The supplemental science analyses proposed above asks important questions concerning the origins of solar wind structures that are of high interest and potential impact. Icme topologies tell US…

Ended Grant For Research Awarded Last action

Contract number
80NSSC22K1359
Awardee
Awarding agency
Obligated
$499,712

Award facts

Contract value 100% obligated
$499,712.05 Current and potential, with all options
Completion date 100% complete
Current and potential, with all options
NAICS code
Not on record
Set-aside
No set-aside
Competition
Not Competed Basic Research
Pricing
Other
Place of performance
Berkeley, CA 94710, USA

Award details come from SAM.gov/FPDS.

Transactions

Action Obligated Date
Other Administrative Action P00002 $0
Other Administrative Action P00001 · Opportunistic science targets for the stereo impact (in-situ measurements of particles and CME transients) investigation $0
Original award $499,712

About this award

This is a $499,712.05 grant awarded by NASA to the University of California, Berkeley (UC Berkeley) to conduct research on the origins and properties of solar wind structures and solar energetic particle (SEP) events. The research aims to improve our understanding of the 3D structure of the heliosphere and solar wind, building upon the goals of the NASA STEREO mission. The grant does not have a set-aside designation. UC Berkeley is the prime contractor, and the parent organization is the State of California Controller's Office, which will administer any resulting funding. The research is expected to enhance the contributions of the STEREO in-situ observations to high-profile heliophysics studies, including investigations into coronal mass ejections, ground-level enhancement events, and interplanetary fine structures.

Description

The supplemental science analyses proposed above asks important questions concerning the origins of solar wind structures that are of high interest and potential impact. Icme topologies tell US about both the origins of these heliospheric disturbances as well as improve the possibilities for forecasting geoeffective events. GLE events are attracting major interest with the increasing preparations for sending humans into deeper space. The IFE phenomenon can tell US more about the sources of the solar wind if they are created by entanglement of flux ropes originating from the sun or inner heliosphere, or they can improve our understanding of the heliosphere dust environment if they are created from solar wind-dust interactions. The proposed enhanced SEP heavy ION data set will improve the uses of stereo data toward understanding SEP sources. Overall, the studies described above build upon the original goals of stereo itself to understand the 3D structure of the heliosphere and solar wind- and enhance the contributions of the stereo in-situ observations to the latest high profile heliophysics research.

Quick answers

Who was awarded contract 80NSSC22K1359?

80NSSC22K1359 was awarded to The Regents Of The University Of California by Shared Services Center (National Aeronautics and Space Administration) on August 1, 2022.

How much is contract 80NSSC22K1359 worth?

The government has obligated $499,712 on 80NSSC22K1359.

Was contract 80NSSC22K1359 competed?

The extent of competition for 80NSSC22K1359 was not competed.

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