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LargE Area burst Polarimeter (LEAP) Phase A Support, 15-R6078

Principal Investigator
Inclusive Dates 
06/08/20 - Current

Background

Theoretical models show that a more complete understanding of the inner structure of gamma-ray bursts (GRBs), including the geometry and physical processes close to the central engine, requires the exploitation of gamma-ray polarimetry. In 2019, we proposed a NASA Astrophysics Mission of Opportunity (MoO) project called LEAP (LargE Area burst Polarimeter) that would address this science by mounting a gamma-ray polarimeter (covering photons in the energy range of 50–500 keV) on the outside of the International Space Station (ISS). The full instrument consists of an array of seven independent polarimeter modules. The large effective area, large field-of-view, and continuous exposure to deep space make it an effective instrument for studying gamma-ray bursts and other transient astrophysical phenomena, including solar flares. If selected for flight, LEAP would be deployed in 2025 for a 2.5-year mission. LEAP is a collaborative effort between SwRI, the University of New Hampshire, the Marshall Space Flight Center, the University of Alabama at Huntsville, and Teledyne Brown Engineering. LEAP was one of two MoO proposals selected by NASA for a Phase A Concept Study, with the Concept Study Report (CSR) due in March 2021, and final flight selection expected in summer of 2021.

Approach

The Phase A study focuses on refining the LEAP instrument design. The instrument will be fabricated at the University of New Hampshire (UNH) with significant support from SwRI. The role of SwRI will include the following:

  • SwRI will design and develop the Central Electronics Box (CEB), including the flight software. The CEB will be responsible for controlling the LEAP instrument, collecting data from the polarimeter modules and from the star tracker, formatting the data, and passing the data onto the ISS for transmission to the ground.
  • SwRI will design and develop the digital electronics board for processing of signals within the polarimeter.
  • SwRI is supporting the instrument mechanical design and instrument systems engineering.
  • SwRI will provide support for SMA during instrument development at UNH.
  • SwRI is supporting the development of a laboratory prototype demonstration during Phase A.
  • SwRI is supporting the preparation of the final CSR during Phase A.
an array of seven independent polarimeter modules

Figure 1: The LEAP instrument (the array of seven square modules) as it would be attached to the ISS.

Accomplishments

Work in developing the CSR is progressing. The deadline for the final CSR is March 4, 2021. A NASA site visit is expected to take place in late May or early June of 2021.