Zobrazeno 1 - 10
of 73
pro vyhledávání: '"Arvydas J. Kliore"'
Autor:
John Klose, Danny Kahan, Andrew F. Nagy, Sami W. Asmar, D. Fleischman, Aseel Anabtawi, Arvydas J. Kliore, E. Barbinis
Publikováno v:
Geophysical Research Letters. 41:5778-5782
Fifty-nine ionsopheric radio occultation observations of the vertical electron density profile in the Saturn ionosphere have been made since the Cassini spacecraft was inserted in orbit around Saturn in 2004. Significant orbit to orbit variations wer
Autor:
Nicole J. Rappaport, E. Barbinis, Richard G. French, Essam A. Marouf, F. Michael Flasar, A. Anabtawi, Colleen A. McGhee, Paul J. Schinder, D. U. Fleischman, Arvydas J. Kliore
Publikováno v:
Icarus. 221:1020-1031
We present the results of six soundings of the atmosphere of Titan by the radio occultation technique using the Cassini spacecraft currently in orbit around Saturn. These occultations occurred during four separate targeted Titan encounters in both th
Autor:
E. Barbinis, Essam A. Marouf, Nicole J. Rappaport, A. Anabtawi, Richard G. French, F. Michael Flasar, Paul J. Schinder, Colleen A. McGhee, Arvydas J. Kliore, D. U. Fleischman
Publikováno v:
Icarus. 215:460-474
We present results from the two radio occultations of the Cassini spacecraft by Titan in 2006, which probed mid-southern latitudes. Three of the ingress and egress soundings occurred within a narrow latitude range, 31.34 deg S near the surface, and t
Autor:
Arvydas J. Kliore, Andrew F. Nagy, Julianne I. Moses, Thomas E. Cravens, T. K. Breus, Michael Mendillo, Olivier Witasse
Publikováno v:
Atmospheres in the Solar System: Comparative Aeronomy
This article reviews our understanding of the ionospheres in the solar system. It provides some basic information on the sources and sinks of the ionospheric plasma, its dynamics, the energetics and the coupling to the neutral atmosphere. Ionospheres
Autor:
D. E. Shemansky, T. G. Gombosi, P. C. Liewer, M. E. Burton, Michel Blanc, Edward C. Sittler, Michel C. Festou, J. H. Waite, Donald G. Mitchell, Fritz M. Neubauer, Ph. Zarka, Robert E. Johnson, Larry W. Esposito, Bruce T. Tsurutani, Eberhard Grün, D. T. Young, J. G. Bradley, David J. Southwood, Stamatios M. Krimigis, William S. Kurth, D. A. Gurnett, M. K. Dougherty, Arvydas J. Kliore, Thomas E. Cravens, J. Feynman, Sylvestre Maurice, Scott Bolton, John D. Richardson, Barry Mauk, Iannis Dandouras
Publikováno v:
Space Science Reviews. 104:253-346
Magnetospheric and plasma science studies at Saturn offer a unique opportunity to explore in-depth two types of magnetospheres. These are an ‘induced’ magnetosphere generated by the interaction of Titan with the surrounding plasma flow and Saturn
Autor:
Arvydas J. Kliore, Indu R. Patel, Gunnar F. Lindal, Donald N. Sweetnam, Henry B. Hotz, J Hunter Waite, Thomas R. McDonough
Publikováno v:
1980, Pioneer Saturn ISBN: 9781118782101
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ae6cb81ff6dd999b3a0acc62c6ba80f6
https://doi.org/10.1002/9781118782101.ch20
https://doi.org/10.1002/9781118782101.ch20
Autor:
Michael R. Combi, Kenneth G. Powell, Konstantin Kabin, Kenneth C. Hansen, Yifan Liu, Arvydas J. Kliore, Andrew F. Nagy, Darren L. DeZeeuw, Tamas I. Gombosi
Publikováno v:
Journal of Geophysical Research: Space Physics. 106:6151-6160
A three-dimensional (3-D) multi-species magnetohydrodynamic model was used to study the interaction of Titan's ionosphere and Saturn's magnetosphere. The three generic species which were considered are light (e.g., H + , H 2 + , and H 3 + ), medium (
Publikováno v:
Planetary and Space Science. 46:367-376
In this paper a possibility to find out some effect of dipole-like intrinsic magnetic field on the plasma scale height at altitudes 180–240 km in the Martian ionosphere, that is above the topside boundary of the chemically controlled region predict
Autor:
K.Y. Pimenov, Tor Hagfors, W. I. Axford, Janet G. Luhmann, A. Krymsky, T.K. Braus, Arvydas J. Kliore
Publikováno v:
Advances in Space Research. 22:463-470
Topside electron density profiles provide information on the solar wind interactions with the terrestrial planets, Venus and Mars. At Mars we have a picture of the topside only from two Viking Lander profiles and from radio occultation measurements.