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...

Full description

Bibliographic Details
Published in:Geophysical Research Letters
Main Authors: Bertucci, Cesar, Romanelli, Norberto Julio, Chaufray, J. Y., Gomez, Daniel Osvaldo, Mazelle, C., Delva, M., Modolo, R., González Galindo, F., Brain, D. A.
Format: Article in Journal/Newspaper
Language:English
Published: American Geophysical Union
Subjects:
Online Access:http://hdl.handle.net/11336/17062
id ftconicet:oai:ri.conicet.gov.ar:11336/17062
record_format openpolar
spelling ftconicet:oai:ri.conicet.gov.ar:11336/17062 2023-10-09T21:55:59+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 Chaufray, J. Y. Gomez, Daniel Osvaldo Mazelle, C. Delva, M. Modolo, R. González Galindo, F. Brain, D. A. application/pdf http://hdl.handle.net/11336/17062 eng eng American Geophysical Union info:eu-repo/semantics/altIdentifier/url/onlinelibrary.wiley.com/doi/10.1002/grl.50709/full info:eu-repo/semantics/altIdentifier/doi/10.1002/grl.50709 http://hdl.handle.net/11336/17062 Bertucci, Cesar; Romanelli, Norberto Julio; Chaufray, J. Y.; Gomez, Daniel Osvaldo; Mazelle, C.; et al.; Temporal variability of waves at the proton cyclotron frequency upstream from Mars: Implications for Mars distant hydrogen exosphere; American Geophysical Union; Geophysical Research Letters; 40; 15; 1-8-2013; 3809-3813 0094-8276 info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ MARS EXOSPHERE PICK UP https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 info:eu-repo/semantics/article info:ar-repo/semantics/artículo info:eu-repo/semantics/publishedVersion ftconicet https://doi.org/10.1002/grl.50709 2023-09-24T19:11:54Z 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. Fil: Bertucci, Cesar. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina Fil: Romanelli, Norberto Julio. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina Fil: Chaufray, J. Y. LATMOS; Francia Fil: Gomez, Daniel Osvaldo. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina Fil: Mazelle, C. IRAP; Francia ... Article in Journal/Newspaper South pole CONICET Digital (Consejo Nacional de Investigaciones Científicas y Técnicas) Argentina South Pole Gomez ENVELOPE(-58.795,-58.795,-62.196,-62.196) Geophysical Research Letters 40 15 3809 3813
institution Open Polar
collection CONICET Digital (Consejo Nacional de Investigaciones Científicas y Técnicas)
op_collection_id ftconicet
language English
topic MARS
EXOSPHERE
PICK UP
https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
spellingShingle MARS
EXOSPHERE
PICK UP
https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
Bertucci, Cesar
Romanelli, Norberto Julio
Chaufray, J. Y.
Gomez, Daniel Osvaldo
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 MARS
EXOSPHERE
PICK UP
https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
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. Fil: Bertucci, Cesar. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina Fil: Romanelli, Norberto Julio. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina Fil: Chaufray, J. Y. LATMOS; Francia Fil: Gomez, Daniel Osvaldo. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina Fil: Mazelle, C. IRAP; Francia ...
format Article in Journal/Newspaper
author Bertucci, Cesar
Romanelli, Norberto Julio
Chaufray, J. Y.
Gomez, Daniel Osvaldo
Mazelle, C.
Delva, M.
Modolo, R.
González Galindo, F.
Brain, D. A.
author_facet Bertucci, Cesar
Romanelli, Norberto Julio
Chaufray, J. Y.
Gomez, Daniel Osvaldo
Mazelle, C.
Delva, M.
Modolo, R.
González Galindo, F.
Brain, D. A.
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
publisher American Geophysical Union
url http://hdl.handle.net/11336/17062
long_lat ENVELOPE(-58.795,-58.795,-62.196,-62.196)
geographic Argentina
South Pole
Gomez
geographic_facet Argentina
South Pole
Gomez
genre South pole
genre_facet South pole
op_relation info:eu-repo/semantics/altIdentifier/url/onlinelibrary.wiley.com/doi/10.1002/grl.50709/full
info:eu-repo/semantics/altIdentifier/doi/10.1002/grl.50709
http://hdl.handle.net/11336/17062
Bertucci, Cesar; Romanelli, Norberto Julio; Chaufray, J. Y.; Gomez, Daniel Osvaldo; Mazelle, C.; et al.; Temporal variability of waves at the proton cyclotron frequency upstream from Mars: Implications for Mars distant hydrogen exosphere; American Geophysical Union; Geophysical Research Letters; 40; 15; 1-8-2013; 3809-3813
0094-8276
op_rights info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
op_doi https://doi.org/10.1002/grl.50709
container_title Geophysical Research Letters
container_volume 40
container_issue 15
container_start_page 3809
op_container_end_page 3813
_version_ 1779320273266278400