High-Energy Gamma Radiation of Solar Flares as an Indicator of Acceleration of Energetic Protons

Viktoriya G. Kurt; B. Yu. Yushkov; K. Kudela; V. I. Galkin

首页> 外文期刊>Cosmic research >High-Energy Gamma Radiation of Solar Flares as an Indicator of Acceleration of Energetic Protons

【24h】

High-Energy Gamma Radiation of Solar Flares as an Indicator of Acceleration of Energetic Protons

机译：太阳耀斑的高能伽马辐射作为高能质子加速的指标

获取原文

获取原文并翻译 | 示例

掌桥外文数据库（机构版） >>

开具论文收录证明 >>

文献代查 >>

页面导航

摘要
著录项
相似文献
相关主题

摘要

Using the SONG detector onboard the CORONAS-F satellite, gamma-ray emission of high energies (>100 MeV) was recorded during four solar flares. In the sequential spectra of gamma rays the peculiarity caused by generation and decay of neutral pions was isolated, which made it possible to determine with a high accuracy the moments of appearance in the solar atmosphere of protons accelerated up to energies above 300 MeV.

机译：使用CORONAS-F卫星上的SONG探测器，在四个太阳耀斑期间记录了高能（> 100 MeV）的伽马射线发射。在伽马射线的连续光谱中，分离了由中性离子的生成和衰减引起的特殊性，这使得可以高精度确定质子在太阳大气中的出现时刻，该质子加速到300 MeV以上的能量。

著录项

来源
《Cosmic research》 |2010年第1期|p.70-79|共10页
作者
Viktoriya G. Kurt; B. Yu. Yushkov; K. Kudela; V. I. Galkin;
展开▼
作者单位

Skobeltsyn Institute of Nuclear Physics, Moscow State University, Moscow, 119991 Russia;

rnSkobeltsyn Institute of Nuclear Physics, Moscow State University, Moscow, 119991 Russia;

Institute of Experimental Physics, Slovak Academy of Sciences, Kosice, 04353 Slovakia;

rnSkobeltsyn Institute of Nuclear Physics, Moscow State University, Moscow, 119991 Russia;

展开▼
收录信息
原文格式 PDF
正文语种 eng
中图分类
关键词

相似文献

外文文献
中文文献
专利

1. The possible existence of high-energy gamma radiation (E_#gamma#r>30 MeV)during solar optical class SF and 3N flares [J] . A M Galper, Yu V Ozerov, A M Khodarovich, Journal of the Moscow Physical Society . 1999,第1期

机译：在太阳光学SF级和3N耀斑期间可能存在高能伽玛辐射（E_＃gamma＃r> 30 MeV）
2. The possible existence of high-energy gamma radiation (E_#gamma#r>30 MeV)during solar optical class SF and 3N flares [J] . A M Galper, Yu V Ozerov, A M Khodarovich, Journal of the Moscow Physical Society . 1999,第1期

机译：在太阳光学SF级和3N耀斑期间可能存在高能伽玛辐射（E_＃gamma＃r> 30 MeV）
3. Hα POLARIZATION DURING A WELL-OBSERVED SOLAR FLARE: PROTON ENERGETICS AND IMPLICATIONS FOR PARTICLE ACCELERATION PROCESSES [J] . A Gordon Emslie, James A Miller, Ethienne Vogt The Astrophysical journal . 2000,第1期

机译：良好观测的太阳耀斑中的Hα极化：质子能量学及其对粒子加速过程的影响
4. Energetics of Nonthermal Electrons and Protons in Intense Solar Flares [C] . Masato Yoshimori, Hiroshi Hirayama, Sunao Mori International Cosmic Ray Conference . 2003

机译：强烈的太阳耀斑的非热电子和质子的能量学
5. Coronal shock acceleration and heliospheric transport of solar energetic protons. [D] . Kozarev, Kamen Asenov. 2013

机译：日冕冲击加速和太阳高能质子的日球运输。
6. Self-generated surface magnetic fields inhibit laser-driven sheath acceleration of high-energy protons [O] . M. Nakatsutsumi, Y. Sentoku, A. Korzhimanov, -1

机译：自生表面磁场会抑制高能质子的激光驱动鞘层加速
7. Comparing Long-duration Gamma-Ray Flares and High-energy Solar Energetic Particles [O] . G. A. de Nolfo, A. Bruno, J. M. Ryan, 2019

机译：比较长时间伽马射线耀斑和高能太阳能粒子

High-Energy Gamma Radiation of Solar Flares as an Indicator of Acceleration of Energetic Protons

摘要

著录项

相似文献

相关主题

期刊订阅