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Dawn Dusk Asymmetries in Planetary Plasma Environments (Hardcover)
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Dawn Dusk Asymmetries in Planetary Plasma Environments (Hardcover)
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Dawn-Dusk Asymmetries in Planetary Plasma Environments Dawn-dusk
asymmetries are ubiquitous features of the plasma environment of
many of the planets in our solar system. They occur when a
particular process or feature is more pronounced at one side of a
planet than the other. For example, recent observations indicate
that Earth's magnetopause is thicker at dawn than at dusk.
Likewise, auroral breakups at Earth are more likely to occur in the
pre-midnight than post-midnight sectors. Increasing availability of
remotely sensed and in situ measurements of planetary ionospheres,
magnetospheres and their interfaces to the solar wind have revealed
significant and persistent dawn-dusk asymmetries. As yet there is
no consensus regarding the source of many of these asymmetries, nor
the physical mechanisms by which they are produced and maintained.
Volume highlights include: * A comprehensive and updated overview
of current knowledge about dawn-dusk asymmetries in the plasma
environments of planets in our solar system and the mechanisms
behind them * Valuable contributions from internationally
recognized experts, covering both observations, simulations and
theories discussing all important aspects of dawn-dusk asymmetries
* Space weather effects are caused by processes in space, mainly
the magnetotail, and can be highly localized on ground. Knowing
where the source, i.e., where dawn-dusk location is will allow for
a better prediction of where the effects on ground will be most
pronounced Covering both observational and theoretical aspects of
dawn dusk asymmetries, Dawn--Dusk Asymmetries in Planetary Plasma
Environments will be a valuable resource for academic researchers
in space physics, planetary science, astrophysics, physics,
geophysics and earth science.
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