Add to ORKGWe present an analytic method to determine the directions of the three-dimensional (3D) heliospheric current sheet (HCS) drift for any tilt angle based on Parker’s heliospheric magnetic field and compare it with published two-dimensional and quasi-3D methods. We also present a new approach to determine the magnitude of the 3D HCS drift numerically. Implications of these new methods for the solar modulation of Galactic cosmic rays are considered and compared with results from prior methods reported in the literature. Our results support the concept that HCS drift plays an important role in the solar modulation of cosmic rays
Aims.We study certain aspects of the solar modulation of galactic cosmic ray intensity during differ...
Abstract: Although cosmic ray (CR) modulation has been widely investigated in the past it is still d...
Drifts due to the curvature and gradients in the heliospheric magnetic field, as well as along the h...
We present an analytic method to determine the directions of the three-dimensional (3D) heliospheric...
PhD (Space Physics), North-West University, Potchefstroom CampusA dominant feature in the heliospher...
Abstract: We present a new method to include a 3D wavy heliospheric current sheet into a 2D numerica...
Drift along the wavy heliospheric neutral sheet is believed to play an important role in cosmic-ray ...
Recently, the modulation of cosmic rays in the heliosphere has increasingly been studied by solving...
Drifts are one of the major cosmic ray modulation mechanisms in the heliosphere. Three types of drif...
[1] We present a quasi-steady two-dimensional (axisymmetric) model of the heliospheric transport of ...
Abstract: The waviness of the heliospheric current sheet (HCS) is incorporated into a 3D model for t...
Transport equation of the galactic cosmic ray (GCR) is numerically solved for qA>0 and qA<0 based on...
The recent 2007-2009 weak and long solar minimum offers unique possibilities for gaining new insight...
The heliospheric current sheet (HCS) is a permanent solar wind feature, with well predicted Earth pa...
Copyright © 2010 American Institute of Physics. This article may be downloaded for personal use only...
Aims.We study certain aspects of the solar modulation of galactic cosmic ray intensity during differ...
Abstract: Although cosmic ray (CR) modulation has been widely investigated in the past it is still d...
Drifts due to the curvature and gradients in the heliospheric magnetic field, as well as along the h...
We present an analytic method to determine the directions of the three-dimensional (3D) heliospheric...
PhD (Space Physics), North-West University, Potchefstroom CampusA dominant feature in the heliospher...
Abstract: We present a new method to include a 3D wavy heliospheric current sheet into a 2D numerica...
Drift along the wavy heliospheric neutral sheet is believed to play an important role in cosmic-ray ...
Recently, the modulation of cosmic rays in the heliosphere has increasingly been studied by solving...
Drifts are one of the major cosmic ray modulation mechanisms in the heliosphere. Three types of drif...
[1] We present a quasi-steady two-dimensional (axisymmetric) model of the heliospheric transport of ...
Abstract: The waviness of the heliospheric current sheet (HCS) is incorporated into a 3D model for t...
Transport equation of the galactic cosmic ray (GCR) is numerically solved for qA>0 and qA<0 based on...
The recent 2007-2009 weak and long solar minimum offers unique possibilities for gaining new insight...
The heliospheric current sheet (HCS) is a permanent solar wind feature, with well predicted Earth pa...
Copyright © 2010 American Institute of Physics. This article may be downloaded for personal use only...
Aims.We study certain aspects of the solar modulation of galactic cosmic ray intensity during differ...
Abstract: Although cosmic ray (CR) modulation has been widely investigated in the past it is still d...
Drifts due to the curvature and gradients in the heliospheric magnetic field, as well as along the h...