Pregled bibliografske jedinice broj: 193836
Broadband Metric-Range Radio Emission Associated with a Moreton/EIT Wave
Broadband Metric-Range Radio Emission Associated with a Moreton/EIT Wave // The Astrophysical journal, 625 (2005), 1; L67-L70 doi:10.1086/430763 (međunarodna recenzija, članak, znanstveni)
CROSBI ID: 193836 Za ispravke kontaktirajte CROSBI podršku putem web obrasca
Naslov
Broadband Metric-Range Radio Emission Associated with a Moreton/EIT Wave
Autori
Vršnak, Bojan ; Magdalenić, Jasmina ; Temmer, Manuela ; Veronig, Astrid ; Warmuth, Alexander ; Mann, Gottfried ; Aurass, Henry ; Otruba, Wolfgang
Izvornik
The Astrophysical journal (0004-637X) 625
(2005), 1;
L67-L70
Vrsta, podvrsta i kategorija rada
Radovi u časopisima, članak, znanstveni
Ključne riječi
Shock Waves ; Sun: Corona
Sažetak
We present the evolution and kinematics of a broadband radio source that propagated collaterally with an Halpha/EIT wave, linking it with the type II burst that was excited higher up in the corona. The NRH wave emission extended from the frequency f~327 to f<151 MHz and was considerably weaker than the flare-related type IV burst. The emission centroid propagated at a height of 0-200 Mm above the solar limb and was intensified when the disturbance passed over enhanced coronal structures. We put forward the ad hoc hypothesis that the NRH wave signature is optically thin gyrosynchrotron emission excited by the passage of the coronal MHD fast-mode shock. The identification of radio emission associated with the coronal wave front is important since it offers us new diagnostic information that could provide us with better insight into the physical conditions in the disturbance itself.
Izvorni jezik
Engleski
Znanstvena područja
Fizika
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