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ICU2005 2005/09/06, Zurich, Switzerland Ultra Wideband Double-Directional Channel Measurements in an Office Environment 1 Jun-ichi Takada 2 Fumio Ohkubo 1 Katsuyuki Haneda Takehiko Kobayashi 3 1, 3: UWB Technology Institute, National


  1. ICU2005 2005/09/06, Zurich, Switzerland Ultra Wideband Double-Directional Channel Measurements in an Office Environment 1 Jun-ichi Takada 2 Fumio Ohkubo 1 Katsuyuki Haneda Takehiko Kobayashi 3 1, 3: UWB Technology Institute, National Institute 1: Tokyo Institute of Technology of Information and Communication Technology 3: Tokyo Denki University 2: NTT Advanced Technology Corporation

  2. Overview of our activities • Channel modeling based on measured data

  3. Table of contents • Background • UWB double-directional measurement – Concept – Double-directional measurement procedure – Parameterization of double-directional channels • Experiment in a meeting room • Experiment in an office • Observation of the results • Summary and future works • Acknowledgement

  4. Background • Impact of double-directional channel sounding activities with UWB signal 1. For UWB systems: – Improvement of the current UWB channel models – Focus is to include spatial channel information 2. For MIMO transmission: – Detailed investigation of the relation between MIMO capacity and physical phenomena – Possibility to cover wide frequency range Final goal: Antenna-independent channel models which are applicable both for UWB and MIMO systems with all operating frequencies

  5. Double-directional channel • Estimating both DOD and DOA enables us to separate antenna effects from channel model (M. Steinbauer et., al, 2001) DOD DOA Tx Rx Propagation Antenna + Propagation = Channel

  6. UWB double-directional measurements • Measurement strategy – MISO/SIMO configurations = double directional meas. SIMO MISO Tx Rx Tx Rx DOA / DTOA estimation DOD / DTOA estimation Connecting DOA and DOD information using DTOA

  7. UWB channel sounding system • Vector Network Analyzer & spatial scanner Synthetic UWB array antenna • 3-D (x-y-z) scanner and UWB antenna Preamp (30dB) • Omni-directional VNA monopole antenna • flat group delay GPIB characteristics PC • frequency • Data acquisition sweeping from • Measurement control 3.1 to 10.6 GHz via GPIB

  8. Specifications of experiment • Arrays × × – Spatial sampling: points in directions 10 10 7 xyz – Element spacing: 48 mm – Frequency range: 3.1 to 10.6 GHz Achieved 10 deg resolution of DOD / DOA azimuth angle, and 0.13 ns resolution of DTOA • Others – DOD / DOA / DTOA estimation algorithm: SAGE – Polarization: vertical-vertical – SNR at the receiver: at least 20 dB – Calibration: function of the VNA and back-to-back (antenna calibration)

  9. Experiment in a meeting room Ceiling: plaster board Tx (2.0 m high) Tx1 Tx2 20 cm Side wall: metal Rx (1.0 m high) Tx-Rx distance: 4.6m

  10. Experiment in a meeting room • The 10 strongest waves # 1 , # 2 , revealed that R x 1 # 5 , # 6 , # 9 1. Many reflected paths from # 1 0 the ceiling were detected 2. Multi-reflected waves were detected due to metal # 3 # 4 side walls 3. Path constitution was # 8 symmetric w.r.t. Tx-Rx line Metal ceiling 天井裏 T x 1 Plaster board # 1 , # 2 # 9 # 7 # 5 , # 6 # 1 T x 1 R x 1 長机 Desk

  11. Experiment in a meeting room • Reflection from ceiling – Many metal pipes inside the plaster board – Metal parts of room lights Metal ceiling 天井裏 Plaster board # 1 , # 2 # 9 # 5 , # 6 # 1 T x 1 R x 1 長机 Desk

  12. Experiment in an office Plaster board Tx (2.0 m high) Rx (1.0 m high) LOS is assured Tx-Rx distance: 7.5m

  13. Experiment in an office W i n d o w • Detected waves revealed that R x 2 1. Reflections from office desks, equipment and # 4 floor are few 2. Reflections from # 2 windows and far wall # 1 , # 3 , are few # 8 , # 9 3. The 10 strongest waves are first-order T x 2 reflections on metal # 5 , # 7 furniture or direct path # 6 # 1 0

  14. Observations of the results • Initial findings from the experiment 1. Reflection occurs on metal wall, furniture, and pipes inside the ceiling 2. Reflection from ceiling is much stronger than those from the floor 3. Reflections from windows are few 4. Office environment reveals complicated propagation phenomena than residential environment due to metal structures of buildings 5. Specular reflection contains stronger power than non- specular scattering 6. Higher-order specular reflection still have strong power in the meeting room due to metal walls

  15. Summary and future works • UWB double-directional channel sounding in the meeting room and office – Channel sounding procedure – Initial findings from measurements • Future works 1. Quantitative analyses of channel behavior • Cluster analyses • Reflection coefficients 2. Channel modeling based on the results 3. Modeling of the residual components 4. Improvement of the SAGE algorithm • To avoid spurious paths, search strategy and reduction of sidelobes should be considered.

  16. Acknowledgement • The authors would like to thank the members of NICT UWB Consortium and UWB Technology Institute in NICT: – Prof. Dr. Kiyomichi – Dr. Makoto Yoshikawa Araki – Dr. Akira Akeyama – Mr. Iwao Nishiyama – Dr. Osamu Sasaki – Dr. Honggang Zhang – Dr. Yuko Rikuta – Mr. Naoto Takahashi – Mr. Takahiro Miyamoto

  17. Specifications of experiment • Signal processing of measured data – SAGE (Space-Alternating Generalized Expectation- Maximization) algorithm – Derivation of DOD, / DOA, DTOA and frequency spectrum of each path Measured data What we want Fourier pair • DOD Spatial transfer • DOA function • DTOA distributions SAGE • Frequency spectrum Features of the SAGE • Maximum-likelihood based estimation (parametric channel estimation) • Widely used in conventional wideband channel sounding, and we modified it to to UWB signals

  18. Observations of the results • Problems 1. There are many weak paths that cannot be identified in the real environment 2. Even the 10 strongest waves, they contain only 20 to 30 % of total received power In the meeting room -100 -95 -100 Before extracting After extracting -90 -95 -85 100 waves 100 waves -90 -80 -85 70 70 60 60 50 50 40 40 30 30 20 20 10 10 0 0 0 45 90 135 180 225 270 315 360 0 45 90 135 180 225 270 315 360 Azimuth angle [deg] Azimuth angle [deg]

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