Add to ORKGSimultaneous magnetic field and charged particle measurements from the Voyager spacecraft at heliographic latitude separations from 10 deg. to 21 deg. are used to determine the latitude gradient of the galactic cosmic ray flux with respect to the interplanetary current sheet. By comparing the ratio of cosmic ray flux at Voyager 1 to that a Voyager 2 during periods when both spacecraft are first nort and then south of the interplanetary current sheet, we find an estimate of the latitudinal gradient with respect to the current sheet of approximately -0.15 + or 0.05% deg under restricted interplanetary conditions
Cosmic ray particle transport in solar corona by drifting along current sheets separating discontinu...
Measurements of radial and latitudinal gradients of galactic cosmic rays and anomalous components no...
Two cosmic rays which pass through the same point going in opposite directions will, in the absence ...
Simultaneous magnetic field and charged particle measurements from the Voyager spacecraft at heliog...
Simultaneous magnetic field and charged particle measurements from the Voyager spacecraft with helio...
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°)...
Since early 1985, negative latitudinal gradients in the fluxes of anomalous and galactic cosmic ray...
Abstract. Since mid-1985, the average flux of>70 MeV/nucleon cosmic rays at Voyager 2 (r•.-17 AU,...
Results of the numerical solution of the anistoropic diffusion equation are presented. The modulatio...
We have used measurements from instruments on Voyagers 1 and 2 and Pioneer 10 to derive simultaneous...
We have used measurements from instruments on Voyagers 1 and 2 and Pioneer 10 to derive simultaneou...
Aspects of the problem of galactic cosmic ray propagation, including inversion of the solar total ma...
The radial gradient of anomalous cosmic ray oxygen measured instantaneously between Voyager 2 and Pi...
We have computed the magnitude and direction of the asymmetry of cosmic-ray particle density gradien...
Cosmic ray particle transport in solar corona by drifting along current sheets separating discontinu...
Measurements of radial and latitudinal gradients of galactic cosmic rays and anomalous components no...
Two cosmic rays which pass through the same point going in opposite directions will, in the absence ...
Simultaneous magnetic field and charged particle measurements from the Voyager spacecraft at heliog...
Simultaneous magnetic field and charged particle measurements from the Voyager spacecraft with helio...
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°)...
Since early 1985, negative latitudinal gradients in the fluxes of anomalous and galactic cosmic ray...
Abstract. Since mid-1985, the average flux of>70 MeV/nucleon cosmic rays at Voyager 2 (r•.-17 AU,...
Results of the numerical solution of the anistoropic diffusion equation are presented. The modulatio...
We have used measurements from instruments on Voyagers 1 and 2 and Pioneer 10 to derive simultaneous...
We have used measurements from instruments on Voyagers 1 and 2 and Pioneer 10 to derive simultaneou...
Aspects of the problem of galactic cosmic ray propagation, including inversion of the solar total ma...
The radial gradient of anomalous cosmic ray oxygen measured instantaneously between Voyager 2 and Pi...
We have computed the magnitude and direction of the asymmetry of cosmic-ray particle density gradien...
Cosmic ray particle transport in solar corona by drifting along current sheets separating discontinu...
Measurements of radial and latitudinal gradients of galactic cosmic rays and anomalous components no...
Two cosmic rays which pass through the same point going in opposite directions will, in the absence ...