The corona is the region of the sun from the surface to about 1 million kilometers into space. Temperatures in the corona can reach as high as two million degree Fahrenheit.
The corona is the region of the sun from the surface to about 1 million kilometers into space. Temperatures in the corona can reach as high as two million degree Fahrenheit.
The temperature of the Sun's corona is millions of degrees Celsius. This high temperature is due to the extreme energy released during solar flares and other solar activities.
corona
The temperature of the sun's corona reaches at least one million degrees and possibly more. This is strange because the surface of the sun has temperatures of five thousand degrees. The corona is much farther away and logically should be cooler.
The corona is the region of the sun from the surface to about 1 million kilometers into space. Temperatures in the corona can reach as high as two million degree Fahrenheit.
The temperature of the sun's corona can reach over a million degrees Fahrenheit.
One interesting thing that has been found about the corona is that it's much hotter than the Sun's surface - while the Sun's surface has a temperature of about 6000 K, the corona has a temperature has a temperature around a million K. This obviously can't be caused by regular heat transfer; scientists are still researching exactly how the energy gets from the Sun to the corona.
The average temperature during the summer in Corona, California is seventy eight degrees. It various based on the year and which whether station you are watching.
The approximate temperature of a plasma stream is typically around 10,000 to 100,000 degrees Celsius.
21C
-400c
Astronomers know the temperature of the Sun's corona is high because they can observe the emission of extreme ultraviolet and X-ray radiation from the corona, which is only possible if the temperature exceeds millions of degrees Celsius. These observations are made using instruments such as spectrometers and telescopes designed for detecting these high-energy wavelengths.