The most energetic solar flares - detection of solar neutrons and solar cosmic rays -

被引：0

作者：

Muraki, Yasushi ^{[1
]}

机构：

[1] Konan Univ, Dept Phys, Higashinada Ku, Kobe, Hyogo 6588501, Japan

来源：

NUCLEAR PHYSICS B-PROCEEDINGS SUPPLEMENTS | 2009年 / 196卷

关键词：

TELESCOPE;

D O I：

10.1016/j.nuclphysbps.2009.09.051

中图分类号：

O412 [相对论、场论]; O572.2 [粒子物理学];

学科分类号：

摘要：

In this talk, I show a typical example of a solar flare event on April 15, 2001 that clearly suggests the particle acceleration mechanism. Then I propose that solar physics is the easiest way to demonstrate the particle acceleration mechanism. In the flare of April 15, 2001, particles were accelerated beyond 56 GeV. The event is highly consistent with the hypothesis that particles are accelerated by the shock acceleration mechanism. The acceleration site was clearly observed by the Yohkoh X-ray telescope and making it possible to compare the Yohkoh X-ray data with ground-based detector data.

引用

页码：267 / 272

页数：6

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