LOFAR tied-array imaging of Type III solar radio bursts
Context. The Sun is an active source of radio emission which is often associated with energetic phenomena such as solar flares and coronal mass ejections (CMEs). At low radio frequencies (< 100 MHz), the Sun has not been imaged extensively because of t
|Collections||ANU Research Publications|
|Source:||Astronomy and Astrophysics|
|Access Rights:||Open Access|
|01_Morosan_LOFAR_tied-array_imaging_of_2014.pdf||2.08 MB||Adobe PDF|
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