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Byron Alderman
Also published under:B. Alderman, Byron E. J. Alderman, B. E. J. Alderman
Affiliation
RAL Space, STFC Rutherford Appleton Laboratory, Oxfordshire, UK
Topic
Schottky Diode,Conversion Efficiency,Frequency Multiplier,Input Power,Output Power,Output Waveguide,Second Harmonic Generation,Advanced Design System,Computer Numerical Control,Computer Numerical Control Machine,Conversion Loss,Coplanar Waveguide,End Wall,Independent Performance,Input Waveguide,Local Oscillator,Local Oscillator Signal,Low Power,Maximum Output Power,Maximum Power,Metal Frame,Noise Temperature,Nominal Length,Optical System,Photocurrent,Polymer Parts,Printing Process,Printing Technology,Short-circuit,Terahertz,Thin Layer Of Gold,Waveguide Cavity,Waveguide Length,Waveguide Structure,Wide Range Of Applications,Wireless,mW Power,Waveguide,Harmonic Balance,Quartz Substrate,Varactor,Dipole Antenna,High Frequency Structure Simulator,Noise Figure,Power Amplifier,Power Meter,Impedance Matching,Microstrip,Return Loss,Antiparallel Diode,
Biography
Byron Alderman received the M.Phys. degree in physics from the
University of Warwick, Coventry, U.K., in 1998, and the Ph.D. degree from The University of Leeds, Leeds, U.K., in
2001.
Following graduation he joined the Millimetre Wave Technology Group, Rutherford Appleton Laboratory, Oxfordshire, U.K. He founded Teratech Components, in Oxfordshire, U.K., in 2010, where he is currently the CEO and a Principal Scientist with the Rutherford Appleton Laboratory. His research interests are in the field of room temperature heterodyne receiver technology for applications in remote sensing and astronomy at millimeter and submillimeter wavelengths.
Following graduation he joined the Millimetre Wave Technology Group, Rutherford Appleton Laboratory, Oxfordshire, U.K. He founded Teratech Components, in Oxfordshire, U.K., in 2010, where he is currently the CEO and a Principal Scientist with the Rutherford Appleton Laboratory. His research interests are in the field of room temperature heterodyne receiver technology for applications in remote sensing and astronomy at millimeter and submillimeter wavelengths.