Solar and stellar X-ray emission are the observed waste products of the interplay between magnetic fields and the motion of stellar plasma. Theoretical understanding of the process of coronal heating is of utmost importance, since the high temperature is what defines the corona in the first place. Most of the research described deals with the aspects of the several rivalling theories for coronal heating. The rest of the papers deal with processes of energy conversion related to flares
The solar corona, the tenuous outer atmosphere of the Sun, is orders of magnitude hotter than the so...
The solar corona has a temperature of order 1 MK, which is almost 200 times the temperature of the u...
This paper discusses the possibility that heating of the solar corona in open field-line regions ema...
The present state of development of the theory of coronal heating is summarized. Coronal heating is ...
Coronal emission comes in two forms, a steady component where the corona is heated to million degree...
Stellar coronae, defined by the ensemble of magnetic field structures above stellar photospheres and...
The effect of the differential rotation of the disk of the Galaxy on magnetic field which penetrates...
We discuss various studies of the global properties of coronal heating. Some of them find power laws...
The defining physical property of the Sun's corona is that the magnetic field dominates the plasma. ...
Context. Observations show that the coronal X-ray emission of the Sun and other stars depends on the...
Context. Twisted magnetic fields should be ubiquitous in the solar corona, particularly in flare-pro...
During the past year this grant has funded research in the interaction between magnetic fields and t...
The temperature of the Sun's outer atmosphere (the corona) exceeds that of the solar surface by abou...
Recent observational data cast serious doubt on the widely held view that the Sun's corona is heated...
The visible corona of the Sun appears to be heated by direct dissipation of magnetic fields. The mag...
The solar corona, the tenuous outer atmosphere of the Sun, is orders of magnitude hotter than the so...
The solar corona has a temperature of order 1 MK, which is almost 200 times the temperature of the u...
This paper discusses the possibility that heating of the solar corona in open field-line regions ema...
The present state of development of the theory of coronal heating is summarized. Coronal heating is ...
Coronal emission comes in two forms, a steady component where the corona is heated to million degree...
Stellar coronae, defined by the ensemble of magnetic field structures above stellar photospheres and...
The effect of the differential rotation of the disk of the Galaxy on magnetic field which penetrates...
We discuss various studies of the global properties of coronal heating. Some of them find power laws...
The defining physical property of the Sun's corona is that the magnetic field dominates the plasma. ...
Context. Observations show that the coronal X-ray emission of the Sun and other stars depends on the...
Context. Twisted magnetic fields should be ubiquitous in the solar corona, particularly in flare-pro...
During the past year this grant has funded research in the interaction between magnetic fields and t...
The temperature of the Sun's outer atmosphere (the corona) exceeds that of the solar surface by abou...
Recent observational data cast serious doubt on the widely held view that the Sun's corona is heated...
The visible corona of the Sun appears to be heated by direct dissipation of magnetic fields. The mag...
The solar corona, the tenuous outer atmosphere of the Sun, is orders of magnitude hotter than the so...
The solar corona has a temperature of order 1 MK, which is almost 200 times the temperature of the u...
This paper discusses the possibility that heating of the solar corona in open field-line regions ema...