Editor's Foreword iii Acknowledgements iv

Incoherent Scatter spectra computed with a typical EISCAT observation of the ionosphere in the ~ 120- 500 km altitude range. The spectra shape varies with the altitude as function of the observed electron temperature and of the ion temperature and composition. The spectral power is scaled to the ele...

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Bibliographic Details
Main Authors: Denis Alcaydé, Tor Hagfors
Other Authors: The Pennsylvania State University CiteSeerX Archives
Format: Text
Language:English
Published: 1997
Subjects:
EISCAT
Online Access:http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.622.8846
http://e7.eiscat.se/groups/Documentation/CourseMaterials/1995Cargese/Cargese book (previous school lectures).pdf
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spelling ftciteseerx:oai:CiteSeerX.psu:10.1.1.622.8846 2023-05-15T16:04:28+02:00 Editor's Foreword iii Acknowledgements iv Denis Alcaydé Tor Hagfors The Pennsylvania State University CiteSeerX Archives 1997 application/pdf http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.622.8846 http://e7.eiscat.se/groups/Documentation/CourseMaterials/1995Cargese/Cargese book (previous school lectures).pdf en eng http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.622.8846 http://e7.eiscat.se/groups/Documentation/CourseMaterials/1995Cargese/Cargese book (previous school lectures).pdf Metadata may be used without restrictions as long as the oai identifier remains attached to it. http://e7.eiscat.se/groups/Documentation/CourseMaterials/1995Cargese/Cargese book (previous school lectures).pdf text 1997 ftciteseerx 2016-01-08T15:05:28Z Incoherent Scatter spectra computed with a typical EISCAT observation of the ionosphere in the ~ 120- 500 km altitude range. The spectra shape varies with the altitude as function of the observed electron temperature and of the ion temperature and composition. The spectral power is scaled to the electron density and the spectra are Text EISCAT Unknown
institution Open Polar
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language English
description Incoherent Scatter spectra computed with a typical EISCAT observation of the ionosphere in the ~ 120- 500 km altitude range. The spectra shape varies with the altitude as function of the observed electron temperature and of the ion temperature and composition. The spectral power is scaled to the electron density and the spectra are
author2 The Pennsylvania State University CiteSeerX Archives
format Text
author Denis Alcaydé
Tor Hagfors
spellingShingle Denis Alcaydé
Tor Hagfors
Editor's Foreword iii Acknowledgements iv
author_facet Denis Alcaydé
Tor Hagfors
author_sort Denis Alcaydé
title Editor's Foreword iii Acknowledgements iv
title_short Editor's Foreword iii Acknowledgements iv
title_full Editor's Foreword iii Acknowledgements iv
title_fullStr Editor's Foreword iii Acknowledgements iv
title_full_unstemmed Editor's Foreword iii Acknowledgements iv
title_sort editor's foreword iii acknowledgements iv
publishDate 1997
url http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.622.8846
http://e7.eiscat.se/groups/Documentation/CourseMaterials/1995Cargese/Cargese book (previous school lectures).pdf
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genre_facet EISCAT
op_source http://e7.eiscat.se/groups/Documentation/CourseMaterials/1995Cargese/Cargese book (previous school lectures).pdf
op_relation http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.622.8846
http://e7.eiscat.se/groups/Documentation/CourseMaterials/1995Cargese/Cargese book (previous school lectures).pdf
op_rights Metadata may be used without restrictions as long as the oai identifier remains attached to it.
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