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Advances in Science and Advances in Science and Techniques for Ground-Based Techniques for Ground-Based Radar Remote-Sensing of the Radar Remote-Sensing of the Earth’s Atmosphere Earth’s Atmosphere Shoichiro Fukao Fukui University of Technology, Fukui Research Institute for Sustainable Humanosphere, Kyoto University, Kyot IGARSS Vancouver, Canada July 24 -29, 2011

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Page 1: Fukao Plenary.ppt

Advances in Science and Techniques Advances in Science and Techniques for Ground-Based Radar Remote-for Ground-Based Radar Remote-

Sensing of the Earth’s AtmosphereSensing of the Earth’s Atmosphere

Shoichiro FukaoFukui University of Technology, Fukui

Research Institute for Sustainable Humanosphere, Kyoto University, Kyoto

IGARSS

Vancouver, Canada July 24 -29, 2011

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Structure of the Earth’s Atmosphere

Troposphere

Mesosphere and

Stratosphere

Thermosphere/Ionosphere

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The Principle of radar techniques

Transmitter

Receiver

Antenna

Pulse

Echo

Target

Frequency

Doppler shift

Frequency

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The latest radar techniques have continuously been applied to the Earth’s

atmosphere

Lower Atmosphere

Middle Atmosphere

Upper Atmosphere

First,meteorologists utilized radars for precipitation measurement.

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The latest radar techniques have continuously been applied to the Earth’s

atmosphere

Lower Atmosphere

Middle Atmosphere

Upper Atmosphere

Next,radar techniques were utilized by upper atmosphere physicists .

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Scatterer in the ionosphere: Free Electrons

Total cross section is comparable to that of a sphere of 1 cmφ.

Incoherent scattering or IS

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The latest radar techniques have continuously been applied to the Earth’s

atmosphere.

Lower Atmosphere

Middle Atmosphere

Upper Atmosphere

Finally,radar techniques were applied to the middle atmosphere.

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Scatterer in the Middle Atmosphere: Turbulence

Bragg scattering

Eddy size responsible for the scattering = One half the radar wavelength

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Scales of eddies of (Inertial subrange) turbulence

Troposphere

Stratosphere

Mesosphere

Ionosphere/Thermosphere

Restricting the radar wavelength for middle atmospheric observations toVHF and UHF.

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Rapid beam scanning required for accurate measurement of wind velocity

Radar antenna

Wind vector measurement :Wind velocity assumed to be uniform within the region where / the duration

while the beam is steered.

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The Middle and Upper Atmosphere radar :The MU radar

Two essential capabilities:-Beam steering on a pulse-to-pulse basis, and- Multiple beam forming

● Several hundred modules of transmitters/ receivers.● Computer control of the whole system

ACTIVE PHASED ARRAY RADAR

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MU

The MU radar, Shigaraki, Japan

Research Institute for Sustainable Humanosphere, Kyoto University

46.5 MHz, 103mφ Yagi array, 1 MW

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The MU radar features an active phased array:

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Mete

oro

logic

al ballo

on

ob

serv

ati

on

6 hrs interval

Atmospheric radars provide continuous wind data with high time and altitude resolutions that have ever been realized.

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MU レーダー観測

Passage of a typhoonMete

oro

logic

al ballo

on

ob

serv

ati

on

Atm

osp

heric ra

dar o

bse

rvatio

n

Atmospheric radars provide continuous wind data with high time and altitude resolutions that have ever been

realized.

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Daily mean (a) eastward (solid) and northward (dashed) radial velocity profiles and hourly mean radial velocity fluctuations in the (b) east and (c) north directions for 17/18 October (after Fritts et al., 1988).

Mean wind (20 oblique) Fluctuations from the mean wind

Vr(Meridional)

Atmospheric waves modulatetropo/stratospheric wind profiles.

MeridionalZonal

Ur(Zonal)

°

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Atmospheric waves modulate mesospheric wind profiles more

extensively

Zonal wind

Heig

ht

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北斎

Analogy to ocean surface waves:Their growth and breaking

Woodcut print painted by Hokusai Katsushika (19th century)

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Atmospheric gravity waves: Propagation and saturation

Deceleration of mean flow

Atmospheric gravity waves

Saturation

Momentum flux

Wave breaking

Turbulence

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Weak wind

Latitudinal distribution of zonal wind velocity in the mesosphere

Theoretically, a strong geostrophic wind exists above the mesosphere.

Observationally, the wind is weak irrespective of season and latitude.

E: Easterly or westward wind W: Westerly or eastward

wind

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Momentum flux measured with the MU radar

Eastward flux

Westward flux

Deceleration of westward windDeceleration of

eastward wind Mean flowwestward

Mean floweastward

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(Model vs Observational results)

Saturation ofatmospheric gravity waves

k :

k-3

k-3

k :

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Gravity waves found to be ubiquitous in the ionosphere and thermosphere

“Gravity waves” continuously modulate the structure anddynamics of this region.

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Dispersion relation for thermospheric gravity waves

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Sata

Darwin

Darwin

Sata

Darwin

EAR

Projected along geomagnetic

field line

Hemispheric conjugacy of nighttime MSTIDs

Otsuka et al., 2004

630-nm airglow imagers simultaneously taken at conjugate points.

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z †FY (t) (t)h (z)Y

X

X

X

h1(z)

h2(z)

h3(z)

Y1(t)

X

h4(z)

X

h5(z)

Reconstructed time series at  z within range volume

zFY (t)

Y2(t)

Y3(t)

Y4(t)

Y5(t)

The principle of range imaging

適用する空間フィルター: T1 2 N 1 N(z) [h (z) h (z) h (z) h (z)]h r / 2 z r / 2 r 150m

2 *F FP (z) E{ Y (t) } h Rh

: (N×N) エルミート行列)()( * tYtYR

( 輝度分布 ~ 強度に比例 )     時系列 (I&Q)

)(1 tY

)(2 tY

)(3 tY

)(4 tY

)(5 tY

T1 2 N 1 NY(t) [Y (t) Y (t) Y (t) Y (t)]

kY (t):周波数 k の複素受信信号列,

Doppler spectrum

レンジ内の任意高度z における-noise, -power,-SNR, -Doppler velocity, -spectral width

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(Range imaging mode)

MUR in range imaging modeMUR in range imaging mode

Detailed observation of turbulence and stable layers at atime and range resolution comparable to standard weather radars.

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Simultaneous measurements with cloud radars

Ka-band (35 GHZ) and W-band (95 GHz) Doppler radars

For profiling cloud structures and processes as well as motions from Doppler shift.

Cirrus detected with a Ka-band radar at shigaraki

94.79GHz FMCW Falcon radar

Ref: http://katla.nd.chiba-u.jp/intro/fmcw.html

MUR reflectivity

MUR vertical air velocity

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3. A better knowledge of turbulence in clouds and at cloud edges (mechanisms, occurrence, intensity)and mainly cirrus Tools: lidar, weather radars, MU radar, IWP, balloon

KH Instability at a cirrus cloud base observed by MUR

KH instability inside cloud observed from lidarConvective instability at a cloud base (solid line)

observed by MUR

Turbulence in clouds

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WINDAS : Wind profiler network and data acquisition system - Japan Meteorological Agency (JMA) 2001 -

・ Consists of thirty-one 1.3GHz profilers (LTR) and control center, and

・ Provides the NWPs with initial values of wind field.

0   

500km

WIND PROFILER SITES

CONTROL CENTER (JMA HQ )

RADIOSONDE STATIONS

LTR, RISH Kyoto Univ.

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Impact of profiler data to MSM for severe rainfall

(c) Composite of radars and rain gauges

(a) 3hr forecast of MSM without profiler data

(b) 3hr forecast of MSM including profiler data

Total Rain Amount for 3hr (mm)

Profiler

200kmRawinsonde

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Operational Wind Profiler Networks

from www.ecmwf.int

NOAA Profiler Network

WINPROF(CWINDE)

Japan Met Agency

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Atmospheric temperature measurement with

RASS: Radio Acoustic Sounding System

Horn speaker system

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RASS profile

Atmospheric temperature profiles with the MU radar - RASS

- Profiles are successively obtained every three minutes.

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RASS contour

Temperature fluctuation and wind vectors

near cold front surfaceCold Front Surface

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Equatorial Atmosphere Radar: EAR

Antenna array (110 m in diameter)

47MHz, 560 Yagi antennas, 100kW

Bukittinggi, West Sumatra, Indonesia(0.20 S, 100.32 E,865 m above sea level)

° °

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The Equatorial Atmosphere Observatory (EAO) Kototabang, Indonesia

μ-rain radar

Ceilometer

Disdrometer

Optical rain gauge

Radiometer

RASS sounder

X-band met radar

GPS receiver

All sky imager

VHF radar

Lidar

EAR receiver

EAR

FMCW radar

Meteor radar

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× : cold-point tropopause

Breaking Kelvin wave

Increase of turbulence

Zonal wind

Turbulence

Large-scale convective system of ISV

成層圏と対流圏の大気の交換

EAR: Breaking of Kelvin wave at the tropopause

wave

waveexcitation

Fujiwara et al., 2003

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Where will the “gene” of active-phased array radars go?

MAARSY, Andoya

Equatorial Atmosphere Radar

MU radar

PANSY radar

An MUR-type radar being build at

Syowa base in the Antarctic

MAARMAARSYSY

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Concluding Remarks- In the last forty years, atmospheric radars have been proving themselves a most powerful tool for revealing the basic processes of the Earth’s atmosphere.

- Currently, various new sophisticated techniques are being developed with atmospheric radars, and their commercial models are successfully implemented to operational weather forecast.

- In the future, they will make most important contributions to studies of the atmospheric sciences, e.g., the climate change.

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Thank you for your attention.