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Eric Priest (astrophysicien, en poste à l'University of St. Andrews, Ecosse)
Eric Priest (British mathematician)
Priest, E. R.
Priest, Eric R.
Priest, Eric Ronald
Ballester, J. L.
Forbes, Terry (1946-...)
Harris, Robert Alan (1943-...)
Instituto de astrofísica de Canarias
Kirk, J. G.
Kirk, John G.
Melrose, Don B. (1940-)
Melrose, Donald B. (1940-)
Russell, C. T.
Ulmschneider, P. (1938-)
Ulmschneider, Peter (1938- ))
Ulmschneider, Peter (1938-)
Union astronomique internationale, Symposium 142 1989
University of St Andrews
3D reconnection of untwisted magnetic flux tubes
3D topology and interaction of complex magnetic flux systems, The
A Flux-Tube Tectonics Model for Solar Coronal Heating Driven by the Magnetic Carpet/a, a href='http://www-solar.mcs.st-andrews.ac.uk/~eric/PAPERS/tectonics.pdf'
Alfven wave support of a dwarf molecular cloud. I. an isothermal model.
analytical MHD wind model with latitudinal dependences obtained using separation of the variables, An
Aspects of Three-Dimensional Magnetic Reconnection - (Invited Review)
Basic plasma processes on the sun proceedings of the 142nd Symposium of the International Astronomical Union, held in Bangalore, India, December 1-5, 1989
Basic properties of complex magnetic fields and magnetic reconnection of the sun
Bifurcations of magnetic topology by the creation or annihilation of null points.
Binary reconnection and the heating of the solar corona/a, a href='http://www-solar.mcs.st-andrews.ac.uk/~eric/PAPERS/binary.pdf'
Can we Extrapolate a Magnetic Field when its Topology is Complex?
CDS theory and analysis
Coronal heating at separators and separatrices
Creativity in science
Current sheets in the Sun's corona
Dipped Magnetic Field Configurations Associated with Filaments and Barbs
Dynamics and structure of quiescent solar prominences
EU Network PLATON
Evolution of magnetic flux in an isolated reconnection process/a, a href='http://www-solar.mcs.st-andrews.ac.uk/~eric/PAPERS/nature.pdf'
evolution of the Sun's open magnetic flux. I. A single bipole, The
Evolution of the Sun's Open Magnetic Flux - II. Full Solar Cycle Simulations, The
Exact MHD Solutions near null points, Physics of magnetic Reconnection
Exact solutions for spine reconnective magnetic annihilation
Exploitation of data from the CDS & SUMER instruments of soho
Flare activity in solar active region 8421 observed by the TRACE satellite
Flux-Tube Tectonics Model for Solar Coronal Heating Driven by the Magnetic Carpet, A
Force-free and Potential Models of a Filament Channel in Which a Filament Forms
framework for understanding the topology of complex coronal structures, A
Fundamentals of activity processes in solar system plasmas. (Supplement)
Generalization of a special class of time-dependent solutions of the two-dimensional magnetohydrodynamic equations to arbitrary pressure profiles
Heating of coronal holes by phase mixing.
Heating of the Solar Corona, The
Heating the Solar Corona by Magnetic Reconnection
How accurately can we determine the coronal heating mechanism in the large-scale solar corona?
How is the solar corona headed?
Importance of Photospheric Intense Flux Tubes for Coronal Heating, The
Kinematic reconnection at a magnetic null point: Spine-aligned current
Linear collapse of spatially linear 2D null points
Linear collapse of spatially linear 3D potential null points
Low-order stellar dynamo models
Magnetic Activity in Stars, Discs and Quasars
Magnetic diffusion and the motion of field lines
Magnetic Flux Transport and the Formation of Filament Channels on the Sun
magnetic nature of solar flares, The
Magnetic null points due to multiple sources of solar photospheric flux
Magnetic reconnection at the sun
Magnetic reconnection. MHD theory and applications
Magnetic reconnection on the sun
Magnetic topologies due to two bipolar regions
Magnetic topologies in the solar corona due to four discrete photospheric flux regions
Mean Field Model for the Formation of Filament Channels on the Sun
Mechanisms of chromospheric and coronal heating : proceedings of the international conference, Heidelberg, 5-8 June 1990
Method to Determine the Heating Mechanisms of the Solar Corona, A
model for elemental coronal flux tubes, A
nature of blinkers and the solar transition region, The
nature of the heating mechanism for the diffuse solar corona, The
Numerical experiments on wave propagation towards a 3D null point due to rotational motion
Numerical experiments on wave propagation towards a 3D null point due to rotational motions
Numerical simulations of the flux tube tectonics model for coronal heating
On the distribution of magnetic null points above the solar photosphere
On the location of energy release and temperature profiles along coronal loops
On the nature of chaotic regions in dissipative hydrodynamics and magnetohydrodynamics
On the nature of three-dimensional magnetic reconnection
Our Magnetic Sun
Phase-mixing in Dissipative Alfven Waves
Physics of magnetic flux ropes
Proceedings of the conference, a crossroads for European solar and heliospheric physics : recent achievements and future mission possibilities : Puerto de la Cruz, Tenerife, Canary Islands, Spain, March 23-27 1998
Reconnection and coronal heating
Reconnection theory in solar physics
Recycling of the Solar Corona's Magnetic Field/a, a href='http://dx.doi.org/10.1086/424659'
Role of Helicity in the Formation of Intermediate Filaments
Separators in 3D Magnetic Fields
Short and long term visitors in solar theory
Simulations of Three-Dimensional Reconnection in the Solar Corona
Solar and Magnetospheric MHD Theory
Solar Flare Theory and the Status of Flare understanding
Solar magnetohydrodynamics and its interaction with other disciplines
Solar MHD Theory Group
Solar-Stellar Connection: Our New Sun, The
Solar system magnetic fields
Solar System MHD Theory
Stability of astrophysical plasmas
Statistical flux tube properties of 3D magnetic carpet fields
Structure and collapse of three-dimensional magnetic neutral points.
study of the unification of quiet-sun transient-event phenomena, A
Sunspots reveal their dark side
Surprises from Our Sun
Theory of 3D reconnection and coronal heating
Theory of Magnetic Reconnection Undergraduate Research Bursary 2003
Three-dimensional magnetic reconnection in the solar corona
Three-dimensional reconnection on the Sun
Three-dimensional separator reconnection - How does it occur?
topological behaviour of 3D null points in the Sun's corona, The
Topological Behaviour of Stable Magnetic Separators, The
Topological bifurcations in three-dimensional magnetic fields.
Topological differences and similarities between force-free and potential models of coronal magnetic fields
Visco-resistive magnetic reconnection due to steady inertialess flows. I. Exact analytical solutions
Visitors in Solar and Magnetospheric MHD
Visitors in solar mhd theory
wavelet analysis of active region oscillations, A
Contributed to or performed:
ASTRONOMICAL SOCIETY OF THE PACIFIC CONFERENCE SERIES
EARTH PLANETS AND SPACE
JOURNAL OF ATMOSPHERIC AND SOLAR TERRESTRIAL PHYSICS
PHYSICS OF PLASMAS