Ch 26-1 The sun

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robtownsend

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The Sun 26.1 Energy From the Sun Forces in Balance Atmosphere Features

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Please write a full essay describing the following phenomen solar and how the Sun\'s magnetic field produces each of prominences, solar flares, CME\'s and auroras. Solution The sun, like the earth, generates a magnetic field that extends out into space. However, the sun\'s magnetic field changes both its shape and intensity over the surface, and over time, much more rapidly.In the Sun, the flows of hot plasma in the convection zone create the solar magnetic field. The plasma is a hot gas \"soup\" with many free charged particles (electrons and protons). The moving charges are a current, and produce magnetic fields, just like the current in coils of wire around the nail. What\'s different in the sun? The convection current is driven by the heat from the Sun\'s fusion, instead of a battery. Sunspots are regions of very strong magnetic field, where the field lines get so crowded together that they push up through the surface, bringing some of the hot plasma with them in a spectacular arc, or loop. We see the end of the loop as a sunspot on the sun\'s visible surface, or photosphere. This dense bundle of field lines creates huge magnetic pressures. What is magnetic pressure? We know what pressure is in a gas: if you compress some gas, like squeezing a balloon, it tries to push out again. A solar flare is a magnetic storm on the Sun which appears to be a very bright spot and a gaseous surface eruption. Solar flares release huge amounts of high-energy particles and gases and are tremendously hot (from 3.6 million to 24 million °F). They are ejected thousands of miles from the surface of the Sun. A solar prominence (also known as a filament) is an arc of gas that erupts from the surface of the Sun. Prominences can loop hundreds of thousands of miles into space. Prominences are held above the Sun\'s surface by strong magnetic fields and can last for many months. At some time in their existence, most prominences will erupt, spewing enormous amounts of solar material into space. The outer solar atmosphere, the corona, is structured by strong magnetic fields. Where these fields are closed, often above sunspot groups, the confined solar atmosphere can suddenly and violently release bubbles of gas and magnetic fields called coronal mass ejections. A large CME can contain a billion tons of matter that can be accelerated to several million miles per hour in a spectacular explosion. Solar material streams out through the interplanetary medium, impacting any planet or spacecraft in its path. CMEs are sometimes associated with flares but can occur independently..

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Ch 26-1 The sun

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