Science in Short ChaptersWilliams, W. Mattieu (William Mattieu)
Science
Science in Short Chapters
Williams, W. Mattieu (William Mattieu)
Science
A little reflection on the above-stated laws of dissociation will show
that the maximum violence of hydrogen explosion will not occur at the
birth of the ejections, but afterwards, when the dissociated gases
have been already hurled beyond the sphere of restraining vapors. If
my explanation is correct, the typical form of a solar prominence
should be that of a spreading tree with a tall stem. At first the least
resistence to radiation and consequent explosive combination must
be in the vertical direction, as this will afford the shortest line
that can be drawn through the thickness of the surrounding jacket of
resisting vapor; but when raised above this envelope, the dissociated
gases, cooled by their own expansion and comparatively free to radiate
in all directions except downwards, will explode laterally as well as
vertically, and thus spread out into a head. My theoretical prominence
will be, in short, a monster rocket proceeding steadily upwards to a
certain extent, and then gradually bursting and projecting its missiles
in every direction from the vertical to the absolutely horizontal.
Should the latter acquire a velocity of about 300 miles per second,
not merely a closed but even an absolutely circular orbit would be
possible. These and the multitude of weaker lateral ejections, reaching
the sun by short parabolic paths, explain the mystery of the inner
corona.
I need only refer Mr. Proctor to his own recently published book on
the Sun, where he will find on plates 4, 5, and 6 a number of drawings
from Zöllner and Respighi, which so thoroughly confirm my necessary
theoretical deductions that they might be a series of fancy sketches of
my own. When we consider that the base of a prominence is only visible
when it happens to start exactly from the limb of the sun, while the
vastly greater proportion of those which are observed, and have been
drawn, have much of the stem cut off from view by the solar rotundity,
the evidence afforded by such drawings in support of my theoretical
deduction, that the typical form of the solar prominences is that of a
palm-tree or bursting rocket, is greatly strengthened.[7]
Public-domain text, read in full here on John Shaqi.
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