Astronomy:SWEAP

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Short description: Solar wind and plasma instrument on the Parker Solar Probe
Diagram of SWEAP, SPC subinstrument
Diagram of SWEAP, SPAN-A subinstrument
SPAN-B

SWEAP (Solar Wind Electrons Alphas and Protons) is an instrument on the unmanned space probe to the Sun, the Parker Solar Probe.[1] The spacecraft with SWEAP on board was launched by a Delta IV Heavy on 12 August 2018 from Cape Canaveral, Florida.[2] SWEAP includes two types of instruments, the Solar Probe Cup (SPC) and Solar Probe Analyzers (SPAN).[3] SWEAP has four sensors overall, and is designed to take measurements of the Solar wind including electrons and ions of hydrogen (protons) and helium (these are the main components of the Solar wind and coronal plasma).[4]

Design

SWEAP consists of the Solar Probe Cup (SPC), a faraday cup which faces the Sun and is designed to measure electrons and ions in the space environment near the Sun; the Solar Probe Analyzers (SPAN-A and SPAN-B);[5][6] and the SWEAP electronics module (SWEM).

The Solar Probe Cup is a Sun facing instrument directly exposed to the Sun, and had to be designed to handle the high temperature conditions at 9-10 Solar radii from the Sun, that are planned for the mission.[7] In operation it peeks out from the probes Sun shield, and is made entirely of refractory materials to endure these conditions. The hottest portion, the grid in front of the cup, can be heated to 3,000 °F (1,650 °C)[8] and is made of tungsten. The wiring connecting to the electronics is made of niobium with sapphire insulators.

SPAN-A and B are behind the heat shield, oriented forward ("ram side") and backward along the spacecraft's orbit, and take electron and ion measurements overs a wide field of view.[9] SPAN-A measure ions and electrons and SPAN-B measures electrons.[10]

Summary:[11]

  • Solar Probe Cup (SPC): Outside solar shield directly exposed to the Sun
  • Solar Probe Analyzers (SPAN)
    • SPAN-Ai: ion electrostatic analyzer (ESA) on the ram side
    • SPAN-Ae: electron electrostatic analyzer on the ram side
    • SPAN-B: electron electrostatic analyzer on the anti-ram side
  • SWEAP Electronics Module (SWEM)

Operations

By September 2018, SWEAP had been turned on and first light data was returned.[12]

Location

Ram-side view, SPAN-A marked

See also

References

  1. ↑ Kasper, Justin C.. "The SWEAP Investigation for Parker Solar Probe". https://www.cfa.harvard.edu/sweap/about_sweap.html. 
  2. ↑ Brown, Geoffrey; Brown, Dwayne; Fox, Karen (12 August 2018). "Parker Solar Probe Launches on Historic Journey to Touch the Sun". Johns Hopkins University Applied Physics Laboratory. http://parkersolarprobe.jhuapl.edu/News-Center/Show-Article.php?articleID=94. 
  3. ↑ Kasper, Justin C.. "The SWEAP Investigation for Parker Solar Probe". https://www.cfa.harvard.edu/sweap/about_sweap.html. 
  4. ↑ Kasper, Justin C.; Abiad, Robert; Austin, Gerry; Balat-Pichelin, Marianne; Bale, Stuart D.; Belcher, John W.; Berg, Peter; Bergner, Henry et al. (2015-10-29). "Solar Wind Electrons Alphas and Protons (SWEAP) Investigation: Design of the Solar Wind and Coronal Plasma Instrument Suite for Solar Probe Plus" (in en). Space Science Reviews 204 (1–4): 131–186. doi:10.1007/s11214-015-0206-3. ISSN 0038-6308. 
  5. ↑ Kasper, Justin C.. "The SWEAP Investigation for Parker Solar Probe". https://www.cfa.harvard.edu/sweap/about_sweap.html. 
  6. ↑ Kasper, Justin C.; Abiad, Robert; Austin, Gerry; Balat-Pichelin, Marianne; Bale, Stuart D.; Belcher, John W.; Berg, Peter; Bergner, Henry et al. (2015-10-29). "Solar Wind Electrons Alphas and Protons (SWEAP) Investigation: Design of the Solar Wind and Coronal Plasma Instrument Suite for Solar Probe Plus" (in en). Space Science Reviews 204 (1–4): 131–186. doi:10.1007/s11214-015-0206-3. ISSN 0038-6308. Bibcode: 2016SSRv..204..131K. 
  7. ↑ Kasper, Justin C.; Abiad, Robert; Austin, Gerry; Balat-Pichelin, Marianne; Bale, Stuart D.; Belcher, John W.; Berg, Peter; Bergner, Henry et al. (2016). "Solar Wind Electrons Alphas and Protons (SWEAP) Investigation: Design of the Solar Wind and Coronal Plasma Instrument Suite for Solar Probe Plus". Space Science Reviews 204 (1–4): 131–186. doi:10.1007/s11214-015-0206-3. Bibcode: 2016SSRv..204..131K. 
  8. ↑ Garner, Rob (2018-07-12). "Parker Solar Probe Instruments" (in en). NASA. https://www.nasa.gov/content/goddard/parker-solar-probe-instruments. 
  9. ↑ Garner, Rob (2018-07-12). "Parker Solar Probe Instruments" (in en). NASA. https://www.nasa.gov/content/goddard/parker-solar-probe-instruments. 
  10. ↑ Garner, Rob (2018-07-12). "Parker Solar Probe Instruments" (in en). NASA. https://www.nasa.gov/content/goddard/parker-solar-probe-instruments. 
  11. ↑ Kasper, Justin C.; Abiad, Robert; Austin, Gerry; Balat-Pichelin, Marianne; Bale, Stuart D.; Belcher, John W.; Berg, Peter; Bergner, Henry et al. (2015-10-29). "Solar Wind Electrons Alphas and Protons (SWEAP) Investigation: Design of the Solar Wind and Coronal Plasma Instrument Suite for Solar Probe Plus" (in en). Space Science Reviews 204 (1–4): 131–186. doi:10.1007/s11214-015-0206-3. ISSN 0038-6308. 
  12. ↑ "Illuminating First Light Data from Parker Solar Probe – Parker Solar Probe" (in en-US). 19 September 2018. https://blogs.nasa.gov/parkersolarprobe/2018/09/19/illuminating-first-light-data-from-parker-solar-probe/. 



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