lmd_Rio2001.bib
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@article{2001AdSpR..27.1851C,
author = {{Chassefière}, E. and {Forget}, F. and {Hourdin}, F. and
{Vial}, F. and {Rème}, H. and {Mazelle}, C. and {Vignes}, D. and
{Sauvaud}, J.-A. and {Blelly}, P.-L. and {Toublanc}, D. and
{Berthelier}, J.-J. and {Cerisier}, J.-C. and {Chanteur}, G. and
{Duvet}, L. and {Menvielle}, M. and {Lilensten}, J. and {Witasse}, O. and
{Touboul}, P. and {Quèmerais}, E. and {Bertaux}, J.-L. and
{Hulot}, G. and {Cohen}, Y. and {Lognonné}, P. and {Barriot}, J.~P. and
{Balmino}, G. and {Blanc}, M. and {Pinet}, P. and {Parrot}, M. and
{Trotignon}, J.-G. and {Moncuquet}, M. and {Bougeret}, J.-L. and
{Issautier}, K. and {Lellouch}, E. and {Meyer}, N. and {Sotin}, C. and
{Grasset}, O. and {Barlier}, F. and {Berger}, C. and {Tarits}, P. and
{Dyment}, J. and {Breuer}, D. and {Spohn}, T. and {P{\"a}tzold}, M. and
{Sperveslage}, K. and {Gough}, P. and {Buckley}, A. and {Szego}, K. and
{Sasaki}, S. and {Smrekar}, S. and {Lyons}, D. and {Acuna}, M. and
{Connerney}, J. and {Purucker}, M. and {Lin}, R. and {Luhmann}, J. and
{Mitchell}, D. and {Leblanc}, F. and {Johnson}, R. and {Clarke}, J. and
{Nagy}, A. and {Young}, D. and {Bougher}, S. and {Keating}, G. and
{Haberle}, R. and {Jakosky}, B. and {Hodges}, R. and {Parmentier}, M. and
{Waite}, H. and {Bass}, D.},
title = {{Scientific objectives of the DYNAMO mission}},
journal = {Advances in Space Research},
year = 2001,
volume = 27,
pages = {1851-1860},
abstract = {{DYNAMO is a small Mars orbiter planned to be launched in 2005 or 2007,
in the frame of the NASA/ CNES Mars exploration program. It is aimed at
improving gravity and magnetic field resolution, in order to better
understand the magnetic, geologic and thermal history of Mars, and at
characterizing current atmospheric escape, which is still poorly
constrained. These objectives are achieved by using a low periapsis
orbit, similar to the one used by the Mars Global Surveyor spacecraft
during its aerobraking phases. The proposed periapsis altitude for
DYNAMO of 120-130 km, coupled with the global distribution of periapses
to be obtained during one Martian year of operation, through about 5000
low passes, will produce a magnetic/gravity field data set with
approximately five times the spatial resolution of MGS. Additional data
on the internal structure will be obtained by mapping the electric
conductivity. Low periapsis provides a unique opportunity to investigate
the chemical and dynamical properties of the deep ionosphere,
thermosphere, and the interaction between the atmosphere and the solar
wind, therefore atmospheric escape, which may have played a crucial role
in removing atmosphere and water from the planet.
}},
doi = {10.1016/S0273-1177(01)00338-6},
adsurl = {http://adsabs.harvard.edu/abs/2001AdSpR..27.1851C},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
