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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Main Authors: Bertucci, Cesar, Romanelli, Norberto Julio, Gomez, Daniel Osvaldo
Language:unknown
Published: 2013
Subjects:
Online Access:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00948276_v40_n15_p3809_Bertucci
https://hdl.handle.net/20.500.12110/paper_00948276_v40_n15_p3809_Bertucci
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spelling ftunibueairesbd:paper:paper_00948276_v40_n15_p3809_Bertucci 2023-05-15T18:22:55+02:00 Temporal variability of waves at the proton cyclotron frequency upstream from Mars: Implications for Mars distant hydrogen exosphere Bertucci, Cesar Romanelli, Norberto Julio Gomez, Daniel Osvaldo 2013 https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00948276_v40_n15_p3809_Bertucci https://hdl.handle.net/20.500.12110/paper_00948276_v40_n15_p3809_Bertucci unknown https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00948276_v40_n15_p3809_Bertucci http://hdl.handle.net/20.500.12110/paper_00948276_v40_n15_p3809_Bertucci Exosphere Hydrogen Mars Pick-up Thermosphere Waves Direct measurement Mars global surveyor Plasma wave generation Southern latitudes Temporal variability Cyclotron resonance Pickups Protons Solar energy corona density Mars Pathfinder orbit determination polar region solar activity temporal variation wave field 2013 ftunibueairesbd https://doi.org/20.500.12110/paper_00948276_v40_n15_p3809_Bertucci 2023-02-16T02:21:47Z 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. Other/Unknown Material South pole Biblioteca Digital FCEN-UBA (Facultad de Ciencias Exactas y Naturales, Universidad de Buenos Aires) Argentina South Pole
institution Open Polar
collection Biblioteca Digital FCEN-UBA (Facultad de Ciencias Exactas y Naturales, Universidad de Buenos Aires)
op_collection_id ftunibueairesbd
language unknown
topic Exosphere
Hydrogen
Mars
Pick-up
Thermosphere
Waves
Direct measurement
Mars global surveyor
Plasma wave generation
Southern latitudes
Temporal variability
Cyclotron resonance
Pickups
Protons
Solar energy
corona
density
Mars Pathfinder
orbit determination
polar region
solar activity
temporal variation
wave field
spellingShingle Exosphere
Hydrogen
Mars
Pick-up
Thermosphere
Waves
Direct measurement
Mars global surveyor
Plasma wave generation
Southern latitudes
Temporal variability
Cyclotron resonance
Pickups
Protons
Solar energy
corona
density
Mars Pathfinder
orbit determination
polar region
solar activity
temporal variation
wave field
Bertucci, Cesar
Romanelli, Norberto Julio
Gomez, Daniel Osvaldo
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
Mars global surveyor
Plasma wave generation
Southern latitudes
Temporal variability
Cyclotron resonance
Pickups
Protons
Solar energy
corona
density
Mars Pathfinder
orbit determination
polar region
solar activity
temporal variation
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. 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.
author Bertucci, Cesar
Romanelli, Norberto Julio
Gomez, Daniel Osvaldo
author_facet Bertucci, Cesar
Romanelli, Norberto Julio
Gomez, Daniel Osvaldo
author_sort Bertucci, Cesar
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
publishDate 2013
url https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00948276_v40_n15_p3809_Bertucci
https://hdl.handle.net/20.500.12110/paper_00948276_v40_n15_p3809_Bertucci
geographic Argentina
South Pole
geographic_facet Argentina
South Pole
genre South pole
genre_facet South pole
op_relation https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00948276_v40_n15_p3809_Bertucci
http://hdl.handle.net/20.500.12110/paper_00948276_v40_n15_p3809_Bertucci
op_doi https://doi.org/20.500.12110/paper_00948276_v40_n15_p3809_Bertucci
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