Atmospheric excitation of polar motion: Comparison of the polar motion spectrum with spectra of effective atmospheric angular momentum functions
Creators
- 1. Ceskoslovenska Akademie Ved, Prague. Astronomicky Ustav
- 2. Belgrade Univ. (Yugoslavia)
Description
The spectra of different combinations of the effective atmospheric angular momentum functions determined by the National Meteorological Center of the USA were compared with the spectrum of polar motion, determined from a combination of all available data by the Bureau International de l'Heure in Paris. The spectra were obtained by the method of fast Fourier transform. To compare the amplitudes and phases, the transfer function derived for an Earth model with a fluid core, visco-elastic mantle and linearily reacting ocean was used. It was found for the dominating annual term that the influence of the wind component is substantially smaller than would show the data sampled at midnight UT but still significant. The combination of the resting wind term with the pressure term corrected for the inverted barometer is however, not sufficient to fully explain the observed polar motion with an annual period. It is shown that the difference in phase can very probably be completely attributed to the influence of ground water storage changes at this frequency. (author). 9 fig., 2 tabs., 38 refs
Additional details
Publishing Information
- Journal Title
- Bulletin of the Astronomical Institutes of Czechoslovakia
- Journal Volume
- 39
- Journal Issue
- 3
- Series
- Bull. Astron. Inst. Czech.
- Journal Page Range
- 172-185
- ISSN
- 0004-6248
- CODEN
- BAICA
INIS
- Country of Publication
- Czech Republic
- Country of Input or Organization
- Serbia and Montenegro
- INIS RN
- 20024597
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- ANGULAR MOMENTUM; EARTH ATMOSPHERE; EARTH PLANET; ROTATION; SPECTRA
- Descriptors DEC
- PLANETS