The background absorption at high latitudes
The high latitude ionosphere is more often disturbed than quiet, i.e. fluxes of charged particles dominate over solar controlled ionisation. Nonetheless, the actual amount of the predictable, solar-controlled ionisation and the resulting absorption is of interest for some applications.
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| Format: | Article |
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Copernicus Publications
2003-01-01
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| Series: | Advances in Radio Science |
| Online Access: | http://www.adv-radio-sci.net/1/325/2003/ars-1-325-2003.pdf |
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doaj-600fe66e2cf848fabab730341b518eda2020-11-24T21:03:50ZdeuCopernicus PublicationsAdvances in Radio Science 1684-99651684-99732003-01-011325327The background absorption at high latitudesM. HarrichM. FriedrichS. R. MarpleK. M. TorkarThe high latitude ionosphere is more often disturbed than quiet, i.e. fluxes of charged particles dominate over solar controlled ionisation. Nonetheless, the actual amount of the predictable, solar-controlled ionisation and the resulting absorption is of interest for some applications.http://www.adv-radio-sci.net/1/325/2003/ars-1-325-2003.pdf |
| collection |
DOAJ |
| language |
deu |
| format |
Article |
| sources |
DOAJ |
| author |
M. Harrich M. Friedrich S. R. Marple K. M. Torkar |
| spellingShingle |
M. Harrich M. Friedrich S. R. Marple K. M. Torkar The background absorption at high latitudes Advances in Radio Science |
| author_facet |
M. Harrich M. Friedrich S. R. Marple K. M. Torkar |
| author_sort |
M. Harrich |
| title |
The background absorption at high latitudes |
| title_short |
The background absorption at high latitudes |
| title_full |
The background absorption at high latitudes |
| title_fullStr |
The background absorption at high latitudes |
| title_full_unstemmed |
The background absorption at high latitudes |
| title_sort |
background absorption at high latitudes |
| publisher |
Copernicus Publications |
| series |
Advances in Radio Science |
| issn |
1684-9965 1684-9973 |
| publishDate |
2003-01-01 |
| description |
The high latitude ionosphere is more often disturbed than quiet, i.e. fluxes of charged particles dominate over solar controlled ionisation. Nonetheless, the actual amount of the predictable, solar-controlled ionisation and the resulting absorption is of interest for some applications. |
| url |
http://www.adv-radio-sci.net/1/325/2003/ars-1-325-2003.pdf |
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AT mharrich thebackgroundabsorptionathighlatitudes AT mfriedrich thebackgroundabsorptionathighlatitudes AT srmarple thebackgroundabsorptionathighlatitudes AT kmtorkar thebackgroundabsorptionathighlatitudes AT mharrich backgroundabsorptionathighlatitudes AT mfriedrich backgroundabsorptionathighlatitudes AT srmarple backgroundabsorptionathighlatitudes AT kmtorkar backgroundabsorptionathighlatitudes |
| _version_ |
1716772856490098688 |