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Traceable Radiometry Underpinning Terrestrial and Helio Studies

From Wikipedia, the free encyclopedia
Planned Earth observation satellite
This article is about a satellite mission. For other uses, seeTruth (disambiguation).
TRUTHS
TRUTHS mission patch
NamesTraceable Radiometry Underpinning Terrestrial- and Helio-Studies
Mission typeSolar radiation measurement,traceability
Mission duration5-8+ years (planned)
Start of mission
Launch date~2030
RocketVega-C (planned)
Launch siteCentre Spatial Guyanais
Orbital parameters
Reference systemGeocentric
RegimePolar
Altitude610 km
Inclination90°
Period96.9 minutes[1]
Repeat interval61 days
Instruments
CSAR - cryogenic solar absolute radiometer
HIS - hyperspectral imaging spectrometer

TRUTHS(TraceableRadiometryUnderpinningTerrestrial- andHelio-Studies) is a plannedEuropean Space Agency (ESA)satellite. It is meant to improve the accuracy, reliability, and integrity ofEarth observation data,[2] and to be the first of a new class of "SI-traceable satellites" (SITSats) that will enable other Earth observation missions to calibrate measurements with reference to them.[3] The mission is led by the UKNational Physical Laboratory (NPL) and its lead scientist for Earth observation, Nigel Fox.[4]

Science goals

[edit]

It has two primary objectives:[5]

  • "To establish agold-standardreference dataset against which to cross-calibrate other sensors, facilitating an upgrade to the performance of the global Earth observing system to ensure interoperability and robust anchoring to an SI reference in space."

A secondary objective of the mission is the use the global hyperspectral data to "constrain and improve retrieval algorithms".[6]

Science instruments

[edit]

Alongside communications and navigation equipment, the scientific payload of the satellite would include three instruments: the cryogenic solar absolute radiometer (CSAR), the onboard calibration system (OBCS), and the hyperspectral imaging spectrometer (HIS).

The instruments would produce global hyperspectral (320 nm to 2400 nm) measurements of "top-of-atmosphere earthspectral radiance (0.3% k=2);solar irradiance (both total and spectrally resolved, 0.02% and 0.3% respectively); and lunar spectral irradiance (0.3%)".[3]

The cryogenic radiometer is the primary standard used by nationalmetrology institutes for radiometric measurements and "recommended as the means to achieve SI traceability".[6] The CSAR, which would be cooled to < 60 K, is therefore considered "the heart of the calibration system".[6]

The mission would be the first to host aprimary standard cryogenicradiometer aboard a satellite.[3] The OBCS would "...transfer calibration traceability from the SI defining power measurement... to a full spectrally resolved radiance calibration of an instrument" – in the case of TRUTHS from the CSAR to the HIS – in a simplified manner to the steps used by terrestrialmetrology institutes.[6] The HIS can then be used to image the Earth, the Moon, and also to "measure incident solar spectral irradiance."[6]

Timeline

[edit]
  • In order to obtain both scientific and financial support for the mission, many reports and academic publications were produced by Fox and collaborators over several decades.[7][8][9][10][11][12]
  • Early 2000s – Mission proposed by the UKNational Physical Laboratory (NPL)[13]
  • 2019 – Adopted at the ESA ministerial conference, with 85% funding from the UK. The remainder from Switzerland, Greece, Czechia, and Romania.[14][15]
  • 2020 –Airbus UK selected as lead contractor,[16]Teledyne e2v selected to provide the infrared detectors.[17]
  • 2021 – AtCOP26: Began early design phase.[18]
  • 2022 – Passed preliminary design, technical, and scientific reviews.[19] Received further funding at the ESA ministerial conference.[20]
  • 2023 – Further funding awarded duringCOP28, toAirbus UK for design and development; and toTeledyne e2v to construct the hyperspectral imaging spectrometer detection system.[21]
  • ~ 2030 – Estimated launch, aboard aVega-C from theGuiana Space Centre.[13]
  • The mission would have a targeted duration of eight or more years, and a minimum duration of five.[6]

See also

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References

[edit]
  1. ^"THE CEOS DATABASE : MISSION, INSTRUMENTS AND MEASUREMENTS - TRUTHS".database.eohandbook.com. Retrieved2023-12-05.
  2. ^"Mission objectives".NPLWebsite. Retrieved2023-12-05.
  3. ^abc"Learn more about TRUTHS".NPLWebsite. Retrieved2023-12-05.
  4. ^"Nigel Fox".NPLWebsite. Retrieved2024-01-12.
  5. ^"Mission objectives".National Physical Laboratory. Retrieved2023-12-03.
  6. ^abcdef"TRUTHS (Traceable Radiometry Underpinning Terrestrial-and Helio-Studies) - eoPortal".www.eoportal.org. Retrieved2023-12-05.
  7. ^Fox, Nigel P.; Aiken, James; et al. (2003-04-08). Fujisada, Hiroyuki; Lurie, Joan B.; Aten, Michelle L.; Weber, Konradin (eds.)."Traceable radiometry underpinning terrestrial- and helio-studies (TRUTHS)".Sensors, Systems, and Next-Generation Satellites VI.4881. SPIE:395–406.Bibcode:2003SPIE.4881..395F.doi:10.1117/12.462438.
  8. ^Fox, Nigel; Green, Paul; et al. (2016). "Traceable Radiometery Underpinning Terrestrial- and Helio- Studies (TRUTHS): Establishing a climate and calibration observatory in space".2016 IEEE International Geoscience and Remote Sensing Symposium (IGARSS). pp. 1939–1942.doi:10.1109/igarss.2016.7729499.ISBN 978-1-5090-3332-4.
  9. ^Boesch, H; Brindley, H; et al. (2022-01-25).SI-traceable space-based climate observation system: a CEOS and GSICS Workshop. National Physical Laboratory, UK, 9-11 Sept 2019 (Report). National Physical Laboratory.doi:10.47120/npl.9319.
  10. ^Fox, Nigel; Green, Paul (2020-07-27)."Traceable Radiometry Underpinning Terrestrial- and Helio-Studies (TRUTHS): An Element of a Space-Based Climate and Calibration Observatory".Remote Sensing.12 (15): 2400.Bibcode:2020RemS...12.2400F.doi:10.3390/rs12152400.ISSN 2072-4292.
  11. ^Fox, Nigel; Kaiser-Weiss, Andrea; et al. (2011-10-28)."Accurate radiometry from space: an essential tool for climate studies".Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences.369 (1953):4028–4063.Bibcode:2011RSPTA.369.4028F.doi:10.1098/rsta.2011.0246.ISSN 1364-503X.PMID 21930564.
  12. ^Fehr, Thorsten; Fox, Nigel; et al. (2023-02-22).Traceable Radiometry Underpinning Terrestrial- and Helio- Studies (TRUTHS) – A 'gold standard' imaging spectrometer in space to support climate emergency reseaerch (Report). Copernicus Meetings.doi:10.5194/egusphere-egu23-12399.
  13. ^ab"TRUTHS Mission Explainer"(PDF).space4climate.com. Space4Climate. July 2023.
  14. ^"Space mission to reveal 'Truths' about climate change".BBC News. 2020-01-22. Retrieved2023-12-03.
  15. ^Norman, Helen (2020-02-03)."Europeans discuss TRUTHS climate change mission".Meteorological Technology International. Retrieved2023-12-03.
  16. ^"Airbus wins European Space Agency TRUTHS mission study for metrological traceability of Earth observation data".www.airbus.com. 28 October 2021. Retrieved2023-12-03.
  17. ^"Teledyne e2v to supply Infrared detector for TRUTHS Climate Change Satellite".UKspace. 2020-12-02. Retrieved2023-12-03.
  18. ^Jewett, Rachel (2021-11-05)."UK-Led TRUTH Mission to Fight Climate Change Moves to Early Design Phase".Via Satellite. Retrieved2023-12-03.
  19. ^"The TRUTHS climate satellite mission passes key test - Space4Climate". 2022-10-12. Retrieved2023-12-03.
  20. ^"NPL TRUTHS mission receives funding".NPLWebsite. Retrieved2023-12-03.
  21. ^"COP28: UK climate satellite contracts".GOV.UK. Retrieved2023-12-05.

External links

[edit]
External videos
video iconTRUTHS mission explanation -Space4Climate (2021)[1]
video iconOnboard Calibration System (OBCS) animation -National Physical Laboratory (2019)[2]
  1. ^"TRUTHS". Space4Climate. 2020-02-26. Retrieved2023-12-02.
  2. ^"SI traceability in-flight".National Physical Laboratory. Retrieved2023-12-02.
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