Solar energetic particle access to distant longitudes through turbulent field-line meandering

Author： Laitinen T.   Kopp A.   Effenberger F.   Dalla S.   Marsh M. S.  

Publisher： Edp Sciences

E-ISSN： 1432-0746|591|issue|A18-A18

ISSN： 0004-6361

Source： Astronomy & Astrophysics, Vol.591, Iss.issue, 2016-06, pp. : A18-A18

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

Abstract

Related content

Prediction of solar active longitudes

By  

Astronomy & Astrophysics, Vol. 484, Iss. 2, 2008-06 ,pp. : 523-527

Edp Sciences

Access to resources Recommend Favorite

Interpretation of second solar spectrum observations of the Sr I 4607 Å line in a quiet region: Turbulent magnetic field strength determination

By  

Astronomy & Astrophysics, Vol. 432, Iss. 1, 2005-03 ,pp. : 295-305

Edp Sciences

Access to resources Recommend Favorite

Second solar spectrum of the Sr I 4607 Å line: depth probing of the turbulent magnetic field strength in a quiet region

By  

Astronomy & Astrophysics, Vol. 457, Iss. 3, 2006-10 ,pp. : 1047-1052

Edp Sciences

Access to resources Recommend Favorite

Solar energetic particle event onset as analyzed from simulated data

By  

Astronomy & Astrophysics, Vol. 420, Iss. 1, 2004-06 ,pp. : 343-350

Edp Sciences

Access to resources Recommend Favorite

Observation of a solar energetic particle event behind previous coronal mass ejection

By  

Astronomy & Astrophysics, Vol. 497, Iss. 1, 2009-04 ,pp. : L1-L4

Edp Sciences

Access to resources Recommend Favorite