Paper
14 February 2003 Hard x-ray polarimetry with the Ramaty High Energy Solar Spectroscopic Imager (RHESSI)
Mark L. McConnell, David M. Smith, A. Gordon Emslie, Robert P. Lin, James M. Ryan
Author Affiliations +
Abstract
Although designed primarily as a hard X-ray imager and spectrometer, the Ramaty High Energy Solar Spectroscopic Imager (RHESSI) is also capable of measuring the polarization of hard X-rays (20-100 keV) from solar flares. This capability arises from the inclusion of a small unobstructed Be scattering element that is strategically located within the cryostat that houses the array of nine germanium detectors. The Ge detectors are segmented, with both a front and rear active volume. Low energy photons (below about 100 keV) can reach a rear segment of a Ge detector only indirectly, by scattering. Low energy photons from the Sun have a direct path to the Be and have a high probability of Compton scattering into a rear segment of a Ge detector. The azimuthal distribution of these scattered photons carries with it a signature of the linear polarization of the incident flux. Sensitivity estimates, based on simulations and in-flight background measurements, indicate that a 20-100 keV polarization sensitivity of less than a few percent can be achieved for X-class flares.
© (2003) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Mark L. McConnell, David M. Smith, A. Gordon Emslie, Robert P. Lin, and James M. Ryan "Hard x-ray polarimetry with the Ramaty High Energy Solar Spectroscopic Imager (RHESSI)", Proc. SPIE 4843, Polarimetry in Astronomy, (14 February 2003); https://doi.org/10.1117/12.458879
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Cited by 4 scholarly publications.
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KEYWORDS
Polarization

Photons

Sensors

Scattering

Germanium

Polarimetry

Modulation

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