INVESTIGADORES
BERTUCCI Cesar
artículos
Título:
Structure of Titan's mid-range magnetic tail: Cassini magnetometer observations during the T9 flyby
Autor/es:
BERTUCCI, C., NEUBAUER, F. M., SZEGO, K., WAHLUND, J.-E., COATES, A. J., DOUGHERTY, M. K., YOUNG, D. T., KURTH, W. S.
Revista:
GEOPHYSICAL RESEARCH LETTERS
Editorial:
American Geophysical Union
Referencias:
Lugar: Washington; Año: 2007 vol. 34 p. 1 - 4
ISSN:
0094-8276
Resumen:
We analyze the magnetic structure of Titans mid-range magnetic tail (56 Titan radii downstream from the moon) during Cassinis T9 flyby. Cassini magnetometer (MAG) measurements reveal a well-defined, induced magnetic tail consisting of two lobes and a distinct central current sheet. MAG observations also indicate that Saturns backgroundmagnetic field is close to the moons orbital plane and that the magnetospheric flow has a significant component in the Saturn-Titan direction. The analysis of MAG data in a coordinate system based on the orientation of the background magnetic field and an estimation of the incoming flow direction suggests that Titans magnetic tail is extremely asymmetric. An important source of these asymmetries is the connection of the inbound tail lobe and the outbound tail lobe to the dayside and nightside hemispheres of Titan, respectively. Another source could be the perturbations generated by changes in the upstream conditions.