NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
Charge state composition in coronal hole and CME related solar wind: Latitudinal variations observed by Ulysses and WINDIron charge states in recurrent coronal hole-associated solar wind flows are obtained in the ecliptic by WIND/SMS, while measurements of iron and silicon from the polar coronal holes are available from Ulysses/SWICS. Ulysses/SWICS also provides ion composition of coronal mass ejection (CME)-related solar wind. Both coronal hole-associated and CME-related solar wind charge charges show heliographic latitudinal variations.
Document ID
19990056503
Acquisition Source
Goddard Space Flight Center
Document Type
Conference Paper
Authors
Galvin, A. B.
(Maryland Univ. College Park, MD United States)
Gloeckler, G.
(Maryland Univ. College Park, MD United States)
Date Acquired
August 19, 2013
Publication Date
December 1, 1997
Publication Information
Publication: Proceedings of the 31st ESALB Symposium on Correlated Phenomena at the Sun, in the Heliosphere and in Geospace
Subject Category
Solar Physics
Funding Number(s)
CONTRACT_GRANT: JPL-955460
CONTRACT_GRANT: NAS5-30370
Distribution Limits
Public
Copyright
Other
Document Inquiry

Available Downloads

There are no available downloads for this record.
No Preview Available