Heliophysics Sentinels 2022

This visualization presents orbits of the current heliophysics satellites covering the space near Earth, out to the orbit of the Moon. This visualization presents orbits of the current heliophysics satellites covering the space near Earth, out to the Moon and then to the Sun-Earth Lagrange point, L1. This visualization presents orbits of the current heliophysics satellites covering the space near Earth, out to the Sun-Earth Lagrange point, L1, and finally a view of the current missions operating in the inner solar system. This visualization presents orbits of the current heliophysics satellites covering the space near Earth, through the solar system, and concluding with a view of the Voyagers, just outside the heliopause. There have been few changes since the 2018 Heliophysics Fleet. Van Allen Probes and SORCE have been decommissioned, while Solar Orbiter, ICON and SET have been added. As of spring 2020, here's a tour of the NASA Heliophysics fleet from the near-Earth satellites out to the Voyagers beyond the heliopause.Excepting the Voyager missions, the satellite orbits are color coded for their observing program:Magenta: TIM (Thermosphere, Ionosphere, Mesosphere) observationsYellow: solar observations and imageryCyan: Geospace and magnetosphereViolet: Heliospheric observations Near-Earth Fleet:Hinode: Observes the Sun in multiple wavelengths up to x-rays. SVS pageTIMED: Studies the upper layers (40-110 miles up) of Earth's atmosphere. SVS pageICON: Works with GOLD on studies of the ionosphere.AIM: Images and measures noctilucent clouds. SVS pageIRIS: Interface Region Imaging Spectrograph is designed to take high-resolution spectra and images of the region between the solar photosphere and solar atmosphere. SVS pageSET: Space Environment Testbed exploring radiation-hardening technologiesGeosynchronous Fleet:SDO: Solar Dynamics Observatory keeps the Sun under continuous observation at 16 megapixel resolution. SVS pageGOLD: Global-scale Observations of the Limb and Disk is a spectroscopic imager for studying the ionosphere.Geospace Fleet:Geotail: Conducts measurements of electrons and ions in the Earth's magnetotail. SVS pageMagnetospheric Multi-scale (MMS): 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 pageTHEMIS: 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 THEMIS-ARTEMIS. SVS page IBEX: The Interstellar Boundary Explorer measures the flux of neutral atoms from the heliopause. SVS pageLunar Orbiting Fleet:THEMIS-ARTEMIS: Two of the THEMIS satellites were moved into lunar orbit to study the interaction of the Earth's magnetosphere with the Moon. SVS page Sun-Earth Lagrange Point One Fleet:The L1 point is a Lagrange Point between the Sun and the Earth. Spacecraft can orbit this location for continuous coverage of the Sun.SOHO: Studies the Sun with cameras and a multitude of other instruments. SVS pageACE: Measures the composition and characteristics of the solar wind. SVS pageWind: Measures particle flows and fields in the solar wind. SVS page Solar Orbiting Fleet:STEREO-A: The remaining STEREO spaceraft orbits the Sun in roughly the same orbit as Earth. SVS pageParker Solar Probe: On an orbit that takes it closer to the Sun than any other mission. SVS pageSolar Orbiter: On an orbit that takes it to high solar latitudes. SVS page Interstellar Fleet:Voyager 1 & Voyager 2: The two Voyager spaceraft orbit originally performed flybys of the outer planets of the solar system but continued to operate. They are now the most distant monitors of the plasma in the space between the stars. At the time of this visualization, Voyager 2 has just crossed the heliopause.SVS page For More InformationSee [NASA.gov](https://www.nasa.gov/mission_pages/sunearth/missions/index.html) Related pages