Martian magnetism with orbiting sub-millimeter sensor: simulated retrieval system
-
Published:2017-01-27
Issue:1
Volume:6
Page:27-37
-
ISSN:2193-0864
-
Container-title:Geoscientific Instrumentation, Methods and Data Systems
-
language:en
-
Short-container-title:Geosci. Instrum. Method. Data Syst.
Author:
Larsson RichardORCID, Milz Mathias, Eriksson PatrickORCID, Mendrok Jana, Kasai Yasuko, Buehler Stefan AlexanderORCID, Diéval CatherineORCID, Brain David, Hartogh PaulORCID
Abstract
Abstract. A Mars-orbiting sub-millimeter sensor can be used to retrieve the magnetic field at low altitudes over large areas of significant planetary crustal magnetism of the surface of Mars from measurements of circularly polarized radiation emitted by the 368 GHz ground-state molecular oxygen absorption line. We design a full retrieval system for one example orbit to show the expected accuracies on the magnetic field components that one realization of such a Mars satellite mission could achieve. For one set of measurements around a tangent profile, we find that the two horizontal components of the magnetic field can be measured at about 200 nT error with a vertical resolution of around 4 km from 6 up to 70 km in tangent altitude. The error is similar regardless of the true strength of the magnetic field, and it can be reduced by repeated measurements over the same area. The method and some of its potential pitfalls are described and discussed.
Publisher
Copernicus GmbH
Subject
Atmospheric Science,Geology,Oceanography
Reference33 articles.
1. Acuña, M. H., Connerney, J. E. P., Wasilewski, P., Lin, R. P., Anderson, K. A., Carlson, C. W., McFadden, J., Curtis, D. W., Mitchell, D., Rème, H., Mazelle, C., Sauvaud, J. A., d'Uston, C., Cros, A., Medale, J. L., Bauer, S. J., Cloutier, P., Mayhew, M., Winterhalter, D., and Ness, N. F.: Magnetic Field and Plasma Observations at Mars: Initial Results of the Mars Global Surveyor Mission, Science, 279, 1676–1680, 1998. 2. Acuña, M. H., Connerney, J. E. P., Ness, N. F., Lin, R. P., Mitchell, D., Carlson, C. W., McFadden, J., Anderson, K. A., Rème, H., Mazelle, C., Vignes, D., Wasilewski, P., and Cloutier, P.: Global Distribution of Crustal Magnetization Discovered by the Mars Global Surveyor MAG/ER Experiment, Science, 284, 790–793, 1999. 3. Brain, D. A., Bagenal, F., Acuña, M. H., and Connerney, J. E. P.: Martian magnetic morphology: Contribution from the solar wind and crust, J. Geophys. Res., 108, 1424, https://doi.org/10.1029/2002JA009482, 2003. 4. Buehler, S. A., Eriksson, P., Kuhn, T., von Engeln, A., and Verdes, C.: ARTS, the atmospheric radiative transfer simulator, J. Quant. Spectrosc. Ra. 91, 65–93, https://doi.org/10.1016/j.jqsrt.2004.05.051, 2005. 5. Buehler, S. A., von Engeln, A., Brocard, E., John, V. O., Kuhn, T., and Eriksson, P.: Recent developments in the line-by-line modeling of outgoing longwave radiation, J. Quant. Spectrosc. Ra., 98, 446–457, https://doi.org/10.1016/j.jqsrt.2005.11.001, 2006.
Cited by
4 articles.
订阅此论文施引文献
订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献
|
|