kaguya image gallery | First report -Sounder Mode- (2/3)

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Observation Mission

XRS :
X-ray Spectrometer

GRS :
Gamma-Ray Spectrometer

MI :
Multi band Imager

SP :
Spectral Profiler

TC :
Terrain Camera

LRS :
Lunar Radar Sounder

LALT :
Laser Altimeter

LMAG :
Lunar Magnetometer

CPS :
Charged Particle Spectrometer

PACE :
Plasma energy Angle and Composition Experiment

RS :
Radio Science

UPI :
Upper-atmosphere and Plasma Imager

RSAT :
Four way Doppler measurements by Relay satellite and Main Orbiter

VRAD :
Differential VLBI Radio Source

HDTV :
High Definition Television

Observation Areas

Landing Site

Land Features

Crater

Observation Target

Earth and Other Planets

Special Contents

QuickTime VR

First report -Sounder Mode- (2/3)

Updated : 2008.01.22

Observation date : 2007.11.20

Simulated radar echoes to be observed by the KAGUYA (left) as it travels over the model surface structure (right) (Kobayashi et al. 2002). In the diagram, vertical and horizontal axes correspond to the apparent depth and positional offset, respectively, and coded in color is the amplitude of radar echo.