Zobrazeno 1 - 10
of 173
pro vyhledávání: '"V. Bothmer"'
Publikováno v:
Annales Geophysicae, Vol 28, Pp 687-696 (2010)
Collimated ejections of plasma called "coronal hole jets" are commonly observed in polar coronal holes. However, such coronal jets are not only a specific features of polar coronal holes but they can also be found in coronal holes appearing at low
Externí odkaz:
https://doaj.org/article/918ffc539fbc412d88f5c219ad1179e0
Publikováno v:
Annales Geophysicae, Vol 23, Pp 625-641 (2005)
The magnetic structure and geomagnetic response of 73 magnetic clouds (MC) observed by the WIND and ACE satellites in solar cycle 23 are examined. The results have been compared with the surveys from the previous solar cycles. The preselected cand
Externí odkaz:
https://doaj.org/article/7e37bd93f01e463cb2c334e2669dc262
Autor:
V. Bothmer, R. Schwenn
Publikováno v:
Annales Geophysicae, Vol 16, Pp 1-24 (1998)
Plasma and magnetic field data from the Helios 1/2 spacecraft have been used to investigate the structure of magnetic clouds (MCs) in the inner heliosphere. 46 MCs were identified in the Helios data for the period 1974–1981 between 0.3 and 1 AU.
Externí odkaz:
https://doaj.org/article/1724d95900164198889387c3306b8ae5
Akademický článek
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Autor:
M. Temmer, V. Bothmer
Aims: We statistically investigate the plasma and magnetic field characteristics of the upstream regions of interplanetary coronal mass ejections (ICMEs) and their evolution as function of distance to the Sun in the inner heliosphere. We use a sample
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fe4cfd4b766c95027aaad9b3194ed65b
Publikováno v:
In Advances in Mathematics 2010 224(1):246-259
Autor:
D. Barnes, J. A. Davies, R. A. Harrison, J. P. Byrne, C. H. Perry, V. Bothmer, J. P. Eastwood, P. T. Gallagher, E. K. J. Kilpua, C. Möstl, L. Rodriguez, A. P. Rouillard, D. Odstrčil
Publikováno v:
SOLAR PHYSICS
SOLAR PHYSICS, 2019, 294, ⟨10.1007/s11207-019-1444-4⟩
SOLAR PHYSICS, 2019, 294, ⟨10.1007/s11207-019-1444-4⟩
International audience; Recent observations with the Heliospheric Imagers (HIs) onboard the twin NASA Solar Terrestrial Relations Observatory (STEREO) spacecraft have provided unprecedented observations of a large number of coronal mass ejections (CM
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e691804790b2083ee014d7edcac55111
http://hdl.handle.net/10138/302529
http://hdl.handle.net/10138/302529
Autor:
V. Bothmer, N. Mrotzek
Publikováno v:
Earth-affecting Solar Transients ISBN: 9789402415698
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::c12f4e868133f1135a7c9ec838955fcc
https://doi.org/10.1007/978-94-024-1570-4_20
https://doi.org/10.1007/978-94-024-1570-4_20
Autor:
v. Bothmer, Hans-Christian1 bothmer@math.uni-hannover.de
Publikováno v:
Quantitative Finance. Oct2003, Vol. 3 Issue 5, p370-375. 6p. 7 Graphs.
Autor:
L. Volpes, V. Bothmer
Publikováno v:
AIP Conference Proceedings.
Coronal mass ejections (CMEs) are large scale eruptions of magnetized plasma propagating from the Sun into interplanetary space with speeds varying from a few tens to more than 2500 km s−1. They cause large-scale turbulence in the heliosphere and a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::eeff8144d21a1456a0a10e8d98637f4e
https://doi.org/10.1063/1.4942572
https://doi.org/10.1063/1.4942572