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On April 18, 2025, the WFI-2 instrument (which on April 14) took images through all three of its polarizers in succession for the first time to create this view. The image is colorized to show the polarization (or angle) of the zodiacal light, a faint glow from dust orbiting the sun. Hue indicates direction, and saturation indicates degree of polarization. For example, a pastel green feature would be slightly polarized in the horizontal direction, while a deep blue feature would be strongly polarized in a diagonal direction. The sun’s location is marked with a star symbol. Other stars in the sky appear white because they are mostly unpolarized compared to the 7% polarization of the zodiacal light. The compact Pleiades star cluster appears just above center, and the V-shaped Hyades star cluster appears to the upper left of the Pleiades. Credit: NASA/SwRI
As instrument commissioning and calibration checks continue for NASA's newly launched PUNCH (Polarimeter to Unify the Corona and Heliosphere) mission, its four spacecraft continue to deliver new images—including its first rainbow-colored view of the sky and the first images taken by two of its instruments.
The goal of PUNCH is to reveal new details of how the solar atmosphere, or corona, unfolds and streams through the solar system as the solar wind. It is the first mission designed to measure the corona and solar wind in three dimensions by studying the polarization of light, which is the direction light travels after it has been scattered by particles.
In PUNCH's images, the polarization is revealed through color coding, resulting in a rainbow image that gives scientists new insight on the solar wind's movement.
Collectively, PUNCH's four satellites include one Narrow Field Imager (NFI) and three Wide Field Imagers (WFIs). The NFI is a coronagraph, which blocks out the bright light from the sun to better see details in the sun's corona. The WFIs are heliospheric imagers that view the very faint, outermost portion of the solar corona and the solar wind itself.
During commissioning, PUNCH’s NFI instrument captured this image of the new moon as it passed by the sun in the sky on April 27, 2025. The new moon appears full, because it is illuminated by Earthshine (sunlight reflected off Earth). The image helped the PUNCH team confirm that the moon will not obscure NFI’s view of the corona and solar wind. The dark circle near the bottom is the shadow of NFI’s occulter, which hides the sun. The occulter, which was not yet fully aligned with the Sun, is surrounded by a narrow bright ring of diffracted light. Around that is a large, hazy circle of stray light glinting off the occulter (the moon is inside that circle). Outside that is a small, dimmer region of the sky that is less affected by glint. Credit: NASA/SwRI
The mission's fully processed science data will stitch together views from all four spacecraft and remove artifacts from the background of space and the cameras themselves. These early images help the mission team confirm that PUNCH's cameras are in focus, working properly, and able to capture the quality observations needed to achieve the mission's goals.
Throughout the remainder of the commissioning phase, scientists will calibrate the instruments' views to reveal illuminating details in the sun's corona.
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NASA's PUNCH catches first rainbow and other new images (2025, May 13)
retrieved 15 June 2025
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NASA's PUNCH mission has begun returning images, including a rainbow-colored view that visualizes light polarization, offering new perspectives on the solar wind and corona. Using one Narrow Field Imager and three Wide Field Imagers, PUNCH aims to map the solar atmosphere and wind in three dimensions, with early data confirming instrument performance and calibration.
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NASA's PUNCH catches first rainbow and other new images
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