Calculating velocity dispersion of hydrogen atoms in solar photosphere

AI Thread Summary
To calculate the velocity dispersion of hydrogen atoms in the solar photosphere at 5800 K, one should consider using the Maxwell distribution. The discussion highlights a lack of familiarity with relevant equations or methods for solving velocity dispersion problems. Guidance is sought on how to approach this calculation, particularly in the context of an astrophysics course. The Maxwell distribution is suggested as a foundational concept to explore further. Understanding this distribution will aid in addressing the problem effectively.
neslorelyks
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1. Calculate the velocity dispersion for hydrogen atoms in the solar photosphere, which has a temperature of 5800 K.


2. I know no equations to solve the problem.



3. I have no idea any method of going about solving for velocity dispersion. I would appreciate any guidance. Thanks
 
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Hi neslorelyks, welcome to PF!:smile:

What course is this problem for? Statistical mechanics perhaps? Introductory astrophysics?
 
I am taking an astrophysics course. Thanks for the reply. I need some guidance about how to go about solving any velocity dispersion problem. Any help would be appreciated.
 
I'm not sure how well it applies to a gas as hot as the Hydrogen in the solar photosphere, but you might want to look up the "Maxwell distribution" in your textbook for starters:wink:
 
Thank you
 
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