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Автор Acuña, M. H.
Автор Connerney, J. E. P.
Автор Ness, N. F.
Дата выпуска 1993
dc.description A simplified description of the Neptunian magnetic field derived from the Goddard Space Flight Center/Bartol Research Institute I8E1 model which includes internal terms up to and including the octupole (but no external terms) has been used to compute numerically L shell values along the Voyager 2 encounter trajectory and those associated with the N1 through N6 moons and N1R through N6R rings. The complex magnetic field geometry and the rapid rotation of the planet combine to produce an expectation of numerous times when absorption signatures should be observed as a result of the interaction between the trapped particle population and the Neptunian moons and rings. Thus a complete understanding of the observed charged particle fluxes and their variation along the Voyager 2 trajectory must take into account these geometrically anticipated interactions. Similar to Uranus, the large tilt between the dipole term and the rotation axis causes the moons and rings to sweep a very large range of L shells. Furthermore, their orbital motion introduces additional periodicities, causing the maxima and minima in L space to vary systematically with time. The unambiguous association of predicted and observed absorption signatures and times with a particular ring or moon is made very difficult by the superposition of many individual effects. The extremely rapid excursion in L space by Voyager 2 near closest approach, a region most significant for magnetic field models, apparently does not facilitate the unique associations previously used at other planets to provide an independent assessment of the global accuracy of the mathematical models of the field which are inherently nonunique.
Формат application.pdf
Копирайт Copyright 1993 by the American Geophysical Union.
Тема MAGNETOSPHERIC PHYSICS
Тема Energetic particles: trapped
Тема Magnetosphere interactions with satellites and rings
Тема Planetary magnetospheres
Тема PLANETARY SCIENCES: SOLID SURFACE PLANETS
Тема Planetology: Solid Surface Planets and Satellites: Magnetic fields
Тема Magnetospheres
Тема PLANETARY SCIENCES: FLUID PLANETS
Тема Magnetospheres
Тема PLANETARY SCIENCES: COMETS AND SMALL BODIES
Тема Magnetospheres
Название Neptune's magnetic field: Calculation of field geometric invariants derived from the I8E1 GSFC/BRI model
Тип article
DOI 10.1029/92JA02981
Electronic ISSN 2156-2202
Print ISSN 0148-0227
Журнал Journal of Geophysical Research: Space Physics
Том 98
Первая страница 11275
Последняя страница 11284
Выпуск A7
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