与 «IONOPAUSE»相关的英语书籍
在以下的参考文献中发现
ionopause的用法。与
ionopause相关的书籍以及同一来源的简短摘要提供其在 英语文献中的使用情境。
Since the ionopause as defined by all these parameters has a finite thickness,
the assignment of a specific ionopause altitude differs somewhat with the
particular parameter employed and various instrumental sensitivity factors. H.
Taylor et al.
2
Elements Of Space Physics
Magnetosheath The region lying between the bow shock and the ionopause
contains the shocked solar plasma and lesser amounts of planetary plasma. This
region is termed as the ionosheath or more commonly magnetosheath.
3
Venus II--geology, Geophysics, Atmosphere, and Solar Wind ...
D. The Ionopause The sharp drop in ion or electron density that occurs at the
boundary between the thermal ionospheric plasma and the superthermal solar
wind plasma on Venus is called the ionopause. Because Venus does not
possess an ...
Stephen Wesley Bougher, Donald M. Hunten, Roger J. Phillips, 1997
The related solar zenith angle dependence of the ionopause altitude determined
from both the topside ionosphere density gradients and the altitudes where
ionospheric thermal and magnetic barrier magnetic pressures balance is shown
in ...
Andrew F. Nagy, Andre Balogh, Thomas E. Cravens, 2008
INSTABILITY OF A COMET IONOPAUSE: CONSEQUENCES OF COLLISIONS
AND COMPRESSIBILITY Alexander I. Ershkovich, Dina Prialnik and Aharon
Eviatar Raymond and Beverly Sackler Faculty of Exact Sciences, Department of ...
6
Origin and Evolution of Planetary Atmospheres: Implications ...
When the solar or stellar wind plasma flows around an ionosphere the interface
between the solar wind and the ionosphere, the ionopause can be a subject to
these plasma instabilities. Disturbances of the interface between the flow of two ...
7
Planetary Aeronomy: Atmosphere Environments in Planetary Systems
An example of the configuration of the ionopause of Venus resulting from the
solar wind interaction with the topside ionosphere of Venus. Pressure balance
between solar wind and ionospheric plasma is based on the Mariner 5
observations ...
Siegfried Bauer, Helmut Lammer, 2004
actually more reminiscent of Titan where /?ionopause~l-4 to 1.8 Rj (Hartle et al.
1982; McNutt and Richardson 1988) than Venus (where /?ionopause~ 1 -03 Rv
according to Luhmann [1986]) and Mars (where /?ionopause~ 1 -15 Rm ...
Alan Stern, David James Tholen, 1997
9
The Mars Plasma Environment
As a result, the real obstacle to the solar wind is observed at the magnetic barrier
whose position is further from the planet than the ionopause (see, for example,
Zhang et al., 1991). If the ionosphere is resistive the ionopause is broadened and
...
By courtesy of the publishers] left to right in the Figure), the altitude of the
ionopause decreases considerably (from 420 to 250 kilometres in this example),
and its thickness simultaneously goes from a few kilometres to more than fifty.
Current ...
