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Affichage des articles dont le libellé est ASTRONOMY - The Sun in X-rays from NuSTAR. Afficher tous les articles
Affichage des articles dont le libellé est ASTRONOMY - The Sun in X-rays from NuSTAR. Afficher tous les articles

23/11/2021

ASTRONOMY - The Sun in X-rays from NuSTAR

 2021 November 23

The featured image shows the Sun in X-ray light as
shown by NASA's NuSTAR satellite -- superimposed on an image
in ultraviolet light taken by NASA's Solar Dynamic Observatory.
Please see the explanation for more detailed information.

The Sun in X-rays from NuSTAR
Image Credit: NASANuSTARSDO

Explanation: Why are the regions above sunspots so hot? Sunspots themselves are a bit cooler than the surrounding solar surface because the magnetic fields that create them reduce convective heating. It is therefore unusual that regions overhead -- even much higher up in the Sun's corona -- can be hundreds of times hotter. To help find the cause, NASA directed the Earth-orbiting Nuclear Spectroscopic Telescope Array (NuSTAR) satellite to point its very sensitive X-ray telescope at the Sun. Featured here is the Sun in ultraviolet light, shown in a red hue as taken by the orbiting Solar Dynamics Observatory (SDO). Superimposed in false-colored green and blue is emission above sunspots detected by NuSTAR in different bands of high-energy X-rays, highlighting regions of extremely high temperature. Clues about the Sun's atmospheric heating mechanisms come from NuSTAR images like this and shed light on solar nanoflares and microflares as brief bursts of energy that may drive the unusual heating.

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