BOSTON
UNIVERSITY |
Planetary Atmospheres and Space Science
Group
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DEPARTMENT
OF
ASTRONOMY |
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Since we are looking for correlations to determine the physics of cause
and effect in planetary aurora, an important element of the auroral
campaign is to have an open workshop to compare data sets from
different missions and instruments. This campaign includes measurements
from HST, Cassini, New Horizons, Earth-based solar wind instruments,
ground-based IR telescopes, and ground-based radio telescopes.
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We are a research group at Boston University
studying the Aurorae on
Jupiter and Saturn. The Hubble Space Telescope (HST) allows us to take
beautiful images of the Aurorae...
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Auroras are light emissions phenomena due to energetic particles
precipitating into the upper atmospheres.
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The project will consist of a concentrated series of HST observations
coordinated with planetary spacecraft and other earth-based
observations in 2007. The temporal resolution of the measurements
combined with the correlation of in situ observations will give us more
insight about the phenomena at stake.
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The HST observations will take place simultaneously with other in situ
observations by Cassini and New Horizon. We expect to also compare with
observations from ground-based telescopes at IR and radio wavelength.
These combined observations
will provide more information abour the correlation between light
emissions and solar wind parameters.
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We will have 128 orbits to observe Jupiter and Saturn, which means that
thousands of images will be collected in different filters. The data
are
currently being processed and organized.
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