NSF award 2605430 · Columbia University

Novel Measurements of Waves and Turbulence in the Corona using High Resolution DKIST Observations

Final report due

28 November 2029

in 1,137 days · The award ends on 31 July 2029.

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award ending 2029-07-31 · Research.gov
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award ending 2029-07-31 · Research.gov
PAPPG 24-1: “at least ten calendar days prior to the end date”
Final report due28 Nov 2029in 1137 days
award ending 2029-07-31 · Research.gov
PAPPG 24-1: “no later than 120-days following the end date of the award”
Project outcomes report due28 Nov 2029in 1137 days
award ending 2029-07-31 · Research.gov
PAPPG 24-1: “no later than 120 days following the end date”
Award is closed out28 Nov 2029in 1137 days
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PAPPG 24-1: “financially closed out 120 days after their expiration date”

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NSF rules say the final report is due no later than 120 days after that.
So the final report is due by 28 November 2029.

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Award card

Award number: 2605430
Period of support: 15 Aug 2026 – 31 Jul 2029
Amount: $519,971
Awardee: Columbia University, NEW York, NY
Program: PLANETARY ASTRONOMY
Directorate: MPS

Abstract

The solar corona is the Sun’s outer atmosphere, with temperatures of millions of degrees. Coronal heating theories aim to explain the high temperature of the corona. Wave-driven models of coronal heating posit that energy is transported to the corona by Alfvenic waves. Although most coronal heating models rely on turbulence, it is not known where and how Alfvenic turbulence emerges in the corona. The project will…

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