Electron density and temperature measurements in the cold plasma environment of Titan: Implications for atmospheric escape
- Autores
- Edberg, N. J. T.; Wahlund, J. E.; Ågren, K.; Morooka, M. W.; Modolo, R.; Bertucci, Cesar; Dougherty, M. K.
- Año de publicación
- 2010
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- We present electron temperature and density measurements of Titan's cold ionospheric plasma from the Langmuir probe instrument on Cassini from 52 flybys. An expression of the density as a function of temperature is presented for altitudes below two Titan radii. The density falls off exponentially with increased temperature as log(ne) = −2.0log(Te) + 0.6 on average around Titan. We show that this relation varies with location around Titan as well as with the solar illumination direction. Significant heating of the electrons appears to take place on the night/wake side of Titan as the density-temperature relation is less steep there. Furthermore, we show that the magnetospheric ram pressure is not balanced by the thermal and magnetic pressure in the topside ionosphere and discuss its implications for plasma escape. The cold ionospheric plasma of Titan extends to higher altitudes in the wake region, indicating the loss of atmosphere down the induced magnetospheric tail.
Fil: Edberg, N. J. T.. Swedish Institute of Space Physics; Suecia
Fil: Wahlund, J. E.. Swedish Institute of Space Physics; Suecia
Fil: Ågren, K.. Swedish Institute of Space Physics; Suecia
Fil: Morooka, M. W.. Swedish Institute of Space Physics; Suecia
Fil: Modolo, R.. LATMOS; Francia
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: Dougherty, M. K.. Imperial College London; Reino Unido - Materia
-
Ionosphere: Ionosphere/magnetosphere interactions
Ionosphere: Planetary ionospheres
Ionosphere: Plasma temperature and density
Magnetospheric Physics: Magnetosphere interactions with satellites and rings - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/20445
Ver los metadatos del registro completo
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Electron density and temperature measurements in the cold plasma environment of Titan: Implications for atmospheric escapeEdberg, N. J. T.Wahlund, J. E.Ågren, K.Morooka, M. W.Modolo, R.Bertucci, CesarDougherty, M. K.Ionosphere: Ionosphere/magnetosphere interactionsIonosphere: Planetary ionospheresIonosphere: Plasma temperature and densityMagnetospheric Physics: Magnetosphere interactions with satellites and ringshttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We present electron temperature and density measurements of Titan's cold ionospheric plasma from the Langmuir probe instrument on Cassini from 52 flybys. An expression of the density as a function of temperature is presented for altitudes below two Titan radii. The density falls off exponentially with increased temperature as log(ne) = −2.0log(Te) + 0.6 on average around Titan. We show that this relation varies with location around Titan as well as with the solar illumination direction. Significant heating of the electrons appears to take place on the night/wake side of Titan as the density-temperature relation is less steep there. Furthermore, we show that the magnetospheric ram pressure is not balanced by the thermal and magnetic pressure in the topside ionosphere and discuss its implications for plasma escape. The cold ionospheric plasma of Titan extends to higher altitudes in the wake region, indicating the loss of atmosphere down the induced magnetospheric tail.Fil: Edberg, N. J. T.. Swedish Institute of Space Physics; SueciaFil: Wahlund, J. E.. Swedish Institute of Space Physics; SueciaFil: Ågren, K.. Swedish Institute of Space Physics; SueciaFil: Morooka, M. W.. Swedish Institute of Space Physics; SueciaFil: Modolo, R.. LATMOS; FranciaFil: 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; ArgentinaFil: Dougherty, M. K.. Imperial College London; Reino UnidoAmerican Geophysical Union2010-10info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/20445Edberg, N. J. T.; Wahlund, J. E.; Ågren, K.; Morooka, M. W.; Modolo, R.; et al.; Electron density and temperature measurements in the cold plasma environment of Titan: Implications for atmospheric escape; American Geophysical Union; Geophysical Research Letters; 37; L20105; 10-2010; 1-50094-8276CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1029/2010GL044544info:eu-repo/semantics/altIdentifier/url/http://onlinelibrary.wiley.com/doi/10.1029/2010GL044544/abstractinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:41:27Zoai:ri.conicet.gov.ar:11336/20445instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-29 10:41:27.589CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
Electron density and temperature measurements in the cold plasma environment of Titan: Implications for atmospheric escape |
title |
Electron density and temperature measurements in the cold plasma environment of Titan: Implications for atmospheric escape |
spellingShingle |
Electron density and temperature measurements in the cold plasma environment of Titan: Implications for atmospheric escape Edberg, N. J. T. Ionosphere: Ionosphere/magnetosphere interactions Ionosphere: Planetary ionospheres Ionosphere: Plasma temperature and density Magnetospheric Physics: Magnetosphere interactions with satellites and rings |
title_short |
Electron density and temperature measurements in the cold plasma environment of Titan: Implications for atmospheric escape |
title_full |
Electron density and temperature measurements in the cold plasma environment of Titan: Implications for atmospheric escape |
title_fullStr |
Electron density and temperature measurements in the cold plasma environment of Titan: Implications for atmospheric escape |
title_full_unstemmed |
Electron density and temperature measurements in the cold plasma environment of Titan: Implications for atmospheric escape |
title_sort |
Electron density and temperature measurements in the cold plasma environment of Titan: Implications for atmospheric escape |
dc.creator.none.fl_str_mv |
Edberg, N. J. T. Wahlund, J. E. Ågren, K. Morooka, M. W. Modolo, R. Bertucci, Cesar Dougherty, M. K. |
author |
Edberg, N. J. T. |
author_facet |
Edberg, N. J. T. Wahlund, J. E. Ågren, K. Morooka, M. W. Modolo, R. Bertucci, Cesar Dougherty, M. K. |
author_role |
author |
author2 |
Wahlund, J. E. Ågren, K. Morooka, M. W. Modolo, R. Bertucci, Cesar Dougherty, M. K. |
author2_role |
author author author author author author |
dc.subject.none.fl_str_mv |
Ionosphere: Ionosphere/magnetosphere interactions Ionosphere: Planetary ionospheres Ionosphere: Plasma temperature and density Magnetospheric Physics: Magnetosphere interactions with satellites and rings |
topic |
Ionosphere: Ionosphere/magnetosphere interactions Ionosphere: Planetary ionospheres Ionosphere: Plasma temperature and density Magnetospheric Physics: Magnetosphere interactions with satellites and rings |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
We present electron temperature and density measurements of Titan's cold ionospheric plasma from the Langmuir probe instrument on Cassini from 52 flybys. An expression of the density as a function of temperature is presented for altitudes below two Titan radii. The density falls off exponentially with increased temperature as log(ne) = −2.0log(Te) + 0.6 on average around Titan. We show that this relation varies with location around Titan as well as with the solar illumination direction. Significant heating of the electrons appears to take place on the night/wake side of Titan as the density-temperature relation is less steep there. Furthermore, we show that the magnetospheric ram pressure is not balanced by the thermal and magnetic pressure in the topside ionosphere and discuss its implications for plasma escape. The cold ionospheric plasma of Titan extends to higher altitudes in the wake region, indicating the loss of atmosphere down the induced magnetospheric tail. Fil: Edberg, N. J. T.. Swedish Institute of Space Physics; Suecia Fil: Wahlund, J. E.. Swedish Institute of Space Physics; Suecia Fil: Ågren, K.. Swedish Institute of Space Physics; Suecia Fil: Morooka, M. W.. Swedish Institute of Space Physics; Suecia Fil: Modolo, R.. LATMOS; Francia 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: Dougherty, M. K.. Imperial College London; Reino Unido |
description |
We present electron temperature and density measurements of Titan's cold ionospheric plasma from the Langmuir probe instrument on Cassini from 52 flybys. An expression of the density as a function of temperature is presented for altitudes below two Titan radii. The density falls off exponentially with increased temperature as log(ne) = −2.0log(Te) + 0.6 on average around Titan. We show that this relation varies with location around Titan as well as with the solar illumination direction. Significant heating of the electrons appears to take place on the night/wake side of Titan as the density-temperature relation is less steep there. Furthermore, we show that the magnetospheric ram pressure is not balanced by the thermal and magnetic pressure in the topside ionosphere and discuss its implications for plasma escape. The cold ionospheric plasma of Titan extends to higher altitudes in the wake region, indicating the loss of atmosphere down the induced magnetospheric tail. |
publishDate |
2010 |
dc.date.none.fl_str_mv |
2010-10 |
dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
format |
article |
status_str |
publishedVersion |
dc.identifier.none.fl_str_mv |
http://hdl.handle.net/11336/20445 Edberg, N. J. T.; Wahlund, J. E.; Ågren, K.; Morooka, M. W.; Modolo, R.; et al.; Electron density and temperature measurements in the cold plasma environment of Titan: Implications for atmospheric escape; American Geophysical Union; Geophysical Research Letters; 37; L20105; 10-2010; 1-5 0094-8276 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/20445 |
identifier_str_mv |
Edberg, N. J. T.; Wahlund, J. E.; Ågren, K.; Morooka, M. W.; Modolo, R.; et al.; Electron density and temperature measurements in the cold plasma environment of Titan: Implications for atmospheric escape; American Geophysical Union; Geophysical Research Letters; 37; L20105; 10-2010; 1-5 0094-8276 CONICET Digital CONICET |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/doi/10.1029/2010GL044544 info:eu-repo/semantics/altIdentifier/url/http://onlinelibrary.wiley.com/doi/10.1029/2010GL044544/abstract |
dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
eu_rights_str_mv |
openAccess |
rights_invalid_str_mv |
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
dc.format.none.fl_str_mv |
application/pdf application/pdf |
dc.publisher.none.fl_str_mv |
American Geophysical Union |
publisher.none.fl_str_mv |
American Geophysical Union |
dc.source.none.fl_str_mv |
reponame:CONICET Digital (CONICET) instname:Consejo Nacional de Investigaciones Científicas y Técnicas |
reponame_str |
CONICET Digital (CONICET) |
collection |
CONICET Digital (CONICET) |
instname_str |
Consejo Nacional de Investigaciones Científicas y Técnicas |
repository.name.fl_str_mv |
CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas |
repository.mail.fl_str_mv |
dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar |
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1844614445533233152 |
score |
13.070432 |