NSF award 2607293 · University of Hawaii

Unsupervised Identification of Coherent Structures: Linking Acceleration Mechanisms to Radiative Signatures in Relativistic Turbulence

Final report due

28 October 2029

in 1,106 days · The award ends on 30 June 2029.

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Decide about an extension2 Mar 2029in 866 days
award ending 2029-06-30 · Research.gov
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Extension request16 May 2029in 941 days
award ending 2029-06-30 · Research.gov
PAPPG 24-1: “at least 45 days prior to the end date”
No-cost extension notice20 Jun 2029in 976 days
award ending 2029-06-30 · Research.gov
PAPPG 24-1: “at least ten calendar days prior to the end date”
Final report due28 Oct 2029in 1106 days
award ending 2029-06-30 · Research.gov
PAPPG 24-1: “no later than 120-days following the end date of the award”
Project outcomes report due28 Oct 2029in 1106 days
award ending 2029-06-30 · Research.gov
PAPPG 24-1: “no later than 120 days following the end date”
Award is closed out28 Oct 2029in 1106 days
award ending 2029-06-30 · Research.gov
PAPPG 24-1: “financially closed out 120 days after their expiration date”

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NSF lists this award's end date as 30 June 2029.
NSF rules say the final report is due no later than 120 days after that.
So the final report is due by 28 October 2029.

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Award card

Award number: 2607293
Period of support: 1 Jul 2026 – 30 Jun 2029
Amount: $686,392
Awardee: University of Hawaii, Honolulu, HI
Program: PLASMA PHYSICS, OFFICE OF MULTIDISCIPLINARY AC
Directorate: MPS

Abstract

Some of the most powerful objects in the universe, such as the jets launched by supermassive black holes, the winds blown off rapidly spinning neutron stars, and the explosions known as gamma-ray bursts, produce enormous amounts of light and accelerate particles to energies far beyond anything achievable on Earth. Understanding the physical processes driving these extreme environments has direct bearing on our…

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