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Proceedings Article

Detector and imaging systems for the gamma-ray imager/polarimeter for solar flares (GRIPS) instrument

[+] Author Affiliations
Nicole Duncan, Gordon Hurford, Pascal Saint-Hilaire, Andreas Zoglauer, Hazel Bain, Steven Boggs, Robert Lin

Space Sciences Lab., Univ. of California, Berkeley (United States)

Albert Shih

NASA Goddard Space Flight Ctr. (United States)

Mark Amman

Lawrence Berkeley National Lab. (United States)

Proc. SPIE 8862, Solar Physics and Space Weather Instrumentation V, 88620W (September 26, 2013); doi:10.1117/12.2024667
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From Conference Volume 8862

  • Solar Physics and Space Weather Instrumentation V
  • Silvano Fineschi; Judy Fennelly
  • San Diego, California, United States | August 25, 2013

abstract

Hard X-ray and gamma-ray emission during solar flares encode information about electron/ion dynamics and provide a proxy to deduce solar atmospheric parameters. Enhanced imaging, spectroscopy and polarimetry of HXR/gamma-ray are emissions over ~20 keV to greater than or approx. equal to 10MeV is needed to study particle transport; the Gamma-Ray Imager/Polarimeter for Solar Flares (GRIPS) instrument is designed to meet these goals. GRIPS' key technological improvements over the current solar state of the art in HXR/gamma-ray energies (RHESSI) include 3D position-sensitive germanium detectors (3D-GeDs) and a single-grid modulation collimator, the Multi-Pitch Rotating Modulator (MPRM). The 3D-GeDs allow GRIPS to reconstruct Compton-scatter tracks of energy deposition, providing enhanced background reduction and polarization measurements. Each of GRIPS' sixteen detectors has 298 electrode strips, each of which has dedicated ASIC/FPGA electronics. In GRIPS' energy range, indirect Fourier imaging provides higher resolution than focusing optics or Compton imaging techniques. The MPRM grid-imaging system has a single-grid design which provides 2x the throughput of a bigrid imaging system like RHESSI. Quasi-continuous resolution from 12.5 - 162 arcsecs is achieved by varying the grid pitch between 1 - 13mm. This spatial resolution will be capable of imaging the separate footpoints in a variety of flare sizes. In comparison, RHESSI's minimum 35 arcsec resolution at the same energy makes footpoints resolvable in only the largest flares. We discuss GRIPS' science goals, the instrument overall, and recent developments in GRIPS' detector and imaging systems. GRIPS is scheduled for an engineering flight from Fort Sumner in September 2014, followed by two long-duration balloon flights from Antarctica in 2015/16. © (2013) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Citation

Nicole Duncan ; Albert Shih ; Gordon Hurford ; Pascal Saint-Hilaire ; Andreas Zoglauer, et al.
" Detector and imaging systems for the gamma-ray imager/polarimeter for solar flares (GRIPS) instrument ", Proc. SPIE 8862, Solar Physics and Space Weather Instrumentation V, 88620W (September 26, 2013); doi:10.1117/12.2024667; http://dx.doi.org/10.1117/12.2024667


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