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  5. Halo Coronal Mass Ejections during Solar Cycle 24: reconstruction of the global scenario and geoeffectiveness
 

Halo Coronal Mass Ejections during Solar Cycle 24: reconstruction of the global scenario and geoeffectiveness

Journal
JOURNAL OF SPACE WEATHER AND SPACE CLIMATE  
Date Issued
2018
Author(s)
Scolini, Camilla
•
MESSEROTTI, Mauro  
•
Poedts, Stefaan
•
Rodriguez, Luciano
DOI
10.1051/swsc/2017046
Abstract
In this study we present a statistical analysis of 53 fast Earth-directed halo CMEs observed by the SOHO/LASCO instrument during the period Jan. 2009-Sep. 2015, and we use this CME sample to test the capabilities of a Sun-to-Earth prediction scheme for CME geoeffectiveness. First, we investigate the CME association with other solar activity features by means of multi-instrument observations of the solar magnetic and plasma properties. Second, using coronagraphic images to derive the CME kinematical properties at 0.1 AU, we propagate the events to 1 AU by means of the WSA-ENLIL+Cone model. Simulation results at Earth are compared with in-situ observations at L1. By applying the pressure balance condition at the magnetopause and a solar wind-Kp index coupling function, we estimate the expected magnetospheric compression and geomagnetic activity level, and compare them with global data records. The analysis indicates that 82% of the CMEs arrived at Earth in the next 4 days. Almost the totality of them compressed the magnetopause below geosynchronous orbits and triggered a geomagnetic storm. Complex sunspot-rich active regions associated with energetic flares result the most favourable configurations from which geoeffective CMEs originate. The analysis of related SEP events shows that 74% of the CMEs associated with major SEPs were geoeffective. Moreover, the SEP production is enhanced in the case of fast and interacting CMEs. In this work we present a first attempt at applying a Sun-to-Earth geoeffectiveness prediction scheme - based on 3D simulations and solar wind-geomagnetic activity coupling functions - to a statistical set of potentially geoeffective halo CMEs. The results of the prediction scheme are in good agreement with geomagnetic activity data records, although further studies performing a fine-tuning of such scheme are needed.

Volume
8
Uri
http://hdl.handle.net/20.500.12386/30812
Url
https://www.swsc-journal.org/articles/swsc/full_html/2018/01/swsc170032/swsc170032.html
Issn Identifier
2115-7251
Ads BibCode
2018JSWSC...8A...9S
Rights
open.access
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swsc170032.pdf

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Pdf editoriale
Size

1.9 MB

Format

Adobe PDF

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bdb5bbcdbaedfd8ed4c7ecffbe69673f

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