Presentation
26 August 2022 The IMpulsive Phase Rapid Energetic Solar Spectrometer (IMPRESS) CubeSat
Author Affiliations +
Abstract
In the past two decades, great advances have been made in investigating hard X-rays from accelerated electrons in solar flares. This emission is of interest because the means by which flares so efficiently accelerate particles are still not understood. Observations from the RHESSI spacecraft led to better understanding in the imaging and spectral domains, but presented difficulty for time domain analysis at scales less than ~2 seconds. This leaves the behavior of flare emission at small timescales poorly explored. The NSF-funded IMpulsive Phase Rapid Energetic Solar Spectrometer (IMPRESS) CubeSat is designed specifically to measure hard X-ray emission up to 100 keV from flares at a tens-of-ms cadence. This will provide novel constraints for flare particle acceleration models. IMPRESS is a student-centered collaboration between UMN, MSU, SwRI, and UCSC. This presentation will describe the science, mission concept, and some design specifics for IMPRESS.
Conference Presentation
© (2022) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Lindsay Glesener, Demoz Gebre-Egziabher, John Sample, Amir Caspi, David M. Smith, William Setterberg, Ty Kozic, Mansour Savadogo, Christian Berger, Lestat Clemmer, Robert Drake, Allan Faulkner, Annsley Greathouse, Kate Hildebrandt, Runsheng Ma, Mel Nightingale, Meredith Wieber, Trevor Knuth, Kyle Houser, Rubin Meuchel, and Larry Springer "The IMpulsive Phase Rapid Energetic Solar Spectrometer (IMPRESS) CubeSat", Proc. SPIE 12181, Space Telescopes and Instrumentation 2022: Ultraviolet to Gamma Ray, 121810I (26 August 2022); https://doi.org/10.1117/12.2630498
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KEYWORDS
Spectroscopy

Hard x-rays

Particles

Scintillators

Sensors

Silicon

Solar processes

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