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Annual synoptic source surface maps in the Carrington Rotation Number versus Heliographic Latitude. The source surface was assumed to be at 2.5 solar radii. The IPS-CAT method was applied to derive these maps.
Version:2.5.0
Annual synoptic source surface maps in the Carrington Rotation Number versus Heliographic Latitude. The source surface was assumed to be at 2.5 solar radii. The IPS-CAT method was applied to derive these maps.
Role | Person | StartDate | StopDate | Note | |
---|---|---|---|---|---|
1. | PrincipalInvestigator | spase://IUGONET/Person/Munetoshi.Tokumaru | |||
2. | MetadataContact | spase://IUGONET/Person/Tomoaki.Hori | |||
3. | MetadataContact | spase://IUGONET/Person/ISEE.Metadata.Management.Group |
Solar wind velocity distribution on the plane of heliographic latitude v.s. Carrington rotation number remotely measured by Interplanetary Scintillation method