Propagation Anomalies

(Propagation prediction is not an exact science - ARRL p.17-184)

 

Aurora Curtain; Northern Lights, radio auroras, solar wind interaction between earth magnetic field and Sunspots & K-index

Fading: Caused by changing ionosphere, the layer heights or passing planes

Static-crash: SIDs

Back Scatter: Reflected signals into the Skip Zone.

Forward Scatter: Ionospheric scatter - freq. Above MUF, useable

                 out to 1200mi.

          Tropospheric scatter - useable out to 500mi from Skip zone.

          Meteor Scatter- last only a few minutes.

MUF - Max Useable Freq.: The highest frequency useable.

FOT – 85% of MUF: Freq. of optimum transmitting, optimum traffic freq.

LUF – Lowest Useable Freq.

Multipath Fading: caused by receiving signal over several paths.

SID - Sudden Ionosphere Disturbances - Solar Flare UV radiation

1.     increases ionization of D layer, blocking out HF comms.

2.      Using E&F layers on side of earth facing flare, Lasts a few minutes.

Es  -  Sporadic-E Opening: Caused by winds flowing in opposite

       Direction-producing wind shears in E region. May to

       August; Dec. to Jan.28 & 50Mhz Bands; 400 to 1300mi.

 

Solar Activity: (Solar Radiation) Radiation of the ionosphere

                Layers. Cycles: Daily - 27 days - Seasonal

Sunspot: Zurich - Increase/Decrease in cycle's approx. 9 to

         13-year cycle; maximum ionization occurs at peak of

         Cycle, "higher the Sunspot Number the better the comms".

Solar Flux Index/Numbers (SFI):  60 to 70  Poor 20m & up  (14MHz)

         (2800MHz Daily 1700Z)   90 to 110 Good up to 12m (24MHz) 

                                120 to 200 Good up to 10m (28MHz)

                                200 to 260 Good to 6 meters

The SFI indications are more descriptive of daily conditions than the Sunspot number. The higher the SFI, the higher the Sunspot number, the stronger the ionosphere becomes, and thus causing a refraction of higher frequencies.

 

R-index Sunspot number (http://sec.noaa.gov/ftpdir/latest/dayind.txt)

K-index Geomagnetic Aura Solar Disturbance activity                   

A-Report is averaging of the K-index

 

K-indicies               A-indices             Range of Condition

K-index 0 to 2           A-index   0  to 8     Quiet

K-index 0 to 3           A-index   8  to 16    Unsettled

K-index  3 to 4          A-index  16 to  30    Active

K-index  4 to 5          A-index  30 to  50    Minor Storm

K-index  6 or greater    A-index  50 to 100    Major Storm

K-index  7 or greater    A-index  100&highter  Severe storm 

 

Smoothed Sunspot Number - Solar Flux Index  -  WWV Forcast, Reports

 (SSNs)  0              = (SFI) 64             MOD QU/UN

        10              =       71             MOD QU/ACTIVE   

        20              =       79             MOD QT-ACTIVE 

        60              =      111             MOD QT-Uns

        70              =      119             sa: Lo = )mo

        90              =      136             gf: Qu-um

       100              =      145             RAD Angle: 6

       110              =      155             Dist: 5854km

       120              =      164             Hops: 2

       140              =      183             MUF (90%):16.3

       160              =      183             MUF (50%):18.7

   180              =      224             MUF (100%): 22.1

   190              =      234          HIGH/QUIET-UNSET

   200              =      245          LOW-MOD/QUIET-UNSET

NOTE: SSNs = SFI (ARRL p.17-184)

 

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