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Titel	Annales Geophysicae ; 21, no. 6
Erscheinungsjahr	2003
Medientyp	Stücktitel
ISSN	0992-7689
Erschienen	In: Annales Geophysicae (ANGEO) ; Nr. 21, no. 6 (2003)
Datensatznummer	96747


Teil von
Annales Geophysicae (ANGEO)


Teil(e)
Ulysses COSPIN observations of cosmic rays and solar energetic particles from the South Pole to the North Pole of the Sun during solar maximum \| R. B. McKibben Solar cycle variations of the energetic H/He intensity ratio at high heliolatitudes and in the ecliptic plane \| D. Lario A survey of 3He enhancements at 2–20 MeV/nucleon: Ulysses COSPIN/LET \| C. Tranquille Magnetic topology of coronal mass ejection events out of the ecliptic: Ulysses/HI-SCALE energetic particle observations \| O. E. Malandraki How did the solar wind structure change around the solar maximum? From interplanetary scintillation observation \| K. Fujiki Consequences of the Solar System passage through dense interstellar clouds \| A. G. Yeghikyan The Ulysses fast latitude scans: COSPIN/KET results \| B. Heber The charge-exchange induced coupling between plasma-gas counterflows in the heliosheath \| H. J. Fahr Latitudinal and radial variation of >2 GeV/n protons and alpha-particles at solar maximum: ULYSSES COSPIN/KET and neutron monitor network observations \| A. V. Belov Breathing of heliospheric structures triggered by the solar-cycle activity \| K. Scherer Imprints from the solar cycle on the helium atom and helium pickup ion distributions \| D. Rucinski Latitudinal extent of large-scale structures in the solar wind \| H. A. Elliott On the heliolatitudinal variation of the galactic cosmic-ray intensity. Comparison with Ulysses measurements \| G. Exarhos Dynamical evolution of the inner heliosphere approaching solar activity maximum: interpreting Ulysses observations using a global MHD model \| P. Riley Charge-sign dependent modulation in the heliosphere over a 22-year cycle \| S. E. S. Ferreira Delay in solar energetic particle onsets at high heliographic latitudes \| S. Dalla The global heliospheric magnetic field polarity distribution as seen at Ulysses \| G. H. Jones From the Sun’s south to the north pole – Ulysses COSPIN/LET composition measurements at solar maximum \| M. Y. Hofer