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The Forecast of Space Weather According to Ground-Based Observatories

Published online by Cambridge University Press:  24 July 2018

Andrey Tlatov
Andrey Tlatov*
Affiliation:
Kislovodsk mountain astronomical station of the Pulkovo observatory, 357700, Gagarina str. 100, Kislovodsk, Russia email: tlatov@mail.ru Kalmyk State University, Elista, Russia
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Abstract

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The space weather forecast can be conditionally divided into three components: 1) The forecast of recurrent slowly varying events which are associated with the topology of a large-scale magnetic field; 2) Evaluation of fluxes of ultraviolet and extreme radiation; 3) Detecting and determining the parameters of eruptions and CME. All three components can be observed and evaluated by ground-based telescopes. In this article we describe the telescopes of the space weather service in Kislovodsk Mountain Astronomical Station. Telescope-magnetograph STOP for the forecast of recurrent events and patrol telescopes-spectrographs for detecting CME and estimating hard radiation fluxes.

Keywords

Sunspace weatherground-based observation
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 13 , Symposium S335: Space Weather of the Heliosphere: Processes and Forecasts , July 2017 , pp. 362 - 364
Copyright
Copyright © International Astronomical Union 2018 

References

Tlatov, A. G., Dormidontov, D. V., Kirpichev, R. V., Pashchenko, M. P. & Shramko, A. D. 2015, Ge&Ae, 55, 961Google Scholar
Tlatov, A. G., Pashchenko, M. P., Ponyavin, D. I., Svidskii, P. M., Peshcherov, V. S. & Demidov, M. L. 2016, Ge&Ae, 56, 969Google Scholar