Zobrazeno 1 - 10
of 153
pro vyhledávání: '"G. Wibberenz"'
Autor:
B. Heber, G. Sarri, G. Wibberenz, C. Paizis, P. Ferrando, A. Raviart, A. Posner, R. Müller-Mellin, H. Kunow
Publikováno v:
Annales Geophysicae, Vol 21, Pp 1275-1288 (2003)
Ulysses, launched in October 1990, began its second out-of-ecliptic orbit in December 1997, and its second fast latitude scan in September 2000. In contrast to the first fast latitude scan in 1994/1995, during the second fast latitude scan sola
Externí odkaz:
https://doaj.org/article/26394e019c1a400e803e246ffae4f8c9
Autor:
Reinhold Müller-Mellin, Philippe Ferrando, Bernd Heber, G. Sarri, H. Kunow, A. Raviart, C. Paizis, G. Wibberenz, Arik Posner
Publikováno v:
Annales Geophysicae
Annales Geophysicae, European Geosciences Union, 2003, 21 (6), pp.1275-1288
Annales Geophysicae, Vol 21, Pp 1275-1288 (2003)
Annales Geophysicae, Vol 21, Iss 6, Pp 1275-1288 (0000)
Annales geophysicae (1988) 21 (2003): 1275–1288.
info:cnr-pdr/source/autori:B. Heber, G. Sarri, G. Wibberenz, C. Paizis, P. Ferrando, A. Raviart, A. Posner, R. Mueller-Mellin, H. Kunow/titolo:The Ulysses fast latitude scans: COSPIN KET results/doi:/rivista:Annales geophysicae (1988)/anno:2003/pagina_da:1275/pagina_a:1288/intervallo_pagine:1275–1288/volume:21
Annales Geophysicae, 2003, 21 (6), pp.1275-1288
Annales Geophysicae, European Geosciences Union, 2003, 21 (6), pp.1275-1288
Annales Geophysicae, Vol 21, Pp 1275-1288 (2003)
Annales Geophysicae, Vol 21, Iss 6, Pp 1275-1288 (0000)
Annales geophysicae (1988) 21 (2003): 1275–1288.
info:cnr-pdr/source/autori:B. Heber, G. Sarri, G. Wibberenz, C. Paizis, P. Ferrando, A. Raviart, A. Posner, R. Mueller-Mellin, H. Kunow/titolo:The Ulysses fast latitude scans: COSPIN KET results/doi:/rivista:Annales geophysicae (1988)/anno:2003/pagina_da:1275/pagina_a:1288/intervallo_pagine:1275–1288/volume:21
Annales Geophysicae, 2003, 21 (6), pp.1275-1288
Ulysses, launched in October 1990, began its second out-of-ecliptic orbit in December 1997, and its second fast latitude scan in September 2000. In contrast to the first fast latitude scan in 1994/1995, during the second fast latitude scan solar acti
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cfd1bbbfb94d8873a093c4f12c56f063
https://www.ann-geophys.net/21/1275/2003/
https://www.ann-geophys.net/21/1275/2003/
Autor:
Reinhold Müller-Mellin, R. B. McKibben, Ming Zhang, Bernd Heber, Richard G. Marsden, Stefan Ferreira, C. Paizis, H. Kunow, M. S. Potgieter, Silvia Dalla, G. Wibberenz, G. Sarri
Publikováno v:
Planetary and Space Science. 55:1-11
Since the 1970's interplanetary electrons in the MeV energy range, of Jovian origin, have been extensively studied from close to the Sun to beyond the Kronian orbit, near the ecliptic. The Ulysses trajectory allowed to study the propagation of these
Autor:
Hilary V. Cane, G. Wibberenz
Publikováno v:
The Astrophysical Journal. 650:1199-1207
For a number of impulsive solar particle events we examine variations of maximum intensities and times to maximum intensity as a function of longitude, using observations from the two Helios spacecraft and near the Earth. We find that electrons in th
Autor:
M. S. Potgieter, Bernd Heber, Stefan Ferreira, R. A. Burger, G. Sarri, R. Mfiller-Mellin, Horst Fichtner, Arik Posner, Philippe Ferrando, C. Paizis, G. Wibberenz, H. Kunow, A. Raviart
Publikováno v:
Advances in space research 32 (2003): 663–668.
info:cnr-pdr/source/autori:B. Heber, P. Ferrando, A. Raviart, C. Paizis, G. Sarri, A. Posner, G. Wibberenz, R. Mueller-Mellin, H. Kunow, M.S. Potgieter, S. E. S. Ferreira, R. A. Burger, H. Fichtner/titolo:Quiet time MeV electron increases at solar maximum. Ulysses COSPIN KET observations/doi:/rivista:Advances in space research/anno:2003/pagina_da:663/pagina_a:668/intervallo_pagine:663–668/volume:32
info:cnr-pdr/source/autori:B. Heber, P. Ferrando, A. Raviart, C. Paizis, G. Sarri, A. Posner, G. Wibberenz, R. Mueller-Mellin, H. Kunow, M.S. Potgieter, S. E. S. Ferreira, R. A. Burger, H. Fichtner/titolo:Quiet time MeV electron increases at solar maximum. Ulysses COSPIN KET observations/doi:/rivista:Advances in space research/anno:2003/pagina_da:663/pagina_a:668/intervallo_pagine:663–668/volume:32
The Ulysses trajectory provides a unique opportunity to study the propagation of MeV electrons in a wide range of heliographic latitudes and during varying conditions in the inner heliosphere. In recent papers we reported Ulysses Kiel Electron Telesc
Autor:
Horst Fichtner, P. Ferrando, Stefan Ferreira, R. A. Burger, Reinhard Schlickeiser, A. Raviart, H. Kunow, Reinhold Müller-Mellin, G. Wibberenz, Arik Posner, C. Paizis, M. S. Potgieter, Bernd Heber
Publikováno v:
The Astrophysical Journal. 579:888-894
The Ulysses trajectory provides a unique opportunity to study the propagation of MeV electrons in a wide range of heliographic latitudes and during varying conditions in the inner heliosphere. From the Ulysses launch up to the beginning of 1998, the
Autor:
J. R. Jokipii, R. J. Forsyth, G. Wibberenz, H. Kunow, Devrie S. Intriligator, Timothy S. Horbury, James Intriligator, J. T. Gosling
Publikováno v:
Journal of Geophysical Research: Space Physics. 106:10625-10634
Pioneer and Ulysses observations of energetic particles and solar wind plasma and magnetic fields are analyzed to study particle transport in corotating interaction regions (CIRs) and near stream interfaces (SIs). Energetic particle diffusion with a
Autor:
Volker Bothmer, M. S. Potgieter, H. Kunow, A. Raviart, Reinhold Müller-Mellin, Arik Posner, Philippe Ferrando, Holger Sierks, B. Heber, C. Paizis, G. Wibberenz
Publikováno v:
Geophysical Research Letters. 26:2133-2136
According to standard drift dominated modulation models the intensity variations of galactic cosmic ray protons and electrons respond differently to the latitudinal extension of the heliospheric current sheet α. In an A>0 solar cycle intensities of
Publikováno v:
Journal of Geophysical Research: Space Physics. 104:12549-12561
Evidence is presented for a 22-year cycle in the amplitude of recurrent, near-Earth, near-Ecliptic, galactic cosmic ray modulations during the solar minimum periods in the mid-1950s to mid-1990s. These modulations are ∼50% larger during A > 0 epoch
Publikováno v:
Geophysical Research Letters. 26:565-568
We show that the variations of the interplanetary magnetic field strength (B) over a 22-year period are tracked by the inverted profile of the cosmic ray density measured by neutron monitors. We suggest that global changes in the Sun's magnetic field