Pregled bibliografske jedinice broj: 647557
Kinematics of Interacting ICMEs and Related Forbush Decrease : Case Study
Kinematics of Interacting ICMEs and Related Forbush Decrease : Case Study // Solar physics, 289 (2014), 1; 351-368 doi:10.1007/s11207-013-0314-8 (međunarodna recenzija, članak, znanstveni)
CROSBI ID: 647557 Za ispravke kontaktirajte CROSBI podršku putem web obrasca
Naslov
Kinematics of Interacting ICMEs and Related Forbush Decrease : Case Study
Autori
Maričić, Darije ; Vršnak, Bojan ; Dumbović, Mateja ; Žic, Tomislav ; Roša, Dragan ; Hržina, Damir ; Lulić, Slaven ; Romštajn, Ivan ; Bušić, Ivan ; Salamon, Krešimir ; Temmer, M. ; Rollett, T. ; Veronig, A. ; Bostanjyan, N. ; Chilingarian, A. ; Mailyan, B. ; Arakelyan, K. ; Hovhannisyan, A. ; Mujić, N.
Izvornik
Solar physics (0038-0938) 289
(2014), 1;
351-368
Vrsta, podvrsta i kategorija rada
Radovi u časopisima, članak, znanstveni
Ključne riječi
cosmic rays ; interplanetary coronal mass ejections ; solar wind ; disturbances
Sažetak
We study heliospheric propagation and some space weather aspects of three Earth-directed interplanetary coronal mass ejections (ICMEs), successively launched from the active region AR 11158 in the period 13 – 15 February 2011. From the analysis of the ICME kinematics, morphological evolution, and in situ observations, we infer that the three ICMEs interacted on their way to Earth, arriving together at 1 AU as a single interplanetary disturbance. Detailed analysis of the in situ data reveals complex internal structure of the disturbance, where signatures of the three initially independent ICMEs could be recognized. The analysis also reveals compression and heating of the middle ICME, as well as ongoing magnetic reconnection between the leading and the middle ICME. We present evidence showing that the propagation of these two, initially slower ICMEs, was boosted by the fastest, third ICME. Finally, we employ the ground-based cosmic ray observations, to show that this complex disturbance produced a single cosmic ray event, i.e., a simple Forbush decrease (FD). The results presented provide a better understanding of the ICME interactions and reveal effects that should be taken into account in forecasting of the arrival of such compound structures.
Izvorni jezik
Engleski
Znanstvena područja
Fizika
POVEZANOST RADA
Profili:
Dragan Roša
(autor)
Darije Maričić
(autor)
Tomislav Žic
(autor)
Slaven Lulić
(autor)
Krešimir Salamon
(autor)
Ivan Romštajn
(autor)
Bojan Vršnak
(autor)
Ibrahim Mujić
(autor)
Mateja Dumbović
(autor)
Citiraj ovu publikaciju:
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