activity
20152019
most citedProminence and Filament Eruptions Observed by the Solar Dynamics Observatory: Statistical Properties, Kinematics, and Online Catalog

147 citations · 296 across the 6 of their papers we have counts for

collaborators

11 papers

astro-ph.SR2019

Radio Burst and Circular Polarization Studies of the Solar Corona at Low Frequencies

Patrick I. McCauley

Low-frequency (80-240 MHz) radio observations of the solar corona are presented using the Murchison Widefield Array (MWA), and several discoveries are reported. The corona is revie…

astro-ph.SR2019

Comprehensive Characterization of Solar Eruptions With Remote and In-Situ Observations, and Modeling: The Major Solar Events on 4 November 2015

Iver H. Cairns, Kamen A. Kozarev, Nariaki V. Nitta +12

Solar energetic particles (SEPs) are an important product of solar activity. They are connected to solar active regions and flares, coronal mass ejections (CMEs), EUV waves, shocks…

astro-ph.IM201935 cited

Science with the Murchison Widefield Array: Phase I Results and Phase II Opportunities

A. P. Beardsley, M. Johnston-Hollitt, C. M. Trott +56

The Murchison Widefield Array (MWA) is an open access telescope dedicated to studying the low frequency (80300 MHz) southern sky. Since beginning operations in mid 2013, the MWA…

astro-ph.SR2019

The Low-Frequency Solar Corona in Circular Polarization

Patrick I. McCauley, Iver H. Cairns, Stephen M. White +4

We present spectropolarimetric imaging observations of the solar corona at low frequencies (80 - 240 MHz) using the Murchison Widefield Array (MWA). These images are the first of t…

astro-ph.SR2019

A weak coronal heating event associated with periodic particle acceleration episodes

Atul Mohan, Patrick I. McCauley, Alpha Mastrano +1

Weak heating events are frequent and ubiquitous in solar corona. They derive their energy from the local magnetic field and form a major source of local heating, signatures of whic…

astro-ph.SR2018

Nonlinear force-free modeling of flare-related magnetic field changes at the photosphere and chromosphere

Lucia Kleint, Michael S. Wheatland, Alpha Mastrano +1

Rapid and stepwise changes of the magnetic field are often observed during flares but cannot be explained by models yet. Using a 45 min sequence of SDO/HMI 135 s fast-cadence vecto…