F-CHROMA
"Flare Chromospheres: Observations, Models and Archives"
| Coordinatore | UNIVERSITY OF GLASGOW
Organization address
address: University Avenue contact info |
| Nazionalità Coordinatore | United Kingdom [UK] |
| Totale costo | 2˙811˙687 € |
| EC contributo | 2˙204˙174 € |
| Programma | FP7-SPACE
Specific Programme "Cooperation": Space |
| Code Call | FP7-SPACE-2013-1 |
| Funding Scheme | CP-FP |
| Anno di inizio | 2013 |
| Periodo (anno-mese-giorno) | 2013-09-24 - 2017-01-01 |
Partecipanti
| # | ||||
|---|---|---|---|---|
| 1 |
UNIVERSITY OF GLASGOW
Organization address
address: University Avenue contact info |
UK (GLASGOW) | coordinator | 471˙072.00 |
| 2 |
UNIVERSITETET I OSLO
Organization address
address: Problemveien 5-7 contact info |
NO (OSLO) | participant | 397˙053.60 |
| 3 |
QUEEN'S UNIVERSITY BELFAST
Organization address
address: University Road contact info |
UK (BELFAST) | participant | 390˙768.40 |
| 4 |
UNIWERSYTET WROCLAWSKI
Organization address
address: Plac Uniwersytecki 1 contact info |
PL (WROCLAW) | participant | 261˙600.00 |
| 5 |
ISTITUTO NAZIONALE DI ASTROFISICA
Organization address
address: Viale del Parco Mellini 84 contact info |
IT (ROMA) | participant | 253˙380.00 |
| 6 |
UNIVERSITA DEGLI STUDI DI CATANIA
Organization address
address: PIAZZA UNIVERSITA 2 contact info |
IT (CATANIA) | participant | 231˙600.00 |
| 7 |
ASTRONOMICKY USTAV AVCR VVI
Organization address
address: Fricova 298 contact info |
CZ (ONDREJOV) | participant | 198˙700.50 |
Mappa
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Obiettivo del progetto (Objective)
'We propose a focused space-based and ground-based multi-mode, multi-wavelength study of solar flares - the most intense energy release events in the solar system. We will center our attention on the flare chromosphere, from which most of the radiation originates. This work calls on space-based and ground-based observations, plus theoretical and modeling expertise. The project will have two major outcomes: advances in our understanding of the physics of energy dissipation and radiation in the flaring solar atmosphere, and a catalogue and archive facility for the solar physics community to access combined ground-based and space-based datasets for well-observed flare events, and flare atmospheric models to aid in data interpretation. It will have scientific impacts for both solar and stellar flare communities. We plan a dissemination activity for public and scientific communities alike, including an effort to involve amateur astronomers in co-ordinated flare campaigns.'