activity
20142026
most citedMultiple Regions of Shock-accelerated Particles during a Solar Coronal Mass Ejection

89 citations · 861 across the 43 of their papers we have counts for

collaborators
Showing 2026Show all

6 papers · 1 filter

astro-ph.SR2026

Tracking a solar energetic eruption and associated energetic particles from Sun to spacecraft

D. E. Morosan, M. Baumgartner-Steinleitner, K. Bhandari +17

Context. Solar energetic particles (SEPs) in the heliosphere are produced by flaring processes on the Sun or shocks driven by coronal mass ejections (CMEs). Electrons, in particula…

econ.GN2026

Participation, selection and indicative bidding in auctions with costly entry

Changxia Ke, Greg Kubitz, Yang Liu

We study auctions with costly entry in which bidders have incomplete information about their affiliated private valuations prior to entry. We examine whether indicative bidding--a…

astro-ph.SR2026

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…

astro-ph.SR2026

Solar energetic particles and their association with radio emissions

Diana E. Morosan, Anshu Kumari, Immanuel Jebaraj +6

Energetic particle populations are ubiquitous throughout the Universe. In our solar system, the most prominent sources of energetic particles are solar flares or collisionless shoc…

astro-ph.SR2026

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…

astro-ph.SR2026

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…