Observation and numerical modeling of chromospheric evaporation during the impulsive phase of a solar flare-Reference-Cited by-同舟云学术

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Observation and numerical modeling of chromospheric evaporation during the impulsive phase of a solar flare

Published:2015-10 Issue:10 Volume:22 Page:101206
ISSN:1070-664X
Container-title:Physics of Plasmas
language:en
Short-container-title:Physics of Plasmas

Author:

Imada Shinsuke¹,Murakami Izumi²³,Watanabe Tetsuya⁴⁵

Affiliation:

1. Institute for Space-Earth Environmental Research, Nagoya University, Furo-cho, Chikusa-ku, Nagoya, Aichi 464-8601, Japan

2. National Institute for Fusion Science, 322-6 Oroshi-cho, Toki, Gifu 509-5292, Japan

3. Department of Fusion Science, SOKENDAI (The Graduate University of Advanced Studies), Toki, Gifu 509-5292, Japan

4. National Astronomical Observatory of Japan, Mitaka, Tokyo 181-8588, Japan

5. Department of Astronomical Science, SOKENDAI (The Graduate University of Advanced Studies), Mitaka, Tokyo 181-8588, Japan

Funder

Japan Society for the Promotion of Science (JSPS)

Publisher

AIP Publishing

Subject

Condensed Matter Physics

Link

http://aip.scitation.org/doi/pdf/10.1063/1.4932335

Reference41 articles.

1. H. Carmichael , in The Physics of Solar Flares, edited by W. N. Hess ( NASA, NASA Special Publication 50; Washington, DC, 1964), p. 451.

2. Model of the High-Energy Phase of Solar Flares

3. Theoretical model of flares and prominences

4. Magnetic reconnection in the corona and the loop prominence phenomenon

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