Remote sensing of the Martian atmosphere with ground-based telescopes

Jeremy Bailey; Sarah Chamberlain; Andrew Simpson; David Crisp

Remote sensing of the Martian atmosphere with ground-based telescopes

Jeremy Bailey, Sarah Chamberlain, Andrew Simpson, David Crisp

Faculty of Science and Engineering

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

Abstract

We are developing techniques for measuring basic properties of the Martian atmosphere using ground-based telescopes. By observing the reflected light spectrum at near-IR wavelengths we can obtain information on the composition and structure of the atmosphere. We use imaging spectroscopy to obtain spectra across the planet’s disk and interpret the data with the help of high-resolution radiative transfer models.

Original language	English
Title of host publication	Proceeding of the Second Workshop on Mars Atmosphere modelling and observations workshop
Editors	S. R. Lewis, L. Montabone, P. L. Read, P. Rogberg
Place of Publication	Paris
Publisher	Laboratoire de Meteorologie Dynamique
Pages	142-145
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

Cite this

@inproceedings{1d57a091656f4a43a7cfb962f3afcb22,

title = "Remote sensing of the Martian atmosphere with ground-based telescopes",

abstract = "We are developing techniques for measuring basic properties of the Martian atmosphere using ground-based telescopes. By observing the reflected light spectrum at near-IR wavelengths we can obtain information on the composition and structure of the atmosphere. We use imaging spectroscopy to obtain spectra across the planet{\textquoteright}s disk and interpret the data with the help of high-resolution radiative transfer models.",

author = "Jeremy Bailey and Sarah Chamberlain and Andrew Simpson and David Crisp",

year = "2006",

language = "English",

pages = "142--145",

editor = "Lewis, {S. R.} and L. Montabone and Read, {P. L.} and P. Rogberg",

booktitle = "Proceeding of the Second Workshop on Mars Atmosphere modelling and observations workshop",

publisher = "Laboratoire de Meteorologie Dynamique",

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

}

Bailey, J, Chamberlain, S, Simpson, A & Crisp, D 2006, Remote sensing of the Martian atmosphere with ground-based telescopes. in SR Lewis, L Montabone, PL Read & P Rogberg (eds), Proceeding of the Second Workshop on Mars Atmosphere modelling and observations workshop. Laboratoire de Meteorologie Dynamique, Paris, pp. 142-145, Workshop on Mars Atmosphere Modelling and Observations (2nd : 2006), Granada, Spain, 27/02/06.

Remote sensing of the Martian atmosphere with ground-based telescopes. / Bailey, Jeremy; Chamberlain, Sarah; Simpson, Andrew et al.
Proceeding of the Second Workshop on Mars Atmosphere modelling and observations workshop. ed. / S. R. Lewis; L. Montabone; P. L. Read; P. Rogberg. Paris: Laboratoire de Meteorologie Dynamique, 2006. p. 142-145.

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

TY - GEN

T1 - Remote sensing of the Martian atmosphere with ground-based telescopes

AU - Bailey, Jeremy

AU - Chamberlain, Sarah

AU - Simpson, Andrew

AU - Crisp, David

PY - 2006

Y1 - 2006

N2 - We are developing techniques for measuring basic properties of the Martian atmosphere using ground-based telescopes. By observing the reflected light spectrum at near-IR wavelengths we can obtain information on the composition and structure of the atmosphere. We use imaging spectroscopy to obtain spectra across the planet’s disk and interpret the data with the help of high-resolution radiative transfer models.

AB - We are developing techniques for measuring basic properties of the Martian atmosphere using ground-based telescopes. By observing the reflected light spectrum at near-IR wavelengths we can obtain information on the composition and structure of the atmosphere. We use imaging spectroscopy to obtain spectra across the planet’s disk and interpret the data with the help of high-resolution radiative transfer models.

M3 - Conference proceeding contribution

SP - 142

EP - 145

BT - Proceeding of the Second Workshop on Mars Atmosphere modelling and observations workshop

A2 - Lewis, S. R.

A2 - Montabone, L.

A2 - Read, P. L.

A2 - Rogberg, P.

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 -

Remote sensing of the Martian atmosphere with ground-based telescopes

Abstract

Workshop

Fingerprint

Cite this