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Van Allen Probes

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Van Allen Probes
Artist's impression of the Van Allen Probes in orbit
NamesRadiation Belt Storm Probes (RBSP)
Mission typeAstrophysics
OperatorNASA
COSPAR ID2012-046A
2012-046B
SATCATno.38752
38753
Websitevanallenprobes.jhuapl.edu
Mission durationPlanned: 2 years
Final: 7 years, 1 month, 17 days
Spacecraft properties
ManufacturerApplied Physics Laboratory
Launch mass~1500 kg for both
Start of mission
Launch date30 August 2012, 08:05(2012-08-30UTC08:05)UTC
RocketAtlas V401
AV-032
Launch siteCape CanaveralSLC-41
ContractorUnited Launch Alliance
End of mission
DisposalDecommissioned
DeactivatedVan Allen Probe A: 18 October 2019(2019-10-19)
Van Allen Probe B: 19 July 2019
Orbital parameters
Reference systemGeocentric
RegimeHighly elliptical
Semi-major axis21,887 km (13,600 mi)
Perigee altitude618 km (384 mi)
Apogee altitude30,414 km (18,898 mi)
Inclination10.2°
Period537.1 minutes
←SDO
MMS→
←SDO
Parker→

TheVan Allen Probes,formerly known as theRadiation Belt Storm Probes(RBSP),[1]were tworobotic spacecraftthat were used to study theVan Allen radiation beltsthat surround Earth.NASAconducted the Van Allen Probes mission as part of theLiving With a Starprogram.[2]Understanding the radiation belt environment and its variability has practical applications in the areas of spacecraft operations, spacecraft system design, mission planning and astronaut safety.[3]The probes were launched on 30 August 2012 and operated for seven years. Both spacecraft were deactivated in 2019 when they ran out of fuel. They are expected todeorbitduring the 2030s.

Overview

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NASA'sGoddard Space Flight Centermanages the overallLiving With a Starprogram of which RBSP is a project, along withSolar Dynamics Observatory(SDO). The Johns Hopkins UniversityApplied Physics Laboratory(APL) was responsible for the overall implementation and instrument management for RBSP. The primary mission was scheduled to last 2 years, with expendables expected to last for 4 years. The primary mission was planned to last only 2 years because there was great concern as to whether the satellite's electronics would survive the hostile radiation environment in the radiation belts for a long period of time. When after 7 years the mission ended, it was not because of electronics failure but because of running out of fuel. This proved the resiliency of the spacecraft's electronics. The spacecraft's longevity in the radiation belts was considered a record-breaking performance for satellites in terms of radiation resiliency.[4]

The spacecraft worked in close collaboration with theBalloon Array for RBSP Relativistic Electron Losses(BARREL), which can measure particles that break out of the belts and make it all the way to Earth's atmosphere.[5][6]

The Applied Physics Laboratory managed, built, and operated the Van Allen Probes for NASA.

The probes are named afterJames Van Allen,the discoverer of the radiation belts they studied.[4]

Milestones

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Launch vehicle

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Probes in front of the first half of the payload fairing

On 16 March 2009 United Launch Alliance (ULA) announced that NASA had awarded ULA a contract to launch RSBP using anAtlas V401 rocket.[9]NASA delayed the launch as it counted down to the four-minute mark early morning on 23 August. After bad weather prevented a launch on 24 August, and a further precautionary delay to protect the rocket and satellites fromHurricane Isaac,liftoff occurred on 30 August 2012 at 4:05 AM EDT.[10]

End of mission

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On 12 February 2019, mission controllers began the process of ending the Van Allen Probes mission by lowering the spacecraft's perigees, which increases their atmospheric drag and results in their eventualdestructive reentryinto the atmosphere. This ensures that the probes reenter in a reasonable timespan, in order to pose little threat with regards to the problem oforbital debris.The probes were projected to cease operations by early 2020, or whenever they ran out of the necessary propellant to keep their solar panels pointed at the Sun. Reentry into the atmosphere is predicted to occur in 2034.[11]

Van Allen Probe B was shut down on 19 July 2019, after mission operators confirmed that it was out of propellant.[12]Van Allen Probe A, also running low on propellant, was deactivated on 18 October 2019, putting an end to the Van Allen Probes mission after seven years in operation.[13]

Science

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RBSP science overview.

TheVan Allen radiation beltsswell and shrink over time as part of a much largerspace weathersystem driven by energy and material that erupt off the Sun's surface and fill the entireSolar System.Space weather is the source ofaurorathat shimmer in the night sky, but it also can disrupt satellites, cause power grid failures and disruptGPScommunications. The Van Allen Probes were built to help scientists understand this region and to better designspacecraftthat can survive the rigors ofouter space.[2]The mission aimed to further scientific understanding of how populations of relativistic electrons and ions in space form or change in response to changes insolar activityand thesolar wind.[2]

The mission's general scientific objectives were to:[2]

  • Discover which processes - singly or in combination - accelerate and transport the particles in the radiation belt, and under what conditions.
  • Understand and quantify the loss of electrons from the radiation belts.
  • Determine the balance between the processes that cause electron acceleration and those that cause losses.
  • Understand how the radiation belts change in the context ofgeomagnetic storms.

In May 2016, the research team published their initial findings, stating that thering currentthat encircles Earth behaves in a much different way than previously understood.[14]The ring current lies at approximately 10,000 to 60,000 kilometres (6,200 to 37,000 mi) from Earth. Electric current variations represent the dynamics of only the low-energy protons. The data indicates that there is a substantial, persistent ring current around the Earth even during non-storm times, which is carried by high-energy protons. During geomagnetic storms, the enhancement of the ring current is due to new, low-energy protons entering the near-Earth region.[14][15]

Scientific results

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March 2015 geomagnetic storm.
This visualization opens with a full view of the radiation belt of trapped electrons circling Earth. We open a slice of the belts, to display a cross-section for clarity and move the camera to a more equatorial view. Earth rotation and solar motion have been turned off for this visualization to reduce distracting additional motions.

In February 2013, a third, temporary radiation belt was discovered using data gathered by the Van Allen Probes. After a few weeks, the third belt was destroyed by a burst of solar wind.[16]

Spacecraft

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Test deployment of RBSP A solar panels and magnetometer

The Van Allen Probes consisted of two spin-stabilized spacecraft that were launched with a single Atlas V rocket. The two probes had to operate in the harsh conditions they were studying; while other satellites have the luxury of turning off or protecting themselves in the middle of intense space weather, the Van Allen Probes had to continue to collect data. The probes were, therefore, built to withstand the constant bombardment of particles and radiation they would experience in this intense area of space.[2]

Instruments

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Schematic view of the probe

Because it was vital that the two craft make identical measurements to observe changes in the radiation belts through both space and time, each probe carried the following instruments:

  1. Energetic Particle, Composition, and Thermal Plasma (ECT) Instrument Suite;[17]The Principal Investigator is Harlan Spence fromUniversity of New Hampshire.[18]Key partners in this investigation areLANL,Southwest Research Institute,Aerospace CorporationandLASP
  2. Electric and Magnetic Field Instrument Suite and Integrated Science (EMFISIS);[19]The Principal Investigator isCraig Kletzingfrom theUniversity of Iowa.
  3. Electric Field and Waves Instrument (EFW); The Principal Investigator is John Wygant from theUniversity of Minnesota.Key partners in this investigation include the University of California at Berkeley and the University of Colorado at Boulder.
  4. Radiation Belt Storm Probes Ion Composition Experiment (RBSPICE); The Principal Investigator isLouis J. Lanzerottifrom theNew Jersey Institute of Technology.Key partners include theApplied Physics Laboratoryand Fundamental Technologies, LLC.
  5. Relativistic Proton Spectrometer (RPS) from theNational Reconnaissance Office

See also

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References

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  1. ^"Van Allen Probes: NASA Renames Radiation Belt Mission to Honor Pioneering Scientist".Science Daily. Reuters. 11 November 2012.Retrieved12 November2012.
  2. ^abcde"RBSP - Mission Overview".NASA.28 March 2012.Retrieved8 July2012.
  3. ^Radiation Belt Storm Probes (RBSP)Archived2 May 2012 at theWayback Machine
  4. ^ab"NASA's resilient van Allen Probes shut down – Spaceflight Now".
  5. ^Karen C. Fox (22 February 2011)."Launching Balloons in Antarctica".NASA.Retrieved13 July2012.
  6. ^Balloon Array for RBSP Relativistic Electron Losses
  7. ^"Construction Begins!".The Johns Hopkins University Applied Physics Laboratory. January 2010. Archived fromthe originalon 24 July 2012.
  8. ^"Probes launched".Space.com.30 August 2012.
  9. ^"United Launch Alliance Atlas V Awarded Four NASA Rocket Launch Missions".ULA. 16 March 2009. Archived fromthe originalon 1 August 2009.
  10. ^"Tropical Storm Isaac Delays NASA Launch".The Brevard Times. Archived fromthe originalon 12 November 2020.Retrieved26 August2012.
  11. ^Gebhardt, Chris (14 February 2019)."Beginning of the end: NASA's Van Allen probes prepare for mission's end".NASASpaceFlight.com.Retrieved17 February2019.
  12. ^"Van Allen Probes Spacecraft B Completes Mission Operations".Applied Physics Laboratory.23 July 2019.Retrieved10 October2019.
  13. ^"Ten Highlights From NASA's Van Allen Probes Mission".NASA.17 October 2019.Retrieved21 October2019.
  14. ^abCowing, Keith (19 May 2016)."Van Allen Probes Reveal Long-term Behavior of Earth's Ring Current".Space Ref.Retrieved20 May2016.[dead link]
  15. ^Gkioulidou, Matina; et al. (19 May 2016)."Storm time dynamics of ring current protons: Implications for the long-term energy budget in the inner magnetosphere".Geophysical Research Letters.43(10): 4736–4744.Bibcode:2016GeoRL..43.4736G.doi:10.1002/2016GL068013.
  16. ^Cowen, Ron (28 February 2013)."Ephemeral third ring of radiation makes appearance around Earth".Nature.doi:10.1038/nature.2013.12529.Retrieved26 March2024.
  17. ^"RBSP-ETC // About".Archived fromthe originalon 10 June 2008.
  18. ^UNH, Kristi Donahue."RBSP ECT team".rbsp-ect.sr.unh.edu.Retrieved24 April2017.
  19. ^Kletzing, C. A.; Kurth, W. S.; Acuna, M.; MacDowall, R. J.; Torbert, R. B.; Averkamp, T.; Bodet, D.; Bounds, S. R.; Chutter, M.; Connerney, J.; Crawford, D.; Dolan, J. S.; Dvorsky, R.; Hospodarsky, G. B.; Howard, J. (1 November 2013)."The Electric and Magnetic Field Instrument Suite and Integrated Science (EMFISIS) on RBSP".Space Science Reviews.179(1): 127–181.doi:10.1007/s11214-013-9993-6.ISSN1572-9672.
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