Capabilities and performance of the high-energy energetic-particles instrument for the parker solar probe mission

M. E. Wiedenbeck; N. G. Angold; B. Birdwell; J. A. Burnham; E. R. Christian; C. M.S. Cohen; W. R. Cook; R. M. Crabill; A. C. Cummings; A. J. Davis; G. Dirks; D. H. Do; D. T. Everett; P. A. Goodwin; J. J. Hanley; L. Hernandez; B. Kecman; J. Klemic; A. W. Labrador; R. A. Leske; S. Lopez; J. T. Link; D. J. McComas; R. A. Mewaldt; H. Miyasaka; B. W. Nahory; J. S. Rankin; G. Riggans; B. Rodriguez; M. D. Rusert; S. A. Shuman; K. M. Simms; E. C. Stone; T. T. Von Rosenvinge; S. E. Weidner; M. L. White

Capabilities and performance of the high-energy energetic-particles instrument for the parker solar probe mission

M. E. Wiedenbeck
, N. G. Angold
, B. Birdwell
, J. A. Burnham
, E. R. Christian
, C. M.S. Cohen
, W. R. Cook
, R. M. Crabill
, A. C. Cummings
, A. J. Davis
, G. Dirks
, D. H. Do
, D. T. Everett
, P. A. Goodwin
, J. J. Hanley
, L. Hernandez
, B. Kecman
, J. Klemic
, A. W. Labrador
, R. A. Leske

S. Lopez, J. T. Link, D. J. McComas, R. A. Mewaldt, H. Miyasaka, B. W. Nahory, J. S. Rankin, G. Riggans, B. Rodriguez, M. D. Rusert, S. A. Shuman, K. M. Simms, E. C. Stone, T. T. Von Rosenvinge, S. E. Weidner, M. L. White

Astrophysical Sciences

Research output: Contribution to journal › Conference article › peer-review

Abstract

NASA's Parker Solar Probe (PSP) spacecraft (formerly Solar Probe Plus) is scheduled for launch in July 2018 with a planned heliocentric orbit that will carry it on a series of close passes by the Sun with perihelion distances that eventually will get below 10 solar radii. Among other in-situ and imaging sensors, the PSP payload includes the two-instrument "Integrated Science Investigation of the Sun" suite, which will make coordinated measurements of energetic ions and electrons. The high-energy instrument (EPI-Hi), operating in the MeV energy range, consists of three detector-telescopes using silicon solid-state sensors for measuring composition, energy spectra, angular distributions, and time structure in solar energetic particle events. The expected performance of this instrument has been studied using accelerator calibrations, radioactive-source tests, and simulations. We present the EPI-Hi measurement capabilities drawing on these calibration data and simulation results for illustrations.

Original language	English (US)
Journal	Proceedings of Science
State	Published - 2017
Event	35th International Cosmic Ray Conference, ICRC 2017 - Bexco, Busan, Korea, Republic of Duration: Jul 10 2017 → Jul 20 2017

All Science Journal Classification (ASJC) codes

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Cite this

Wiedenbeck, M. E., Angold, N. G., Birdwell, B., Burnham, J. A., Christian, E. R., Cohen, C. M. S., Cook, W. R., Crabill, R. M., Cummings, A. C., Davis, A. J., Dirks, G., Do, D. H., Everett, D. T., Goodwin, P. A., Hanley, J. J., Hernandez, L., Kecman, B., Klemic, J., Labrador, A. W., ... White, M. L. (2017). Capabilities and performance of the high-energy energetic-particles instrument for the parker solar probe mission. Proceedings of Science.

@article{661bd3fa703948e39acc0cc0653dd46a,

title = "Capabilities and performance of the high-energy energetic-particles instrument for the parker solar probe mission",

abstract = "NASA's Parker Solar Probe (PSP) spacecraft (formerly Solar Probe Plus) is scheduled for launch in July 2018 with a planned heliocentric orbit that will carry it on a series of close passes by the Sun with perihelion distances that eventually will get below 10 solar radii. Among other in-situ and imaging sensors, the PSP payload includes the two-instrument {"}Integrated Science Investigation of the Sun{"} suite, which will make coordinated measurements of energetic ions and electrons. The high-energy instrument (EPI-Hi), operating in the MeV energy range, consists of three detector-telescopes using silicon solid-state sensors for measuring composition, energy spectra, angular distributions, and time structure in solar energetic particle events. The expected performance of this instrument has been studied using accelerator calibrations, radioactive-source tests, and simulations. We present the EPI-Hi measurement capabilities drawing on these calibration data and simulation results for illustrations.",

author = "Wiedenbeck, \{M. E.\} and Angold, \{N. G.\} and B. Birdwell and Burnham, \{J. A.\} and Christian, \{E. R.\} and Cohen, \{C. M.S.\} and Cook, \{W. R.\} and Crabill, \{R. M.\} and Cummings, \{A. C.\} and Davis, \{A. J.\} and G. Dirks and Do, \{D. H.\} and Everett, \{D. T.\} and Goodwin, \{P. A.\} and Hanley, \{J. J.\} and L. Hernandez and B. Kecman and J. Klemic and Labrador, \{A. W.\} and Leske, \{R. A.\} and S. Lopez and Link, \{J. T.\} and McComas, \{D. J.\} and Mewaldt, \{R. A.\} and H. Miyasaka and Nahory, \{B. W.\} and Rankin, \{J. S.\} and G. Riggans and B. Rodriguez and Rusert, \{M. D.\} and Shuman, \{S. A.\} and Simms, \{K. M.\} and Stone, \{E. C.\} and \{Von Rosenvinge\}, \{T. T.\} and Weidner, \{S. E.\} and White, \{M. L.\}",

note = "Publisher Copyright: {\textcopyright} Copyright owned by the author(s) under the terms of the Creative Commons Attribution-Non Commercial-No Derivatives 4.0 International License (CC BY-NC-ND 4.0).; 35th International Cosmic Ray Conference, ICRC 2017 ; Conference date: 10-07-2017 Through 20-07-2017",

year = "2017",

language = "English (US)",

journal = "Proceedings of Science",

issn = "1824-8039",

publisher = "Sissa Medialab Srl",

}

Wiedenbeck, ME, Angold, NG, Birdwell, B, Burnham, JA, Christian, ER, Cohen, CMS, Cook, WR, Crabill, RM, Cummings, AC, Davis, AJ, Dirks, G, Do, DH, Everett, DT, Goodwin, PA, Hanley, JJ, Hernandez, L, Kecman, B, Klemic, J, Labrador, AW, Leske, RA, Lopez, S, Link, JT, McComas, DJ, Mewaldt, RA, Miyasaka, H, Nahory, BW, Rankin, JS, Riggans, G, Rodriguez, B, Rusert, MD, Shuman, SA, Simms, KM, Stone, EC, Von Rosenvinge, TT, Weidner, SE & White, ML 2017, 'Capabilities and performance of the high-energy energetic-particles instrument for the parker solar probe mission', Proceedings of Science.

TY - JOUR

T1 - Capabilities and performance of the high-energy energetic-particles instrument for the parker solar probe mission

AU - Wiedenbeck, M. E.

AU - Angold, N. G.

AU - Birdwell, B.

AU - Burnham, J. A.

AU - Christian, E. R.

AU - Cohen, C. M.S.

AU - Cook, W. R.

AU - Crabill, R. M.

AU - Cummings, A. C.

AU - Davis, A. J.

AU - Dirks, G.

AU - Do, D. H.

AU - Everett, D. T.

AU - Goodwin, P. A.

AU - Hanley, J. J.

AU - Hernandez, L.

AU - Kecman, B.

AU - Klemic, J.

AU - Labrador, A. W.

AU - Leske, R. A.

AU - Lopez, S.

AU - Link, J. T.

AU - McComas, D. J.

AU - Mewaldt, R. A.

AU - Miyasaka, H.

AU - Nahory, B. W.

AU - Rankin, J. S.

AU - Riggans, G.

AU - Rodriguez, B.

AU - Rusert, M. D.

AU - Shuman, S. A.

AU - Simms, K. M.

AU - Stone, E. C.

AU - Von Rosenvinge, T. T.

AU - Weidner, S. E.

AU - White, M. L.

N1 - Publisher Copyright: © Copyright owned by the author(s) under the terms of the Creative Commons Attribution-Non Commercial-No Derivatives 4.0 International License (CC BY-NC-ND 4.0).

PY - 2017

Y1 - 2017

N2 - NASA's Parker Solar Probe (PSP) spacecraft (formerly Solar Probe Plus) is scheduled for launch in July 2018 with a planned heliocentric orbit that will carry it on a series of close passes by the Sun with perihelion distances that eventually will get below 10 solar radii. Among other in-situ and imaging sensors, the PSP payload includes the two-instrument "Integrated Science Investigation of the Sun" suite, which will make coordinated measurements of energetic ions and electrons. The high-energy instrument (EPI-Hi), operating in the MeV energy range, consists of three detector-telescopes using silicon solid-state sensors for measuring composition, energy spectra, angular distributions, and time structure in solar energetic particle events. The expected performance of this instrument has been studied using accelerator calibrations, radioactive-source tests, and simulations. We present the EPI-Hi measurement capabilities drawing on these calibration data and simulation results for illustrations.

AB - NASA's Parker Solar Probe (PSP) spacecraft (formerly Solar Probe Plus) is scheduled for launch in July 2018 with a planned heliocentric orbit that will carry it on a series of close passes by the Sun with perihelion distances that eventually will get below 10 solar radii. Among other in-situ and imaging sensors, the PSP payload includes the two-instrument "Integrated Science Investigation of the Sun" suite, which will make coordinated measurements of energetic ions and electrons. The high-energy instrument (EPI-Hi), operating in the MeV energy range, consists of three detector-telescopes using silicon solid-state sensors for measuring composition, energy spectra, angular distributions, and time structure in solar energetic particle events. The expected performance of this instrument has been studied using accelerator calibrations, radioactive-source tests, and simulations. We present the EPI-Hi measurement capabilities drawing on these calibration data and simulation results for illustrations.

UR - https://www.scopus.com/pages/publications/85046057089

UR - https://www.scopus.com/pages/publications/85046057089#tab=citedBy

M3 - Conference article

AN - SCOPUS:85046057089

SN - 1824-8039

JO - Proceedings of Science

JF - Proceedings of Science

T2 - 35th International Cosmic Ray Conference, ICRC 2017

Y2 - 10 July 2017 through 20 July 2017

ER -

Capabilities and performance of the high-energy energetic-particles instrument for the parker solar probe mission

Abstract

All Science Journal Classification (ASJC) codes

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