Open AccessInterplanetary magnetic field polarities inferred from the north–south cosmic ray anisotropy
Author(s) -
Laurenza M.,
Storini M.,
Moreno G.,
Fujii Z.
Publication year - 2003
Publication title -
journal of geophysical research: space physics
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.67
H-Index - 298
eISSN - 2156-2202
pISSN - 0148-0227
DOI - 10.1029/2002ja009509
Subject(s) - interplanetary magnetic field , interplanetary spaceflight , anisotropy , cosmic ray , polarity (international relations) , physics , astrophysics , earth's magnetic field , magnetic field , sunspot , geology , geophysics , computational physics , astronomy , solar wind , optics , genetics , quantum mechanics , biology , cell
The interplanetary magnetic field sector polarity at the Earth's location can be inferred from ground measurements of the cosmic ray north‐south anisotropy. We present here the results of a systematic comparison between inferred and directly measured polarities in the period from January 1971 through December 1997. The overall success rate of the prediction method is 72%, in rather good agreement with previous findings. On the other hand, our analysis shows for the first time the limits of the method and calls for warning in its use. In fact, it turns out that the inferred polarities are affected by a bias, which becomes more relevant around the sunspot minimum. Even though the bias cannot be removed, it is possible to select conditions, occurring for 30% of the time, under which the inferred polarities are very reliable (the success rate being 95%).