Traveling waves in the martian atmosphere from MGS TES Nadir data

By D. Banfield, B. Conrath, P. Gierasch, Robert J. Wilson, Michael D. Smith. 2004

132 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Atmospheric Science

View Paper: https://www.semanticscholar.org/paper/1a4125727958b93bb71a40a7b632fa740fcaf6b6

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. Michael D. Smith
2. S. R. Lewis
3. J. Murphy
4. Peter L Read
5. R. Haberle
6. J. Pearl
7. B. Conrath
8. M. Kahre

In Atmospheric Science

1. Michael D. Smith
2. J. Murphy
3. Peter L Read
4. S. R. Lewis
5. J. Pearl
6. M. Kahre
7. B. Conrath
8. R. Haberle

Citations in the corpus

• Spacecraft Observations of the Martian Atmosphere (2008, background): “…global-scale monitoring of atmospheric temperatures made possible by TES observations shows a variety of waves, which play an important role in the horizontal and vertical transport of heat, momentum, and atmospheric constituents such as aerosols and water vapor (e.g., Banfield et al. 2003, 2004).”
• Assimilation of thermal emission spectrometer atmospheric data during the Mars Global Surveyor aerobraking period (2007, methodology): “Data assimilation has been suggested by several authors (Banfield et al., 1995; Lewis and Read, 1995; Lewis et al., 1996, 1997; Houben, 1999; Kass, 1999) as an effective tool with which to analyze spacecraft observations of the martian atmosphere. The advantages of data assimilation for this problem”
• Modeling the Martian dust cycle and surface dust reservoirs with the NASA Ames general circulation model (2006, background): “Simulated temporally and zonally averaged temperatures at the equinoxes and solstices reflect the corresponding TES-derived temperature fields (Figure 4) [ Banfield et al., 2004 ].”
• Interannual variability in TES atmospheric observations of Mars during 1999–2003 (2004, result): “Earlier results from MGS mapping have (for example) given overviews of TES atmospheric results (Smith et al., 2001a,b, 2003a), have described a retrieval for water vapor abundance (Smith, 2002), have analyzed the structure of waves in the martian atmosphere Banfield et al., 2002, 2003; Wilson et a”