STELLAR ABERRATION FROM THE STANDPOINT OF THE RADIATION CONVECTION HYPOTHESIS

被引:4
作者
PHIPPS, TE
机构
关键词
STELLAR ABERRATION; RELATIVITY; NEO-HERTZIAN ELECTROMAGNETISM; RADIATION CONVECTION HYPOTHESIS;
D O I
10.4006/1.3028919
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
A previously advanced hypothesis of radiation convection by the absorber, deduced from the so-called neo-Hertzian electromagnetism, 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.
引用
收藏
页码:368 / 372
页数:5
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