Statistics of Joule heating in the auroral zone and polar cap using Astrid-2 satellite Poynting flux
We make a statistical study of ionospheric Joule heating with the Poynting flux method using six months of Astrid-2/EMMA electric and magnetic field data during 1999 (solar maximum year). For the background magnetic field we use the IGRF model. Our results are in agreement with earlier statistic...
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2004-12-01
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Series: | Annales Geophysicae |
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doaj-0dd4ac1d32b94459a3390578e51fd82b2020-11-24T23:31:39ZengCopernicus PublicationsAnnales Geophysicae0992-76891432-05762004-12-01224133414210.5194/angeo-22-4133-2004Statistics of Joule heating in the auroral zone and polar cap using Astrid-2 satellite Poynting fluxA. Olsson0P. Janhunen1T. Karlsson2N. Ivchenko3L. G. Blomberg4Swedish Institute of Space Physics, Uppsala, SwedenFinnish Meteorological Institute, Space Research, Helsinki, FinlandAlfvén Laboratory, Royal Institute of Techology, Stockholm, SwedenAlfvén Laboratory, Royal Institute of Techology, Stockholm, SwedenAlfvén Laboratory, Royal Institute of Techology, Stockholm, SwedenWe make a statistical study of ionospheric Joule heating with the Poynting flux method using six months of Astrid-2/EMMA electric and magnetic field data during 1999 (solar maximum year). For the background magnetic field we use the IGRF model. Our results are in agreement with earlier statistical satellite studies using both the Σ<i><sub>P</sub>E</i><sup>2</sup> method and the Poynting flux method. We present a rather comprehensive set of fitted Joule heating formulas expressing the Joule heating in given magnetic local time (MLT) and invariant latitude (ILAT) range under given solar illumination conditions as a function of the <i>K<sub>p</sub></i> index, the <i>AE</i> index, the Akasofu epsilon parameter and the solar wind kinetic energy flux. The study thus provides improved and more detailed estimates of the statistical Joule heating. Such estimates are necessary building blocks for future quantitative studies of the power budget in the magnetosphere and in the nightside auroral region.<br><br> <b>Key words.</b> Ionosphere (electric fields and currents; ionosphere-magnetosphere interactions) – Magnetospheric physics (magnetospheric configuration and dynamics)https://www.ann-geophys.net/22/4133/2004/angeo-22-4133-2004.pdf |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
A. Olsson P. Janhunen T. Karlsson N. Ivchenko L. G. Blomberg |
spellingShingle |
A. Olsson P. Janhunen T. Karlsson N. Ivchenko L. G. Blomberg Statistics of Joule heating in the auroral zone and polar cap using Astrid-2 satellite Poynting flux Annales Geophysicae |
author_facet |
A. Olsson P. Janhunen T. Karlsson N. Ivchenko L. G. Blomberg |
author_sort |
A. Olsson |
title |
Statistics of Joule heating in the auroral zone and polar cap using Astrid-2 satellite Poynting flux |
title_short |
Statistics of Joule heating in the auroral zone and polar cap using Astrid-2 satellite Poynting flux |
title_full |
Statistics of Joule heating in the auroral zone and polar cap using Astrid-2 satellite Poynting flux |
title_fullStr |
Statistics of Joule heating in the auroral zone and polar cap using Astrid-2 satellite Poynting flux |
title_full_unstemmed |
Statistics of Joule heating in the auroral zone and polar cap using Astrid-2 satellite Poynting flux |
title_sort |
statistics of joule heating in the auroral zone and polar cap using astrid-2 satellite poynting flux |
publisher |
Copernicus Publications |
series |
Annales Geophysicae |
issn |
0992-7689 1432-0576 |
publishDate |
2004-12-01 |
description |
We make a statistical study of ionospheric Joule heating with the
Poynting flux method using six months of Astrid-2/EMMA electric and
magnetic field data during 1999 (solar maximum year). For the
background magnetic field we use the IGRF model. Our results are in
agreement with earlier statistical satellite studies using both the
Σ<i><sub>P</sub>E</i><sup>2</sup> method and the Poynting flux method. We present a
rather comprehensive set of fitted Joule heating formulas expressing
the Joule heating in given magnetic local time (MLT) and invariant
latitude (ILAT) range under given solar illumination conditions as a
function of the <i>K<sub>p</sub></i> index, the <i>AE</i> index, the Akasofu epsilon parameter
and the solar wind kinetic energy flux. The study thus provides
improved and more detailed estimates of the statistical Joule
heating. Such estimates are necessary building blocks for future
quantitative studies of the power budget in the magnetosphere and in
the nightside auroral region.<br><br>
<b>Key words.</b> Ionosphere (electric fields and currents;
ionosphere-magnetosphere interactions) – Magnetospheric
physics (magnetospheric configuration and dynamics) |
url |
https://www.ann-geophys.net/22/4133/2004/angeo-22-4133-2004.pdf |
work_keys_str_mv |
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