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  2. File:Parker Solar Probe 3D model.stl - Wikipedia

    en.wikipedia.org/wiki/File:Parker_Solar_Probe_3D...

    The SOHO (ESA & NASA) joint project implies that all materials created by its probe are copyrighted and require permission for commercial non-educational use. Images featured on the Astronomy Picture of the Day (APOD) web site may be copyrighted. The National Space Science Data Center (NSSDC) site has been known to host copyrighted content.

  3. Parker Solar Probe - Wikipedia

    en.wikipedia.org/wiki/Parker_Solar_Probe

    [1] [37]: 31 The solar shield is hexagonal, mounted on the Sun-facing side of the spacecraft, 2.3 m (7 ft 7 in) in diameter, [38] 11.4 cm (4.5 in) thick, and is made of two panels of reinforced carbon–carbon composite with a lightweight 11-centimeter-thick (4.5 in) carbon foam core, [39] which is designed to withstand temperatures outside the ...

  4. Solar and Heliospheric Observatory - Wikipedia

    en.wikipedia.org/wiki/Solar_and_Heliospheric...

    The Solar and Heliospheric Observatory (SOHO) is a European Space Agency (ESA) spacecraft built by a European industrial consortium led by Matra Marconi Space (now Airbus Defence and Space) that was launched on a Lockheed Martin Atlas IIAS launch vehicle on 2 December 1995, to study the Sun. It has also discovered more than 5,000 comets. [2]

  5. Cluster II (spacecraft) - Wikipedia

    en.wikipedia.org/wiki/Cluster_II_(spacecraft)

    For the first time in space history, this mission was able to collect three-dimensional information on how the solar wind interacts with the magnetosphere and affects near-Earth space and its atmosphere, including aurorae. The spacecraft were cylindrical (2.9 x 1.3 m, see online 3D model) and were spinning at 15 rotations per minute.

  6. Extreme ultraviolet Imaging Telescope - Wikipedia

    en.wikipedia.org/wiki/Extreme_ultraviolet...

    The Extreme ultraviolet Imaging Telescope (EIT) is an instrument on the SOHO spacecraft used to obtain high-resolution images of the solar corona in the ultraviolet range. The EIT instrument is sensitive to light of four different wavelengths: 17.1, 19.5, 28.4, and 30.4 nm, corresponding to light produced by highly ionized iron (XI)/(X), (XII), (XV), and helium (II), respectively.

  7. Large Angle and Spectrometric Coronagraph - Wikipedia

    en.wikipedia.org/wiki/Large_Angle_and...

    The Large Angle and Spectrometric Coronagraph (LASCO) on board the Solar and Heliospheric Observatory satellite (SOHO) consists of three solar coronagraphs with nested fields of view: [1] C1 - a Fabry–Pérot interferometer coronagraph imaging from 1.1 to 3 solar radii, non-functional since the 24 June 1998 SOHO Mission Interruption [2]

  8. FreeFlyer - Wikipedia

    en.wikipedia.org/wiki/FreeFlyer

    FreeFlyer has been used to support many spacecraft missions, for mission planning analysis, operational analysis, or both. Specific mission examples include the International Space Station (ISS), [7] the JSpOC Mission System, [8] the Earth Observing System, [9] [10] Solar Dynamics Observatory (SDO), [11] and Magnetospheric Multiscale Mission (MMS).

  9. Halo orbit - Wikipedia

    en.wikipedia.org/wiki/Halo_orbit

    The first mission to use a halo orbit was ISEE-3, a joint ESA and NASA spacecraft launched in 1978. It traveled to the Sun–Earth L 1 point and remained there for several years. The next mission to use a halo orbit was Solar and Heliospheric Observatory (SOHO), also a joint ESA/NASA mission to study the Sun, which arrived at Sun–Earth L 1 in ...