Difference between revisions of "Radiative Processes"

From PGSC Wiki
Jump to: navigation, search
 
(6 intermediate revisions by 3 users not shown)
Line 1: Line 1:
Questions in this categoryhave been asked by HB
+
Questions in this category have been asked by HB, PJ, JW
  
 
*What are synchrotron, bremsstralung, and cyclotron radiation?
 
*What are synchrotron, bremsstralung, and cyclotron radiation?
 +
 
*What are the major absorption and scattering processes?  
 
*What are the major absorption and scattering processes?  
 
**Sketch each process and its spectrum.
 
**Sketch each process and its spectrum.
 +
 
*What is blackbody radiation?
 
*What is blackbody radiation?
* What is the typical timescale for Synchrotron cooling?
+
 
 +
*What is the typical timescale for Synchrotron cooling?
 +
 
 +
*For hot plasma emitting X-ray, in what temperature do we observe continuous emission, in what temperature do we observe lines?
 +
 
 +
*What is the radiative mechanism for the optical emission of the Crab nebular? And what's the energy source for it?
 +
 
 +
*What's the mechanism for 21cm lines? If we detect the existence of 21cm lines, what does it tell us?
 +
 
 +
*When one looks at X-ray emission from intracluster gas, how does one determine the temperature of the gas?
 +
 
 +
*How does the break on synchrotron and bremsstrahlung radiation indicate age?
 +
 
 +
[[Astrophysics]]

Latest revision as of 17:04, 25 April 2011

Questions in this category have been asked by HB, PJ, JW

  • What are synchrotron, bremsstralung, and cyclotron radiation?
  • What are the major absorption and scattering processes?
    • Sketch each process and its spectrum.
  • What is blackbody radiation?
  • What is the typical timescale for Synchrotron cooling?
  • For hot plasma emitting X-ray, in what temperature do we observe continuous emission, in what temperature do we observe lines?
  • What is the radiative mechanism for the optical emission of the Crab nebular? And what's the energy source for it?
  • What's the mechanism for 21cm lines? If we detect the existence of 21cm lines, what does it tell us?
  • When one looks at X-ray emission from intracluster gas, how does one determine the temperature of the gas?
  • How does the break on synchrotron and bremsstrahlung radiation indicate age?

Astrophysics