Within the statistical limits imposed by the currently available data and the noise inherent in the determination of the latitudinal gradient, no evidence for the expected change in the latitudinal gradient from pre-1980 to post-1980 epochs can be found. In addition, the rigidity dependence of the gradient appears to be the same in the two epochs. Thus, no evidence is found for a sensitivity of the latitudinal gradient to the polarity of the largescale heliospheric magnetic field such as has been predicted by models incorporating particle drifts
Context. During the transition from solar cycle 23 to 24 from 2006 to 2009, the Sun was in an unusua...
We have used data from the Voyager I (VI), Voyager 2 (V2), and Pioneer IO (PIO) spacecraft to monit...
The radial and latitudinal gradients of anomalous cosmic rays (ACRs) in the heliosphere are expect...
We have used measurements from instruments on Voyagers 1 and 2 and Pioneer 10 to derive simultaneous...
We have computed the magnitude and direction of the asymmetry of cosmic-ray particle density gradien...
Cosmic ray drift directions depend both on the charge of the particle population under consideration...
Since early 1985, negative latitudinal gradients in the fluxes of anomalous and galactic cosmic ray...
Since mid-1985, the average flux of >70 MeV/nucleon cosmic rays at Voyager 2 (r_2 ∼ 17 AU, Θ_2 ∼ 0°)...
Simultaneous magnetic field and charged particle measurements from the Voyager spacecraft with helio...
We have used measurements from instruments on Voyagers 1 and 2 and Pioneer 10 to derive simultaneou...
The significant effect of drift on the radial and latitudinal dependence of cosmic rays for consecut...
A well-established, comprehensive 3-D numerical modulation model is applied to simulate galactic pro...
Abstract. Since mid-1985, the average flux of>70 MeV/nucleon cosmic rays at Voyager 2 (r•.-17 AU,...
Two cosmic rays which pass through the same point going in opposite directions will, in the absence ...
The cosmic rays differential intensity inside the heliosphere, for energy below 30 GeV/nuc, depends ...
Context. During the transition from solar cycle 23 to 24 from 2006 to 2009, the Sun was in an unusua...
We have used data from the Voyager I (VI), Voyager 2 (V2), and Pioneer IO (PIO) spacecraft to monit...
The radial and latitudinal gradients of anomalous cosmic rays (ACRs) in the heliosphere are expect...
We have used measurements from instruments on Voyagers 1 and 2 and Pioneer 10 to derive simultaneous...
We have computed the magnitude and direction of the asymmetry of cosmic-ray particle density gradien...
Cosmic ray drift directions depend both on the charge of the particle population under consideration...
Since early 1985, negative latitudinal gradients in the fluxes of anomalous and galactic cosmic ray...
Since mid-1985, the average flux of >70 MeV/nucleon cosmic rays at Voyager 2 (r_2 ∼ 17 AU, Θ_2 ∼ 0°)...
Simultaneous magnetic field and charged particle measurements from the Voyager spacecraft with helio...
We have used measurements from instruments on Voyagers 1 and 2 and Pioneer 10 to derive simultaneou...
The significant effect of drift on the radial and latitudinal dependence of cosmic rays for consecut...
A well-established, comprehensive 3-D numerical modulation model is applied to simulate galactic pro...
Abstract. Since mid-1985, the average flux of>70 MeV/nucleon cosmic rays at Voyager 2 (r•.-17 AU,...
Two cosmic rays which pass through the same point going in opposite directions will, in the absence ...
The cosmic rays differential intensity inside the heliosphere, for energy below 30 GeV/nuc, depends ...
Context. During the transition from solar cycle 23 to 24 from 2006 to 2009, the Sun was in an unusua...
We have used data from the Voyager I (VI), Voyager 2 (V2), and Pioneer IO (PIO) spacecraft to monit...
The radial and latitudinal gradients of anomalous cosmic rays (ACRs) in the heliosphere are expect...
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