Telescope for recording coronal mass ejections SPOT-CME
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Abstract
We present a project of the new patrol telescope for regular solar observations with a cadence of about one minute. The instrument is intended to detect and determine parameters of coronal mass ejections and solar flares. It allows one to observe velocity fields in both the solar atmosphere and coronal ejections. The telescope is designed based on an air-proof single-volume scheme, may be mounted without a pavilion, and operates as a robotic telescope. It can be used within the Solar Service network.
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The work was supported by the Ministry of Education and Science of the Russian Federation under state assignment No. 075-03-2026-375.
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References
Berezin I.A., Tlatov A.G., Pevtsov A.A., 2023. Astrophys. J., vol. 950, no. 2, p. 100.
Tlatov A.G., Shramko A.D., Chernov Y.O., Strelkov M.A., Naga Varun E., 2017. Geomagnetism and Aeronomy, vol. 57, no. 7, pp. 854–858.