Anomalous frequency shifts in the solar system
| dc.creator | Moret-Bailly, Jacques | |
| dc.date | 2005-07-19 | |
| dc.date.accessioned | 2026-07-07T05:55:32Z | |
| dc.date.available | 2026-07-07T05:55:32Z | |
| dc.description | The improvements of the observations of the solar system allowed by the use of probes and big instruments let appear several problems: The frequencies of the radio signals received from the probes sent over 5 UA from the Sun are too high; the explanation by spicules or siphon-flows of the frequency shifts of UV emissions observed on the surface of the sun by SOHO is not satisfactory; the anisotropy of the CMB seems bound to the ecliptic. This problems are solved using a coherent optical effect, deduced from standard spectroscopy and easily observed with lasers. In a gas containing atomic hydrogen in states 2S and (or) 2P, transfers of energy between light beams, allowed by thermodynamics, produce the required frequency shifts or amplifications. | |
| dc.description | 9 pages 3 figures | |
| dc.identifier | https://arxiv.org/abs/physics/0507141 | |
| dc.identifier | http://arxiv.org/abs/physics/0507141 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/87271 | |
| dc.subject | General Physics | |
| dc.title | Anomalous frequency shifts in the solar system | |
| dc.type | text |