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Solar Physics

All articles tagged with #solar physics

Backyard timelapse reveals edge-on solar plasma loop arcade
space1 month ago

Backyard timelapse reveals edge-on solar plasma loop arcade

Astrophotographer Mark Johnston captured a two-hour timelapse from his Scottsdale, Arizona backyard showing a rare coronal loop arcade—arches of hot plasma shaped by the Sun's magnetic field—extending above the solar limb, including visible coronal rain as material cools and falls along magnetic lines. The sequence, recorded on Aug. 21, 2026, was captured with a TEC160FL refractor and hydrogen-alpha solar imaging gear, delivering an edge-on view of the Sun from home.

Seventeen-Spacecraft Observation Reveals Two-Part Solar Eruption
space1 month ago

Seventeen-Spacecraft Observation Reveals Two-Part Solar Eruption

A December 2024 coronal mass ejection was tracked by a record 17 spacecraft spread across the solar system, showing the eruption consisted of two asymmetric lobes traveling at different speeds rather than a single front. This wide, off-axis coverage allowed scientists to reconstruct the CME’s two-dimensional shape and evolution, improving forecasts of how such solar storms propagate and boosting warning time for future crewed missions beyond Earth. Observations came from missions including SOHO, SDO, STEREO-A, MMS, ARTEMIS, Wind, ACE, GOES, DSCOVR, BepiColombo, MAVEN, Solar Orbiter, Europa Clipper, and others; the findings were published in Science Advances.

Aditya-L1 uncovers magnetic fix behind the Sun's scorching corona
science1 month ago

Aditya-L1 uncovers magnetic fix behind the Sun's scorching corona

New findings from India's Aditya-L1 mission show the Sun's outer atmosphere, the corona, is heated mainly by magnetic-field-line reconnection (≈93%), with surface waves contributing about 7%. By analyzing a highly energetic CME on 5 August 2024, scientists quantified energy replenishment and confirmed the corona remains exceptionally hot despite repeated eruptions; the results, published in Astrophysical Journal Letters, provide a key benchmark for solar physics.

Maui’s Sun-Telescope: how a 3.6-ton mirror stays cool enough to image the Sun
science1 month ago

Maui’s Sun-Telescope: how a 3.6-ton mirror stays cool enough to image the Sun

On Maui’s Haleakalā, the Daniel K. Inouye Solar Telescope uses a 3.6-ton Zerodur primary mirror and a seven-mile Dynalene coolant loop across 13 independent temperature zones; a heat-stop dumps about 95% of the incoming heat from a 12 kW beam, with nightly ice cooling to prevent overheating, enabling the sharpest solar images yet (roughly 20 km resolution) and revealing fine-scale solar features while funding questions loom over its operation.

NASA’s sky-high eclipse mission reveals the Sun’s hidden fireworks
science2 months ago

NASA’s sky-high eclipse mission reveals the Sun’s hidden fireworks

NASA will fly a WB-57 research plane at about 50,000 feet off Iceland to chase a total solar eclipse, using high-speed cameras to capture the Sun’s corona—prominences and nanoflares—in order to extend totality for nearly three minutes and gather data that improves understanding of solar physics and space weather, a method favored over ground- or space-based observations for its data richness despite harsh conditions, building on a long history of eclipse missions.

Sun Reveals Magnetic Whirlpools in Ultra-Clear Solar Images
science2 months ago

Sun Reveals Magnetic Whirlpools in Ultra-Clear Solar Images

Ultra-detailed images from the Inouye Solar Telescope show Kelvin-Helmholtz swirl patterns in the Sun’s magnetic field, with vortices about 50–65 kilometers apart. These twisting motions transfer and concentrate magnetic energy, potentially fueling solar eruptions such as flares and coronal mass ejections, which can affect space weather and threaten power grids and satellites.

Sun Surface Unveils Kelvin-Helmholtz Vortices, Illuminating Solar Magnetism
science2 months ago

Sun Surface Unveils Kelvin-Helmholtz Vortices, Illuminating Solar Magnetism

Scientists using the Daniel Inouye Solar Telescope on Haleakalā captured high‑resolution images of the Sun’s surface, revealing small plasma vortices formed by Kelvin‑Helmholtz Instability. These vortices help drive magnetic field mixing and heat transport toward the Sun’s outer atmosphere, offering new insights into solar flares, coronal mass ejections, and why the Sun’s atmosphere is hotter than its surface.

Sun’s surface reveals Kelvin–Helmholtz whirlpools captured by the Inouye Solar Telescope
space2 months ago

Sun’s surface reveals Kelvin–Helmholtz whirlpools captured by the Inouye Solar Telescope

New ultra-high-resolution images from the Daniel K. Inouye Solar Telescope reveal thousands of tiny whirlpools on the Sun’s surface, providing the first direct observation of Kelvin–Helmholtz instabilities on the Sun. The observed vortices, matching computer simulations, may help mix magnetic fields and contribute to heating the corona and driving space-weather events like solar flares and CMEs.

Sun’s surface whirlpools revealed by ultra-high-resolution telescope
science-space2 months ago

Sun’s surface whirlpools revealed by ultra-high-resolution telescope

Using the Daniel K. Inouye Solar Telescope near Maui, scientists captured the Sun’s visible surface in unprecedented detail, revealing Kelvin-Helmholtz instabilities—tiny swirling vortices along magnetic boundaries—that could explain why the Sun’s outer atmosphere (the corona) is hotter than its surface and how magnetic energy is built, released and transported to drive solar flares and coronal mass ejections. The observations align with advanced simulations and may improve space-weather forecasting that affects satellites and power grids.

Sun's surface reveals tiny plasma vortices captured in unprecedented detail
science2 months ago

Sun's surface reveals tiny plasma vortices captured in unprecedented detail

Using the world’s largest solar telescope, astronomers captured the Sun’s visible surface at unprecedented resolution, revealing vortices as small as about 12 miles wide at the edges of solar granules and linking them to Kelvin-Helmholtz instabilities driven by convection and magnetic fields, shedding light on the dynamic processes shaping the Sun’s photosphere.

Sun Surface Reveals Ubiquitous Whirlpools in New High-Res Images
science2 months ago

Sun Surface Reveals Ubiquitous Whirlpools in New High-Res Images

High-resolution images from the NSF’s Daniel K. Inouye Solar Telescope show Kelvin-Helmholtz instabilities across the Sun’s magnetic boundaries, revealing ubiquitous small-scale whirlpools that may help mix plasma and magnetic fields, influence energy transport, and contribute to understanding space weather; findings published in Nature.

Gravity, not a bigger engine, drives Parker Solar Probe's sun-speed record
space3 months ago

Gravity, not a bigger engine, drives Parker Solar Probe's sun-speed record

Parker Solar Probe reached a record ~430,000 mph near the Sun not primarily through propulsion, but through seven Venus gravity assists over seven years that gradually lowered its solar orbit. As the probe fell closer to the Sun, the Sun's gravity converted potential energy into kinetic energy, making it the fastest human-made object in history. The feat highlights orbital design and gravity as key drivers in spaceflight, while the mission continues to study the Sun’s corona and solar wind.

Sun's preflare signals mapped hours before a powerful X9 flare
space3 months ago

Sun's preflare signals mapped hours before a powerful X9 flare

Space.com reports that scientists using IRIS data captured a rare preflare window for the Oct. 3, 2024 X9 solar flare. They tracked three plasma properties—brightness, line-of-sight velocity, and non-thermal velocity (turbulence)—which began rising about three hours before eruption and showed regular oscillations (roughly 7–10 minutes and 18–21 minutes) near a boundary where opposite magnetic fields meet. About 15–20 minutes before the flare, the sun’s atmosphere became more volatile, signaling possible magnetic energy release. While the study suggests a potential precursor signature from combining these signals, it analyses a single event, and more flares must be studied before reliable early warnings can be developed. The findings were published in Solar Physics.