Publication Date:
2007-12-08
Description:
The heating of the solar chromosphere and corona is a long-standing puzzle in solar physics. Hinode observations show the ubiquitous presence of chromospheric anemone jets outside sunspots in active regions. They are typically 3 to 7 arc seconds = 2000 to 5000 kilometers long and 0.2 to 0.4 arc second = 150 to 300 kilometers wide, and their velocity is 10 to 20 kilometers per second. These small jets have an inverted Y-shape, similar to the shape of x-ray anemone jets in the corona. These features imply that magnetic reconnection similar to that in the corona is occurring at a much smaller spatial scale throughout the chromosphere and suggest that the heating of the solar chromosphere and corona may be related to small-scale ubiquitous reconnection.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Shibata, Kazunari -- Nakamura, Tahei -- Matsumoto, Takuma -- Otsuji, Kenichi -- Okamoto, Takenori J -- Nishizuka, Naoto -- Kawate, Tomoko -- Watanabe, Hiroko -- Nagata, Shin'ichi -- Ueno, Satoru -- Kitai, Reizaburo -- Nozawa, Satoshi -- Tsuneta, Saku -- Suematsu, Yoshinori -- Ichimoto, Kiyoshi -- Shimizu, Toshifumi -- Katsukawa, Yukio -- Tarbell, Theodore D -- Berger, Thomas E -- Lites, Bruce W -- Shine, Richard A -- Title, Alan M -- New York, N.Y. -- Science. 2007 Dec 7;318(5856):1591-4.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Kwasan and Hida Observatories, Kyoto University, Yamashina, Kyoto 607-8471, Japan. shibata@kwasan.kyoto-u.ac.jp〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/18063790" target="_blank"〉PubMed〈/a〉
Print ISSN:
0036-8075
Electronic ISSN:
1095-9203
Topics:
Biology
,
Chemistry and Pharmacology
,
Computer Science
,
Medicine
,
Natural Sciences in General
,
Physics
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