Time dependent model of the interplanetary Lyman $\sf \alpha$ glow: applications to the SWAN data

E-ISSN： 1432-0746|488|1|351-359

ISSN： 0004-6361

Source： Astronomy & Astrophysics, Vol.488, Iss.1, 2008-09, pp. : 351-359

Disclaimer: Any content in publications that violate the sovereignty, the constitution or regulations of the PRC is not accepted or approved by CNPIEC.

Previous Menu Next

Related content

Effects of the heliospheric interface on the interplanetaryLyman $\alpha$ glow seen at 1 AU from the Sun

Astronomy & Astrophysics, Vol. 396, Iss. 1, 2002-12 ,pp. : 269-281

Edp Sciences

Access to resources Recommend Favorite

Response of the groove in heliospheric Lyman-$\alpha$ glow to latitude-dependent ionization rate

Astronomy & Astrophysics, Vol. 408, Iss. 3, 2003-09 ,pp. : 1155-1164

Edp Sciences

Access to resources Recommend Favorite

Interplanetary Lyman $\alpha$ line profiles: variations with solar activity cycle

Astronomy & Astrophysics, Vol. 455, Iss. 3, 2006-09 ,pp. : 1135-1142

Edp Sciences

Access to resources Recommend Favorite

Collisional effects in the far red wing of Lyman-$\sf \alpha$

Astronomy & Astrophysics, Vol. 493, Iss. 3, 2009-01 ,pp. : 1155-1160

Edp Sciences

Access to resources Recommend Favorite

Latitudinal structure and north-south asymmetry of the solar windfrom Lyman-$\alpha$ remote sensing by SWAN

Astronomy & Astrophysics, Vol. 408, Iss. 3, 2003-09 ,pp. : 1165-1177

Edp Sciences

Access to resources Recommend Favorite