07-Radar and History Anthea
-
Upload
nick-numlk -
Category
Documents
-
view
10 -
download
0
description
Transcript of 07-Radar and History Anthea
-
MIT Haystack ObservatoryHaystack 2003-AJC 08/01/11
Haystack Radar (HY)
Haystack Auxiliary Radar (HAX)
Millstone Hill Radar (MHR)
OUTLINE
More history Index of RefractionMore basic radar
-
MIT Haystack ObservatoryHaystack 2003-AJC 08/01/11
It is frequently said that, although the atomic bomb ended World War II, it was
radar that won the war.
-
MIT Haystack ObservatoryHaystack 2003-AJC 08/01/11
MIT Radiation Laboratory The primary technical barrier to developing UHF systems was the lack of a usable source for generating high-power microwaves. In February 1940, John Randall and Harry Boot at Birmingham University in the UK built a resonant cavity magnetron. Bombing of London Sept 1940 May 1941 (The Blitz) Britain was interested in developing practical applications for airborne microwave radar, but did not have the large-scale manufacturing ability to mass produce magnetrons. In1940, Britain partnered with the US National Defense Research Committee (NDRC)
-
MIT Haystack ObservatoryHaystack 2003-AJC 08/01/11
MIT Radiation Laboratory
Over the course of five years, MIT researchers designed 50 percent of the radar used in World War II and invented over 100 different
radar systems.
Including: Airborne bombing radars Shipboard search radars Harbor and coastal defense radars Interrogate-friend-or-foe beacon systems Long-range navigation (LORAN) system Critical contributions of the Radiation Laboratory were:
the microwave early-warning (MEW) radars, which effectively nullified the V-1 threat to London, and
air-to-surface vessel (ASV) radars, which turned the tide on the U-boat threat to Allied shipping.
-
MIT Haystack ObservatoryHaystack 2003-AJC 08/01/11
Millstone
The BMEWS Prototype
Millstone Radar1957
-
MIT Haystack ObservatoryHaystack 2003-AJC 08/01/11
Millstone
The BMEWS Prototype
Millstone Radar1957
SputnikA-Scope Trace
TransmitterPulse
Echo
Range
Am
plitu
de
First in Space Surveillance
-
MIT Haystack ObservatoryHaystack 2003-AJC 08/01/11
Outline
More History Index of Refraction More Basic Radar
Appleton - Hartree
but also
-
MIT Haystack ObservatoryHaystack 2003-AJC 08/01/11
Outline
More History Index of Refraction More Basic Radar
Appleton - Hartree
but also
-
MIT Haystack ObservatoryHaystack 2003-AJC 08/01/11
Radar Range Measurement
Transmi
tted
Pulse
Reflecte
d
Pulse
Range
Target
Target range = c2
where c = speed of light = round trip time
-
MIT Haystack ObservatoryHaystack 2003-AJC 08/01/11
Phase Velocity, Group Velocity, Index of
-
MIT Haystack ObservatoryHaystack 2003-AJC 08/01/11
Phase Velocity, Group Velocity, Index of
-
MIT Haystack ObservatoryHaystack 2003-AJC 08/01/11
Illustration of Atmospheric Effects
Elevation Refraction Range Delay
-
MIT Haystack ObservatoryHaystack 2003-AJC 08/01/11
Appleton-Hartree Equation
-
MIT Haystack ObservatoryHaystack 2003-AJC 08/01/11
-
MIT Haystack ObservatoryHaystack 2003-AJC 08/01/11
Outline
More History Index of Refraction More Basic Radar
-
MIT Haystack ObservatoryHaystack 2003-AJC 08/01/11
RADARRAdio Detection And Ranging
Radar observables: Target range Target angles (azimuth & elevation) Target size (radar cross section) Target speed (Doppler) Target features (imaging)
Antenna
TransmittedPulse
TargetCross
Section
Propagation
ReflectedPulse
(echo)
-
MIT Haystack ObservatoryHaystack 2003-AJC 08/01/11
Radar Block Diagram
Transmitter
PulseCompression
Recording
Receiver
Tracking &Parameter Estimation
Console /Display
Antenna
PropagationMedium
TargetCross
Section DopplerProcessingA / D
WaveformGenerator
Detection
Signal Processor
Main Computer
-
MIT Haystack ObservatoryHaystack 2003-AJC 08/01/11
Radar Range Equation
R
Transmitted Pulse
Received Pulse
Received SignalEnergy
TransmitPower
TransmitGain
SpreadFactor
TargetRCS
SpreadFactor
ReceiveAperture
DwellTime
Target Cross Section
Antenna Aperture ATransmit Power PT
PT4A2 4R2
1 4R2
1 A
Losses
L1=
-
MIT Haystack ObservatoryHaystack 2003-AJC 08/01/11
Pulsed RadarTerminology and Concepts
Pow
er
Duty cycle =
Average power = Peak power * Duty cycle
Peak
pow
er
Time
Pulse length
Pulse repetition interval(PRI)
Pulse lengthPulse repetition interval
Pulse repetition frequency (PRF) = 1/(PRI)
Continuous wave (CW) radar: Duty cycle = 100% (always on)
TargetReturn
-
MIT Haystack ObservatoryHaystack 2003-AJC 08/01/11
Pulsed RadarTerminology and Concepts
Pow
er
Duty cycle =
Average power = Peak power * Duty cycle
Peak
pow
er
Time
Pulse length
Pulse repetition interval(PRI)
Pulse lengthPulse repetition interval
Pulse repetition frequency (PRF) = 1/(PRI)
Continuous wave (CW) radar: Duty cycle = 100% (always on)
TargetReturn
1 Mwatt
100 kWatt
10%
100 sec
1 msec
1 kHz
1 watt
-
MIT Haystack ObservatoryHaystack 2003-AJC 08/01/11
Radar Waveforms
Waves?
or Pulses?
What do radars transmit?
-
MIT Haystack ObservatoryHaystack 2003-AJC 08/01/11
Radar Waveforms
Waves?
or Pulses?
Waves, modulatedby on-off action of
pulse envelope
What do radars transmit?
-
MIT Haystack ObservatoryHaystack 2003-AJC 08/01/11
Properties of WavesRelationship Between Frequency and Wavelength
Speed of light, c c = 3x108 m/sec = 300,000,000 m/sec
Frequency (1/s) =Speed of light (m/s)Wavelength (m)
Examples: Frequency Wavelength 100 MHz 3 m 1 GHz 30 cm 3 GHz 10 cm 10 GHz 3 cm
-
MIT Haystack ObservatoryHaystack 2003-AJC 08/01/11
Properties of WavesPhase and Amplitude
Amplitude (volts)
Phase,
90 phase offset
A
Amplitude (volts)
Phase,
A
-
MIT Haystack ObservatoryHaystack 2003-AJC 08/01/11
Properties of WavesConstructive vs. Destructive Addition
Constructive(in phase)
Destructive(180 out of phase)
Partially Constructive(somewhat out of phase)
Non-coherent signals(noise)
-
MIT Haystack ObservatoryHaystack 2003-AJC 08/01/11
Polarization
x
yElectric Field
Magnetic Field
Electromagnetic Wave
-
MIT Haystack ObservatoryHaystack 2003-AJC 08/01/11
Polarization
x
yElectric Field
Magnetic Field
Electromagnetic Wave
x
y
zE
Horizontal Polarization
Electric Field
Magnetic Field
Electromagnetic Wave
x
y
z
E
Vertical Polarization
-
MIT Haystack ObservatoryHaystack 2003-AJC 08/01/11
Doppler Effect
-
MIT Haystack ObservatoryHaystack 2003-AJC 08/01/11
Doppler Shift Concept
= cf
-
MIT Haystack ObservatoryHaystack 2003-AJC 08/01/11
Doppler Shift Concept
c v
= cf
-
MIT Haystack ObservatoryHaystack 2003-AJC 08/01/11
Doppler Shift Concept
c v
= cf
c v
f = c
-
MIT Haystack ObservatoryHaystack 2003-AJC 08/01/11
Doppler Shift Concept
c v
= cf
c v
f = c
-
MIT Haystack ObservatoryHaystack 2003-AJC 08/01/11
Doppler Shift Concept
c v
= cf
c v
f = c
-
MIT Haystack ObservatoryHaystack 2003-AJC 08/01/11
Doppler Shift Concept
c v
= cf
c v
f = c
c
f = f (2v/) Dopplershift
-
MIT Haystack ObservatoryHaystack 2003-AJC 08/01/11
Resolving Doppler
Tx signal: cos(2fot)Doppler shifted: cos[2(fo+ fD)t]
Multiply by cos(2fot) -> Low pass filter -> cos(2fDt)
BUT, the sign of fD is lost (cosine is an even function)
So, instead useexp(j2fDt) = cos(2fDt) + jsin(2fDt)
Generate this signal by mixing cos and sin via two oscillators (same frequency, 90o out of phase)
Components are called I (In phase) and Q (Quadrature): Aexp(j2fDt) = I + jQ