Computer Science
Scientific paper
Oct 2011
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf...56t&link_type=abstract
EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.56
Computer Science
Scientific paper
The disappearance of dark Southern Equatorial Belt (SEB) in 2010 is not exclusive but very rare event on Jupiter. Preceding cases of the SEB disappearance or very low contrast took place in 1989 and yet no less 8 times during the last century : in 1952, 1949, 1943, 1940-1941, 1936-1937, 1927-1928, 1926 according [1,2]. In 1904 the NEB disappeared, if the orientation of two pictures for that time in [1] is right. It is evident that these changes are connected with more or less intensive vertical atmospheric circulation at low latitudes. Now we have an opportunity to search probable changes in the cloud structure from the study of the molecular absorption bands measurements on Jupiter's disk and to compare them for SEB and NEB during "usual" and "unusual" state of the SEB region.
Bondarenko Natalia
Karimov Abdusalom
Kharitonova G.
Kirienko G.
Tejfel Victor
No associations
LandOfFree
The molecular absorption bands behavior on Jupiter before and at the Southern Equatorial Belt disappearance. 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 The molecular absorption bands behavior on Jupiter before and at the Southern Equatorial Belt disappearance., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The molecular absorption bands behavior on Jupiter before and at the Southern Equatorial Belt disappearance. will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1655400