[Baps] BU seminar Thursday 24th - Marissa Vogt (Univ of Leicester) Jupiter’s Dynamic Magnetosphere
Paul Withers
withers at bu.edu
Fri Oct 18 17:15:18 EDT 2013
Also, advance warning of Paul Mahaffy and MSL mass spectrometer results
from the surface of Mars on Thursday 31st.
http://www.bu.edu/csp/edoutreach/seminar/
-------- Original Message --------
Subject: [Announce] THURSDAY: Marissa Vogt (Univ of Leicester) Space
Physics Seminar
Date: Fri, 18 Oct 2013 20:56:56 +0000
From: Savoie, Alyson L <asavoie at bu.edu>
To: announce at skynet.bu.edu <announce at skynet.bu.edu>,
csp_seminar at skynet.bu.edu <csp_seminar at skynet.bu.edu>, iar at skynet.bu.edu
<iar at skynet.bu.edu>
Space physics seminar
Marissa Vogt
University of Leicester
*Jupiter’s Dynamic Magnetosphere*
*Thursday, October 24, 2013*
*725 Commonwealth Ave.*
*Refreshments at 3:30pm in CAS 500*
*Talk begins at 4:00pm in CAS 502*
Abstract:
The gas giant Jupiter possesses a strong internal magnetic field that
produces the largest magnetosphere in our solar system and leads to
spectacular auroral emissions. Eight spacecraft have now visited the
Jovian system, yielding a wealth of information about Jupiter’s
rotation-dominated magnetosphere and its internal plasma source, the
volcanically active moon Io. The Galileo spacecraft, which was in orbit
around Jupiter from 1995 to 2003, has provided the most extensive
spatial coverage of the magnetosphere and the opportunity to study
temporal changes on long time scales. In this talk I discuss the dynamic
nature of Jupiter’s magnetosphere and aurora, using both in situ
spacecraft measurements and Earth-based telescope observations to
illustrate changes on time scales from days to several years. I will
focus on recent work in which we characterize long-term changes in
Jupiter’s magnetic field configuration due to current sheet variability
and will discuss the resulting implications for the aurora. Finally, I
will consider the relative roles of the solar wind and internal factors,
such as rotational stresses or changes in Io’s plasma production, in
driving the many temporal variations in Jupiter’s magnetosphere.
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