STLP 9128 E special - 80-1700 MHz Stacked Log Periodic Antenna
PRD Precision Reference Dipole 30 - 1000 MHz
PCD 3100 Precision Conical Dipole 30 MHz - 1 GHz
STLP 9128 E - 80-1500 MHz Stacked Log Periodic Antenna
AM 9144 - Modular Antenna Mast
VHBD 9134-4 + Elements, 20 - 200 MHz, 4kW High-Power Biconical Antenna
VHBA 9123 + Elements, 20 - 300 MHz, 100 W, Rx Biconical Antenna
VHA 9103B + Elements, 20 - 600 MHz, 10W, Rx Biconical Antenna
BCOI 9180, Booster Coils for High Power Baluns
HFBA 9122 + Elements, 0.1 - 500 MHz, 10 W, Rx Biconical Antenna
SY3-EMC, 30 - 200 MHz, 2500 Watts, Tuned Yagi
Products
BBHA 9120 C - 2-18 GHz Double Ridged Horn Antenna
The broadband horn antenna BBHA 9120 C is a linear polarized double ridged horn antenna.
- 2 GHz to 18 (20) GHz
- SMA - female
STLP 9128 E special - 80-1700 MHz Stacked Log Periodic Antenna
The STLP 9128 E special is nearly identical like the STLP 9120 E but with folded longest elements and smaller structure angle.
- 80 - 1700(2700) MHz
- Type N (female) or Type 7/16 (female)
PRD Precision Reference Dipole 30 - 1000 MHz
Highly accurate reference for antenna calibrations, site validations, and EMC conformance tests according to ANSI C63.4, ANSI C63.5, CISPR 16-1, CISPR/A/244/FDIS Uncertainty in the antenna factors: less than 0.15 dB (95.5%) at the resonance frequency
PCD 3100 Precision Conical Dipole 30 MHz - 1 GHz
Highly Accurate Reference Antenna for Site validation measurements according to CISPR 16-1-4 in fully anechoic rooms
STLP 9128 E - 80-1500 MHz Stacked Log Periodic Antenna
STLP 9128 E - Stacked Log Periodic Antenna
- (65)80-1500(3000) MHz
- Type 7/16 female
Type N female
AM 9144 - Modular Antenna Mast
The double telescopic antenna mast/tripod is continuously height-adjustable. The mast rods are made of glass fiber to avoid unwanted reflexions. The modular design makes it possible to use different telescope parts and it can be mounted on a mast foot made of stainless steel or one made out of low-reflective fiberglass. Both of them provide a secure stand and easy adjustment on uneven ground. Antennas or adapters can be mounted on the 3/8" male thread.
VHBD 9134-4 + Elements, 20 - 200 MHz, 4kW High-Power Biconical Antenna
- VHBD 9134-4 antenna holder/balun in combination with required elements:
- Biconical Elements: BBLA 9136
- Open-Cone Elements: BBFA 9146, FBAL 9178, BBAE 9179
- high power antenna holder/balun
- 50:200 Ohm
- 20-200 MHz, 4 kW, 7/16-female connector
VHBA 9123 + Elements, 20 - 300 MHz, 100 W, Rx Biconical Antenna
- VHBB 9123 antenna holder/balun in combination with required elements:
- Biconical Elements: BBA 9106, BBLA 9136, BBAK 9137, BBVK 9138
- Open-Cone Elements: FBAB 9177, FBAL 9178, BBFA 9146
- Better antenna factor below 50 MHz, also EMV application 100 W
- 50:200 Ohm
- 20-300 MHz(dependent on elements), 100 W, Type N (f)
VHA 9103B + Elements, 20 - 600 MHz, 10W, Rx Biconical Antenna
- VHA 9103B antenna holder/balun in combination with required elements:
- Biconical Elements: BBA 9106, BBLA 9136, BBAK 9137, BBVK 9138
- Open-Cone Elements: FBAB 9177, FBAL 9178, BBFA 9146
- Especially to measure very high field strength
- 1:1 Balun
- 20-600 MHz(dependent on elements), 10 W, Type N (f)
BCOI 9180, Booster Coils for High Power Baluns
- Booster coils for varying the element loading of high power biconical
- Allows for better matching in low-frequency testing
- Helps compensate for chamber loading
HFBA 9122 + Elements, 0.1 - 500 MHz, 10 W, Rx Biconical Antenna
- HFBA 9122 antenna holder/balun in combination with required elements:
- Biconical Elements: BBA 9106, BBLA 9136, BBAK 9137, BBVK 9138
- Open-Cone Elements: FBAB 9177, FBAL 9178
- Especially to measure very high field strength
- 1:1 Balun
- 0.1-500 MHz(dependent on elements), 10 W, Type N (f)
SY3-EMC, 30 - 200 MHz, 2500 Watts, Tuned Yagi
The SteppIR SY3-EMC Auto-tuned Yagi system is the solution to MIL-STD-461G and RS-103 for radiated susceptibility testing over the 30-200 MHz frequency range – making it the only system in the world that can legitimately claim to reach or exceed the required 200 V/m @1 Meter, at the fundamental frequency.
