- PII
- S30346460S0367676525060057-1
- DOI
- 10.7868/S3034646025060057
- Publication type
- Article
- Status
- Published
- Authors
- Volume/ Edition
- Volume 80 / Issue number 6
- Pages
- 863-868
- Abstract
- A method for determining a complex operational predictor of space weather disturbance is proposed. The calculations are based on different types of time series: solar activity in the radio and gamma bands, solar wind energy, variations in the flux of cosmic rays according to the data of the world network of neutron monitors and the multidirectional muon hodoscope. The technique has been tested in the analysis of a powerful geomagnetic disturbance (Dst = −412 nT). The sequence of predictors was obtained in "real" time ranging from 2–3 days to several hours.
- Keywords
- солнечная активность космическая погода фликкер-шумовая спектроскопия космические лучи комплексный предиктор
- Date of publication
- 01.06.2025
- Year of publication
- 2025
- Number of purchasers
- 0
- Views
- 39
References
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