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Latitudinal and radial gradients of galactic cosmic ray protons in the inner heliosphere - PAMELA and Ulysses observations
DOI: 10.5194/astra-7-425-2011 Bibcode: 2011ASTRA...7..425D

Gieseler, J.; Heber, B.; Picozza, P. +5 more

Ulysses, launched on 6 October 1990, was placed in an elliptical, high inclined (80.2°) orbit around the Sun, and was switched off in June 2009. It has been the only spacecraft exploring high-latitude regions of the inner heliosphere. The Kiel Electron Telescope (KET) aboard Ulysses measures electrons from 3 MeV to a few GeV and protons and helium…

2011 Astrophysics and Space Sciences Transactions
Ulysses 56
Three dimensional model of the interplanetary magnetic field and 27-day variation of the galactic cosmic ray intensity
DOI: 10.5194/astra-7-351-2011 Bibcode: 2011ASTRA...7..351W

Wawrzynczak, A.; Modzelewska, R.; Alania, M. V.

We present a model of the 27-day variation of the galactic cosmic ray (GCR) intensity for three dimensional (3-D) heliosphere with the heliolongitudinal and heliolatitudinal dependent radial solar wind speed for the period of 1995 - minimum epoch of solar activity (A>0). In the present model we implement heliolongitudinal asymmetry of solar win…

2011 Astrophysics and Space Sciences Transactions
Ulysses 1
Observations of anomalous transport of energetic electrons in the heliosphere
DOI: 10.5194/astra-4-27-2008 Bibcode: 2008ASTRA...4...27P

Perri, S.; Zimbardo, G.

We study the propagation of energetic particles, accelerated by interplanetary shock waves, upstream of the shock, considering the possibility of having anomalous transport. The theoretical treatment of the anomalous transport is developed via the propagator formalism, considering that in the case of a superdiffusive transport the propagator has p…

2008 Astrophysics and Space Sciences Transactions
Ulysses 8