THE ROYAL ASTRONOMICAL SOCIETY OF CANADA
STANDING COMMITTEE ON OBSERVATIONAL ACTIVITIES
AURORA SECTION Bulletin No.3
The Starting Committee on Observational Activities is interested in expanding the present
visual survey of aurora borealis (northern lights) in the skies over Canada. Many in-
dividual members of the R.A.S.C. are currently reporting their observations of aurora to
their Centres and to the National Research Council Aurora Survey. Two Centres, Edmonton
and Montreal, have been carrying out extensive visual studies of the aurora for many years.
Other programmes of aurora reporting are known to exist in the Calgary and Halifax Centres.
More recently sane members of the Hamilton Centre have expressed an interest in beginning
a study of aurora.
At present, the sun-spat activity is at a minimum as a new eleven-year cycle begins. At
any given station in the mid-latitudes, the number of auroras occurring can be shown to
follow the solar cycle. As the number of sun-spots increases, so does the number of
For the benefit of those amateur astronomers not familiar with the appearance of the
aurora, some characteristics will be briefly outlined:
BRIGHTNESS: Aurora vary in brightness from WEAK (comparable with the Milky Way) to
BRIGHT (that of a moonlit cumulus cloud). The majority of aurora seen are
classified as MEDIUM (with brightness resembling a moonlit cirrus cloud).
COLOUR: Auroras are usually coloured yellow green; the intensity of colour depends
on the brightness, the brighter the display the more colour observed. In
the brightest displays, reddish or violet hues may shown as well as the yellow
green, and should be noted.
FORM: Sometimes the aurora appears as a faint GLOW near the northern horizon
resembling the dawn, except in colour. Cirrus clouds near the northern
horizon, if illuminated by city lights or moonlight, will tend to be more
reddish in colour and thus are easily distinguished from aurora.
Generally higher in the northern sky a HOMOGENEOUS ARC may appear as a thin
band of light with a diffuse upper edge and a sharply defined lower edge.
Several such arcs may occur at one time with sane joining at the ends. A
homogeneous arc may increase in brightness and break into a RATED ARC. For
long rays, this may resemble a drapery or curtain hanging from overhead
points in the sky.
In active displays of aurora, several rayed arcs may appear parallel to One
another. Waves of motion along the form may develop in such displays,
folding and unfolding as these waves move along the length of arc. The
brightest part of the arc may drift slowly or rapidly east or west, or
alternate in direction rapidly.
Bundles or patches of isolated RAYS accompany many displays or aurora,
resembling a searchlight beam in a dusty atmosphere and mixed in with other
AURORA Section, Bulletin No.3 -2-
OBSERVING THE AURORA
New observers should gain experience by searching the sky for aurora whenever taking part
in outdoor astronomical observing. Presence or absence of aurora, area of the sky
covered, brightness, and colour, will form the basis of your initial reports. The torus
of aurora can be classified with more experience. Eventually, the elevations of the
forms of aurora in the sky can be measured along the magnetic meridian.
For recording aurora, the sky has been divided into four quadrants. The most important
quadrant for your observations is the one centred on your north and extending from NW to
NE at the horizon up to the zenith (Figure 2). Each quadrant has been divided into
three zones, frau 0 to 30° elevation, 30° to 60°, and fran 60° to the zenith. In
reporting, you should note the quadrant and zones containing glows, lower borders of arcs
and ends of isolated rays ù An illustration of this procedure is shown in figures 1 and 2.
TIME OF OBSERVATION
Observations should be made approximately on the hour whenever no aurora is in the sky or
whenever only quiet forms such as the glow or a faint homogeneous arc are present. How-
ever, when an arc begins to show sane signs of becoming active (greatly increased bright-
ness or the appearance of motion or rays) the display should then be observed half hourly.
It is important that observations be collected from many locations to chart completely
the course of an auroral display. Thus a single report of the presence or absence of
aurora from Winnipeg may fill a gap left by a Regina observer not able to make an
observation. Even if you can not report regularly, your occasional reports will be
most helpful. Contribute as much data on the report form as your experience allows.
If a report originating in London states that aurora occurred low in the north between
20 hours (8 PM) and 23 hours (11 PM) on March 10/11, 1965, this may confirm another ob-
servation from north Toronto where sane uncertainty existed about the observation.
Upon request, the Auroral Centre, National Research Council, Ottawa 2, Ontario, will
forward to interested observers a supply of report forms, mailing envelopes and a complete
set of observing instructions.
I am anxious to contact representatives of local Centres concerning the accumulation of
duplicate copies of visual aurora reports so that an independent R.A.S.C. survey can be
made over the next eleven-year sun-spot cycle.
Earl Milton, National Co-ordinator,
2 Spence Street, Apt. 12,
September 1965. REGINA, Saskatchewan.
Tuesday, August 4, 2015 - 9:33pm
Aurora Section Bulletin No. 3