A General Review of Physics

Still under development, however changes are made regularly - check back by later.

The Electromagnetic Spectrum

CLICK HERE for a LARGER IMAGE

The electromagnetic spectrum is a continuum of all electromagnetic waves arranged according to frequency and wavelength.. They can all travel through empty space and they all travel at the same speed. This speed is sometimes called The Speed of Light. It is 300 000 000 m/s (three hundred million metres per second). The sun, earth, and other bodies radiate electromagnetic energy of varying wavelengths. Electromagnetic energy passes through space at the speed of light in the form of sinusoidal waves. The wavelength is the distance from wavecrest to wavecrest (see figure below - again, click on the image to enlarge).

CLICK HERE for a LARGER IMAGE

CLICK HERE for a LARGER IMAGE

Light is a particular type of electromagnetic radiation that can be seen and sensed by the human eye, but this energy exists at a wide range of wavelengths. The micron is the basic unit for measuring the wavelength of electomagnetic waves. The spectrum of waves is divided into sections based on wavelength. The shortest waves are gamma rays, which have wavelengths of 10e-6 microns or less. The longest waves are radio waves, which have wavelengths of many kilometers. The range of visible consists of the narrow portion of the spectrum, from 0.4 microns (blue) to 0.7 microns (red).

CLICK HERE for a LARGER IMAGE

 

Emission Line Spectra

Lyman Series

Where
l = the wavelength (in Angstroms)
R = Constant (in Parsecs)
n = 2, 3, 4, 5...

Balmer Series

Where
l = the wavelength (in Angstroms)
R = Constant (in Parsecs)
n = 3, 4, 5, 6...

   
Paschen Series

Where
l = the wavelength (in Angstroms)
R = Constant (in Parsecs)
n = 4, 5, 6, 7...

Brackett Series

Where
l = the wavelength (in Angstroms)
R = Constant (in Parsecs)
n = 5, 6, 7, 8...

   

Bohrs Postulate

Ea - Eb = hv

Ea = Electron energy in OUTER Orbit
Eb = Electron energy in INNER Orbit
h = Plancks Constant
v = Frequency of emitted radiation

Frequency of Emitted Radiation

Where:

v = Frequency
c = velocity
l = the wavelength (in Angstroms)

Transition Energy from First Orbital to the Second Orbital

Where:

l = the wavelength (in Angstroms)
h = Plancks Constant
v = Frequency of emitted radiation
c = velocity
W = number calculated from Bohrs Postulate
R = Constant (in Parsecs)

   
Transition Energy from any Orbital to the Second Orbital

Where:
l = the wavelength (in Angstroms)
R = Constant (in Parsecs)
n = 3, 4, 5, 6...

Transition Energy from any Orbital to the First Orbital

Where:
l = the wavelength (in Angstroms)
R = Constant (in Parsecs)
n = 2, 3, 4, 5...

   
Stefans Law

Where:

E = Rate of Energy Emission
s = Stefan-Boltzmann Constant
T = Absolute Temperature

Star Size

Dsol = Solar Diameter (in A.U)
Dd = Distance from Observer (in Parsecs)
A = Angular Diameter (in Arc Seconds)

   
Absolute Bolometric Magnitude

Total Luminosity

   
Dissociation Formula

   

  Further Research, Reading, and/or Review :  
  An EXCELLENT REVIEW of Mathematics for CCD Spectrographic Analysis

by Christian Buil

 
  Last Updated:  
     
  RETURN TO MAIN PAGE  
     
   
     
 

Click Here!