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Publishers version - DTU Orbit

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Notation<br />

B detector bandwidth<br />

c speed of light<br />

Cn index structure constant<br />

CNR carrier-to-noise ratio<br />

CRLB Cramer Rao lower bound<br />

CW continuous wave<br />

do coherence diameter of the beam<br />

DBS Doppler beam swinging<br />

FFT fast Fourier transform<br />

Fi intermediate frequency<br />

Fs sampling frequency<br />

Ft instrumental geometrical focus distance (wave curvature radius at telescope)<br />

FWHM full width half maximum<br />

< i2 NEP ><br />

< i<br />

detector noise<br />

2 RIN ><br />

< i<br />

rin noise<br />

2 SN ><br />

I(Z)<br />

shot noise<br />

Lorentzian function<br />

IPP inter pulse period<br />

LMA large mode area<br />

LOS line of sight<br />

LO local oscillator<br />

MLE maximum likelihood estimator<br />

MO master oscillator<br />

MOPA master oscillator power amplifier<br />

NEP noise equivalent power density<br />

PLO local oscillator power<br />

Ppeak transmitted pulse peak power<br />

Pr total optical power<br />

PRF pulse repetition frequency<br />

PRFmax maximum pulse repetition frequency<br />

N number of average pulses<br />

R focus distance<br />

RWF(Z) range weighting function<br />

S detector sensitivity<br />

SNR signal to noise ratio<br />

Tatm atmospheric round trip transmission<br />

Tinst instrumental round trip transmission<br />

u north-south wind speed component<br />

v east-west wind speed component<br />

VAD velocity azimuth display<br />

Vd(Z) velocity measurement at one point<br />

Vri LOS velocities, i = N North, i = E East, i = S South, i = W West and i = Z Zenith<br />

w vertical wind speed component<br />

Z height<br />

Zmax maximum height to be measured<br />

Zo distance where I(Z) is maximum, i.e. signal to noise is maximum<br />

Zr Rayleigh distance<br />

β backscattering atmospheric coefficient<br />

∆Z half of FWHM geometric depth of focus<br />

ηfoc focusing efficiency<br />

ηhet heterodyne efficiency<br />

θ lidar cone angle<br />

λ laser wavelength<br />

ν optical frequency<br />

σ efficient telescope aperture radius<br />

σv global velocity resolution<br />

σvcrlb Cramer Rao lower bound of velocity resolution<br />

σvsat smallest value of the velocity resolution<br />

τ pulse duration<br />

τc finite correlation time<br />

τm measurement time<br />

120 <strong>DTU</strong> Wind Energy-E-Report-0029(EN)

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