Abstract
The three-to-five-month elliptical orbit of Parker Solar Probe (PSP), approaching within 10 solar radii of the Sun, will allow the Wide-field Imager for Solar Probe (WISPR) to view the corona with unprecedented spatial resolution from multiple viewpoints. WISPR has a wide fixed angular field of view, extending from \(13.5^{\circ}\) to \(108^{\circ}\) from the Sun and approximately \(50^{\circ}\) in the transverse direction, but the physical extent of the imaged coronal region varies directly with the distance of the spacecraft from the Sun. In a solar encounter period of approximately 10 days around perihelion, PSP covers over 100 – 200° of heliographic longitude and the distance from the Sun varies by a factor of two to five. In this paper, we use synthetic white-light images to study the effects of the rapid elliptical orbit on the images that can be anticipated for WISPR’s observations. We find that sequences of images can help identify coronal density features that will be sampled by in-situ instruments. We also find that the multiple viewpoints, provided by the rapid motion near perihelion, can be used to obtain three-dimensional information on the coronal density features.
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Acknowledgements
We gratefully acknowledge the help and support of Jeffrey R. Hall, JPL, William Thompson, Adnet System, Inc. and the WISPR team throughout this work. We are also thankful for early enthusiastic support from WISPR-team member Eric M. DeJong, JPL (deceased). This work was begun with the invaluable help of Caltech SURF student Yubo Su. The work of PCL was conducted at the Jet Propulsion Laboratory, California Institute of Technology under a contract from NASA. A.V. is supported by the WISPR Phase E program at APL. AT and RAH are supported by a contract from the NASA PSP program for the WISPR program. V.B. and G.N. acknowledge support of the Coronagraphic German and US SolarProbePlus Survey (CGAUSS) project for WISPR by the German Aerospace Center (DLR) under grant 50OL1901 as national contribution to the Parker Solar Probe mission.
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Liewer, P., Vourlidas, A., Thernisien, A. et al. Simulating White Light Images of Coronal Structures for WISPR/Parker Solar Probe: Effects of the Near-Sun Elliptical Orbit. Sol Phys 294, 93 (2019). https://doi.org/10.1007/s11207-019-1489-4
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DOI: https://doi.org/10.1007/s11207-019-1489-4