Webb1 jan. 2012 · An empirical model of the photosphere rests on observations of: (1) the solar constant—which fixes the temperature scale, (2) limb darkening—from which the … WebbThe photosphere is the bright visible surface of the sun, with a surface temperature of 5,800 K. The chromosphere consists of the bright gases just above the photosphere of …
The sun
Webb29 maj 2024 · The visible surface of the Sun, or the photosphere, is around 6,000°C.But a few thousand kilometers above it — a small distance when we consider the size of the … Webb1. In the upper photosphere, the electrons join with the ions to neutralize the atom. When a photon strikes this atom (the atom absorbs the photon), it promotes a electron from a low energy shell to an higher energy shell. The electron then falls back to the lower energy shell emitting a photon in a different direction. lithoglyphus naticoides
Chromosphere - Wikipedia
WebbThe Sun’s atmosphere Solar atmosphere is generally subdivided into multiple layers. From bottom to top: photosphere, chromosphere, transition region, corona, heliosphere In its simplest form it is modelled as a single component, plane-parallel atmosphere Density drops exponentially: (for isothermal atmosphere). T=6000K Hρ≈ 100km WebbThe photosphere is the lowest of the three layers that make up the Sun's atmosphere. Because the two upper layers are transparent to most of the wavelengths of visible light, the photosphere can be easily appreciated. We can not see beyond the bright gases of the photosphere, so that everything underneath it is considered the interior of the Sun. Webb22 jan. 2013 · The sun's magnetic fields rise through the convection zone and erupt through the photosphere into the chromosphere and corona. The eruptions lead to solar activity, which includes such phenomena as sunspots, flares, prominences, and coronal mass ejections. Credit: NASA/Goddard. Link to unlabeled version. Last Updated: Aug 7, … im so wavey