From the 1 of 10 linked papers with an AI index.
10 papers
The location and propagation of fine structures in type II solar radio bursts
S. Normo, K. Bhandari, A. Nadiger +1
Solar eruptions such as coronal mass ejections can drive collisionless shocks that are good particle accelerators. Electrons accelerated by these shocks can be observed remotely vi…
Solar energetic particles and their association with radio emissions
Diana E. Morosan, Anshu Kumari, Immanuel Jebaraj +6
The paper discusses how solar radio burst observations, especially with the SKA, can be used to study the acceleration and escape of solar energetic particles (SEPs) associated wit…
Probing the Solar Corona and the Solar Wind Using Angular Broadening Observations with the SKA
Peijin Zhang, John Morgan, Divya Oberoi +9
Angular broadening observations of compact radio sources provide a powerful method for probing the solar corona and solar wind. Such observations enable studies of the phase struct…
Comprehensive study of solar type II radio bursts and the properties of the associated shock waves
K. Bhandari, D. E. Morosan, S. Normo
Type II radio bursts are solar radio emissions generated by electrons accelerated by coronal shocks. These bursts are typically found close to expanding coronal mass ejections (CME…
Solar Radio Bursts in the metric to kilometric range
Anshu Kumari, Mugundhan V., Diana E. Morosan +6
Solar radio bursts (SRBs) are intense emissions observed in radio wavelengths most frequently during solar transients, such as coronal mass ejections (CMEs) and flares. SRBs are di…
On the source sizes of type II radio bursts with LOFAR
A. Kumari, D. E. Morosan, V. Mugundhan +5
Solar radio bursts can provide important insights into the underlying physical mechanisms that drive the small and large-scale eruptions on the Sun. Since metric radio observations…