Mastering Optical Depth: Simplifying the Concept for Beginners

  • Context: High School 
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Discussion Overview

The discussion centers around the concept of optical depth, particularly in the context of its definition, applications, and relevance in astronomy. Participants express varying levels of understanding and seek simpler explanations suitable for beginners.

Discussion Character

  • Exploratory
  • Conceptual clarification
  • Debate/contested
  • Homework-related

Main Points Raised

  • One participant expresses difficulty understanding optical depth and requests simpler explanations.
  • Another participant provides a link to a comprehensive document on radiative transfer in stellar atmospheres, suggesting it contains relevant information.
  • A different participant questions the necessity of the lengthy document, indicating a preference for simpler, high school-level resources.
  • Several participants suggest alternative resources, including a Wikipedia page on optical depth, while encouraging the original poster to specify their questions.
  • One participant defines optical depth as a measure of opacity along a path to radiation, noting its importance in determining the amounts of atoms or molecules in gases.
  • Another participant explains the relationship between optical depth and the probability of a photon escaping a medium, introducing the mathematical expression e^(-tau).

Areas of Agreement / Disagreement

Participants do not reach a consensus on the best resources for understanding optical depth, with some advocating for more complex materials while others seek simpler explanations. The discussion remains unresolved regarding the optimal approach to learning about the topic.

Contextual Notes

Some participants highlight the need for clearer questions to provide better assistance, indicating that the original poster's vague inquiries may hinder effective communication. There is also an acknowledgment of varying levels of English proficiency among participants, which may affect comprehension.

O-r-i-o-n
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Hi Everyone!
I was wondering if someone could help me with Optical Depth, I read some articles about it but since my English isn't that good I couldn't Get it well! I have some views about the Opacity But when it comes to optical depth I'll get lost :D
help!
 
Astronomy news on Phys.org
This contains everything you need basically;)

"RADIATIVE TRANSFER
IN
STELLAR ATMOSPHERES"

http://www.astro.uu.nl/~rutten/rrweb/rjr-material/masters/rtsa/afy.pdf


It is better with precisie questions, how are we supposed to help you if we don't know what you are struggeling with? And if your english is not that good, improve it, "everything" is written in english.
 
275 pages? what would you have sent me if I had said my English is good? :D
Thanks man but I needed sth simpler , sthh in high school level (or a little higher)
 
Already read that one , but thanks! I got somethings from that!
 
I don't have a specific question about Optical Depth , I just want to know what it is and what are it's uses and why astronomers use it. and about the 275 pages , really? because the number freaked me out so I didn't go to the details :D , thanks I'll check it out
 
its not only about optical depth, it is about radiative transfer. Why didnt you read the table of contents? First part of chapter 2 introduces optical depth etc.
 
It's basically just a measure of how opaque a given path is to radiation. Optical depth is proportional to the number of (light-absorbing) particles along a given line of sight, so it's a very useful quantity in astronomy when it comes to working out the amounts of atoms or molecules in different gases you're looking through.
 
  • #10
The optical depth related to the probability of escape of a photon traveling trough a medium. The probability for a photon to escape is e^(-tau), where tau is the optical depth (and is a function of wavelength or frequency).
 
  • #11
Thank you all! Got what I needed!
 

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