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David Stansby

Affiliations: 
2015-2019 Imperial College London, London, England, United Kingdom 
 2019- University College London 
Area:
solar physics, solar wind, heliosphere
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"David Stansby"
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Timothy Horbury grad student Imperial College London

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Publications

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Stansby D, Berčič L, Matteini L, et al. (2021) Sensitivity of solar wind mass flux to coronal temperature Astronomy & Astrophysics. 650: L2
Woodham LD, Horbury TS, Matteini L, et al. (2021) Enhanced proton parallel temperature inside patches of switchbacks in the inner heliosphere Astronomy & Astrophysics. 650: L1
Stansby D. (2020) In-situ Observations of the Sub-Alfvénic Solar Wind by Helios Research Notes of the Aas. 4: 51
Badman ST, Bale SD, Martínez Oliveros JC, et al. (2020) Magnetic Connectivity of the Ecliptic Plane within 0.5 au: Potential Field Source Surface Modeling of the First Parker Solar Probe Encounter The Astrophysical Journal Supplement Series. 246: 23
Möstl C, Weiss AJ, Bailey RL, et al. (2020) Prediction of the In Situ Coronal Mass Ejection Rate for Solar Cycle 25: Implications for Parker Solar Probe In Situ Observations The Astrophysical Journal. 903: 92
Němeček Z, Ďurovcová T, Šafránková J, et al. (2020) What is the Solar Wind Frame of Reference The Astrophysical Journal. 889: 163
Stansby D, Matteini L, Horbury TS, et al. (2020) The origin of slow Alfvénic solar wind at solar minimum Monthly Notices of the Royal Astronomical Society. 492: 39-44
Zouganelis I, De Groof A, Walsh AP, et al. (2020) The Solar Orbiter Science Activity Plan Astronomy & Astrophysics. 642: A3
Stansby D, Baker D, Brooks DH, et al. (2020) Directly comparing coronal and solar wind elemental fractionation Astronomy and Astrophysics. 640
Perrone D, D'Amicis R, Marco RD, et al. (2020) Highly Alfvénic slow solar wind at 0.3 au during a solar minimum: Helios insights for Parker Solar Probe and Solar Orbiter Astronomy and Astrophysics. 633
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