Spectral peculiarities of high energy X-ray radiation, gamma radiation, and Submillimeter radio emission in the impulsive phase of a solar flare
dc.contributor.author | Makhmutov V.S. | |
dc.contributor.author | Kurt V.G. | |
dc.contributor.author | Yushkov B.Yu. | |
dc.contributor.author | Grechnev V.V. | |
dc.contributor.author | Kaufmann P. | |
dc.contributor.author | Raulin J.-P. | |
dc.contributor.author | Bazilevskaya G.A. | |
dc.contributor.author | Stozhkov Yu.I. | |
dc.date.accessioned | 2024-03-13T01:11:09Z | |
dc.date.available | 2024-03-13T01:11:09Z | |
dc.date.issued | 2011 | |
dc.description.abstract | 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). © 2011 Allerton Press, Inc. | |
dc.description.firstpage | 747 | |
dc.description.issuenumber | 6 | |
dc.description.lastpage | 750 | |
dc.description.volume | 75 | |
dc.identifier.doi | 10.3103/S106287381106030X | |
dc.identifier.issn | 1062-8738 | |
dc.identifier.uri | https://dspace.mackenzie.br/handle/10899/36981 | |
dc.relation.ispartof | Bulletin of the Russian Academy of Sciences: Physics | |
dc.rights | Acesso Restrito | |
dc.title | Spectral peculiarities of high energy X-ray radiation, gamma radiation, and Submillimeter radio emission in the impulsive phase of a solar flare | |
dc.type | Artigo | |
local.scopus.citations | 3 | |
local.scopus.eid | 2-s2.0-79960502649 | |
local.scopus.subject | Argentina | |
local.scopus.subject | CORONAS-F | |
local.scopus.subject | Energy ranges | |
local.scopus.subject | Energy spectra | |
local.scopus.subject | Experimental data | |
local.scopus.subject | Frequency spectra | |
local.scopus.subject | Ground-based observations | |
local.scopus.subject | High energy x-rays | |
local.scopus.subject | Impulsive phase | |
local.scopus.subject | Radio emission | |
local.scopus.subject | Solar events | |
local.scopus.subject | Solar flare | |
local.scopus.subject | Solar X-rays | |
local.scopus.subject | Submillimeters | |
local.scopus.subject | Temporal behavior | |
local.scopus.subject | Wide frequency range | |
local.scopus.updated | 2024-05-01 | |
local.scopus.url | https://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=79960502649&origin=inward |