Add to ORKGRecent publications have related long-term variations in cosmic ray intensity at the Earth with long term variations in the tilt of the neutral sheet in the inner heliosphere. The tilt of the neutral sheet from 1971 to 1974 is compared with the cosmic ray intensity at Earth, recorded by the Mt. Washington neutron monitor. The remarkable large decreases in cosmic ray intensity which occurred in 1973 and 1974 correlate well with excursions in the tilt of the neutral sheet which occurred earlier during these same two years
Abstract Context: Galactic cosmic ray (GCR) intensities around solar minimum times are modulated by ...
Since the early 1970's, anomalous cosmic ray (ACR) intensities at 1 AU at solar minimum have general...
This paper reports Pioneer 10 (P10) and Pioneer 11 (P11) observations of the intensity J(E(sub p) gr...
Results of the numerical solution of the anistoropic diffusion equation are presented. The modulatio...
The method of calculating energy losses along regular particle trajectories is applied to obtain the...
The distribution of cosmic ray intensity perpendicular to solar equatorial plane, was investigated b...
AbstractGalactic cosmic ray intensities (GCRs) observed by five neutron monitors (NMs) have been use...
Using cosmic ray intensity data from the Deep River Neutron monitor and the relation between solar w...
Since mid-1985, the average flux of >70 MeV/nucleon cosmic rays at Voyager 2 (r_2 ∼ 17 AU, Θ_2 ∼ 0°)...
We have computed the magnitude and direction of the asymmetry of cosmic-ray particle density gradien...
A statistical study between the cosmic ray intensity, as observed by a neutron monitor, and of the g...
The radial gradient of anomalous cosmic ray oxygen measured instantaneously between Voyager 2 and Pi...
It is now established that the solar modulation of cosmic rays is produced by turbulent magnetic fie...
The network of cosmic ray observatories reaching across the heliosphere has given new insight into t...
The purpose of this project was to use the cosmic ray data from the IMP, Voyager and Pioneer spacecr...
Abstract Context: Galactic cosmic ray (GCR) intensities around solar minimum times are modulated by ...
Since the early 1970's, anomalous cosmic ray (ACR) intensities at 1 AU at solar minimum have general...
This paper reports Pioneer 10 (P10) and Pioneer 11 (P11) observations of the intensity J(E(sub p) gr...
Results of the numerical solution of the anistoropic diffusion equation are presented. The modulatio...
The method of calculating energy losses along regular particle trajectories is applied to obtain the...
The distribution of cosmic ray intensity perpendicular to solar equatorial plane, was investigated b...
AbstractGalactic cosmic ray intensities (GCRs) observed by five neutron monitors (NMs) have been use...
Using cosmic ray intensity data from the Deep River Neutron monitor and the relation between solar w...
Since mid-1985, the average flux of >70 MeV/nucleon cosmic rays at Voyager 2 (r_2 ∼ 17 AU, Θ_2 ∼ 0°)...
We have computed the magnitude and direction of the asymmetry of cosmic-ray particle density gradien...
A statistical study between the cosmic ray intensity, as observed by a neutron monitor, and of the g...
The radial gradient of anomalous cosmic ray oxygen measured instantaneously between Voyager 2 and Pi...
It is now established that the solar modulation of cosmic rays is produced by turbulent magnetic fie...
The network of cosmic ray observatories reaching across the heliosphere has given new insight into t...
The purpose of this project was to use the cosmic ray data from the IMP, Voyager and Pioneer spacecr...
Abstract Context: Galactic cosmic ray (GCR) intensities around solar minimum times are modulated by ...
Since the early 1970's, anomalous cosmic ray (ACR) intensities at 1 AU at solar minimum have general...
This paper reports Pioneer 10 (P10) and Pioneer 11 (P11) observations of the intensity J(E(sub p) gr...