CoRoT reveals a magnetic activity cycle in a sun-like star

Science

Volumn 329, Issue 5995, 2010, Pages 1032-

  García, Rafael A ^a   Mathur, Savita ^b   Salabert, David ^c,d   Ballot, Jérôme ^e   Régulo, Clara ^c,d   Metcalfe, Travis S ^b   Baglin, Annie ^f  

^a CEA SACLAY   (France)

^b NATIONAL CENTER FOR ATMOSPHERIC RESEARCH   (United States)

^c INSTITUTO DE ASTROFÍSICA DE CANARIAS   (Spain)

^d UNIVERSIDAD DE LA LAGUNA   (Spain)

^e UNIVERSITÉ DE TOULOUSE   (France)

^f UNIVERSITÉ PARIS DIDEROT   (France)

Author keywords

[No Author keywords available]

Indexed keywords

CALCIUM;

ASTRONOMY; EXTRATERRESTRIAL MATTER; MAGNETIC FIELD; SOLAR SYSTEM;

ACOUSTICS; ASTRONOMY; EVOLUTION; LIGHT; MAGNETIC FIELD; MAGNETISM; OSCILLATION; PRIORITY JOURNAL; SHORT SURVEY; SOLAR CYCLE; SUN;

EID: 77956128251     PISSN: 00368075     EISSN: 10959203     Source Type: Journal    
DOI: 10.1126/science.1191064     Document Type: Short Survey

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14. The CoRoT space mission has been developed and is operated by CNES, with contributions from Austria, Belgium, Brazil, European Space Agency (Research Science Support Department and Science Program), Germany, and Spain. This work has been partially supported by the Spanish National Research Plan (grant PNAyA2007-62650) and by the "Programme National de Physique Stellaire" at CEA/Saclay. NCAR is supported by NSF.