Table of thermodynamic temperatures: more meaningful column heading; {{val}}
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!Temperature |
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!Kelvin |
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!Peak emittance<br />[[wavelength]]<ref>The cited emission wavelengths are for true black bodies in equilibrium. In this table, only the sun so qualifies. [https://physics.nist.gov/cgi-bin/cuu/Value?bwien CODATA recommended value] of {{val|2.897771955|end=...|e=-3|u=m⋅K}} used for Wien displacement law constant ''b''.</ref> of<br />[[Wien's displacement law|black-body photons]] |
!Peak emittance<br />[[wavelength]]<ref>The cited emission wavelengths are for true black bodies in equilibrium. In this table, only the sun so qualifies. [https://physics.nist.gov/cgi-bin/cuu/Value?bwien CODATA recommended value] of {{val|2.897771955|end=...|e=-3|u=m⋅K}} used for Wien displacement law constant ''b''.</ref> of<br />[[Wien's displacement law|black-body photons]] |
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|style="text-align:right"|[[Lightning|Lightning bolt's]]<br />channel |
|style="text-align:right"|[[Lightning|Lightning bolt's]]<br />channel |
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|28,000 K |
|{{val|28,000|u=K}} |
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|100 nm<br />(far [[ultraviolet]] light) |
|100 nm<br />(far [[ultraviolet]] light) |
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