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Re: CMBR and neutron stars

Subject: Re: CMBR and neutron stars
From: "N:dlzc D:aol T:com \(dlzc\)" <N: dlzc1 D:cox T:>
Date: Mon, 8 Aug 2005 17:05:36 -0700
Newsgroups: sci.astro
Dear Steve Willner:

"Steve Willner" <willner@xxxxxxxxxxxxxxx> wrote in message 
news:42f7d731$1@xxxxxxxxxxxxxxxxxxxxxxxxxx
> In article <fOTIe.260908$Qo.161878@fed1read01>,
> "N:dlzc D:aol T:com \(dlzc\)" <N: dlzc1 D:cox T:net@xxxxxxxxxx> 
> writes:
> [in the solar atmosphere]
>> OK.  Note however that you can observe over a pretty long
>> distance, and it is approximately isothermal along along the
>> line-of-site.
>
> Except for very special wavelengths (e.g., in spectral lines of
> exactly the right opacity), I think you will have a hard time 
> finding
> a line of sight through or into the solar atmosphere that is 
> even
> approximately isothermal.

...and observation at/near very special wavelengths will make 
determination/estimation of a blackbody curve a sort of private 
joke.  Thanks!

David A. Smith 



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