How Do You Convert Monochromatic Flux Between Wavelength and Frequency Units?

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SUMMARY

The discussion centers on converting monochromatic flux between wavelength and frequency units, specifically using the formulas F(Δf) = ΔE / ΔtΔfΔA and F(Δλ) = ΔE / ΔtΔλΔA. The user seeks clarification on the derivation process, which involves differentiation or integration. Understanding these conversions is crucial for accurately analyzing stellar flux measurements in astrophysics.

PREREQUISITES
  • Understanding of monochromatic flux concepts
  • Familiarity with energy, time, and area in physics
  • Basic knowledge of differentiation and integration
  • Experience with astrophysical measurements and units
NEXT STEPS
  • Study the relationship between frequency and wavelength in electromagnetic radiation
  • Learn about the principles of differentiation and integration in physics
  • Research astrophysical flux measurements and their applications
  • Explore the implications of monochromatic flux in stellar astrophysics
USEFUL FOR

Students in astrophysics, physics educators, and anyone involved in the analysis of stellar flux measurements will benefit from this discussion.

jeebs
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hi, I am having trouble deriving an expression for converting between monochromatic flux expressed in wavelength and in frequency units.

i think that the monochromatic flux of a star is found by

F(Δf) = ΔE / ΔtΔfΔA

F(Δλ) = ΔE / ΔtΔλΔA

where
E = energy,
t = time,
Δf = frequency bandwidth,
A = area of photon collecting surface, and
Δλ = wavelength bandwidth.

i was shown how to do this question by my tutor but i can't remember how to do it, it involved differentiation or integration i think...

so can you please help, its important that i find out how to do this quickly.

thanks!

oh, and if you take the time to answer, could you please give me an explanation, as the answer itself doesn't really teach me anything, I'm more interested in how you found that answer.
 
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I think you should be posting this in the homework section.
 

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