The OBSPM (OBservatoire Solaire de Paris a
Meudon) heliograph provides 3 images every 1.5 minute of the
solar disk in the H alpha line at 3 wavelengths: line core and
at 0.5 Angstroms from it on each side. A Lyot filter with a
0.5 Angstrom bandpass is used. The objective is to detect and
observe solar eruptions at a high temporal cadence.
Version:2.2.2
The OBSPM (OBservatoire Solaire de Paris a
Meudon) heliograph provides 3 images every 1.5 minute of the
solar disk in the H alpha line at 3 wavelengths: line core and
at 0.5 Angstroms from it on each side. A Lyot filter with a
0.5 Angstrom bandpass is used. The objective is to detect and
observe solar eruptions at a high temporal cadence.
| Role | Person | |
|---|---|---|
| 1. | GeneralContact | spase://SMWG/Person/Jean-Marie.Malherbe |