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Pregled bibliografske jedinice broj: 912788

Properties and relationship between solar eruptive flares and Coronal Mass Ejections during rising phase of Solar Cycles 23 and 24


Ibrahim, Syed; Shanmugaraju, A.; Moon, Y.-J.; Vršnak, Bojan; Umapathy, S.
Properties and relationship between solar eruptive flares and Coronal Mass Ejections during rising phase of Solar Cycles 23 and 24 // Advances in space research, 61 (2018), 1; 540-551 doi:10.1016/j.asr.2017.09.015 (međunarodna recenzija, članak, znanstveni)


Naslov
Properties and relationship between solar eruptive flares and Coronal Mass Ejections during rising phase of Solar Cycles 23 and 24

Autori
Ibrahim, Syed ; Shanmugaraju, A. ; Moon, Y.-J. ; Vršnak, Bojan ; Umapathy, S.

Izvornik
Advances in space research (0273-1177) 61 (2018), 1; 540-551

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

Ključne riječi
Coronal Mass Ejection (CME) ; Flare

Sažetak
Statistical relationship between major flares and the associated CMEs during rising phases of Solar Cycles 23 and 24 are studied. Totally more than 6000 and 10, 000 CMEs were observed by SOHO/LASCO (Solar and Heliospheric Observatory/Large Angle Spectrometric Coronagraph) during 23rd [May 1996– June 2002] and 24th [December 2008–December 2014] solar cycles, respectively. In particular, we studied the relationship between properties of flares and CMEs using the limb events (longitude 70–85°) to avoid projection effects of CMEs and partial occultation of flares that occurred near 90°. After selecting a sample of limb flares, we used certain spatial and temporal constraints to find the flare-CME pairs. Using these constraints, we compiled 129 events in Solar Cycle 23 and 92 events in Solar Cycle 24. We compared the flare- CME relationship in the two solar cycles and no significant differences are found between the two cycles. We only found out that the CME mean width was slightly larger and the CME mean acceleration was slightly higher in cycle 24, and that there was somewhat a better relation between flare flux and CME deceleration in cycle 24 than in cycle 23.

Izvorni jezik
Engleski

Znanstvena područja
Fizika



POVEZANOST RADA


Projekt / tema
HRZZ-IP-2013-11-6212 - Promjenjivost Sunca i zvijezda (Bojan Vršnak, )

Ustanove
Geodetski fakultet, Zagreb

Profili:

Avatar Url Bojan Vršnak (autor)

Citiraj ovu publikaciju

Ibrahim, Syed; Shanmugaraju, A.; Moon, Y.-J.; Vršnak, Bojan; Umapathy, S.
Properties and relationship between solar eruptive flares and Coronal Mass Ejections during rising phase of Solar Cycles 23 and 24 // Advances in space research, 61 (2018), 1; 540-551 doi:10.1016/j.asr.2017.09.015 (međunarodna recenzija, članak, znanstveni)
Ibrahim, S., Shanmugaraju, A., Moon, Y., Vršnak, B. & Umapathy, S. (2018) Properties and relationship between solar eruptive flares and Coronal Mass Ejections during rising phase of Solar Cycles 23 and 24. Advances in space research, 61 (1), 540-551 doi:10.1016/j.asr.2017.09.015.
@article{article, year = {2018}, pages = {540-551}, DOI = {10.1016/j.asr.2017.09.015}, keywords = {Coronal Mass Ejection (CME), Flare}, journal = {Advances in space research}, doi = {10.1016/j.asr.2017.09.015}, volume = {61}, number = {1}, issn = {0273-1177}, title = {Properties and relationship between solar eruptive flares and Coronal Mass Ejections during rising phase of Solar Cycles 23 and 24}, keyword = {Coronal Mass Ejection (CME), Flare} }

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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