This Week on Galileo
January 22-28, 2001
DOY 2001/22-28
Galileo nears the end of a 14-week-long collaboration with the Cassini spacecraft
This week, Galileo nears the end of a 14-week-long collaboration with
the Cassini spacecraft to study the influence of the solar wind on
the Jovian magnetosphere. Galileo is in week 13 of its contribution
to this study, which was initiated in late October, 2000. Galileo
performs one engineering activity this week. On Wednesday, the
spacecraft executes standard maintenance on its onboard tape
recorder. Galileo's tape recorder is a
reel-to-reel mechanical type and these regular maintenance activities
are performed to keep the tape recorder in good operating shape.
Galileo's contribution to the study of the solar wind's influence on
the Jovian magnetosphere comes in the form of a low-resolution survey
being performed by the Fields and Particles instruments. This suite
of six instruments is comprised of the Dust Detector, Energetic
Particle Detector, Heavy Ion Counter, Magnetometer, Plasma Detector,
and Plasma Wave instrument.
During the past 13 weeks, Galileo has flown from the solar wind, into
the Jovian magnetosphere, and now back out into the solar wind.
Cassini, on the other hand, was generally expected to remain outside
the magnetosphere until after its flyby of Jupiter, when it would fly
along the boundary region of the magnetosphere and solar wind as it
left the vicinity of Jupiter.
Measurements now indicate that Cassini entered the bow shock region
on December 27, three days prior to its closest approach to Jupiter.
Cassini has since crossed into and out of the magnetosphere multiple
times as the solar wind "blew" stronger and then weaker. The solar
wind is a stream of charged particles and gas that emanate from the
Sun. Because the solar wind waxes and wanes with changes in the Sun,
it exerts varying amounts of pressure on the Jovian magnetosphere.
The magnetosphere responds by shrinking when the solar wind pressure
is high, and ballooning outward when it is low.
Currently, Galileo is in the solar wind, while Cassini is moving
through the magnetotail, or vast "downstream" portion to the
magnetosphere that extends as far outward as Saturn. Thus, Galileo
will measure variations in the solar wind while Cassini observes the
response of the downstream parts of Jupiter's magnetosphere.
This series of joint observations is expected to provide new insights
into how the solar wind affects the magnetospheres of Jupiter and
other planets, including Earth.
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