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The Wide-Field Imager for Solar Probe (WISPR) is an imaging instrument of the '' Parker Solar Probe'' mission to the Sun, launched in August 2018. Imaging targets include visible light images of the corona, solar wind, shocks, solar ejecta, etc. Development of WISPR was led by the
U.S. Naval Research Laboratory The United States Naval Research Laboratory (NRL) is the corporate research laboratory for the United States Navy and the United States Marine Corps. It was founded in 1923 and conducts basic scientific research, applied research, technological ...
. The ''Parker Solar Probe'' with WISPR on board was launched by a Delta IV Heavy on 12 August 2018 from
Cape Canaveral , image = cape canaveral.jpg , image_size = 300 , caption = View of Cape Canaveral from space in 1991 , map = Florida#USA , map_width = 300 , type =Cape , map_caption = Location in Florida , location ...
, Florida. WISPR is intended take advantage of the spacecraft's proximity to the Sun by taking coronagraph-style images of the solar corona and features like coronal streamers, plumes, and
mass ejections Mass is an intrinsic property of a body. It was traditionally believed to be related to the quantity of matter in a physical body, until the discovery of the atom and particle physics. It was found that different atoms and different element ...
. One of the goals is to better understand the structure of the solar corona near the Sun. WISPR is designed to study the electron density and velocity structure of the corona. The instrument field of view is planned to extend from 13 to 108 degrees away from the Sun, and does not directly image the Sun; the area of interest is a very wide field extending away from the Sun. WISPR includes two separate telescopes, each with a radiation-hardened
CMOS Complementary metal–oxide–semiconductor (CMOS, pronounced "sea-moss", ) is a type of metal–oxide–semiconductor field-effect transistor (MOSFET) fabrication process that uses complementary and symmetrical pairs of p-type and n-type MOSFE ...
imager with resolution of 2,048×1,920 pixels. The CMOS sensors are an
active pixel sensor An active-pixel sensor (APS) is an image sensor where each pixel sensor unit cell has a photodetector (typically a pinned photodiode) and one or more active transistors. In a metal–oxide–semiconductor (MOS) active-pixel sensor, MOS field-effec ...
type of detector. The WISPR first light image was published in September 2018. In December, a view of the corona including a coronal streamer was released. In November 2018, a video of WIPSR recording solar wind during the spacecraft's first close pass to the Sun was released. One project scientist noted, "The data we’re seeing from Parker Solar Probe’s instruments is showing us details about solar structures and processes that we have never seen before,"


Development

The
stray light Stray light is light in an optical system, which was not intended in the design. The light may be from the intended source, but follow paths other than intended, or it may be from a source other than the intended source. This light will often set a ...
and baffle for WISPR was modeled during development of the instrument. Two noted cases where stray material caused issue with space imaging includes the Infrared Telescope (IRT) flown on the Space Shuttle Spacelab-2 mission, in which a piece of mylar insulation broke loose and floated into the line-of-sight of the telescope corrupting data. This was on the STS-51-F in the year 1985. Another case was in the 2010s on the Gaia spacecraft for which some stray light was identified coming from fibers of the sunshield, protruding beyond the edges of the shield.


Gallery

File:WISPR first light image.png, WISPR first light image. The right portion of the image is from WISPR's inner telescope, which is a 40-degree field of view and begins 58.5 degrees from the Sun's center. The left portion is from the outer telescope, which is a 58-degree field of view and ends about 160 degrees from the Sun. File:Parker-view-of-earth.jpg, The view from the probe's WISPR instrument on Sept. 25, 2018, shows Earth, the bright sphere near the middle of the right-hand panel. The elongated mark toward the bottom of the panel is a lens reflection from the WISPR instrument File:Parker Solar Probe coronal stream wispr-big 1-st flyby.jpg, Photo from the WISPR shows a coronal streamer, seen over the east limb of the Sun on Nov. 8, 2018, at 1:12 a.m. EST. The fine structure of the streamer is very clear, with at least two rays visible. Parker Solar Probe was about 16.9 million miles from the Sun's surface when this image was taken. The bright object near the center of the image is Mercury, and the dark spots are a result of background correction. File:Wispr merged six planets.jpg, When Parker Solar Probe was making its closest approach to the Sun on June 7, 2020, WISPR captured the planets Mercury, Venus, Earth, Mars, Jupiter and Saturn in its field of view File:Venus-ParkerSolarProbe-July2020.jpg, Photo taken by the probe during its second Venus flyby, July 2020 File:Parker Solar Probe flew by Venus on its fourth flyby.gif, As Parker Solar Probe flew by Venus on its fourth flyby, its WISPR instrument captured these images, showing the nightside surface of the planet File:Parker Solar Probe Encounters Streamers on the Way to the Sun.webm, As the probe passed through the Sun's corona in early 2021, it flew by structures called coronal streamers


See also

* FIELDS *
IS☉IS Integrated Science Investigation of the Sun or IS☉IS, is an instrument aboard the '' Parker Solar Probe'', a space probe designed to study the Sun. IS☉IS is focused on measuring energetic particles from the Sun, including electrons, protons, a ...
* SWEAP


References


External links


Looking at the Corona with WISPR on Parker Solar Probe
(April 16, 2018) {{Psp Parker Solar Probe Space imagers Solar telescopes