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In-Situ Solar Wind and Magnetic Field Signatures of Interplanetary Coronal Mass Ejections
Space Science Reviews, 2006Thomas Zurbuchen, Ian Richardson
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Hannibal the Coronal (mass ejection)
Tre intensi brillamenti solari in tre giorni, dalla regione attiva Ar 4274, ai quali hanno fatto seguito altrettante espulsioni coronali di massa dirette verso il nostro pianeta. Nelle prossime ore potrebbero in parte sovrapporsi, dando luogo a una forte tempesta geomagnetica.openaire +1 more source
Philosophical Transactions Series A, Mathematical, Physical, and Engineering Sciences, 2019
Neel P Savani, Angelos Vourlidas
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Neel P Savani, Angelos Vourlidas
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Mass loss via solar wind and coronal mass ejections during solar cycles 23 and 24
Monthly Notices of the Royal Astronomical Society, 2019Nandita Srivastava +2 more
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A catalog of white light coronal mass ejections observed by the SOHO spacecraft
Journal of Geophysical Research: Space Physics, 2004Nat Gopalswamy +2 more
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The association of coronal mass ejection transients with other forms of solar activity
Solar Physics, 1979John T. Gosling, A I Poland, R H Munro
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Higher-speed coronal mass ejections and their geoeffectiveness
Journal of Astrophysics and Astronomy, 2018Asheesh Bhargawa, Abhay Kumar Singh
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Activity associated with coronal mass ejections at solar minimum: SMM observations from 1984–1986
Solar Physics, 1991Orville St Cyr, D F Webb, O C Cyr
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