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Prominence

Published on Mar 22, 2016

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PRESENTATION OUTLINE

PROMINENCE

BY DIEGO GUTIERREZ

What is a prominence?
an eruption of a flamelike tongue of relatively cool, high-density gas from the solar chromosphere into the corona where it can be seen during a solar eclipse or by observing strong spectral lines in its emission spectrum.

A prominence is also called a corona

A solar prominence (also known as a filament) is an arc of gas that erupts from the surface of the Sun

A typical prominence extends over many thousands of kilometers

Some prominences are so powerful that they throw out matter from the Sun into space at speeds ranging from 600 km/s to more than 1000 km/s.

Photo by sdomission

The prominence plasma is typically a hundred times cooler and denser than the coronal plasma.

Photo by seishin17

A solar permanence can be bigger than Jupiter and the earth

Prominences may last for a few days or even for a few months.

Prominences appear either as flame-coloured projections when the disk of the Sun is totally eclipsed

In 1868 French astronomer Pierre Janssen and British astronomer Sir Joseph Norman Lockyer independently announced a method of observing prominences by spectroscope without waiting for an eclipse

Photo by arche288