z-logo
open-access-imgOpen Access
Helioseismically Determined Near‐Surface Flows Underlying a Quiescent Filament
Author(s) -
Bradley W. Hindman,
D. A. Haber,
Juri Toomre
Publication year - 2006
Publication title -
the astrophysical journal
Language(s) - Uncategorized
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/508603
Subject(s) - physics , protein filament , solar prominence , astrophysics , convection , helioseismology , magnetic field , magnetic flux , magnetohydrodynamics , photosphere , convection zone , coronal hole , sunspot , mechanics , coronal mass ejection , solar wind , genetics , quantum mechanics , biology

The content you want is available to Zendy users.

Already have an account? Click here to sign in.
Having issues? You can contact us here
Accelerating Research

Address

John Eccles House
Robert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom