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| Content Provider | IEEE Xplore Digital Library |
|---|---|
| Author | Moret-Bailly, J. |
| Copyright Year | 2006 |
| Abstract | Summary form only given. The periodicity of redshifts z=0.062 (or its multiple 0.62) was observed by Tifft and other authors, in particular it generates the Lyman forest of the quasars. The whole spectrum of the quasars is obtained supposing that a micro-quasar is surrounded by a cloud of hydrogen it accretes. The very redshifted emission lines are produced in a very close, hot region where hydrogen is fully dissociated in protons and electrons. On the path to the Earth, a sufficient pressure, at 100 000 K, produces excited atomic hydrogen which shifts the emission lines. At a lower temperature, and a pressure of the order of 100 Pa, run and stop phases may produce strong, broad emission and absorption lines. But, a strong radio emission from the kernel ionizes fully the hydrogen, so that, in the radio-loud quasars, all images of a line are superposed. Finally, the periodicity generates the Lyman forest. The lines become sharper and sharper while the mean absorption decreases because the lifetime of excited hydrogen increases with the decrease of the pressure. The excited hydrogen which surrounds the quasars may redshift the light of object observed close to them, named "very red objects". Halton Arp observed quasars which seem ejected from a galaxy. The quasars are more redshifted than the galaxy because they produce by Lyman pumping more excited hydrogen close than far. Pioneer 10 and 11 probes seem having an anomalous acceleration beyond 5 UA because their radio signals have too high a frequency. It appears that the radio emissions are strongly perturbed if they cross the corona and some other regions, but they recover the continuity after: the propagation of the wave plays a role. As there is only the solar wind on the path of the light, something happens in the solar wind beyond 5 UA. A transfer of energy from the solar light blueshifts the radio waves where, beyond 5 UA, the cooling of the solar wind generates H*. The same blueshift produces the anisotropy of the CMB bound to the ecliptic |
| Sponsorship | Plasma Sci. and Applications Comm. IEEE Nuclear and Plasma Sci. Soc |
| Starting Page | 264 |
| Ending Page | 264 |
| File Size | 243733 |
| Page Count | 1 |
| File Format | |
| ISBN | 1424401259 |
| DOI | 10.1109/PLASMA.2006.1707136 |
| Language | English |
| Publisher | Institute of Electrical and Electronics Engineers, Inc. (IEEE) |
| Publisher Date | 2006-06-04 |
| Publisher Place | USA |
| Access Restriction | Subscribed |
| Rights Holder | Institute of Electrical and Electronics Engineers, Inc. (IEEE) |
| Subject Keyword | Optical propagation Atomic beams Hydrogen Astrophysics Electromagnetic wave absorption Wind energy generation Clouds Protons Electron emission Earth |
| Content Type | Text |
| Resource Type | Article |
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