Zobrazeno 1 - 6
of 6
pro vyhledávání: '"Yu. A. Kupryakov"'
Publikováno v:
Annales Geophysicae, Vol 26, Pp 2975-2982 (2008)
We present results of the 18 August 2002 flare analysis as an example for developing a diagnostic tool for thermal and non-thermal processes in chromospheric lines. Taking into account the hard X-ray (HXR) emission, we attempted to derive the Hα
Externí odkaz:
https://doaj.org/article/4f4d7da298534c41898fe59e13efc755
Publikováno v:
Astronomy Reports. 65:876-883
We present the results of the analysis of the observational data for the eruptive event of June 7, 2011 obtained both on spacecraft (SDO, LASCO) and using ground-based solar instruments. The event was characterized by deceleration of the shock front
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::1b12c68d8d1e77f687c660fae5fa4107
https://doi.org/10.1134/s1063772921100188
https://doi.org/10.1134/s1063772921100188
Publikováno v:
Astronomical & Astrophysical Transactions. 26:267-273
On the occasion of the 175-year anniversary of the Moscow State University Sternberg Astronomical Institute we would like to outline the history and some results obtained by the Institute in cooperation with the Ondřejov Astronomical Institute of th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ab8422557928afb74c922e75c6c36823
https://doi.org/10.1080/10556790701415328
https://doi.org/10.1080/10556790701415328
Autor:
P. Schwartz, Petr Heinzel, Edward E. DeLuca, Pavel Kotrč, Yu. A. Kupryakov, L. Golub, František Fárník
Publikováno v:
Astronomy & Astrophysics. 574:A62
Context. Total masses of six solar prominences were estimated using prominence multi-spectral observations (in EUV, X-rays, Hα, and Ca ii H). The observations were made during the observing campaign from April through June 2011. Aims. The aim of the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a573a28556b33134670667df16b79432
https://doi.org/10.1051/0004-6361/201423513
https://doi.org/10.1051/0004-6361/201423513
Autor:
O. B. Smirnova, Pavel Kotrč, A. V. Gorshkov, Yu. A. Kupryakov, Petr Heinzel, E. V. Kononovich
Publikováno v:
International Astronomical Union Colloquium. 144:361-363
We have determined principal plasma parameters in a filament by applying the appropriate cloud model to several observed spectral lines. Then we compared them to prominence models from the recent numerical NLTE modelling of Gouttebrozeet al. (1993) (
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::9df4543dee3d1cf98d423e393ed8d2e7
https://doi.org/10.1017/s0252921100025616
https://doi.org/10.1017/s0252921100025616
Publikováno v:
ResearcherID
Motions in the Solar Atmosphere ISBN: 9789048151516
Motions in the Solar Atmosphere ISBN: 9789048151516
Hα spectra and filtergrams of the eruptive prominence observed with a high temporal resolution on September 18, 1995 were analysed to reconstruct motions and structures. A numerical code for the interpretation of patterns in solar spectra inclined d
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1770135d530174f030e45201d36aa146
http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcAuth=ORCID&SrcApp=OrcidOrg&DestLinkType=FullRecord&DestApp=WOS_CPL&KeyUT=WOS:000079746900018&KeyUID=WOS:000079746900018
http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcAuth=ORCID&SrcApp=OrcidOrg&DestLinkType=FullRecord&DestApp=WOS_CPL&KeyUT=WOS:000079746900018&KeyUID=WOS:000079746900018
