Shortly after the seminal paper “Self-Organized Criticality: An explanation of 1/f noise” by
Bak et al.(1987), the idea has been applied to solar physics, in “Avalanches and the …

We present a review of the different aspects associated with the interaction of successive
coronal mass ejections (CMEs) in the corona and inner heliosphere, focusing on the …

The production mechanism of repeating fast radio bursts (FRBs) is still a mystery, and
correlations between burst occurrence times and energies may provide important clues to …

We present a statistical analysis of solar coronal mass ejections (CMEs) based on 23 years
of quasi-continuous observations with the LASCO coronagraph, thus covering two complete …

This paper discusses a near real-time approach to solar active-region monitoring and flare
prediction using the Big Bear Solar Observatory Active Region Monitor (ARM). Every hour …

M dwarf stars are known for their vigorous flaring. This flaring could impact the climate of
orbiting planets, making it important to characterize M dwarf flares at the short wavelengths …

We test statistically the hypothesis that radio pulsar glitches result from an avalanche
process, in which angular momentum is transferred erratically from the flywheel-like …

Abstract In 2003 January, the Chandra Orion Ultradeep Project (COUP) detected about
1400 young stars during a 13.2 day observation of the Orion Nebula Cluster (ONC). This …

This paper is a pedagogical introduction to avalanche models of solar flares, including a
comprehensive review of recent modeling efforts and directions. This class of flare model is …

Context. Repeating fast radio bursts (FRBs) present excellent opportunities to identify FRB
progenitors and host environments as well as to decipher the underlying emission …