Title of article :
Dynamics of Saturnʹs magnetodisk near Titanʹs orbit: Comparison of Cassini magnetometer observations from real and virtual Titan flybys
Author/Authors :
Simon، نويسنده , , Sven and Wennmacher، نويسنده , , Alexandre and Neubauer، نويسنده , , Fritz M. and Bertucci، نويسنده , , Cesar L. and Kriegel، نويسنده , , Hendrik and Russell، نويسنده , , Christopher T. and Dougherty، نويسنده , , Michele K.، نويسنده ,
Issue Information :
روزنامه با شماره پیاپی سال 2010
Abstract :
We analyze the variability of the ambient magnetospheric field along Titanʹs orbit at 20.3 Saturn radii. However, while our preceding study (Simon et al., 2010) focused on Cassini magnetometer observations from the 62 Titan flybys (TA–T62) between October 2004 and October 2009, the present work discusses magnetic field data that were collected near Titanʹs orbit when the moon was far away. In analogy to the observations during TA–T62, the magnetospheric fields detected during these 79 “virtual” Titan flybys are strongly affected by the presence of Saturnʹs bowl-shaped and highly dynamic magnetodisk current sheet. We therefore provide a systematic classification of the magnetic field observations as magnetodisk current sheet or lobe-type scenarios. Among the 141 (62 real+79 virtual) crossings of Titanʹs orbit between July 2004 and December 2009, only 17 encounters (9 real+8 virtual) took place within quiet, magnetodisk lobe-type fields. During another 50 encounters (21 real+29 virtual), rapid transitions between current sheet and lobe fields were observed around the moonʹs orbital plane. Most of the encounters (54=22 real+32 virtual) occurred when Titanʹs orbit was embedded in highly distorted current sheet fields, thereby invalidating the frequently applied idealized picture of Titan interacting with a homogeneous and stationary magnetospheric background field. The locations of real and virtual Titan flybys are correlated to each other. Each of the 62 real Titan flybys possesses at least one virtual counterpart that occurred shortly before or after the real encounter and at nearly the same orbital position. A systematic comparison between Cassini magnetometer observations from the real Titan flybys and their virtual companions suggests that there is no clear evidence of Titan exerting a significant level of control on the vertical oscillatory motion of the magnetodisk near its orbit.
Keywords :
Plasma interaction with unmagnetized bodies , Titan , Magnetodisk current sheet and lobes , Cassini flybys , Saturnיs magnetosphere
Journal title :
PLANETARY AND SPACE SCIENCE
Journal title :
PLANETARY AND SPACE SCIENCE