Modulation of Galactic Cosmic Ray Particles observed on board
the Ulysses Spacecraft
B. Heber, A. Raviart, C. Paizis, M. Bialk, W. Dröge,
R. Ducros, P. Ferrando, H. Kunow, R. Müller-Mellin,
C. Rastoin, K. Röhrs, and G. Wibberenz.
Modulation of Galactic Cosmic Rays Particles observed on board the Ulysses
Spacecraft
Proceedings of the 23th International Cosmic Ray Conference
3. 1993
Contents
The variation of electron, proton and alpha-particle fluxes has been analysed
using the data collected bey the Kiel Electron Telescope on board the Ulysses
spacecraft from November 1990 to January 1993. During that time
Ulysses traveled between 1 AU and 5.4 AU close to the ecliptic plane.
The authors present fluxes, temporal variations, and radial gradients of
galactic cosmic rays from > 30 MeV/n, using
IMP-8
and
Kiel neutron monitor
They conclude, that the variation of nuclei > 1000 MV/c magnetic
rigidity can be fitted with a model assuming exponential variations with time
and radial distance. The annual variation for nuclei decreases with increasing
mean magnetic rigidity, whereas the annual variation of electrons seems to be
weaker. The radial gradient for nuclei in the GV rigidity range from the data
analysed so far shows a slight decrease with rigidity. The averaged value of
about 3.3 %/AU determined directly for relativistic particles is in good
agreement with integral gradients from previous missions.
Channel T P gamma_3 gamma
MeV/n MV %/a %/a
P116 125 - 320 680 107 +- 5.6
P190 320 - 2100 1620 91.2+- 9.7 77.0+-2.0
P4000 > 2100 6000 27.1+- 2.4 23.6+-1.0
A32 34 - 125 800 218 +-22
A116 125 - 320 1140 123 +-16.7
A190 320 - 2100 3240 81.6+- 6.9 71.1+-4.1
A4000 > 2100 12000 16.6+- 4.3 14.1+-0.6
E12 60 - 500 120 12 +- 5
E300 > 150 800 61 +-20
KNM > 1500 17100 14.9+- 3.5 10.4+-1.0
IMP-8 > 106 2000 76.5+- 5.0
Energy ranges T, weighted mean rigidity P and temporal rate
of increase gamma for protons, alpha-particles and electrons of
KET, IMP-8 and the Kiel neutron monitor (KNM)
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