CaltechAUTHORS
  A Caltech Library Service

Preliminary assessment of Termoskan observations of Mars

Murray, B. and Naraeva, M. K. and Selivanov, A. S. and Betts, B. H. and Svitek, T. and Kharlamov, V. D. and Romanov, A. V. and Santee, M. L. and Gektin, Y. M. and Fomin, D. A. and Paige, D. A. and Panfilov, A. S. and Crisp, D. and Head, J. W. and Murchie, S. L. and Martin, T. Z. (1991) Preliminary assessment of Termoskan observations of Mars. Planetary and Space Science, 39 (1-2). pp. 237-265. ISSN 0032-0633. https://resolver.caltech.edu/CaltechAUTHORS:20140410-092259617

Full text is not posted in this repository. Consult Related URLs below.

Use this Persistent URL to link to this item: https://resolver.caltech.edu/CaltechAUTHORS:20140410-092259617

Abstract

In February and March, 1989, the Termoskan instrument onboard the Phobos '88 spacecraft acquired a limited set of very high resolution observations of the 8–12 μm thermal emission from Mars' equatorial regions. Simultaneous and coincident observations were acquired in the 0.5 to 1.0 μm region also. We have evaluated quantitatively about 25% of those data and find close agreement with the lower-resolution Viking Orbiter Infrared Thermal Mapper (IRTM) observations, demonstrating the accuracy of the Termoskan system. Termoskan's thermal emission panoramas display limb brightening at the morning limb, which we interpret as arising from the presence of a diurnal ice crystal haze there. Detached hazes at high altitude also are evident in the visible panorama of the evening limb. The Phobos '88 orbit enabled Termoskan to record the visible shadow from the Martian moonlet Phobos and to measure the surface thermal response to that shadow's passage. Analysis of one such data set shows that the uppermost fraction of a millimeter is two to four times more insulating than the uppermost centimeters sensed by the IRTM experiment. The Termoskan data are of direct importance to the planning and execution of the PMIRR and TES experiments of the U.S. Mars Observer mission to be launched in 1992. An improved version of Termoskan is planned for the Mars '94 mission of the U.S.S.R. Those data will be of still higher surface resolution and, thus, complement well the expected PMIRR and TES global data sets.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1016/0032-0633(91)90147-3DOIArticle
ORCID:
AuthorORCID
Crisp, D.0000-0002-4573-9998
Additional Information:© 1991 Pergamon Press. Camera-ready copy received 18 September 1990. This work was supported by NASA grant NAGW 1426.
Funders:
Funding AgencyGrant Number
NASANAGW 1426
Other Numbering System:
Other Numbering System NameOther Numbering System ID
Caltech Division of Geological and Planetary Sciences4820
Issue or Number:1-2
Record Number:CaltechAUTHORS:20140410-092259617
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20140410-092259617
Official Citation:B. Murray, M.K. Naraeva, A.S. Selivanov, B.H. Betts, T. Svitek, V.D Kharlamov, A.V. Romanov, M.L. Santee, Y.M. Gektin, D.A. Fomin, D.A. Paige, A.S. Panfilov, D. Crisp, J.W. Head, S.L. Murchie, Martin T.Z., Preliminary assessment of Termoskan observations of Mars, Planetary and Space Science, Volume 39, Issues 1–2, January–February 1991, Pages 237-265, ISSN 0032-0633, http://dx.doi.org/10.1016/0032-0633(91)90147-3. (http://www.sciencedirect.com/science/article/pii/0032063391901473)
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:44846
Collection:CaltechAUTHORS
Deposited By: Ruth Sustaita
Deposited On:10 Apr 2014 16:40
Last Modified:30 Oct 2019 17:37

Repository Staff Only: item control page