The 2012 Earth-Orbiting Heliophysics Fleet
- Visualizations by:
- Tom Bridgman
- View full credits
Revision (November 9, 2012): The RBSP mission has been renamed the Van Allen Probes. NASA Press Release.
The satellite orbits are color coded for their observing program:
Magenta: TIM (Thermosphere, Ionosphere, Mesosphere) observations Yellow: solar observations and imagery Cyan: Geospace and magnetosphere Violet: Heliospheric observations
Near-Earth Fleet:
- Hinode: Observes the Sun in multiple wavelengths up to x-rays. SVS page
- RHESSI : Observes the Sun in x-rays and gamma-rays. SVS page
- TIMED: Studies the upper layers (40-110 miles up) of the Earth's atmosphere.
- FAST: Measures particles and fields in regions where aurora form.
- CINDI: Measures interactions of neutral and charged particles in the ionosphere.
- SORCE: Monitors solar intensity across a broad range of the electromagnetic spectrum.
- AIM: Images and measures noctilucent clouds. SVS page
- RBSP: (Renamed the Van Allen Probes) Designed to study the impact of space weather on Earth's radiation belts. SVS page
Geosynchronous Fleet:
- SDO: Solar Dynamics Observatory keeps the Sun under continuous observation at 16 megapixel resolution.
- GOES: The newest GOES satellites include a solar X-ray imager operated by NOAA.
Geospace Fleet:
- Geotail: Conducts measurements of electrons and ions in the Earth's magnetotail.
- Cluster: This is a group of four satellites which fly in formation to measure how particles and fields in the magnetosphere vary in space and time. SVS page
- THEMIS: This is a fleet of three satellites to study how magnetospheric instabilities produce substorms. Two of the original five satellites were moved into lunar orbit to become ARTEMIS.SVS page
- IBEX: The Interstellar Boundary Explorer measures the flux of neutral atoms from the heliopause.
Lunar Orbiting Fleet
- ARTEMIS: Two of the THEMIS satellites were moved into lunar orbit to study the interaction of the Earth's magnetosphere with the Moon.
Note: A number of near-Earth missions had their orbits generated from Two-Line orbital elements valid in July 2012. Orbit perturbations since then may result in significant deviation from the actual satellite position for the time frame of this visualization.
Credits
Please give credit for this item to:
NASA/Goddard Space Flight Center Scientific Visualization Studio
Animator
- Tom Bridgman (GST) [Lead]
Producer
- Scott Wiessinger (KBRwyle)
Missions
This visualization is related to the following missions:Series
This visualization can be found in the following series:Datasets used in this visualization
DE421 (A.K.A. JPL DE421)
Planetary ephemerides
Dataset can be found at: http://ssd.jpl.nasa.gov/?ephemerides#planets
See more visualizations using this data setSTK Ephemeris (A.K.A. Satellite ToolKit Ephemeris)
Satellite ephemerides
See more visualizations using this data setSpace-Track TLE (A.K.A. Space-Track Two-Line Elements)
Satellite ephemerides
Dataset can be found at: http://Space-Track.org
See more visualizations using this data setSPICE Ephemerides (A.K.A. SPICE Ephemerides)
Satellite and planetary ephemerides
See more visualizations using this data setSSCweb ephemerides (A.K.A. SSCweb)
Satellite ephemerides
Dataset can be found at: http://sscweb.gsfc.nasa.gov
See more visualizations using this data setNote: While we identify the data sets used in these visualizations, we do not store any further details nor the data sets themselves on our site.