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See all on WikipediaCoronal loop - Wikipedia
In solar physics, a coronal loop is a well-defined arch-like structure in the Sun's atmosphere made up of relatively dense plasma confined and isolated from the surrounding medium by magnetic flux tubes. Coronal loops begin and end at two footpoints on the photosphere and project into the transition … See more
Due to a natural process called the solar dynamo driven by heat produced in the Sun's core, convective motion of the electrically conductive plasma which makes up the Sun … See more
Wikipedia text under CC-BY-SA license Solar prominence - Wikipedia
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, often in a loop shape. Prominences are anchored to the Sun's surface in the much brighter photosphere, and extend outwards into the solar corona. While the corona consists of extremely hot plasma, prominences contain much cooler pl…
Wikipedia · Text under CC-BY-SA license- Estimated Reading Time: 9 mins
Coronal Loops - Center for Science Education
WEBCoronal loops are ropey, curving strands of plasma that appear as arcs above the Sun's surface. Hot, dense plasma causes these loops to glow. The electrified plasma flows along the curving lines of powerful magnetic …
Solar Prominences | Total Solar Eclipse 2017 - NASA
Why is the Sun’s corona so hot? Why are prominences so cool?
WEBAug 1, 2017 · An erupting prominence and the associated expulsion of the surrounding coronal loop system can lead to one of the most dramatic solar events: a coronal mass …
What is a solar prominence? - NASA
WEBA solar prominence (also known as a filament when viewed against the solar disk) is a large, bright feature extending outward from the Sun’s surface. Prominences are …
SWS - The Sun and Solar Activity - What is a Coronal Hole
WEB3 days ago · Coronal holes occur when the Sun's magnetic field is open to interplanetary space. Conversely, in regions where the solar magnetic fields loop back to the Sun …
Coronal Loops - NSO - National Solar Observatory
WEBCoronal loops are bright curving structures arcing above the surface of the Sun. Driven by the looping lines of the Sun’s twisted and powerful magnetic fields, these arcs of plasma are usually, but not always, rooted in sunspots.
A solar illusion: Coronal loops may not be what they …
WEBMar 2, 2022 · Many coronal loops — ropey strands of plasma that scientists have long thought existed in the Sun’s atmosphere — may actually be optical illusions, according to a new paper that challenges …
15.4: Solar Activity above the Photosphere - Physics LibreTexts
WEBJul 29, 2023 · Moving higher into the Sun’s atmosphere, we come to the spectacular phenomena called prominences (Figure 15.19), which usually originate near sunspots. …
Unveiling the mystery of solar-coronal heating - AIP …
WEBApr 1, 2023 · Bright coronal loops, which take the form of coronal condensations (regions of warmer, denser plasma) and bright spots, are common around the time of solar maxima. Larger faint loops that last …
What Is the Sun's Corona? | NASA Space Place – NASA Science …
WEBSep 27, 2024 · The Sun’s corona is the outermost part of the Sun’s atmosphere. The corona is usually hidden by the bright light of the Sun's surface. That makes it difficult to see …
Red Dots around Total Solar Eclipse Explained - Scientific American
WEBApr 8, 2024 · A solar prominence is a massive loop of the sun’s plasma that hangs attached to the visible surface of the sun, forming perhaps within a day but lasting as …
Prominences, Solar Flares, Coronal Mass Ejections - Britannica
WEB2 days ago · Loop prominences, on the other hand, are cooling from a very hot post-flare coronal condensation and have just become visible. Thus, they show high-excitation …
Prominences: The Key to Understanding Solar Activity
WEBProminences are spectacular manifestations of both quiescent and eruptive solar activity. The largest examples can be seen with the naked eye during eclipses, making …
Solar Prominences: Observations | Living Reviews in Solar Physics
WEBMar 12, 2014 · Solar prominences are one of the most common features of the solar atmosphere. They are found in the corona but they are one hundred times cooler and …
Streamers and Loops: What the Sun’s Hyperactive Phase Means …
WEBMar 21, 2024 · The prominences appear like streamers that are anchored to the surface of the Sun, with energy and radiation accelerated along magnetic field lines, and a solar …
Prominence/Filaments - NSO - National Solar Observatory
WEBWhen a prominence breaks free of the Sun, astronomers call this detachment a coronal mass ejection, or CME. A solar prominence is a large, bright and often looping feature …
Coronal Holes | NOAA / NWS Space Weather Prediction Center
WEBCoronal holes appear as dark areas in the solar corona in extreme ultraviolet (EUV) and soft x-ray solar images. They appear dark because they are cooler, less dense regions than …
Coronal Loops - an overview | ScienceDirect Topics
WEBCoronal loops are curvilinear structures in the solar corona that align with the magnetic field and are defined by the spatial extent of the heating source. They consist of thermally …
Solar prominences: theory and models - PMC - National Center …
WEBOct 22, 2018 · The focus for this review is the physical state of the non-erupting prominence, i.e., the nature of its magnetohydrodynamic (MHD) quasi-equilibrium. In …
Coronal Transverse Magnetohydrodynamic Waves in a Solar …
WEBDec 7, 2007 · Solar prominences are classified as either quiescent or active region (AR), the latter referring to material suspended above sunspot magnetic regions. Quiescent …
Transequatorial loop - Wikipedia
WEBPictured is the Sun as seen in soft x-ray with a transequatorial loop slightly right of center arcing across the solar equator. In solar physics, a transequatorial loop is a structure …
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