Introduction to Solar Radio Astronomy and Radio Physics:
Gespeichert in:
| 1. Verfasser: | |
|---|---|
| Format: | Elektronisch E-Book |
| Sprache: | English |
| Veröffentlicht: |
Dordrecht
Springer Netherlands
1979
|
| Schriftenreihe: | Geophysics and Astrophysics Monographs, An International Series of Fundamental Textbooks
16 |
| Schlagworte: | |
| Online-Zugang: | Volltext |
| Beschreibung: | 1. 1. Short History of Solar Radio Astronomy Since its birth in the forties of our century, solar radio astronomy has grown into an extensive scientific branch comprising a number of quite different topics covering technical sciences, astrophysics, plasma physics, solar-terrestrial physics, and other disciplines. Historically, the story of radio astronomy goes back to the times of James Clerk Maxwell, whose well known phenomenological electromagnetic field equations have become the basis of present-time radio physics. As a direct consequence of these equations, Maxwell was able to prognosticate the existence of radio waves which fifteen years later were experimentally detected by the famous work of Heinrich Hertz (1887/88). However, all attempts to detect radio waves from cosmic objects failed until 1932, which was mainly due to the early stage of development of receiving techniques and the as yet missing knowledge of the existence of a screening ionosphere (which was detected in 1925). Therefore, famous inventors like Thomas Edison and A. E. Kennelly, as well as Sir Oliver Lodge, were unsuccessful in receiving any radio emission from the Sun or other extraterrestrial sources. Another hindering point was that nobody could a priori expect that solar radio emission should have something to do with solar activity so that unfortunately by chance some experiments were carried out just at periods of low solar activity. This was also why Karl Guthe Jansky at the birth of radio astronomy detected galactic radio waves but no emission from the Sun |
| Beschreibung: | 1 Online-Ressource (XVIII, 332 p) |
| ISBN: | 9789400994027 9789027709974 |
| DOI: | 10.1007/978-94-009-9402-7 |
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Datensatz im Suchindex
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| dewey-full | 523.01 |
| dewey-hundreds | 500 - Natural sciences and mathematics |
| dewey-ones | 523 - Specific celestial bodies and phenomena |
| dewey-raw | 523.01 |
| dewey-search | 523.01 |
| dewey-sort | 3523.01 |
| dewey-tens | 520 - Astronomy and allied sciences |
| discipline | Physik |
| doi_str_mv | 10.1007/978-94-009-9402-7 |
| format | Electronic eBook |
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| isbn | 9789400994027 9789027709974 |
| language | English |
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| spelling | Krüger, A. Verfasser aut Introduction to Solar Radio Astronomy and Radio Physics by A. Krüger Dordrecht Springer Netherlands 1979 1 Online-Ressource (XVIII, 332 p) txt rdacontent c rdamedia cr rdacarrier Geophysics and Astrophysics Monographs, An International Series of Fundamental Textbooks 16 1. 1. Short History of Solar Radio Astronomy Since its birth in the forties of our century, solar radio astronomy has grown into an extensive scientific branch comprising a number of quite different topics covering technical sciences, astrophysics, plasma physics, solar-terrestrial physics, and other disciplines. Historically, the story of radio astronomy goes back to the times of James Clerk Maxwell, whose well known phenomenological electromagnetic field equations have become the basis of present-time radio physics. As a direct consequence of these equations, Maxwell was able to prognosticate the existence of radio waves which fifteen years later were experimentally detected by the famous work of Heinrich Hertz (1887/88). However, all attempts to detect radio waves from cosmic objects failed until 1932, which was mainly due to the early stage of development of receiving techniques and the as yet missing knowledge of the existence of a screening ionosphere (which was detected in 1925). Therefore, famous inventors like Thomas Edison and A. E. Kennelly, as well as Sir Oliver Lodge, were unsuccessful in receiving any radio emission from the Sun or other extraterrestrial sources. Another hindering point was that nobody could a priori expect that solar radio emission should have something to do with solar activity so that unfortunately by chance some experiments were carried out just at periods of low solar activity. This was also why Karl Guthe Jansky at the birth of radio astronomy detected galactic radio waves but no emission from the Sun Physics Astrophysics and Astroparticles Radioastronomie (DE-588)4048200-5 gnd rswk-swf Sonne (DE-588)1236963652 gnd rswk-swf Radioastronomie (DE-588)4048200-5 s Sonne (DE-588)1236963652 g 1\p DE-604 https://doi.org/10.1007/978-94-009-9402-7 Verlag Volltext 1\p cgwrk 20201028 DE-101 https://d-nb.info/provenance/plan#cgwrk |
| spellingShingle | Krüger, A. Introduction to Solar Radio Astronomy and Radio Physics Physics Astrophysics and Astroparticles Radioastronomie (DE-588)4048200-5 gnd |
| subject_GND | (DE-588)4048200-5 (DE-588)1236963652 |
| title | Introduction to Solar Radio Astronomy and Radio Physics |
| title_auth | Introduction to Solar Radio Astronomy and Radio Physics |
| title_exact_search | Introduction to Solar Radio Astronomy and Radio Physics |
| title_full | Introduction to Solar Radio Astronomy and Radio Physics by A. Krüger |
| title_fullStr | Introduction to Solar Radio Astronomy and Radio Physics by A. Krüger |
| title_full_unstemmed | Introduction to Solar Radio Astronomy and Radio Physics by A. Krüger |
| title_short | Introduction to Solar Radio Astronomy and Radio Physics |
| title_sort | introduction to solar radio astronomy and radio physics |
| topic | Physics Astrophysics and Astroparticles Radioastronomie (DE-588)4048200-5 gnd |
| topic_facet | Physics Astrophysics and Astroparticles Radioastronomie Sonne |
| url | https://doi.org/10.1007/978-94-009-9402-7 |
| work_keys_str_mv | AT krugera introductiontosolarradioastronomyandradiophysics |