Effect of large-scale inhomogeneity of solar wind velocity on distribution of directions of interplanetary magnetic field vector
Using data with hourly resolution obtained in near-Earth heliosphere in 1965–2014, we have calculated statistical characteristics of the angles describing the direction of the interplanetary magnetic field (IMF): root-mean-square deviations of azimuthal and elevation angles, asymmetries of their dis...
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| Format: | Article |
| Language: | English |
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INFRA-M
2019-09-01
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| Series: | Solar-Terrestrial Physics |
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| Online Access: | https://naukaru.ru/en/nauka/article/30595/view |