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Responses of the Magnetosphere to Interplanetary Disturbances

  • Chapter
Physics of Magnetospheric Substorms

Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 47))

Abstract

Large-scale interplanetary disturbances, their origins and their effects on the magnetosphere, have been discussed in a number of reviews (cf. S.T.P., Chapter 7). In studying magnetospheric substorms, it is important, first of all, to identify characteristics of the response of the magnetosphere to various interplanetary disturbances, and to distinguish them from substorm-associated changes. This is because these interplanetary disturbances are almost always present even during a fairly quiet period. Thus, when magnetospheric quantities are monitored by satellite-borne instruments or by ground-based instruments, the response of the magnetosphere to these disturbances is recorded as ‘noise’ in addition to the substorm ‘signal’. For example, a weak shock wave compresses the magnetosphere, and its effect is observed as an increase of the magnetic field of order of 10 y throughout the magnetosphere. This amount is relatively small on the ground where the field intensity is large (~50000 γ). However, it is relatively a very large change in the magnetotail, since the magnetotail field intensity in the high latitude lobe is only of order 10–30 γ. Thus, one must identify the compression effects in the records, by monitoring the solar wind pressure, and distinguish them from substorm-associated changes. In the following, we discuss three elementary interplanetary disturbances and their magnetospheric responses.

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Akasofu, SI. (1977). Responses of the Magnetosphere to Interplanetary Disturbances. In: Physics of Magnetospheric Substorms. Astrophysics and Space Science Library, vol 47. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-1164-8_5

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