SPICAM: Studying the global structure and composition of the martian atmosphere

J. L. Bertaux; D. Fonteyn; O. Korablev; E. Chassefière; E. Dimarellis; J. P. Dubois; A. Hauchecorne; F. Lefèvre; M. Cabane; P. Rannou; A. C. Levasseur-Regourd; G. Cernogora; E. Quemerais; C. Hermans; G. Kockarts; C. Lippens; M. De Maziere; D. Moreau; C. Muller; E. Neefs; P. C. Simon; F. Forget; F. Hourdin; O. Talagrand; V. I. Moroz; A. Rodin; B. Sandel; A. Stern

SPICAM: Studying the global structure and composition of the martian atmosphere

J. L. Bertaux
, D. Fonteyn
, O. Korablev
, E. Chassefière
, E. Dimarellis
, J. P. Dubois
, A. Hauchecorne
, F. Lefèvre
, M. Cabane
, P. Rannou
, A. C. Levasseur-Regourd
, G. Cernogora
, E. Quemerais
, C. Hermans
, G. Kockarts
, C. Lippens
, M. De Maziere
, D. Moreau
, C. Muller
, E. Neefs

P. C. Simon, F. Forget, F. Hourdin, O. Talagrand, V. I. Moroz, A. Rodin, B. Sandel, A. Stern

Résultats de recherche: Contribution à un journal › Article › Revue par des pairs

Résumé

The SPICAM (SPectroscopy for the Investigation of the Characteristics of the Atmosphere of Mars) instrument consists of two spectrometers. The UV spectrometer addresses key issues about ozone and its H₂O coupling, aerosols, the atmospheric vertical temperature structure and the ionosphere. The IR spectrometer is aimed primarily at H₂O abundances and vertical profiling of H₂O and aerosols. SPICAM's density/temperature profiles will aid the development of meteorological and dynamical atmospheric models from the surface up to 160 km altitude. UV observations of the upper atmosphere will study the ionosphere and its direct interaction with the solar wind. They will also allow a better understanding of escape mechanisms, crucial for insight into the long-term evolution of the atmosphere.

langue originale	Anglais
Pages (de - à)	95-120
Nombre de pages	26
journal	European Space Agency, (Special Publication) ESA SP
Numéro de publication	1240
état	Publié - 1 août 2004

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Bertaux, J. L., Fonteyn, D., Korablev, O., Chassefière, E., Dimarellis, E., Dubois, J. P., Hauchecorne, A., Lefèvre, F., Cabane, M., Rannou, P., Levasseur-Regourd, A. C., Cernogora, G., Quemerais, E., Hermans, C., Kockarts, G., Lippens, C., De Maziere, M., Moreau, D., Muller, C., ... Stern, A. (2004). SPICAM: Studying the global structure and composition of the martian atmosphere. European Space Agency, (Special Publication) ESA SP, (1240), 95-120.

@article{08522e673646429f9c00a8a8e4076d52,

title = "SPICAM: Studying the global structure and composition of the martian atmosphere",

abstract = "The SPICAM (SPectroscopy for the Investigation of the Characteristics of the Atmosphere of Mars) instrument consists of two spectrometers. The UV spectrometer addresses key issues about ozone and its H2O coupling, aerosols, the atmospheric vertical temperature structure and the ionosphere. The IR spectrometer is aimed primarily at H2O abundances and vertical profiling of H2O and aerosols. SPICAM's density/temperature profiles will aid the development of meteorological and dynamical atmospheric models from the surface up to 160 km altitude. UV observations of the upper atmosphere will study the ionosphere and its direct interaction with the solar wind. They will also allow a better understanding of escape mechanisms, crucial for insight into the long-term evolution of the atmosphere.",

author = "Bertaux, \{J. L.\} and D. Fonteyn and O. Korablev and E. Chassefi{\`e}re and E. Dimarellis and Dubois, \{J. P.\} and A. Hauchecorne and F. Lef{\`e}vre and M. Cabane and P. Rannou and Levasseur-Regourd, \{A. C.\} and G. Cernogora and E. Quemerais and C. Hermans and G. Kockarts and C. Lippens and \{De Maziere\}, M. and D. Moreau and C. Muller and E. Neefs and Simon, \{P. C.\} and F. Forget and F. Hourdin and O. Talagrand and Moroz, \{V. I.\} and A. Rodin and B. Sandel and A. Stern",

year = "2004",

month = aug,

day = "1",

language = "English",

pages = "95--120",

journal = "European Space Agency, (Special Publication) ESA SP",

issn = "0379-6566",

number = "1240",

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Bertaux, JL, Fonteyn, D, Korablev, O, Chassefière, E, Dimarellis, E, Dubois, JP, Hauchecorne, A, Lefèvre, F, Cabane, M, Rannou, P, Levasseur-Regourd, AC, Cernogora, G, Quemerais, E, Hermans, C, Kockarts, G, Lippens, C, De Maziere, M, Moreau, D, Muller, C, Neefs, E, Simon, PC, Forget, F , Hourdin, F, Talagrand, O, Moroz, VI, Rodin, A, Sandel, B & Stern, A 2004, 'SPICAM: Studying the global structure and composition of the martian atmosphere', European Space Agency, (Special Publication) ESA SP, Numéro 1240, p. 95-120.

TY - JOUR

T1 - SPICAM

T2 - Studying the global structure and composition of the martian atmosphere

AU - Bertaux, J. L.

AU - Fonteyn, D.

AU - Korablev, O.

AU - Chassefière, E.

AU - Dimarellis, E.

AU - Dubois, J. P.

AU - Hauchecorne, A.

AU - Lefèvre, F.

AU - Cabane, M.

AU - Rannou, P.

AU - Levasseur-Regourd, A. C.

AU - Cernogora, G.

AU - Quemerais, E.

AU - Hermans, C.

AU - Kockarts, G.

AU - Lippens, C.

AU - De Maziere, M.

AU - Moreau, D.

AU - Muller, C.

AU - Neefs, E.

AU - Simon, P. C.

AU - Forget, F.

AU - Hourdin, F.

AU - Talagrand, O.

AU - Moroz, V. I.

AU - Rodin, A.

AU - Sandel, B.

AU - Stern, A.

PY - 2004/8/1

Y1 - 2004/8/1

N2 - The SPICAM (SPectroscopy for the Investigation of the Characteristics of the Atmosphere of Mars) instrument consists of two spectrometers. The UV spectrometer addresses key issues about ozone and its H2O coupling, aerosols, the atmospheric vertical temperature structure and the ionosphere. The IR spectrometer is aimed primarily at H2O abundances and vertical profiling of H2O and aerosols. SPICAM's density/temperature profiles will aid the development of meteorological and dynamical atmospheric models from the surface up to 160 km altitude. UV observations of the upper atmosphere will study the ionosphere and its direct interaction with the solar wind. They will also allow a better understanding of escape mechanisms, crucial for insight into the long-term evolution of the atmosphere.

AB - The SPICAM (SPectroscopy for the Investigation of the Characteristics of the Atmosphere of Mars) instrument consists of two spectrometers. The UV spectrometer addresses key issues about ozone and its H2O coupling, aerosols, the atmospheric vertical temperature structure and the ionosphere. The IR spectrometer is aimed primarily at H2O abundances and vertical profiling of H2O and aerosols. SPICAM's density/temperature profiles will aid the development of meteorological and dynamical atmospheric models from the surface up to 160 km altitude. UV observations of the upper atmosphere will study the ionosphere and its direct interaction with the solar wind. They will also allow a better understanding of escape mechanisms, crucial for insight into the long-term evolution of the atmosphere.

UR - https://www.scopus.com/pages/publications/4243100602

M3 - Article

AN - SCOPUS:4243100602

SN - 0379-6566

SP - 95

EP - 120

JO - European Space Agency, (Special Publication) ESA SP

JF - European Space Agency, (Special Publication) ESA SP

IS - 1240

ER -

SPICAM: Studying the global structure and composition of the martian atmosphere

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