Zobrazeno 1 - 10
of 1 882
pro vyhledávání: '"Mercury's magnetic field"'
Autor:
Toepfer, S., Narita, Y., Glassmeier, K. -H., Heyner, D., Kolhey, P., Motschmann, U., Langlais, B., Institut für Theoretische Physik, Technische Universität Braunschweig, Braunschweig, Germany, Institut für Geophysik und extraterrestrische Physik, Technische Universität Braunschweig, Braunschweig, Germany, Deutsches Zentrum für Luft- und Raumfahrt, Institut für Planetenforschung, Berlin, Germany, Laboratoire de Planétologie et Géodynamique, UMR 6112, CNRS, Université de Nantes, Université d’Angers, Nantes, France
Publikováno v:
Earth Planets and Space
Earth Planets and Space, Springer/Terra Scientific Publishing Company, 2021, 73 (1), ⟨10.1186/s40623-021-01386-4⟩
Earth, Planets and Space, Vol 73, Iss 1, Pp 1-18 (2021)
Earth, planets and space : EPS, volume 73, Article number: 65--1343-8832
Earth Planets and Space, Springer/Terra Scientific Publishing Company, 2021, 73 (1), ⟨10.1186/s40623-021-01386-4⟩
Earth, Planets and Space, Vol 73, Iss 1, Pp 1-18 (2021)
Earth, planets and space : EPS, volume 73, Article number: 65--1343-8832
The parameterization of the magnetospheric field contribution, generated by currents flowing in the magnetosphere is of major importance for the analysis of Mercury’s internal magnetic field. Using a combination of the Gauss and the Mie representat
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::57d05e92ae80593287197663ff8ece56
https://hal.archives-ouvertes.fr/hal-03284462/document
https://hal.archives-ouvertes.fr/hal-03284462/document
Autor:
Daniel Heyner, Patrick Kolhey, Karl-Heinz Glassmeier, Uwe Motschmann, Yasuhito Narita, Simon Toepfer, W. Exner
Publikováno v:
Earth, planets and space : EPS, volume 73, Article number: 204 (2021). https://doi.org/10.1186/s40623-021-01536-8--http://www.bibliothek.uni-regensburg.de/ezeit/?2087663--http://link.springer.com/journal/40623--http://www.terrapub.co.jp/journals/EPS/index.html--1880-5981
Earth, Planets and Space, Vol 73, Iss 1, Pp 1-14 (2021)
Earth, Planets and Space, Vol 73, Iss 1, Pp 1-14 (2021)
Poloidal–toroidal magnetic field decomposition is a useful application of the Mie representation and the decomposition method enables us to determine the current density observationally and unambiguously in the local region of magnetic field measur
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::14d2370acf6c49ceeff8a661f95da39e
http://publikationsserver.tu-braunschweig.de/get/69918
http://publikationsserver.tu-braunschweig.de/get/69918
Autor:
John V. Shebalin
Publikováno v:
Physics of the Earth and Planetary Interiors. 285:59-75
Ideal magnetohydrodynamic (MHD) turbulence contains an intrinsic statistical mechanism called ‘broken ergodicity’ for producing an energetic, large-scale, quasi-stationary coherent structure. Since MHD turbulence occurs in the Earth’s liquid ou
Publikováno v:
Planetary and Space Science. 210:105379
Based on the Magnetometer observations of the MErcury Surface, Space ENvironment, GEochemistry, and Ranging (MESSENGER) spacecraft in orbit around Mercury, we construct a global magnetic field model of Mercury's magnetosphere using radial basis funct
Publikováno v:
Journal of Geophysical Research: Space Physics. 122:9751-9762
The effects of decreasing the intrinsic magnetic field on the upper atmospheric dynamics at low-to middle- latitudes are investigated using the Ground-to-topside model of Atmosphere and Ionosphere for Aeronomy (GAIA). GAIA incorporates a meteorologic
Publikováno v:
Brazilian Journal of Physics. 47:447-459
Magnetic field reconnection has shown to be the dominant process in the solar wind-Earth’s magnetosphere interaction. It enables mass, momentum, and energy exchange between different plasma regimes, and it is regarded as an efficient plasma acceler
Publikováno v:
Geophysical Research Letters. 44:5936-5942
The Juno spacecraft was launched on August 5, 2011 and spent nearly 5 years traveling through the inner heliosphere on its way to Jupiter. The Magnetic Field Investigation (MAG) was powered on shortly after launch and obtained vector measurements of
Publikováno v:
Journal of Geophysical Research: Planets. 122:1243-1257
The martian magnetic field is unique among those of the terrestrial planets. It is the net result of the interaction of the solar wind and the interplanetary magnetic field (IMF) with crustal remnant magnetization and a planetary ionosphere. Internal
Autor:
A.A. Vasylenko
Publikováno v:
Kosmìčna nauka ì tehnologìâ. 23:73-80
Autor:
Xiao-Jia Zhang, John E. P. Connerney, Chris Paranicas, Qianli Ma, Scott Bolton, Barry Mauk, Richard M. Thorne, Dennis Haggerty, Wen Li
Publikováno v:
Geophysical Research Letters. 44:4472-4480
In inner planetary magnetospheres, pitch angle distributions of charged particles are shaped by the global magnetic field topology when they bounce fast along magnetic field lines. Therefore, one can estimate the magnetic field intensity at the top o