Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/43707/1/11207_2005_Article_BF02276570.pd
The instrumental advances made in this new era of 4 m class solar telescopes with unmatched spectrop...
Context. In sunspots, the geometric height of continuum optical depth unity is depressed compared to...
The purpose of space weather is the systemic study of the Sun–Earth system, in order to determine th...
Abstract Context: Systematic observations of magnetic field strength and polarity in sunspots began...
Aims. We investigate the height dependence of the magnetic field of a sunspot, which has been until...
Context. Systematic observations of magnetic field strength and polarity in sunspots began at Mount ...
Ph.D. University of Hawaii at Manoa 2011.Includes bibliographical references.This dissertation focus...
We have the strongest of reasons to infer the existence of free electricity in the sun. At high temp...
Ground magnetic field measurements can be mathematically related to an overhead ionospheric equivale...
We present observational evidence for the existence of a current sheet in the chromosphere above a s...
We present an investigation of a single sunspot observed in the neutral Fe line at 1089.6 nm with ...
Abstract. Sunspots, seen as cool regions on the surface of the Sun, are a thermal phenomenon. Sunspo...
Abstract. We have analysed two-dimensional spectro-polarimetric data taken with the MSDP observing m...
A multi-wavelength photometric analysis was performed in order to study the sub-structure of a sunsp...
We exhibit the effects of Faraday rotation on the direction of the transverse component of the magne...
The instrumental advances made in this new era of 4 m class solar telescopes with unmatched spectrop...
Context. In sunspots, the geometric height of continuum optical depth unity is depressed compared to...
The purpose of space weather is the systemic study of the Sun–Earth system, in order to determine th...
Abstract Context: Systematic observations of magnetic field strength and polarity in sunspots began...
Aims. We investigate the height dependence of the magnetic field of a sunspot, which has been until...
Context. Systematic observations of magnetic field strength and polarity in sunspots began at Mount ...
Ph.D. University of Hawaii at Manoa 2011.Includes bibliographical references.This dissertation focus...
We have the strongest of reasons to infer the existence of free electricity in the sun. At high temp...
Ground magnetic field measurements can be mathematically related to an overhead ionospheric equivale...
We present observational evidence for the existence of a current sheet in the chromosphere above a s...
We present an investigation of a single sunspot observed in the neutral Fe line at 1089.6 nm with ...
Abstract. Sunspots, seen as cool regions on the surface of the Sun, are a thermal phenomenon. Sunspo...
Abstract. We have analysed two-dimensional spectro-polarimetric data taken with the MSDP observing m...
A multi-wavelength photometric analysis was performed in order to study the sub-structure of a sunsp...
We exhibit the effects of Faraday rotation on the direction of the transverse component of the magne...
The instrumental advances made in this new era of 4 m class solar telescopes with unmatched spectrop...
Context. In sunspots, the geometric height of continuum optical depth unity is depressed compared to...
The purpose of space weather is the systemic study of the Sun–Earth system, in order to determine th...