David Stansby
Affiliations: | 2015-2019 | Imperial College London, London, England, United Kingdom | |
| 2019- | University College London |
Area:
solar physics, solar wind, heliosphereGoogle:
"David Stansby"Mean distance: (not calculated yet)
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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 |