API VERSION: 1.2 API SOURCE: NASA/JPL Horizons API ******************************************************************************* Revised: Apr 27, 2024 Wind Spacecraft / (Earth) -8 https://wind.nasa.gov/ https://hpde.io/SMWG/Observatory/Wind https://www.nasa.gov/feature/goddard/2019/25-years-of-science-in-the-solar-wind BACKGROUND: The primary science objectives of the Wind mission are: - Provide plasma, energetic particle, and magnetic field data for magnetospheric and ionospheric studies - Investigate plasma processes occurring in the near-Earth solar wind - Provide baseline, 1 AU, ecliptic plane observations for inner and outer heliospheric missions Wind is a spin-stabilized spacecraft launched on a Delta II 7925-10 rocket 1994-Nov-1 @ 09:31 UTC from pad 17B at Cape Canaveral, FL. The spacecraft has visited many regions of the near-Earth space environment. For the first nine months of operation, Wind was placed in a double-lunar swingby orbit near the ecliptic plane, with apogee from 80 to 250 Earth radii and perigee of between 5 and 10 Earth radii. In this orbit, lunar gravity assists were used to keep its apogee over the day hemisphere of the Earth, and magnetospheric observations were made through several orbit passages. Wind was then temporarily inserted into a small amplitude "halo" orbit, about the sunward Sun-Earth gravitational equilibrium point (SEMB-L1), varying from 235 to 265 Earth radii (Re). In 2001 and 2002, Wind had a distant prograde orbit that took it +/- 300 Re leading and lagging Earth. This orbit provided a wide baseline to study solar wind structures and correlations. In 2003 (Nov 2003 to Feb 2004), Wind reached the L2 Lagrange point 240 Re anti-sunward from Earth providing a 500 Re spatial separation from ACE solar wind observations along with measurements of the distant Earth magnetotail. In late June of 2004, Wind used its last lunar gravity assist to insert into a L1 Lissajous orbit to observe the unperturbed solar wind prior to it impacting the magnetosphere of Earth, providing an approx. one-hour warning of changes in the solar wind. On June 26, 2020, Wind completed the first halo orbit insertion maneuver. A second was completed on August 31, 2020, a third on November 9, 2020. The maneuvers were necessary to prevent Wind from entering the solar exclusion zone around the solar disk, where solar radio emissions can interfere with spacecraft communications. The halo orbit is an ellipse tilted with respect to the ecliptic plane, while Lissajous has an out-of-plane (z) component oscillation decoupled from in-plane components. Wind currently has enough fuel to continue its mission at L1 into the 2070s. SPACECRAFT PHYSICAL CHARACTERISTICS: Bus size : 2.4 x 1.8 m cylinder Power : 370 Watts (body mounted solar panels) Launch mass: 1250 kg Dry mass : 950 kg Extension : Long wire spin-plane antennas, inertial booms, and spin-plane appendages to support sensors. Experiment booms deployed along both Z axes. Spin rate : 20 rpm (~3 s period) w/axis < 1 degree from normal to ecliptic (spacecraft +Z spin axis aligned with south ecliptic pole) SCIENCE INSTRUMENTS 1. Magnetic Field Investigation (MFI) 2. Solar Wind Experiment (SWE) Faraday Cup - Ion Data Electron Data 3. 3D Plasma Analyzer 4. SMS Suprathermal Particle Data 5. EPACT High Energy Particle Data 6. WAVES Radio and Plasma Waves Data 7. KONUS and TGRS Data (gamma ray) SPACECRAFT TRAJECTORY: This trajectory is a concatenation of weekly predictions provided by GSFC. Based on tracking data up to 2024-Apr-22, prediction thereafter. Trajectory currently starts in 2019, but will eventually be extended to earlier dates. Trajectory name Start Stop ---------------------------- ----------- ----------- Wind_merged 2019-Oct-08 2024-Jul-16 *******************************************************************************