Intermediate degree solar oscillations
Spectra of solar intensity oscillations in the degree range ℓ = 20–98 were obtained with a 92% duty cycle over a 50 hour period from the geographic South Pole. After correction for solar rotation, the spectra have been averaged over azimuthal order m and fit with Lorentzian functions to provide valu...
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Language: | English |
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Cambridge University Press (CUP)
1988
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Online Access: | http://dx.doi.org/10.1017/s0074180900157687 https://www.cambridge.org/core/services/aop-cambridge-core/content/view/S0074180900157687 |
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crcambridgeupr:10.1017/s0074180900157687 2024-03-03T08:48:50+00:00 Intermediate degree solar oscillations Duvall, T. L. Harvey, J. W. Pomerantz, M. A. 1988 http://dx.doi.org/10.1017/s0074180900157687 https://www.cambridge.org/core/services/aop-cambridge-core/content/view/S0074180900157687 en eng Cambridge University Press (CUP) https://www.cambridge.org/core/terms Symposium - International Astronomical Union volume 123, page 37-40 ISSN 0074-1809 journal-article 1988 crcambridgeupr https://doi.org/10.1017/s0074180900157687 2024-02-08T08:32:34Z Spectra of solar intensity oscillations in the degree range ℓ = 20–98 were obtained with a 92% duty cycle over a 50 hour period from the geographic South Pole. After correction for solar rotation, the spectra have been averaged over azimuthal order m and fit with Lorentzian functions to provide values of background noise, amplitude, frequency and line width for 636 oscillation modes. The background noise is nearly independent of frequency in the range containing strong p-modes. The amplitude envelope shows little dependence on ℓ value and a frequency dependence similar to that of Doppler oscillations but shifted to higher frequency. Line widths increase at higher frequency and at higher ℓ values. Article in Journal/Newspaper South pole Cambridge University Press South Pole Symposium - International Astronomical Union 123 37 40 |
institution |
Open Polar |
collection |
Cambridge University Press |
op_collection_id |
crcambridgeupr |
language |
English |
description |
Spectra of solar intensity oscillations in the degree range ℓ = 20–98 were obtained with a 92% duty cycle over a 50 hour period from the geographic South Pole. After correction for solar rotation, the spectra have been averaged over azimuthal order m and fit with Lorentzian functions to provide values of background noise, amplitude, frequency and line width for 636 oscillation modes. The background noise is nearly independent of frequency in the range containing strong p-modes. The amplitude envelope shows little dependence on ℓ value and a frequency dependence similar to that of Doppler oscillations but shifted to higher frequency. Line widths increase at higher frequency and at higher ℓ values. |
format |
Article in Journal/Newspaper |
author |
Duvall, T. L. Harvey, J. W. Pomerantz, M. A. |
spellingShingle |
Duvall, T. L. Harvey, J. W. Pomerantz, M. A. Intermediate degree solar oscillations |
author_facet |
Duvall, T. L. Harvey, J. W. Pomerantz, M. A. |
author_sort |
Duvall, T. L. |
title |
Intermediate degree solar oscillations |
title_short |
Intermediate degree solar oscillations |
title_full |
Intermediate degree solar oscillations |
title_fullStr |
Intermediate degree solar oscillations |
title_full_unstemmed |
Intermediate degree solar oscillations |
title_sort |
intermediate degree solar oscillations |
publisher |
Cambridge University Press (CUP) |
publishDate |
1988 |
url |
http://dx.doi.org/10.1017/s0074180900157687 https://www.cambridge.org/core/services/aop-cambridge-core/content/view/S0074180900157687 |
geographic |
South Pole |
geographic_facet |
South Pole |
genre |
South pole |
genre_facet |
South pole |
op_source |
Symposium - International Astronomical Union volume 123, page 37-40 ISSN 0074-1809 |
op_rights |
https://www.cambridge.org/core/terms |
op_doi |
https://doi.org/10.1017/s0074180900157687 |
container_title |
Symposium - International Astronomical Union |
container_volume |
123 |
container_start_page |
37 |
op_container_end_page |
40 |
_version_ |
1792505849802915840 |