Home
Purchase
Support Forum
Get Our CD-ROM
News
Mac OS X Software
Mac OS 9 Software
Windows Software
Ham Radio iPhone/iPad
Linux Software
Documentation
Support/FAQ
Update Policy
Lost Reg Code?

Radiation Detectors
USB Icom CI-V Interface
MIL-STD-188 Interface

General Interest Programs
  Atomic Mac/PC
  Audiocorder
  Audio Toolbox
  Black Cat Timer
  Diet Sleuth
  iUnit
  Graffikon
  Graph Paper Maker
  Health Tracker
  Knitting Wizard
  Label Wizard
  Prog Audio Gen
  Sound Byte

Amateur Radio Programs
  Audiocorder
  Black Cat CW Keyer
  DX Toolbox
  Elmer
  iDXCluster
  MatchMaker
  MININEC Pro
  Morse Mania
  MultiMode
  RF Toolbox

iPhone Programs
  Atoms To Go
  dB Calc
  Drill Calc
  Elmer Extra
  Elmer General
  Elmer Tech
  Field Strength Calc
  iAttenuate
  iFunctionGenerator
  iSoundex
  iSoundByte
  iSweep
  iUnit
  Photon Calc
  RF Link Calc
  Transmission Line Calc
  Weather Calc
  Wire Calc

About Black Cat Systems
Geiger Counter
Site Map
Our software for Mac OSX
Privacy Policy
Press/Media
HFunderground
Apple /// Emulator

Macintosh Links
Shortwave Radio
Pirate Radio
Spy Numbers Stations
Science and Electronics
Ham Radio Software
Geiger Counters

HF Shortwave Radio Propagation Information - Solar Flares

Sometimes, especially during periods of high solar activity, the magnetic lines in the Sun can become so twisted that they eventually release a large amount of energy in the form of a solar flare. These flares produce a large amount of x-ray radiation. This radiation can strongly ionize the D layer in a short amount of time, a minute or less, resulting in a large amount of attenuation of radio waves passing through the affected region (that is, the side of the Earth facing the Sun). Large flares can cause ionization levels sufficient to completely stop all shortwave propagation, causing the infamous "HF Blackouts".

Several satellites in orbit around the Earth continuously monitor the x-ray levels from the Sun, and can detect solar flares as they occur.

Solar flares are categorized according to their strength, using letters and numbers. The letters range are A,B,C,M and X, and a number follows the letter, such as C4.5 or M8.2, etc. A flares are the weakest, and X flares the strongest. There is no upper limit. The strongest flare ever recorded was an X28, in November of 2003. It was possibly higher, some think as high as X40, but the sensors used to measure flares cannot go that high.

DX Toolbox gives you the current solar x-ray conditions, as well as graphs showing the past several days readings, and alerts you to solar flares immediately when they occur.

In addition to major solar flares, there is a constant background of x-ray radiation from the Sun. In general, the lower this background level, the better radio propagation conditions are.

Large solar flares can also eject bursts of charged particles, called Coronal Mass Ejections. These CMEs can strike the Earth if the flare occurs on a region of the Sun facing the Earth. If so, they can disrupt the Earth's magnetic fields, causing auroras (northern and southern lights) which can affect shortwave radio propagation. They can also cause generally higher noise levels, and weaker signals.

[Table of Contents]
Previous [Solar Flux]
Next [A Index and K Index]