Coronal jets represent important manifestations of ubiquitous solar transients, which may be
the source of significant mass and energy input to the upper solar atmosphere and the solar …

The Sun's outer atmosphere is heated to temperatures of millions of degrees, and solar
plasma flows out into interplanetary space at supersonic speeds. This paper reviews our …

We present EUV solar observations showing evidence for omnipresent jetting activity driven
by small-scale magnetic reconnection at the base of the solar corona. We argue that the …

Coronal holes are areas on the Sun with open magnetic field lines. They are a source region
of the solar wind, but how the wind emerges from coronal holes is not known. We observed …

Measurements of the near-Sun solar wind by the Parker Solar Probe have revealed the
presence of large numbers of discrete Alfvénic impulses with an anti-sunward sense of …

Context. Recent observations by the Extreme Ultraviolet Imager (EUI) on board Solar Orbiter
have characterized prevalent small-scale transient brightenings in the corona above the …

The solar chromosphere forms a crucial, yet complex and until recently poorly understood,
interface between the solar photosphere and the heliosphere.▪ Advances in high-resolution …

The heating of the solar chromosphere and corona to the observed high temperatures, imply
the presence of ongoing heating that balances the strong radiative and thermal conduction …

We report the presence of intermittent, short discrete enhancements in plasma speed in the
near-Sun high-speed solar wind. Lasting tens of seconds to minutes in spacecraft …

Solar coronal loops are the building blocks of the solar corona. These dynamic structures
are shaped by the magnetic field that expands into the solar atmosphere. They can be …