Tag: Parker Solar Probe
-

Parker Solar Probe Reveals 2D Maps of the Sun’s Invisible Corona
New Window Into the Sun’s Outer Atmosphere In a milestone for solar science, NASA has produced detailed two-dimensional maps of the sun’s corona—the outermost layer of the Sun’s atmosphere. Crafted from years of close solar passages by the Parker Solar Probe, these maps reveal the corona’s complex structure at moments of peak solar activity, offering…
-

NASA’s Parker Solar Probe maps the unseen sun at its most active moment
Introduction: a new window into the sun’s outer atmosphere Scientists have achieved a historic milestone: creating detailed, two‑dimensional maps of the sun’s outer atmosphere, or corona, during the star’s most dynamic phase. This breakthrough comes from data gathered by NASA’s Parker Solar Probe, a spacecraft designed to plunge close to the sun and endure extreme…
-

Parker Solar Probe Maps the Sun’s Hidden Atmosphere at Peak Activity
Revealing the Sun’s Hidden Border Scientists have achieved a milestone in solar observation by producing detailed 2D maps of the sun’s outer atmosphere, or corona, using data from NASA’s Parker Solar Probe. The maps capture the corona at its most active moments, when solar winds and magnetic forces surge outward into space. This development marks…
-

Parker Solar Probe Captures Solar Wind U-Turn: New Clues from the Sun
What the Parker Solar Probe Found NASA’s Parker Solar Probe has delivered the clearest look yet at solar wind material that curls away from the Sun and then makes a surprising U-turn, returning toward the star. This striking behavior helps scientists observe the complex choreography of solar wind as it escapes the Sun’s outer atmosphere,…
-

Parker Solar Probe Captures Solar Wind U-Turn: Solar Recycling Revealed
New View of Solar Wind Dynamics The Parker Solar Probe, NASA’s mission designed to skim the outer layers of the Sun, has delivered the clearest evidence yet of solar material changing direction in a dramatic “U-turn.” This unexpected behavior comes as researchers sift through hundreds of data points collected as the spacecraft flew through the…
-

Parker Solar Probe Reveals Solar Wind U-Turn Phenomenon
Bright Insight from a Solar Pioneer NASA’s Parker Solar Probe has once again pushed the boundaries of solar science, capturing the most detailed view yet of the solar wind as it escapes the Sun and then appears to loop back in a surprising U-turn. This closer look helps scientists better understand how material leaves the…
-

Solar Storms and Solar Wind: How Particles from the Sun Interact with Earth
What are solar wind and solar storms? Every day, Earth experiences weather—wind, rain, and storms. But there’s also weather in space, driven by the Sun. Two key ideas scientists talk about are the solar wind and solar storms. The solar wind is a continuous stream of charged particles, mainly protons and electrons, that blow outward…
-

Solar Storms and Solar Wind: How Particles from the Sun Shape Life on Earth
What are solar wind and solar storms? Every day, Earth experiences weather in the sky—wind, clouds, rain. But there’s also weather in space, driven by the Sun. Two key phenomena in space weather are the solar wind and solar storms. The solar wind is a steady stream of charged particles—mostly protons and electrons—that flows continuously…
-

Solar storms and solar wind: How the Sun shapes space weather
What are solar wind and solar storms? Every day, Earth experiences weather—wind, rain, and storms. In space, there is also weather, created by the Sun. Two key players in space weather are the solar wind and solar storms. The solar wind is a constant, ever-present flow of charged particles blasting outward from the Sun. Solar…
-

Helio Highlights: The Sun and Our Lives
The Sun and Our Lives: Why This Matters On a clear night, thousands of stars glitter in the sky, but during the day there is one constant: the Sun. Its proximity—about 93 million miles (150 million kilometers)—makes it not only the nearest star but also the energy engine that powers life on Earth. Astronomers measure…
