Zobrazeno 1 - 8
of 8
pro vyhledávání: '"G. S. Ivanov-Kholodnyi"'
Publikováno v:
Geomagnetism and Aeronomy. 56:585-591
The influence of the earthquake probability diurnal variation on specific features in the weekend effect in global seismic activity is revealed. The dependence of the global earthquake number on the local time and its possible relation to a quiet sol
Autor:
S. A. Boldyrev, A. P. Ignat'ev, V. G. Mordovskaya, O. P. Kolomiitsev, S. I. Boldyrev, G. S. Ivanov-Kholodnyi
Publikováno v:
Geomagnetism and Aeronomy. 50:679-685
A method for determining the basic atmosphere O/N2 based on the solar observations is described. It is shown that, on XUV images of the Sun received by transillumination of the atmosphere, it is possible to observe its state controlling the O/N2 rati
Publikováno v:
Solar System Research. 41:420-424
We report the results of our analysis of the variations in the orbit of the CORONAS-F satellite (August 31, 2001–December 6, 2005) during the low-orbit flight stage. We show that extreme solar events and the accompanying phenomena in the near-Earth
Autor:
S. I. Boldyrev, V. A. Surotkin, I. A. Zhitnik, O. P. Kolomiitsev, G. S. Ivanov-Kholodnyi, Sergey Kuzin, V. D. Kuznetsov
Publikováno v:
Solar System Research. 40:326-330
The measurement data obtained onboard the CORONAS-F spacecraft are compared to the parameters of the Earth’s upper atmosphere calculated by models. Examination of model results and their comparison to the experimental data show that current models
Autor:
A. I. Osin, G. S. Ivanov-Kholodnyi, O. P. Kolomiitsev, S. I. Boldyrev, A. N. Afanas'ev, V. D. Kuznetsov
Publikováno v:
Solar System Research. 39:501-507
The results of analysis of the trajectory parameters of the orbit of the CORONAS-F spacecraft since its launch (July 2001) and to the present time are reported. Two independent methods are used to compute a prediction for the active lifetime of the s
Autor:
Irina Myagkova, A. K. Svirzhevskaya, A. V. Bogomolov, Igor Veselovsky, Sergey Kuzin, A. A. Nusinov, V. N. Ishkov, V. D. Kuznetsov, Karel Kudela, Vladimir Slemzin, Victor V. Grechnev, Y.I. Denisov, A. K. Markeev, S. I. Avdyushin, V. L. Shishov, R. V. Gorgutsa, Z. Smith, Alexei Dmitriev, A. V. Mitrofanov, A. A. Pertsov, G. S. Ivanov-Kholodnyi, M. A. Zeldovich, E. A. Eroshenko, Volker Bothmer, G. A. Zherebtsov, Georgy Zastenker, G. Lawrence, O. S. Yakovchouk, Yu. I. Stozhkov, P. M. Svidsky, A. P. Ignat'ev, I. I. Sobel'man, Alla Suvorova, A. N. Podorolsky, V. I. Vlasov, B. M. Kuzhevsky, O. P. Kolomiytsev, I. A. Zhitnik, Eduard Vashenyuk, V. G. Kurt, N. K. Sukhodrev, S. I. Svertilov, I. G. Mitrofanov, N. S. Svirzhevsky, O. V. Morozov, V. V. Fomichev, M. L. Litvak, I. M. Chertok, B.Y. Yushkov, M. I. Panasyuk, Victor Yanke, I. P. Tindo, S. N. Oparin, Olga Panasenco, Andrei Zhukov, S. N. Kuznetsov, M. Dryer, E. P. Romashets, Igor A. Krasheninnikov, A. A. Gnezdilov, S. K. Tokhchukova, I. V. Chashey, V. S. Makhmutov, Anatoli Petrukovich, Leonid Lazutin, G. A. Bazilevskaya, Yu. I. Logachev, A. V. Belov, L. N. Leshchenko, Lev Zelenyi, D. E. Sobolev, Yu. I. Yermolaev, K. A. Boyarchuk, Sergey A. Bogachev, V. M. Bogod
Publikováno v:
Cosmic Research. 42:435-488
We present new observational data on the phenomena of extremely high activity on the Sun and in the heliosphere that took place in October-November 2003. A large variety of solar and heliospheric parameters give evidence that the interval under consi
Autor:
A. Zhitnik, A. P. Ignat'ev, Sergey Kuzin, O. Bugaenko, S. N. Oparin, A. I. Stepanov, V. V. Krutov, A. A. Pertsov, K. A. Boyarchuk, A. V. Mitrofanov, Vladimir Slemzin, G. S. Ivanov-Kholodnyi
Publikováno v:
Solar System Research. 37:296-301
We consider the effects of the absorption of solar XUV radiation by the Earth's atmosphere that were observed in the solar images obtained with the TEREK-K telescope onboard the Coronas-I satellite in May–June 1994 at low solar activity and with th
Publikováno v:
Bulletin of the Russian Academy of Sciences: Physics. 71:593-595
Results of studying the character and possible succession of cause-effect relations (in going from a disturbance source on the Sun to a response in the lithosphere in the range of periods from several days to the 11-year solar cycle) have been presen