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2019
Authors: Riley Pete, Downs Cooper, Linker Jon A., Mikic Zoran, Lionello Roberto, et al.
Title: Predicting the Structure of the Solar Corona and Inner Heliosphere during Parker Solar Probe 's First Perihelion Pass
Abstract:

NASA’s Parker Solar Probe (PSP) spacecraft reached its first perihelion of 35.7 solar radii on 2018 November 5. To aid in mission planning, and in anticipation of the unprecedented measurements to be returned, in late October, we developed a three-dimensional magnetohydrodynamic (MHD) solution for the solar corona and inner heliosphere, driven by the then available observations of the Sun’s photospheric magnetic field. Our model incorporates a wave-turbulence-driven model to heat the corona. Here, we present our predictions for the structure of the solar corona and the likely in situ measurements that PSP will be returning over the next few months. We infer that, in the days prior to first encounter, PSP was immersed in wind emanating from a well-established, positive-polarity north. . .
Date: 04/2019 Publisher: The Astrophysical Journal Pages: L15 DOI: 10.3847/2041-8213/ab0ec3 Available at: http://stacks.iop.org/2041-8205/874/i=2/a=L15?key=crossref.94a3f13ef95cab063c2cc60115d0f410http://stacks.iop.org/2041-8205/874/i=2/a=L15/pd
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Authors: Lamy Philippe, Floyd Olivier, Mikic Zoran, and Riley Pete
Title: Validation of MHD Model Predictions of the Corona with LASCO-C2 Polarized Brightness Images
Abstract:

Progress in our understanding of the solar corona requires that the results of advanced magnetohydrodynamic models driven by measured magnetic fields, and particularly the underlying heating models, be thoroughly compared with coronal observations. The comparison has so far mainly concerned the global morphology of the corona, synthetic images calculated from the models being compared with observed images. We go one step further by performing detailed quantitative comparisons between the calculated polarized radiance p B using the three-dimensional electron density produced by MHD models and well calibrated polarized images obtained by the Large Angle Spectrometric Coronagraph LASCO-C2 coronagraph complemented by ground-based images when available from the Mauna Loa Solar Observatory Ma. . .
Date: 11/2019 Publisher: Solar Physics DOI: 10.1007/s11207-019-1549-9 Available at: http://link.springer.com/10.1007/s11207-019-1549-9http://link.springer.com/content/pdf/10.1007/s11207-019-1549-9.pdfhttp://link.springer.com/content/pdf/10.1007/s11207-019-1549-9.pdfhttp://link.springer.com/article/10.1007/s11207-019-1549-9/fulltext.html
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2016
Authors: Vourlidas Angelos, Howard Russell A., Plunkett Simon P., Korendyke Clarence M., Thernisien Arnaud F. R., et al.
Title: The Wide-Field Imager for Solar Probe Plus (WISPR)
Abstract: N/A
Date: 02/2015 Publisher: Space Science Reviews Pages: 83 - 130 DOI: 10.1007/s11214-014-0114-y Available at: http://link.springer.com/content/pdf/10.1007/s11214-014-0114-y.pdf
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2013
Authors: Vourlidas Angelos, Howard Russell A., Plunkett Simon P., Korendyke Clarence M., Carter Michael T., et al.
Title: SPIE ProceedingsSeeing the corona with the solar probe plus mission: the wide-field imager for solar probe+ (WISPR)
Abstract: N/A
Date: 09/2013 Publisher: SPIE DOI: 10.1117/12.2027508 Available at: http://proceedings.spiedigitallibrary.org/proceeding.aspx?doi=10.1117/12.2027508
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