[PPRAANet] New NOAA Solar Storm Scales
[email protected]
[email protected]
Fri, 19 Apr 2002 19:41:29 EDT
Gang,
Recently, various organizations, most notably the National Oceonographic
and Atmospheric Administration (NOAA), has adopted a "new" set of scales
to better communicate to the public the anticipated effects of solar and
geomagnetic storms. Actually, there is nothing new about these scales
at all, they have been around for years and on the NOAA websites, but have
seldom been used. As of April 1, 2002, most agencies are now using these
scales, including NOAA solar alerts and the hourly WWV solar and
geomagnetic updates.
Here is a synopsis of the new scales. The complete tables can be
found at: http://www.sec.noaa.gov/NOAAscales
GEOMAGNETIC STORMS
==================
CLASS Kp= STORM EFFECTS TO HF PROPAGATION AURORA
-------------------------------------------------------------------------
G1 Kp=5 Minor Minor noise & fading Extreme high latitudes
G2 Kp=6 Moderate Fading at higher latitudes Aurora US/VE border
G3 Kp=7 Strong Intermittent From Oregon to Illinois
G4 Kp=8 Severe Very difficult & sporadic From N. CA to AL
& poss. power grid failures
G5 Kp=9 Extreme Near or total HF blackout To S. Tex. and Florida
& poss. power grid failures
-------------------------------------------------------------------------
SOLAR(RADIO) STORMS
===================
CLASS FLARE STORM EFFECTS TO HF PROPAGATION
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R1 M1 Minor Weak degradation
R2 M5 Moderate Limited blackouts on sunlit side of Earth
R3 X1 Strong HF blackout on sunlit side; limited elsewhere
R4 X10 Severe Global HF blackout, 24 hour duration
R5 X20 Extreme Global HF blackout, 2-3 day duration
-------------------------------------------------------------------------
A few definitions:
Kp = planetary K-index of geomagnetic disturbances. The K-index is
measured every 3 hours and reported on WWV and www.sec.noaa.gov
The 24-hour average is called the A-index
Flare = the approximate size of the solar flare triggering the solar and
radio storm.
A reminder ...
When a major flare occurs, it produces a solar/radio storm immediately
and will persist from tens of minutes to 2-3 hours. Then it's over.
This is from the speed-of-light (relativistic) energy being released by
the flare event.
If the solar flare is located near the center of the sun and produces a
CME (Coronal Mass Ejection), the shockwave from the CME will most likely
hit the earth and trigger a geomagnetic storm. This shockwave travels
about 500-1200 km/sec., and takes 2-3 days to reach the earth. Thus, a
geomagnetic storm will occur 2-3 days AFTER the flare event, and this
storm will last hours to a full day in duration. This shockwave is what
also triggers aurora.
72, Paul NA5N
via w0rw