Orbital change experiments with a Mars general circulation model

By R. Haberle, J. Murphy, J. Schaeffer. 2003

228 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/fdc9cfd86d48749ff4188deb682847d8f3b7e290

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In Astronomy and Astrophysics

Citations in the corpus

Tropical mountain glaciers on Mars: Altitude-dependence of ice accumulation, accumulation conditions, formation times, glacier dynamics, and implications for planetary spin-axis/orbital history (2007, background): “Furthermore, atmospheric GCMs have improved sufficiently to include high-resolution simulations of circulation under different spin-axis/orbital parameter variations and to include the transport and deposition of water (Richardson and Wilson, 2002; Haberle et al., 2003; Mischna et al., 2004).”
Long-term monitoring of martian gully formation and evolution with MRO/HiRISE (2015, background): “However, the greater intensity of the seasonal cycle at higher obliquity (Haberle et al., 2003) could enhance seasonal frost processes for intervals at times before a few hundred ka.”
3D modelling of the early Martian Climate under a denser CO2 atmosphere: Temperatures and CO2 ice clouds. (2012, background): “…as high as 20◦) and above 60◦ (with amplitude of 9◦) Varying the obliquity or the season of perihelion in models of the present-day Mars climate system has a profound impact on the surface temperatures and the water cycle (e.g. Haberle et al. 2003, Forget et al. 2006, Montmessin et al. 2007a).”
Subsurface structure of Planum Boreum from Mars Reconnaissance Orbiter Shallow Radar soundings (2009, background): “Experiments with an atmospheric general circulation model (Haberle et al., 2003) suggest that, during times of high obliquity, atmospheric dynamics are favorable for lifting dust at high latitudes.”
North polar cap of Mars: Polar layered deposit characterization and identification of a fundamental climate signal (2005, unknown): “In this case, the combination of increased dust storm activity and decreased ice deposition and retention during periods of mean high obliquity [e.g., Jakosky et al., 1995; Richardson and Wilson, 2002; Haberle et al., 2003; Mischna et al., 2003] could produce a higher dust-to-ice ratio and a gener”
Mars Global Digital Dune Database and initial science results (2007, background): “MGD3 extends from 65 N to 65 S latitude and includes 550 dune fields, covering 70,000 km2, with an estimated total volume of 3,600 km3.”
Transverse Aeolian Ridges (TARs) on Mars (2008, background): “The first scenario is not well-supported by Global Circulation Models (GCM) of Mars' atmosphere, even under different obliquity conditions (Haberle et al., 2003): the mid to high latitudes appear to be the regions with the greatest potential for sediment transport, rather than the least.”