630504Eclipse5_p1

Click on the thumbnail at the bottom right of this page to go to the bitmap scan of this document. The text of this document appears immediately below.

                        ROYAL ASTRONOMICAL SOCIETY OF CANADA
                     Standing Committee on Observational Activities
                      Programme for Solar Eclispe of July 20, 1963

Bulletin No. 5                Basic Observation Programme           May 4, 1963
                            Section C. Visual Observations

    This section of the basic observation programme covers visual observations made
during the total phase either with the naked eye or with telescopic aiti and with the
emphasis on drawings or sketches, supplemented by verbal descriptions of detail seen.

Dark Adaptation. jt is common knowledge that our ability to see dim light is pro-
portional to the length of tame that the "rod" cells of the eye's retina remain
unstimulated. To see fine detail during the brief period of totality, the eye must
first become dark adapted, a process that takes at least twenty minutes. The gradual
darkening of the sky during the partial phase is not suflicient to produce the des-
ired effect, and the following methods of dark adaptation are suggested,

 (1) The observer is blindfolded during the approach of totality. This rather drastic
     measure deprives him of the thflll of seeing the sudden transition front partial
     to total phase when the corona sinnes forth in all its beauty True, he can
     watch the end of totality and the subsequent partial phase but it is not as
     spectacular as the approach.

 (2) The observer can wear dark red goggles during the approach of totality, for it
     has been fohd that the rods are practically unstimulated by the red end of
     the spectrum. This method aflows activity during the period of adaptation.
     Care must still be taken to provide adequate protection for the eyes when
     looking directly at the sun.

 (3) The observer can wear a black patch over his "observing" eye, watching the
     approach of totality with the other and removing the patch only after the
     beginning of totality. This method is particularly, sqitable for those making
     telescopic observations for most observer invariably use the same eye at the
     eyepiece. 

1. CORONA                                                      

     Regardless of the ztumbei of photographs taken, visual observations of the solar
corona will be useful, for the human eye, if properly dark adapted, can see fine
detail that is difficult to photograph without over-exposing other aretts. The
problem, of course, in making visual observations is to record faithfully the detail
that one sees - the shape and extent of the corona, the variations in intensity 
and to do this in a very limited period of time. The observer should not trust to
memory but should complete his drawing from actual observation tharing the period of
totality. This is a tall order and it is suggested that the observer practise before-
hand, making drawings frdth. pro jected Slides of the solar corona. For the sake of
uniformity it is suggested that a two inch circle represent the sun's disk. A verbal
description, recorded immediately after totality, should supplement the drawing.
As mentioned in Bulletin No. 4, at sun-spot minimum it is expected that the corona
will have long equatorial streamers and short polar plumes.  Observations can be
made with the naked eye or with a telescope. The report form should give details of
equipment used. The telescopic observer has the disadvantage that, since no filters
are used during totality, he must be ready to stop a few seconas before the end of
totality to avoid the possibility of injury to his eyes.