Winds and cloud structure on Jupiter's 2009 South Equatorial Belt Fade

Details Winds and cloud structure on Jupiter's 2009 South Equatorial Belt Fade Winds and cloud structure on Jupiter's 2009 South Equatorial Belt Fade

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf..889b&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.889

Computer Science

Scientific paper

Jupiter's South Equatorial Belt (SEB) is known to suffer global albedo changes with a not well defined period [1]. The transition from a "belt-like" aspect (low albedo at visible wavelengths) to a "zone-like" (bright albedo) is known as a "Fade". During 2009 the SEB suffered a fading process and became completely transformed to a zone by the first observations in 2010. In this work, we study the winds and the vertical cloud structure during the fade process at visual wavelengths from Hubble Space Telescope (HST) and International Outer Planet Watch ((IOPW) images.

Affiliated with

Also associated with

No associations

Rating

Winds and cloud structure on Jupiter's 2009 South Equatorial Belt Fade does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Winds and cloud structure on Jupiter's 2009 South Equatorial Belt Fade, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Winds and cloud structure on Jupiter's 2009 South Equatorial Belt Fade will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1481251