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AZgazer
2004-Apr-30, 06:03 PM
I was reading some information about the Sun and I came across something that confused me. (I am only listing the portion I found confusing.) The diagram/explanation of each layer of the sun gave these stats. Radiative, 5,000,000 K; Convection, 5,800 K; Photosphere, 4,400 K - 6,600 K; Chromosphere, 30,000 K.

How does the temperature go from hot to cooler and back to hotter again? Why are the outter temperatures so much hotter than the "middle" regions?

Hamlet
2004-Apr-30, 06:18 PM
I was reading some information about the Sun and I came across something that confused me. (I am only listing the portion I found confusing.) The diagram/explanation of each layer of the sun gave these stats. Radiative, 5,000,000 K; Convection, 5,800 K; Photosphere, 4,400 K - 6,600 K; Chromosphere, 30,000 K.

How does the temperature go from hot to cooler and back to hotter again? Why are the outter temperatures so much hotter than the "middle" regions?

It's still a bit of a mystery, but there are a few theories floating around.

This (http://www.sunblock99.org.uk/sb99/people/KGalsgaa/sb99_num.html) has a little more.

It's been a while since I've seen anything new on this phenomenon, but it is quite interesting.

crazy4space
2004-Apr-30, 06:30 PM
Wait until you try to find the magnetic poles. #-o If you think that one is hard check out the actual rotation. :o

milli360
2004-May-01, 08:16 PM
How does the temperature go from hot to cooler and back to hotter again? Why are the outter temperatures so much hotter than the "middle" regions?
Here's an interesting graphic (http://www.enchantedlearning.com/subjects/astronomy/planets/earth/Atmosphere.shtml) about the Earth's own atmospheric regions, and how temperature varies within them.