INVESTIGADORES
BERTUCCI Cesar
artículos
Título:
MGS MAG/ER Observations at the Magnetic Pileup Boundary of Mars: Draping Enhancement and Low Frequency Waves
Autor/es:
BERTUCCI, C., MAZELLE, C., CRIDER, D.H., MITCHELL, D.L., SAUER, K., ACUÑA, M.H., CONNERNEY, J.E.P., LIN, R.P., NESS, N.F., WINTERHALTER, D.
Revista:
ADVANCES IN SPACE RESEARCH
Editorial:
Elsevier
Referencias:
Lugar: Amsterdam; Año: 2004 vol. 33 p. 1938 - 1944
ISSN:
0273-1177
Resumen:
The magnetic pileup boundary (MPB) is a sharp, thin, and permanent
plasma boundary reported, up to now, at comets and Mars, and located
between the bow shock and the ionospheric boundary. The MPB separates
the magnetosheath, a region with high wave activity, from the magnetic
pileup region, where the interplanetary magnetic field piles up
regularly in front of the planetary obstacle. We use magnetic field and
electron plasma measurements from the MAG/ER experiment onboard the Mars
Global Surveyor spacecraft to study two characteristic features of the
MPB. The first feature is the sudden enhancement of the magnetic field
line draping at the MPB. This new signature reveals that the MPB marks
the entry into the veritable induced magnetosphere, where the magnetic
field topology is more regular, in opposition to what is observed in the
magnetosheath. Secondly, we study the properties and the occurrence of
compressive, linearly polarized, low frequency waves, frequently
observed on both sides of the boundary. An analysis of the correlation
between the magnetic and the electron data reveals that on the upstream
side the waves are mirror mode waves, while on the downstream side they
are large amplitude, quasi-monochromatic fast magnetosonic waves. The
presence of these features at other atmospheric, unmagnetized bodies can
be used as indicators of the existence of a MPB.