Add to ORKGWe present results from observations of Moving Magnetic Features (MMFs) of different types observed on region NOAA 11005. The analyses is based on spectro-polarimetric data obtained with the Interferometric Bidimensional Spectrometer (IBIS) at various spectral ranges. We present new evidences of bipolar MMFs observed to stream out from pores and show the temporal evolution of magnetic, dynamic and morphological properties of these features
We present the results from first spectropolarimetric observations of the solar photosphere acquired...
Context. Numerous magnetohydrodynamic oscillations have been reported within solar pores over the pa...
Context. Magnetic bright points (MBPs) are dynamic, small-scale magnetic elements often found with f...
We present results from observations of Moving Magnetic Features (MMFs) of different types observed ...
Context. Moving magnetic features (MMFs) are small-size magnetic elements that are seen to stream ou...
A. J. Kaithakkal et. al.©2017 The American Astronomical Society. All rights reserved.Spectropolarime...
Context. Mechanisms responsible for active-region formation, evolution, and decay have been investig...
Movies of magnetograms of sunspots often show small-size magnetic patches that move radially away an...
We studied the formation of a pore in AR NOAA 11462. We analysed data obtained with the IBIS at the...
Aims. Recent simulations of solar magneto-convection have offered new levels of understanding of the...
Context. Mechanisms responsible for active-region formation, evolution, and decay have been investig...
We analyze the evolution of a pore in the active region NOAA 10940 using the data obtained by the Hi...
Context. Solar pores are intense concentrations of magnetic fields on the solar surface and plasma f...
Five days of coordinated observation were carried out from 24–29 September, 1987 at Big Bear and Hua...
Small magnetic structures can be seen in G-band filtergrams as isolated bright points, strings of br...
We present the results from first spectropolarimetric observations of the solar photosphere acquired...
Context. Numerous magnetohydrodynamic oscillations have been reported within solar pores over the pa...
Context. Magnetic bright points (MBPs) are dynamic, small-scale magnetic elements often found with f...
We present results from observations of Moving Magnetic Features (MMFs) of different types observed ...
Context. Moving magnetic features (MMFs) are small-size magnetic elements that are seen to stream ou...
A. J. Kaithakkal et. al.©2017 The American Astronomical Society. All rights reserved.Spectropolarime...
Context. Mechanisms responsible for active-region formation, evolution, and decay have been investig...
Movies of magnetograms of sunspots often show small-size magnetic patches that move radially away an...
We studied the formation of a pore in AR NOAA 11462. We analysed data obtained with the IBIS at the...
Aims. Recent simulations of solar magneto-convection have offered new levels of understanding of the...
Context. Mechanisms responsible for active-region formation, evolution, and decay have been investig...
We analyze the evolution of a pore in the active region NOAA 10940 using the data obtained by the Hi...
Context. Solar pores are intense concentrations of magnetic fields on the solar surface and plasma f...
Five days of coordinated observation were carried out from 24–29 September, 1987 at Big Bear and Hua...
Small magnetic structures can be seen in G-band filtergrams as isolated bright points, strings of br...
We present the results from first spectropolarimetric observations of the solar photosphere acquired...
Context. Numerous magnetohydrodynamic oscillations have been reported within solar pores over the pa...
Context. Magnetic bright points (MBPs) are dynamic, small-scale magnetic elements often found with f...