z-logo
open-access-imgOpen Access
Magnetohydrodynamic Turbulence of Coronal Active Regions and the Distribution of Nanoflares
Author(s) -
P. Dmitruk,
Daniel O. Gómez,
E. E. DeLuca
Publication year - 1998
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/306182
Subject(s) - physics , nanoflares , dissipation , magnetohydrodynamic turbulence , coronal loop , magnetohydrodynamics , magnetohydrodynamic drive , astrophysics , solar flare , turbulence , dissipative system , flare , magnetic energy , computational physics , corona (planetary geology) , mechanics , classical mechanics , plasma , solar wind , magnetic field , coronal mass ejection , magnetization , quantum mechanics , astrobiology , venus , thermodynamics

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