Conservation of Solar Energy

Details Conservation of Solar Energy Conservation of Solar Energy

Mar 1882

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1882natur..25..504a&link_type=abstract

Nature, Volume 25, Issue 648, pp. 504 (1882).

Physics

Scientific paper

WHILE Dr. Siemens' novel and ingenious theory described in his paper before the Royal Society, and published in NATURE, will doubtless be adequately criticised in its more physical aspects by those who are better acquainted than myself with ``the intricacies of solar physics,'' I may perhaps be allowed to point out one or two conclusions which appear somewhat opposed to the laws of mechanics. The author, for example, lays great stress upon the ``high rotative velocity of the sun,'' which at the solar equator, according to his figures, is four and a half times that at the terrestrial equator. To this ``high rotative velocity'' Dr. Siemens attributes the supposed expulsion from the solar equator of the products of combustion of the gases drawn in by the assumed fan-action at the solar poles.

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