Lyndsay Fletcher astrophysicist
Fletcher, Lyndsay
Fletcher, L.
Fletcher, Lyndsay 1968-
VIAF ID: 23145971373632330412 (Personal)
Permalink: http://viaf.org/viaf/23145971373632330412
Preferred Forms
- 100 1 _ ‡a Fletcher, L.
-
- 100 1 _ ‡a Fletcher, Lyndsay
- 100 1 _ ‡a Fletcher, Lyndsay
- 100 1 _ ‡a Fletcher, Lyndsay ‡d 1968-
- 100 0 _ ‡a Lyndsay Fletcher ‡c astrophysicist
4xx's: Alternate Name Forms (9)
Works
Title | Sources |
---|---|
Dynamics in restructuring active regions observed during SOHO/Yohkoh/GBO campaigns | |
Electric Current Circuits in Astrophysics | |
Electron Inertial Effects on Rapid Energy Redistribution at Magnetic X‐Points | |
Elementary energy release events in flaring loops: effects of chromospheric evaporation on X-rays | |
The emission measure distribution of impulsive phase flare footpoints | |
The Energy Release Process in Solar Flares; Constraints from TRACE Observations | |
Erratum: Depth of a strong jovian jet from a planetary-scale disturbance driven by storms | |
The Europa Imaging System (EIS): High-Resolution, 3-D Insight into Europa’s Geology, Ice Shell, and Potential for Current Activity | |
The EVE Doppler Sensitivity and Flare Observations | |
Evidence for the Flare Trigger Site and Three‐Dimensional Reconnection in Multiwavelength Observations of a Solar Flare | |
Evolution of an eruptive flare loop system | |
Fast Alfven Wave Heating and Acceleration of Ions in a Nonuniform Magnetoplasma | |
Fip Enhancement by Alfvén Ionization | |
Flare ribbon energetics in the early phase of an SDO flare | |
Formation of the thermal infrared continuum in solar flares | |
From large-scale loops to the sites of dense flaring loops: preferential conditions for long-period pulsations in solar flares | |
Hard X-Ray Emission from a Mirror Trap at the Top of Reconnecting Loops | |
The Height Distribution of Hard X-Rays in Impulsive Solar Flares | |
High-Resolution Observations of Plasma Jets in the Solar Corona | |
Hinode/EIS plasma diagnostics in the flaring solar chromosphere | |
HαLINE PROFILE ASYMMETRIES AND THE CHROMOSPHERIC FLARE VELOCITY FIELD | |
Impulsive Heating of Solar Flare Ribbons Above 10 MK | |
Impulsive Phase Flare Energy Transport by Large‐Scale Alfvén Waves and the Electron Acceleration Problem | |
Impulsive thermal X-ray emission from a low-lying coronal loop | |
Invisible sunspots and rate of solar magnetic flux emergence | |
Lepton models for TeV emission from SNR RX J1713.7-3946 | |
Modeling of the Hydrogen Lyman Lines in Solar Flares | |
Modelling Particle Transport with Stochastic Simulations | |
Modelling the Longitudinal Asymmetry in Sunspot Emergence: The Role of the Wilson Depression | |
Multialtitude Observations of a Coronal Jet during the Third Whole Sun Month Campaign | |
Non-Gaussian Velocity Distributions in Solar Flares from Extreme Ultraviolet Lines: A Possible Diagnostic of Ion Acceleration | |
Numerical simulations of chromospheric hard X-ray source sizes in solar flares | |
The Observational Motivation for Computational Advances in Solar Flare Physics | |
Observations of conduction driven evaporation in the early rise phase of solar flares | |
Observations of enhanced extreme ultraviolet continua during an x-class solar flare using SDO/EVE | |
Observations of simultaneous coronal loop shrinkage and expansion during the decay phase of a solar flare | |
On the origin of a sunquake during the 2014 March 29 X1 flare | |
Onset of electron acceleration in a flare loop | |
The optical depth of white-light flare continuum | |
Optical spectral observations of a flickering white-light kernel in a C1 solar flare | |
Optimal filtering of solar images using soft morphological processing techniques | |
Overview of Solar Flares | |
Partially-erupting prominences: a comparison between observations and model-predicted observables | |
Physical properties of white-light sources in the 2011 February 15 solar flare | |
Plasma Diagnostics of Transition Region “Moss” using [ITAL]SOHO[/ITAL]/CDS and [ITAL]TRACE[/ITAL] | |
The plasmoid instability in a confined solar flare | |
Possible liquid water origin for Atacama Desert mudflow and recent gully deposits on Mars | |
Preface | |
Probing the Physics of the Solar Atmosphere with the Multi-slit Solar Explorer (MUSE). II. Flares and Eruptions | |
Propagation of alfvenic waves from Corona to chromosphere and consequences for solar flares | |
The radiated energy budget of chromospheric plasma in a major solar flare deduced from multi-wavelength observations | |
RADYNVERSION: Learning to Invert a Solar Flare Atmosphere with Invertible Neural Networks | |
Recent Advances in Understanding Particle Acceleration Processes in Solar Flares | |
Recruiting flare hunters for citizen science | |
Relationship between hard and soft X-ray emission components of a solar flare | |
The relative timing of supra-arcade downflows in solar flares | |
The role of filament activation in a solar eruption | |
Seismology of contracting and expanding coronal loops using damping of kink oscillations by mode coupling | |
Solar active region emergence and flare productivity | |
Solar And Cosmic Ray Physics And The Space Environment: Studies For And With LISA | |
Solar and stellar flares observations, simulations, and synergies | |
Solar Particle Acceleration Radiation and Kinetics (SPARK) | |
A solar tornado observed by EIS | |
The Spectral Content of SDO/AIA 1600 and 1700 Å Filters from Flare and Plage Observations | |
Spectroscopic Measurements of the Ion Velocity Distribution at the Base of the Fast Solar Wind | |
The Structure and Evolution of a Sigmoidal Active Region | |
Structures in the Outer Solar Atmosphere | |
Test-particle simulations of collisional impurity transport in rotating spherical tokamak plasmas | |
Triggering the Radio Emission from AE Aqr | |
Ultra-violet footpoints as tracers of coronal magnetic connectivity and restructuring during a solar flare | |
Unambiguous Evidence of Coronal Implosions during Solar Eruptions and Flares | |
Using Active Contours for Semi-Automated Tracking of UV and EUV Solar Flare Ribbons | |
Variation of solar oscillation frequencies in solar cycle 23 and their relation to sunspot area and number | |
Where is the chromospheric response to conductive energy input from a hot pre-flare coronal loop? | |
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