Zobrazeno 1 - 10
of 12
pro vyhledávání: '"N. S. Shilova"'
Autor:
N. S. Shilova
Publikováno v:
Geomagnetism and Aeronomy. 48:709-712
The duration of elementary eruption process and intervals between them for flares of different importance have been determined based on the photometric data for flares, observed by a TRACE spacecraft at a wavelength of 195 A. It has been revealed tha
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::060b7088d802beeb708be6105042d706
https://doi.org/10.1134/s0016793208060029
https://doi.org/10.1134/s0016793208060029
Autor:
N. S. Shilova
Publikováno v:
Solar System Research. 40:437-440
The cells of photospheric background magnetic fields during Carrington rotation 2009 in October–November 2003 are considered. The small number of large sunspots and the high activity on the Sun in this period allow the correspondence between the ac
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::07653a681cb8604524a8fde5452fcd9d
https://doi.org/10.1134/s0038094606050091
https://doi.org/10.1134/s0038094606050091
Autor:
E. I. Mogilevsky, N. S. Shilova
Publikováno v:
Geomagnetism and Aeronomy. 46:303-308
Solar flare films obtained on the TRACE spacecraft with a resolution of 1″ in the 160-nm (CIV) band with a frame separation of 2 s are examined. It has been indicated that the flare scenario is determined by the dynamics of numerous structures of a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::8582bc9b0388a0dec4b5009b5568c8e5
https://doi.org/10.1134/s0016793206030030
https://doi.org/10.1134/s0016793206030030
Publikováno v:
Astronomical & Astrophysical Transactions. 24:25-33
The problem of energy transport by magnetohydrodynamic (MHD) solitons to the local region of a solar flare is considered within the framework of a new concept on the nature of solar flares as an effect of the unloading of matter and energy under self
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::3abfe72a084227b2534b9f8215013fd7
https://doi.org/10.1080/10556790500093219
https://doi.org/10.1080/10556790500093219
Autor:
M. M. Molodenskii, N. S. Shilova
Publikováno v:
Astronomy Reports. 46:591-596
Halo-type motions of plasma in the solar corona—so-called coronal mass ejections (CME)—are considered. This type of CME is relatively rare due to the requirement for a particular orientation of the magnetic-moment vector M (parallel to the line o
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::43010a4310184810abbb2cd893eeb06f
https://doi.org/10.1134/1.1495035
https://doi.org/10.1134/1.1495035
Publikováno v:
The Astrophysical Journal. 567:1225-1233
Based on Yohkoh/SXT, SOHO/EIT images and movies, as well as on Hα, He I 10830 A heliograms and other relevant data, we analyze an event of 1999 December 28, which is interesting in at least two aspects. (1) A major horseshoe-shaped Hα filament appe
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::453bee49644a027826afaa9893347c0b
https://doi.org/10.1086/338584
https://doi.org/10.1086/338584
Autor:
N. S. Shilova
Publikováno v:
Astronomy and Astrophysics Supplement Series. 144:371-377
The white-light lms of coronal mass ejections for April - May, 1998 (SOHO LASCO C2, C3), retrieved from Internet, are considered. The positions of active re- gions on visible and back sides of the Sun for each day are studied. It is shown that a regi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::47dfc356641e8ff9846de282bf94fbae
https://doi.org/10.1051/aas:2000215
https://doi.org/10.1051/aas:2000215
Publikováno v:
Solar Physics. 176:107-121
This paper is aimed at establishing the relationship between the large-scale magnetic fields (LSMF), coronal holes (CH), and active regions (AR) in the Sun. The LSMF structure was analyzed by calculating the vector photospheric magnetic field under a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::5a2e912647ed3fc17223d2185c45bd1d
https://doi.org/10.1023/a:1004908014970
https://doi.org/10.1023/a:1004908014970
Autor:
N. S. Shilova
Publikováno v:
Astronomical & Astrophysical Transactions. 21:327-329
It is very likely that, due to the substantial role of scattering in the formation of lines, the observation of dimming in SOHO EIT 171 and 195A filtergrams demonstrates the high-speed, dense clouds of solar coronal mass ejection matter.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::8607722e7ca3667872134dccfb3e2b09
https://doi.org/10.1080/10556790215600
https://doi.org/10.1080/10556790215600
Publikováno v:
Pharmaceutical Chemistry Journal. 42
Optimum conditions for the analytical determination of isonicotinic acid hydrazide in urine using ammonium metavanadate are established. Anoninvasive method for the indirect determination of N-acetyltransferase activity in human hepatocytes that is b
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::2f0160045bdd2deec2bf4cdcab309e4b
https://doi.org/10.1007/s11094-008-0157-z
https://doi.org/10.1007/s11094-008-0157-z