Titlebook: Cosmic Rays in the Heliosphere; Volume Resulting fro L. A. Fisk,J. R. Jokipii,K.-P. Wenzel Book 1998 Springer Science+Business Media Dordre

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书目名称Cosmic Rays in the Heliosphere影响因子(影响力)




书目名称Cosmic Rays in the Heliosphere影响因子(影响力)学科排名




书目名称Cosmic Rays in the Heliosphere网络公开度




书目名称Cosmic Rays in the Heliosphere网络公开度学科排名




书目名称Cosmic Rays in the Heliosphere被引频次




书目名称Cosmic Rays in the Heliosphere被引频次学科排名




书目名称Cosmic Rays in the Heliosphere年度引用




书目名称Cosmic Rays in the Heliosphere年度引用学科排名




书目名称Cosmic Rays in the Heliosphere读者反馈




书目名称Cosmic Rays in the Heliosphere读者反馈学科排名

DOSE

索赔

Three-Dimensional Solar Modulation of Cosmic Rays and Anomalous Components in the Inner Heliospherehe first comprehensive exploration of modulation as a function of latitude from 80° S to 80° N heliographic latitude. Among the principal findings for the inner heliosphere are: a) the cosmic ray intensity depends only weakly on heliographic latitude; b) for the nuclear components, and especially fo

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Anomalous Cosmic Rays and Solar Modulationdinal and radial gradients of these particles exhibit a 22-year periodicity in concert with the reversal of the Sun’s magnetic field. The power-law index of the low energy portion of the energy spectrum of ACRs at the shock in 1996 appears to be ≤ −1.3, suggesting that the strength of the solar wind

坦白

Cosmic Ray Electronsgative slope, which may in some way be related to electrons released from the magnetosphere of the planet Jupiter. If there is such a relationship, its nature is not established, and alternative explanations for the upturn exist. At higher energies, electrons are predominantly negatively charged, an

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The Solar Wind — Inner Heliospheremission to the many low latitude inner heliosphere missions that preceded it. The two major omissions are the high latitude solar wind at solar maximum, which will he measured during the second Ulysses polar passages. and the solar wind near the Sun. which could he analyzed by a Solar Probe mission.

FRAUD

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Magnetic Fields in the Inner Heliosphereake place in the solar wind. The division between the inner and outer regions of the heliosphere is the result of dynamic processes which form large scale structures with increasing heliocentric distance. The structure of the HMF is normally described in the reference frame based on Parker’s geometr

积习难改

Voyager Observations of the Magnetic Field in the Distant Heliospherend negative magnetic polarities are observed, and by the unipolar regions above and below the sector zone. Distinct corotating streams and interactions regions are found primarily in the sector zone during the declining phase of the solar cycle. Within a few AU, the streams and interaction regions a