Zobrazeno 1 - 10
of 27
pro vyhledávání: '"Paul L. Rothwell"'
Autor:
Paul L. Rothwell
Publikováno v:
Physics of Plasmas. 11:1740-1743
Vasyliunas [Phys. Plasmas 11, 1738 (2004)] claims that the co-rotation electric field must be derived from the generalized Ohm’s law to be physically correct. However, laboratory results show that the rotation of a magnetic source produces electric
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::92712178ad6e2bf42b7ec870e6d377f3
https://doi.org/10.1063/1.1667493
https://doi.org/10.1063/1.1667493
Autor:
Paul L. Rothwell
Publikováno v:
Physics of Plasmas. 10:2971-2977
Magnetohydrodynamic theory has been widely and successfully applied to explain many aspects of magnetospheric behavior. In particular, it has been used to predict where and when field-aligned auroral currents of electrons and ions will flow between t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ee65eb24d9c029837e12474f916abdbd
https://doi.org/10.1063/1.1582473
https://doi.org/10.1063/1.1582473
Publikováno v:
Journal of Geophysical Research: Space Physics. 105:10739-10749
We propose a model to explain how ion dynamics create an Alfven wave generator in the equatorial region that can be applied to the stable arc problem. For example, in the earthward drifting magnetotail plasma, phase bunching of O+ ions (and to a much
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::981ade8d230604a774f707fc4578e29b
https://doi.org/10.1029/1999ja900360
https://doi.org/10.1029/1999ja900360
Publikováno v:
IEEE Transactions on Plasma Science. 28:1912-1919
In space weather prediction, the transport of solar wind energy through the magnetosphere is a major aspect. For the transport of energy from the magnetosphere to the ionosphere, magnetic field-aligned (Birkeland) currents are a very important agent.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::1c49411e0e65a7167e6a9d3135e1ef7a
https://doi.org/10.1109/27.902219
https://doi.org/10.1109/27.902219
Publikováno v:
Journal of Geophysical Research: Space Physics. 103:6913-6916
It is shown, by using a circuit model for the magnetospheric current system, that the substorm breakup can be triggered either by some instability anywhere in the circuit or by a decrease in the generator emf, i.e., a northward turning of the interpl
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::5abd1a14fce3db4b55a7c5f0b9c9b152
https://doi.org/10.1029/97ja03684
https://doi.org/10.1029/97ja03684
Publikováno v:
Journal of Geophysical Research: Space Physics. 96:13967-13975
We have developed a model describing the structure of a prebreakup arc based on an ionospheric Cowling channel and its extension into the magnetosphere. A coupled two-circuit representation of the substorm current wedge is used which is locally super
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::dd48c7777e0d11e57988a0dbcb6f657d
https://doi.org/10.1029/91ja01268
https://doi.org/10.1029/91ja01268
Autor:
Paul L. Rothwell, J. Jasperse
Publikováno v:
Journal of Geophysical Research. 111
[1] A global ionospheric electrostatic potential model, which we refer to as Nopper-Carovillano (N-C), can be linked with a magnetospheric potential model. The latter model, which we refer to as Hill-Siscoe-Ober (H-S-O), computes a transpolar potenti
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::0cd279d8be14acfb26272e04a270500e
https://doi.org/10.1029/2004ja010992
https://doi.org/10.1029/2004ja010992
Publikováno v:
39th Aerospace Sciences Meeting and Exhibit.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::8009086829d7b59720ccf5221b314f38
https://doi.org/10.2514/6.2001-241
https://doi.org/10.2514/6.2001-241
Publikováno v:
Journal of Geophysical Research: Space Physics. 101:27461-27461
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::33befa64ca6206ccfafb72b4e4033a11
https://doi.org/10.1029/96ja01607
https://doi.org/10.1029/96ja01607
Publikováno v:
Journal of Geophysical Research. 100:14875
For an MHD description of a plasma a distinct separation between the macroscopic and microscopic spatial and temporal scales is assumed. In this paper we solve the particle dynamics with finite first and second spatial derivatives in the electric fie
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a72ab29163b20c3d4479e056df2c8267
https://doi.org/10.1029/95ja00627
https://doi.org/10.1029/95ja00627