The Trouvelot astronomical drawings manualTrouvelot, E. L. (Etienne Leopold)
Science
The Trouvelot astronomical drawings manual
Trouvelot, E. L. (Etienne Leopold)
Astronomy -- Pictorial works
The auroral phenomena are also connected in some way with electricity,
and generate serious disturbances in the electric currents traversing
our telegraphic lines, which are thus often rendered useless for the
transmission of messages during great auroral displays. It sometimes
happens, however, during such displays, that the telegraphic lines can
be operated for a long distance, without the assistance of a battery;
the aurora, or at least its cause, furnishing the necessary electric
current for the working of the line. During auroras, the telephonic
lines are also greatly affected, and all kinds of noises and
crepitations are heard in the instruments.
Two observations of mine, which may have a bearing on the subject,
present some interest, as they seem to indicate the action of the aurora
on some of the clouds of our atmosphere. On January 6th, 1872, after I
had been observing a brilliant aurora for over one hour, an isolated
black cumulus cloud appeared at a little distance from the western
extremity of the dark auroral segment. This cloud, probably driven by
the wind, rapidly advanced eastward, and was soon followed by a
succession of similar clouds, all starting from the same point. All
these black clouds apparently followed the same path, which was not a
straight line, but parallel to and concentric with the border of the
dark auroral segment. When the first cloud arrived in the vicinity of
the magnetic meridian passing through the middle of the auroral arc, it
very rapidly dissolved, and on reaching this meridian became invisible.
The same phenomenon was observed with the succession of black clouds
following, each rapidly dissolving as it approached the magnetic
meridian. This phenomenon of black clouds vanishing like phantoms in
crossing the magnetic meridian, was observed for nearly an hour. On June
17th, 1879, I observed a similar phenomenon during a fine auroral
display. About midway between the horizon and the polar star, but a
little to the west of the magnetic meridian, there was a large black
cumulo-stratus cloud which very slowly advanced eastward. As it
progressed in that direction, its eastern extremity was dissolved in
traversing the magnetic meridian; while, at the same time, several short
and quite bright auroral rays issued from its western extremity, which
in its turn dissolved rapidly, as if burned or melted away in the
production of the auroral flame.
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