PUNCH News

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Also see the NASA PUNCH blog

Current front page items
2025-04-13 PUNCH Science Nugget

During the week of 2025 April 7, PUNCH collected calibration data from the instruments – our last chance to take advantage of closed doors, before they open. Even these “dark frames”, taken with the doors closed, are interesting to look at. These images are “Level 0” (unprocessed) data products generated by the Science Operations Center (SOC), with full flight metadata attached. The cameras are working properly, with low noise levels. The images are brighter on the right because PUNCH uses dual readout detectors, with separate digitizers for the two halves of the images; they have slightly different zero points, an effect we remove at “Level 1” and higher. There is a very small amount of light visible in the upper left, which we believe is stray light scattered by the closed instrument door itself. Over the South Atlantic Anomaly in Earth’s magnetic field, an area of enhanced cosmic ray flux, we see significant particle impacts on the detector. The rate of impacts agrees with calculations performed over six years ago, during the mission’s Phase A concept study.


2025-04-04 PUNCH Science Nugget

PUNCH will maintain the constellation with a novel, water-powered, shot-glass-sized rocket engine attached to each spacecraft. Each spacecraft carries about a British pint (600 g) of water in a small canister. To run the engine, PUNCH electrolyzes about 1/10 tsp (0.5 mL) of water, building up small stores of hydrogen and oxygen at about 200 psi. Then it burns the fuel in just a few seconds. Each cycle delivers a “kick” of about one inch/sec (2 cm/sec): just enough to correct for small orbital shifts and keep the constellation stable. PUNCH is the first space mission to use this type of engine, which carries safe propellant but is complex to operate.


2025-04-02 PUNCH Science Nugget

On March 29, 2025, many folks went outside to catch a glimpse of the partially eclipsed Sun, as the Earth carried them through the Moon’s shadow. PUNCH, orbiting high overhead, also passed through the shadow. Orbital velocities are high, so each spacecraft passed through the darkest part of the partial eclipse (the Moon’s penumbra) at a slightly different time, about eight minutes apart. Even though the instruments’ doors are still closed for commissioning, PUNCH registered the eclipse. During the brief interval of darkest shadow, the solar arrays couldn’t keep up with on-board power usage and each spacecraft briefly switched to battery power, using slightly less than 1% of its battery capacity to keep operating normally through the brief gap.


Archive
2025-03-31 PUNCH Science Nugget

While making its unique observations, PUNCH will augment a fleet of international spacecraft observing the Sun and solar system, including NASA's Parker Solar Probe and STEREO missions, the European Space Agency's (ESA) Solar Orbiter and Jupiter Icy Moon Explorer (JUICE) missions, and the ESA/Japanese Space Agency's (JAXA) BepiColombo mission, all of which afford unique joint science opportunities. The longitudinal trajectories of these missions are shown along with the orbits of Mercury, Venus, and Mars relative to an Earth-stationary frame of reference. On this scale, PUNCH is always located at Earth. Trajectories were generated by the Austrian Space Weather Office / GeoSphere Austria (Möstl/Davies/Weiler) – further details and additional movies available.


2025-03-24 PUNCH Science Nugget

The Science Operations Center (SOC) for PUNCH received the first data packets from the four spacecraft. The data downlinks included both engineering and test image packets. The SOC successfully decompressed the packets and reconstructed the expected striped test pattern image. Using a test pattern allows the SOC to verify that data is properly transmitted and formed into images. The spacecraft sends engineering packets down alongside the images that indicate spacecraft parameters such as orientation and position. The SOC’s automated processing routines ingested this data and confirmed the spacecraft are pointing toward the Sun as expected. A good estimate of the spacecraft pointing is critical for the SOC’s data processing; it would not be possible to construct the seamless mosaics required to answer PUNCH’s science questions without it. The next step is to collect and process calibration images without light on the sensor, commonly called dark images. More information about the SOC processing can be found on GitHub.


2025-03-16 PUNCH Science Nugget

The heliophysics community came out to celebrate the impending launch by presenting and discussing the latest developments in PUNCH science, including the origin and evolution of the ambient solar wind and turbulence within it, and the physics, tracking and predictability of transient events such as coronal mass ejections, corotating interaction regions, and shocks. Beyond these primary PUNCH science topics, the workshop provided a forum for exploring PUNCH connections to the magnetosphere and aurora, zodiacal dust, and sun-grazing comets and other solar system objects. PUNCH's readiness to engage scientists around the world was demonstrated through presentations and a hands-on tutorial on data access, and its synergies with a range of community missions and models explored through panel discussions. The meeting took place February 25th and 26th, 2025 at Cal Poly in San Luis Obispo, CA, and benefited from the support and involvement of Cal Poly students and faculty. It was further enriched by PUNCH outreach events before and during the meeting.


2025-03-14 PUNCH Science Nugget

The four PUNCH spacecraft are separating nominally and performing well sixty hours post-launch, as they prepare for their groundbreaking science. All four have demonstrated high speed S-band communications, entered fine pointing mode, and are in good health and ready to transition to “normal operations”. Commissioning will continue, but will be staffed single shift only (rather than 24-hours) and use nominal pass priority with the ground data network provider. Ground tracks from the spacecraft themselves (using on board GPS) agree with NORAD tracks and are consistent with both the mission design and deployment videos from launch day. The PUNCH Observatories carry orbital-trim thrusters; a midcourse correction is planned for later in March, to ensure identical orbital planes and even spacing as the PUNCH WFI Observatories drift to 120° relative spacing in mean anomaly.



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