The origin of belt/zone contrasts in the atmosphere of Jupiter and their correlation with 5-mu m opacity

Registos relacionados

• The Origin of Belt/Zone Contrasts in the Atmosphere of Jupiter and Their Correlation with 5-μm Opacity
  Por: Irwin, P, et al.
  Publicado em: (2001)
• Correlation of near-infrared albedo and 5-micron brightness variations in Jupiter's atmosphere
  Por: Irwin, P, et al.
  Publicado em: (2002)
• Analysis of Jupiter North Equatorial Belt hot spots in the 4-5 mu m range from Galileo near-infrared mapping spectrometer observations: Measurements of cloud opacity, water, and ammonia
  Por: Roos-Serote, M, et al.
  Publicado em: (1998)
• The solar reflected component in Jupiter's 5-mu m spectra from NIMS/Galileo observations
  Por: Drossart, P, et al.
  Publicado em: (1998)
• Radiative transfer models for Galileo NIMS studies of the atmosphere of Jupiter
  Por: Irwin, P, et al.
  Publicado em: (1997)