## Info

leg(EC0)

Fig. 4.29.1. Accelerated particle spectra at the sub-luminal shock wave ( u1 = 0.5c, y/1 = 45° and ub1= 0.71c) for (a) the flat (Eq. 4.29.1) and (b) the Kolmogorov (Eq. 4.29.2) wave spectrum of magnetic field perturbations. The upstream perturbation amplitude ¿.B/B01 = 0.3, 1.0, and 3.0 are given near the respective results. Linear fits to the power-law parts of the spectra are presented and values of the phase space distribution function spectral indices a = 3.08, 3.24, and 3.55 for (a) and a = 3.16, 3.43, and 3.69 for (b) are given. particles of energies in the range indicated by arrows can effectively interact with the magnetic field inhomogeneities (kmin < kres < kmax ). From Niemiec and Ostrowski (2003a).

The following features are visible in the spectra from Fig. 4.29.1:
{"ft_lang_label":"__label__en","ft_lang_prob":0.7946734,"math_prob":0.9893309,"size":837,"snap":"2020-10-2020-16","text_gpt3_token_len":267,"char_repetition_ratio":0.12244898,"word_repetition_ratio":0.0,"special_character_ratio":0.32258064,"punctuation_ratio":0.2,"nsfw_num_words":0,"has_unicode_error":false,"math_prob_llama3":0.98524106,"pos_list":[0],"im_url_duplicate_count":[null],"WARC_HEADER":"{\"WARC-Type\":\"response\",\"WARC-Date\":\"2020-04-02T08:19:21Z\",\"WARC-Record-ID\":\"<urn:uuid:ee6ef346-3102-42a0-9b5c-b6d523aca4a6>\",\"Content-Length\":\"11925\",\"Content-Type\":\"application/http; msgtype=response\",\"WARC-Warcinfo-ID\":\"<urn:uuid:e11ca91e-2fa8-440c-940e-e09bf0a476ce>\",\"WARC-Concurrent-To\":\"<urn:uuid:4e69a8a4-2a5d-4e00-84d3-62d4f6c54d15>\",\"WARC-IP-Address\":\"104.31.74.232\",\"WARC-Target-URI\":\"https://www.astronomyclub.xyz/particle-acceleration/info-lga.html\",\"WARC-Payload-Digest\":\"sha1:D3GXWAOX5SAMVGMF6WYNGD2XIIO43FI2\",\"WARC-Block-Digest\":\"sha1:C2F6N6NUW3MF53VO6F5U655YSZFCZZHB\",\"WARC-Identified-Payload-Type\":\"text/html\",\"warc_filename\":\"/cc_download/warc_2020/CC-MAIN-2020-16/CC-MAIN-2020-16_segments_1585370506870.41_warc_CC-MAIN-20200402080824-20200402110824-00545.warc.gz\"}"}