Pregled bibliografske jedinice broj: 728149
Interaction Between Two CMEs During 14 – 15 February 2011 and Their Unusual Radio Signature
Interaction Between Two CMEs During 14 – 15 February 2011 and Their Unusual Radio Signature // Solar physics, 289 (2014), 12; 4621-4632 doi:10.1007/s11207-014-0591-x (međunarodna recenzija, članak, znanstveni)
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Naslov
Interaction Between Two CMEs During 14 – 15 February 2011 and Their Unusual Radio Signature
Autori
Shanmugaraju, Annamalai ; Subramanian, Prasanna ; Vršnak, Bojan ; Ibrahim, Syed
Izvornik
Solar physics (0038-0938) 289
(2014), 12;
4621-4632
Vrsta, podvrsta i kategorija rada
Radovi u časopisima, članak, znanstveni
Ključne riječi
Coronal mass ejections Interacting coronal mass ejections Type-II radio bursts
Sažetak
We report a detailed analysis of an interaction between two coronal mass ejections (CMEs) that were observed on 14 – 15 February 2011 and the corresponding radio enhancement, which was similar to the “CME cannibalism” reported by Gopalswamy et al. (Astrophys. J. 548, L91, 2001). A primary CME, with a mean field-of-view velocity of 669 km s−1 in the Solar and Heliospheric Observatory (SOHO)/Large Angle Spectrometric Coronagraph (LASCO), was more than as twice as fast as the slow CME preceding it (326 km s−1), which indicates that the two CMEs interacted. A radio-enhancement signature (in the frequency range 1 MHz – 400 kHz) due to the CME interaction was analyzed and interpreted using the CME data from LASCO and from the Solar Terrestrial Relations Observatory (STEREO) HI-1, radio data from Wind/Radio and Plasma Wave Experiment (WAVES), and employing known electron-density models and kinematic modeling. The following results are obtained: i) The CME interaction occurred around 05:00 – 10:00 UT in a height range 20 – 25 R⊙. An unusual radio signature is observed during the time of interaction in the Wind/WAVES dynamic radio spectrum. ii) The enhancement duration shows that the interaction segment might be wider than 5 R⊙. iii) The shock height estimated using density models for the radio enhancement region is 10 – 30 R⊙. iv) Using kinematic modeling and assuming a completely inelastic collision, the decrease of kinetic energy based on speeds from LASCO data is determined to be 0.77×1023 J, and 3.67×1023 J if speeds from STEREO data are considered. vi) The acceleration, momentum, and force are found to be a=−168 m s−2, I=6.1×1018 kg m s−1, and F=1.7×1015 N, respectively, using STEREO data.
Izvorni jezik
Engleski
Znanstvena područja
Fizika
POVEZANOST RADA
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