Auroræ: Their Characters and SpectraCapron, J. Rand
History
Auroræ: Their Characters and Spectra
Capron, J. Rand
Auroras
See whether indications of great auroral activity are associated with the
widening or increased brilliancy of any of the auroral lines.
Remember that if auroral displays are due to gaseous particles thrown
into vibration of electric disturbance, increased electric tension
may either (1) dissociate those particles and thus give rise to a new
spectrum, the one previously observed becoming dimmer; or (2) throw the
particles into more intense vibration without dissociation, and thus give
rise to new lines, those previously observed becoming brighter.
Careful records of auroral phenomena from both ships may enable the
height of some, observed from both, to be determined. It will be very
important that those the heights of which are determined by such means
should be carefully observed by the spectroscope, in order to observe
whether certain characteristics of the spectrum can be associated with
the height of the Aurora.
APPENDIX C.
EXTRACTS FROM PARLIAMENTARY BLUE BOOK, CONTAINING THE “RESULTS DERIVED
FROM THE ARCTIC EXPEDITION 1875-76.” (Eyre and Spottiswoode, 1878.)
_Auroras observed 1875-1876, at Floebery Beach and Discovery Bay._
_By Lieutenant A. C. PARR, R.N._
Though the auroral glow was often present, and served in some degree to
lighten the darkness of the sky during the long winter, when the moon was
absent, the actual appearances of the Aurora itself were few, and the
nimbus worthy of any particular remark extremely small. Those which were
stationary assumed the form of low arches, with streamers flashing up to
them from the horizon, and usually to the eastward. But the more common
form was for an arch to appear low down in some part of the sky where the
glow was brightest; at first it was very faint and narrow, but as it rose
gradually in the heavens it would increase both in size and intensity,
till on arriving near the zenith, with its ends extending nearly to the
horizon, it would be about the breadth of three or four rainbows, and its
colour that of white fleecy clouds lit up by the rays of the full moon.
On reaching this point, however, its course was nearly run; for after
appearing to remain stationary, as little white gaps would suddenly rend
the arch asunder, the portions thus detached seemed to roll together and
concentrate all their brightness in the smaller space, and then gradually
fade away and become extinct. Sometimes a very pale green would show
itself in the more luminous patches, and once or twice there was a slight
suspicion of red; but never was the whole sky illuminated by streams
running in all directions, and forming coronæ, while these colours varied
every moment.
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