David Stansby
www.davidstansby.com
0000-0002-1365-1908
University College London
20 papers found
Refreshing results…
In-situ Observations of the Sub-Alfvénic Solar Wind by Helios
Signatures of Coronal Loop Opening via Interchange Reconnection in the Slow Solar Wind at 1 AU
What is the Solar Wind Frame of Reference?
Magnetic Connectivity of the Ecliptic Plane within 0.5 au: Potential Field Source Surface Modeling of the First Parker Solar Probe Encounter
Highly Alfvénic slow solar wind at 0.3 au during a solar minimum: Helios insights for Parker Solar Probe and Solar Orbiter
Linear Stability in the Inner Heliosphere: Helios Re-evaluated
The origin of slow Alfvénic solar wind at solar minimum
Thermodynamics of pure fast solar wind: radial evolution of the temperature–speed relationship in the inner heliosphere
Towards Construction of a Solar Wind “Reanalysis” Dataset: Application to the First Perihelion Pass of Parker Solar Probe
The rotation angle distribution underlying magnetic field fluctuations in the 1/f range of solar wind turbulent spectra
Predicting Large-scale Coronal Structure for Parker Solar Probe Using Open Source Software
Alpha particle thermodynamics in the inner heliosphere fast solar wind
On the 1/ f Spectrum in the Solar Wind and Its Connection with Magnetic Compressibility
Snakes on a Spaceship—An Overview of Python in Heliophysics
Radial evolution of the solar wind in pure high-speed streams: HELIOS revised observations
A New Inner Heliosphere Proton Parameter Dataset from the Helios Mission
Diagnosing solar wind origins usingin situmeasurements in the inner heliosphere
Number density structures in the inner heliosphere
Short, large-amplitude speed enhancements in the near-Sunfast solar wind
Experimental Determination of Whistler Wave Dispersion Relation in the Solar Wind
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