Miscellanea Curiosa, Vol. 1: Containing a collection of some of the principal phaenomena in nature, accounted for by the greatest philosophers of this age
History
Miscellanea Curiosa, Vol. 1: Containing a collection of some of the principal phaenomena in nature, accounted for by the greatest philosophers of this age
Natural history; Science -- Early works to 1800; Voyages and travels -- Early works to 1800
There having lately arisen some Discourse about that part of the Heat of
Weather, simply produced by the Action of the Sun; and I having
affirmed, that if that were considered, as the only Cause of the Heat of
the Weather, I saw no Reason, but that under the Pole the solstitical
Day ought to be as hot as it is under the Æquinoctial, when the Sun
comes vertical, or over the Zenith: For this Reason, that for all the 24
Hours of that Day under the Pole, the Sun's Beams are inclined to the
Horizon, with an Angle of 23½ Degrees; and under the Æquinoctial,
though he come vertical, yet he shines no more than 12 Hours, and is
again 12 Hours absent; and that for 3 Hours 8 Minutes of that 12 Hours,
he is not so much elevated as under the Pole; so that he is not 9 of the
whole 24, higher than 'tis there, and is 15 Hours lower. Now the simple
Action of the Sun is, as all other Impulses or Stroaks, more or less
forceable, according to the _Sinus_ of the Angle of Incidence, or to the
Perpendicular let fall on the Plain, whence the vertical Ray (being that
of the greatest Heat,) being put _Radius_, the force of the Sun on the
Horizontal Surface of the Earth will be to that, as the _Sinus_ of the
Sun's Altitude at any other time. This being allow'd for true, it will
then follow, that the time of the continuance of the Sun's shining being
taken for a _Basis_, and the _Sines_ of the Sun's Altitudes erected
thereon as Perpendiculars, and a Curve drawn through the Extremities of
those Perpendiculars, the _Area_ comprehended shall be proportionate to
the Collection of the Heat of all the Beams of the Sun in that space of
time. Hence it will follow, that under the Pole the Collection of all
the Heat of a tropical Day, is proportionate to a Rectangle of the
_Sine_ of 23½ _gr._ into 24 Hours, or the Circumference of a Circle;
that is, the _Sine_ of 23½ _gr._ being nearly 4 Tenths of _Radius_;
as 3/10 into 12 Hours. Or the Polar Heat is equal to that of the Sun
containing 12 Hours above the Horizon, at 53 _gr._ height, than which
the Sun is not 5 Hours more elevated under the Æquinoctial.
Public-domain text, read in full here on John Shaqi.
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