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Global-scale Observations of the Limb and Disk

Global-scale Observations of the Limb and Disk (GOLD) is a heliophysics Mission of Opportunity (MOU) for NASA's Explorers program.[6] Led by Richard Eastes at the Laboratory for Atmospheric and Space Physics, which is located at the University of Colorado Boulder, GOLD's mission is to image the boundary between Earth and space in order to answer questions about the effects of solar and atmospheric variability of Earth's space weather.[7] GOLD was one of 11 proposals selected, of the 42 submitted, for further study in September 2011.[8] On 12 April 2013, NASA announced that GOLD, along with the Ionospheric Connection Explorer (ICON), had been selected for flight in 2017.[6] GOLD, along with its commercial host satellite SES-14, launched on 25 January 2018.[9]

Global-scale Observations of the Limb and Disk
SES-14 with GOLD (bottom left of satellite)
NamesGOLD
Mission typeObservation of Earth's thermosphere and ionosphere
OperatorLaboratory for Atmospheric and Space Physics
COSPAR ID2018-012B
SATCAT no.43175
Websitegold.cs.ucf.edu
Mission duration2 years (planned) [1]
Spacecraft properties
Spacecraft typeExplorer
ManufacturerLaboratory for Atmospheric and Space Physics
Launch mass36.8 kg (81 lb) [2]
Dimensions51 cm × 55 cm × 69 cm (20 in × 22 in × 27 in) [2]
Power72.4 watts [2]
Start of mission
Launch date25 January 2018, 22:20 UTC[3]
RocketAriane 5 ECA, VA241
Launch siteCentre Spatial Guyanais, Kourou, ELA-3
ContractorArianespace
Entered serviceOctober 2018
Orbital parameters
Reference systemGeocentric orbit (planned) [4]
RegimeGeostationary orbit
Main Imaging spectrograph
WavelengthsFar ultraviolet[5]
Transponders
Bandwidth6 Mbps [2]
 

Mission concept and history

GOLD is intended to perform a two-year mission imaging Earth's thermosphere and ionosphere from geostationary orbit. GOLD is a two-channel far-ultraviolet (FUV) imaging spectrograph built by the Laboratory for Atmospheric and Space Physics at the University of Colorado Boulder and flown as a hosted payload on the commercial communications satellite SES-14.[10] Additional organizations participating in the GOLD mission include the National Center for Atmospheric Research, Virginia Tech, the University of California, Berkeley, the University of Central Florida, Computational Physics Inc., the National Oceanic and Atmospheric Administration (NOAA), the U.S. Naval Research Laboratory (NRL), Boston University, and Clemson University.

In June 2017, SES announced the successful integration of GOLD with the SES-14 satellite under construction at Airbus Defence and Space in Toulouse, France.[11] GOLD was launched on 25 January 2018 at 22:20 UTC aboard Ariane 5 ECA VA241 from the Centre spatial Guyanais.[9]

Scientific objectives

The scientific objectives of the GOLD mission are to determine how geomagnetic storms alter the temperature and composition of Earth's atmosphere, to analyze the global-scale response of the thermosphere to solar extreme-ultraviolet variability, to investigate the significance of atmospheric waves and tides propagating from below the temperature structure of the thermosphere and to resolve how the structure of the equatorial ionosphere influences the formation and evolution of equatorial plasma density irregularities. The viewpoint provided by GOLD's geostationary orbit – from which the same hemisphere is always observable – is a new perspective on the Earth's upper atmosphere. This viewpoint allows local time, universal time and longitudinal variations of the thermosphere and ionosphere's response to the various forcing mechanisms to be uniquely determined.[7]

Results

Data from GOLD has been used to confirm that variation in the equatorial ionization anomaly at night and in the early morning is governed by atmospheric waves in the lower atmosphere. GOLD observations have also implicated gravity waves emanating from the lower atmosphere in the seeding of equatorial plasma bubbles, which degrade GPS performance.[12] GOLD daytime observations on thermosphere column density ratio of atomix oxygen and Nitregon bring a lot of new findings. First, GOLD observation shows that even weak, or minor geomagnetic activity (maximum Kp=1.7) can still generate significant disturbance in the thermosphere and ionosphere. This is crucial for the space weather forecast because the pre-quiet condition before the disturbed time determines the accuracy of forecast. Furthermore, the neutral tongue, which is an enhancement of O/N2 surrounded by depletion of O/N2, and had only been discovered in model simulations, is observed firstly by GOLD.This modify the classic theory of thermospheric composition disturbance during storm time. The theory only predict that the disturbance corotate from day to night, but did not mention what else occur to the depletion.

References

  1. ^ Mason, Tom (29 January 2018). "GOLD Powers on for the First Time". University of Central Florida. Retrieved 22 June 2019.
  2. ^ a b c d Eastes, Richard (24 March 2016). Global-scale Observations of the Limb and Disk (GOLD): Mission of Opportunity (PDF). Managing Partners and Resources, PI Team Masters Forum #6. NASA. Retrieved 5 December 2022.
  3. ^ Nowakowski, Tomasz (25 January 2018). "Ariane 5 rocket places 2 satellites into orbit despite telemetry anomaly". Spaceflight Insider. Retrieved 1 February 2018.
  4. ^ "Trajectory: Explorer-1 1958-001A". NASA. 14 May 2020. Retrieved 13 February 2021.   This article incorporates text from this source, which is in the public domain.
  5. ^ Russell, Kendall (25 May 2017). "NASA Integrates Ultraviolet Space Spectrograph with SES 14". Satellite Today. Retrieved 1 February 2018.
  6. ^ a b Brown, Dwayne (12 April 2013). "NASA Selects Explorer Projects to Probe Earth's Upper Atmosphere" (Press release). NASA. Retrieved 24 May 2013.   This article incorporates text from this source, which is in the public domain.
  7. ^ a b Eastes, Richard (May 2009). "NASA Mission to Explore Forcing of Earth's Space Environment". Eos. 90 (18): 155. Bibcode:2009EOSTr..90..155E. doi:10.1029/2009EO180002.
  8. ^ Brown, Dwayne (29 September 2011). "NASA Selects Science Investigations For Concept Studies" (Press release). NASA. Retrieved 24 May 2013.   This article incorporates text from this source, which is in the public domain.
  9. ^ a b Clark, Stephen (26 January 2018). "Ariane 5 deploys two telecom satellites in orbit despite telemetry loss". Spaceflight Now. Retrieved 26 January 2018.
  10. ^ Binette, Chad (15 April 2013). "$55 Million Grant Makes UCF, Florida History". University of Central Florida. Retrieved 24 May 2013.
  11. ^ Payer, Markus; Kossobokova, Natalia (23 May 2017). "SES-14 Integrates NASA Ultraviolet Space Spectrograph" (Press release). SES. Retrieved 7 June 2017.
  12. ^ Frazier, Sarah (14 January 2021). "Research Highlights from NASA's GOLD Mission". NASA. Retrieved 14 January 2021.   This article incorporates text from this source, which is in the public domain.

External links

global, scale, observations, limb, disk, gold, heliophysics, mission, opportunity, nasa, explorers, program, richard, eastes, laboratory, atmospheric, space, physics, which, located, university, colorado, boulder, gold, mission, image, boundary, between, earth. Global scale Observations of the Limb and Disk GOLD is a heliophysics Mission of Opportunity MOU for NASA s Explorers program 6 Led by Richard Eastes at the Laboratory for Atmospheric and Space Physics which is located at the University of Colorado Boulder GOLD s mission is to image the boundary between Earth and space in order to answer questions about the effects of solar and atmospheric variability of Earth s space weather 7 GOLD was one of 11 proposals selected of the 42 submitted for further study in September 2011 8 On 12 April 2013 NASA announced that GOLD along with the Ionospheric Connection Explorer ICON had been selected for flight in 2017 6 GOLD along with its commercial host satellite SES 14 launched on 25 January 2018 9 Global scale Observations of the Limb and DiskSES 14 with GOLD bottom left of satellite NamesGOLDMission typeObservation of Earth s thermosphere and ionosphereOperatorLaboratory for Atmospheric and Space PhysicsCOSPAR ID2018 012BSATCAT no 43175Websitegold wbr cs wbr ucf wbr eduMission duration2 years planned 1 Spacecraft propertiesSpacecraft typeExplorerManufacturerLaboratory for Atmospheric and Space PhysicsLaunch mass36 8 kg 81 lb 2 Dimensions51 cm 55 cm 69 cm 20 in 22 in 27 in 2 Power72 4 watts 2 Start of missionLaunch date25 January 2018 22 20 UTC 3 RocketAriane 5 ECA VA241Launch siteCentre Spatial Guyanais Kourou ELA 3ContractorArianespaceEntered serviceOctober 2018Orbital parametersReference systemGeocentric orbit planned 4 RegimeGeostationary orbitMain Imaging spectrographWavelengthsFar ultraviolet 5 TranspondersBandwidth6 Mbps 2 Explorers Program Contents 1 Mission concept and history 2 Scientific objectives 3 Results 4 References 5 External linksMission concept and history EditGOLD is intended to perform a two year mission imaging Earth s thermosphere and ionosphere from geostationary orbit GOLD is a two channel far ultraviolet FUV imaging spectrograph built by the Laboratory for Atmospheric and Space Physics at the University of Colorado Boulder and flown as a hosted payload on the commercial communications satellite SES 14 10 Additional organizations participating in the GOLD mission include the National Center for Atmospheric Research Virginia Tech the University of California Berkeley the University of Central Florida Computational Physics Inc the National Oceanic and Atmospheric Administration NOAA the U S Naval Research Laboratory NRL Boston University and Clemson University In June 2017 SES announced the successful integration of GOLD with the SES 14 satellite under construction at Airbus Defence and Space in Toulouse France 11 GOLD was launched on 25 January 2018 at 22 20 UTC aboard Ariane 5 ECA VA241 from the Centre spatial Guyanais 9 Scientific objectives EditThe scientific objectives of the GOLD mission are to determine how geomagnetic storms alter the temperature and composition of Earth s atmosphere to analyze the global scale response of the thermosphere to solar extreme ultraviolet variability to investigate the significance of atmospheric waves and tides propagating from below the temperature structure of the thermosphere and to resolve how the structure of the equatorial ionosphere influences the formation and evolution of equatorial plasma density irregularities The viewpoint provided by GOLD s geostationary orbit from which the same hemisphere is always observable is a new perspective on the Earth s upper atmosphere This viewpoint allows local time universal time and longitudinal variations of the thermosphere and ionosphere s response to the various forcing mechanisms to be uniquely determined 7 Results EditData from GOLD has been used to confirm that variation in the equatorial ionization anomaly at night and in the early morning is governed by atmospheric waves in the lower atmosphere GOLD observations have also implicated gravity waves emanating from the lower atmosphere in the seeding of equatorial plasma bubbles which degrade GPS performance 12 GOLD daytime observations on thermosphere column density ratio of atomix oxygen and Nitregon bring a lot of new findings First GOLD observation shows that even weak or minor geomagnetic activity maximum Kp 1 7 can still generate significant disturbance in the thermosphere and ionosphere This is crucial for the space weather forecast because the pre quiet condition before the disturbed time determines the accuracy of forecast Furthermore the neutral tongue which is an enhancement of O N2 surrounded by depletion of O N2 and had only been discovered in model simulations is observed firstly by GOLD This modify the classic theory of thermospheric composition disturbance during storm time The theory only predict that the disturbance corotate from day to night but did not mention what else occur to the depletion References Edit Mason Tom 29 January 2018 GOLD Powers on for the First Time University of Central Florida Retrieved 22 June 2019 a b c d Eastes Richard 24 March 2016 Global scale Observations of the Limb and Disk GOLD Mission of Opportunity PDF Managing Partners and Resources PI Team Masters Forum 6 NASA Retrieved 5 December 2022 Nowakowski Tomasz 25 January 2018 Ariane 5 rocket places 2 satellites into orbit despite telemetry anomaly Spaceflight Insider Retrieved 1 February 2018 Trajectory Explorer 1 1958 001A NASA 14 May 2020 Retrieved 13 February 2021 This article incorporates text from this source which is in the public domain Russell Kendall 25 May 2017 NASA Integrates Ultraviolet Space Spectrograph with SES 14 Satellite Today Retrieved 1 February 2018 a b Brown Dwayne 12 April 2013 NASA Selects Explorer Projects to Probe Earth s Upper Atmosphere Press release NASA Retrieved 24 May 2013 This article incorporates text from this source which is in the public domain a b Eastes Richard May 2009 NASA Mission to Explore Forcing of Earth s Space Environment Eos 90 18 155 Bibcode 2009EOSTr 90 155E doi 10 1029 2009EO180002 Brown Dwayne 29 September 2011 NASA Selects Science Investigations For Concept Studies Press release NASA Retrieved 24 May 2013 This article incorporates text from this source which is in the public domain a b Clark Stephen 26 January 2018 Ariane 5 deploys two telecom satellites in orbit despite telemetry loss Spaceflight Now Retrieved 26 January 2018 Binette Chad 15 April 2013 55 Million Grant Makes UCF Florida History University of Central Florida Retrieved 24 May 2013 Payer Markus Kossobokova Natalia 23 May 2017 SES 14 Integrates NASA Ultraviolet Space Spectrograph Press release SES Retrieved 7 June 2017 Frazier Sarah 14 January 2021 Research Highlights from NASA s GOLD Mission NASA Retrieved 14 January 2021 This article incorporates text from this source which is in the public domain External links EditGOLD website by the University of Central Florida GOLD website by NASA Retrieved from https en wikipedia org w index php title Global scale Observations of the Limb and Disk amp oldid 1125826110, wikipedia, wiki, book, books, library,

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