SWA16 - 4481.0 kHz
KD4IZ Hell
QSL SV1OI (1985)
Denmark-1965-0.80
RDA-100
Cambridge IM-501 tape recorder
QSL AJ6AC (1956)
VHF yagi antennas
Denmark-1979-1.60
Poland-1965-RocketMail
Sunset in Mdina
20210611 0120 7090.5 kHz KD4IZ
Great Britain-1972-RocketMail
EC-MTE @LGAV
SX-DGQ @LGAV
SX-NEA @LGAV
TC-JPA
ADR safety valve testing
Proteus-2049
SX-HPD
Minolta Mini 16 Slide Projector,
UK 1977 13p
QSL YA/SV5DZG (2002)
NOAA-Multibeam SONAR
Gibraltar 2018 20p+50p
TAAF 2021 €1.20
Greece-revenue-1909-0.50
OK0EU beacons
QSL SV8QG (2018)
QSL 9V1JA (2001)
France LaPoste-2021
20210406-0024-DRA5
QSL ZF2QS (2002)
QSL ZL2AH (2001)
Hellenic Coast Guard CoA
Decimal Day Machin stamps
HF-Fax_20210325_0932
BCM95821
QSL EIRT (1971) DL
QSL ERT (1981) 2
QSL ERT (1981) 1
URE QSL stamp 4
Sony TC-150
KSC-03PD-3300
Black Arrow (model)
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Calibration-Horn-1967


The Calibration Horn Antenna, nicknamed the “Little Big Horn,” at Green Bank in 1967. As its name implies, this 120-foot long horn antenna was used to measure the intensity of radio waves coming from the sky’s strongest non-solar radio source, Cassiopeia A. The Calibration Horn measured a total power output for Cas A at a frequency of 1.4 GHz (a wavelength of 20cm), and thus provided astronomers with a standard reference point on the sky against which they could measure other sources.
Credit: NRAO/AUI/NSF
Source: public.nrao.edu/gallery/little-big-horn
Credit: NRAO/AUI/NSF
Source: public.nrao.edu/gallery/little-big-horn
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