NASA’s SunRISE comprises six small satellites, seen at
left lined up in a clean room, with solar arrays deployed. They will fly in
formation, as depicted in the artist’s concept at right, working as one large
radio telescope in Earth orbit.
Space Dynamics Laboratory/Allison Bills (photograph);
NASA/JPL-Caltech
NASA is targeting a summer 2026 launch
for its SunRISE (Sun Radio Interferometer Space Experiment) mission. The
heliophysics mission will launch as a rideshare aboard a United Launch Alliance
Vulcan Centaur rocket, sponsored by the United States Space Force’s Space
Systems Command.
The SunRISE mission will study solar
radio bursts and map the Sun’s magnetic field from the outer corona to
interplanetary space. Solar radio bursts result when vast quantities of energy
stored in the Sun’s magnetic field have accelerated particles to high speeds.
These energetic particles can stream into the solar system, where they can
impact spacecraft beyond the protective reach of the Earth’s magnetic field.
Studying how these bursts are generated will improve understanding of the Sun’s
radiation impacts on the space environment and, in turn, help lead to better
protection of astronauts and satellites. 
Solar radio bursts can arrive at Earth
shortly before potentially harmful particle radiation. The SunRISE mission has
the unique capability to image the approximate location of the burst and the
direction energetic particles are streaming, which can help space weather
forecasters better understand where a pending radiation event will be directed
and predict its effects.
A constellation of six small satellites,
each the size of a toaster oven, SunRISE will operate as one large radio
telescope about 6 miles (10 kilometers) wide, transmitting data to Earth via
NASA’s Deep Space Network. The SunRISE team will use the precise time and
position information received to combine the data from the individual SmallSats
into a virtual radio telescope — a technique known as interferometry. SunRISE
observes the Sun at radio wavelengths that are absorbed by the upper layers of
the Earth’s atmosphere, a region known as the ionosphere. By being in space,
SunRISE can conduct science that is not possible by ground-based radio
telescopes.
The SunRISE mission will complement
other NASA heliophysics missions, such as NASA’s Solar TErrestrial RElations
Observatory, Parker Solar Probe, and the Solar Orbiter satellite, an
international cooperative mission between ESA (European Space Agency) and NASA.
NASA’s SunRISE is a Mission of Opportunity under the Heliophysics Division of the agency’s Science Mission Directorate at NASA Headquarters in Washington. These missions are part of the Explorers Program, managed by NASA’s Goddard Space Flight Center in Greenbelt, Maryland. The mission’s science investigation is led by the University of Michigan in Ann Arbor, which also provides the science operations center, and the project is managed by NASA’s Jet Propulsion Laboratory in Southern California, a division of Caltech in Pasadena, California, which also provides the mission operations center. Utah State University’s Space Dynamics Laboratory built the SunRISE spacecraft.

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