin en yaygın konularından biridir. el-Abbâs b. el-Ahnef, Kays b. Mulavvah, Ebû Nuvâs gazel söylemiş şairlerdendir.

 Konuyla ilgili yayınlar
Ayyıldız, Esat (2019). el-'Abbâs B. El-Ahnef: İdealize Edilmiş Ask Temalı Gazellerin Abbâsî Dönemindeki Özgün Bir Temsilcisi. Uluslararası Bilim, Teknoloji ve Sosyal Bilimlerde Güncel Gelişmeler Sempozyumu, 3, 209-216.

Ayyıldız, Esat (2016). Abbasî Dönemine Kadar 'Uzrî Gazel , Yüksek Lisans Tezi, Ankara.

 Kaynakça

 Dış kaynaklar

 Pala, İskender (1999 27.bas. 2016), Ansiklopedik Divan Şiiri Sözlüğü, İstanbul:Kapı Yayınları, ISBN 9758950218, Sayfa
 Dilçin, Cem (1983) Örneklerle Türk Şiir Bilgisi, Ankara:Türk Dil Kurumu Yayınları ISBN 9789751604897
 İpekten, Haluk (1994, 14.bas.2011), Eski Türk Edebiyatı Nazım şekilleri ve Arûz, İstanbul:Dergah Yayınları, ISBN 9759953539
 Muallim Nâci, (haz. M. A. Yekta Saraç), (2004) Edebiyat Terimleri: Istılahât-ı Edebiyye, İstanbul:
 Tural, Sadık Kemal (ed.) (2001, 2003, 2004, 2005, 2006), Türk Dünyası Edebiyat Terimleri ve Kavramları Ansiklopedik Sözlüğü 5 Cilt, Atatürk Kültür Merkezi Yayınları,  ISBN 3990000025722
 İsen, Mustafa; Macit, Mahsun; Horata, Osman; Kılıç, Filiz; ve Aksoyak, İ. Hakkı, (2002) Eski Türk Edebiyatı El Kitabı, İstanbul:Grafiker Yayınları  ISBN 9786054512232

 Dış bağlantılar

 İpekten, Haluk (1996) "Gazel", Türkiye Diyanet Vakfı İslâm Ansiklopedisi. c.13 say. 440-442'' Online:

Arap icatları

Gazel


Emmaste, Estonya'nın Hiiu iline bağlı dört kırsal kesim belediyesinden biridir. 197 kilometrekarelik yüzölçümü ile Emmaste, Hiiu'nun 40 km ötesinde yer alır. Baltık Denizi'ne kıyısı olan beldenin, %62'si ormanlar ile kaplıdır. Sayısı 1289 olan toplam nüfusun 289'u köylerde yaşar.

Hiiu (il)

Emmaste


1+1=2 er en kortfilm fra 2003 instrueret af Rum Malmros efter eget manuskript.

Handling
Det neurotiske overklasseløg Lise gør altid alting 2 gange, og køber altid 2 af alting. Men en dag er der kun 1 grapefrugt tilbage i supermarkedet; Lise's indkøbstur udvikler sig til et mareridt, da hun under jagten efter 2 grapefrugter forvilder sig ind i byens slumkvarter.

Referencer

Eksterne henvisninger

Kortfilm fra Danmark
Danske film fra 2003

1+1=2


Ottenbüttel Almanya'nın kuzeyinde Schleswig-Holstein eyaletinde, Steinburg iline bağlı yerleşim yeri. 10,04 km² yüzölçüme sahiptir. Nüfusu, 30 Eylül 2006 itibarıyla 755 olarak tespit edilmiştir. Belediye Başkanlığı Heinz Maaß tarafından yürütülmektedir.

Dış bağlantılar
 www.amtitzehoe-land.de

Steinburg iline bağlı yerleşim birimleri

Ottenbüttel


Dalaman Havalimanı (IATA: DLM, ICAO: LTBS) Muğla'nın Dalaman ilçesi sınırları içerisinde bulunan uluslararası havalimanı. Şehir merkezinin 6 km güneyinde yer alan havalimanı; Milas-Bodrum Havalimanı ile birlikte Muğla'ya hizmet veren iki uluslararası havalimanından biridir.

Tarihçe

Yapımına 1976 yılında başlanmış ve 1981 yılında hava meydanı olarak hizmete girmiştir. 1989 yılında yönetim kurulu kararıyla havalimanı statüsünü almıştır.

7 Mart 2014 tarihinde yapılan ihalede en yüksek teklifi 705 milyon Euro ile YDA Havalimanı Yatırım ve İşletme A.Ş. yaptı. İhale sonucunda YDA Havalimanı Yatırım ve İşletme A.Ş. 31 Aralık 2040 tarihine kadar havalimanının işletme hakkına sahip oldu.

Teknik özellikler

Günün 24 saati sivil ve askeri hava ulaşımına açık tutulan Dalaman Havalimanı CAT I (Kategori I) niteliklerine sahiptir.

Dalaman Hava Meydan Komutanlığı ile ortak kullanılan havalimanının güney ucunda askeri üs bulunmaktadır ve yedek hava limanı olarak kullanılmaktadır. Üs, 1. Hava Kuvveti Komutanlığı, Balıkesir 9. Ana Jet Üs Komutanlığına bağlıdır.

Toplam 9.343.000 m² kurulu alanı bulunan Liman, 2594 m² iç ve 21588 m² dış hat terminal binasına, 3000x45 m boyutlarında beton kaplamalı piste, 3000x30 m boyutlarında taksiruta ve 932x205 m boyutlarında 57 uçak kapasiteli bir aprona sahiptir.

Teknik Özellik Tabloları: https://www.dhmi.gov.tr/Sayfalar/Havalimani/Dalaman/TeknikBilgilerveKolayliklar.aspx

Terminal

Yeni dış hatlar terminali (Terminal 2)

2 Aralık 2003 tarihinde ihale edilen ve Ağustos 2004 tarihinde yapımına başlanılan Dalaman Havalimanı Yeni Dış Hatlar Terminal Binasının yapımını, normal süresinden 8 ay önce, 24 ay içerisinde tamamlanmış ve 1 Temmuz 2006 itibarı ile hizmete girmiştir. YDA Havalimanı Yatırım ve İşletme A.Ş. tarafından Yap-İşlet-Devret modeli ile işletilmekte olan Dalaman Havalimanı Yeni Dış Hatlar Terminali 95.000 m²'lik kapalı alanı ile eski dış hatlar terminalin 4 katı büyüklüğündedir. Dış Hatlar Terminali'ne ek olarak 210.000 m²'lik ek bir apron, 45.000 m²'lik ve toplam 950 araç kapasiteli bir otoparkı ile CIP ve VIP binaları bulunmaktadır.

 10 milyon yolcu/yıl kapasiteli,
 12 yolcu köprüsü,
 CUTE terminalleri ile donatılmış 87 check-in kontuarı,
 64 pasaport kontuarı,
 Bagaj Handling Sistemi ile entegre 5 seviyeli otomatik patlayıcı algılama sistemi

ve diğer kolaylıklara sahip olacak şekilde inşa edilmiştir. Yeni dış hatlar terminalinin devreye girmesiyle daha önce dış hatlar terminali olarak hizmet vermekte olan terminal, yenilenerek iç hat terminali olarak hizmet vermeye başlamıştır.

YDA Dalaman Dış Hatlar Terminali, ISO 9001 Kalite Belgesi, ISO 22000 Gıda Güvenliği, ISO/IEC 27001 Bilgi Güvenliği, ISO 14001 Çevre Belgesi, TS 13001 HACCP Gıda Güvenliği Belgesi, OHSAS 18001 İş Sağlığı ve Güvenliği Belgesi almaya hak kazanmıştır.

Havayolları ve uçuş noktaları

Düzenli/Yılboyu uçuşlar

Sezonluk uçuşlar

Charter uçuşlar

İstatistikler

Ulaşım

Dalaman havalimana ulaşım taksi ve otobüs işletmeleri tarafından sağlanmaktadır. Göcek'e 24 km, Fethiye'ye 50 km ve Marmaris'e 89 km uzaklıktadır.

Havaş ve MUTTAŞ servisleri, Dalaman Havalimanı'ndan Marmaris ve Fethiye merkezlerine karşılıklı seferlerle yolcu taşımaktadır. Dalaman Havalimanı'ndan şehir merkezlerine ulaşmak isteyen yolcular, Dalaman Havalimanı İç Hatlar Terminali çıkışında bulunan Havaş ve Muttaş servislerinden yararlanabilmektedir.

Dış bağlantılar

 Havaş Web Sitesi

Yer Hizmetleri

Dalaman Havalimanı'na sefer yapan havayolları, havayollarına hizmet veren yer hizmeti kuruluşları ve havayolları iletişim bilgilerine https://www.dalamanairport.aero/ucuslar/havayollari/  adresinden ulaşabilmektedir.

Dış bağlantılar

 TGS Web Sitesi
 Havaş Web Sitesi

Kaynakça

Dış bağlantılar
YDA Dalaman Havalimanı  Resmi Web Sitesi
 Google Harita - Uydu Görüntüsü

Türkiye'deki havalimanları
Muğla ilindeki altyapı
Muğla ilinde ulaşım
Havalimanı
1981'de kurulan havalimanları
1981'de Türkiye'de kurulan oluşumlar

Dalaman Havalimanı


Violetas imperiales es una coproducción hispanofrancesa dirigida por Richard Pottier y estrenada el 12 de diciembre de 1952, protagonizada por Carmen Sevilla y Luis Mariano. Existen dos versiones anteriores anteriores de esta misma historia, protagonizadas ambas por Raquel Meller en 1923 (muda) y 1932 (cine sonoro).

Argumento
Violeta (Carmen Sevilla) es una humilde gitana granadina que augura por azar tras leerle la mano a la joven Eugenia de Montijo (Simone Valère) que a ésta le espera subir a un trono. Cuando Eugenia, tras su boda con Napoleón III se instala en París, no duda en contratar a Violeta como su asistenta privada. Allí la joven se enfrenta a los avances amorosos de Juan de Ayala (Luis Mariano), primo de la emperatriz.

«Inspiración» para Dalí
En 1938 el pintor Salvador Dalí dio el título Violetas imperiales a uno de sus cuadros surrealistas. Por cronología, hubo de referirse a alguna de las dos películas de Raquel Meller. Este cuadro fue adquirido en 2015 por la Fundación Gala-Salvador Dalí de Figueras.

Enlaces externos
 Ficha en Hoycinema
 Ficha en Filmaffinity

Películas de Francia
Películas españolas ambientadas en el siglo XIX
Películas ambientadas en Granada
España en 1952
Películas de Carmen Sevilla
Películas ambientadas en los años 1850
Películas ambientadas en París
Representaciones culturales de Napoleón III

Violetas imperiales


Der Mählbrief, Maalbrief oder auch Zerte ist die Urkunde über den Bauvertrag eines Handelsschiffes. Bis etwa 1900 verlangten z. B. die russischen Hafenbehörden beim Einklarieren eines ausländischen Kauffahrteischiffes vom Kapitän neben anderen Schiffspapieren auch die Vorlage des amtlich beglaubigten Mählbriefes.
In dem Dokument mussten außer Gattung, Abmessungen und Tonnage des Schiffes die Zahlungsmodalitäten zwischen Reeder und Bauwerft angegeben sein. Außerdem mussten der Ort und Zeitpunkt der Kiellegung, der Tag des Stapellaufs und der Fertigstellung sowie Zeitpunkt und Ort der Schiffsübergabe an den Reeder enthalten sein. Wie auch aus dem Schiffszertifikat mussten aus dem Mählbrief die Eigentumsverhältnisse an dem Schiff zur Zeit des Einklarierens für die Abfertigungsbehörden ersichtlich sein.

Literatur
 Carl Th. von Soden und Henry A. Tobiesen, "NAUTA" Prakktisches Handbuch für Seefahrer, Rheder und Kaufleute, Verlag P.Salomon & Comp. Hamburg 1854

Siehe auch
 Beilbrief

Einzelnachweise

Recht in der Schifffahrt

Mählbrief


est un genre éteint d'acritarches, des microfossiles à paroi organique auxquels il n'est pas possible d'attribuer une affinité biologique avec certitude (on les regroupe dans les Biota incertae sedis).

Les espèces datent de l'Ordovicien.

Liste des espèces
 †Cheleutochroa beechenbankensis Richards & Mullins, 2003
 †Cheleutochroa diaphorosa Turner, 1984
 †Cheleutochroa differta Uutela & Tynni, 1991
 †Cheleutochroa elegans Uutela & Tynni, 1991
 †Cheleutochroa gymnobrachiata Loeblich & Tappan, 1978
 †Cheleutochroa homoia Turner, 1984
 †Cheleutochroa meionia Turner, 1984
 †Cheleutochroa oculata Uutela & Tynni, 1991
 †Cheleutochroa ramosa Uutela & Tynni, 1991
 †Cheleutochroa rugosa Uutela & Tynni, 1991
 †Cheleutochroa tuberculosa Uutela & Tynni, 1991
 †Cheleutochroa venosa Uutela & Tynni, 1991
 †Cheleutochroa venosior Uutela & Tynni, 1991

Liens externes

  AR Loeblich Jr et H Tappan, Some middle and late ordovician microphytoplankton from Central North America, Journal of Paleontology, 1978 (lien sur JSTOR).
  Cheleutochroa sur le site Fossiilid.info (site visité le 31 mars 2022).
  Cheleutochroa sur le site Palynodata (site visité le 31 mars 2022).

Notes et références

Acritarcha
Genre d'eucaryotes préhistoriques (nom scientifique)
Taxon éteint de l'Ordovicien
Taxon fossile non connu en Paleobiology Database
Taxon fossile décrit en 1978

Cheleutochroa


Alain Filhol, né le  à Toulouse, est un ancien pilote automobile français.

Carrière
Alain Filhol a commencé sa carrière en course automobile en 1995 en Formule 3000. Cependant, il ne réussit à marquer de points dans aucune des deux courses auxquelles il participe et se classe à la  place du championnat. Au cours des années suivantes, il a concouru en Porsche Carrera Cup française, en Championnat FIA GT, en Championnat de France FFSA GT, en Championnat de France des voitures de tourisme (où il a notamment piloté une Nissan Primera), aux 24 Heures du Mans et aux Le Mans Series.

Résultats aux 24 Heures du Mans

Liens externes

Notes et références

Pilote automobile français
Pilote des 24 Heures du Mans
Naissance à Toulouse
Naissance en mai 1951

Alain Filhol


Ryke Geerd Hamer (), un fost medic german, a inițiat "Noua Medicină Germanică", anterior cunoscută sub numele de "Noua Medicină Germană" și "Noua Medicină", un sistem de pseudo-medicină, care pretinde a fi capabilă de a vindeca cancerul. Liga Elvețiană (Anti-)Cancer a descris abordarea lui Hamer ca fiind "periculoasă, mai ales că induce pacienților un sentiment de securitate  fals și astfel că ei sunt lipsiți de alte tratamente eficiente".

Hamer a avut licență de a practica medicina din 1963 până în 1986, când i-a fost revocată pentru malpraxis. Sistemul lui Hamer a ajuns în atenția publicului în 1995, când părinții unui copil care suferea de cancer au refuzat tratamentul medical în favoarea metodei Hamer. Hamer a fost acuzat și condamnat la închisoare în mai multe țări europene: 19 luni în Germania și din septembrie 2004 până în februarie 2006 închis la pușcăria din Fleury-Mérogis.

Hamer a susținut că metoda sa este o alternativă "germanică" la medicina clinică, care ar face parte dintr-o conspirație evreiască de decimare a non-evreilor.

Presa a raportat de multe ori despre victimele pe care le-a făcut Hamer.

Referințe

Legături externe
 Noua Medicină Germană: o năzbâtie periculoasă, 17 august 2017, Cristian Român, stiintasitehnica.com

Nașteri în 1935
Medici germani din secolul al XX-lea
Medicină alternativă
Teoreticieni ai conspirației
Decese în 2017

Ryke Geerd Hamer


رامى شعبان (-6-1975 -)، ولد في السويد من أب مصري وأم فنلندية، لاعب كرة قدم يلعب في مركز حراسة المرمى.

عن اللاعب

ولد رامى شعبان في مقاطعة فيسكساترا في السويد بالعاصمة السويدية ستوكهولم في ال 30 من يونيو لعام 1975...وبدأ ممارسة الكرة في النادي المحلبFisksätra IF..وكان أول ظهور له مع الفريق عندما بلغ التاسعة عشر وذلك عندما شارك مع فريقه عام 1994..ثم عاد رامي إلى القاهرة من أجل دراسته الجامعية وفي هذه الأثناء لعب لنادي الزمالك في عام 1995 وشارك في 5 مباريات.. ونظرا لعدم الاقتناع بمستواه انتقل اللاعب ولعب لنادي اتحاد عثمان (نادي مزارع دينا حالياً) وشارك في حوالي 5 مباريات في الفترة من عام (95..96)..

ثم عاد إلى السويد وشارك مع نادي ناكا في الدرجة الثالثة قبل أن يلعب ديرجارديز الذي أحرز معه بطولة الدرجة الثانية ثم الوصيف في الدرجة الأولى في الموسم الذي يليه عام 2002، وفي أغسطس من عام 2002..انتقل رامي شعبان إلى نادي Arsenal الإنجليزي في ظل بحث النادي عن حارس بديل للدولي الإنجليزي الشهير ديفيد سيمان والذي أعلن اعتزاله عقب مونديال 2002...
وشارك رامي في بعض مباريات الدوري الإنجليزي وكذلك مباريات الشامبيونز لييج ضد أيندهوفين والتي انتهت بالتعادل السلبي وأظهر مستوى جيد ومنها مباراته أمام روما في الاستاد الأوليمبي بروما..

ولكن كانت مشاركاته مع المدفعجية محدودة نظرا لكثرة إصاباته.. فبعد أن شارك بصفة أساسية في عدة مباريات مع الأرسنال أصيب بكسر في القدم في إحدى تدريبات الفريق عشية الكريسماس وهو ما أبعده فترة طويلة عن الملاعب امتدت لعدة شهور.., ورغم ذلك تمسك مسؤولو أرسنال به حتى تم علاجه.. إلى أن عاد من الإصابة فقام الأرسنال في يناير من عام 2004 بإعارته لمدة شهر واحد إلى نادي West Ham United الإنجليزي ولم يشارك معهم في أي مباراة.

وفي فبراير 2004..انضم رامي إلى نادي Brighton & Hove Albion الذي يلعب في دوري الدرجة الثانية الإنجليزي وشارك معهم في 6 مباريات وكان أول ظهور له أمام فريق Sunderland ساهم مع فريقه بالفوز 2-1..وبعد انتهاء عقده مع الفريق انتقل رامي في صفقة انتقال حر إلى نادي Fredrikstad F.K النرويجي وشارك معهم في 11 مباراة منذ انتقاله صيف 2006 وانتقل اللاعب مؤخرا إلى نادي هاماربي السويدي عام 2008 وهو النادي ذات الشعبية الأولى في ستوكهولم وفي السويد كلها ويدافع رامي عن ألوان النادي الخضراء والأبيض بصفة غير أساسية.

-استدعي رامي إلى منتخب السويد لأول مرة مع القائمة التي ستذهب لمونديال ألمانيا 2006 على الرغم من عدم مشاركته في أي مباراة دولية من قبل.. وشارك في مباراة إعدادية للمونديال أمام منتخب فنلندا (منتخب والدته) كاحتياطي ونزل بديلاً في الشوط الثاني وحافظ على نظافة شباكه لتنتهب المباراة 0-0

-وفى 10 يونيو 2006 شارك رامي أساسيا في كأس العالم في المباراة الافتتاحية التي جمعت السويد بترينداد وتوباجو والتي انتهت بالتعادل السلبي 0-0

-وحتى الآن., شارك رامي في 4 مباريات رسمية مع السويد في التصفيات المؤهلة لنهائيات امم أوروبا 2008 ومنها مباراة إسبانيا والتي انتهت بالتعادل السلبي 0-0

-شارك رامي مع المنتخب السويدي في 11 مباراة دولية حتى الآن نذكر منها مباراته أمام المنتخب المصري في فبراير الماضي والتي انتهت بفوز منتخب مصر 2-0.

الالقاب
-12/نوفمبر :- كأس النرويج مع Fredrikstad لأول مرة منذ 22 عام 3- 0 على Sandefjord

-13/نوفمبر :-أفضل حارس مرمى سويدي لعام 2006 .

مراجع

وصلات خارجية

لاعبو كرة قدم رجالية سويديون
لاعبو كرة قدم رجالية سويديون مغتربون
لاعبو كرة قدم رجالية مغتربون في النرويج
لاعبو كرة قدم رجالية مغتربون في إنجلترا
حراس مرمى كرة قدم رجالية
أشخاص على قيد الحياة
رياضيون سويديون مغتربون في إنجلترا
رياضيون سويديون من أصل إفريقي
رياضيون من ستوكهولم
سويديون من أصل فنلندي
سويديون من أصل مصري
لاعبو الدوري الإنجليزي الممتاز
لاعبو الدوري السويدي لكرة القدم الدرجة الأولى
لاعبو الدوري المصري الممتاز
لاعبو الدوري النرويجي الممتاز
لاعبو برايتون أند هوف ألبيون
لاعبو بطولة أمم أوروبا 2008
لاعبو دوري الدرجة الأولى الإنجليزي
لاعبو ديبورتيس تيموكو
لاعبو كأس العالم 2006
لاعبو كرة قدم سويديون
لاعبو كرة قدم سويديون مغتربون
لاعبو كرة قدم مغتربون في النرويج
لاعبو كرة قدم مغتربون في إنجلترا
لاعبو كرة قدم مغتربون في تشيلي
لاعبو كرة قدم من ستوكهولم
لاعبو منتخب السويد تحت 21 سنة لكرة القدم
لاعبو منتخب السويد لكرة القدم
لاعبو نادي آرسنال
لاعبو نادي الزمالك
لاعبو نادي فريدريكستاد
لاعبو نادي كوكيمبو أونيدو
لاعبو نادي هاماربي
لاعبو نادي يورغوردينس
لاعبو وست هام يونايتد
مواليد 1395 هـ
مواليد 1975
مواليد في ستوكهولم

رامي شعبان


Kejsergås () er en andefugl, der lever i det østlige Sibirien og det vestlige Alaska.

Noter
 Avibase - the world bird database

Eksterne henvisninger

Fugle fra Alaska
Fugle fra Nordasien
Gæs

Kejsergås


ගණිතය හෝ පරිගණක විද්‍යාවේදී,

"ඇල්ගොරිතමයක් යනු නිශ්චිත ගැටළු පන්තියක් විසඳීමට හෝ ගණනය කිරීමක් සිදු කිරීමට සාමාන්‍යයෙන් භාවිතා වන හොඳින් අර්ථ දක්වා ඇති උපදෙස්වල සීමිත අනුපිළිවෙලකි."

ඇල්ගොරිතම් ගණනය කිරීම්, දත්ත සැකසීම, ස්වයංක්‍රීය තර්කනය, ස්වයංක්‍රීය තීරණ ගැනීම සඳහා භාවිතා වේ.

ඉතිහාසය

අවිධිමත් අර්ථ දැක්වීම

විධිමත් කිරීම
පරිගණක දත්ත සැකසීමට ඇල්ගොරිතම අත්‍යවශ්‍ය වේ. බොහෝ පරිගණක වැඩසටහන් වල පරිගණකයක් ඉටු කළ යුතු නිශ්චිත උපදෙස් විස්තර කරනුයේ ඇල්ගොරිතම භාවිතයෙනි.

ඇල්ගොරිතම ප්රකාශ කිරීම
ඇල්ගොරිතම ප්රකාශ කිරීම පහත පරිදි පිළිගත් මට්ටම් තුනකට වර්ග කළ හැක.

 ඉහළ මට්ටමේ විස්තරීකරණය
 ක්රියාත්මක කිරීම විස්තරීකරණය
 විධිමත් විස්තරීකරණය

නිර්මාණය කිරීම
ඇල්ගොරිතම නිර්මාණය යනු, ගැටළු විසඳීම සහ ඉංජිනේරු ඇල්ගොරිතම සඳහා ක්‍රමයක් හෝ ගණිතමය ක්‍රියාවලියක් ගොඩනැගිමයි. ඇල්ගොරිතම නිර්මාණයේ වැදගත්ම අංගයක් වන්නේ ඇල්ගොරිතම තුළදී සම්පත් කාර්යක්ෂමතාව(ධාවන කාලය, මතක භාවිත ප්‍රමාණය) භාවිතා වීමයි.

ඇල්ගොරිතම සෑදීමේ සාමාන්ය පියවර:

01. ගැටළු නිර්වචනය.

02. ආකෘතියක් සංවර්ධනය කිරීම.

03. ඇල්ගොරිතමයේ පිරිවිතර ගොඩනැගිම.

04. ඇල්ගොරිතමයක් නිර්මාණය කිරීම.

05. ඇල්ගොරිතමයේ නිවැරදි බව පරීක්ෂා කිරීම.

06. ඇල්ගොරිතම විශ්ලේෂණය.

07. ඇල්ගොරිතම ක්රියාත්මක කිරීම.

08. වැඩසටහන පරීක්ෂා කිරීම.

09. ලේඛන(Documentation) සකස් කිරීම.

ඇල්ගොරිතම්


Experimentul București este un film românesc din 2013 regizat de Tom Wilson. Rolurile principale au fost interpretate de actorii Carmen Anton, Daniel Bilt, Andrei Juvina.

Prezentare

Distribuție
Distribuția filmului este alcătuită din:

Note

Legături externe

Vezi și
 2013 în film

Filme românești
Filme în limba română
Filme din 2013
Filme documentare românești

Experimentul București


Giampaolo Lomi (* 4. Februar 1930 in Livorno; † 18. August 2021 in Foligno) war ein italienischer Filmschaffender.

Leben
Lomi nahm 1956 an einer Amazonas-Expedition als Kameratechniker teil, blieb in Brasilien und drehte dort einige Dokumentarfilme. Am Theater assistierte er Adolfo Celi, organisierte europäische Produktionen in Südamerika und inszenierte einige Kurzfilme für regionale Fernsehstationen. Er arbeitete in den 1960er und zu Beginn der 1970er Jahre bei zwei Mondo-Filmen mit Gualtiero Jacopetti und bei einem Film mit John Frankenheimer zusammen und drehte mit Edoardo Mulargia als Koregisseur einen Giallo im Jahr 1972. Nach einer Komödie, I baroni (1975), folgte sein letzter für das Kino gedrehter Film, der Dokumentarstreifen Il vescovo del silenzio über den umstrittenen Bischof Marcel Lefebvre.

Lomi gründete und leitete lange Jahre auf den Philippinen das Internationale Filmfestival Manila und arbeitete von 1985 bis 2004 an zahlreichen Skripten und Drehbüchern.

Filmografie (Auswahl)
 1972: Inferno unter heißer Sonne (Al tropico del cancro) (Co-Regie)
 1975: I baroni

Weblinks

 Curriculum Vitae

Einzelnachweise

Filmregisseur
Dokumentarfilmer
Drehbuchautor
Italiener
Geboren 1930
Gestorben 2021
Mann

Giampaolo Lomi


The Council for the Development of French in Louisiana (CODOFIL; ) is Louisiana's Office of Francophone Affairs (). It is a state agency whose multiple legislative mandates include developing opportunities to use the French language in tourism, economic development, culture, education and international relations. CODOFIL is governed by a board of 23 members and administratively placed within the Louisiana Office of Cultural Development's Department of Culture, Recreation and Tourism, overseen by the Lieutenant Governor. CODOFIL is the only state agency in the United States whose purpose is to serve a linguistic population.

Today, CODOFIL's role is to promote and support French immersion and French as a second language in education; it acts as a partner to the Louisiana Department of Education (LDOE), whose role is to manage Louisiana's school districts. CODOFIL continues to recruit and sponsor French, Belgian and Canadian associate teachers as per its accords with those countries, who are placed alongside local teachers upon LDOE's recommendation. CODOFIL encourages Louisiana Francophones to continue transmission of the state's heritage language via its scholarship program (providing opportunities for pedagogical advancement) and the Escadrille Louisiane program (which allows non-native speakers to perfect French at the Université de Rennes in exchange for a minimum 3-year teaching commitment of French in Louisiana).

CODOFIL has also worked to instill pride in all Louisiana Francophones in their linguistic identity rather than to uphold one variety of French language or another.

Mission and vision
The Council for the Development of French in Louisiana's mission is to "work toward the creation of an eco-system that permits the development of French in the economic, educational, cultural and professional sectors and in which Louisiana's French and Creole speakers are valorized in their cultural and linguistic identity." It seeks to "provide access to economic, educational, cultural and professional opportunities in French to all Louisianians." CODOFIL endorses revitalization of the French language in Louisiana through French immersion programs in schools, and CODOFIL does this by inviting French-speaking teachers from French-speaking communities around the world to Louisiana. In order for schools to have teachers for the immersion program, schools must send requests for teachers to CODOFIL first, then CODOFIL select teachers from the list of applicants that fit with the schools' criteria for the immersion program and send them to teach the immersion programs there. CODOFIL also endorses the Cajun Music Festival as a way to promote Cajun culture through Cajun music and keep the Cajun tradition alive.

Board
CODOFIL originally consisted of a chairman and an advisory committee, all appointed by the governor of Louisiana. Today it is administered by a president, an executive director, and a board of as many as 23 non-paid directors. In addition to the governor, various Louisiana organizations nominate and select board members, who serve for a term of four years.

History
The Council for the Development of French in Louisiana (CODOFIL) was established in 1968 to promote the preservation of French language and culture in Louisiana. The Louisiana state legislature has greatly shifted its stance on the status of French. Since the passage of Legislative Act No. 409 in 1968, the Louisiana governor is granted the authorization "to establish the Council for the Development of Louisiana-French" and that the agency is to consist of no more than fifty members, including a chairman. The name was soon changed to CODOFIL and was granted the power to "do anything possible and necessary to encourage the development, usage and preservation of French as it exists in Louisiana".

James R. Domengeaux, a former state legislator and former United States Congressman of ethnic French descent, was the driving force behind CODOFIL's creation. A semi-retired attorney at the time, Domengeaux began his crusade for restoring French in Louisiana after Senator Edgar G. "Sonny" Mouton, Jr., of Lafayette obtained passage of an "urge-and-request" resolution for Louisiana school boards to help reverse the decline of the use of the French language within the state. Domengeaux traveled around Louisiana to gain support for his campaign to make Louisiana a bilingual state through French language education. By the spring of 1968, Domengeaux had gained enough interest from the public and support from officials, to present his plan to the legislature. Legislators, such as J. Burton Angelle of Breaux Bridge voted to create CODOFIL, and the measure was signed into law in July 1968 by Governor John McKeithen. The law empowered CODOFIL to "do any and all things necessary to accomplish the development, utilization, and preservation of the French language ... for the cultural, economic, and tourist[ic] benefit of the State."

Criticism
Although CODOFIL aims to promote the French language and culture in Louisiana, this does not come without controversies among critics in Louisiana. A common criticism is that CODOFIL emphasizes education in Standard French over the local Louisiana French for economic purposes instead of cultural purposes. Critics claim that not only does CODOFIL attempt to homogenize the type of French dialect through inviting foreign Francophone teachers over relying on local French-speaking Cajuns and Creoles for the French language immersion program, CODOFIL also homogenizes French culture in Louisiana by prioritizing a Cajun identity over Creole identity when it comes to Louisiana's Francophone identity. Despite this, a survey conducted on the French immersion program shows that a majority of the teachers in the immersion program support integration of Cajun culture and Louisiana French into the curriculum, with 69% saying yes to teaching Cajun or Louisiana French into the curriculum, and 72% for Franco-Louisianan cultural aspect relating to the Louisiana French language, although the issue still remains for Louisiana Creole, with 90% of the teachers in the survey say no to integrating Creole into the curriculum in contrast to Louisiana French. Another criticism of CODOFIL's approach on cultural revival through festivals comes from critics such as the musician James Bau Graves, who view that CODOFIL commodifies Cajun culture through music festival and cultural activities and conserving it for tourism instead of preserving it. Graves views that the commercialization of Cajun culture prevents it from preserving because it hinders any attempts for the culture to adapt to the modern era, and homogenizes Cajun culture to a commodity. On the other hand, Barry Jean Ancelet views that the commercialization of Cajun culture allows more exposure to tourists and the international community. Ancelet views that exposure of Cajun culture to the outside allows appreciation from the international community and helps cultural preservation and revitalization possible by bolstering cultural pride and funding for the community.

See also
French in the United States
List of language regulators
Language revival
Acadiana
Curtis Joubert
Armand Brinkhaus

Sources

External links

1968 establishments in Louisiana
French-American culture in Louisiana
Francophonie
Language regulators
Louisiana law
Cajun language
Cultural promotion organizations
French language in the United States
Humanities organizations
Languages of Louisiana


Kóreuflói (kóreska: 서 조선 만 eða 서한만), er flói sem myndar norðausturhluta Gulahafs, milli suðausturstrandar Liaoning héraðs Kína og vesturstrandar Norður-Kóreu héraðanna Norður-Pyongan, Suður Pyongan og Suður Hwanghae. Kóreuflói er aðskilinn frá Bóhaíhafi með Liaodong-skaga.

Í Kóreuflóa renna þrjú helstu fljót Norður-Kóreu: Yalu fljót (sem rís á Paektu-fjalli og myndar stóran hluta landamæra Kína og Norður-Kóreu), Chongchon og Taedong - auk fjölda minni ána í Kína.

Flóinn er tiltölulega grunnur og nær sjaldan meira en 50 metra dýpi. Munur á flóði og fjöru er óvenju hár eða 6 til 12 metra. Margir breiðir sandgrynningar teygja sig meðfram ströndinni og í flóanum er fjöldi fjölda grýttra eyja, þar á meðal Ch'o, Sŏk og Sinmi eyjar í Norður-Kóreu og Ch'ang-shan og Ta-ch'ang-shan eyjar í Kína. Helstu hafnir við Kóreuflóa eru í norður-kóresku borgunum Namp'o og Sinŭiju og kínversku borgunum Lü-shun og Tan-tung.

Heimildir

Austur-Kínahaf
Landafræði Kína
Landafræði Norður-Kóreu

Kóreuflói


Le parc national de Kiang Ouest est l'une des plus grandes et des plus importantes réserves animales de Gambie. Il est déclaré parc national en 1987 et est géré par le Gambia Department of Parks and Wildlife Management.

Géographie
Le parc couvre une superficie de 11 526 hectares et est situé sur la rive sud du fleuve Gambie dans la division de Lower Rivir du district de Kiang West.

Les bâtiments administratifs du parc sont situées dans le village de Dumbuto, à 145 kilomètres de la capitale gambienne Banjul et 100 kilomètres de la côte gambienne. Le fleuve Gambie marque la limite nord du parc. Trois bolons (ruisseaux) - le Jarin, Jali et Nganingkoi - divisent l'intérieur du parc en trois sections. Le parc est inhabité, avec des villages situés à proximité de ses frontières.

La majeure partie du parc est située sur un plateau de basse altitude et est principalement constituée de savane guinéenne et de forêts sèches de plantes décidues (ou plantes à feuilles caduques), ainsi que de vasières et de criques de mangrove.

Flore
Les types de végétation dans le parc comprennent la savane guinéenne et la forêt sèche à feuilles caduques.

Les espèces d'arbres du parc comprennent le baobab (Adansonia digitata), l'acacia rouge (Acacia seyal), le Pterocarpus erinaceus, le Ceiba pentandra, le Terminalia macroptera, le Prosopis africana et les espèces de Ficus. Les graminées du parc comprennent l'Andropogon.

Faune

Le parc est une zone importante pour la faune gambienne, car des individus de la plupart de ses espèces de mammifères restantes s'y trouvent. Ces mammifères comprennent la loutre à joues blanches (Aonyx capensis), le guib harnaché (Tragelaphus scriptus), le caracal (Caracal caracal), le céphalophe de Grimm (Sylvicapra grimmia), le léopard (Panthera pardus pardus), la mangouste des marais (Atilax paludinosus), le serval (Leptailurus serval), le sitatunga (Tragelaphus spekii), la hyène tachetée (Crocuta crocuta), et le phacochère (Phacochoerus africanus). Des lamantins d'Afrique de l'Ouest (Trichechus sengalensis) et des dauphins à bosse sont parfois observés dans le bolon de Jarin.

Les espèces de reptiles du parc comprennent le python africain (Python sebae), la tortue de Bell (Kinixys belliana nogueyi), le crocodile d'Afrique de l'Ouest (Crocodylus suchus), le varan du Nil (Varanus niloticus), la vipère (Bitis arietans), le python royal (Python regius), et le cobra cracheur (Naja nigricollis).

Le parc compte plus de 300 espèces d'oiseaux, soit plus de la moitié de toutes les espèces d'oiseaux enregistrées en Gambie. Certaines des espèces d'oiseaux du parc ont une distribution très locale et sont rarement observées dans d'autres endroits de la Gambie. On compte 21 oiseaux de proie, y compris des espèces d'aigle, de faucon, de busard, de faucon et de vautour. Il y a un assez grand nombre d'oiseaux de proie dans le parc pendant la saison sèche. D'autres espèces d'oiseaux dans le parc comprennent dix espèces de martin-pêcheur, le calao terrestre et le perroquet à cou brun (Poicephalus robustus fuscicollis), qui se reproduit dans les mangroves du parc. D'autres espèces d'oiseaux comprennent le traquet front blanc (Myrmecocichla albifrons), la cisticole de Dorst (Cisticola guinea), la courvite de Burchell (Cursorius rufus), le bruant à ventre jaune (Emberiza affinis) et le bruant à calotte marron (Plocepasser superciliosus), qui ont des distributions restreintes en Gambie. Le bateleur des savanes (Terathopius ecaudatus), une espèce d'aigle à queue courte qui est le symbole officiel du parc. Il y chasse les gangas et les pigeons, et y est le plus souvent observé de juillet à septembre.

Conservation et tourisme

Les populations locales sont autorisées à ramasser une petite quantité de bois de chauffage et de produits forestiers, ainsi qu'à cultiver du riz dans les limites du parc.

Les incendies de forêt annuels affectent gravement le parc. En 2001, un grand incendie brûle dans toute la longueur du parc pendant deux jours.

Le parc reçoit peu de touristes, notamment de novembre à janvier. Le siège du parc et les bungalows touristiques sont situés à Dumbutu.

Tendaba Camp, dans le village de Tendaba, est ouvert depuis les années 1970 et est la base la plus établie pour les excursions dans le parc national. Les chalets de ce camp accueillent également les touristes. Toutefois, le réseau routier du parc est sous-développé.

Tubabkollon Point, situé près d'une plage de sable au bord du fleuve Gambie au nord-est du parc, est un bon endroit pour observer la faune. Le parc est de plus en plus connu comme un endroit privilégié pour l'observation des oiseaux.

Références

Aire protégée en Gambie
Aire protégée créée en 1987
Aire protégée de l'UICN - catégorie II

Parc national de Kiang Ouest


Limbach ist ein Ortsteil von Probstzella im Landkreis Saalfeld-Rudolstadt in Thüringen.

Geografie
Limbach liegt südwestlich von Marktgölitz und beherbergt 70 Einwohner in einem Seitental des Loquitzgrundes. Der Weiler ist in einem Talkessel gebaut worden. Die Gemarkung des Orte umfasst 362,91 Hektar.

Geschichte
Das Dörfchen wurde vor seiner urkundlichen Ersterwähnung 1386 mit mehreren ähnlichen Namen genannt, sodass eine genaue Zuordnung nicht möglich war. 1386 nannte man das Dorf Ludenbach.
1394 verschenkte Graf Otto VII. von Orlamünde das Dörfchen Limbach dem Landgrafen und an den Grafen von Pappenheim. Das Limbacher Freigut wurde 1621 an einen Herren von Lengefeld von den Pappenheimern beliehen. Die Einwohner waren Leineweber, Holzhauer, Bergleute und Fuhrmänner. Die besitzlosen Arbeiter waren sogenannte Rucksackbauern, die meist nur Kleinvieh (Ziegen, Schafe und Geflügel) hatten.

1952 betrieb man einen gemeindeeigenen Teerofen sowie eine Pottaschensiederei. Es gab auch eine Pechhütte. Schieferbergbau wurde seit Jahrhunderten betrieben. 1860 ging man sogar zum Tiefbau über. 1902 gab es eine Wasserversorgung. 1911 führte der Ort die Elektroenergie ein. 1953 gründete man die LPG Einheit. Am 1. Januar 1974 kam Limbach zu Marktgölitz.

Einzelnachweise

Weblinks

Geographie (Probstzella)
Ort im Landkreis Saalfeld-Rudolstadt
Ehemalige Gemeinde (Landkreis Saalfeld-Rudolstadt)
Ersterwähnung 1386
Gemeindeauflösung 1974

Limbach (Probstzella)


Aulnay-sous-Bois is the major railway station in the town of Aulnay-sous-Bois, in the department of Seine-Saint-Denis). It is on the RER B and the Transilien K lines. The station is also the terminus for tramway T4.

Photo gallery

See also
 List of stations of the Paris RER

References

External links

Réseau Express Régional stations
Railway stations in Seine-Saint-Denis
Railway stations in France opened in 1875

Aulnay-sous-Bois station


NGC 7413 je eliptična galaktika u zviježđu Pegazu.

Izvori

Vanjske poveznice

  Hartmut Frommert: Revidirani Novi opći katalog
  Izvangalaktička baza podataka NASA-e i IPAC-a
  Astronomska baza podataka SIMBAD
   VizieR
 DSS-ova slika NGC 7413
  Auke Slotegraaf: NGC 7413 Deep Sky Observer's Companion
  NGC 7413 DSO-tražilica
  Courtney Seligman: Objekti Novog općeg kataloga: NGC 7400 - 7449

7413

NGC 7413


Valentovce este o comună slovacă, aflată în districtul Medzilaborce din regiunea Prešov. Localitatea se află la , se întinde pe o suprafață de  și în 2017 număra 44 de locuitori.

Note

Legături externe

Localități din Slovacia

Valentovce


Tucuxi-delfinen (Sotalia fluviatilis) er en lille delfin, der kun lever i ferskvand i Sydamerikas Amazonflod og dens store bifloder. Den er normalt omrking 140 centimeter lang. Dens nære slægtning Sotalia guianensis lever i salt- og brakvand i flodmundinger og lavvande kystområder i Syd- og Mellemamerika samt Caribien.

Se også
 Floddelfiner

Kilder

Delfiner

Tucuxi-delfin


Pygeum  es un género de plantas con flores de la familia de las rosáceas. Ahora es considerado un grupo de especies dentro del género Prunus. Incluye siete especies. La especie tipo es: Pygeum zeylanicum Gaertn. (ahora Prunus ceylanica).

Especies
Pygeum coccineum (Elmer) Elmer
Pygeum henryi Dunn
Pygeum laxiflorum Merr. ex H.L.Li
Pygeum macrocarpum T.T.Yu & L.T.Lu
Pygeum oblongum T.T. Yu & L.T. Lu
Pygeum topengii Merr.
Pygeum wilsonii Koehne

Taxonomía
Pygeum fue descrito por Joseph Gaertner y publicado en De Fructibus et Seminibus Plantarum. . . . 1: 218, en el año 1788

Referencias

Amygdaleae

Pygeum


Dlo/Magnolia es una productora de televisión española establecida en el año 2004. Ha producido varios programas y series de éxito como Pánico en el plató, El método Gonzo o Camera Café, entre otros. Forma parte del grupo internacional Banijay Group.

Mayoritariamente, casi toda la producción de Magnolia ha sido destinada al grupo Mediaset España, especialmente para Telecinco.

Historia
El nacimiento de Magnolia TV se produce en el año 2004. La llegada de esta productora hizo que el panorama audiovisual cambiara, y se convirtiera en un fenómeno televisivo. Telecinco es una de las cadenas que apuesta por los programas de esta productora, además se ofreció a Magnolia para la creación de reality shows y distribuirlos en televisión. Camera Café fue su primer proyecto. Fue una serie que se emitió de lunes a jueves en Telecinco, en el acces prime time durante cuatro años y con más de 500 capítulos emitidos. Más tarde llegaría la producción de más espacios como Supernanny (2006-2014), ¡Clever! (2007) y Supervivientes (2006-2015), MYHYV (2008-2015), entre otros.

El objetivo social de Magnolia TV es la creación, la producción y coproducción, la comercialización y la explotación de programas de entretenimiento o actualidad para su difusión en televisión, la grabación de series, programas o documentales y otros productos audiovisuales de cualquier género.

Programas

Series

Véase también
 Mediaset España
 Banijay Group

Referencias

Mediaset España
Productoras de televisión de España

Dlo/Magnolia


An Diuris fastidiosa in uska species han Liliopsida nga ginhulagway ni Richard Sanders Rogers. An Diuris fastidiosa in nahilalakip ha genus nga Diuris, ngan familia nga Orchidaceae. Waray hini subspecies nga nakalista.

Mga kasarigan

Diuris

Diuris fastidiosa


بلدة مار مخايل اللبنانية والمعروفة باسم بلدة مار مخايل - بنابيل
 قرية مار مخايل هي إحدى القرى اللبنانية من قرى قضاء المتن في محافظة جبل لبنان.

صفحات توضيح أسماء أماكن

مار مخايل (توضيح)


12819 Susumutakahasi este un asteroid din centura principală de asteroizi.

Descriere
12819 Susumutakahasi este un asteroid din centura principală de asteroizi. A fost descoperit pe  la Moriyama de Robert H. McNaught și Yasukazu Ikari. Asteroidul prezintă o orbită caracterizată de o semiaxă mare de 3,12 ua, o excentricitate de 0,04 și o înclinație de 7,3° în raport cu ecliptica.

Vezi și
 Lista planetelor minore: 12001-13000
 Centura de asteroizi

Referințe

Obiecte astronomice descoperite în 1996
Centura de asteroizi

12819 Susumutakahasi


علاج الأنسولين التقليدي (بالإنجليزية:Conventional insulin therapy) هو نظام علاجي للعلاج من مرض السكري، والذي يختلف عن علاج الأنسولين المكثف الحديث.

هذه الطريقة القديمة (قبل تطور أجهزة مراقبة جلوكوز الدم المنزلية) لا زالت مستخدمة في نسبة من الحالات.

و هذا العلاج التقليدي بالأنسولين يتضمن:

 الحقن بمزيج من الأنسولين السريع والمتوسط، ويتم مرتين أو ثلاث مرات يوميا.  أو لتحسين دورة الجلوكوز ليلا يُعطى مزيج عند الإفطار والغداء، بينما يُعطى السريع فقط عند العشاء. أو يُعطى الأنسولين المتوسط فقط عند المساء.
 يتم جدولة الوجبات لتتناسب مع جرعات الأنسولين.
 المدى المستهدف لمستوى الجلوكوز في الدم يكون أعلى من المرغوب فيه في النظام المكثف.
 القياسات المتكررة لمستويات السكر في الدم لم تكن متاحة.

الجانب السلبي لهذا الأسلوب هوأنه من الصعب تحقيق نتائج جيدة كما هو الحال بالنسبة ضبط السكري مع مراقبة علاج الأنسولين المكثفة. بينما أحد إيجابياته أنه يُمكِن مرضى السكري من الحياة العادية دون التدخلات المتكررة في نظام العلاج المكثف.

مراجع

سكري
علاجات الإنسولين

علاج الأنسولين التقليدي


Et lokalirriterende stof er et stof, som har en generende virkning på en bestemt del af kroppen og fremkalder fx udslæt, hævelse eller kløe. Stoffet kan være en væske, et pulver, en gasart el.lign. Alkohol er et eksempel på et stof, der i visse koncentrationer kan virke lokalirriterende på slimhinderne.

Mærkning
Hvis et produkt indeholder 1% eller mere af et lokalirriterende stof, så skal det mærkes med en af følgende risikosætninger:
 R 36/37/38 Irriterer øjnene, åndedrætsorganerne og huden
 R 43 Kan give overfølsomhed ved kontakt med huden

Referencer

Kemiske forbindelser
Sikkerhed i kemi

Lokalirriterende stof


James Blood Ulmer  (St. Matthews, Carolina del Sur, 2 de febrero de 1942) es un guitarrista, flautista, cantante y compositor estadounidense de jazz.

Biografía
De familia originaria de las Sea Islands, la tradición musical de estas estuvo presente en su formación desde niño. A los trece años interpretó con un grupo de góspel, aunque se alejó durante un tiempo de la música para dedicarse al deporte. En 1959 inició su carrera musical tocando con grupos de rock de Pittsburg, donde se había trasladado su familia. Luego, tras una época de aprendizaje con Chuck Edwards y George Benson, comienza a tocar con músicos de funky jazz, como Jimmy Smith y Richard Groove Holmes.

A mediados de la década de 1960, organiza su propio grupo ("Blood & The Bloodbrothers"), con el que tocó durante tres años, hasta trasladarse a Detroit para estudiar e impartir clases de guitarra. En 1971 se incorpora a los Jazz Messengers de Art Blakey y toca, además, con Joe Henderson y Paul Bley. Después, realizó varias grabaciones, entre otros con Larry Young, antes de entrar a formar parte del grupo de Ornette Coleman (1972-1977), a la par que participa en grabaciones y conciertos con otros músicos, como David Murray, Ronald Shannon Jackson, Dewey Redman, Billy Higgins, Don Cherry, George Adams, Cecil McBee o Arthur Blythe.

A partir de 1980, graba discos como líder con regularidad, con sus propios grupos o con músicos como Murray, Adams o Bill Lasswell. ficha por Blue Note. A partir de mediados de los años 2000, además de sus giras y grabaciones, realiza actividades como ser jurado para los Independent Music Awards.

El estilo de Ulmer es, en palabras del crítico Phillipe Bodoin, "exacerbado y violento, inspirado tanto en el jazz como en el rock y el blues, aprovechando todas las posibilidades técnicas y lectrónicas disponibles hoy en día. Como arreglista y compositor crea climas líricos y ritmos hipnóticos y repetitivos". Para Joachim Berendt, Ulmer se ha convertido en el precursor de la música "no wave". Pasa del free al funk, concretando el primero y musicalizando el segundo.

Discografía

Como líder
 Revealing (In + Out, 1977)
 Tales of Captain Black (Artists House, 1978)
 Are You Glad to Be in America? (Rough Trade, 1980)
 Free Lancing (Columbia, 1981)
 Black Rock (Columbia, 1982)
 Odyssey (Columbia, 1984)
 Live at the Caravan of Dreams (Caravan of Dreams, 1986)
 America - Do You Remember the Love? (Blue Note, 1987)
 Blues Allnight (In +  Out, 1989)
 Black and Blues (DIW, 1990)
 Blues Preacher (DIW/Columbia, 1992)
 Harmolodic Guitar with Strings (DIW, 1993)
 Live at the Bayerischer Hof (In +  Out, 1994)
 Music Speaks Louder Than Words (DIW, 1995)
 Forbidden Blues (DIW, 1996)
 Blue Blood Innerhythmic, (2001)
 Memphis Blood: The Sun Sessions (Hyena Records, 2003)
 No Escape from the Blues: The Electric Lady Sessions (M, 2003)
 Birthright (Hyena, 2005)
 Bad Blood in the City: The Piety Street Sessions (Hyena, 2007)
 In and Out (In & Out Records, 2010)

Con "Odyssey the Band"
 Odyssey (Columbia, 3-5/83) con Charles Burnham y Warren Benbow
 Part Time (Rough Trade, 1983)
 Reunion (Knitting Factory, 1997) con Burnham y Benbow
 Back in Time (Pi Records, 2005) con Burnham y Benbow

Con "Music Revelation Ensemble"
 No Wave (Moers, 1980)
 Music Revelation Ensemble (DIW, 1988)
 Electric Jazz (DIW, 1990)
 After Dark (DIW, 1991)
 In the Name of... (DIW, 1993)
 Cross Fire (DIW, 1996)

Con "Phalanx"
 Phalanx (Moers, 1985)
 Original Phalanx (DIW, 1987)
 In Touch (DIW, 1988)
 Got Something (Moers, 1991)

Con "Third Rail"
 South Delta Space Age (Antilles, 1995)

Referencias

Notas

Bibliografía
 Joachim E. Berendt: El Jazz: Origen y desarrollo (Fondo de Cultura Económica. Madrid, 1986. ISBN 84-375-0260-8)
 CARLES, Phillipe; CLERGEAT, André & COMOLLI, Jean-Louis: Dictionaire du jazz . Robert Laffont Edt, París, 1988. ISBN 2-221-04516-5

Enlaces externos

 Entrevista con Furious en 1998

Guitarristas de jazz de Estados Unidos
Músicos de blues
Músicos de jazz-rock
Músicos de jazz moderno

James Blood Ulmer


حلبة المصارعة هي المكان الذي يتم فيه التنافس في رياضة المصارعة.

البناء و الترتيب
بناء و ترتيب حلبة المصارعة -التقليدية- يشبه إلى حد كبير حلبة الملاكمة، إلا أن في المصارعة تكون الحلبة محاطة بثلاث حبال بدل الأربع، كما أن الحبال في المصارعة غير مربوطين معًا.

حلبة المصارعة مكونة من بناء حديدي مرتفع عن الأرض، و مغطى بالرغوة الصخرية Foam و الحصير Mat ، و الحبال لا تحيط الحلبة بشكل كلي بل يوجد مسافة بينها و بين طرف الحلبة، و أسفل الحلبة مغطى بقماش لمنع رؤية ما فيها. و في كل زاوية توضع ثلاث قطع من الإسفنج عادة لتغطية الحديد الذي يربط بين الحبال.

تستخدم شركة WWE ( المصارعة العالمية الترفيهية ) حلبة بارتفاع 20 قدم. و يكون أسفل الحلبة مليئ بمختلف أنواع الأسلحة.

الأنواع

الحلبة التقليدية يكون فيها أربع زوايا، أما في الحلبات المطورة مثل شركة (Total Non Stop Action Wrestling (TNA فالحلبة مكونة من 6 زوايا.

انظر أيضًا
 أنواع مباريات المصارعة الحرة
 ضربات المصارعة الحرة
 التثبيت في المصارعة الحرة

مراجع

مصارعة محترفة
معدات فنون قتال

حلبة مصارعة


This article provides a timeline of the Cassini–Huygens mission (commonly called Cassini). Cassini was a collaboration between the United States' NASA, the European Space Agency ("ESA"), and the Italian Space Agency ("ASI") to send a probe to study the Saturnian system, including the planet, its rings, and its natural satellites. The Flagship-class uncrewed robotic spacecraft comprised both NASA's Cassini probe, and ESA's Huygens lander which was designed to land on Saturn's largest moon, Titan. Cassini was the fourth space probe to visit Saturn and the first to enter its orbit. The craft were named after astronomers Giovanni Cassini and Christiaan Huygens.

Launched aboard a Titan IVB/Centaur on 15 October 1997, Cassini had a nearly 20-year life span, with 13 of these years spent orbiting Saturn. The voyage to Saturn included flybys of Venus (April 1998 and June 1999), Earth (August 1999), the asteroid 2685 Masursky, and Jupiter (December 2000). The probes entered orbit on 1 July 2004, and the mission ended on 15 September 2017, when Cassini flew into Saturn's upper atmosphere in order to prevent any risk of contaminating Saturn's moons, some of which have active environments that could potentially bear life. The mission is widely perceived to have succeeded beyond expectations. Cassini-Huygens has been described by NASA's Planetary Science Division Director as a "mission of firsts", that has revolutionized human understanding of the Saturnian system, including its moons and rings, and our understanding of where life might be found in the Solar System.

Cassinis primary mission lasted for four years, from June 2004 to May 2008. The mission was extended for another two years until September 2010, under the name of Cassini Equinox Mission. The mission was extended a second and final time with the Cassini Solstice Mission, lasting until the spacecraft's destruction in September 2017.

The Huygens module traveled with Cassini until its separation from the probe on 25 December 2004; it was successfully landed by parachute on Titan on 14 January 2005. It successfully returned data to Earth for around 90 minutes, using the orbiter as a relay. This was the first landing ever accomplished in the outer Solar System and the first landing on a moon other than our own.

At the end of its mission, the Cassini spacecraft executed the "Grand Finale" of its mission: several risky passes through the gaps between Saturn and Saturn's inner rings. The purpose of this phase was to maximize Cassini scientific outcome before the spacecraft was destroyed. The atmospheric entry of Cassini effectively ended the mission, although data analysis and production is still ongoing.

Launch and cruise phase (1997–2003)

15 October 1997 01:43 Pacific Daylight Time (PDT)  – Cassini launched at 08:43 UTC inside Titan IVB/Centaur rocket at Cape Canaveral.

26 April 1998 06:52 PDT – Gravity-assisted flyby of Venus at 284 km, receiving a boost in speed of about 7 kilometers per second.

3 December 1998 22:06 PST – Cassini fired its main rocket engine for 90 minutes, setting the spacecraft on course for its second Venus flyby in 1999. The engine burn slowed the spacecraft by close to 450 meters per second (about 1,006 miles per hour) relative to the Sun. Cassinis speed went from 67,860 kilometers per hour (42,168 miles per hour) at the start of the maneuver to 66,240 kilometers per hour (41,161 miles per hour) at the end of the engine firing.

24 June 1999 13:30 PDT – Gravity-assisted flyby of Venus at 623 km.

18 August 1999 03:28 UTC − Gravity-assisted flyby of Earth. An hour 20 minutes before closest approach, Cassini made the closest approach to the Moon at 377,000 km, and took a series of calibration images.
The spacecraft flew past Earth at a distance of , passing most closely above the eastern South Pacific at . Cassini received a 5.5-kilometer-per-second (about 12,000-mile-per-hour) boost in velocity.

23 January 2000 – flyby of Asteroid 2685 Masursky around 10:00 UTC. Cassini took images 5 to 7 hours before at 1.6 million km distance and estimated a diameter of 15 to 20 km.

30 December 2000 10:05 UTC − Gravity-assisted flyby of Jupiter. Cassini was at its closest point (9.7 million kilometres, 137 Jovian radii) to Jupiter at this date, and performed many scientific measurements. It also produced the most detailed global color portrait of Jupiter ever produced (seen on the right); the smallest visible features are approximately  across.

30 May 2001 – During the coast phase between Jupiter and Saturn, it was noticed that "haze" became visible in the pictures taken by the narrow-angle camera of Cassini. This was first seen when a picture of the star Maia in the Pleiades was taken after a routine heating period.

23 July 2002 – In late January, a test was performed to remove the "haze" from the narrow-angle camera lens by heating it. Warming the camera to 4 degrees Celsius (39 degrees Fahrenheit) for eight days produced positive results. Later, the heating was extended to 60 days, and a picture of the star Spica showed an improvement of more than 90 percent compared to before the heating period. On 9 July, a picture showed that the removal procedure was completed successfully, which was announced on 23 July.

10 October 2003 – The Cassini science team announced the results of a test of Einstein's theory of gravity, using radio signals from the Cassini probe. The researchers observed a frequency shift in the radio waves to and from the space craft, as those signals traveled close to the Sun. Past tests were in agreement with the theoretical predictions with an accuracy of one part in one thousand. The Cassini experiment improved this to about 20 parts in a million, with the data still supporting Einstein's theory.

Primary mission (2004–2008)

27 February 2004 – A new, high-resolution picture of Saturn taken by Cassini on 9 February was released, and it was noted that mission scientists were puzzled by the fact that no "spokes" in Saturn's ring are visible. These dark structures in the "B" section of the ring had been discovered in pictures taken by the Voyager probe in 1981. Another picture, in infrared light, taken on 16 February shows cloud height differences and the same disturbance visible throughout the 1990s in Hubble Space Telescope images.

12 March 2004 – Pictures taken on 23 February do show a feature discovered by Voyager: Clumps in the outer "F"-ring. What could not be ascertained at the time was the exact lifetime of these clumps, and it is hoped that Cassini will provide conclusive data about this question. The first set of pictures shows a set of "clumps" moving along the "F" ring.

26 March 2004 – The Cassini science team published the first sequence of pictures of Saturn showing clouds moving at high speed around the planet. Using a filter to better see water haze on top of the dense cloud cover, motions in the equatorial and southern regions are clearly visible. The pictures were taken during the days from 15 to 19 February.

8 April 2004 – The first "long-term" observation of cloud dynamics in Saturn's atmosphere were published by mission scientists. A set of pictures shows two storms in the southern latitudes merge during a period from 19 to 20 March. Both storms had a diameter of about  before they merged.

15 April 2004 – NASA announced that two moons discovered by Voyager 1 were sighted again by Cassini in pictures taken on 10 March: Prometheus and Pandora. These are no ordinary moons, but their gravitational effects on the "F" ring led scientists to call them "shepherd moons". They fascinate all researchers interested in the dynamics of the ring system, because their orbits are close enough that they interact with each other in a chaotic manner. They have a history of defying predictions of their orbits. One of Cassini's missions will be to monitor the movements of these bodies closely.

18 May 2004 – Cassini entered the Saturn system. The gravitational pull of Saturn began to overtake the influence of the Sun.

20 May 2004 – The first picture of Titan with better resolution than any Earth-based observation was released. It was taken 5 May from a distance of 29.3 million kilometers (18.2 million miles).

27 May 2004 – TCM-20, the Phoebe approach TCM (Trajectory Correction Maneuver) was executed at 22:26:00 UTC. This was a 5-minute and 56 second burn of the main engine, which was not used since December 1998. It therefore doubled as a "dress rehearsal" for the 96 minute burn during "Saturn Orbit Insertion" (SOI). However, TCM-20 was mainly designed to change Cassini's velocity by 34.7 m/s (78 mph), setting up a flyby of the moon Phoebe 11 June.

11 June 2004 – Cassini flew by the moon Phoebe at 19:33 UT in Spacecraft Event Time at 2068 kilometers distance. All of the eleven onboard instruments operated as expected and all data was acquired. Scientists plan to use the data to create global maps of the cratered moon, and to determine Phoebe's composition, mass and density. It took scientists several days to pore over the data to make more concrete conclusions.

16 June 2004 – TCM-21 took place with a 38-second main engine burn. It was planned as the last correction of the trajectory of Cassini before SOI. A few days later the final TCM-22 tentatively scheduled for 21 June was canceled.

1 July 2004 – The Saturn Orbit Insertion burn was successfully executed. At 7:11 p.m. PDT (10:11 p.m. EDT), Cassini crossed the ring plane between Saturn's F and G rings. Its antenna was oriented forward acting as a shield against small ring particles. At 7:36 p.m. PDT (10:36 p.m. EDT), the spacecraft began a critical 96-minute main engine burn to cut its velocity by 626 meters per second and permit a 0.02 x 9 million kilometer Saturn orbit. Right after that burn, pictures of the rings were taken and sent back to mission scientist as the spacecraft approached within 19,980 kilometers (12,400 miles) from the cloud tops. Scientists were surprised by the clarity and detail of the pictures and will be poring over them for quite some time. "We won't see the whole puzzle, only pieces, but what we are seeing is dramatic," said Dr. Carolyn Porco, Cassini imaging team leader, Space Science Institute, Boulder, Colo. "The images are mind-boggling, just mind-boggling. I've been working on this mission for 14 years and I shouldn't be surprised, but it is remarkable how startling it is to see these images for the first time."

2 July 2004 – Cassinis first flyby of Titan was executed and first close up pictures were sent back to Earth. Due to the planning of the initial orbit, Cassini was passing over the south pole of the moon and from a larger distance than in later flybys. However, during a press conference on 3 June, mission scientist presented pictures that are already forcing them to rethink previous theories. It now seems that the darker and brighter albedo features on the surface do represent different materials. But in contrast to expectation, the icy regions seem to be darker than the areas where other (possibly organic) matter is mixed in with the ice.

16 August 2004 – Mission scientists announce the discovery of two new moons of Saturn, and with it the successful start of one of the programs of Cassini: Locating small and yet unknown moons. Later named "Methone" (S/2004 S 1) and "Pallene" (S/2004 S 2), these objects are small compared to other moons and they orbit between Mimas and Enceladus.

23 August 2004 – At a distance of 9 million kilometers from Saturn, the last major firing of the main engine took place to adjust the next closest approach and avoid the particles in the ring system. The 51 minute burn increased the velocity of the probe by 325 meters per second, moving the orbital periapsis point about 300,000 km farther away from Saturn than its smallest distance during SOI. At the same time, the new course will bring Cassini very close to Titan on its next flyby.

14 September 2004 – Final checkout of the Huygens lander was completed successfully. The separation of the probe stays scheduled for 25 December, with the landing anticipated on 14 January 2005.

26 October 2004 – The second flyby of Titan (called "Titan-A") was successfully executed. Data started to arrive at the JPL mission center at 01:30 UTC, 27 October, and included the highest resolution pictures ever taken of the surface of that moon. Also, first high-resolution infra-red spectra and pictures were taken from the atmosphere and surface. The spacecraft successfully skimmed the hazy, smoggy atmosphere of Titan, coming within 1,176 kilometers of Titan's surface. The flyby was the closest that any spacecraft has ever come to Titan. The pictures, spectra, and radar data revealed a complex, puzzling surface. Analysis of all data is on-going. The only glitch during the "Titan-A" event involved the CIRS instrument. During playback, the instrument team observed corrupted data. A decision was made to power the instrument off to reboot it. CIRS was powered back on within 24 hours and returned to its nominal state.

23 November 2004 – The last in-flight checkout of the Huygens probe before separation was completed successfully. All systems are ready for an on-time deployment of the probe.

13 December 2004 – The "Titan-B" flyby was executed successfully and the collected data are analyzed by mission scientists.

25 December 2004 – Huygens probe separated from Cassini orbiter at 02:00 UTC.

27 December – NASA published a picture of Huygens taken from Cassini two days after release. It reported that the analysis of that picture shows that the probe is on the correct course within the expected error range. These checks were necessary in order to place the orbiter in the correct orientation to receive the data from the probe when it enters Titan's atmosphere.

28 December 2004 – OTM-10 was executed at 03:00 UTC in Spacecraft Event Time. This maneuver, also called the Orbit Deflection Maneuver (ODM), took Cassini off of a Titan-impacting trajectory and on to a flyby trajectory with the required altitude to receive data from the Huygens probe as it plunges into Titan.

31 December 2004 – Cassinis flyby of Iapetus occurred at 18:45:37 UTC at an altitude of 122645 kilometers. First raw pictures were available the next day.

14 January 2005 – Huygens entered Titan's atmosphere at 09:06 UTC and had landed softly on its surface about two hours later. This was confirmed by the reception of the carrier wave emitted by the probe during its descent and touchdown. At 16:19 UTC the Cassini orbiter started to relay to Earth the scientific data received from the probe. The first picture was released at 19:45 UTC, showing a view from about 16 km above the surface. A second picture taken from the probe at rest on the surface was released a short time later. Analysis of the data is ongoing.

15 February 2005 – Successful Titan flyby, with new regions of its surface scanned by radar. Cassinis mapping radar acquired a picture that shows a large crater on Titan, with an estimated diameter of .

17 February 2005 – The first close flyby of Enceladus was executed and first closeup images were sent back to Earth. The flyby distance was about .

17 March 2005 – The Cassini probe reveals that Saturn's moon Enceladus has an atmosphere. It has been described as "substantial" by its discoverers.

16 April 2005 – The fifth planned flyby of Titan with a minimum distance of about 1,025 kilometers was executed at 19:12 UTC. This was the closest flyby up to this date, and provided the opportunity to obtain more detailed data on the constituents in the upper atmosphere of Titan. The first analysis of that data showed a large range of complex carbon molecules. On 25 April a mass plot was published that demonstrates the existence of these molecules.

3 May 2005 – Cassini begins Radio occultation experiments on Saturn's Rings, to determine ring particle size distribution, on the scale of centimetres.

10 May 2005 – At the beginning of a period of focussed observation of the ring system of Saturn, slated to take until September, mission scientists announced the discovery of a new moon in the "Keeler gap" inside the "A" ring. Provisionally named S/2005 S 1 and later named Daphnis, it was first seen in a time-lapse sequence of images taken on 1 May. Imaging scientists had predicted the new moon's presence and its orbital distance from Saturn after last July's sighting of a set of peculiar spiky and wispy features in the Keeler gap's outer edge.

14 July 2005 – The closest flyby of Enceladus with a distance of  was executed successfully. First raw pictures were published.

7 September 2005 – Flyby of Titan at a distance of , data gathered partially lost due to software problem.

26 September 2005 – Flyby of Hyperion at a distance of , the closest flyby and only visit to the moon during the primary mission.

27 July 2006 – NASA confirms the presence of hydrocarbon lakes in Titan's northern polar region.

28 May 2008 – Cassini completed its 43rd flyby of Titan, ending its primary mission. Renamed Cassini Equinox mission, Cassini observed Saturn during its equinox crossing, or summertime.

Cassini Equinox mission (2008–2010)

9 August, 11 August, 9 October, and 31 October 2008 – With closest approach at 50, 25, and 200 km, respectively, Cassinis last three Enceladus flybys of 2008 utilized a new imaging technique named "skeet shooting" to successfully acquire very high resolution images. The flybys also allowed Cassini to directly sample Enceladus's cryovolcanic plumes.

3 November, 14 November, 5 December, and 21 December 2009 – Titan flybys 46 through 49 concentrated on radar, VIMS, and INMS sampling of Titan and its thick atmosphere. T47 involved high-resolution VIMS coverage of the Huygens landing site, while the other three flybys made use of radar and RSS. T49 allowed radar coverage of Ontario Lacus, one of the largest methane lakes on Titan.

June - October 2009 – Cassini observed Saturn during its equinox, or the time of Saturn's year where the sun is directly over its equator.

2 November 2010 – Cassini was triggered into a protective standby mode, or "safe mode", after a bit flip caused it to miss an important instruction. NASA announced the interruption in scientific processes on 8 November. However, by 8 November some of the craft's functionality had already been partly restored. Nominal scientific instrument sequencing events were successfully started on 10 November. Cassini was reactivated as scheduled on 24 November and has returned to perfect working order, in time for two scheduled close fly-bys with Enceladus. At this point there has been no public disclosure as to the data loss impact of the 11 November (T-73) flyby. However, no images were acquired on the 11 November polar flyby.

Cassini Solstice Mission (2010–2017)
On 3 February 2010, NASA announced that a second mission extension until May 2017, a few months past Saturn's summer solstice, had been funded. The schedule included an additional 155 orbits, with 54 flybys of Titan, 11 of Enceladus, 2 of Rhea, and 3 of Dione. One of the flybys of Titan dipped below the ionosphere.

Grand Finale (2017)

On 15 September 2017, Cassini was deliberately disposed of by a controlled fall into Saturn's atmosphere, ending its nearly two-decade-long mission. The last signal was received at 11:55:46 UTC.

Cassini orbiter travel milestones

Detailed timeline of Huygens mission

All times given after 2005-Jan-14 09:11 UTC are expected event times and may differ from actual event times. This page will be updated after descent has occurred with corrections if they are necessary.

The data used in this section has been slightly out of date, an updated version of ephemeris from ESA was available 2005 January 6.

Timeline of Huygens landing process
{| class="wikitable"
|-
!  style="width:200px; text-align:center;"| Date (UTC)
!  style="width:400px; text-align:center;"| Description
|- style="vertical-align:top;"
|  style="text-align:center; " | 2004 December 25, 02:00
|  style="text-align:left; "| Huygens separates from Cassini. Its flight path initially takes it away from Titan.
|- style="vertical-align:top;"
|  style="text-align:center; " | 2005 January 03, 20:01
|  style="text-align:left; "| Huygens reaches a maximum distance of 4,658,661 kilometers from Titan.
|- style="vertical-align:top;"
|  style="text-align:center; " | 2005 January 11, 12:00
|  style="text-align:left; "| Cassini rise in the east (azimuth = 93 degrees) as seen from the landing site
|- style="vertical-align:top;"
|  style="text-align:center; " | 2005 January 12, 11:20
|  style="text-align:left; " |Huygens is 1,000,000 kilometers from Titan.
|- style="vertical-align:top;"
|  style="text-align:center; " | 2005 January 13, 09:21
|  style="text-align:left; "| Huygens is 500,000 kilometers from Titan.
|- style="vertical-align:top;"
|  style="text-align:center; " | 2005 January 14, 04:23
|  style="text-align:left; "| Huygens is 100,000 kilometers from Titan.
|- style="vertical-align:top;"
|  style="text-align:center; " | 2005 January 14, 06:50
|  style="text-align:left; " |Cassini turns on probe radio link receivers. Huygens is 50,000 km from Titan.
|- style="vertical-align:top;"
|  style="text-align:center; " | 2005 January 14, 07:02
|  style="text-align:left; " |Cassini begins to turn radio dish toward Titan
|- style="vertical-align:top;"
|  style="text-align:center; " | 2005 January 14, 07:14
|  style="text-align:left; " |Cassini turn to Titan complete; 3 minutes later orbiter X-band downlink disabled
|- style="vertical-align:top;"
|  style="text-align:center; "| 2005 January 14, 08:29
|  style="text-align:left; "| Saturn occulted by Titan as seen from Huygens
|- style="vertical-align:top;"
|  style="text-align:center; "| 2005 January 14, 08:38
|  style="text-align:left; "| Saturn's rings occulted by Titan as seen from Huygens
|- style="vertical-align:top;"
|  style="text-align:center; "| 2005 January 14, 08:44
|  style="text-align:left; "| Probe turns transmitters on; low power mode
|- style="vertical-align:top;"
|  style="text-align:center; " | 2005 January 14, 08:48
|  style="text-align:left; "| Huygens is 10,000 kilometers from Titan.
|- style="vertical-align:top;"
|  style="text-align:center; "| 2005 January 14, 09:06
|  style="text-align:left; "| Huygens enters the atmosphere of Titan
|- style="vertical-align:top;"
|  style="text-align:center; "| 2005 January 14, 09:09
|  style="text-align:left; "| Huygens feels maximum deceleration
|- style="vertical-align:top;"
|  style="text-align:center; "| 2005 January 14, 09:10
|  style="text-align:left; "|Huygens deploys its pilot chute, followed closely by the main chute.
|- style="vertical-align:top;"
|  style="text-align:center; " | 2005 January 14, 09:11
|  style="text-align:left; " |Huygens begins data transmission to Cassini.
|- style="vertical-align:top;"
|  style="text-align:center; " | 2005 January 14, 09:18
|  style="text-align:left; " | Release front shield; transmitters switch to high power mode; instruments configured for descent and measurements commence
|- style="vertical-align:top;"
|  style="text-align:center; "| 2005 January 14, 09:25
|  style="text-align:left; "| Main parachute separates; deploy stabilizing drogue chute
|- style="vertical-align:top;"
|  style="text-align:center; "| 2005 January 14, 09:49
|  style="text-align:left; "|Huygens activates its surface proximity sensor, allowing it to measure its altitude and spin rate.
|- style="vertical-align:top;"
|  style="text-align:center; " | 2005 January 14, 09:57
|  style="text-align:left; " | The Gas Chromatograph Mass Spectrometer, the last instrument to be activated, begins to sample the atmosphere.
|- style="vertical-align:top;"
|  style="text-align:center; vertical-align:top;" | 2005 January 14, 11:12
|  style="text-align:left; vertical-align:top;" |Cassini makes its closest flyby of Titan (Titan-C) at an altitude of 59,996 kilometers at a speed of 5,401 meters per second and 93 degree phase angle (azimuth = 278 degrees, elevation = 33 degrees as seen from the landing site)
|- style="vertical-align:top;"
|  style="text-align:center; " | 2005 January 14, 11:30
|  style="text-align:left; " |Huygens turns on its descent imager lamp.
|- style="vertical-align:top;"
|  style="text-align:center; " | 2005 January 14, 11:37
|  style="text-align:left; " |Huygens lands on the surface of Titan
|- style="vertical-align:top;"
|  style="text-align:center; " | 2005 January 14, 13:11
|  style="text-align:left; " |Cassini sets in the west (azimuth = 272 degrees) as seen from the landing site
|- style="vertical-align:top;"
|  style="text-align:center; " | 2005 January 14, 13:47
|  style="text-align:left; " |Cassini stops probe data collection
|- style="vertical-align:top;"
|  style="text-align:center; " | 2005 January 14, 18:14
|  style="text-align:left; "| Cassini sends the first of Huygens''' data back to Earth.
|}

Fly-bys
Following is a list of close fly-bys of Saturn's moons (at less than 5000 km). The closest approach for each moon is bolded.

Primary mission

Extended (Equinox) mission

Solstice mission
The second extended mission was scheduled from 2010 October 12 through the Saturnian summer solstice in May 2017, followed by two dozen proximal orbits of Saturn and the rings. Cassinis final optical navigation image of the mission was taken on 20 September 2016. The Cassini'' mission ended on 15 September 2017, when the craft disintegrated in Saturn's atmosphere.

Proximal orbits

References

External links
 Cassini–Huygens press release archives
 "Cassini–Huygens Saturn Arrival" June 2004 (pdf)
 Draft White paper for Solar System Decadal Survey 2013–2023: Cassini–Huygens Solstice Mission 2009 (pdf)
 Tour dates

Spaceflight timelines

Timeline of Cassini–Huygens


Die US Open 1986 im Badminton fanden vom 11. bis zum 16. November 1986 in Manhattan Beach in Kalifornien statt. Das Preisgeld betrug 5.000 US-Dollar.

Finalergebnisse

Weblinks
http://newspapers.nl.sg/Digitised/Page/straitstimes19861118.1.30.aspx

1986
Badminton 1986
Badmintonwettbewerb in Manhattan Beach

US Open 1986 (Badminton)


Tahir-hanuma Tuzlić (? – 23. kolovoza 1922.),  dobrotvorka, vakifa velikog vakufa. Dolazi iz begovske obitelji Tuzlića.

Životopis
Unuka Mahmud-bega i kći Osman-bega. Braća su joj bili Mehmed i Šemsi, a sestre Zuhra i Hafiza.  Udala se za Bećir-bega Gradaščevića. Obudovila je bez potomstva. Godine 1907. uvakufila je brojne nekretnine i posjede u "..dobrotvorne, bogougodne i prosvjetne svrhe". Objekte i posjede upisala je na tuzlanskom Šerijatskom sudu u vakuf. Za muteveliju je izabrala Esad-efendiju Kulovića. Njen je vakuf jedan od najvećih u tuzlanskom kraju, pored mnoštva drugih velikih i malih vakufa. U njemu su se našli kuće, bašče, dućani i magaze, zgrada Kotarskog predstojništva koju je držala pod zakupom, oko 12 njiva, livada i avlija. Zahtijevala je da se vakuf zove Evladijet-vakuf. Tahira je udomila i othranila Osmana Vilovića, koji je rano ostao sirotan. Vilović je poslije bio tuzlanski gradonačelnik (1908. – 1922.). Tahira je umrla 23. kolovoza 1922. godine. Sestra Hafiza oproučno je ostavila značajna sredstva za obnovu Jalske džamije u Tuzli. 1891. godine džamija je temeljito obnovljena. Tahira-hanuma je pokopana na lijevoj strani ulaza u Jalsku džamiju. Mezar joj obilježavaju lijepo ukrašeni nišani.

Izvori

Životopisi, Tuzla

Tahira-hanuma Tuzlić


تتناول نظرية التوبو Category Theory البنى الرياضية المختلفة بطريقة مجردة لتدرس خصائصها الأساسية والعلاقات المتبادلة فيما بينها وهي شديدة الصلة مع الطوبولوجيا الجبرية خصوصا في بداية نشأتها عندما تأسست من قبل صموئيل ايلينبيرغ وساوندرز ماك لين في 1945. تظهر التصانيف في جميع فروع الرياضيات وبعض فروع المعلوماتية النظرية والفيزياء الرياضية.

خلفية حول الموضوع

دراسة التصنيفات محاولة لالتقاط ما هو شائع ومشترك في الأصناف المختلفة للبنى الرياضية المتنوعة.

ليكن لدينا الصف Grp من الزمر groups المؤلفة من جميع الغراض التي لها «بنية مجموعة» "group structure". بشكل أكثر تحديدا، Grp تتألف من جميع المجموعات G المزودة بعلاقة ثنائية والتي تحقق مجموعة من البدهيات axiom. وعن طريق مجموعة البدهيات تلك يمكن للمرء استنتاج مجموعة من المبرهنات حول الزمر. فمثلا من المسلمات الأساسية يمكن الاستنتاج مباشرة أن العنصر الحيادي identity element للزمرة يكون وحيدا.

وبدلا من التركيز على الأغراض المفردة (الزمر) التي تمتلك نفس الخواص والبنية، كما تفعل النظريات الرياضية عادة، تحاول نظرية التصنيف ان تركز على انحفاظ الشكل morphism - أي العمليات المحافظة على البنية - بين مختلف الأغراض. وقد تبين من دراسة انحفاظات الشكل أنها تمكننا من معرفة المزيد حول بنية الأغراض ذاتها (الزمر هنا). انحفاظات الشكل morphisms هنا هي تشاكل الزمر group homomorphism. تشاكل الزمر بين زمرتين «هو ما يحفظ بنية الزمرة» بشكل دقيق - أي أنه إسقاط دقيق لزمرة على أخرى، غنع «عملية» تأخذ الزمرة إلى زمرة أخرى. ومجمل المعلومات حول بنية الزمرة الأولى تصبح في الزمرة الثانية. دراسة تشاكلات الزمر تؤمن وسيلة ممتازة لدراسة الخواص العامة للزمر ونتائج بدهيات الزمر.

نظرية الفئة
نظريات رياضياتية

نظرية التوبو


An Dendrochilum haslamii in uska species han Liliopsida nga ginhulagway ni Oakes Ames. An Dendrochilum haslamii in nahilalakip ha genus nga Dendrochilum, ngan familia nga Orchidaceae.

Subspecies

Ini nga species ginbahin ha masunod nga subspecies:

 D. h. haslamii
 D. h. quadrilobum

Mga kasarigan

Dendrochilum

Dendrochilum haslamii


La Playa Maracas (en inglés: Maracas Beach)
Es una playa en la isla de caribeña de Trinidad. Se encuentra en el lado norte de la isla, a una hora de la ciudad capital de Puerto España, siguiendo una ruta montañosa. A diferencia de muchas de las playas del norte de Trinidad, la Playa de Maracas está protegida por una profunda bahía. Es una de las playas más conocidas en la isla de Trinidad y es considerada por algunos como la playa más hermosa (considerando su tamaño) más cercana a la ciudad capital.

Uno de los aspectos más famosos de la playa de Maracas son las docenas de chozas donde se cocinan alimenos y se cocinan platos exóticos.

Véase también
Geografía de Trinidad y Tobago
Mar Caribe

Referencias

Playas de Trinidad y Tobago

Playa Maracas