The NEMESIS planetary atmosphere radiative transfer and retrieval tool
With the exception of in situ atmospheric probes, the most useful way to study the atmospheres of other planets is to observe their electromagnetic spectra through remote observations, either from ground-based telescopes or from spacecraft. Atmospheric properties most consistent with these observed...
Main Authors: | Irwin, P, Teanby, N, de Kok, R, Fletcher, L, Howett, C, Tsang, C, Wilson, C, Calcutt, S, Nixon, C, Parrish, P |
---|---|
Format: | Journal article |
Language: | English |
Published: |
2008
|
Similar Items
-
Meridional variations in stratospheric acetylene and ethane in the southern hemisphere of the saturnian atmosphere as determined from Cassini/CIRS measurements
by: Howett, C, et al.
Published: (2007) -
Vertical profiles of HCN, HC3N, and C2H2 in Titan's atmosphere derived from Cassini/CIRS data
by: Teanby, N, et al.
Published: (2007) -
Radiative transfer models for Galileo NIMS studies of the atmosphere of Jupiter
by: Irwin, P, et al.
Published: (1997) -
Differentiability and retrievability of CO2 and H2O clouds on Mars from MRO/MCS measurements: A radiative-transfer study
by: Hurley, J, et al.
Published: (2014) -
Genesis and NEMESIS.
by: Goding, C
Published: (2008)