Difference between revisions of "Stellar Aberration from the Standpoint of the Radiation Convection Hypothesis"
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| − | A previously advanced hypothesis of radiation convection by the absorber, deduced from the so-called neo-Hertzian electomagnetism, is tested for its ability to account for the facts of stellar aberration. The test is passed at first order. Satellite astronomy may in the future offer some hope of observationally distinguishing this theory from special relativity.[[Category:Scientific Paper]] | + | A previously advanced hypothesis of radiation convection by the absorber, deduced from the so-called neo-Hertzian electomagnetism, is tested for its ability to account for the facts of stellar aberration. The test is passed at first order. Satellite astronomy may in the future offer some hope of observationally distinguishing this theory from special relativity. |
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| + | [[Category:Scientific Paper|stellar aberration standpoint radiation convection hypothesis]] | ||
[[Category:Relativity]] | [[Category:Relativity]] | ||
Revision as of 11:06, 1 January 2017
| Scientific Paper | |
|---|---|
| Title | Stellar Aberration from the Standpoint of the Radiation Convection Hypothesis |
| Author(s) | Thomas E Phipps |
| Keywords | Stellar Aberration, Radiation Convection |
| Published | 1991 |
| Journal | Physics Essays |
| Volume | 5 |
| Number | 3 |
| Pages | 368-372 |
Abstract
A previously advanced hypothesis of radiation convection by the absorber, deduced from the so-called neo-Hertzian electomagnetism, is tested for its ability to account for the facts of stellar aberration. The test is passed at first order. Satellite astronomy may in the future offer some hope of observationally distinguishing this theory from special relativity.
