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Propagation

Why a frequency gives a different result at midday than at night.

Bodenwelle
follows the earth's surface, carries far on long wave and 160 m
Raumwelle
is refracted in the ionosphere and comes back down far away
D-Schicht
lowest layer at 60 to 90 km altitude, only present by day, mainly absorbs the low bands
E-Schicht
lower layer, present by day, attenuates low frequencies
F2-Schicht
the decisive layer for long-distance contacts on HF
Sporadic E
short-lived clouds in the E layer, open up 6 m and 2 m for long distances in summer
MUF
highest usable frequency for a path
LUF
lowest usable frequency, below it absorption eats the signal
Skip-Zone
dead zone between the end of the ground wave and the first hop
Grayline
twilight line, along which contacts work particularly well
Sonnenfleckenzahl
rough measure of solar activity, a high value helps the high bands
Solarflux, A- und K-Index
indices for solar radiation and disturbances of the earth's magnetic field
Aurora
reflection off the aurora, distorts the audio heavily
Ionosonde
transmitter that sends straight up and measures the height and critical frequency of the layers from the echoes
foF2
critical frequency of the F2 layer at vertical incidence, measured by the ionosonde
MUF(3000)
MUF for a 3000 km hop, roughly three times foF2
hmF2
height of the densest part of the F2 layer, usually 250 to 400 km; the higher it is, the longer the hop
Sprungweite
distance after which a ray reaches the ground again after one reflection; via the F2 layer at most about 4000 km
Abstrahlwinkel
angle above the horizon at which an antenna radiates; low angles hop far, steep ones short
Sekantengesetz
at oblique incidence a ray still turns back at a higher frequency than at vertical incidence: f = foF2 / cos of the angle of incidence
foEs
critical frequency of a sporadic E cloud at vertical incidence; from about 10 MHz 6 m opens over about 2000 km
Kp-Index
disturbance of the earth's magnetic field per three hours, averaged worldwide, 0 to 9; from 5 it counts as a storm
Bz
north-south component of the magnetic field in the solar wind; if it points south (negative) for a long time, it couples to the earth's magnetic field and things get unsettled
Sonnenwind
stream of charged particles from the sun, normally around 400 km/s; fast and dense it disturbs the earth's magnetic field
Flare-Klasse
strength of a solar X-ray flare: A, B, C, M, X, each letter ten times stronger; from M upwards HF drops out briefly on the daylight side
D-RAP
NOAA map showing up to which frequency the D layer currently absorbs 1 dB
Tropo
extended range on VHF/UHF due to temperature inversions

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Q codes Abbreviations in telegraphy RST report Phonetic alphabet Callsigns in Germany Law and administration Regulation and radio policy DARC, DOK and awards Portable programmes Repeater operation Modes Propagation Shack technology

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