Click Here to
Order this information in Print

Click Here to
Order this information on CD-ROM

Click Here to
Download this information in PDF Format

 

Click here to make tpub.com your Home Page

Page Title: Figure 1-1 Atmospheric Layers
Back | Up | Next

Click here for a printable version

Google


Web
www.tpub.com

Home


   
Information Categories
.... Administration
Advancement
Aerographer
Automotive
Aviation
Combat
Construction
Diving
Draftsman
Engineering
Electronics
Food and Cooking
Math
Medical
Music
Nuclear Fundamentals
Photography
Religion
USMC
   
Products
  Educational CD-ROM's
Printed Manuals
Downloadable Books

   
Back
Chapter 1 Wave Propagation
Up
Electronics Technician Volume 07-Antennas and Wave Propagation
Next
Ionospheric Layers

Figure 1.1—Atmospheric layers. since they have the greatest effect on your job. Daily of  the  ultraviolet  energy  that  initially  set  them  free variations  in  the  ionosphere  produce  four  cloud-like layers  of  electrically-charged  gas  atoms  called  ions, which   enable   radio   waves   to   be   propagated   great distances  around  the  earth.  Ions  are  formed  by  a process  called  ionization. Ionization In  ionization,  high-energy  ultraviolet  light  waves from the sun periodically enter the ionosphere, strike neutral  gas  atoms,  and  knock  one  or  more  electrons free from each atom. When the electrons are knocked free,  the  atoms  become  positively  charged  (positive ions) and remain in space, along with the negatively- charged free electrons. The free electrons absorb some and  form  an  ionized  layer. Since the atmosphere is bombarded by ultraviolet waves  of  differing  frequencies,  several  ionized  layers are  formed  at  different  altitudes.  Ultraviolet  waves of   higher   frequencies   penetrate   the   most,   so   they produce  ionized  layers  in  the  lower  portion  of  the ionosphere.   Conversely,   ultraviolet   waves   of   lower frequencies  penetrate  the  least,  so  they  form  layers in  the  upper  regions  of  the  ionosphere. An  important  factor  in  determining  the  density of  these  ionized  layers  is  the  elevation  angle  of  the sun.  Since  this  angle  changes  frequently,  the  height and  thickness  of  the  ionized  layers  vary,  depending 1-2

Privacy Statement - Press Release - Copyright Information. - Contact Us - Support Integrated Publishing