13 citations as recorded by crossref.

1. Evaluation of a potential field source surface model with elliptical source surfaces via ballistic back mapping of in situ spacecraft data M. Kruse et al. 10.1051/0004-6361/202039120
2. Modeling CME encounters at Parker Solar Probe with OSPREI: Dependence on photospheric and coronal conditions V. Ledvina et al. 10.1051/0004-6361/202245445
3. A New View of the Coupling of the Sun and the Heliosphere T. Zurbuchen 10.1146/annurev.astro.45.010807.154030
4. Quantifying the Difference Between the Flux-Tube Expansion Factor at the Source Surface and at the Alfvén Surface Using a Global MHD Model for the Solar Wind O. Cohen 10.1007/s11207-015-0739-3
5. An elliptic expansion of the potential field source surface model M. Kruse et al. 10.1051/0004-6361/202037734
6. Coronal Field Opens at Lower Height During the Solar Cycles 22 and 23 Minimum Periods: IMF Comparison Suggests the Source Surface Should Be Lowered C. Lee et al. 10.1007/s11207-010-9699-9
7. Solar cycle changes in coronal holes and space weather cycles J. Luhmann et al. 10.1029/2001JA007550
8. Estimating uncertainties in the back-mapping of the fast solar wind A. Koukras et al. 10.1051/0004-6361/202244327
9. Three-dimensional inversion of corona structure and simulation of solar wind parameters based on the photospheric magnetic field deduced from the Global Oscillation Network Group X. Zhang et al. 10.3389/fspas.2023.1234391
10. Reconstructing Coronal Hole Areas With EUHFORIA and Adapted WSA Model: Optimizing the Model Parameters E. Asvestari et al. 10.1029/2019JA027173
11. A new stationary analytical model of the heliospheric current sheet and the plasma sheet R. Kislov et al. 10.1002/2015JA021294
12. Adjusting the Potential Field Source Surface Height Based on Magnetohydrodynamic Simulations Z. Huang et al. 10.3847/2041-8213/ad3547
13. On Solutions of the PFSS Model With GONG Synoptic Maps for 2006–2018 L. Nikolić 10.1029/2019SW002205