PUNCH News

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.

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.

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.

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.

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.

In the predawn hours of March 4, the PUNCH spacecraft – now encapsulated in a 43-foot-tall Falcon 9 fairing – were transported across Vandenberg Space Force Base to the SpaceX hangar and pad failiities at Space Launch Center 4, on the south side of the base. The moment was captured by a passenger on the morning Amtrak train from San Luis Obispo to Los Angeles, visible through the tinted window of a passenger car as the train paused at the Surf Beach station west of VSFB. Photo credit: Catherine Bandy.

The four PUNCH spacecraft are now at Vandenberg Space Force Base (VSFB) in California, undergoing final test and integration to the “launch stack” with the SPHEREx spacecraft. All five spacecraft are planned to launch on a Falcon 9 rocket from Vandenberg Space Force Base no earlier than February 27, 2025.