Solar physics is the branch of astrophysics that specializes in the study of the Sun. It intersects with many disciplines of pure physics and astrophysics...
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ejections, solar particle events, and other eruptive solar phenomena. The occurrence of solar flares varies with the 11-year solar cycle. Solar flares are...
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Astrophysics (redirect from Astro physics)
studied in celestial mechanics. Among the subjects studied are the Sun (solar physics), other stars, galaxies, extrasolar planets, the interstellar medium...
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Total Solar Irradiance data Archived 2013-07-06 at the Wayback Machine updated every Monday N0NBH Solar data and tools SolarCycle24.com Solar Physics Web...
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Sun (redirect from Solar diameter)
(March 2015). "On the Determination and Constancy of the Solar Oblateness". Solar Physics. 290 (3): 673–687. Bibcode:2015SoPh..290..673M. doi:10.1007/s11207-015-0655-6...
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Space physics, also known as space plasma physics, is the study of naturally occurring plasmas within Earth's upper atmosphere and the rest of the Solar System...
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Carrington Event (redirect from The Solar Tempest of 1859)
(PDF). Solar Physics. 224 (1–2): 407–422. Bibcode:2004SoPh..224..407C. doi:10.1007/s11207-005-4980-z. S2CID 120093108. "Near miss: The Solar superstorm...
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The Parker Solar Probe (PSP; previously Solar Probe, Solar Probe Plus or Solar Probe+) is a NASA space probe launched in 2018 to make observations of...
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In solar physics, a prominence, sometimes referred to as a filament, is a large plasma and magnetic field structure extending outward from the Sun's surface...
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In solar physics and observation, granules are convection cells in the Sun's photosphere. They are caused by currents of plasma in the Sun's convective...
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The Institute for Solar Physics (Swedish: Institutet för solfysik) is a Swedish research institute. It is managed as an independent institute associated...
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Solarization refers to a phenomenon in physics where a material undergoes a temporary change in color after being subjected to high-energy electromagnetic...
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Helioseismology (redirect from Solar oscillation)
in stellar models and must instead be a problem of particle physics. The so-called solar neutrino problem was ultimately resolved by neutrino oscillations...
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Sunspot (redirect from Solar pore)
recognizable Solar phenomena and despite the fact that they are mostly visible in the solar photosphere they usually affect the entire solar atmosphere...
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for Solar Physics (aka: KIS; German: Institut für Sonnenphysik), from 2018 to 2023, the institute's name was Leibniz Institute for Solar Physics, formerly...
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Stellar corona (redirect from Corona (physics))
physics Why is the Sun's corona so much hotter than the Sun's surface? More unsolved problems in physics The coronal heating problem in solar physics...
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fellow, research scientist and assistant research professor at the Solar Physics Group at Montana State University, Bozeman, US. He returned to India...
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In solar physics, a spicule, also known as a fibril or mottle, is a dynamic jet of plasma in the Sun's chromosphere about 300 km in diameter. They move...
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interactions in the solar corona". Solar Physics. 18 (2): 258. Bibcode:1971SoPh...18..258P. doi:10.1007/BF00145940. S2CID 120816610. "Solar System Exploration:...
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Solar phenomena are natural phenomena which occur within the atmosphere of the Sun. They take many forms, including solar wind, radio wave flux, solar...
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heliophysics, which is an interdisciplinary combination of solar physics and planetary science. In the Solar System, the Sun can produce intense geomagnetic and...
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Observatory, La Palma in the Canary Islands. It is run by the Institute for Solar Physics of Stockholm University. The primary element is a single fused silica...
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Solar Physics is a peer-reviewed scientific journal published monthly by Springer Science+Business Media. The editors-in-chief are Lidia van Driel-Gesztelyi...
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Variations in the Solar Differential Rotation", Solar Physics, 212 (1): 23–49. St. John, C., 1918. "The Present Condition of the Problem of Solar Rotation",...
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the center to about 0.2 of the solar radius (139,000 km; 86,000 mi). It is the hottest part of the Sun and of the Solar System. It has a density of 150...
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The Solar Physics Division of the American Astronomical Society (AAS/SPD) or (AAS-SPD), often referred to as simply the "Solar Physics Division" (SPD)...
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Solar cycle 25 is the current solar cycle, the 25th since 1755, when extensive recording of solar sunspot activity began. It began in December 2019 with...
67 KB (3,031 words) - 04:00, 21 May 2025
Dipankar Banerjee ( born 1965) is an Indian solar physicist. He is a senior Professor of Solar Physics at the Indian Institute of Astrophysics (Bangalore)...
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Coronal mass ejection (category Solar phenomena)
then to the solar physics branch head, Dr. Tousey. Earlier observations of coronal transients or even phenomena observed visually during solar eclipses are...
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European Solar Physics Division (ESPD) of the European Physical Society (EPS), is an organisation whose purpose is to promote solar physics and represent...
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