Drolias, B.; Quenby, J. J.; Witcombe, A.; Korth, A.; Keppler, E.; Blake, J. B.: Numerical simulations of non-adiabatic particle motions in the Jovian magnetosphere; comparisons with ULYSSES observations. Planetary and Space Science 44, S. 153 - 161 (1996)
Friedel, R. H. W.; Korth, A.; Kremser, G.: Substorm onsets observed by CRRES: Determination of energetic particle source regions. Journal Geophysical Research 101, S. 13137 - 13154 (1996)
Keppler, E.; Drolias, B.; Fränz, M.; Korth, A.; Reuss, M. K.; Blake, J. B.; Quenby, J. J.: The high latitude pass of ULYSSES: energetic particle observations with EPAC. Astronomy and Astrophysics 316, S. 464 - 480 (1996)
Pu, Z. Y.; Hong, M. H.; Wang, X. M.; Chen, Z. X.; Fu, S. Y.; Zong, Q.-G.; Wang, J. F.; Liu, Z. X.; Korth, A.; Friedel, R. H. W.et al.; Kremser, G.: A substorm expansion model based on configuration instability of the near-Earth magnetotail: I. Configuration instability in the near-Earth magnetotail. Acta Geophysica Sinica 39, S. 141 (1996)
Blake, J. B.; Fennell, J. F.; Friesen, L. M.; Johnson, B. M.; Kolasinski, W. A.; Mabry, D. J.; Osborn, J. V.; Penzin, S. H.; Schnauss, E. R.; Spence, H. E.et al.; Baker, D. N.; Belian, R.; Fritz, T. A.; Ford, W.; Laubscher, B.; Stiglich, R.; Baraze, R. A.; Hilsenrath, M. F.; Imhof, W. L.; Kilner, J. R.; Mobilia, J.; Voss, D. H.; Korth, A.; Güll, M.; Fischer, K.; Grande, M.; Hall, D.: CEPPAD. Space Science Reviews 71, S. (7)531 - (7)562 (1995)
Friedel, R. H. W.; Korth, A.: Long-term observations of keV ion and electron variability in the outer radiation belt from CRRES. Geophysical Research Letters 22, S. 1853 - 1856 (1995)
Keppler, E.; Fränz, M.; Korth, A.; Krupp, N.; Reuss, M. K.; Wilken, B.; Balogh, A.; Forsyth, R. J.; Quenby, J. J.; Blake, B.: Energetic particle observations at high heliographic latitudes. Space Science Reviews 72, S. 285 - 289 (1995)
Keppler, E.; Fränz, M.; Korth, A.; Reuss, M. K.; Blake, J. B.; Seidel, R.; Quenby, J. J.; Witte, M.: Observations of energetic particles with EPAC on Ulysses in polar latitudes of the heliosphere. Science 268, S. 1013 - 1016 (1995)
Kirsch, E.; McKenna-Lawlor, S.; Korth, A.; Schwenn, R.: Particle fluxes observed in the magnetic pileup regions of Comets Halley and Grigg-Skjellerup. Advances in Space Research 16, S. (4)29 - (4)34 (1995)
Kopányi, V.; Korth, A.: Energetic particle dropouts observed in the morning sector by the geostationary satellite GEOS-2. Geophysical Research Letters 22, S. 73 - 76 (1995)
Krupp, N.; Keppler, E.; Korth, A.; Fränz, M.; Reuss, M. K.; Balogh, A.; Dougherty, M. K.: Ion measurements in the Jovian magnetosphere by the Ulysses EPAC experiment: A comparison between dawn and dusk sectors. Advances in Space Research 16, S. (4)183 - (4)186 (1995)
Korth, A.; Vampola, A. L.: Cross-L motion of a relativistic electron belt formed in the slot region. Journal Geophysical Research 99 (A7), S. 13529 - 13535 (1994)
Pulkkinen, T. I.; Baker, D. N.; Toivanen, P. K.; Pellinen, R. J.; Friedel, R. H. W.; Korth, A.: Magnetospheric field and current distributions during the substorm recovery phase. Journal Geophysical Research 99 (A6), S. 10955 - 10966 (1994)
Rème, H.; Mazelle, C.; d'Uston, C.; Korth, A.; Lin, R. P.; Chaizy, P.: There is no ``cometopause'' at comet Halley. Journal Geophysical Research 99 (A2), S. 2301 - 2308 (1994)
Krupp, N.; Keppler, E.; Korth, A.; Fränz, M.; Balogh, A.; Dougherty, M. K.: Three-dimensional particle anisotropies in and near the plasma sheet of Jupiter observed by the EPAC experiment on board the Ulysses spacecraft. Planetary and Space Science 41, S. 953 - 966 (1993)
Keppler, E.; Blake, J. B.; Fränz, M.; Korth, A.; Krupp, N.; Quenby, J. J.; Witte, M.; Woch, J.: An overview of energetic particle measurements in the Jovian magnetosphere with the EPAC sensor on Ulysses. Science 257, S. 1553 - 1557 (1992)
Bewerbungsfrist 1 Oktober 2023. Promotionsprojekte in Planetenwissenschaften, Sonnenphysik, Astrophysik, Magnetfelder der Sonne, Helioseismologie, Asteroseismologie ...
In der mittleren Korona der Sonne entdeckt ein Forscherteam netzartige, dynamische Plasmastrukturen – und einen wichtigen Hinweis auf den Antrieb des Sonnenwindes.