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Pregled bibliografske jedinice broj: 475410

Origin of coronal shock waves associated with slow coronal mass ejections


Magdalenić, Jasmina; Marque, Christoph; Zhukov, Andrei; Vršnak, Bojan; Žic, Tomislav
Origin of coronal shock waves associated with slow coronal mass ejections // The Astrophysical journal, 718 (2010), 1; 266-278 doi:10.1088/0004-637X/718/1/266 (međunarodna recenzija, članak, znanstveni)


Naslov
Origin of coronal shock waves associated with slow coronal mass ejections

Autori
Magdalenić, Jasmina ; Marque, Christoph ; Zhukov, Andrei ; Vršnak, Bojan ; Žic, Tomislav

Izvornik
The Astrophysical journal (0004-637X) 718 (2010), 1; 266-278

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

Ključne riječi
shock waves – Sun: corona – Sun: coronal mass ejections (CMEs) – Sun: flares – Sun: radioradiation
(shock waves – Sun:corona–Sun:coronal mass ejections (CMEs) – Sun: flares – Sun: radioradiation)

Sažetak
We present a multiwavelength study of five coronal mass ejection/flare events (CME/flare) and associated coronal shock waves manifested as type II radio bursts. The study is focused on the events in which the flare energy release, and not the associated CME, is themost probable source of the shock wave. Therefore, we selected events associated with rather slow CMEs (reported mean velocity below 500 km s−1). To ensure minimal projection effects, only events related to flares situated close to the solar limb were included in the study. We used radio dynamic spectra, positions of radio sources observed by the Nan¸cay Radioheliograph, GOES soft X-ray flux measurements, Large Angle Spectroscopic Coronagraph, and Extreme-ultraviolet Imaging Telescope observations. The kinematics of the shock wave signatures, type II radio bursts, were analyzed and compared with the flare evolution and the CME kinematics.We found that the velocities of the shock waves were significantly higher, up to one order of magnitude, than the contemporaneous CME velocities. On the other hand, shock waves were closely temporally associated with the flare energy release thatwas very impulsive in all events. This suggests that the impulsive increase of the pressure in the flare was the source of the shock wave. In four events the shock wave was most probably flare-generated, and in one event results were inconclusive due to a very close temporal synchronization of the CME, flare, and shock.

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 Jasmina Magdalenić (autor)

Avatar Url Bojan Vršnak (autor)

Avatar Url Tomislav Žic (autor)

Citiraj ovu publikaciju

Magdalenić, Jasmina; Marque, Christoph; Zhukov, Andrei; Vršnak, Bojan; Žic, Tomislav
Origin of coronal shock waves associated with slow coronal mass ejections // The Astrophysical journal, 718 (2010), 1; 266-278 doi:10.1088/0004-637X/718/1/266 (međunarodna recenzija, članak, znanstveni)
Magdalenić, J., Marque, C., Zhukov, A., Vršnak, B. & Žic, T. (2010) Origin of coronal shock waves associated with slow coronal mass ejections. The Astrophysical journal, 718 (1), 266-278 doi:10.1088/0004-637X/718/1/266.
@article{article, year = {2010}, pages = {266-278}, DOI = {10.1088/0004-637X/718/1/266}, keywords = {shock waves – Sun:corona–Sun:coronal mass ejections (CMEs) – Sun: flares – Sun: radioradiation}, journal = {The Astrophysical journal}, doi = {10.1088/0004-637X/718/1/266}, volume = {718}, number = {1}, issn = {0004-637X}, title = {Origin of coronal shock waves associated with slow coronal mass ejections}, keyword = {shock waves – Sun:corona–Sun:coronal mass ejections (CMEs) – Sun: flares – Sun: radioradiation} }

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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