z-logo
open-access-imgOpen Access
Delay Time from Flare to SC-Storm as Function of Pre-Existing Geomagnetic Conditions.
Author(s) -
Marion W. Haurwitz
Publication year - 1962
Publication title -
the astronomical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.61
H-Index - 271
eISSN - 1538-3881
pISSN - 0004-6256
DOI - 10.1086/108629
Subject(s) - physics , geomagnetic storm , flare , solar flare , earth's magnetic field , function (biology) , astronomy , storm , coronal mass ejection , astrophysics , meteorology , solar wind , magnetic field , evolutionary biology , biology , quantum mechanics

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