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Correlation between CME and Flare Parameters (with and without Type II Bursts)


Shanmugaraju, A.; Moon, Yong-Jae; Vršnak, Bojan
Correlation between CME and Flare Parameters (with and without Type II Bursts) // Solar physics, 270 (2011), 273-284 doi:10.1007/s11207-011-9752-3 (međunarodna recenzija, članak, znanstveni)


Naslov
Correlation between CME and Flare Parameters (with and without Type II Bursts)

Autori
Shanmugaraju, A. ; Moon, Yong-Jae ; Vršnak, Bojan

Izvornik
Solar physics (0038-0938) 270 (2011); 273-284

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

Ključne riječi
coronal mass ejections; flares

Sažetak
CMEs and flares are the two energetic phenomena on the Sun responsible for generating shocks. Our main aim is to study the relation between the physical properties of CMEs and flares associated with and without type II radio bursts.We considered a set of 290 SOHO/LASCO CMEs associated with GOES X-ray flares observed during the period from January 1997 to December 2000. The relationship between the flares and CMEs is examined for the two sets i) with metric-type IIs and ii) without metric-type IIs. Physical properties such as rise time, duration, and strength of the flares and width, speed, and acceleration of CMEs are considered. We examined the energy relationship and temporal relationship between the CMEs and flares. First, all the events in each group were considered, and then the limb events in each group were considered separately. While there is a relationship between the temporal characteristics of flares and CME properties in the case of with-type IIs, it is absent in the case of all without-type IIs. Among all the relations studied, the correlation between flare duration and CME properties is found to be highly significant compared to the other relations. Also, the relationship between flare strength and CME speed found in the with-type II events is absent in the case of all without-type II events. However, when the limb without-type II events (with reduced time window between flare and CME) are studied separately, we found the energy relationship and the temporal relationship.

Izvorni jezik
Engleski

Znanstvena područja
Fizika



POVEZANOST RADA


Projekt / tema
007-0000000-1362 - Eruptivni procesi u Sunčevoj atmosferi (Bojan Vršnak, )

Ustanove
Geodetski fakultet, Zagreb

Profili:

Avatar Url Bojan Vršnak (autor)

Citiraj ovu publikaciju

Shanmugaraju, A.; Moon, Yong-Jae; Vršnak, Bojan
Correlation between CME and Flare Parameters (with and without Type II Bursts) // Solar physics, 270 (2011), 273-284 doi:10.1007/s11207-011-9752-3 (međunarodna recenzija, članak, znanstveni)
Shanmugaraju, A., Moon, Y. & Vršnak, B. (2011) Correlation between CME and Flare Parameters (with and without Type II Bursts). Solar physics, 270, 273-284 doi:10.1007/s11207-011-9752-3.
@article{article, year = {2011}, pages = {273-284}, DOI = {10.1007/s11207-011-9752-3}, keywords = {coronal mass ejections, flares}, journal = {Solar physics}, doi = {10.1007/s11207-011-9752-3}, volume = {270}, issn = {0038-0938}, title = {Correlation between CME and Flare Parameters (with and without Type II Bursts)}, keyword = {coronal mass ejections, flares} }

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


Uključenost u ostale bibliografske baze podataka:


  • NASA-ADS


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