Zobrazeno 1 - 10
of 71
pro vyhledávání: '"V. I. Shematovich"'
Autor:
S. Krauss, B. Fichtinger, H. Lammer, W. Hausleitner, Yu. N. Kulikov, I. Ribas, V. I. Shematovich, D. Bisikalo, H. I. M. Lichtenegger, T. V. Zaqarashvili, M. L. Khodachenko, A. Hanslmeier
Publikováno v:
Annales Geophysicae, Vol 30, Pp 1129-1141 (2012)
We analyzed the measured thermospheric response of an extreme solar X17.2 flare that irradiated the Earth's upper atmosphere during the so-called Halloween events in late October/early November 2003. We suggest that such events can serve as proxie
Externí odkaz:
https://doaj.org/article/e32b8687af6f47299355b657ebc97c7f
Publikováno v:
Annales Geophysicae, Vol 23, Pp 1473-1480 (2005)
Hydrogen line profiles measured from space-borne or ground-based instruments provide useful information to study the physical processes occurring in the proton aurora and to estimate the proton flux characteristics. The line shape of the hydrogen
Externí odkaz:
https://doaj.org/article/91544831c1664f92a09bb95437c33523
Publikováno v:
Annales Geophysicae, Vol 21, Pp 2165-2173 (2003)
The combination of simultaneous global images of the north polar region obtained with the IMAGE-FUV imaging system makes it possible to globally map the properties of the electron and proton auroral precipitation. The SI12 imager, which observe
Externí odkaz:
https://doaj.org/article/b4dda38a9b034e9bbe3ce80ef195b6dc
Autor:
A. A. Avtaeva, V. I. Shematovich
Publikováno v:
Astronomy Reports. 66:1254-1261
Publikováno v:
Astronomy Reports. 66:1318-1324
Autor:
A. A. Avtaeva, V. I. Shematovich
Publikováno v:
Solar System Research. 56:67-75
Publikováno v:
Astronomy Reports. 66:245-254
Autor:
I. S. Savanov, V. I. Shematovich
Publikováno v:
Astrophysical Bulletin. 76:450-471
Autor:
D. V. Bisikalo, V. I. Shematovich
Publikováno v:
Astronomy Reports. 65:869-875
We present the kinetic Monte-Carlo model, which was developed to describe the influence of a proton flux from the undisturbed solar wind on the daytime atmosphere of Mars. For the first time, the degradation of the solar-wind proton spectrum in the c
Publikováno v:
Physics-Uspekhi. 64:747-800