Saint Andrews University, School of Mathematics and Statistics
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Affiliated Works
sorted by decreasing year, and then by display-name
- TRACE, SOHO/EIT, and SOHO/MDI Observations of AR0030, Including Rotating Sunspots and the July 15, 2002 X3.0 Flare in Ultraviolet and Extreme Ultraviolet
- Coronal Seismology and the Propagation of Acoustic Waves Along Coronal Loops
- On the Role of Fast Shocks in Creating Relativistic Electrons in the Solar Corona
- Photospheric Oscillations in the Solar Atmosphere: Driving Chromospheric Spicules and Coronal Waves
- Feature Tracking of Hinode Magnetograms
- Optimization Approach for the Computation of 3D Magnetohydrostatic Coronal Equilibria From Multi-Spacecraft Observations
- Role of field line topology and anomalous viscosity and resistivity in the mechanism leading to the formation of the slow solar wind
- Theory, Simulations, and Laboratory Experiments of Auroral Kilometric Radiation
- Three-dimensional Resistive-MHD Model for X-ray Bright Points and Coronal Jets
- Nonlinear Force-Free Magnetic Field Modeling of the Solar Corona: A Critical Assessment
- Slip-Squashing Factors as a Measure of Three-Dimensional Magnetic Reconnection
- Electron thermal effects on electron acceleration and energy cascades in geomagnetic field line resonances
- Ionosphere-Magnetosphere Waves
- Production of narrow-scale Alfvén waves by E-region depletion, phase-mixing and feedback instability
- A Linear Stability Analysis of a Collisionless Distribution Function for the Force-Free Harris Sheet
- Loss Cone Evolution & Particle Escape In Collapsing Magnetic Trap Models
- The impact of cloud microphysical processes in the TTL on the water vapour budget of the stratosphere
- Heating and energetics in reconnecting twisted coronal loops in a gravitationally-atmosphere: effects of loop geometry and footpoint driving
- A Low Beta and Exact Kinetic Equilibrium for a 1D Nonlinear Force-Free field
- Are Tornado-Like Magnetic Structures Able to Support Solar Prominence Plasma?
- Symmetric MHD Equilibria with Anisotropic Pressure and Currents with a Field-Aligned Component
- A subsurface hydrology model that traces oxygen isotopes
- IRIS and SDO/AIA observations of coronal heating associated with spicules
- Reconnection Microjets in the Pre-eruption Phase of a Prominence/Coronal Rain Complex
- Theoretical models of non-Maxwellian equilibria for one-dimensional collisionless plasmas
- Observations and Modeling of Transition Region and Coronal Heating Associated with Spicules
- 3-D Simulation Study of the Spreading/Elongation of Ribbons in Two-Ribbon Flares
- First Determination of 2D Speed Distribution within the Bodies of Coronal Mass Ejections with Cross-correlation Analysis
- Sub-Alfvènic Spreading of 3D Collisionless Magnetic Reconnection and Application to Two-Ribbon Solar Flares
- Evolution of High-m Poloidal Alfven Waves in a Dipole Magnetic Field
- Metis - Solar Orbiter Topical Team on "Modelling of CME propagation/evolution in corona and solar wind in connection with Space Weather"
- Observations and numerical simulations of the relationship between ULF wave power, radial Alfvén speed profile, and magnetopause location
- Polarization Properties of Three Dimensional Alfvénic Field Line Resonances in a Compressed Dipole Magnetic Topology
- Scaling theory of magnetic reconnection spreading
- Studying CMEs with Metis on-board Solar Orbiter: constraints from synthetic data analysis