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About the PROBA2 Science Center | PROBA2 Science Center

About the PROBA2 Science Center

PROBA2

The PROBA2 Science Center, located at the Royal Observatory of Belgium in Brussels, oversees scientific operations and data processing for ESA's PROBA2 spacecraft. The P2SC is the primary archive and distribution center for data from SWAP and LYRA, as well as the primary maintainer of calibration tools, data analysis software, and additional instrument data. The P2SC is also home to the science operations center, where instrument observing plans are devised and, with the help of ESA's Spacecraft Operations Center in Redu, Belgium, loaded onto the spacecraft. Finally, the P2SC serves as the main site for coordination of the PROBA2 Science Working Team, coordinating special scientific campaigns, supporting science data users and guest investigators, and organizing PROBA2 outreach efforts.

PROBA2 is a small ESA satellite with a scientific mission to explore the active Sun and its effect on the near-earth environment and a broader mission to provide a test platform for new instrument and platform technology. The mission overview page provides additional information about PROBA2 and its on board instrumentation and advanced platform technology.

If you require special assistance, you can contact the instrument teams directly using the contact page on this new site.

News

Preparing for Comet C/2024 S1 (ATLAS)

UPDATE: the comet desintegrated before it reached the SWAP field-of-view.

A sungrazer comet is racing towards its close encouter with the solar corona. As part of a massive, world-wide campaign to study the comet, the SWAP imager will attempt to capture images of the comet as it passes the sun. If SWAP is able to see the comet, the observations could yield important information both about comets, the solar corona, and the sun's complex magnetic field.

Exceptional detection of an X9.0 flare by PROBA2

On October 3, the Sun unleashed its most powerful eruption since 2017: a solar flare classified as X9.0 on the GOES scale, accompanied by a significant coronal mass ejection. We also observed a signal related to this flare in the Herzberg channel which is extremely rare.

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