Results of 20-year solar observations in the He I λ 1083 nm line at the Crimean Astrophysical Observatory

Main Article Content

Olga Andreeva
Valentina Malashchuk

Abstract

During 1999–2018, an extensive dataset of images of the solar disk in the He I λ 1083 nm line was acquired at the Crimean Astrophysical Observatory (CrAO) with the Solar Tower Telescope – 2 (STT-2). Over this period, the image processing underwent various changes. No observations were carried out from mid-2018 to the end of 2019. In 2020, the process of observations and image processing at the telescope was modernized. Currently, all images acquired during different periods prior to modernization are being processed using a unified method to form a catalog. This work presents a brief historical overview of observations in the He I λ 1083 nm line at CrAO, a concise description, and fragments from the catalog.

Keywords: CrAO, solar telescope, observations in the He I λ 1083 nm line, coronal holes

Article Details

Section

Magnetism and activity of the Sun and stars – 2021 Conference proceedings

How to Cite

Andreeva O., Malashchuk V., 2024. Acta Astrophysica Taurica, vol. 5, no. 2, pp. 21–24. Available at: https://astrophysicatauricum.org/index.php/aat/article/view/82 (Accessed: 22 March 2026)

References

Malashchuk V.M., Andreeva O.A, 2019. Astron. Astrophys. Trans., vol. 31, no. 2, pp. 217–236.

Stepanian N.N. et al., 2000. Izv. Krymsk. Astrofiz. Observ., vol. 96, p. 194. (In Russ.)

Stepanian N., Sunitsa G., Malashchuk V., 2014. Bull. Crimean Astrophys. Observ., vol. 110, no. 1, pp. 149–160.