For each Carrington rotation, there are two coronal
synoptic maps of the sun in each of 3 Fe lines (171A, 195A, 284A) and
in He (304A) These maps are from the Extreme Ultraviolet Imaging Telescope
(EIT) on the SOHO spacecraft. The two maps for a given day and wavelength
differ in that one has latitude on the Y axis and the other has sin(lat).
There is also a FITS file for each day and wavelength. As of 01/11/2012,
the maps spanned Carrington rotations 1911 (start day June 28, 1996)
through 2055 (end date April 26, 2006)
Version:2.7.1
Version:2.7.1
For each Carrington rotation, there are two coronal
synoptic maps of the sun in each of 3 Fe lines (171A, 195A, 284A) and
in He (304A) These maps are from the Extreme Ultraviolet Imaging Telescope
(EIT) on the SOHO spacecraft. The two maps for a given day and wavelength
differ in that one has latitude on the Y axis and the other has sin(lat).
There is also a FITS file for each day and wavelength. As of 01/11/2012,
the maps spanned Carrington rotations 1911 (start day June 28, 1996)
through 2055 (end date April 26, 2006)
| Role | Person | StartDate | StopDate | Note | |
|---|---|---|---|---|---|
| 1. | PrincipalInvestigator | spase://SMWG/Person/Jean-Pierre.Delaboudiniere | |||
| 2. | GeneralContact | spase://SMWG/Person/Elena.Benevolenskaya |
For general info about synoptic maps, plus links to
several sets of such maps