Temporal variability of waves at the proton cyclotron frequency upstream from Mars: Implications for Mars distant hydrogen exosphere

We report on the temporal variability of the occurrence of waves at the local proton cyclotron frequency upstream from the Martian bow shock from Mars Global Surveyor observations during the first aerobraking and science phasing orbit periods. Observations at high southern latitudes during minimum-t...

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Autores principales: Bertucci, C., Romanelli, N., Chaufray, J.Y., Gomez, D., Mazelle, C., Delva, M., Modolo, R., González-Galindo, F., Brain, D.A.
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Acceso en línea:http://hdl.handle.net/20.500.12110/paper_00948276_v40_n15_p3809_Bertucci
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spelling todo:paper_00948276_v40_n15_p3809_Bertucci2023-10-03T14:56:33Z Temporal variability of waves at the proton cyclotron frequency upstream from Mars: Implications for Mars distant hydrogen exosphere Bertucci, C. Romanelli, N. Chaufray, J.Y. Gomez, D. Mazelle, C. Delva, M. Modolo, R. González-Galindo, F. Brain, D.A. Exosphere Hydrogen Mars Pick-up Thermosphere Waves Direct measurement Exosphere Mars Mars global surveyor Plasma wave generation Southern latitudes Temporal variability Thermosphere Cyclotron resonance Pickups Protons Solar energy Waves Hydrogen corona density Mars Mars Pathfinder orbit determination polar region solar activity temporal variation thermosphere wave field We report on the temporal variability of the occurrence of waves at the local proton cyclotron frequency upstream from the Martian bow shock from Mars Global Surveyor observations during the first aerobraking and science phasing orbit periods. Observations at high southern latitudes during minimum-to-mean solar activity show that the wave occurrence rate is significantly higher around perihelion/southern summer solstice than around the spring and autumn equinoxes. A similar trend is observed in the hydrogen (H) exospheric density profiles over the Martian dayside and South Pole obtained from a model including UV thermospheric heating effects. In spite of the complexity in the ion pickup and plasma wave generation and evolution processes, these results support the idea that variations in the occurrence of waves could be used to study the temporal evolution of the distant Martian H corona and its coupling with the thermosphere at altitudes currently inaccessible to direct measurements. © 2013. American Geophysical Union. All Rights Reserved. Fil:Bertucci, C. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. Fil:Romanelli, N. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. Fil:Gomez, D. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. JOUR info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_00948276_v40_n15_p3809_Bertucci
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-134
collection Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
topic Exosphere
Hydrogen
Mars
Pick-up
Thermosphere
Waves
Direct measurement
Exosphere
Mars
Mars global surveyor
Plasma wave generation
Southern latitudes
Temporal variability
Thermosphere
Cyclotron resonance
Pickups
Protons
Solar energy
Waves
Hydrogen
corona
density
Mars
Mars Pathfinder
orbit determination
polar region
solar activity
temporal variation
thermosphere
wave field
spellingShingle Exosphere
Hydrogen
Mars
Pick-up
Thermosphere
Waves
Direct measurement
Exosphere
Mars
Mars global surveyor
Plasma wave generation
Southern latitudes
Temporal variability
Thermosphere
Cyclotron resonance
Pickups
Protons
Solar energy
Waves
Hydrogen
corona
density
Mars
Mars Pathfinder
orbit determination
polar region
solar activity
temporal variation
thermosphere
wave field
Bertucci, C.
Romanelli, N.
Chaufray, J.Y.
Gomez, D.
Mazelle, C.
Delva, M.
Modolo, R.
González-Galindo, F.
Brain, D.A.
Temporal variability of waves at the proton cyclotron frequency upstream from Mars: Implications for Mars distant hydrogen exosphere
topic_facet Exosphere
Hydrogen
Mars
Pick-up
Thermosphere
Waves
Direct measurement
Exosphere
Mars
Mars global surveyor
Plasma wave generation
Southern latitudes
Temporal variability
Thermosphere
Cyclotron resonance
Pickups
Protons
Solar energy
Waves
Hydrogen
corona
density
Mars
Mars Pathfinder
orbit determination
polar region
solar activity
temporal variation
thermosphere
wave field
description We report on the temporal variability of the occurrence of waves at the local proton cyclotron frequency upstream from the Martian bow shock from Mars Global Surveyor observations during the first aerobraking and science phasing orbit periods. Observations at high southern latitudes during minimum-to-mean solar activity show that the wave occurrence rate is significantly higher around perihelion/southern summer solstice than around the spring and autumn equinoxes. A similar trend is observed in the hydrogen (H) exospheric density profiles over the Martian dayside and South Pole obtained from a model including UV thermospheric heating effects. In spite of the complexity in the ion pickup and plasma wave generation and evolution processes, these results support the idea that variations in the occurrence of waves could be used to study the temporal evolution of the distant Martian H corona and its coupling with the thermosphere at altitudes currently inaccessible to direct measurements. © 2013. American Geophysical Union. All Rights Reserved.
format JOUR
author Bertucci, C.
Romanelli, N.
Chaufray, J.Y.
Gomez, D.
Mazelle, C.
Delva, M.
Modolo, R.
González-Galindo, F.
Brain, D.A.
author_facet Bertucci, C.
Romanelli, N.
Chaufray, J.Y.
Gomez, D.
Mazelle, C.
Delva, M.
Modolo, R.
González-Galindo, F.
Brain, D.A.
author_sort Bertucci, C.
title Temporal variability of waves at the proton cyclotron frequency upstream from Mars: Implications for Mars distant hydrogen exosphere
title_short Temporal variability of waves at the proton cyclotron frequency upstream from Mars: Implications for Mars distant hydrogen exosphere
title_full Temporal variability of waves at the proton cyclotron frequency upstream from Mars: Implications for Mars distant hydrogen exosphere
title_fullStr Temporal variability of waves at the proton cyclotron frequency upstream from Mars: Implications for Mars distant hydrogen exosphere
title_full_unstemmed Temporal variability of waves at the proton cyclotron frequency upstream from Mars: Implications for Mars distant hydrogen exosphere
title_sort temporal variability of waves at the proton cyclotron frequency upstream from mars: implications for mars distant hydrogen exosphere
url http://hdl.handle.net/20.500.12110/paper_00948276_v40_n15_p3809_Bertucci
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