Second
EGSO Use Case
Emergence of an Active Region
Author: J. Aboudarham
Objective:
Follow an active region from the time it appears in the photosphere to
its appearance in transition region and corona in order to study its
evolution.
Data Sets:
1) Full Sun images (for instance Ha [6563 Å] and Ca II K line
[approx. 3980 Å] for chromosphere, EIT 172 Å for low
corona, Nançay radiolehiograph data for corona) and magnetograms
(MDI) in order to determine interesting new active regions.
2) High resolution visible data and magnetograms (spectral scans) are
needed to determine the emergence of the active region, such as THEMIS
polarimetric observations of the region in photospheric G-band of
Hydrogen (4307 Å) (or any photospheric line sensitive to magnetic
field) and Ha data (or any chromospheric line sensitive to magnetic
field). Dopplergrams are also of interest.
3) Coronographic and radio observations to follow the evolution of the
active region in higher atmosphere.
Data Selection:
• Look for new active regions on full sun magnetograms and images (ie.
find active regions then go back to the time just before the active
region is first observed – hereafter Time0).
• Look for high resolution polarimetric observations of the region in
photosphere and chromosphere at Time0 and for two days.
• Search for the time (Time1) when active region appears in transition
region and low corona (from
Time0, during no more than a few days).
• Search for UV and radio data at Time1.
Data Processing during the Selection Phase:
No processing is needed for the data during selection phase.
Data Processing for Selected Data:
• High resolution data must be calibrated (or codes for calibration
easily available)
• Data processing of polarimetric observations in order to obtain
magnetic field is not needed in my opinion: it is part of the
scientific work. But all informations concerning it must be available
(such as instrument drift, instrument internal polarization if any, ...)