000004087 001__ 4087
000004087 005__ 20220922151055.0
000004087 0247_ $$2DOI$$a10.1016/j.asr.2018.06.037
000004087 037__ $$aSCART-2019-0130
000004087 100__ $$aDąbrowski, B. P. 
000004087 245__ $$aObservations of the Sun using LOFAR Baldy station
000004087 260__ $$c2018
000004087 520__ $$aWe report first results of solar spectroscopic observations carried out with the Baldy LOFAR (LOw-Frequency ARray) station, Poland from October 2016 to July 2017. During this time, we observed different types of radio emission: type I and type III radio bursts. Our observations show that the station is fully operational and it is capable to work efficiently in the single station mode for solar observations. Furthermore, in this paper we will briefly describe the observational technique and instrument capabilities and show some examples of first observations.
000004087 536__ $$aBRAIN.be/$$cCCSOM/$$fCCSOM
000004087 594__ $$aNO
000004087 700__ $$aMorosan, D. E. 
000004087 700__ $$aFallows, R. A.
000004087 700__ $$aBlaszkiewicz, L. 
000004087 700__ $$aKrankowski, A. 
000004087 700__ $$aMagdalenic, J. 
000004087 700__ $$aVocks, C. 
000004087 700__ $$aMann, G. 
000004087 700__ $$aZucca, P. 
000004087 700__ $$aSidorowicz, T.
000004087 700__ $$aHajduk, M.
000004087 700__ $$aKotulak, K.
000004087 700__ $$aFron, A. 
000004087 700__ $$aSniadkowska, K.
000004087 773__ $$c1895-1903$$n7$$pAdvances in Space Research$$v62$$y2018
000004087 8560_ $$fjasmina.magdalenic@observatoire.be
000004087 905__ $$apublished in
000004087 980__ $$aREFERD