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Improved Forecasting of Solar Particle Events and their Effects on Space Electronics

Award Information
Agency: National Aeronautics and Space Administration
Branch: N/A
Contract: NNX16CG63C
Agency Tracking Number: 150014
Amount: $749,933.00
Phase: Phase II
Program: STTR
Solicitation Topic Code: T6.02
Solicitation Number: N/A
Solicitation Year: 2015
Award Year: 2016
Award Start Date (Proposal Award Date): 2016-09-27
Award End Date (Contract End Date): 2018-09-26
Small Business Information
701 McMillian Way Northwest, Suite D
Huntsville, AL 35806-2923
United States
HUBZone Owned: No
Woman Owned: No
Socially and Economically Disadvantaged: Yes
Principal Investigator
 Ashok Raman
 Senior Principal Engineer
 (256) 726-4800
Business Contact
 Silvia Harvey
Title: Business Official
Phone: (256) 726-4858
Research Institution
 The University of Alabama in Huntsville
 Gloria Greene
301 Sparkman Drive, NW
Huntsville, AL 35899-1911
United States

 (256) 824-2657
 Domestic Nonprofit Research Organization

High-energy space radiation from Galactic Cosmic Rays and Solar Particle Events (SPEs) pose significant risks to equipment and astronaut health in NASA missions. Energetic particles from SPEs associated with flares and coronal mass ejections (CMEs) may adversely affect not only beyond-Low-Earth-Orbit missions, but also aircraft avionics, communications, and airline crew/passenger health. It is crucial to develop a capability to forecast SPEs and their effects on systems to guide planning of mission-related tasks and risk mitigation strategies.
CFD Research Corporation (CFDRC), University of Alabama in Huntsville (UAH), and Vanderbilt University (VU) propose to develop a comprehensive forecasting capability - SPE Forecast (SPE4) - comprising state-of-the-art modules integrated within a novel computational framework. SPE4 will include: (a) the MAG4 code for probability forecasts of flares/CMEs, and SPEs, (b) the PATH code for solar particle transport through the heliosphere, (c) Geant4-based transport calculations including geomagnetic modulation and atmospheric interactions (for avionics) to yield spectra of SPE-induced energetic protons/heavy ions, interfaced to (d) the CR?ME96 code for calculation of resulting effects in electronics.
In Phase I, we demonstrated the superior capability of MAG4, PATH, and Geant4 for their respective tasks using a prior solar event case. A controller script was developed for automated code execution and data transfer across interfaces. Functionality of the overall event-to-effects capability was demonstrated using the 28-Sep-2012 event. We developed a concept of the final software product for NASA based on client-server architecture. In Phase II, we will collaborate with VU to interface calculated particle spectra with CR?ME96 to determine single-event effects in electronics. We will enhance robustness, accuracy, and execution speed via improved models and procedures, and demonstrate the software for persistent 24x7 SPE monitoring.

* Information listed above is at the time of submission. *

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