The EUI instrument suite is composed of three telescopes: one dual-band full-sun imager (FSI) working alternatively at the 17.4 nm and 30.4 nm EUV passbands (named “FSI174/304”), and two high resolution imagers (HRI), one at the hydrogen Lyman-α line at 121.6 nm, (named “HRILy-α”) and one in the extreme UV line at 17.4 nm (named “HRIEUV”).
Version:2.7.1
The EUI instrument suite is composed of three telescopes: one dual-band full-sun imager (FSI) working alternatively at the 17.4 nm and 30.4 nm EUV passbands (named “FSI174/304”), and two high resolution imagers (HRI), one at the hydrogen Lyman-α line at 121.6 nm, (named “HRILy-α”) and one in the extreme UV line at 17.4 nm (named “HRIEUV”).
| Role | Person | StartDate | StopDate | Note | |
|---|---|---|---|---|---|
| 1. | PrincipalInvestigator | spase://SMWG/Person/Frederic.Auchere |
Level 3 (L3) data corresponds to a further processing of L2 data for visualisation purposes. The L3 image files are intended for visualisation through JHelioviewer. L2 images without the keyword WAVELNTH (e.g., because a wrong filter position was selected) are excluded from processing. The L3 file version number is identical to the L2 file version number.
Level 3 (L3) data corresponds to a further processing of L2 data for visualisation purposes. The L3 image files are intended for visualisation through JHelioviewer. L2 images without the keyword WAVELNTH (e.g., because a wrong filter position was selected) are excluded from processing. The L3 file version number is identical to the L2 file version number.
Data from one dual-band full-sun imager (FSI) working alternatively at the 174 Å and 304 Å EUV.