White Light Flare & Dynamic Sun Challenges
Two challenges were set during the Solar Section Meeting in 2023 February:
– White light flares. With more complex sunspot group expected to appear over the next few years, the chances of X and M type flares appearing are higher, some of which may also appear in white light as well as in Hydrogen Alpha (Hα). Thus, observers are encouraged to observe in white light if they see a bright Hα flare. Observations of any white light flares should be sent to the Director Lyn Smith.
– Capturing the Dynamic Sun. This is to encourage the observation of how solar features change over time. In white light, the appearance of sunspots groups can change from day to day while in Hα features can also change from day to day but also over hours or even minutes. This challenge is to run from 2023 May to 2023 September with submitted drawings or images being included in this page, the Section Newsletter and in the Journal.
Examples of the dynamic sun are shown below (most recent at the bottom of the page):













































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