Earth  Sun  ID: 4589

Heliophysics Sentinels 2017

There have been few changes since the 2015 Earth-Orbiting Heliophysics Fleet. As of summer 2017, here's a tour of the NASA Heliophysics fleet from the near-Earth satellites out to the Voyagers beyond the heliopause.

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 Earth's atmosphere. SVS page
  • SORCE: Monitors solar intensity across a broad range of the electromagnetic spectrum.
  • AIM: Images and measures noctilucent clouds. SVS page
  • Van Allen Probes: Two probes moving along the same orbit designed to study the impact of space weather on Earth's radiation belts. SVS page
  • TWINS: Two Wide-Angle Imaging Neutral-Atom Spectrometers are two probes observing the Earth with neutral atom imagers.
  • IRIS: Interface Region Imaging Spectrograph is designed to take high-resolution spectra and images of the region between the solar photosphere and solar atmosphere. SVS page

Geosynchronous Fleet:

  • SDO: Solar Dynamics Observatory keeps the Sun under continuous observation at 16 megapixel resolution. SVS page

Geospace Fleet:

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. 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.

Solar Orbiting Fleet:

  • STEREO-A & STEREO-B: The two STEREO spaceraft orbit the Sun in roughly the same orbit as Earth. There have been some communications problems with STEREO-B since 2014. 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. SVS page
Major changes with earlier versions:
  • L1 fleet, STEREOs and Voyagers added
  • CINDI de-orbited and removed
  • Camera move extended to out beyond the heliopause
 

Older Version


Visualization Credits

Tom Bridgman (GST): Lead Visualizer
Laurence Schuler (ADNET Systems Inc.): Technical Support
Ian Jones (ADNET Systems Inc.): Technical Support
Please give credit for this item to:
NASA's Scientific Visualization Studio

Short URL to share this page:
http://svs.gsfc.nasa.gov/4589

Missions:
ACE
AIM
ARTEMIS
Geotail
Hinode (Solar-b)
IBEX
IRIS: Interface Region Imaging Spectrograph
Magnetospheric Multiscale (MMS)
RHESSI
SDO
SOHO
Solar Radiation and Climate Experiment (SORCE)
STEREO
THEMIS
TIMED
Van Allen Probes
Voyager
WIND

Data Used:
SSCweb
JPL/Horizon Orbital Ephemerides
Space-Track Two-Line Elements
DE 431
Note: 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.

Keywords:
SVS >> SOHO
SVS >> Hyperwall
SVS >> Solar Dynamics Observatory
SVS >> Spacecraft >> Voyager
SVS >> Satellite Orbit
NASA Science >> Earth
NASA Science >> Sun