Interplanetary magnetic field associated changes in cosmic ray intensity and geomagnetic field during 1973-75

Physics – Space Physics

Scientific paper

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Cosmic Rays, Interplanetary Magnetic Fields, Magnetic Variations, Solar Activity Effects, Solar Terrestrial Interactions, Data Correlation, Geomagnetism, Histograms, Particle Intensity

Scientific paper

The effect of interplanetary magnetic field (IMF) B and its Bz component on cosmic ray intensity and geomagnetic field variations have been examined for the period 1973-75. It is observed that (1) B not less than 10 gamma (magnetic blobs) is a pre-requisite in producing cosmic ray intensity and geomagnetic field variations of varying magnitudes; (2) the longer existence of magnetic blobs on successive days produces larger decreases in cosmic ray intensity and geomagnetic field; (3) the southward component (Bz) of IMF generally gives rise to large Ap changes, though it is not effective in producing cosmic ray intensity decreases.

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