Data Access
data designed to reveal the variations in solar K-corona via a subtraction of a "background" model (L2b data; see below) that primarily removes the dominant F-coronal signal. These data are usually in units of MSB, though this should be verified by inspection of the FITS headers. We do not provide L3 data for the high-cadence observations. Important: please see our disclaimer about the L3 data product.
Version:2.5.0
data designed to reveal the variations in solar K-corona via a subtraction of a "background" model (L2b data; see below) that primarily removes the dominant F-coronal signal. These data are usually in units of MSB, though this should be verified by inspection of the FITS headers. We do not provide L3 data for the high-cadence observations. Important: please see our disclaimer about the L3 data product.
Role | Person | StartDate | StopDate | Note | |
---|---|---|---|---|---|
1. | PrincipalInvestigator | spase://SMWG/Person/Mark.Linton | |||
2. | ProjectScientist | spase://SMWG/Person/Angelos.Vourlidas | |||
3. | Scientist | spase://SMWG/Person/Guillermo.Stenborg | |||
4. | DataProducer | spase://SMWG/Person/Nathan.B.Rich | |||
5. | InstrumentScientist | spase://SMWG/Person/Phil.Hess | |||
6. | HostContact | spase://SMWG/Person/Karl.Battams | |||
7. | FormerPI | spase://SMWG/Person/Russell.A.Howard | |||
8. | MetadataContact | spase://SMWG/Person/Seiji.Yashiro |
In FITS via http from NRL
Helioprojective Zenith Polynomial Coordinate