Ionospheric research 50 years ago, today and tomorrow

Fifty years ago the processes responsible for the formation of the ionospheric layers were well established, Appleton, Bartels and Chapman having been in the vanguard of the exploration phase of ionospheric research. Routine observations were being carried out in some locations, but in other areas,...

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Published in:Journal of Atmospheric and Solar-Terrestrial Physics
Main Authors: Rodger, A.S., Jarvis, M.J.
Format: Article in Journal/Newspaper
Language:unknown
Published: Elsevier 2000
Subjects:
Online Access:http://nora.nerc.ac.uk/id/eprint/502368/
https://doi.org/10.1016/S1364-6826(00)00116-4
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spelling ftnerc:oai:nora.nerc.ac.uk:502368 2023-05-15T13:48:07+02:00 Ionospheric research 50 years ago, today and tomorrow Rodger, A.S. Jarvis, M.J. 2000 http://nora.nerc.ac.uk/id/eprint/502368/ https://doi.org/10.1016/S1364-6826(00)00116-4 unknown Elsevier Rodger, A.S.; Jarvis, M.J. 2000 Ionospheric research 50 years ago, today and tomorrow. Journal of Atmospheric and Solar-Terrestrial Physics, 62 (17-18). 1629-1645. https://doi.org/10.1016/S1364-6826(00)00116-4 <https://doi.org/10.1016/S1364-6826(00)00116-4> Publication - Article PeerReviewed 2000 ftnerc https://doi.org/10.1016/S1364-6826(00)00116-4 2023-02-04T19:37:13Z Fifty years ago the processes responsible for the formation of the ionospheric layers were well established, Appleton, Bartels and Chapman having been in the vanguard of the exploration phase of ionospheric research. Routine observations were being carried out in some locations, but in other areas, such as Antarctica, the first measurements were only being undertaken. Thus, a global perspective of the ionosphere was still emerging. In the intervening years, there have been many very significant findings. Energy from the atmosphere both above and below the ionosphere has been shown to have a major influence its structure and dynamics. Winds up to 1 km s-1 blow at F-region altitudes and the solar wind imposes a cross-polar cap potential > 100 kV on the ionosphere when the interplanetary magnetic field has a strong southward component. The ionosphere itself is not simply a passive window on atmospheric and plasma processes. It is the major source of plasma for the magnetosphere, and its lower boundary is critical in the reflection of planetary waves back into the stratosphere and troposphere. Evolving technology has made a vast improvement in our ability to observe and model the ionosphere; some key developments are summarised. The paper also provides a few illustrations of the topics studied over the last 50 yr, namely F-region storms, plasma irregularities and long-term changes. Although the climatology of the ionosphere is well understood and can be modelled successfully, predicting the ionospheric weather accurately is not yet possible. The paper concludes by identifying some key topics where further understanding will be essential if reliable modelling and forecasting are to be achieved. Article in Journal/Newspaper Antarc* Antarctica Natural Environment Research Council: NERC Open Research Archive Journal of Atmospheric and Solar-Terrestrial Physics 62 17-18 1629 1645
institution Open Polar
collection Natural Environment Research Council: NERC Open Research Archive
op_collection_id ftnerc
language unknown
description Fifty years ago the processes responsible for the formation of the ionospheric layers were well established, Appleton, Bartels and Chapman having been in the vanguard of the exploration phase of ionospheric research. Routine observations were being carried out in some locations, but in other areas, such as Antarctica, the first measurements were only being undertaken. Thus, a global perspective of the ionosphere was still emerging. In the intervening years, there have been many very significant findings. Energy from the atmosphere both above and below the ionosphere has been shown to have a major influence its structure and dynamics. Winds up to 1 km s-1 blow at F-region altitudes and the solar wind imposes a cross-polar cap potential > 100 kV on the ionosphere when the interplanetary magnetic field has a strong southward component. The ionosphere itself is not simply a passive window on atmospheric and plasma processes. It is the major source of plasma for the magnetosphere, and its lower boundary is critical in the reflection of planetary waves back into the stratosphere and troposphere. Evolving technology has made a vast improvement in our ability to observe and model the ionosphere; some key developments are summarised. The paper also provides a few illustrations of the topics studied over the last 50 yr, namely F-region storms, plasma irregularities and long-term changes. Although the climatology of the ionosphere is well understood and can be modelled successfully, predicting the ionospheric weather accurately is not yet possible. The paper concludes by identifying some key topics where further understanding will be essential if reliable modelling and forecasting are to be achieved.
format Article in Journal/Newspaper
author Rodger, A.S.
Jarvis, M.J.
spellingShingle Rodger, A.S.
Jarvis, M.J.
Ionospheric research 50 years ago, today and tomorrow
author_facet Rodger, A.S.
Jarvis, M.J.
author_sort Rodger, A.S.
title Ionospheric research 50 years ago, today and tomorrow
title_short Ionospheric research 50 years ago, today and tomorrow
title_full Ionospheric research 50 years ago, today and tomorrow
title_fullStr Ionospheric research 50 years ago, today and tomorrow
title_full_unstemmed Ionospheric research 50 years ago, today and tomorrow
title_sort ionospheric research 50 years ago, today and tomorrow
publisher Elsevier
publishDate 2000
url http://nora.nerc.ac.uk/id/eprint/502368/
https://doi.org/10.1016/S1364-6826(00)00116-4
genre Antarc*
Antarctica
genre_facet Antarc*
Antarctica
op_relation Rodger, A.S.; Jarvis, M.J. 2000 Ionospheric research 50 years ago, today and tomorrow. Journal of Atmospheric and Solar-Terrestrial Physics, 62 (17-18). 1629-1645. https://doi.org/10.1016/S1364-6826(00)00116-4 <https://doi.org/10.1016/S1364-6826(00)00116-4>
op_doi https://doi.org/10.1016/S1364-6826(00)00116-4
container_title Journal of Atmospheric and Solar-Terrestrial Physics
container_volume 62
container_issue 17-18
container_start_page 1629
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