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| Content Provider | Springer Nature Link |
|---|---|
| Author | Efimov, A. I. Lukanina, L. A. Rogashkova, A. I. Samoznaev, L. N. Chashei, I. V. Bird, M. K. Paetzold, M. |
| Copyright Year | 2015 |
| Abstract | Fluctuations in the Faraday rotation of the plane of polarization of S-band (2.3 GHz) radio signals transmitted through the solar corona by the HELIOS-1 AND HELIOS-2 space probes are analyzed. Simultaneous measurements of the Faraday-rotation fluctuations at the Goldstone and Canberra stations have yielded estimates of the velocity of perturbations of the magnetic field in the circumsolar plasma at heliocentric distances of three to six solar radii. The velocity of these perturbations is a combination of the Alfvén and solar-wind speeds. Temporal spectra of the Faraday-rotation fluctuations are obtained based on a large volume of observational data obtained in various years in four cycles of radio-sounding experiments. Filtration of the input data using spectral, correlation, and wavelet analyses shows that trains of quasi-periodic oscillations of the magnetic field with various amplitudes and periods from 2 to 160 min are regularly present in the Faraday-rotation fluctuations. This quasi-periodic character of these perturbations supports their connection with Alfvén waves propagating in the circumsolar plasma. |
| Starting Page | 313 |
| Ending Page | 326 |
| Page Count | 14 |
| File Format | |
| ISSN | 10637729 |
| Journal | Astronomy Reports |
| Volume Number | 59 |
| Issue Number | 4 |
| e-ISSN | 15626881 |
| Language | English |
| Publisher | Pleiades Publishing |
| Publisher Date | 2015-04-15 |
| Publisher Place | Moscow |
| Access Restriction | One Nation One Subscription (ONOS) |
| Subject Keyword | Astronomy, Observations and Techniques |
| Content Type | Text |
| Resource Type | Article |
| Subject | Astronomy and Astrophysics Space and Planetary Science |
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