![]() It is almost certain that its energy comes from the Sun's internal furnace, which also supplies the rest of the Sun's heat. The source of the corona's heat remains a puzzle. Such high levels of ionization require the atoms to be buffeted around by extremely high temperatures, around 1,000,000 C (1,800,000 F). Unknown spectral lines emitted by the corona were similarly credited to a new element "coronium" until Edlen showed that they came from the familiar atoms of iron, nickel and calcium, after they had lost an appreciable number of electrons (e.g. Later, in 1895, William Ramsey actually discovered helium on Earth. In the 19th century, some of the spectral lines of sunlight did not match the lines of any substance on Earth, and it was proposed that they came from a new unknown chemical element, named helium (from the Greek helios-Sun). Much of that is sunlight scattered by coronal dust, but some light is also produced by the corona itself, in narrowly defined colors ("spectral lines") characteristic of its emitting atoms. XThe most remarkable aspect of the corona is its high temperature, deduced by the Swedish astronomer Bengt Edlen in 1942 after a study of the corona's light. Astronomers have named them "helmet streamers" because of their resemblance to spiked helmets worn by knights (and also to those used by some German soldiers up to 1918). ![]() From the tops of such "arches" long streamers may extend, to distances of the Sun's diameter or even more, looking like pulled taffy, as if some process was pulling material away from the tops of the arches into space, (which is of course what the solar wind actually does). Structures observed in the corona above sunspots often have horseshoe-shaped outlines, again suggesting that they follow magnetic field lines. For instance, short "plumes" rising from the polar regions of the Sun look very much like field lines coming out of the end of a bar magnet, and they therefore suggest that the Sun, in addition to the intense fields of sunspots, also has a global magnetic field like the Earth's. Structures visible in the corona at such times suggest that they are shaped by magnetic fields, and therefore, that the corona consists of plasma. Such a geomagnetic storm can also create problems for spacecraft operations, resulting in surface charging and tracking problems.During a total eclipse of the Sun, when for a few minutes the Moon completely covers the Sun's face, a glow appears around the darkened Sun-the solar corona, the Sun's outermost atmosphere. G4 storms, in particular, are the strongest and are capable of causing widespread voltage control problems in power grids and mistakenly tripping critical electric assets of the grid in protection systems. Geomagnetic storms are disturbances to Earth's magnetic field due to solar material from CME - large expulsions of plasma and magnetic fields from the Sun's atmosphere. But the blow, which came before time, was far from moderate.Ī coronal mass ejection hit our planet's magnetic field on April 23, resulting in a severe G4-class geomagnetic storm. Space weather experts were expecting G1- (Minor) to G2-class (Moderate) geomagnetic storms to strike Earth on April 24. The scary part? It hurled a cloud of debris in our planet's direction! ![]() ![]() And on Friday, a massive magnetic filament snaking across the Sun's southern hemisphere exploded. The last few months have been rather eventful for the Sun, what with randomly blowing up and shooting out coronal mass ejections.
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