NMDB and space weather forecasting

From the creation of NMDB in 2007 and through the growth in the number of stations and the data accumulation, the ShICRA SB RAS group continuously have used its facilities. For the last years we have created a method for short-term forecasting of intense geomagnetic storms with an advance time 1-2 d...

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Main Authors: Gololobov, Petr Yu., Starodubtsev, Sergey A., Grigoryev, Vladislav G., Zverev, Anton S.
Format: Book Part
Language:English
Published: 2023
Subjects:
Online Access:https://doi.org/10.38072/2748-3150/p33
https://nbn-resolving.org/urn:nbn:de:gbv:8:3-2023-00510-7
https://macau.uni-kiel.de/receive/macau_mods_00003832
https://macau.uni-kiel.de/servlets/MCRFileNodeServlet/macau_derivate_00005425/kiel-up_2748-3150_p33.pdf
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author Gololobov, Petr Yu.
Starodubtsev, Sergey A.
Grigoryev, Vladislav G.
Zverev, Anton S.
author_facet Gololobov, Petr Yu.
Starodubtsev, Sergey A.
Grigoryev, Vladislav G.
Zverev, Anton S.
author_sort Gololobov, Petr Yu.
collection MACAU: Open Access Repository of Kiel University
container_start_page 81
description From the creation of NMDB in 2007 and through the growth in the number of stations and the data accumulation, the ShICRA SB RAS group continuously have used its facilities. For the last years we have created a method for short-term forecasting of intense geomagnetic storms with an advance time 1-2 days. The probability of forecasting is around 80%. We have reported about the method in the previous NMDB: virtual symposium on cosmic ray studies with neutron detectors in 2020. The method is based on the global survey method that was developed in Yakutsk in 1960s and uses the world network of neutron monitors as a single multidirectional device. The method is intended to estimate hourly dynamics of cosmic ray anisotropy in free-space. Note that only with the NMDB creation we managed to implement it in real time mode. Now we started work on creating another method for space weather forecasting by measurements of cosmic ray fluctuations. For this purpose, we use 1-min data of NMDB. In the current report we present the first results of our investigation on forecasting of intense geomagnetic storms with Dst < -50 nT. The results obtained indicate the possibility of developing and implementing in real time a method for predicting strong geophysical manifestations of space weather on the basis of ground-based cosmic ray measurements.
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op_relation NMDB@Athens -- urn:nbn:de:gbv:8:3-2023-00486-0 -- 978-3-928794-99-2 -- 10.38072/2748-3150/v2 -- info:eu-repo/grantAgreement/EC/FP7/213007/EU/Real-Time database for high resolution Neutron Monitor measurements/NMDB -- W4388776508
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spelling ftunivkiel:oai:macau.uni-kiel.de:macau_mods_00003832 2025-01-17T01:19:42+00:00 NMDB and space weather forecasting Gololobov, Petr Yu. Starodubtsev, Sergey A. Grigoryev, Vladislav G. Zverev, Anton S. 2023-03-08 https://doi.org/10.38072/2748-3150/p33 https://nbn-resolving.org/urn:nbn:de:gbv:8:3-2023-00510-7 https://macau.uni-kiel.de/receive/macau_mods_00003832 https://macau.uni-kiel.de/servlets/MCRFileNodeServlet/macau_derivate_00005425/kiel-up_2748-3150_p33.pdf eng eng NMDB@Athens -- urn:nbn:de:gbv:8:3-2023-00486-0 -- 978-3-928794-99-2 -- 10.38072/2748-3150/v2 -- info:eu-repo/grantAgreement/EC/FP7/213007/EU/Real-Time database for high resolution Neutron Monitor measurements/NMDB -- W4388776508 https://creativecommons.org/licenses/by/4.0/ info:eu-repo/semantics/openAccess article Chapter ddc:530 ddc:600 cosmic rays neutron monitor magnetohydrodynamic waves fluctuations turbulence spectrum chapter Text doc-type:BookPart 2023 ftunivkiel https://doi.org/10.38072/2748-3150/p3310.38072/2748-3150/v2 2024-11-27T15:16:03Z From the creation of NMDB in 2007 and through the growth in the number of stations and the data accumulation, the ShICRA SB RAS group continuously have used its facilities. For the last years we have created a method for short-term forecasting of intense geomagnetic storms with an advance time 1-2 days. The probability of forecasting is around 80%. We have reported about the method in the previous NMDB: virtual symposium on cosmic ray studies with neutron detectors in 2020. The method is based on the global survey method that was developed in Yakutsk in 1960s and uses the world network of neutron monitors as a single multidirectional device. The method is intended to estimate hourly dynamics of cosmic ray anisotropy in free-space. Note that only with the NMDB creation we managed to implement it in real time mode. Now we started work on creating another method for space weather forecasting by measurements of cosmic ray fluctuations. For this purpose, we use 1-min data of NMDB. In the current report we present the first results of our investigation on forecasting of intense geomagnetic storms with Dst < -50 nT. The results obtained indicate the possibility of developing and implementing in real time a method for predicting strong geophysical manifestations of space weather on the basis of ground-based cosmic ray measurements. Book Part Yakutsk MACAU: Open Access Repository of Kiel University Yakutsk 81 87
spellingShingle article
Chapter
ddc:530
ddc:600
cosmic rays
neutron monitor
magnetohydrodynamic waves
fluctuations
turbulence spectrum
Gololobov, Petr Yu.
Starodubtsev, Sergey A.
Grigoryev, Vladislav G.
Zverev, Anton S.
NMDB and space weather forecasting
title NMDB and space weather forecasting
title_full NMDB and space weather forecasting
title_fullStr NMDB and space weather forecasting
title_full_unstemmed NMDB and space weather forecasting
title_short NMDB and space weather forecasting
title_sort nmdb and space weather forecasting
topic article
Chapter
ddc:530
ddc:600
cosmic rays
neutron monitor
magnetohydrodynamic waves
fluctuations
turbulence spectrum
topic_facet article
Chapter
ddc:530
ddc:600
cosmic rays
neutron monitor
magnetohydrodynamic waves
fluctuations
turbulence spectrum
url https://doi.org/10.38072/2748-3150/p33
https://nbn-resolving.org/urn:nbn:de:gbv:8:3-2023-00510-7
https://macau.uni-kiel.de/receive/macau_mods_00003832
https://macau.uni-kiel.de/servlets/MCRFileNodeServlet/macau_derivate_00005425/kiel-up_2748-3150_p33.pdf