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All issues Astron. Astrophys. Suppl. Ser., 122 3 (1997) 585-592 Article references

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THE INFLUENCE OF NUMERICAL RESOLUTION ON CORONAL DENSITY IN HYDRODYNAMIC MODELS OF IMPULSIVE HEATING

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PLASMA SLOSHING IN PULSE-HEATED SOLAR AND STELLAR CORONAL LOOPS

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X-Ray Flare Oscillations Track Plasma Sloshing along Star-disk Magnetic Tubes in the Orion Star-forming Region

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The Astrophysical Journal 856 (1) 51 (2018)
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The radiative response of solar loop plasma subject to transient heating

S. J. Bradshaw and H. E. Mason
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Multi-wavelength observations and modelling of a canonical solar flare

C. L. Raftery, P. T. Gallagher, R. O. Milligan and J. A. Klimchuk
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Emission Measure Distribution in Loops Impulsively Heated at the Footpoints

Paola Testa, Giovanni Peres and Fabio Reale
The Astrophysical Journal 622 (1) 695 (2005)
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Modeling a Coronal Loop Heated by Magnetohydrodynamic Turbulence Nanoflares

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CORONAL FUZZINESS MODELED WITH PULSE-HEATED MULTI-STRANDED LOOP SYSTEMS

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Modelling long duration X-ray flares on the UX Ari late-type subgiant

I. M. Livshits
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Detailed Diagnostics of an X‐Ray Flare in the Single Giant HR 9024

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X-RAY FLARES OF EV Lac: STATISTICS, SPECTRA, AND DIAGNOSTICS

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Optical microflaring on the nearby flare star binary UV Ceti

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X-ray and optical bursts and flares in YSOs: results from a 5-day XMM-Newton monitoring campaign of L1551

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Origin of prolonged X-ray flares on active late-type stars

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ENTHALPY-BASED THERMAL EVOLUTION OF LOOPS. III. COMPARISON OF ZERO-DIMENSIONAL MODELS

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Bright X‐Ray Flares in Orion Young Stars from COUP: Evidence for Star‐Disk Magnetic Fields?

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A large X-ray flare from the Herbig Ae star V892 Tau

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X-ray emission from dense plasma in classical T Tauri stars: hydrodynamic modeling of the accretion shock

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On the Coronal Temperature in Solar Microflares

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A new approach for modelling chromospheric evaporation in response to enhanced coronal heating

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Large-amplitude Quasiperiodic Pulsations as Evidence of Impulsive Heating in Hot Transient Loop Systems Detected in the EUV with SDO/AIA

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A Brightening Coronal Loop Observed byTRACE. II. Loop Modeling and Constraints on Heating

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Relationship between impulsive and post-eruptive processes in solar X-ray flares

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Modelling the solar transition region using an adaptive conduction method

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