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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Main Authors: A. Olsson, P. Janhunen, T. Karlsson, N. Ivchenko, L. G. Blomberg
Format: Article
Language:English
Published: Copernicus Publications 2004-12-01
Series:Annales Geophysicae
Online Access:https://www.ann-geophys.net/22/4133/2004/angeo-22-4133-2004.pdf
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spelling 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
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