Add to ORKGWe analyzed the structure of the magnetic field in active regions at coronal altitudes, determined using multiwavelength observations of polarized radio emission in the microwave range at the radiotelescope RATAN-600. The observations were compared with the current-free magnetic field extrapolation of the photospheric field. It is shown that the measured magnetic field is always larger than the reconstructed field at the same height. The slopes of the tubes obtained by this method corresponds to the slopes obtained for the reconstructed field, although the degree of the slope differ significantly. The measured magnetic field structure is probably more complicated than the structure obtained by the reconstruction. Comparison of our measureme...
Magnetic fields play a crucial role for the physics of the dilute and hot upper parts of the solar a...
In this paper, coronal magnetic field structures are compared with coronal holes, interplanetary pla...
The characteristics of the observed polarization of radio waves are determined by the emission mech-...
We analyzed the structure of the magnetic field in active regions at coronal altitudes, determined u...
Radio observations of some active regions (ARs) obtained with the Nobeyama radiolieliograph at lambd...
Abstract. Solar active region coronae are known for strong magnetic fields permeating tenuous plasma...
Unusual spectra with a significant decrease in circularly polarised emissions (Stokes parameter V ) ...
Localized increase of the magnetic field observed by routine methods on the photosphere result in th...
It is analysed the discrepancy about the coronal magnetic field between solar optic and solar radio ...
We present a new technique for the measurement of magnetic fields in the solar chromosphere - corona...
<p>The Solar Corona is a teneous medium of magnetized plasma with an inherent distribution of number...
Abstract. Magnetic fields in the solar corona are responsible for a wide range of phenomena. However...
Three dimensional structure of an active region is determined from observations with the Very Large ...
The solar atmosphere being magnetic in nature, the understanding of the structure and evolution of t...
Solar active regions are the source of the most violent events observed on the Sun, some of which ha...
Magnetic fields play a crucial role for the physics of the dilute and hot upper parts of the solar a...
In this paper, coronal magnetic field structures are compared with coronal holes, interplanetary pla...
The characteristics of the observed polarization of radio waves are determined by the emission mech-...
We analyzed the structure of the magnetic field in active regions at coronal altitudes, determined u...
Radio observations of some active regions (ARs) obtained with the Nobeyama radiolieliograph at lambd...
Abstract. Solar active region coronae are known for strong magnetic fields permeating tenuous plasma...
Unusual spectra with a significant decrease in circularly polarised emissions (Stokes parameter V ) ...
Localized increase of the magnetic field observed by routine methods on the photosphere result in th...
It is analysed the discrepancy about the coronal magnetic field between solar optic and solar radio ...
We present a new technique for the measurement of magnetic fields in the solar chromosphere - corona...
<p>The Solar Corona is a teneous medium of magnetized plasma with an inherent distribution of number...
Abstract. Magnetic fields in the solar corona are responsible for a wide range of phenomena. However...
Three dimensional structure of an active region is determined from observations with the Very Large ...
The solar atmosphere being magnetic in nature, the understanding of the structure and evolution of t...
Solar active regions are the source of the most violent events observed on the Sun, some of which ha...
Magnetic fields play a crucial role for the physics of the dilute and hot upper parts of the solar a...
In this paper, coronal magnetic field structures are compared with coronal holes, interplanetary pla...
The characteristics of the observed polarization of radio waves are determined by the emission mech-...