Graphics: Auroral Activity | Solar
X-Ray Flux | Sunspots | SOHO
| D-Region Asorbtion | MUF | Solar
X-Ray Absorption | E-Layer

| SOLAR FLUX INDEX (SFI)
While increasing SFI may be good for HF propagation, it also tends to correspond with high Ap and K indices, which cause D-Layer absorption and noisy band condition.
|
||||||||||||||||||||||||
|
PLANETARY Ap INDEX The subscript "p" means planetary and designates a global magnetic activity index. The following 13 observatories, which lie between 46 and 63 degrees north and south geomagnetic latitude, now contribute to the planetary indices: Lerwick (UK), Eskdalemuir (UK), Hartland (UK), Ottawa (Canada), Fredericksburg (USA), Meannook (Canada), Sitka (USA), Eyrewell (New Zealand), Canberra (Australia), Lovo (Sweden), Brorfelde (Denmark), Wingst (Germany), and Niemegk (Germany).
|
||||||||||||||||||||||||
|
THREE-HOUR-RANGE INDEX K K indices isolate solar particle effects on the earth's magnetic field; over a 3-hour period, they classify into disturbance levels the range of variation of the more unsettled horizontal field component. Each activity level relates almost logarithmically to its corresponding disturbance amplitude. Three-hour indices discriminate conservatively between true magnetic field perturbations and the quiet-day variations produced by ionospheric currents. K indices range in 28 steps from 0 (quiet) to 9 (greatly disturbed) with fractional parts expressed in thirds of a unit. A K-value equal to 27, for example, means 2 and 2/3 or 3-; a K-value equal to 30 means 3 and 0/3 or 3 exactly; and a K-value equal to 33 means 3 and 1/3 or 3+. The arithmetic mean of the K values scaled at the 13 observatories listed above gives Kp.
|
||||||||||||||||||||||||
|
EQUIVALENT AMPLITUDE The a-index ranges from 0 to 400 and represents a K-value converted to a linear scale in gammas (nanoTeslas, nT) – a scale that measures equivalent disturbance amplitude of a station at which K=9 has a lower limit of 400 gammas.
|
||||||||||||||||||||||||
|
|||||
Auroral Activity (North)Click on map for NOAA
website |
Auroral Activity (South)Click on map for NOAA website |
Solar X-Ray Flux |
|||
SunspotsClick on image for NASA Sunspot
website |
SOHO Solar Images
|
D-Region AbsorptionClick on map for NOAA website
|
|||
Maximum Useable
|
20 MHz Solar X-Ray
|
E-Layer Critical
|
|||
Victor Amateur Radio Association Home Page
|
Page Maintained by Pete Greene,
N2LVI Contact: Peter Greene, N2LVI Last Updated: 18 February 2008 © 2003-2008 Victor Amateur Radio Association. All rights reserved. |