2021
DOI: 10.1029/2020ja029015
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The Cusp Plasma Imaging Detector (CuPID) CubeSat Observatory: Mission Overview

Abstract: Cube Satellites (CubeSats) are rapidly increasing in utility and have moved from primarily an education tool to a highly capable platform for scientific research. In-situ (Crew et al., 2016;Li et al., 2013) as well as remote sensing (Mason et al., 2016) measurements from CubeSat platforms have led to significant advances in space sciences. As the number of CubeSats launching into orbit increases rapidly each year (Swartwout, 2018), this platform will continue to serve as a test-bed for innovative technologies … Show more

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Cited by 9 publications
(5 citation statements)
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“…Additional design heritage stems from the CuPID cubesat mission which flew a single optic X-ray imager (Walsh et al. 2021 ; Atz et al. 2022a ).…”
Section: Instrument Designmentioning
confidence: 99%
See 1 more Smart Citation
“…Additional design heritage stems from the CuPID cubesat mission which flew a single optic X-ray imager (Walsh et al. 2021 ; Atz et al. 2022a ).…”
Section: Instrument Designmentioning
confidence: 99%
“…The DXL mission provided observational evidence for the solar wind charge-exchange contribution to the soft X-ray galactic background (Galeazzi et al 2014). Additional design heritage stems from the CuPID cubesat mission which flew a single optic X-ray imager (Walsh et al 2021;Atz et al 2022a). A similar tiled-MPO instrument has recently flown on the Lobster Eye Imager for Astronomy (LEIA) (Zhang et al 2022) and will soon be carried on the Soft X-ray Imager (SXI) (Sembay et al 2024) as part of the SMILE mission (Raab et al 2016).…”
Section: Instrument Designmentioning
confidence: 99%
“…The CuPID mission [34,35] is a six-unit (6U) Cube spacecraft project of NASA's CubeSat Launch Initiative (CSLI) [36]. To study macroscale properties of solar wind-magnetosphere interaction, i.e., dayside magnetopause reconnection, the spacecraft measures soft X-rays emitted from the process of charge-exchange between solar wind ions and neutral atoms in the magnetosheath and the magnetospheric cusps.…”
Section: Cusp Plasma Imaging Detector (Cupid; 2021 Usa)mentioning
confidence: 99%
“…Low‐energy (<30 keV) particle measurements from low‐altitude spacecraft (such as DMSP) have been used to identify the polar cap (or open/closed field line) boundary based on energy‐latitude dispersion of polar rain (<1 keV diffusive electrons in the polar cap) precipitation near this boundary (Gallardo‐Lacourt et al., 2022; Wing & Zhang, 2015; Winningham & Heikkila, 1974). Similar dispersion in low‐energy ions, also termed cusp ion steps, have been utilized to identify the cusp proper that is linked to the dayside magnetopause reconnection region (Heikkila & Winningham, 1971; Smith & Lockwood, 1996; Walsh et al., 2021). Newell and Meng (1992) used tens of thousands of individual particle precipitation measurements by the low‐altitude satellites of DMSP to construct an ionospheric map into various dayside magnetospheric regions, such as the dayside cusp, lower‐latitude boundary layer, mantle, plasma sheet, and polar rain, based on plasma precipitation characteristics with energies below ∼30 keV.…”
Section: Introductionmentioning
confidence: 99%