Coordinatore | KIEPENHEUER-INSTITUT FUER SONNENPHYSIK
Organization address
address: SCHONECKSTRASSE 6 contact info |
Nazionalità Coordinatore | Germany [DE] |
Totale costo | 3˙218˙568 € |
EC contributo | 1˙994˙615 € |
Programma | FP7-SPACE
Specific Programme "Cooperation": Space |
Code Call | FP7-SPACE-2012-1 |
Funding Scheme | CP-FP |
Anno di inizio | 2013 |
Periodo (anno-mese-giorno) | 2013-01-01 - 2016-12-31 |
# | ||||
---|---|---|---|---|
1 |
KIEPENHEUER-INSTITUT FUER SONNENPHYSIK
Organization address
address: SCHONECKSTRASSE 6 contact info |
DE (Freiburg im Breisgau) | coordinator | 232˙040.00 |
2 |
OBSERVATOIRE DE PARIS
Organization address
address: AVENUE DE L OBSERVATOIRE 61 contact info |
FR (PARIS) | participant | 346˙500.00 |
3 |
MAX PLANCK GESELLSCHAFT ZUR FOERDERUNG DER WISSENSCHAFTEN E.V.
Organization address
address: Hofgartenstrasse 8 contact info |
DE (MUENCHEN) | participant | 294˙870.00 |
4 |
KATHOLIEKE UNIVERSITEIT LEUVEN
Organization address
address: Oude Markt 13 contact info |
BE (LEUVEN) | participant | 243˙700.00 |
5 |
THE UNIVERSITY OF BIRMINGHAM
Organization address
address: Edgbaston contact info |
UK (BIRMINGHAM) | participant | 208˙260.00 |
6 |
COMMISSARIAT A L ENERGIE ATOMIQUE ET AUX ENERGIES ALTERNATIVES
Organization address
address: RUE LEBLANC 25 contact info |
FR (PARIS 15) | participant | 180˙725.00 |
7 |
CENTRO DE INVESTIGACAO EM ASTRONOMIA E ASTROFISICA DA UNIVERSIDADE DO PORTO
Organization address
address: Rua das Estrelas contact info |
PT (Porto) | participant | 150˙460.00 |
8 |
AARHUS UNIVERSITET
Organization address
address: Nordre Ringgade 1 contact info |
DK (AARHUS C) | participant | 144˙660.00 |
9 |
INSTITUTO DE ASTROFISICA DE CANARIAS
Organization address
address: CALLE VIA LACTEA contact info |
ES (SAN CRISTOBAL DE LA LAGUNA) | participant | 97˙940.00 |
10 |
ISTITUTO NAZIONALE DI ASTROFISICA
Organization address
address: Viale del Parco Mellini 84 contact info |
IT (ROMA) | participant | 95˙460.00 |
11 | "DET KONGELIGE BIBLIOTEK, NATIONALBIBLIOTEK OG KOBENHAVNS UNIVERSITETSBIBLIOTEK" | DK | participant | 0.00 |
12 |
AGENCIA ESTATAL CONSEJO SUPERIOR DE INVESTIGACIONES CIENTIFICAS
Organization address
address: CALLE SERRANO 117 contact info |
ES (MADRID) | participant | 0.00 |
13 |
ASSOCIATION OF UNIVERSITIES FOR RESEARCH IN ASTRONOMY
Organization address
address: NEW YORK AVENUE NW 1212 SUITE 450 contact info |
US (WASHINGTON DC) | participant | 0.00 |
14 |
MAGYAR TUDOMANYOS AKADEMIA CSILLAGASZATI ES FOLDTUDOMANYI KUTATOKOZPONT
Organization address
address: CSATKAI ENDRE UTCA 6-8 contact info |
HU (Sopron) | participant | 0.00 |
15 |
UNIVERSITE PARIS-SUD
Organization address
address: RUE GEORGES CLEMENCEAU 15 contact info |
FR (ORSAY) | participant | 0.00 |
16 |
UNIVERSITE PAUL SABATIER TOULOUSE III
Organization address
address: ROUTE DE NARBONNE 118 contact info |
FR (TOULOUSE CEDEX 9) | participant | 0.00 |
17 |
UNIVERSITY CORPORATION FOR ATMOSPHERIC RESEARCH NONPROFIT CORPORATION
Organization address
address: Table Mesa Drive 1850 contact info |
US (Boulder Co) | participant | 0.00 |
Esplora la "nuvola delle parole (Word Cloud) per avere un'idea di massima del progetto.
'Observations of oscillations on the solar and stellar surfaces have emerged as a unique and extremely powerful tool to gain information on, and understanding of, the processes in the Sun and stars, and the origin of the variability in the solar and stellar output. Through helio- and asteroseismology detailed inferences of the internal structure and rotation of the Sun, and extensive information on the properties of a broad range of stars can be obtained.
Space-based observations play a leading role in helio- and asteroseismology, in close synergy with ground-based observations as well as theoretical modelling. Long observing sequences are essential for measuring the oscillation frequencies with the precision required, and to extract the lowest mode frequencies involved. The enormous value of long-term space-based observations has been demonstrated in the solar case by the joint ESA/NASA SOHO mission (Solar and Heliospheric Observatory. This is now being followed by instruments on the NASA Solar Dynamics Observatory (SDO) mission.Large volumes of exquisite data on stellar oscillations of stars with a broad range of masses and ages are being collected by the CNES space mission CoRoT (Convection, Rotation and Transit) and the NASA Kepler mission.
Extensive Earth-based observations of solar oscillations have been undertaken with the GONG network (Global Oscillations Network Group) and the Birmingham Oscillation Network (BiSON) to ensure continuous monitoring. A asteroseismic network, SONG (Stellar Observations Network Group) is being established under Danish leadership. Equally important for asteroseismology is the availability of supplementary data on the stars from more traditional observations, to determine their surface temperature, composition, radius, etc. Only through a coordinated use of the space- and ground-based data can the full potential of helio- and asteroseismology be realized.'
No parts of our Universe are harder to explore than the interior of stars. With the support of the EU, asteroseismologists make use of oscillations observed on the surface of pulsating stars to study their internal structure.