Understanding Spectral Index: A Plain Explanation

  • Thread starter Thread starter Sanjay87
  • Start date Start date
  • Tags Tags
    Explanation Index
Click For Summary
Spectral index is a measure used in radio astronomy to describe how the brightness of synchrotron sources changes with frequency. It is represented by the equation S ∝ ν^α, where S is brightness and ν is frequency. A negative spectral index (α) indicates that the source appears fainter at higher frequencies, while a positive index means it appears brighter. Understanding spectral index is crucial for interpreting data from synchrotron sources effectively. Clear explanations of this concept help bridge the gap between complex academic texts and practical understanding.
Sanjay87
Messages
20
Reaction score
0
Hi,

Can anybody please explain to me (in everyday language) what spectral index is? The wikipedia entry doesn't shed much light, and a lot of the textbooks give very convoluted explanations for its derivation.

Thanks.
 
Astronomy news on Phys.org
In radio terms (in my experience), spectral index applies to synchrotron sources which have brightness, S, which changes with for different frequencies, \nu, such that S \propto \nu^{\alpha}. For a negative \alpha this means that when a synchrotron source is observed at higher frequencies, it will be fainter. The opposite is true for positive \alpha.
 
Last edited:

Similar threads

  • · Replies 1 ·
Replies
1
Views
5K
  • · Replies 8 ·
Replies
8
Views
5K
  • · Replies 72 ·
3
Replies
72
Views
7K
  • · Replies 2 ·
Replies
2
Views
2K
  • · Replies 1 ·
Replies
1
Views
1K
  • · Replies 2 ·
Replies
2
Views
1K
  • · Replies 4 ·
Replies
4
Views
2K
  • · Replies 5 ·
Replies
5
Views
2K
  • · Replies 16 ·
Replies
16
Views
4K
  • · Replies 2 ·
Replies
2
Views
4K