z-logo
open-access-imgOpen Access
On the Inflation of the Geomagnetic Field during a Magnetic Storm
Author(s) -
Ferraro V. C. A.
Publication year - 1971
Publication title -
geophysical journal of the royal astronomical society
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.302
H-Index - 168
eISSN - 1365-246X
pISSN - 0016-8009
DOI - 10.1111/j.1365-246x.1971.tb02196.x
Subject(s) - geomagnetic storm , earth's magnetic field , geophysics , magnetic field , storm , geology , physics , plasma , geodesy , inflation (cosmology) , ring current , computational physics , atmospheric sciences , meteorology , astronomy , nuclear physics , quantum mechanics
Summary A more accurate discussion than in an earlier paper is given of the inflation of the geomagnetic field during the main phase of a magnetic storm. The radial velocity of the injected plasma is found to be of the order of 1 km s ‐1 . Energy consideration suggests that a proton plasma of energy density of 2.4 × 10 −7 erg cm ‐3 would be more than adequate to supply the magnetic energy of the storm.

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