High energy cosmic-ray nuclei results on Ulysses: 2. Effects of a recurrent high-speed stream from the southern polar coronal hole
Kunow, H. ; Dröge, W. ; Heber, B. ; Müller-Mellin, R. ; Röhrs, K. ; Sierks, H. ; Wibberenz, G. ; Ducros, R. ; Ferrando, P. ; Rastoin, C. ; Raviart, A. ; Paizis, C.
Springer
Published 1995
Springer
Published 1995
ISSN: |
1572-9672
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Keywords: |
Heliosphere ; solar modulation ; Ulysses ; Corotating Interaction Region
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Source: |
Springer Online Journal Archives 1860-2000
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Topics: |
Physics
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Notes: |
Abstract Since June 1992 the Kiel Electron Telescope on board ULYSSES measures 26-day variations of the order of 6% in the fluxes of high energy H and He. In May 1993 ULYSSES entered into the unipolar region of the southern polar coronal hole, but continued to observe similar effects: increases in the MeV proton channels due to acceleration near the shocks of the corotating interaction region and decreases in the intensity of galactic nuclei associated with the same region. Amplitude variations are presented for different magnetic rigidities and the effects are discussed in view of corotating shock development in a 3-dimensional heliospheric structure.
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Type of Medium: |
Electronic Resource
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URL: |
_version_ | 1798296496519512064 |
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autor | Kunow, H. Dröge, W. Heber, B. Müller-Mellin, R. Röhrs, K. Sierks, H. Wibberenz, G. Ducros, R. Ferrando, P. Rastoin, C. Raviart, A. Paizis, C. |
autorsonst | Kunow, H. Dröge, W. Heber, B. Müller-Mellin, R. Röhrs, K. Sierks, H. Wibberenz, G. Ducros, R. Ferrando, P. Rastoin, C. Raviart, A. Paizis, C. |
book_url | http://dx.doi.org/10.1007/BF00768811 |
datenlieferant | nat_lic_papers |
hauptsatz | hsatz_simple |
identnr | NLM19593895X |
issn | 1572-9672 |
journal_name | Space science reviews |
materialart | 1 |
notes | Abstract Since June 1992 the Kiel Electron Telescope on board ULYSSES measures 26-day variations of the order of 6% in the fluxes of high energy H and He. In May 1993 ULYSSES entered into the unipolar region of the southern polar coronal hole, but continued to observe similar effects: increases in the MeV proton channels due to acceleration near the shocks of the corotating interaction region and decreases in the intensity of galactic nuclei associated with the same region. Amplitude variations are presented for different magnetic rigidities and the effects are discussed in view of corotating shock development in a 3-dimensional heliospheric structure. |
package_name | Springer |
publikationsjahr_anzeige | 1995 |
publikationsjahr_facette | 1995 |
publikationsjahr_intervall | 8004:1995-1999 |
publikationsjahr_sort | 1995 |
publisher | Springer |
reference | 72 (1995), S. 397-402 |
schlagwort | Heliosphere solar modulation Ulysses Corotating Interaction Region |
search_space | articles |
shingle_author_1 | Kunow, H. Dröge, W. Heber, B. Müller-Mellin, R. Röhrs, K. Sierks, H. Wibberenz, G. Ducros, R. Ferrando, P. Rastoin, C. Raviart, A. Paizis, C. |
shingle_author_2 | Kunow, H. Dröge, W. Heber, B. Müller-Mellin, R. Röhrs, K. Sierks, H. Wibberenz, G. Ducros, R. Ferrando, P. Rastoin, C. Raviart, A. Paizis, C. |
shingle_author_3 | Kunow, H. Dröge, W. Heber, B. Müller-Mellin, R. Röhrs, K. Sierks, H. Wibberenz, G. Ducros, R. Ferrando, P. Rastoin, C. Raviart, A. Paizis, C. |
shingle_author_4 | Kunow, H. Dröge, W. Heber, B. Müller-Mellin, R. Röhrs, K. Sierks, H. Wibberenz, G. Ducros, R. Ferrando, P. Rastoin, C. Raviart, A. Paizis, C. |
shingle_catch_all_1 | Kunow, H. Dröge, W. Heber, B. Müller-Mellin, R. Röhrs, K. Sierks, H. Wibberenz, G. Ducros, R. Ferrando, P. Rastoin, C. Raviart, A. Paizis, C. High energy cosmic-ray nuclei results on Ulysses: 2. Effects of a recurrent high-speed stream from the southern polar coronal hole Heliosphere solar modulation Ulysses Corotating Interaction Region Heliosphere solar modulation Ulysses Corotating Interaction Region Abstract Since June 1992 the Kiel Electron Telescope on board ULYSSES measures 26-day variations of the order of 6% in the fluxes of high energy H and He. In May 1993 ULYSSES entered into the unipolar region of the southern polar coronal hole, but continued to observe similar effects: increases in the MeV proton channels due to acceleration near the shocks of the corotating interaction region and decreases in the intensity of galactic nuclei associated with the same region. Amplitude variations are presented for different magnetic rigidities and the effects are discussed in view of corotating shock development in a 3-dimensional heliospheric structure. 1572-9672 15729672 Springer |
shingle_catch_all_2 | Kunow, H. Dröge, W. Heber, B. Müller-Mellin, R. Röhrs, K. Sierks, H. Wibberenz, G. Ducros, R. Ferrando, P. Rastoin, C. Raviart, A. Paizis, C. High energy cosmic-ray nuclei results on Ulysses: 2. Effects of a recurrent high-speed stream from the southern polar coronal hole Heliosphere solar modulation Ulysses Corotating Interaction Region Heliosphere solar modulation Ulysses Corotating Interaction Region Abstract Since June 1992 the Kiel Electron Telescope on board ULYSSES measures 26-day variations of the order of 6% in the fluxes of high energy H and He. In May 1993 ULYSSES entered into the unipolar region of the southern polar coronal hole, but continued to observe similar effects: increases in the MeV proton channels due to acceleration near the shocks of the corotating interaction region and decreases in the intensity of galactic nuclei associated with the same region. Amplitude variations are presented for different magnetic rigidities and the effects are discussed in view of corotating shock development in a 3-dimensional heliospheric structure. 1572-9672 15729672 Springer |
shingle_catch_all_3 | Kunow, H. Dröge, W. Heber, B. Müller-Mellin, R. Röhrs, K. Sierks, H. Wibberenz, G. Ducros, R. Ferrando, P. Rastoin, C. Raviart, A. Paizis, C. High energy cosmic-ray nuclei results on Ulysses: 2. Effects of a recurrent high-speed stream from the southern polar coronal hole Heliosphere solar modulation Ulysses Corotating Interaction Region Heliosphere solar modulation Ulysses Corotating Interaction Region Abstract Since June 1992 the Kiel Electron Telescope on board ULYSSES measures 26-day variations of the order of 6% in the fluxes of high energy H and He. In May 1993 ULYSSES entered into the unipolar region of the southern polar coronal hole, but continued to observe similar effects: increases in the MeV proton channels due to acceleration near the shocks of the corotating interaction region and decreases in the intensity of galactic nuclei associated with the same region. Amplitude variations are presented for different magnetic rigidities and the effects are discussed in view of corotating shock development in a 3-dimensional heliospheric structure. 1572-9672 15729672 Springer |
shingle_catch_all_4 | Kunow, H. Dröge, W. Heber, B. Müller-Mellin, R. Röhrs, K. Sierks, H. Wibberenz, G. Ducros, R. Ferrando, P. Rastoin, C. Raviart, A. Paizis, C. High energy cosmic-ray nuclei results on Ulysses: 2. Effects of a recurrent high-speed stream from the southern polar coronal hole Heliosphere solar modulation Ulysses Corotating Interaction Region Heliosphere solar modulation Ulysses Corotating Interaction Region Abstract Since June 1992 the Kiel Electron Telescope on board ULYSSES measures 26-day variations of the order of 6% in the fluxes of high energy H and He. In May 1993 ULYSSES entered into the unipolar region of the southern polar coronal hole, but continued to observe similar effects: increases in the MeV proton channels due to acceleration near the shocks of the corotating interaction region and decreases in the intensity of galactic nuclei associated with the same region. Amplitude variations are presented for different magnetic rigidities and the effects are discussed in view of corotating shock development in a 3-dimensional heliospheric structure. 1572-9672 15729672 Springer |
shingle_title_1 | High energy cosmic-ray nuclei results on Ulysses: 2. Effects of a recurrent high-speed stream from the southern polar coronal hole |
shingle_title_2 | High energy cosmic-ray nuclei results on Ulysses: 2. Effects of a recurrent high-speed stream from the southern polar coronal hole |
shingle_title_3 | High energy cosmic-ray nuclei results on Ulysses: 2. Effects of a recurrent high-speed stream from the southern polar coronal hole |
shingle_title_4 | High energy cosmic-ray nuclei results on Ulysses: 2. Effects of a recurrent high-speed stream from the southern polar coronal hole |
sigel_instance_filter | dkfz geomar wilbert ipn albert fhp |
source_archive | Springer Online Journal Archives 1860-2000 |
timestamp | 2024-05-06T09:53:01.360Z |
titel | High energy cosmic-ray nuclei results on Ulysses: 2. Effects of a recurrent high-speed stream from the southern polar coronal hole |
titel_suche | High energy cosmic-ray nuclei results on Ulysses: 2. Effects of a recurrent high-speed stream from the southern polar coronal hole |
topic | U |
uid | nat_lic_papers_NLM19593895X |