The Extreme Ultraviolet (EUV) monitor is part of the Langmuir Probe and Waves (LPW) instrument and measures solar
EUV input and variability, and wave heating of the Martian upper atmosphere.
Goals:
* Measure solar emissions from different regions of the Sun in three distinct EUV bands
* Three channels provide a complete EUV spectrum (0.1-190 nm) to serve as a proxy for
input to the Flare Irradiance Spectral Model (FISM) model
Version:2.4.1
The Extreme Ultraviolet (EUV) monitor is part of the Langmuir Probe and Waves (LPW) instrument and measures solar
EUV input and variability, and wave heating of the Martian upper atmosphere.
Goals:
* Measure solar emissions from different regions of the Sun in three distinct EUV bands
* Three channels provide a complete EUV spectrum (0.1-190 nm) to serve as a proxy for
input to the Flare Irradiance Spectral Model (FISM) model
| Role | Person | StartDate | StopDate | Note | |
|---|---|---|---|---|---|
| 1. | PrincipalInvestigator | spase://CNES/Person/CDPP-AMDA/Frank.Eparvier |