First-authored, refereed papers of D. Stansby
A list of first-authored, refereed publications of D. Stansby, derived from the SAO/NASA Astrophysics Data System (ADS). The number in brackets after each title indicates the number of citations that the paper has received.
Orcid ID: 0000-0002-1365-1908
List of publications ordered by citations
Number of papers: 10
No. of citations: 447
2021
- Sensitivity of solar wind mass flux to coronal temperature [10]
Stansby, D., Berčič, L., Matteini, L., Owen, C. J., French, R. J., Baker, D. & Badman, S. T., A&A, 650, L2
- Active Region Contributions to the Solar Wind over Multiple Solar Cycles [21]
Stansby, David, Green, Lucie M., van Driel-Gesztelyi, Lidia & Horbury, Timothy S., Solar Physics, 296, 116
2020
- The origin of slow Alfvénic solar wind at solar minimum [46]
Stansby, D., Matteini, L., Horbury, T. S., Perrone, D., D'Amicis, R. & Berčič, L., MNRAS, 492, 39
- Directly comparing coronal and solar wind elemental fractionation [26]
Stansby, D., Baker, D., Brooks, D. H. & Owen, C. J., A&A, 640, A28
- pfsspy: A Python package for potential field source surface modelling [109]
Stansby, David, Yeates, Anthony & Badman, Samuel, The Journal of Open Source Software, 5, 2732
2019
- Diagnosing solar wind origins using in situ measurements in the inner heliosphere [63]
Stansby, D., Horbury, T. S. & Matteini, L., MNRAS, 482, 1706
- Alpha particle thermodynamics in the inner heliosphere fast solar wind [43]
Stansby, D., Perrone, D., Matteini, L., Horbury, T. S. & Salem, C. S., A&A, 623, L2
2018
- Number density structures in the inner heliosphere [12]
Stansby, D. & Horbury, T. S., A&A, 613, A62
- A New Inner Heliosphere Proton Parameter Dataset from the Helios Mission [40]
Stansby, David, Salem, Chadi, Matteini, Lorenzo & Horbury, Timothy, Solar Physics, 293, 155
2016
- Experimental Determination of Whistler Wave Dispersion Relation in the Solar Wind [77]
Stansby, D., Horbury, T. S., Chen, C. H. K. & Matteini, L., The Astrophysical Journal Letters, 829, L16
Created on Tue Sep 22 04:29:20 2026.
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