Science in Short ChaptersWilliams, W. Mattieu (William Mattieu)
Science
Science in Short Chapters
Williams, W. Mattieu (William Mattieu)
Science
My present business, however, is to show how these vortices and
eruptions—this down-rush in one part of the solar atmosphere and
up-rush in another—contribute to the permanent maintenance of the
solar light and heat. It must be understood that these outbursts are
only visible to us as luminous prominences during the period of their
explosive outburst, and while still subject to great expansive tension.
Long after they have ceased to be visible to us their expansion must
continue, until they finally and fully mingle with the medium into
which they are flung, and attain a corresponding degree of rarefaction.
This must occur at tens and hundreds of thousands of miles above
the photosphere, according to the magnitude of the ejection. The
spectroscopic researches of Frankland and Lockyer having shown that
the atmospheric pressure at about the outer surface of the photosphere
does not far exceed that of our atmosphere, I may safely regard all
the upper portion of these solar ejections as having left the solar
atmosphere proper, and become commingled with the general interstellar
medium.
If the sun were stationary, or merely rotating, in the midst of this
universal atmosphere, the same material that is ejected to-day would
in the course of time return, and be whirled into the great sun-spot
eddies; but such is not the case; the sun is driving through the ether
with a velocity of about 450,000 miles per twenty four hours.
What must be the consequence of this motion? The sun will carry its own
special atmospheric matter with it; but it cannot thus carry the whole
of the interstellar medium. There must be a limit, graduated no doubt,
but still a practical limit, at which its own atmosphere will leave
behind, or pass through, the general atmospheric matter. There must be
a heaping or condensation of this matter in the front, a rarefaction or
wake in the rear, and a continuous bow of newly encountered atmosphere
around the boundaries in the opposite direction to that of the sun’s
motion. The result of this must be that a great portion of the ejected
atmospheric matter of the prominences will be swept permanently to
the rear, and its place supplied by the material occupying the space
into which the sun is advancing. We are thus presented with a mighty
machinery of solar respiration; some of this newly arriving atmospheric
matter must be stirred into the vortices, its quantity being exactly
equivalent to that of the old material expired by the explosive
eruptions, and left in the rear.
Public-domain text, read in full here on John Shaqi.
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