Sunspots are the most readily visible manifestations of solar magnetic field concentrations
and of their interaction with the Sun's plasma. Although sunspots have been extensively …

We analytically study the damping of Alfvén mode oscillations in the chromosphere and in
coronal loops. In the partially ionized chromosphere the dominant damping process of …

This paper presents a new diagnostic tool for the inference of the thermal, dynamic, and
magnetic properties of the solar chromosphere. It consists of a non-LTE inversion code of …

We confirm recent results about the differences in temperature and magnetic field strength
between the umbra of large and small sunspots. Five Stokes I-and V-spectra from the …

The properties of two Fe I lines at 15648.5 A and 15652.9 A in the infrared H-band are
investigated using numerical radiative transfer calculations. It is shown that using this …

Infrared lines as probes of solar magnetic features. III - Strong and weak magne ADS
Classic is now deprecated. It will be completely retired in October 2019. This page will …

We present the first Hinode/EUV Imaging Spectrometer observations of 5 minute quasi-
periodic oscillations detected in a transition-region line (He ii) and five coronal lines (Fe x …

We present an analysis of hard X-ray imaging observations from one of the first solar flares
observed with the Reuven Ramaty High-Energy Solar Spectroscopic Imager (RHESSI) …

We present results of an analysis of time series data observed in sunspot umbral regions.
The data were obtained in the context of the SOHO Joint Observing Program (JOP) 97 in …

Infrared lines as probes of solar magnetic features. V - The magnetic structure ADS Classic is
now deprecated. It will be completely retired in October 2019. This page will automatically …