Derivation of Martian meteorological parameters using ground-based telescopes and forward-modelling

A. J. Simpson; J. A. Bailey; S. Chamberlain; M. R. Walter; D. Crisp

Derivation of Martian meteorological parameters using ground-based telescopes and forward-modelling

A. J. Simpson, J. A. Bailey, S. Chamberlain, M. R. Walter, D. Crisp

Faculty of Science and Engineering

Research output: Chapter in Book/Report/Conference proceeding › Conference proceeding contribution

Abstract

Ground-based telescopes offer a number of advantages for characterising the Martian atmosphere, including the ability to use high resolution (R ~ 30000) spectroscopy and to simultaneously characterise the atmospheric state across an entire hemisphere. In October/November 2005 we obtained high-resolution ground-based spectra of Mars in the 1.6 μm and 2.0 μm CO2 bands using IRTF/CSHELL and Gemini South/GNIRS with the intention of deriving temperature, pressure and dust optical depth maps from these. We will make use of a forward-modelling technique to iteratively match our observational spectra to simulated spectra created using SMART and VSTAR. We present preliminary results demonstrating our models and observations match closely.

Original language	English
Title of host publication	Proceedings of Second Workshop on Mars atmosphere modelling and observations
Editors	F. Forget
Place of Publication	Paris
Publisher	Laboratoire de Meteorologie Dynamique
Number of pages	4
Publication status	Published - 2006
Event	Workshop on Mars Atmosphere Modelling and Observations (2nd : 2006) - Granada, Spain Duration: 27 Feb 2006 → 3 Mar 2006

Workshop

Workshop	Workshop on Mars Atmosphere Modelling and Observations (2nd : 2006)
City	Granada, Spain
Period	27/02/06 → 3/03/06

Keywords

Martian atmosphere

Access to Document

http://www-mars.lmd.jussieu.fr/granada2006/abstracts/Simpson_Granada2006.pdf

Cite this

Simpson, A. J., Bailey, J. A., Chamberlain, S., Walter, M. R., & Crisp, D. (2006). Derivation of Martian meteorological parameters using ground-based telescopes and forward-modelling. In F. Forget (Ed.), Proceedings of Second Workshop on Mars atmosphere modelling and observations Laboratoire de Meteorologie Dynamique. http://www-mars.lmd.jussieu.fr/granada2006/abstracts/Simpson_Granada2006.pdf

@inproceedings{c47aa315b4594ba8ab83740cda7b7879,

title = "Derivation of Martian meteorological parameters using ground-based telescopes and forward-modelling",

abstract = "Ground-based telescopes offer a number of advantages for characterising the Martian atmosphere, including the ability to use high resolution (R ~ 30000) spectroscopy and to simultaneously characterise the atmospheric state across an entire hemisphere. In October/November 2005 we obtained high-resolution ground-based spectra of Mars in the 1.6 μm and 2.0 μm CO2 bands using IRTF/CSHELL and Gemini South/GNIRS with the intention of deriving temperature, pressure and dust optical depth maps from these. We will make use of a forward-modelling technique to iteratively match our observational spectra to simulated spectra created using SMART and VSTAR. We present preliminary results demonstrating our models and observations match closely.",

keywords = "Martian atmosphere",

author = "Simpson, {A. J.} and Bailey, {J. A.} and S. Chamberlain and Walter, {M. R.} and D. Crisp",

year = "2006",

language = "English",

editor = "F. Forget",

booktitle = "Proceedings of Second Workshop on Mars atmosphere modelling and observations",

publisher = "Laboratoire de Meteorologie Dynamique",

note = "Workshop on Mars Atmosphere Modelling and Observations (2nd : 2006) ; Conference date: 27-02-2006 Through 03-03-2006",

}

Simpson, AJ, Bailey, JA, Chamberlain, S, Walter, MR & Crisp, D 2006, Derivation of Martian meteorological parameters using ground-based telescopes and forward-modelling. in F Forget (ed.), Proceedings of Second Workshop on Mars atmosphere modelling and observations. Laboratoire de Meteorologie Dynamique, Paris, Workshop on Mars Atmosphere Modelling and Observations (2nd : 2006), Granada, Spain, 27/02/06. <http://www-mars.lmd.jussieu.fr/granada2006/abstracts/Simpson_Granada2006.pdf>

Derivation of Martian meteorological parameters using ground-based telescopes and forward-modelling. / Simpson, A. J.; Bailey, J. A.; Chamberlain, S. et al.
Proceedings of Second Workshop on Mars atmosphere modelling and observations. ed. / F. Forget. Paris: Laboratoire de Meteorologie Dynamique, 2006.

Research output: Chapter in Book/Report/Conference proceeding › Conference proceeding contribution

TY - GEN

T1 - Derivation of Martian meteorological parameters using ground-based telescopes and forward-modelling

AU - Simpson, A. J.

AU - Bailey, J. A.

AU - Chamberlain, S.

AU - Walter, M. R.

AU - Crisp, D.

PY - 2006

Y1 - 2006

N2 - Ground-based telescopes offer a number of advantages for characterising the Martian atmosphere, including the ability to use high resolution (R ~ 30000) spectroscopy and to simultaneously characterise the atmospheric state across an entire hemisphere. In October/November 2005 we obtained high-resolution ground-based spectra of Mars in the 1.6 μm and 2.0 μm CO2 bands using IRTF/CSHELL and Gemini South/GNIRS with the intention of deriving temperature, pressure and dust optical depth maps from these. We will make use of a forward-modelling technique to iteratively match our observational spectra to simulated spectra created using SMART and VSTAR. We present preliminary results demonstrating our models and observations match closely.

AB - Ground-based telescopes offer a number of advantages for characterising the Martian atmosphere, including the ability to use high resolution (R ~ 30000) spectroscopy and to simultaneously characterise the atmospheric state across an entire hemisphere. In October/November 2005 we obtained high-resolution ground-based spectra of Mars in the 1.6 μm and 2.0 μm CO2 bands using IRTF/CSHELL and Gemini South/GNIRS with the intention of deriving temperature, pressure and dust optical depth maps from these. We will make use of a forward-modelling technique to iteratively match our observational spectra to simulated spectra created using SMART and VSTAR. We present preliminary results demonstrating our models and observations match closely.

KW - Martian atmosphere

M3 - Conference proceeding contribution

BT - Proceedings of Second Workshop on Mars atmosphere modelling and observations

A2 - Forget, F.

PB - Laboratoire de Meteorologie Dynamique

CY - Paris

T2 - Workshop on Mars Atmosphere Modelling and Observations (2nd : 2006)

Y2 - 27 February 2006 through 3 March 2006

ER -

Derivation of Martian meteorological parameters using ground-based telescopes and forward-modelling

Abstract

Workshop

Keywords

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