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Nicholeen Viall

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Nicholeen Viall is an American solar physicist who is the Chair of the American Astronomical Society's Solar Physics Division. Viall is known for her work on connecting dynamics of the solar corona to dynamics of the solar wind, based on observed variability of the corona-heliosphere system with both remote-sensing instruments and in-situ probes,[1] and for her work on understanding evolution of the plasma in the inner heliosphere.[2][3] She is the mission scientist for NASA's PUNCH mission, and a co-investigator on the ISS/CODEX and Parker Solar Probe/WISPR coronal imaging instruments.

Education

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Viall graduated from the University of Washington in 2004 with a Bachelors of Science in Astronomy and Physics. She received her Master of Arts in Astronomy at Boston University in 2007 and PhD in 2010.[4] She is a graduate of Kentwood High School.[5]

Honors and awards

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References

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  1. ^ Viall, N.M., Spence, H.E., Vourlidas, A., and Howard, R., "Examining Periodic Solar-Wind Density Structures Observed in the SECCHI Helisopheric Imagers", 2010, Solar Physics 261, 175.
  2. ^ Viall, N.M., and Borovsky, J.E., "Nine Outstanding Questions of Solar Wind Physics", 2020, J. Geophys. Res. Grand Challenges in the Earth and Space Sciences, 125.
  3. ^ Viall, N.M., DeForest, C.E., and Kepko, L., "Mesoscale Structure in the Solar Wind", 2021, Frontiers in Astronomy and Solar System Physics 8, 139.
  4. ^ "The Teams". Polarimeter to UNify the Corona and Heliosphere. Retrieved 17 July 2024.
  5. ^ Once in a Great While: 2000 Tapestry. Kentwood High School. 2000. p. 60.
  6. ^ "Cambridge: About the Eddington Lecture". Retrieved 13 March 2023.
  7. ^ "RAS: RAS Ordinary Meeting schedule, March 2023". Retrieved 13 March 2023.
  8. ^ "AAS/SPD: Harvey Prize Previous Winners". Retrieved 13 March 2023.
  9. ^ "NASA/GSFC Solar Physics Laboratory: Awards Won". Retrieved 13 March 2023.
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