Relation between the area of polar coronal holes and the solar wind speed at a minimum between solar cycles 22 and 23
We have used data from the space telescope SOHO/EIT and the spectrometer VEIS on the Wind spacecraft to compare the solar wind (SW) speed near Earth's orbit with changes in the area of polar coronal holes (CHs) on the Sun during the 1996 solar activity minimum. We have found that in March 1996...
Main Authors: | , |
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Format: | Article |
Language: | English |
Published: |
INFRA-M
2023-09-01
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Series: | Solar-Terrestrial Physics |
Subjects: | |
Online Access: | https://naukaru.ru/en/nauka/article/64149/view |