Dayside auroral activity and magnetic flux transfer from the solar wind Article Published Version DAYSIDE AURORAL ACTIVITY AND MAGNETIC FLUX TRANSFER FROM THE SOLAR WIND
Abstract. Combined observations by meridianscanning photometers and the EISCAT radar show that the "midday-auroral breakup" phenomenon is associated with major increases in ionospheric flow. A
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Format: | Text |
Language: | English |
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Online Access: | http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.1036.2020 |
Summary: | Abstract. Combined observations by meridianscanning photometers and the EISCAT radar show that the "midday-auroral breakup" phenomenon is associated with major increases in ionospheric flow. A |
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