http://arxiv.org/abs/1802.04348
Data obtained over the last three solar cycles have been analysed to reveal the relationships between the intensity of the photospheric field measured along the line of sight by the WSO group at heliolatitudes from -75 to 75 degrees and the intensity of the interplanetary magnetic field and absolute values of the perturbations of the different characteristics of the solar wind at the Earth orbit, and geomagnetic parameters. provided by the OMNI team.
The heliospheric and geomagnetic data are found to be divided into two groups characterized by their response to variability of the solar magnetic field latitudinal structures on short and on long time scales.
E. Gavryuseva
Wed, 14 Feb 18
7/68
Comments: 14 pages, 6 Postscript figures. arXiv admin note: substantial text overlap with arXiv:1802.03135