Abstract Solar Probe Plus (SPP) will be the first spacecraft to fly into the low solar corona.
SPP's main science goal is to determine the structure and dynamics of the Sun's coronal …

While it is certain that the fast solar wind originates from coronal holes, where and how the
slow solar wind (SSW) is formed remains an outstanding question in solar physics even in …

Aims We aim to investigate and characterize the morphology and dynamics of small-scale
coronal plasma density inhomogeneities detected as brighter, denser features propagating …

Coronal pseudostreamers, which separate like-polarity coronal holes, do not have current
sheet extensions, unlike the familiar helmet streamers that separate opposite-polarity holes …

We present a method that isolates time-varying components from coronagraph and extreme
ultraviolet images, allowing substreamer transients propagating within streamers to be …

The past solar minimum is characterized by several peculiar aspects and by a complex
magnetic topology with two different types of coronal streamers: pseudo-streamers and …

ABSTRACT A set of co-aligned high-resolution images from the Atmospheric Imaging
Assembly (AIA) on board the Solar Dynamics Observatory is used to investigate propagating …

Transverse waves are sometimes observed in solar helmet streamers, typically after the
passage of a coronal mass ejection (CME). The CME-driven shock wave moves the …

We revisit a quiet 14 day period of solar minimum during 2008 January and track
substreamer propagating disturbances (PDs) from low heights in STEREO/EUVI to the …

Faraday rotation (FR) of transcoronal radio transmissions from spacecraft near superior
conjunction enables study of the temporal variations in coronal plasma density, velocity, and …