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The solar wind is an uninterrupted flow of highly ionised plasma that streams from compact sources at or near the Sun, accelerates across the low solar corona, and expands into the whole interplanetary space. The physical properties of any wind strea
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::09c82ce98c0eac02f0659b250030ef0a
https://doi.org/10.5194/egusphere-egu23-12000
https://doi.org/10.5194/egusphere-egu23-12000
