Duration of Synchrotron Radiation in a Typical Supernova Remnant - Maple Application Center
Application Center Applications Duration of Synchrotron Radiation in a Typical Supernova Remnant

Duration of Synchrotron Radiation in a Typical Supernova Remnant

Author
: Dr. Robert Roseberry
Engineering software solutions from Maplesoft
This Application runs in Maple. Don't have Maple? No problem!
 Try Maple free for 15 days!
Find an estimate for the length of time a typical supernova remnant can radiate, given its magnetic field strength.

For more information on how to do this problem, and for tables of relevant data, see www.canismajor.ca.

Application Details

Publish Date: September 25, 2017
Created In: Maple 2017
Language: English

More Like This

Calculating the Zeeman Effect
Graphing the Planck Function
Planck's law, Stefan-Boltzmann law, Wien's law
Calculating and Graphing the Bremsstrahlung Emission Over All Frequencies for the Orion Nebula
Radio-Band and B-Band Luminosity and Brightness of Galaxy NGC 5236
Synchrotron Radiation: the Crab Nebula
Radiative Pressure