... international missions as Interball project (Tail Probe (1995), Auroral Probe (1996 ... studying the planet of Venus and the Halley comet and the other world-wide known ...
... 1949--Britain puts the first jet airliner into service, the Comet. ... ahead of the magnetosphere, and a long magnetic tail on the night side of the Earth ... 3) explores the distant magnetotail, before heading for comet Giacobini-Zinner ...
... 1949 --Britain puts the first jet airliner into service, the Comet. ... ahead of the magnetosphere, and a long magnetic tail on the night side of the Earth ... distant magnetotail, observes that the distant tail plasma flows (past about 70 RE ...
... it encountered a burst of energetic particles, which could be the result of a substorm-type event in Marcury's magnetic tail ... magnetic cavities are also formed around Venus, the Moon and comets (and probably, Mars), but if the obstacle is not a ...
... Consider the geotail: The density and temperature in the plasma sheet vary continuously, but can we tell how at any time they vary with distance down the tail or across the tail? ...
... it encountered a burst of energetic particles, which could be the result of a substorm-type event in Marcury's magnetic tail ... magnetic cavities are also formed around Venus, the Moon and comets (and probably, Mars), but if the obstacle is not a ...
... about the Sun, planets, moons, asteroids, comets and meteoroids found within the ... Includes access to summary images . LANL GEM Substorm/Tail Campaign Data . ... Data, plots and interpretation for the GEM Tail-Substorm campaigns. ...
... A.Fedorov, J.-A.Sauvaud, J.T.Steinberg and G.Rostoker, Coordinated WIND, INTERBALL - Tail and ground observations of Kelvin-Helmholtz instability and waves in the near-tail equatorial magnetopause at dusk: January 11, 1997, submitted to J. Geophys ...
... plasma ions, as neutrals or grains from Io, or meteoroid and comet impacts ... It is seen that the suprathermal tails in the H2O and O2 EDFs are formed due to the ... Suprathermal tails at energies higher than escape energy (E > 0.38 eV) are formed ...
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Ссылки http://www.iki.rssi.ru/conf/2009elw/presentations/presentations_pdf/session3/Shematovich_ELW.pdf -- 1173.2 Кб -- 02.03.2009 Похожие документы