Zobrazeno 1 - 10
of 30
pro vyhledávání: '"M. D. Kartalev"'
Autor:
Martin Rubin, Gabor Toth, M. D. Kartalev, Kirk C. Hansen, Tamas I. Gombosi, Christoph Koenders, Wing-Huen Ip
Publikováno v:
Rubin, Martin; Gombosi, T. I.; Hansen, K. C.; Ip, W.-H.; Kartalev, M. D.; Koenders, C.; Tóth, G. (2015). Modeled Interaction of Comet 67P/Churyumov-Gerasimenko with the Solar Wind Inside 2 AU. Earth, moon, and planets, 116(3), pp. 141-157. Springer 10.1007/s11038-015-9476-8
Earth Moon and Planets
Earth Moon and Planets
Periodic comets move around the Sun on elliptical orbits. As such comet 67P/Churyumov Gerasimenko (hereafter 67P) spends a portion of time in the inner solar system where it is exposed to increased solar insolation. Therefore given the change in heli
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::40c09c5a727d6a751abcea7c7469dd36
http://doc.rero.ch/record/330941/files/11038_2015_Article_9476.pdf
http://doc.rero.ch/record/330941/files/11038_2015_Article_9476.pdf
Publikováno v:
Journal of Geophysical Research: Space Physics. 124:1866-1882
Publikováno v:
AIP Conference Proceedings.
Our investigation is based on the results of the numerical simulation, which describes the interaction of the solar wind with the Earth’s magnetosphere. The 3D numerical magnetosheath-magnetosphere model is adopted for the description of this inter
Publikováno v:
Advances in Space Research. 58:188-195
This paper describes an approach to a theoretical interpretation of Interball-1 satellite measurements data in two cases of the satellite’s crossings of the magnetosheath. An interpretation is made of both the measured crossings of the magnetosheat
Publikováno v:
MATEC Web of Conferences, Vol 145, p 03003 (2018)
We investigate the behaviour of the plasma parameters in the magnetosheath in a case when Interball-1 satellite stayed in the magnetosheath, crossing the tail magnetopause. In our analysis we apply the numerical magnetosheath-magnetosphere model as a
Publikováno v:
Journal of Theoretical and Applied Mechanics. 42:71-90
Solar Wind-Comet Exosphere Interaction. 2. Could the Single-Fluid Gas-Dynamic Model be Applicable to the Rosetta Mission The capabilities of a single fluid gasdynamic model of solar wind-comet exosphere interaction, presented in the accompanying (Ker
Publikováno v:
MATEC Web of Conferences, Vol 145, p 03004 (2018)
This paper presents a case study of the plasma parameters in the magnetosheath, based on THEMIS measurements. As a theoretical tool we apply the self-consistent magnetosheath-magnetosphere model. A specific aspect of the model is that the positions o
Publikováno v:
Cosmic Research. 46:469-483
A possibility of description of the properties of plasma flow in the magnetosheath using the INME hydrodynamical model is considered on the basis of a comparison with experimental data. This model is characterized by a high degree of self-consistency
Publikováno v:
Journal of Atmospheric and Solar-Terrestrial Physics. 70:627-636
We report on some comparisons of plasma measurements during satellite magnetosheath crossing with model predicted variations along the same trajectory. We utilize a new self-consistent model of the magnetosheath–magnetosphere system. The model incl
A possible explanation for the dominant effect of South American thunderstorms on the Carnegie curve
Publikováno v:
Journal of Atmospheric and Solar-Terrestrial Physics. 68:457-468
The Carnegie curve shows the variation of the vertical electric field near the Earth's surface with Universal Time. The largest of the three maxima in this variation occurs at the time of maximum thunderstorm activity over the Americas, although this