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Pregled bibliografske jedinice broj: 1253008

Geomagnetic storm forecasting from solar coronal holes


Nitti, Simona; Podladchikova, Tatiana; Hofmeister, Stefan; Veronig, Astrid; Verbanac, Giuliana; Bandić, Mario
Geomagnetic storm forecasting from solar coronal holes // Monthly notices of the Royal Astronomical Society, 519 (2023), 2; 3182-3193 doi:10.1007/s11207-022-02086-2 (međunarodna recenzija, članak, znanstveni)


CROSBI ID: 1253008 Za ispravke kontaktirajte CROSBI podršku putem web obrasca

Naslov
Geomagnetic storm forecasting from solar coronal holes

Autori
Nitti, Simona ; Podladchikova, Tatiana ; Hofmeister, Stefan ; Veronig, Astrid ; Verbanac, Giuliana ; Bandić, Mario

Izvornik
Monthly notices of the Royal Astronomical Society (0035-8711) 519 (2023), 2; 3182-3193

Vrsta, podvrsta i kategorija rada
Radovi u časopisima, članak, znanstveni

Ključne riječi
Sun corona ; Sun magnetic fields ; Sun solar wind ; Sun solar-terrestrial relations ; magnetic reconnection ; methods: data analysis

Sažetak
Coronal holes (CHs) are the source of high-speed streams (HSSs) in the solar wind, whose interaction with the slow solar wind creates corotating interaction regions (CIRs) in the heliosphere. Whenever the CIRs hit the Earth, they can cause geomagnetic storms. We develop a method to predict the strength of CIR/HSS-driven geomagnetic storms directly from solar observations using the CH areas and associated magnetic field polarity. First, we build a data set comprising the properties of CHs on the Sun, the associated HSSs, CIRs, and orientation of the interplanetary magnetic field (IMF) at L1, and the strength of the associated geomagnetic storms by the geomagnetic indices Dst and Kp. Then, we predict the Dst and Kp indices using a Gaussian process model, which accounts for the annual variation of the orientation of Earth’s magnetic field axis. We demonstrate that the polarity of the IMF at L1 associated with CIRs is preserved in around 83 per cent of cases when compared to the polarity of their CH sources. Testing our model o v er the period 2010–2020, we obtained a correlation coefficient between the predicted and observed Dst index of R = 0.63/0.73, and Kp index of R = 0.65/0.67, for HSSs having a polarity tow ards/aw ay from the Sun. These findings demonstrate the possibility of predicting CIR/HSS-driven geomagnetic storms directly from solar observations and extending the forecasting lead time up to several days, which is relevant for enhancing space weather predictions.

Izvorni jezik
Engleski

Znanstvena područja
Fizika, Geofizika



POVEZANOST RADA


Ustanove:
Prirodoslovno-matematički fakultet, Zagreb

Profili:

Avatar Url Giuliana Verbanac (autor)

Poveznice na cjeloviti tekst rada:

doi

Citiraj ovu publikaciju:

Nitti, Simona; Podladchikova, Tatiana; Hofmeister, Stefan; Veronig, Astrid; Verbanac, Giuliana; Bandić, Mario
Geomagnetic storm forecasting from solar coronal holes // Monthly notices of the Royal Astronomical Society, 519 (2023), 2; 3182-3193 doi:10.1007/s11207-022-02086-2 (međunarodna recenzija, članak, znanstveni)
Nitti, S., Podladchikova, T., Hofmeister, S., Veronig, A., Verbanac, G. & Bandić, M. (2023) Geomagnetic storm forecasting from solar coronal holes. Monthly notices of the Royal Astronomical Society, 519 (2), 3182-3193 doi:10.1007/s11207-022-02086-2.
@article{article, author = {Nitti, Simona and Podladchikova, Tatiana and Hofmeister, Stefan and Veronig, Astrid and Verbanac, Giuliana and Bandi\'{c}, Mario}, year = {2023}, pages = {3182-3193}, DOI = {10.1007/s11207-022-02086-2}, keywords = {Sun corona, Sun magnetic fields, Sun solar wind, Sun solar-terrestrial relations, magnetic reconnection, methods: data analysis}, journal = {Monthly notices of the Royal Astronomical Society}, doi = {10.1007/s11207-022-02086-2}, volume = {519}, number = {2}, issn = {0035-8711}, title = {Geomagnetic storm forecasting from solar coronal holes}, keyword = {Sun corona, Sun magnetic fields, Sun solar wind, Sun solar-terrestrial relations, magnetic reconnection, methods: data analysis} }
@article{article, author = {Nitti, Simona and Podladchikova, Tatiana and Hofmeister, Stefan and Veronig, Astrid and Verbanac, Giuliana and Bandi\'{c}, Mario}, year = {2023}, pages = {3182-3193}, DOI = {10.1007/s11207-022-02086-2}, keywords = {Sun corona, Sun magnetic fields, Sun solar wind, Sun solar-terrestrial relations, magnetic reconnection, methods: data analysis}, journal = {Monthly notices of the Royal Astronomical Society}, doi = {10.1007/s11207-022-02086-2}, volume = {519}, number = {2}, issn = {0035-8711}, title = {Geomagnetic storm forecasting from solar coronal holes}, keyword = {Sun corona, Sun magnetic fields, Sun solar wind, Sun solar-terrestrial relations, magnetic reconnection, methods: data analysis} }

Časopis indeksira:


  • Current Contents Connect (CCC)
  • Web of Science Core Collection (WoSCC)
    • Science Citation Index Expanded (SCI-EXP)
    • SCI-EXP, SSCI i/ili A&HCI
  • Scopus


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