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Travelling waves in the Sun's corona

Travelling waves in the Sun's corona

Date: 20 September 2010
Satellite: SOHO
Depicts: Sun's corona
Copyright: ESA/NASA - SOHO/EIT

This sequence of images shows a wave propagating in the solar corona at a speed of about 300 kilometres per second. The four images have been taken over a time interval of just over half an hour. The moving wavefront is a result of a Coronal Mass Ejection (CME), a colossal eruption during which enormous amounts of gas are released from the Sun into outer space.

The images have been taken by SOHO's Extreme ultraviolet Imaging Telescope (EIT) at a wavelength of 195 Å, corresponding to the emission line of 11-times ionised iron atoms (Fe XII) and showing material at temperatures of about 1.5 million Kelvin.

This series of snapshots was taken on 12 May 1997.

Last Update: 1 September 2019
24-Jun-2024 01:28 UT

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