Chemical profiles in Neptune's atmosphere as derived from EVLA and historical radio observations

Details Chemical profiles in Neptune's atmosphere as derived from EVLA and historical radio observations Chemical profiles in Neptune's atmosphere as derived from EVLA and historical radio observations

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf..695n&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.695

Computer Science

Scientific paper

We present results from modeling the chemical composition of the atmosphere of Neptune. Our models employ radiative transfer calculations to generate synthetic spectra from 0.03 to 21 cm for comparison with full-disk observations from 1966 to present. This observation dataset is augmented with spatially resolved observations from the Very Large Array and its recent improvement, the Expanded Very Large Array, allowing for the investigation of the chemical abundances' variance with latitude and longitude.

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