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A bleeding heart, a seal of fate
There is no crime, I'll re a?? instate
Love is a weakness, Lust conquers all
Cross my soul and hope to die
Where do you draw the line?
Enter my mind, can you stop the rage
No one shall mourn or pity your grave
Believe the lie, the line that you toe,
If you just do, do as you're told
The meaning of lust
The soul of life
When you're screaming from the sky
It's now or never
Inside your brain
It's a hollow hideaway
Out of pride, I'll isolate.my fears
Never turned my back on why you were here
Mapped out in scars, look to the skies
Your only salvation, so close your eyes

subset: commoncrawl


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All of these outfits are simply but some how are wonderful! I love all of them….I would definelty wear all of these outfits. 🙂 <3
1. Theyskens' Theory Fall 2011 RTW, 2. SJP via Pacific Coast News, 3. Shevah V. via Lookbook
Corduroy pants are among winter's trendiest pieces, but if you're stumped about how to wear these retro-inspired trousers, you've come to the right place! Read on for some tips and tricks for wearing cords, as well as some outfits for inspiration:
4 Tips & Tricks for Rocking Corduroy Pants:
- If the word "corduroy" gives you visions of the huge, bell-bottomed pants your mom wore in the '70s, just know that cords have come a long way since then! Today's versions come in every style from skinny to boot-cut and are available in a rainbow of different colors.
- That being said, if you're not ready to commit to a colorful pair of cords, look for a neutral pair in black, tan or gray.
- Since corduroy fabric has such a retro vibe, try to create a balance by wearing your cords with modern tops and accessories.
- Having trouble figuring out what to wear with cords? Just style them the same as you would your favorite pair of jeans — it's that simple!
5 Stylish Ways to Wear Cords
Outfit 1: Menswear-Inspired
Product Info: Cords- Anthropologie, Top- J. Crew, Cardigan- Madewell, Earrings- Fossil, Necklace- J. Crew, Oxfords- ModCloth
For this look, start by pairing some zipper-detailed cords with a classic striped top, then layer on a matching navy cardigan. Add some sparkly oxfords and fun jewelry for an outfit that's perfect for classes.
Outfit 2: Denim Copycat
Product Info: Cords- Urban Outfitters, Top- Topshop, Jacket- Dorothy Perkins, Bracelet- ModCloth, Watch- Woolrich, Flats- DSW
These cords are perfect for the corduroy-shy girl — from a distance, they look just like jeans! This means that you can wear them however you'd like, but for this look, I went in a more feminine direction. Pair a printed floral tee with a blush-colored kimono jacket and add some woven black flats. Accessorize with a matching watch and pretty bracelet for a comfy and cute everyday outfit.
Outfit 3: Red-y for Nighttime
Product Info: Cords- ASOS, Top- Topshop, Jacket- Miss Selfridge, Boots- H&M, Ring- Topshop
This outfit is a little more edgy, which makes it perfect for a casual night out. The dark red cords look great when paired with a lacy top, while the moto-style jacket adds some edge. Tuck the cords into some ankle booties, and for the finishing touch, add an oversized cocktail ring.
Outfit 4: Comfy Chic
Product Info: Cords- J. Crew, Top- Reiss, Cardigan- Old Navy, Pumps- Bakers, Necklace- Nicole Miller
Dress up a pair of black, bootcut cords and a plain gray t-shirt by adding a colorful wrap cardigan. Add a matching pair of teal pumps and a statement necklace for a bold, yet understated look.
Outfit 5: Pink Lady
Product Info: Cords- LOFT, Sweater- H&M, Headband- ASOS, Wedges- Piperlime, Earrings- Topshop
If you're ready to dive into this trend headfirst, why not rock a pair of colorful cords? Since these pink ones from LOFT are so bright, try wearing them with neutral sweater for balance. Add a pair of wedge pumps and accessorize with some chandelier earrings and a light pink headband.
What do you think?
Would you ever wear a pair of cords? What do you think of these outfits? Which one is your favorite? How would you wear cords? Let me know what you think by leaving a comment below!


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The tools you need to digitalize your business
For construction companies
Mobile Worker is a field service management and mobile workforce time tracking software. Mobile Worker solution gives the overview and easy control of working and machine hours, consumption of goods, tools and equipment.
Android application comes in 13 languages. Ios and Android application works even offline. Mobile Worker apps are intuitive and easy to use.


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Abstract and Keywords
It was once presumed that costs of Internet adoption were too great for gang members to absorb. They lacked the financial resources to access the Internet or the technological know-how to use it. That is no longer the case, which leads to two questions: What are gang members doing online? What are the responses to gangs online? The growing research on this topic indicates that gang members are online and using the Internet at a rate comparable to their peers. This occurs in the United States and abroad. Gangs do not exploit the Internet to its criminal potential, even though the law enforcement community suggests otherwise. This is most likely due to the low technological capacities of gang members. However, gang members do engage in higher rates of crime and deviance online than their non-gang peers. Gang members also use the Internet to posture, provoke, and project group power, particularly on leading social media platforms such as Facebook, Twitter, and YouTube, which in turn allows activities occurring online to have ramifications for crime and violence offline. It is debatable whether online space is as important to gangs as physical space, but the Internet is undoubtedly a valuable medium to gangs. The potential for conflict and the posting of gang images has attracted the attention of law enforcement as well as researchers to document this activity. Platforms are being developed to anticipate the spilling of online gang conflicts offline. Since the Internet is a value-neutral medium that engages youth and young adults, it is anticipated that social media and the Internet will continue to appeal to gangs and gang members for the foreseeable future.
Keywords: street gangs, social media, Internet, Internet banging, cybercrime
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New Genentech breast cancer drug shows late stage trial success
SOUTH SAN FRANCISCO, Calif.Genentech, a member of the Roche Group, recently announced top-line results of EMILIA, the first randomized Phase III study of trastuzumab emtansine (T-DM1), showing that people who received trastuzumab emtansine lived significantly longer without their disease getting worse (progression-free survival) compared to those who received lapatinib plus Xeloda (capecitabine).
The study enrolled people with HER2-positive metastatic breast cancer who had previously received treatment with Herceptin (trastuzumab) and a taxane chemotherapy. Final results for overall survival (OS), a co-primary efficacy endpoint of EMILIA, are not yet mature. According to Genentech, the safety profile of trastuzumab emtansine was consistent with that seen in previous studies.
Trastuzumab emtansine is an investigational medicine known as an antibody-drug conjugate (ADC). It is comprised of the antibody trastuzumab and the chemotherapy DM1 attached together using a stable linker. It is designed to target and inhibit HER2 signaling and deliver the chemotherapy directly inside HER2- positive cancer cells. According to Genenetch, trastuzumab emtansine "reinforces Roche's personalized healthcare approach of developing targeted medicines to fight cancer."
"Trastuzumab emtansine represents a new approach for the treatment of people with HER2-positive breast cancer that comes from our decades of research on the HER pathway," said Dr. Hal Barron, chief medical officer and head of Global Product Development. "We are excited about the EMILIA results because trastuzumab emtansine is our first antibody-drug conjugate and it may help people who still need more treatment options for this aggressive disease. We will work to submit these data to regulatory authorities as quickly as possible."
Based on these findings, Genentech plans to submit a Biologics License Application for trastuzumab emtansine to the U.S. Food and Drug Administration this year for HER2-positive mBC. In addition, Roche plans to submit a Marketing Authorization Application to the European Medicines Agency this year for the same indication. Genentech licenses technology for trastuzumab emtansine under an agreement with ImmunoGen Inc.
As Luke Timmerman noted at Xconomy.com, "Even though Genentech is responsible for development, and will keep the vast majority of product revenues for itself, today's result is an important moment for ImmunoGen. The company stands to collect a 'mid-single digit' percentage royalty on worldwide sales from T-DM1, because of its contribution to help link the antibody to the toxin. ImmunoGen has no products of its own on the market, and the approval of T-DM1 would provide a significant percentage from a potential multi-billion dollar seller."
EMILIA (TDM4370g/BO21977) is an international, Phase III, randomized, open-label study comparing trastuzumab emtansine alone to lapatinib in combination with Xeloda in 991 people with HER2-positive mBC whose disease progressed after initial treatment with Herceptin and a taxane chemotherapy.
The co-primary efficacy endpoints of the study are progression-free survival (as assessed by an independent review committee) and overall survival. Other study endpoints include safety profile, one-year and two-year survival rates, progression-free survival as assessed by investigator, overall response rate, duration of response and quality of life.
In addition to EMILIA, there are two ongoing Phase III studies of trastuzumab emtansine. MARIANNE is comparing three different regimens (trastuzumab emtansine alone, trastuzumab emtansine plus pertuzumab, and Herceptin plus a taxane chemotherapy) in people with HER2-positive metastatic breast cancer who have not been previously treated for their metastatic disease. TH3RESA is comparing trastuzumab emtansine to physician's choice of treatment in people with HER2-positive metastatic breast cancer who have already received both Herceptin and lapatinib.
According to Genentech, "Building on the results of trastuzumab emtansine studies to date, Roche/Genentech have approximately 30 ADCs in the pipeline."
Code: E03301201


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Creative Settlement: What Can We Learn From the Bezos?
MacKenzie and Jeff Bezos announced details of their settlement agreement last week, signaling the end of a very high conflict – and very public – divorce without the need for significant litigation. As the wealthiest couple in history, the Amazon Founder and CEO and his now-former wife faced a unique set of challenges when dissolving their union.
The Bezos settlement is notable for many reasons not the least being that the assets being divided represented significant wealth acquired during the course of the marriage, rather than resources brought to the union by either party. But what is the most striking to us here at Seiden Family Law is actually the creativity of the settlement and the fact that they worked so well together to reach an agreement.
Under terms of their settlement, MacKenzie will retain her Amazon shares (and thus the ability to ride the wave of the stock price) and Jeff maintains the voting rights that were essential to his continued role within the company. This out-of-the-box solution is one that reflects a mutual desire for both the good of the family and the good of the company founded during their marriage. It respects and reflects the best interests of all parties, and emphasizes compromise over conflict.
There's an important life lesson in this very public divorce, and it isn't about the drama leading up to the separation or even the details of the eventual settlement. It's the way the Bezos worked together to find an inventive solution to their situation. As a firm, we pride ourselves on our ability to think creatively in a wide range of settlement circumstances, and we see the Bezos situation as an inspiring case of creativity and vision.
How can we help you to think creatively about your situation?


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We are proud to say, we can ship to virtually any address in the world, from a local delivery to an international shipment, we are always on hand to make the process as smooth as possible.
Delivery Time.
International deliveries, for Europe please allow up to 5 days via economy and 3 days priority, this is the service we expect from FedEx and UPS. All other countries please allow up to 8 days economy and 5 days priority.
All prices are in GBP. © Copyright 2020 International Control Components Ltd. Sitemap | Registered in England No. 09600224 VAT. GB219638387
All named products profiled herein are trademarks of their respective companies. E&OE.
While we make reference to brand name merchandise, we are in no way endorsed or associated by these companies.


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Funding Solar Projects: Funding & C-PACE Finance
Pope Energy, located in Boston, Massachusetts, has over 30 years of experience in bringing finance solutions to finance and build projects. If a customer desires to own a commercial solar project and does not have the capability to monetize tax credits and accelerated depreciation, we have a financing solution to meet your needs. If a customer desires to own a solar system, we are able to place power purchase agreements (PPA's) or tariff agreements in place, as well as leverage banking relationships to finance solar projects.
CPACE (Commercial Property Assessed Clean Energy) Finance
CPACE finance represents a paradigm shift funding 100% of the costs of renewable energy, energy efficiency, water conservation, environmental health, and safety improvements through the property tax bill.
Funding does not need to come from capital budgets. Energy savings must exceed the cost of improvements to enable cash flow for the repayment obligation. The repayment obligation is tied to the municipal assessment of the property and runs with the property as opposed to a property owner.
The CPACE finance model provides for the following:
- 100% Financing
- No Out-Of-Pocket Expenses
- Long-Term Financing (Up to 25 Years)
- Lower Energy Costs
- Cash Flow Positive Projects
- No Personal Guarantees
- Competitive Rates and Terms
- Owner Retains All Tax Incentives
- Combine with Utility Incentives
- Automatic Transfer Upon Sale
- Preserves Capital for Core Business
CPACE financing must be enabled by each state legislature and specifically approved by each municipality, as well have the consent of the first mortgage holder. Pope Energy and CPACE program facilitators are able to assist with municipal and mortgage holder approvals.
Connecticut and Rhode Island have robust CPACE programs, a growing program in New York, and a developing program in Massachusetts.
Contact us to discuss ways to procure funding for solar panel projects. We are based in Boston, Massachusetts, and serve clients throughout Massachusetts, Rhode Island, Connecticut, New Hampshire, Vermont and New York.


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OSCE Mission to Moldova launches campaign against gender-based violence
CHISINAU, 25 November 2010 -The OSCE Mission to Moldova today launched a series of awareness-raising activities, including continuing performances of a play, as part of the international 16-Day Campaign Against Gender-Based Violence.
The Campaign, launched in 1991, aims to prevent combat gender-based violence by raising public awareness globally. The 16 days start on 25 November, the International Day for the Elimination of Violence Against Women; and end on 10 December, International Human Rights Day.
The OSCE Mission's contributions to the campaign in Moldova include a 6 December performance in Chisinau of the play Casa M, based on real-life stories of Moldovan victims of violence. The Mission will also support a mobile exhibition, a television talk show, youth drawing and sports competitions, leaflets, posters, a Facebook webpage, university lectures and roundtables and seminars on international and domestic law and practice.
The Campaign will end on 10 December with a roundtable meeting dedicated to the role of men and boys in combating violence against women.
"We hope that a new coalition will be set up in Moldova of men and boys speaking out against violence against women," said Eugenia Benigni, the Mission's Anti-Trafficking and Gender Adviser.
The roundtable meeting will also focus on Moldova's new legislation on gender-based violence and the participation of women in peace building and the security sector to mark the 10th anniversary of United Nations Security Council Resolution 1325, which promotes an increased role for women in conflict prevention and resolution.
The OSCE Mission supports the 16-Day Campaign in Moldova in co-operation with the OSCE Office for Democratic Institutions and Human Rights, the Ministry of Labour, Social Protection and the Family, non-governmental organizations, academics, national and international experts, as well as United Nations agencies.


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Dartholm, located on quiet Shore Road in Southwest Harbor overlooking the picturesque harbor, has an unusual history. Originally built as a dance hall in the early 1900's, Dartholm was repurposed to become the summer residence for the president of Dartmouth (hence its unusual name), and recently updated to be a gracious shingle-style cottage available for year-round living. Views from the traditional cottage are expansive, be it the yachts and lobster boats traversing the harbor, or the scenic views of Somes Sound, the Cranberry Islands and mountains of Acadia beyond, Dartholm optimizes what life on the waterfront has to offer.
Dartholm has been beautifully restored and renovated, a wonderful blend of traditional elements and modern conveniences. There are five bedrooms in the main house with the master suite and an additional bedroom suite on the first floor, a warm and inviting living room, Cottage style dining room, modern chef's kitchen and den. Additionally, a seasonal one-bedroom guest house offers an additional living area with full kitchen, laundry and bath. Most rooms enjoy the many varied harbor, island and mountain views.
Dartholm has been impeccably maintained and includes a beautifully landscaped private back yard with deck, two car garage, garden shed, deep water dock and two moorings.
The Town of Southwest Harbor, a vibrant year-round community, offers a multitude of quaint restaurants and shops, and is a well-known center for all types of boating activity; certainly an area that would complement life at Dartholm.
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Yes, in the firs thalf they were going on about how great of a team SMU is and talked up the AAC having 5 bids.
There is no way the AAC gets 5 bids this year. No way.
Some ECU Perspective
Anything involving SMU basketball belongs here.
Moderators: PonyPride, SmooPower
Re: Some ECU Perspective
Yes, in the firs thalf they were going on about how great of a team SMU is and talked up the AAC having 5 bids.
There is no way the AAC gets 5 bids this year. No way.
Re: Some ECU Perspective
I get not liking coaches or certain players, but I can't get behind the hope to miss the tournament.
High school gym? Losing that game in Madison Square Garden would have been OK?
KD, TJ, EC going 1-15 will mean a loss against anyone.
No way AAC gets 5 teams in.
Re: Some ECU Perspective
Funny.... that's exactly what happened to the defense!
Party at The Wopper!
Re: Some ECU Perspective
I am not hoping we miss the tournament. I am saying that the ECU loss was bad enough to be the game that will keep us from making the NCAA tournament if we happen to win enough games to even garner consideration. I hope I'm wrong and hope we beat Houston on Wednesday. I will be at the game.
Re: Some ECU Perspective
If he isnt happy now then what the hell was he feeling for the last 2 years?
Yikes. No TJ and especially Reggie is devastating.
Re: Some ECU Perspective
[quoteDid anyone else catch the announcer saying that SMU is a lock for the Tourney?][/quote]
Just as they were fastening the buckles on his straight jacket.
Re: Some ECU Perspective
So what does it say about Tulsa after they go to ECU and win easily, just days after they beat Houston in Tulsa? We'll find out more about ECU after their visit to Moody next week. I still think they are one of the lower level teams when all is said and done. Question is whether we are going to be right there with them. Too early to tell.
Re: Some ECU Perspective
Looks like it so far.
Shake It Off Moody
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The Electronic Home
We pride ourselves for providing a fast, friendly and reliable service. Based and operating in Letchworth Garden City, with offices in Hatfield – working in Hitchin, Stevenage, Welwyn, Hatfield and St Albans. The Electronic Home specialises in the sale, installation and repair of home computer and audio/visual consumer electronic products. It is in our interest […]
Smart Merchants Limited
Our Mission: To establish a business that offers unrivalled service and value for money to its customers. Please note we cannot guarantee all images displayed on the website are fully accurate please see product information for full specification on each product


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DEAR ABBY: I have a friend in her mid-40s who has naturally dark hair she keeps cut short. It looked fine.
A few months ago, she bleached her hair platinum blond. She said she was going for a look that will include dark roots, but she has kept the roots platinum, so now her hair just looks white — especially in pictures. She posted photos of herself with her boyfriend on Facebook, and while I was scrolling down, my initial reaction was, "Who is that elderly woman he's sitting with?"
A mutual friend commented to me how bad my friend's hair looks and how aging it is. Should I mention to her that her hair color makes her look 20 years older? Telling someone her hair doesn't look good can be hurtful, but if it were me, I'd want to know. — HELPFUL IN HAWAII
DEAR HELPFUL: Be diplomatic, but tell her. A tactful way to lead in would be to say you saw the pictures she posted on Facebook and the platinum hair makes her look "older." However, unless she asks how much older, don't volunteer, because if you say it's two decades, she may take offense.
DEAR ABBY: What is the rule for tipping in drive-thrus? I never thought a tip was necessary in places like that. If the service is good, a tip is warranted. Now many drive-thrus have a tip jar out on the ledge of the window.
It's like everyone seems to think they deserve one. A tip is expected when you get your vehicle inspected, your tires changed, your oil changed, manicures and hairstyling, among other things. How much is appropriate to tip for services? I certainly don't want to devalue someone's service if times have changed and this is commonplace. — DRIVE-THRU TIPPING
DEAR DRIVE-THRU: For restaurant servers, hairstylists and manicurists, a 15 to 20 percent tip is expected. The same is true for taxi drivers, hotel personnel and skycaps. In other situations, a tip may be offered when the service performed has been exceptional.
If the service you received at the drive-thru was prompt, your order was correct and the person at the window was pleasant and helpful, either give the workers a couple of dollars or the loose change that's returned to you. However, a tip is not required.
DEAR ABBY: A woman friend of mine is angry at me because I have started dating a mutual friend of ours. She says when someone wants to date someone's friend, the polite thing to do is ask how the friend feels about it. Mind you, the man I'm going out with isn't her ex and was as good a friend to me as he was to her. If I had discussed the matter with her, what difference would it have made? She doesn't own him. Does her logic make sense to you? — FREE AGENT IN TEXAS
DEAR FREE AGENT: No. Your "friend" has no prior claim on the man you are dating. That she would try to insert herself into your romantic life makes no sense, and you would be foolish to allow it.
Dear Abby is written by Abigail Van Buren, also known as Jeanne Phillips, and was founded by her mother, Pauline Phillips. Contact Dear Abby at www.DearAbby.com or P.O. Box 69440, Los Angeles, CA 90069.
Good advice for everyone — teens to seniors — is in "The Anger in All of Us and How to Deal With It." To order, send your name and mailing address, plus check or money order for $7 (U.S. funds) to: Dear Abby, Anger Booklet, P.O. Box 447, Mount Morris, IL 61054-0447. (Shipping and handling are included in the price.)
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Working late one Friday night in the office for a small trucking company, I was the only one there. I had some more work to get done and didn't want to work on Saturday. I like to wear sexy clothing, but its not allowed during business hours, so I bring a change of clothes to work with me.
That night I was wearing a real tight mini skirt that was quite thin and a little transparent and sat low on the hip. I was wearing a black thong underneath. I had on a light skimpy spaghetti string top that was also transparent and fit high enough to show my belly. I wasn't wearing a bra and my tits showed through the material.
The material was light and cool and my nipples were visible. My nipples were always hard because the office was air conditioned.
I didn't mind though, because I really enjoyed the tingly feeling they gave me. Sometimes I'd play with them and make them even harder which also made my pussy hot and start throbbing, so sometimes I'd masturbate and made myself cum.
Sometimes I'd watch myself in a mirror and that made me even hotter. That night was no different. I completed my work and just had some filing to do. I thought I was alone. I did not hear the trucks pull up outside the warehouse or the drivers come into the office.
When I finished the work I needed to do on the computer, I filed the copies in the filing cabinet. Since my skirt was so short when I bent over, my thong was showing with my ass and pussy. I thought, since I was alone it really didn't matter. But the thought that someone was watching made my pussy wet and start throbbing.
Just as I was finished filing, and I was going to sit on one of the couches in the reception area and start playing with myself, I felt hands gently take my hips, keeping me slightly bent over. I felt a leg gently spread my legs and then felt the rubbing of the hot groin going up and down my ass and pussy. I could feel his cock was already hard and as he was rubbing it against me it turned rock hard and hot.
I could feel it throbbing as it strained against the tight fit of his jeans. This made me real horny and I realized my fantasy of someone watching was real after all. While he was doing that another man appeared in front of me and started squeezing, sucking and biting my tits and nipples.
I had fantasized about hot office fucking, but this was beyond my wildest fantasies. After a few minutes, the three of us went to the couch and I let them slowly undress me as they licked and nibbled all over my body. I was throbbing so hard, I knew I was going to cum any minute.
I pushed them both away and rubbed my wet, hot, pulsating pussy and pink, hard clit until I came like I've never cum before. They both had their clothes off and were stroking their, long, hard cocks and watched me.
I came several times, but I wasn't finished by no means. Watching them stroking their cocks and making them so big and hard kept me horny and wanting them to do whatever they wanted to me.
They both came over to me on either side and I took their cocks in my hands, shocked at how hot and throbbing they were. I licked and sucked on both their cocks one after another. I sucked and stroked them until they were both ready to cum.
Although, I enjoyed the feel and taste of their rock hard cocks in my mouth, I wanted them to cum in my pussy and ass. They helped me up and one laid on the couch and I got on top of him, straddling him letting his cock slide into my tight wet pussy. Being rock hard and throbbing, he couldn't hold his load and his cock exploded inside me.
I kept riding his cock letting it ram me over and over, it felt so good.
I like a good hard fuck after I cum. He was not close to being finished either as I felt his cock swelling up inside me. While this was going on the other driver was fingering my ass making it ready for him to slide his cock in.
When he finally slid his cock up my ass, he was also so rock hard and throbbing that he couldn't hold his load either and exploded inside me filling my ass with his hot cum.
He kept ramming my ass and the other one kept ramming my pussy. I had never tried double fucking before and didn't know it would feel so good.
I came over and over while they were ramming me from both ends. They held their load as long as they could and then we all came at the same time. I felt my pussy throb harder and faster as their hard cocks started pulsating hard and fast as they filed my pussy and ass with their hot, sticky cum. Minutes later our orgasms subsided I felt their hot sticky cum run down my ass and pussy as they pulled their still hard cocks out of me.
They licked my pussy and ass clean of our juices and I licked their cocks clean. I decided I would work late hours more often after that. And they said next time they were in town, they'd be happy to pay me a visit for another round.
I couldn't help but think how horny truck drivers must get after being on the road so long. I was very happy to ablige them.


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Daniel Goodfellow made his Commonwealth Games debut on the Gold Coast where he won gold in the men's 10m syncronised platform diving.
Daniel won a bronze medal in the men's 10m synchronised platform event with his diving partner, Team England's Tom Daley at the 2016 Summer Olympic Games in Rio de Janeiro.
He is coached by Marc Holdsworth at City of Leeds Diving Club.
19 October 1996
City of Leeds
Gold Coast 2018
Gold Coast 2018 Commonwealth Games - Gold men's 10m syncronised platform
Rio 2016 Olympic Games - Bronze
2016 European Championships - Silver
2016 World Cup - Bronze
2013 European Junior Championships - Gold


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text: Unisex Home / Unisex / Unisex All-in-Ones Unisex All-in-Ones Unisex All-in-Ones £15.03 £18.04 (inc. VAT) RRP: £0.00 Stock Status: In Stock Available in 3 different sizes Sizes: Medium Large Extra Large Are you eligible for VAT relief?: Yes I am VAT exempt No I am not VAT exempt Add to your Wish List Information Reviews These are designed for those facing moderate to severe problems, which may include bowel leakage. The soft hypoallergenic top sheet makes contact comfortable, while the reinforced core will absorb and then retain fluid. The shape is designed to fit close to the body, two adhesive tapes on each side give an individual fit, while side elastication will minimise leakage. A wetness indicator shows when it is time to change. Size Waist Absorption Medium 80-120cm 31-47inches 2550ml Large 100-150cm 39-59inches 2640ml Extra Large 110-160cm 43-63inches 2880ml Pack of 30 If you would like a regular order please contact us via telephone on FREEPHONE 080 196 2070. Not yet reviewed Write an online review and share your thoughts with other shoppers! Be the first to review this product Related Products Womens Pull up Pants From: £12.49 Underpads £9.49


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Phone: 970-328-8500Fax: 970-328-1448Sheriff's Office 0885 E Chambers AvenueP.O. Box 359Eagle, Colorado email@example.com
Sheriff James Van Beek - Valley Voices
April 13, 2017
The joys of being a patrol officer are often expressed in the little moments. An impromptu football toss with some kids in the park; a chat with an elderly woman walking her dog; stepping out of the car and having a young child run up to give you a hug; letting a group of kids switch on the police lights and giggle with excitement; noticing someone in need and connecting them with those who can help; volunteering at a community event … It is truly a privilege to work in this place we call home.
Living in Eagle County can make us feel exempt from events happening elsewhere. It is our job to understand that we are not, and to prepare for any possible contingency. The magnificence of our environment and friendliness of its residents, generates global appeal and that requires additional security measures. As patrol officers, we are the front line of defense. We must remain vigilant so that others needn't be. Tragedy can occur anywhere, at any time and even with our extensive level of training, we are still affected by certain events.
A typical traffic stop can suddenly become a deadly encounter. You notice a car driving erratically. It's mid-afternoon and you wonder if they have begun an early happy hour, are distracted by a phone text, or perhaps dealing with a rambunctious dog in the front seat — any number of things could be going on, but they don't appear to be in control of their car and the results could be disastrous. You pull them over to make sure things are OK.
As you exit your vehicle, you notice quite a bit of movement in the car. The driver has leaned over several times and the passenger is reaching for something in the back. Your training alerts you to potential danger. While it could simply be a mom, talking to her child in the back seat, it could also be a gang member traveling through, and reaching for a gun — you don't know and must be ready for anything.
Not a moment goes by that we aren't cognizant of potential dangers that may occur in the most unassuming places: our parks, schools, recreational facilities, outdoor venues, shopping areas, basically anywhere. Even when things start out innocently, they can abruptly turn tragic.
A child out past curfew can become a missing person. An outdoor excursion can become a life-threatening ordeal. A reach for the radio can become a deadly car accident. An evening out to a restaurant or pub may result in someone becoming intoxicated and exhibiting behavior that turns violent. Escalation can turn a simple argument into something deadlier. This aggression can make its way home, creating the potential for domestic violence. Unintentional and even deadly consequences can result from unfiltered aggression. We must often be the calming force for a peaceful resolution, and at times that means removing one or more parties from the equation and taking them into protective custody.
Nothing prepares you for the images permanently embedded in your mind, of the dead bodies you encounter from various situations: accidents, suicides, outdoor incidents, murders, drug overdoses, natural causes, but especially those of children. Patrol officers are committed to making sure any tragedy is immediately contained, even at great personal risk. It's a tough job but completely worth it. We have the honor of protecting our incredible community, insuring a positive future for our children.
Getting selected for this position is not easy. All patrol officers must complete a state certified Police Officers Standards & Training (POST) program, which covers all areas of law enforcement including: investigations, firearms, law, intelligence, civil liability, arrest procedures, detention skills, traffic, field operations, community relations, drugs, self-defense, control tactics, surveillance, driving techniques and additional county procedures.
There are also continual training mandates throughout an officer's career. Applicants must pass an extensive background check, polygraph, psychological test, college transcript evaluation and multiple interviews. In addition, officers must possess a true desire to help others — those seeking bravado are quickly eliminated. In addition, there are personal sacrifices.
Driving through our neighborhoods, thoughts may wander to your youngest, who is competing in a state championship, which you are unable to attend. The 12-hour shift, which changes from nights to days every eight weeks, is an equitable solution for all officers, but makes planning family events and holidays a challenge. Balancing law enforcement with family life can be difficult, yet most agree, it is worth the cost.
Patrol operations with the Eagle County Sheriff's Office is a fulfilling opportunity, and while it can be quite dangerous and requires unwavering dedication, it is also the honor of a lifetime.
James van Beek is the Eagle County sheriff.
500 Broadway - P.O. Box 850 | Eagle, CO 81631 | 970-328-8600 | Contact Us


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News BriefsShvat 13, 5773 , 24/01/13
Joseph's Tomb Desecrated again
Over 2,500 worshippers were allowed into Joseph's tomb in Shchem for a prayer service Wednesday night, and were shocked to find the entrance suffused with urine, and windows blackened following an attempted arson. Samaria maintenance rapidly washed down the area and the service continued uninterrupted. Samaria regional Council Chairman Gershon Mesika reflected, "Only inhuman barbarians could desecrate so holy a place."
Other archived news briefs:Jan 24 2013, 08:37 AM, 1/24/2013


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Picture of Katherine Heigl Wearing Curls at the Killers Premiere
Love It or Hate It? Katherine Heigl's Corkscrew Curls
Katherine walked the red carpet at the premiere of her new movie Killers last night looking like anything but an assassin. While she's usually slicked back and sleek, for this premiere she chose to go with sweet, fluffy corkscrew curls that remind me a little bit of Shirley Temple's famous style.
Curls like this are a good styling choice if you're growing out your hair and want to disguise awkward length, or just want a look that's pretty and wholesome, but it can also come off sometimes as slightly girlish on grown women. What do you think? Did Katherine pull it off, or is this a look she should deep-six?


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Dear XebiaLabs community,
We are pleased to announce the release of XL Release 6.1.0. This release introduces code-centric features that allow teams to build releases in a new Groovy-based DSL, the Xfile.
By defining releases with code, developers can use the same tools and practices to manage releases that they use for other project artifacts. They can version releases and store them in source control, easily compare multiple versions of a release, and apply the review cycles that they already use for the applications they are coding. And this code-centric capability works in addition to XebiaLabs' GUI-centric workflow, providing a versatile, dual-mode approach.
In addition, this release includes:
- Improved performance when loading releases and retrieving dependencies for Gate tasks
- Optimized memory usage and default server parameters for better performance
- Scheduling support and new display options for custom script tasks
- A new task type for executing Groovy scripts as part of the release process
- A new task type for executing Groovy or Python scripts that are stored outside XL Release
- A complete refactoring of the XL Deploy task type to provide better integration between XL Release and XL Deploy
- An easy way to retrieve information such as configuration files and logs that you can send to the XebiaLabs Support Team when troubleshooting issues
Before upgrading, please read about the changes in the release manual and review the upgrade instructions.
You can download the release at the XebiaLabs Software Distribution site.
XL Release 6.1.0 is a short-term support (STS) version that will be supported until it is superseded by the next STS or long-term support (LTS) version. For more information, refer to Short-term support/Long-term support policy.


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As someone who has taught online university courses since 2009 and taught high school level social studies for 13 years before that, I have met many colleagues who share similar experiences teaching. One commonality? Academic integrity is something we all strive to promote in our courses yet still find elusive in some respects. We try different methods for monitoring student activity in Canvas tests and quizzes and we develop writing assignments that are more authentic in nature in hopes that we get an authentic product from our students as a result. I came across this short article offering up three other strategies we can implement in our courses to help alleviate plagiarism. If you have any strategies that have worked well for you, whether online or face-to-face, please feel free to share them in reply to this post.
Article link: Keys to Stopping Plagiarism


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Willem-Jan van Elk
Willem-Jan van Elk (1961) is convinced that information projects can only be successful if realised in close interplay with business...
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Roel Geers
Roel Geers (1952) was one of the founders of hgrv in 1991, a place where he had already had a long service record. He began his career in 1970 as a...
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Martijn Kole
Martijn Kole (1970) has filled management and directorship functions in the international media, telecom and advisory world after his training in...
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Leo van Veen
Leo van Veen (1955) began his career as an information technician in the banking world. He quickly came to the conclusion that the installation of...
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At Oxess we carefully produce all products by hand, including all race boards. We only use very high-quality materials. Thanks to the experience of more than 25 years in snowboard construction, Oxess builds snowboards of highest quality and durability.
Race boards from Oxess impress with their high performance, both in terms of smooth-running, carving characteristics and ice grip. This is done by adapting the progression of board stiffness and flexibility to the customer's individual needs by using special materials (carbon, fiberglass, titanal, rubber) and CNC-milled wood cores.
Ingemar Walder
With the TC (Torsion Control) developed by Oxess, the power is optimally distributed to the board by means of 3D-construction. Thus, these forces can act where they are needed. Ideal preconditions for top athletes as well.
While we use carbon as a top sheet for slope riders, since it makes the board very agile and allows a wide application area, we work almost exclusively with titanal for racers, which makes the board extremely smooth running.
Of course, we can also customize all models for special requirements according to the customer's needs.
Meanwhile Oxess is very well represented in alpine racing. Athletes from various national teams and junior squads in Europe, Asia and America appreciate the individual support of Team Oxess and the possibility to tailor the ideal snowboard for themselves. Oxess hence, makes a significant contribution to a successful career. Olympic gold medalists, World champions, World Cup winner, countless podium places on Oxess snowboards are proof enough.


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On last night's episode of Impact Wrestling, it was revealed that "The Monster" Abyss will be the 2018 inductee in the Impact Wrestling Hall of Fame.
As fans are aware, Abyss is one of the few Impact Originals left on the roster, and has been with the company since their inception in 2002. Abyss is also one of only a handful of Impact Grand Slam Champions, as he has held the X Division Championship, the Impact World Tag Team Championship (once with James Storm and once with Crazzy Steve) the (now-retired) Television Championship, as well as the National Wrestling Alliance World Tag Team Championship (with A.J. Styles) and World Heavyweight Championship during Impact's time as an NWA affiliate from 2002 to 2007.
.@TherealAbyss' Hall of Fame ceremony will take place October 13th over Bound For Glory weekend at McHale's Pub in midtown Manhattan. Tickets are available NOW!— IMPACT (@IMPACTWRESTLING) September 21, 2018
(Tickets are included as part of the Bound For Glory VIP Packages)
TICKETS: https://t.co/PU8vYrWXKC pic.twitter.com/wiHTMaiTxA
⚡ "@TherealAbyss Was Announced For The IMPACT Hall Of Fame On IMPACT!"https://t.co/JSsoNgssEG— IMPACT (@IMPACTWRESTLING) September 21, 2018
Here is Abyss' Hall of Fame video package:


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Totally Rad, dude; like totally!!!
jcpt928 21 Apr 2009 19:57
OK Donny, I have to admit, this is totally wicked awesome!! Bro, I wish I had thought of something like this first!! >.<
I can't wait to see how it's used - this will be too much fun I think. Peace out!! ^_^
"A life lived for others, is a life lived to the fullest…if everyone lives for everyone else, then noone is left out."
Gilly. is. amazing. <3 (:
Unfold Totally Rad, dude; like totally!!! by jcpt928, 21 Apr 2009 19:57


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With the increased cost of today's sophisticated electric meters, it is more important than ever to protect that investment from vandalism, tampering and severe storms. Brooks protective covers are constructed with heavy gauge galvanized steel and powder coated with an oven-baked enamel to withstand abuses that would normally destroy the meter. Protective meter covers greatly reduce current surge during electrical storms. Brooks round protective covers are available with or without a tough Lexan window, in a variety of lengths to fit almost any size meter. The hinged face plate opens to allow full access to demand reset meters. All units are easily secured with seals or padlocks.Mounting ears are provided for installation on Ringless meter sockets. For ring-type meter sockets, the mounting ears are snapped off, and mounting screws provided are used to install the cover.
*Additional sizes available. Contact Brooks for model numbers.


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There's no use to even try to deny it anymore. Apple's iPhone 5C and 5S are hours away from becoming reality. But with everything from their looks to their specs and pricing structures revealed in a bundle of reports of late, there's very little that can still surprise us.
In fact, it's as if the two are official already. More so as new alleged promotional documents have come to light, most likely unveiling the final set of specs of the iPhone 5S. As usual, you're advised to treat the spill of information with care and an (un) healthy dose of salt, though the odds of the intel being fake are in all honesty astronomical.
That said, the biggest change and most noteworthy upgrade the 5S will bring to the table compared with its predecessor is, as expected, a fingerprint sensor. You know, the feature that Samsung, Sony and LG all avoided to use for their new flagship devices, but that Pantech surprisingly decided to cram inside its Vega LTE-A.
Moving on, it looks as if Apple's "next big thing" will look exactly the same as last year's big thing, rocking identical dimensions (123.8 x 58.6 x 7.6 mm) and weight (112 grams). Not to be snarky or anything, but are we sure that parody video was truly a parody? It sure doesn't feel like it.
But hey, at least the iPhone 5S is tipped to pack an upgraded A7 processor, which rumor has it will be roughly 30% faster than the A6. And a slightly better front-facing camera with 2 MP sensor. Plus, an 8 MP rear snapper with lower f/2.0 aperture and 1,080p video recording support up to 120 fps.
The display is claimed to be identical both in size (4 inches) and resolution (1,136 x 640 pixels), the battery will reportedly offer 8 hours of continuous use in talk time and 4G LTE speeds will be missing… from this particular version of the iPhone 5S being advertised, namely the model headed to China Unicom. Fret not though, as other variants will most definitely come with LTE in tow.
Still, will this, how shall I put it delicately, bland list of features be enough to convince you to upgrade? Will you instead go for the iPhone 5C? Sound off below.
Sources: Phone Arena and CTechCN


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Our Building Envelope Services
Arnold & Associates has the tools, equipment, personnel necessary to perform a large volume of roofing and waterproofing consulting projects both nationally and internationally.
Here are three solid and compelling reasons to choose Arnold & Associates roofing and waterproofing consulting services in support of your next project.
1. Quality. We believe quality starts with quality specifications that are installed by quality contractors. Our professional expertise combined with years of specialized roofing and waterproofing consulting will provide you with long term quality systems.
2. Proven Technology. We are independent of any ties with manufacturers, material suppliers or contractors. With 50 plus years of field experience has provided us knowledge of technology. We know what works! This combined with concise specifications, comprehensive construction documents, detailed plans and detailed drawings, and on-site inspections, will ensure the success of your project.
3. High Standards. This begins with each associate setting high standards for his work and carries forward into his document development, contractor pre-qualification and finally into the standard of the work of the project. You benefit from successful and timely project outcomes that are consistently at or below budget.
Let us help you avoid costly errors with all of your roofing and waterproofing project needs!


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Treating customers fairly is at the core of our business operations. We appreciate that looking after our customer's interests is paramount to client confidence.
The Financial Conduct Authority (FCA) has promoted TCF as a philosophy and produced six outcomes. These objectives have been incorporated as a culture and applied to all our processes and procedures.
Outcome 1
Consumers can be confident that they are dealing with firms where TCF is central to the corporate culture
Outcome 2
Products and services are designed to meet the needs of identified consumer groups and targeted accordingly
Outcome 3
Consumers are provided with clear information and kept appropriately informed before, during and after the point of sale
Outcome 4
Where consumers receive advice, it is suitable and takes account of their circumstances
Outcome 5
Consumers are provided with products that perform as firms have led them to expect, and the associated service is both of an acceptable standard and as they have been led to expect
Outcome 6
There are no unreasonable post-sale barriers imposed by firms when consumers want to change product, switch provider, submit a claim or make a complaint


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This is a delicious, light fluffy chocolate cake without a hint of animal produce! Great to make with kids, this is a pretty foolproof recipe. Challenge your guests to guess what's missing!
This can very easily be made gluten free by using gluten free flour and baking powder. You may need to increase the amount of water you add, as gluten free flour can be more absorbent.
I made this recipe yesterday for my daughter who is vegan. It was so easy to make and was huge... We all tried it and it was delicious, as good and if not better than a regular chocolate cake - 16 Nov 2014 (Review from Allrecipes UK & Ireland)
Easy to make and extremely good, wouldn't know it's vegan, used lemon juice instead of the white wine vinegar... - 03 Jan 2015 (Review from Allrecipes UK & Ireland)
This is one amazing cake! I made this for my sisters wedding as there was a handful of vegan guests. It quickly became known as 'the little chocolate cake'. It was even demolished before the actual wedding cake. I'm going to make it again for a birthday at work but not tell anyone it's totally vegan. Thank you so much for sharing this recipe!! - 09 Nov 2014 (Review from Allrecipes UK & Ireland)


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Joe Mathieu Turns Boston Anchorman
P.O.T.U.S. channel anchor and program director, Joe Mathieu, is leaving Sirius XM for Boston's WBZ NewsRadio. After an extensive search, WBZ tapped Mathieu to take the reigns of New England's top morning radio news broadcast. It's a homecoming for Mathieu who hails from northern Connecticut and started his radio career in Boston in 1996. Joe started covering Washington D.C. in 1998 and spent seven years as managing editor and anchor at the CBS MarketWatch Radio Network before he developed and launched Sirius XM's P.O.T.U.S. channel in 2007. Congrats to Joe!
*Per the usual, you can read an abbreviated version of this post (sans attribution) on DCRTV.com in about 40 minutes.


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Rob Davis and his team are efficient on the basketball court. Not with their ball movement or free-throw percentage. The Hoopfest site manager and his crew's efficiency lies in actually making a basketball court.
On the Friday of Hoopfest weekend when the 9-to-5ers leave work to head home, not much appears out of the ordinary in downtown Spokane. This year is a little different with the addition of the pre-tournament festivities near Riverfront Park, but by and large, the city looks as it should. Then, somehow, merely hours later, 42 city blocks have been closed off, cars replaced by basketball courts.
The largest three-on-three basketball tournament in the world needs roughly 3,000 volunteers to make the event tick, but setting up the infrastructure takes far less —about 125 dedicated folks.
"From the guys that drive the trucks to bring in the stuff to the forklift drivers, a lot of those guys have been doing it for a long time, and the people who oversee them have been doing that for a long time," says Davis, Hoopfest site manager.
The experience of the volunteers, coupled with Davis' exhaustive planning, allows for a rapid setup process.
"We close the streets at 7 pm Friday night," Davis says. "They should pretty much have 461 courts built and taped by midnight."
That's five hours, and there's a Shock game at Spokane Arena on Friday night, which prevents nearby courts from being built until 10 pm. Physically setting up the event takes place in an amazingly short period of time. But for Davis, the physical setup process began a few months back at a warehouse east of downtown.
"I started in early April bringing the [baskets] out of the warehouse," Davis says. "Right now all of these baskets — and there are 25 semi-truck loads of baskets — are all staged in specific loads."
Between the initial sorting of baskets into loads and actually loading them up onto the trucks, Davis had to make one very important group happy: the sponsors. All 461 of the backboards are emblazoned with a sponsor's logo. As it turns out, it's not easy being a backboard — and not just because their job is to get hit by flying basketballs.
"A lot of the backboards have been damaged," Davis said. "So we have to take inventory and see how many are damaged. The ones that are damaged need to be redone. That takes all the way up through May."
Then, on the Wednesday and Thursday before Hoopfest, those 25 semi-truck loads are moved into downtown. The baskets are unloaded at staging locations — parking meters or lots near their final court location. Davis and his crews divide the city center into four zones, each with between 115 and 120 courts. At each zone there is just one forklift.
Markings along the curb, measured and set in advance to assure that the all courts fit, at the proper size, aid crews in placing the baskets and laying tape. One possible slowdown comes in the tape-laying process.
Last year, rain caused a bit of a scare as wet streets initially prevented tape from sticking, but the volunteers got the job done and Hoopfest carried on.
"Obviously we couldn't do this without the volunteers," Davis says. "Everybody who does this is a volunteer. There are only six full-time employees. It's that unique relationship that really sets this town apart for doing these kind of things."
So it's not just meticulous planning by one of six full-time employees, coupled with a team of efficient volunteers. Spokane also helps set up Hoopfest.
"Spokane's a unique setting," Davis said. "That's why it doesn't work in other places." ♦


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Freezing Rain
While taking a bowl of kitchen waste out to the compost pile yesterday I noticed some rain had frozen on the Red Russian kale leaves. So beautiful, especially with the purple veins of the kale running underneath it!
This is what you get when you have a 50 degree day with rain and a 30 degree drop in temperature by nightfall. Everything is covered in tiny jewels the next day!
4 Comments to "Freezing Rain"
You capture some of the greatest things in your photos!!!
to Kelly's comment
What beautiful photos! I think I'm going to have to look at raindrops a little more closely now!
to MeghanO's comment
Those pictures are incredible!
to Allie's comment
Wow that's gorgeous.
to AgrarianLife's comment


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I M Wright, B J Fraser, F W Menk
Cooperative Research Centre for Satellite Systems
Department of Physics
University of Newcastle
Apparent drift motion of polar cap arcs may be indicative of plasma convection processes in the ionospheric plasma. The dynamics of a number of individual polar cap events observed by a dual wavelength allsky imager at Scott Base have been analysed in detail. The imager, which records optical emissions at 630 nm and 428.7 nm has been operated at Scott Base, (-79.96°, 327.61° magnetic), during the winters of 1996 to 1998. The events presented have been selected to show representative examples of arcs observed primarily in the dayside. Of interest is the speed and direction of the polar cap arc drift motion with respect to solar wind and interplanetary magnetic field conditions. Events were observed between 10:00 and 19:00 local time (mid-morning to dusk), where drift velocities varied between 60 m/s away from the invariant pole and 1000 m/s polewards. Another example shows a drift velocity of 300 m/s perpendicular to the pole direction. Each of the examples shows different velocities and drift direction, for differing solar wind conditions, and different times. The small number of images in the initial data set needs to be expanded into a full three year data set, and include data from other instruments, in order to fully understand the correlations of polar cap arc drifts with solar wind/interplanetary magnetic field (IMF) conditions.
The observation of optical auroral forms that occur in the polar cap has led to the identification, and naming, of a wide range of emissions including: polar cap arcs, extremely high latitude auroras, sun aligned arcs, transpolar arcs, horse collar auroras, and theta aurora. It is difficult to interrelate these as they have been defined by various authors under a wide range of conditions and over a period of observations that began in 1907. In a recent review paper, Zhu, et al., [1997] use the term polar cap arc to differentiate aurora seen in the polar cap or poleward of the auroral oval from auroral oval emissions. Unlike auroral zone arcs these are seen more during northward IMF and quiet magnetic conditions . Early observations, made visually, and by film based allsky camera, identified properties of polar cap arcs including the Sun-Earth orientation, transverse motions, the occurrence only at high latitude, and the negative correlation with magnetic activity.
The launching of low Earth orbit satellites in the 1970's, for example the DMSP series, enabled particle measurements to be related to optical emissions [Hardy et al, 1982 ]. However, the orbits limited these studies to relatively local regions, and spin scanning resulted in coarse resolution in time and position. UV imaging and the high altitude elliptical orbit of DE 1 in the 1980's led to the first view of the theta aurora spanning the entire polar cap, a phenomenon that ISIS 2 and DMSP could not see. The DE-1 and 2 satellites found that polar cap arc precipitation had plasma sheet or plasma sheet boundary layer (PSBL) characteristics suggesting the arcs occur on closed field lines [Peterson and Shelley, 1984; Frank, 1988]. This was supported by the observed conjugacy of transpolar arcs [Craven, et al., 1991]. However, others, (e.g. Hardy et al ,1982; Gussenhoven and Mullen, 1989), have seen polar rain and relativistic electrons near polar arcs suggesting a source on open field lines. It is still not clear whether polar cap arcs occur on open or closed field lines, or whether the same phenomenon can arise under either of these conditions. (The review by Zhu, et al., [1997] contains comprehensive references)
Continued observations of high latitude optical emissions are needed to resolve questions about their relationship to open/closed field lines, and equally importantly, to the ionosphere convection that accompanies them. This study uses images of polar cap aurora acquired at Scott Base to investigate the scale, the motions, and dynamics of these phenomena to examine these questions. In particular the behaviour of small scale, relative to the polar cap, arcs of less than 1000 km length are noted.
An Allsky digital imager has been operating at Scott Base, Antarctica since 1996 to record optical phenomena during the darkness of the Antarctic winter. The first season of operation produced some 28 days of data when aurora was visible for some time during the 24 UT hours, over the 1996 Austral winter. In 1997, the second season, 22 days of useful data were obtained. All the data from the first two seasons were recorded during quiet magnetic conditions, Kp ~ 2. The presence of cloud, or interference from sun or moon light, prevented collection of image from other times. For 1998, there were 36 days of good data recorded, some during more active conditions. Out of the data from the three operation periods, on some 38 occasions the drift motion of detected arcs have been selected for further study. The intensity and structures of arcs can vary during their lifetime. The average lifetime is some tens of minutes, but they occasionally exist for longer than 1 hour.
New Zealand's Scott Base Station is at Pram Point on Ross Island in the Ross Sea, and the US base, Mc Murdo, is a few kilometres away at Discovery Point. Both New Zealand and the USA each have a permanent observatory/laboratory at Arrival Heights which is about 60 metres above sea level, and four kilometres inland from the coast. Arrival Heights is located at 77 ° 49' 46" S, 166°39' 40" E geographically and is -79.96°, 327.61° CGM magnetic. This geographic location experiences total darkness at local noon for several weeks as the Sun is below the horizon during winter. These conditions allow the study of dayside emissions that normally are invisible.
Figure 1, which superimposes the quiet time (Kp ~ 2) auroral oval of Feldstein and Starkov [1967] for each 6 hour interval over the map of Antarctica, shows Scott Base, (SB), is completely within the polar cap, except for the hours around 1800 UT, when the quiet time auroral oval may also enter the field of view. The circle, which is centred on Scott Base, represents a 1000 km diameter field of view (see section 2.3), and the auroral oval is shown rotating around the fixed imager location. The direction to the sun is indicated by the arrows. This Figure shows the upwards looking imager view, and the superimposed map of Antarctica is reversed left to right. In the images, the direction to the geomagnetic pole (MP) is to the upper left at 45°. The geographic pole is labelled "SP". At Scott Base, local solar noon is at 0056 UT.
Observations are recorded as two side by side circular horizon to horizon images of the sky. The left image contains 630 nm wavelength information and the right hand image is of 427.8 nm. There are examples presented in the later Figures. The Allsky system is housed in Antarctica New Zealand's Arrival Heights laboratory using a light trap below a glass dome in the roof. Room temperature air from the laboratory is circulated through the light trap and dome to minimise icing inside the dome. Figure 2 shows the schematic arrangement of the imager. It was manufactured by Keo Consultants of Boston and is similar to units used by the US at South Pole station and the US PENGUIn research project. Keo Consultants also supplied a different version of the instrument to the Australian Antarctic Division. A Canon 16 mm focal length "fish eye" lens creates a horizon to horizon image of the sky. This image is collimated so essentially parallel rays are passed through a dual pass band interference filter that only passes 630 nm and 428.7 nm wavelengths to a beam splitting prism. The prism produces the two side by side images of the whole sky, one image has the 427.8 nm wavelength removed by another interference filter, and the other has the 630 nm information removed.
These side by side images, are focussed onto an image intensifier. Keo Consultants documentation states the system detects minimum emissions of 50 Rayleigh. An intensifier is needed to detect optical emissions of this level. This intensifier was developed for night time military uses and has ramifications that will be discussed later. The output intensifier image is scanned by a CCD television camera. The camera includes a power supply for the intensifier, the TV camera, a rough calibration light, and a mechanical shutter below the objective lens that is interlocked with a light detector. The shutter and light dependant resistor protect the image intensifier from the damage that would result if an image of the sun was allowed to fall on the input.
Under normal operation the Allsky camera will take a pair of exposures every thirty seconds. One exposure of 0.9 seconds duration, and the other 0.3 s are achieved by allowing the CCD to integrate for these periods by suspending the normal television scanning at 25 frames per second. These automatically gain controlled images are 8-bit digitised, compressed, and then written to magneto-optical disc. In this paper we concentrate on the 0.9 s exposures which provide more detailed images than the 0.3 s exposures. The operation of the system is software controlled from a dedicated PC, with a video monitor for image display.
Auroral properties that can be observed from the ground include; apparent extent, apparent velocity, and apparent intensity. From a single observation point, assumptions need to be made to estimate actual values for these parameters. These assumptions depend on the performance of the of the observing device, and experience based on observations and results from previous work.
The electron - oxygen reaction that produces the red 630 nm radiation occurs at altitudes from 200 km to as high as 450 km, depending on atmospheric conditions such as the concentration of oxygen. [Carlson and Egeland, 1995]. The nitrogen - electron reaction responsible for the blue 427.8 nm emissions only occurs lower in the ionosphere, at about 120 km altitude. Estimates of size and movement of auroral events need to take the altitude into consideration.
An arbitrary assumption we make is that the red image occurs at an altitude of 250 ± 50 km, a Figure used by other workers e.g. Sandholt, et al., 1998, which is twice the assumed altitude of the blue image. A 1000 km diameter field of view used in this study corresponds to the 120 km altitude maximum field of view (FOV) of the lens. The geometry of the fish-eye lens compresses the image to the edges of the field so that the central 250 km diameter of sky occupies half the image. The resolution of the 256 by 256 pixel system is very coarse at the edge of the FOV and only very large scale features can be discerned away from the centre of the images. Small scale arcs, relative to the scale of the polar cap, can be well resolved in the centre 250 km area, and it is the behaviour of narrow arcs of less than 1000 km in length that is studied here.
The recorded image is dependent on the instantaneous response of a photon cascade device (the image intensifier) and consequently there is an inherent uncertainty in the level of the recorded signal. The effect of the image intensifier is shown in Figure 3. This shows the response of the imager system during tests made to back calibrate the first season's data on the laboratory bench. A low light intensity test target using light emitting diodes (LED's) was constructed. This consisted of a grey square mounted in a matt black light proof box. The camera could be operated seeing only this square, filling the central third of the field of view, with all extraneous light excluded. The voltage fed LED light source could be varied to produce images with the same intensities as natural signals found in observed arcs. The images recorded from this test box consist of a square in the centre of each of the red and blue side by side images. Allowing for the uneven illumination in the test box, a horizontal scan of intensities across the centre line of this test image should show an increase and then a decrease at the target square boundaries in each of the red and blue images, with a reasonable plateau between.
The plot in Figure 3(a) shows the response across line 128 (out of 256 lines) in one 0.9 second image recorded from the test target. The y-axis values are arbitrary pixel intensities which vary between 0 and 255, as determined by the intensifier gain and the compression software. In this instance the maximum is about 65, which is comparable with intensities from many auroral events. The x-axis is the pixel location number across the image. The edges of the square in the red image are seen at pixel 48 and at pixel 90, and in the blue image at about 153 and about 200 in Figure 3(a). Ideally, all test images recorded under identical conditions should be the same. In Figure 3(b), the response for another five images (0.9 s) recorded successively every 2 seconds with the same target are superimposed on the original plot of Figure 3(a). In Figure 3(b), the single trace response is not replicated. A broadly similar response to Figure 3(a) is seen, but due to the variability of the intensifier, the only boundary edge that remains well defined is at pixel 90.
In Figure 3(c) the range of the six traces from Figure 3(b) is shown, with arrows marking points of interest. The edges remain reasonably well defined in the red and blue images, provided that the response is above the noise level. This is indicated by the vertical arrows. The approximate background noise (intensity level 22 ±3 in the field data, and in the tests) is indicated by the horizontal dashed line. The oblique arrow shows where the response in the blue image is sufficiently low to be lost in system noise even when a blue target is present.
It is seen that successive images of an unchanging target are not identical pixel by pixel, but can vary by about 25%. Averaged over time and area the variable response of the intensifier should, for a constant signal, provide a meaningful average response. However, in this application of an image intensifier a significant error must result when capturing single images of aurora that vary in both time and space. The recorded intensity could be anywhere within the 25% band. The recorded position of edges of arcs in the images has an error range of about 5% however. By estimating the centre of an arc in the red images, and allowing for altitude, reliable velocity estimates can be made.
There are many examples in the field data of blue arcs apparently switching on or off in successive exposures which is explained by the system's blue response shown in Figure 3(c). As the result of the testing, it is apparent that absolute calibration of the system is not possible, and intensity ratios of instantaneous red/blue images are unreliable. Intensity ratios have not been used in this study.
The Allsky data recorded over the Antarctic winters has provided many images where the aurora has been well enough defined, and of sufficient intensity, to make reasonable deductions of spatial and temporal characteristics using the altitude assumptions mentioned above. The motion of polar cap arcs may display an aspect of overall ionosphere convection , or they may be quite localised. Examples of polar cap auroras discussed here have been selected for events displaying a definite drift motion. The prevailing IMF conditions (projected from upstream), which indirectly drive ionospheric convection are also presented for these events. These examples show polar arc drift motion can be quite varied.
On this day between 23:23:00 and 23:31:30 UT, as shown in Figure 4, a very bright, broad, roughly sun aligned arc formed from the SSE, where it was attached to the auroral oval, extending to the NNW. It moved poleward, (to the west) as a loop, and then collapsed to the south within 6 minutes. At the south east, where this arc was connected to the auroral oval, it did not show much movement. The auroral oval, which should be seen in the lower left of the images is partly obscured by icing inside the dome. The thumbnail, Figure 4(a), shows the raw image of 23:27:00 UT, and the composite negative image, (b), shows the positions of the arc every 30 seconds, moving from east to west for the period in the red image. The blue image (right side) shows positions of the arc between 23:25:00 and 23:28:30 UT. Here is an example of the blue image apparently switching on and off, as mentioned above. Assuming an altitude of 250 km for the red emissions, the westward velocity was 500 ±80 m/s over the centre of the field of view. At this time the direction to the sun is just east of north, and is indicated by the arrowhead. Figure 4(c) shows the solar wind conditions from the WIND spacecraft Magnetic Field Instrument (MFI) data. The vertical line labelled 23:24 eq relates to the conditions expected at the Earth at the time of the event, taking into consideration the prevailing solar wind velocity and travel time to the magnetopause. Kp was 1-, Bz was weakly positive, having been so mostly for the previous hours, By was also weakly positive, Bx at 23:24 eq was negative. The total B field was about 5 nT. There were two other similar arc events, with similar short lives, though not as intense, during the period 22:00 June 20 to 00:35 June 21, around mid day local time, with drift motion towards the invariant pole.
The thumbnail, Figure 5(a), shows the raw image seen at 21:52 UT. This event also occurred just before local noon. A sun aligned arc is visible in both red and blue images above dawn and cloud interference. The arc drift motion is eastwards, away from the magnetic pole. The composite image, Figure 5(b) shows positions of this arc, which had a slower drift motion, every 2 minutes between 21:37 and 21:59 UT. At the end of this period the arc collapses lengthwise to a vestige patch in the south, after experiencing eastward drift velocities of between 60 ±8 m/s and 200 ±25 m/s. The higher velocity was seen in the south. Kp= 2 at 21:00 UT. As seen in Figure 5(c), where the vertical line indicates the conditions projected to a time within this event, Bz = 0, and had been for the preceding hour. By, Bx_ -2 nT with Btot = 5 nT. For the drift direction of this arc By was negative while for the 1996 June 20 event described above By was positive.
The raw image, Figure 6(a), is shown for 22:10:00 UT, one of the images used to make the composite image in Figure 6(b). This shows the locations of this arc every 30 seconds, in the red image, between 22:08:00 UT, the initial position, and 22:14:00 UT when it faded from view. Again the blue image is visible for less time than the red one. There is interference from the sun at the top left of the images, and the moon at the top right, and again there is some ice inside the dome on the lower left side of the images. This arc, another example from before local noon, apparently rotated about its northern end. The velocity overhead was about 500 ±65 m/s while at the south end it could have exceeded 1000 ±125 m/s. Again in Figure 6(c) the MFI data with the prevailing conditions indicated shows the total B tot field strength was of the order of 5 nT and had been stable for the previous hour or two, By = +2 nT, and Bx_-2 nT this time. B z was positive, about +2 nT, before the event, and although fluctuating, it remained mostly positive throughout the event. While the north end of this arc remained fixed, the rotation of the southern end was towards the pole.
This arc, shown in Figure 7 moved north at about 300 ±40 m/s from 06:50 UT to arrive overhead at about 07:02 where it remained until fading into cloud/interference. This corresponds to 19:00 local time, around dusk. The thumbnail Figure 7(a) shows the raw data at 07:05 UT. There is no information in the blue image due to the presence of the moon. (A small spot visible 180° from the moon in the red image is a reflection of the moon from the inside of the spherical dome). In the composite image, Figure 7(b), the positions at 2 minute intervals from 06:50 until 07:16 UT are shown. This arc is again essentially aligned with the sunwards direction, the sun being west-south-west at the time. The solar wind data are shown in Figure 7(c) with the projected time of the arc onset marked. The B tot field is greater than the previous examples at around 10 nT and is more variable. Bx was between 8 nT and 5 nT for the preceding period, and remained positive. By was strongly negative at -10 nT, and had been negative for some time. Bz shows a sudden increase from around 1 nT to 6 nT at the start of this event. However as the viewing conditions were not perfect it is not possible to know if we have detected the actual birth of this event, or if it became visible after it was established.
The drift velocities of the first three arcs presented here were, 500 m/s poleward, 200 m/s anti-poleward, and a "rotating" arc with up to 1000 m/s poleward motion, all recorded around local noon. The relation of the By direction to the poleward/anti poleward drift motion in these specific examples is in agreement with the findings reported by Valledares et al., [1994], that the east-west component of the IMF can control drift motion. The fourth event, from 0700 UT (local dusk), shows a drift of 300 m/s northwards which is unrelated to the poleward direction. This arc is aligned with the sun direction. As stated before, all the polar cap arc examples presented here, and observed so far in the study are associated with northwards IMF. This is expected from reports in all the previous literature. The rotation of polar cap arcs is not well documented.
The four examples here were selected to show that there are several differing drift motion regimes. Detailed examination of the other identified events in our data is needed to establish trends. The images selected here represent some aspects of polar cap arc phenomena. Our data does contain aurora from the oval, and arcs that can be sufficiently long in extent to span the entire field of view. The straight or nearly straight localised arcs, aligned sunwards, or to the cusp (Valledares, et al., 1994) direction described here are unique to polar cap conditions. Specific examples that occur when reliable satellite data on IMF and solar wind are also available, are therefore potentially useful to examine in detail.
It is not clear whether these arcs occur on magnetic field lines that are "open" to the interplanetary magnetic field, or field lines that map back into the magnetotail. Where the field lines map depends on the model of convection that applies, and more evidence is needed to justify either or both propositions. This paper presents preliminary observation results and the relation of these events with IMF By, Bx, and solar wind conditions will be expanded. Specific events will be related to data from magnetometers, riometers, and other photometers from the polar cap PENGUIn and AGO program and ionospheric convection patterns.
The assistance of Antarctica New Zealand personnel at both Scott Base and Christchurch, New Zealand is gratefully acknowledged. This research was supported by a grant from the Australia Research Council, the University of Newcastle, and the Cooperative Research Centre for Satellite Systems with financial support from the Commonwealth of Australia through the CRC program.
Carlson(Jr), H.C., and A. Egeland, The Aurora and the Auroral Ionosphere, in Introduction to Space Physics eds Kivelson M.G., and C.T. Russell, Cambridge University Press, New York, 1995.
Craven, J.D., J.S. Murphree, L.A. Frank, and L. Cogger, Simultaneous optical observations of transpolar arcs in the two polar caps, Geophysical Research Letters, Vol 18 No 12, 2297-2300, 1991.
Feldstein, Y.I., and G. V. Starkov, Dynamics of the Auroral Belt and Polar Geomagnetic Disturbances, Planet. Space Sci., Vol 15, 209, 1967
Frank, L.A., Dynamics of the near-Earth magnetotail: Recent observations, Modelling Magnetosphere Plasma, Geophysical Monograph, 44, (T.E. Moore and J.H. Waite , Jr. ed)s, AGU, 261, 1988
Gussenhoven, M.S., and E.G. Mullen, Simultaneous relativistic electron and aurora particle access to the polar caps during interplanetary magnetic field Bz northwards: A scenario for an open field line source of auroral particles, Journal of Geophysical Research, 94 A12, 17121- 17132, 1989
Hardy, D.A., W.J. Burke, and M.S. Gussenhoven, DMSP optical and electron measurements in the vicinity of polar cap arcs, Journal of Geophysical Research, 87 A4, 2413-2430, 1982
Sandholt, P.E., C.J. Farrugia, J. Moen, and S.W.H. Cowley, Dayside auroral configurations: Responses to southward and northward rotations of the interplanetary magnetic field, Journal of Geophysical Research, 103 A9, 20,279-20,295, 1998.
Peterson W.K., and E.G. Shelley, Origin of the plasma in a cross-polar cap auroral feature (theta aurora), Journal of Geophysical Research, 89 A8, 6729-6736, 1984
Valledares, C.E., H.C. Carlson Jr, and K. Fukui, Interplanetary magnetic field dependency of stable Sun-aligned polar cap arcs, Journal of Geophysical Research, 99 A4, 6247-6272, 1994.
Zhu, L., R.W. Schunk, and J.J. Sojka, Polar cap arcs: a review, Journal of Atmospheric and Solar-Terrestrial Physics, Vol 59 (No 10), 1087-1126, 1997.


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Roll Chair, Height Adjustable, Small-
Roll Chair, Height Adjustable, Small
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