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A possible line-like emission feature at 8 keV in the Seyfert 1.2 UGC 3973

The High‐Temperature Response of theTRACE171 A and 195 A Channels

Spectral Atlas of X‐Ray Lines Emitted during Solar Flares Based on CHIANTI

Properties of a Sunspot Plume Observed with the Coronal Diagnostic Spectrometer Aboard theSolar and Heliospheric Observatory

Flare X-Ray Observations of AB Doradus: Evidence of Stellar Coronal Opacity

Constraints on the ionizing flux emitted by T Tauri stars

The Solar-B EUV imaging spectrometer and its science goals

Modeling CHANDRA low energy transmission grating spectrometer observations of classical novae with PHOENIX

Detection of X-ray emission from β Pictoris with XMM-Newton: a cool corona, a boundary layer or what?

CORONAS‐F/SPIRIT EUV observations of October–November 2003 solar eruptive events in combination with SOHO/EIT data

Detecting Intracluster Gas Motion in Galaxy Clusters: MockAstro‐E2Observations

Electron density along a coronal loop observed with CDS/SOHO

Plasma diagnostics of active-region evolution and implications for coronal heating

All Coronal Loops Are the Same: Evidence to the Contrary

Helium Abundance in High‐Temperature Solar Flare Plasmas

Correlation between coronal hole and quiet Sun intensities: Evidence for continuous reconnection

The Evolution of Supernovae in Circumstellar Wind‐Blown Bubbles. I. Introduction and One‐Dimensional Calculations

A solar active region loop compared with a 2D MHD model

Radial variations in the Io plasma torus during the Cassini era

Fe VII lines in the spectrum of RR Telescopii

The thermal X-ray spectrum of the 2003 April 26 solar flare

Modeling temporal variability of plasma conditions in the Io torus during the Cassini era

Solar Variability and Its Effects on Climate

Relativistic multireference many-body perturbation theory calculations on ions of the phosphorus isoelectronic sequence

The Far‐Ultraviolet Spectrum of the Io Plasma Torus

ANGULAR DIAMETER DISTANCE IN PERTURBED FRIEDMANN SPACETIME: EFFECTS OF GRAVITATIONAL WAVES

Solar Variability and Its Effects on Climate

Signature of oscillations in coronal bright points

X-ray emission from a metal depleted accretion shock onto the classical T Tauri star TW Hya

High-accuracy calculations of term energies and lifetimes of silicon-like ions with nuclear chargesZ= 24–30

Relativistic many-body perturbation calculations on extreme ultraviolet and soft-x-ray transition energies in siliconlike iron

Extreme‐Ultraviolet Emission Lines of Sxin Solar Flare and Active Region Spectra

The Relationship of the Chromosphere to the Lower Solar Transition Region

Extreme‐Ultraviolet and X‐Ray Spectroscopy of a Solar Flare Loop Observed at High Time Resolution: A Case Study in Chromospheric Evaporation

Coronal Heating through Braiding of Magnetic Field Lines

Variability of the EUV quiet Sun emission and reference spectrum using SUMER

On the widths of the Mg X lines near 60 nm in the corona

Solar and Space Weather Radiophysics

Identification and analysis of soft X-ray lines of Ar xiii-Ar xvi in laboratory and astrophysical plasmas

A Detailed Study of Opacity in the Upper Atmosphere of Proxima Centauri

Models for Solar Magnetic Loops. IV. On the Relation between Coronal and Footpoint Plasma in Active Region Loops

Going Slitless: Images of Forbidden‐Line Emission Regions of Classical T Tauri Stars Observed with theHubble Space Telescope

Newly Identified Forbidden Transitions within the Ground Configuration of Ions of Very Low Abundance P, Cl, K, and Co

Atomic Data and Spectral Line Intensities for Caviii

Constraints on the Cluster Mass‐Temperature Relation Imposed by the Diffuse X‐Ray Background

Close Association of an Extreme‐Ultraviolet Sunspot Plume with Depressions in the Sunspot Radio Emission

Properties of the Lower Transition Region: The Widths of Optically Allowed and Intersystem Spectral Lines

Active Region Streamer Diagnostics 2001 September 14–16

The SUMER spectral atlas of solar coronal features

Radiative data for Fe XIII

On the nature of EIT waves, EUV dimmings and their link to CMEs