Baird B4-6x6 Non-Penetrating Roof Mount (NPRM)
The Baird B4-6x6 NPRM is anon-penetrating roof mount used for flat roof type installations for satellite antenna's up to and including 1.2M. The B4 is one of the most robust antenna mounts available in the industry and can be quickly assembled on the roof by one person. It provides a stable base platform and level pole for securely mounting your antenna that is commonly used for satellite receive only applications and two-way VSAT installations. Each mount can be configured with different mast pipe O.D. diameters and mast heights to accommodate a wide range of satellite antennas and include integrated ballast trays that accommodate standard concrete block sizes that can be used for ballast. The standard “single tray” ballast tray can be expanded into multiple trays to accommodate additional ballast weight while increasing the mount footprint to support higher wind loading requirements.
Proper mount selection for your satellite antenna is a critical step to safely securing your outdoor equipment for the long term. Baird makes the best antenna mounts and is hands down our go to mount for any satellite installation. Please call us for assistance with any Baird mount for your next installation.
-Footprint: 6.25' x 6.00' = 37.5 sq. Ft.
-Mast Diameter: 2.88" O.D.
-Finish: Hot dip galvanized
-Mfg.: Made in the USA
Satcom Staff Notes:
-Typical application: 1.2M VSAT installations
-Mount assembly hardware: included
-Installation level of difficulty: easy
-Assembly time: less than 30 minutes
-Tools required: standard socket set / box wrenches
-Other mast heights available: yes, call for options
-Other mast O.D. available: yes, call for options
-Rubber roof pads: optional, call for pricing
Installation note: Additional ballast weight for the mount and target antenna are required for proper system installation. Ballast weight recommendations are based on antenna size, type, wind loading and building roof height of installation location. Ballast calculations are available on request.