Spectral peculiarities of high energy X-ray radiation, gamma radiation, and Submillimeter radio emission in the impulsive phase of a solar flare

Makhmutov V.S.; Kurt V.G.; Yushkov B.Yu.; Grechnev V.V.; Kaufmann P.; Raulin J.-P.; Bazilevskaya G.A.; Stozhkov Yu.I.

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Spectral peculiarities of high energy X-ray radiation, gamma radiation, and Submillimeter radio emission in the impulsive phase of a solar flare

机译：太阳耀斑的脉冲相中高能X射线辐射，γ辐射和亚毫米波辐射的光谱特性

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We analyze experimental data on the temporal behavior of fluxes and energy spectra of hard solar X-ray and gamma radiation in the energy range of 0.015 to 300 MeV, obtained onboard the CORONAS-F satellite during a solar flare on August 25, 2001. These data are compared with measurements of the radio emission fluxes over the wide frequency range of 1-405 GHz. For our analysis, we use data obtained onboard the YOHKOH, TRACE and GOES satellites, along with ground-based observations of this solar event using the Solar Submillimeter Telescope (SST; Argentina). For the first time, we find nearly simultaneous changes in the energy spectra of gamma radiation over the range 10-150 MeV and the frequency spectrum of radio emission at the beginning and during a impulsive phase of this event (whose duration did not exceed three minutes).

机译：我们分析了2001年8月25日太阳耀斑期间在CORONAS-F卫星上获得的，在0.015至300 MeV能量范围内的硬太阳X射线和伽马射线通量和能谱的时间行为的实验数据。将数据与1-405 GHz宽频率范围内的无线电发射通量的测量结果进行比较。对于我们的分析，我们使用从YOHKOH，TRACE和GOES卫星上获得的数据，以及使用太阳亚毫米望远镜（SST;阿根廷）对该事件的地面观测。第一次，我们发现在此事件的开始和冲动阶段（持续时间不超过三分钟），在10-150 MeV范围内的伽马辐射能谱和无线电发射的频谱几乎同时发生变化）。

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《Bulletin of the Russian Academy of Sciences. Physics》 |2011年第6期|共4页
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Makhmutov V.S.; Kurt V.G.; Yushkov B.Yu.; Grechnev V.V.; Kaufmann P.; Raulin J.-P.; Bazilevskaya G.A.; Stozhkov Yu.I.;
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中图分类物理学;
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1. Spectral peculiarities of high energy X-ray radiation, gamma radiation, and Submillimeter radio emission in the impulsive phase of a solar flare [J] . Makhmutov V.S., Kurt V.G., Yushkov B.Yu., Bulletin of the Russian Academy of Sciences. Physics . 2011,第6期

机译：太阳耀斑的脉冲相中高能X射线辐射，γ辐射和亚毫米波辐射的光谱特性
2. Analysis of Intermittency in Submillimeter Radio and Hard X-Ray Data During the Impulsive Phase of a Solar Flare [J] . Gimenez de Castro G., Simoes P. J. A., Raulin J. -P., Solar physics . 2016,第7期

机译：太阳耀斑脉冲阶段亚毫米波无线电和硬X射线数据的间歇性分析
3. Production of energy-dependent time delays in impulsive solar flare hard X-ray emission by short-duration spectral index variations [J] . T.N.Larosa, Steven N.Shore The Astrophysical journal . 1998,第1期

机译：通过短时光谱指数变化在脉冲太阳耀斑硬X射线发射中产生与能量有关的时间延迟
4. Large solar flares of October - November, 2003 - development in Soft X-ray, Hard X-ray and gamma-ray emissions [C] . Sergey N. Kuznetsov, V. G. Kurt, I. N. Myagkova, International Astronomical Union . 2004

机译：2003年10月 - 11月的大型太阳耀斑 - 软X射线，硬X射线和伽马射线排放的开发
5. X-ray observations of the impulsive phase of solar flares with the Yohkoh satellite. [D] . Phillips, Andrew. 1997

机译：用Yohkoh卫星对太阳耀斑的脉冲相位进行X射线观察。
6. Balance between Health Risks and Benefits for Outdoor Workers Exposed to Solar Radiation: An Overview on the Role of Near Infrared Radiation Alone and in Combination with Other Solar Spectral Bands [O] . Carlo Grandi, Maria Concetta D’Ovidio 2020

机译：暴露在太阳辐射下的户外工作人员的健康风险和收益之间的平衡：单独近红外辐射以及与其他太阳光谱带结合使用的概述
7. Analysis of intermittency in submillimeter radio and hard x-ray data during the impulsive phase of a solar flare [O] . Giménez de Castro G., Simões P.J.A., Raulin J.-P., 2016

机译：分析太阳耀斑冲动阶段亚毫米波无线电和硬X射线数据的间歇性

Spectral peculiarities of high energy X-ray radiation, gamma radiation, and Submillimeter radio emission in the impulsive phase of a solar flare

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