{ "id": 12927, "url": "https://svs.gsfc.nasa.gov/12927/", "page_type": "Produced Video", "title": "Looking at the Corona with WISPR on Parker Solar Probe", "description": "The Wide-Field Imager for Solar Probe, or WISPR, is aboard NASA’s Parker Solar Probe to take images of the solar corona (the Sun’s atmosphere) and inner heliosphere. WISPR’s telescopes will provide white-light images of the solar wind, shocks, solar ejecta and other structures as they approach and pass the spacecraft. Parker Solar Probe is scheduled for launch in July 2018. It will be the first spacecraft ever to fly through the solar corona to investigate the evolution of the solar wind and heating of the solar corona. WISPR does not look directly at the Sun. Its very wide field-of-view extends from 13° away from the center of the Sun to 108° from the Sun. || ", "release_date": "2018-04-16T12:00:00-04:00", "update_date": "2023-05-03T13:46:53.455695-04:00", "main_image": { "id": 404946, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012900/a012927/12927_streamerinner02_CaseA_Liewer.00100_print.jpg", "filename": "12927_streamerinner02_CaseA_Liewer.00100_print.jpg", "media_type": "Image", "alt_text": "This video shows six days of simulated observations from WISPR on its second orbit as the spacecraft approaches and flies through a highly structured coronal streamer emanating from the Sun. The video starts as the spacecrafts is about 50 solar radii from the Sun; at the end, the spacecraft is about 35 solar radii from the Sun flying through the streamer. Density streamers form at the top of large magnetic structure in the corona that often overlie sunspots and active regions. They are the corona rays that become visible during total solar eclipses.Credit: NASA/JPL/WISPR Team", "width": 1024, "height": 1024, "pixels": 1048576 }, "main_video": { "id": 404896, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012900/a012927/LARGE_MP4_12927_PSPCMEFOV2018V091080p_large.webm", "filename": "LARGE_MP4_12927_PSPCMEFOV2018V091080p_large.webm", "media_type": "Movie", "alt_text": "This animation shows Parker Solar Probe flying through the solar corona and coronal mass ejections. The fields-of-view of the WISPR telescopes can be seen as the transparent pyramids pointing out the side of the spacecraft.Credit: NASA/JPL/WISPR Team", "width": 1920, "height": 1080, "pixels": 2073600 }, "progress": "Complete", "media_groups": [ { "id": 327161, "url": "https://svs.gsfc.nasa.gov/12927/#media_group_327161", "widget": "Basic text with HTML", "title": "", "caption": "", "description": "The Wide-Field Imager for Solar Probe, or WISPR, is aboard NASA’s Parker Solar Probe to take images of the solar corona (the Sun’s atmosphere) and inner heliosphere. WISPR’s telescopes will provide white-light images of the solar wind, shocks, solar ejecta and other structures as they approach and pass the spacecraft. Parker Solar Probe is scheduled for launch in July 2018. It will be the first spacecraft ever to fly through the solar corona to investigate the evolution of the solar wind and heating of the solar corona. WISPR does not look directly at the Sun. Its very wide field-of-view extends from 13° away from the center of the Sun to 108° from the Sun.", "items": [], "extra_data": {} }, { "id": 327162, "url": "https://svs.gsfc.nasa.gov/12927/#media_group_327162", "widget": "Video player", "title": "", "caption": "", "description": "This animation shows Parker Solar Probe flying through the solar corona and coronal mass ejections. The fields-of-view of the WISPR telescopes can be seen as the transparent pyramids pointing out the side of the spacecraft.

Credit: NASA/JPL/WISPR Team", "items": [ { "id": 249397, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 404904, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012900/a012927/LARGE_MP4_12927_PSPCMEFOV2018V091080p_large.00001_print.jpg", "filename": "LARGE_MP4_12927_PSPCMEFOV2018V091080p_large.00001_print.jpg", "media_type": "Image", "alt_text": "This animation shows Parker Solar Probe flying through the solar corona and coronal mass ejections. 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WISpr iis pointed slight away from the Sun to image the corona.

Credit: NASA/JPL/WISPR Team

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The movie shows how as Parker Solar Probe get closer to the Sun on each orbit, the size of the fields-of-view change. The FOV are scaled properly with respect to the size of the Sun, and the time scales of this change and the SECCHI images are the same.

Credit: NASA/JPL/WISPR Team

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