Auroræ: Their Characters and SpectraCapron, J. Rand
History
Auroræ: Their Characters and Spectra
Capron, J. Rand
Auroras
As an addition to the instances of Tycho, Picard, &c., mentioned in the
note on p. 73, Mr. Pratt has also sent me his notes of some observations
by him, of “local obscuration of the floor of Plato.” As somewhat
condensed, they are as follows:—1872, July 16. While in other parts of
the floor spots and streaks were well visible, “the N.W. portion was
in such a hazy condition that nothing could be defined upon it.” 1873,
Nov. 1. 27 light streaks seen (7 new): the brightness of the streaks was
in excess of their usual character, as compared with the craterlets;
“an _obliteration_ or _invisibility_ of _all_ the light streaks in the
neighbourhood of craterlet no. 1 was very noticeable;” and also “a
similar obliteration of the N. end of the streak called the Sector, near
craterlet 3.” 1874, January 1. 18 light streaks seen, including 3 new,
“some of which outshone other longer known ones. This was curious; for
had they been as bright within the last two years as on this occasion
I must have noticed them.” Mr. Pratt points out, as worthy of remark,
that some months previous to November 1st, 1873, neither craterlets
nor streaks on the floor of Plato “had maintained their previous
characteristic brightness,”—a fact which he thinks ought to be considered
together with the outbreak of brilliancy of both orders on that day, as
well as the apparently sudden existence of new ones.
[Sidenote: Observation by Mr. Hirst of a dark shade on the moon.]
The ‘Observatory,’ March 1, 1879, p. 375, contains an account, by Mr. H.
C. Russell, of some Astronomical Experiments made on the Blue Mountains,
near Sydney, N. S. W. Among these it is noticed that on 21st October,
1878, at 9 A.M., when looking at the moon, Mr. Hirst found that a large
part of it was covered with a dark shade, quite as dark as the shadow
of the earth during an eclipse of the moon. Its outline was generally
circular, and fainter near the edges. Conspicuous bright lunar objects
could be seen through it; but it quite obliterated the view of about half
the moon’s terminator, while those parts of the terminator not in the
shadow were distinctly seen.
No change in the position of the shade could be detected after three
hours’ watching. The observation is made, “One could hardly resist the
conviction that it was a shadow; yet it could not be the shadow of any
known body. If produced by a comet, it must be one of more than ordinary
density, although dark bodies have been seen crossing the sun which were
doubtless comets.” The diameter of the shadow from the part of it seen on
the moon was estimated at about three quarters that of the moon[11].
CHAPTER VIII.
AURORA AND THE SOLAR CORONA.
[Sidenote: Aurora and the solar corona. Mr. Norman Lockyer’s ‘Solar
Physics.’]
Public-domain text, read in full here on John Shaqi.
Reviews
Reviews
No reviews yet
Be the first to share your thoughts on this work.
Elsewhere in the archive
Join the Discussion
Join the discussion
Sign in to leave a comment or review.
Sign InorCreate an account