In this review we focus on the fundamental theory of magnetohydrodynamic reconnection,
together with applications to understanding a wide range of dynamic processes in the solar …

This paper outlines the current understanding of solar flares, mainly focused on
magnetohydrodynamic (MHD) processes responsible for producing a flare. Observations …

Plasma and magnetic field data from the Helios 1/2 spacecraft have been used to
investigate the structure of magnetic clouds (MCs) in the inner heliosphere. 46 MCs were …

Basic topology of twisted magnetic configurations in solar flares ADS Classic is now deprecated.
It will be completely retired in October 2019. This page will automatically redirect to the new …

Observations and models of solar prominences are reviewed. We focus on non-eruptive
prominences, and describe recent progress in four areas of prominence research:(1) …

Observational conditions for the formation and maintenance of filaments are reviewed since
1989 in the light of recent findings on their structure, chirality, inferred magnetic topology …

Images of the X-ray corona near the solar disk's center were examined for large, transient
brightenings of the type known to be associated with H &agr; filament eruptions and coronal …

Soft X‐ray images of solar active regions frequently show S‐or inverse‐S (sigmoidal)
morphology. We have studied the Yohkoh Soft X‐Ray Telescope video movie for 1993 and …

This review puts together what we have learned about coronal structures and
phenomenology to synthesize a physical picture of the corona as a voluminous, thermally …

This chapter provides an overview of current efforts in the theory and modeling of CMEs.
Five key areas are discussed:(1) CME initiation;(2) CME evolution and propagation;(3) the …