X-ray and ultraviolet (UV) observations of the outer solar atmosphere have been used for
many decades to measure the fundamental parameters of the solar plasma. This review …

Soft X-ray spectroscopy of solar flares - an overview ADS Classic is now deprecated. It will be
completely retired in October 2019. This page will automatically redirect to the new ADS …

Abstract The Bragg Crystal Spectrometer (BCS) is one of the instruments which makes up
the scientific payload of the SOLAR-A mission. The spectrometer employs four bent …

The problem of electrodynamic coupling of stellar coronal loops where beta is less than 1 to
underlying velocity fields where beta is greater than approximately 1 is treated. A rigorous …

Solar flare X-ray spectra from the Solar Maximum Mission Flat Crystal Spectromet ADS Classic
is now deprecated. It will be completely retired in October 2019. This page will automatically …

We present the first model of resonant heating of coronal loops that incorporates the
dependence of the loop density on the heating rate. By adopting the quasi-static equilibrium …

Spectral line widths are often observed to be larger than can be accounted for by thermal
and instrumental broadening alone. This excess broadening is a key observational …

The first nonlinear study of the instability of the resonant absorption is presented in this
paper. The nonlinear evolution of the resonant absorption of Alfvén waves in an …

Coronal heating by the resonant absorption of Alfven waves: Wavenumber scaling l ADS
Classic is now deprecated. It will be completely retired in October 2019. This page will …

Numerical simulations of the MHD equations for a fully compressible, low-beta, resistive
plasma are used to study the resonance absorption process for the heating of coronal active …