Oxygen abundance in coronal streamers

In a previous work we developed a stationary proton-electron MHD model of the solar corona, suitable for the minimum-activity epochs. In the present work, we use empirically derived information from the past solar minimum for the oxygen parameters (temperatures and outflow velocity) to develop an ox...

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Detalles Bibliográficos
Autores principales:	Vásquez, A.M., Raymond, J.C.
Formato:	JOUR
Materias:	Solar wind Sun: abundances Sun: corona Sun: UV radiation
Acceso en línea:	http://hdl.handle.net/20.500.12110/paper_0004637X_v619_n2I_p1132_Vasquez
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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