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Radars and Meteorology

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Title: Radars and Meteorology


1
  • Radars and Meteorology
  • Shri S.H. Damle
  • Indian Institute of Tropical Meteorology
  • Pune

2
Radar Meteorology
  • Historical Back Ground
  • Basic concept of Radar
  • Nikola Tesla 1900
  • Article in Century Magazine

3
  • Some british German Patents on Detection
    Ranging of Remote metallic objects by Radio Waves
    1900-1906
  • First practical Demonstration of Ranging using
    FM-CW transmitter.
  • Dec 1924
  • Appleton Kings College London
  • Barnet - Cambridge University

4
  • They observed the reflections from ionospheric
    layers beyond 100 km The Appleton Layer
  • Use of Pulsed Techniques
  • Breit Tuve Carneigy Institute 1925, with NRL
    collaborations.
  • Again Inospheric Echoes 150 km away.

5
  • Work in another direction was being perused by a
    young engineer turned Meteorologist (Sir) Watson.
    Watt 1915
  • Study of e-m radiation by lightening in
    thunderstorms
  • Objective Timely thunderstorm warnings to world
    War I aviations.

6
  • 1935 World War II scenario
  • British govt. committee on scientific survey of
    Air Defence (CSSAD)
  • Consultations with sir Watson Watt Wilkins
  • Proposal firmed up 27 Feb 1935
  • Successful Demonstration of detection ranging
    of aircraft July 1935.

7
  • This early war time effort firmly established
    that RADAR was a tool of Aviation.
  • Since it evolved through the effort of
    meteorologists meteorology was clubbed as part of
    civil Aviation. Even in India as in many other
    countries Dept. of meteorology was a part of Dept
    of civil Aviation

8
  • 1940 Dr. J.W. Ryde work on a 10 cm Radar Most
    probably related to precipitation detection but
    no direct record of the period wartime secrecy.
  • 1946 Rydes publication on estimation of
    attenuation and echoing properties of clouds
    rain.
  • Thus 1940-46 may be marked as the Birth of Radar
    Meteorology.

9
  • Early Radars deployed in RADAR Meteorology
  • S C Band 2700 MHz / 5600 MHz
  • Most of these were pulsed incoherent Radars the
    Tx source being high power Magnetrons
  • These were suitable for receiving echoes form
    precipitation/detecting, cyclonic/severe weather
    system mostly Intensify/reflectivity estimations.

10
  • Quantitative Estimation of wind fields could only
    be done by scan to scan tracking
  • Reflectivity Mapping DVIP
  • The advent of Klystron Technology then led to
    development of Doppler weather Radars which could
    directly measure the average wind speeds in the
    cyclonic systems
  • The advances in digital/computational Technology
    then gave further impetus to these Radar system
    developments.

11
  • The Polarization diversity Radar An effort to
    improve precipitation measurements by weather
    Radars
  • Hydrometeors/Raindrops tend to elongated as
    they fall from height.
  • The scattering x-sections in the two
    polarizations is therefore different.
  • The differential reflectivity in the two
    polarizations give a better handle on rain rate
    estimation.
  • Typical dual polarization radar requires
    polarization switching n a pulse to pulse basis
    requiring advanced high power switching
    technology.

12
The Clear air Radar Wind profiler
  • Gradients in refractive index fluctuations
    leading to e-m back scatter
  • The average wind carries along these
    irregularities and in turn they become tracers of
    mean wind.
  • A Radar operating at wavelength ? is most
    sensitive to scale sizes of these irregularities
    of ?/2 or multiples of ?/2.

13
  • The atmospheric Radar Eqn volume Target Eqn
    The signal power

14
  • Note
  • Dependence on 1/R2
  • Proportional to Ae PT power Aperture product
  • Proportional to - The Radar pulse length
  • ? volume Reflectivity of atmospheric Target

15
The Noise Power
  • In Practice
  • One integrates nc pulses assuming the signal
    remain coherent during the period - typically
    upto few seconds in troposphere.
  • Invariably use spectral processing to detect the
    signal and use DFFT techniques with P points DFT
  • Integrate certain number (ni) of spectra
    incoherently the delectability is then defined
    as (S/N)dt

16
Coding Decoding
  • Coding offers dual advantages
  • Good/High resolution
  • High average power
  • A long single pulse made up of segment of pulses
  • Binary phase coding is one convenient form of
    coding technique which is suitable for digital
    implementation

17
  • The carrier phase is altered either as 0o or 180o
    according to a binary code
  • Complementary code sequences are popular in
    profiler applications
  • If A B are two complementary codes then they
    possess the property that the range side lobes of
    autocorrelation function of A are in opposite
    sign to the autocorrelation function of B.

18
  • Thus if the complementary sequences A B are
    transmitted one after the other and on receive
    side their autocorrelation functions are added
    the range side lobes disappear in the receiver
    output leaving in the receiver output a single
    peak at signal location.

19
  • Once we know A B are complementary codes, then
  • are also complementary.
  • Examples A AB -
  • B - AB -
  • Use of m baud complementary code pair sequence,
    subsequent decoding addition on receive side
    thus provides a (S/N) improvement by a factor m.

20
  • This is because all the target returned energy
    which was distributed in range side lobes is
    recovered this is as if Transmit power is
    increased m times compared to a single pulse
    (code) transmission.
  • In the Pune profiler a 8 baud code pair sequence
    (baud length 2 microsecond) is used in the higher
    height mode of operation. The code pair is -
    -
  • - ---
  • which can be generated from the basic pair
    -

21
Receiver system Hardware consideration
  • Since Cn2 in atmosphere could vary by more than
    70 dB ( 7 orders of magnitude) a high dynamic
    range receiver is required.
  • The signal dynamic range is to be achieved
    without saturation of any stage because of
    background noise.
  • RF video gain is to be adjusted such that the
    lowest expected signal level at Rx input is
    amplified upto atleast one bit level of the
    ADC.
  • This will ensure full utilization of the DSPG

22
I-Q Imbalance
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24
The basic vector wind computation
  • Vradial(east) ucos? wsin?
  • Vradial (north) vcos? wsin?
  • W (zenith) w
  • U V being Zonal and Meridional component of the
    wind.
  • W Zenith beam estimate of vertical velocity.

25
Quality controls on data
  • Range tracking temporal continuity
  • consensus averaging
  • Need to know beam position angle ? accurately.
  • If ugtgtw
  • Vre ucos? therefore
  • Thus for 1 accuracy of radial wind
  • Is approximately .170 for ?750

26
Similar systems abroad
  • NOAA Network at 449 MHz Typical specs
    identical with Pune profiler-Summary performance

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32
  • Thank You
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