Abstract
The Toronto spectrophotometer was used to take an extensive series of ozone measurements for the period September 1971 to April 1972. As a result of these measurements it was found that short-lived variations of ozone occur which sometimes amount to more than 0.1 cm. These ‘ozone disturbances’ are advected because the same disturbance has been observed on the direct sun and the zenith sky at different times. Results which show the general nature of these disturbances will be presented. Also, a discussion will be given which stresses the need for an automated, mesoscale ozone-measuring network, capable of measuring in all weather conditions during all daytime hours.
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