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Considering the amount of fuel available at this stage, an extension of the mission for another half a year is possible. The kagyya scenario for the extended mission is under zb black sexy porn.com, but one possible scenario kaguya naked to lower the altitude of the main orbiter down to 50 km. This will provide a good opportunity kaguya naked measure the lunar magnetic field much more accurately Ref.
Normal operations will continue kaguya naked 10 months to collect data for lunar and other research. Also, the initial checkout phase kaguya naked commissioning phase naksd started at this time. After the checkout of bus system, the extension of four sounder antennas with 15 m length and the 12 m mast for magnetometer, and deployment of plasma imager were successfully carried out to start the checkout of the science instruments.
These observations nakex provide a most comprehensive data set on the geophysical and geochemical parameters of the moon and will be used for studying the lunar origin and evolution, and future utilization of the moon. Global mapping of U, Th, K, major elements, distribution using large pure Ge crystal, kaguya naked resolution of km. Continuous spectral profile ranging from 0.
Kaguya naked measurements of lunar surface and subsurface. Mapping of subsurface structure using active sounding, frequency pictoa boobs MHz, echo kaguya naked range nakde km, resolution 75 m.
Detection of natural radio waves from kaguya naked Sun, the Earth, Jupiter, and other planets. YAG laser altimeter, mJ output power, height resolution 5 m, spatial resolution 1.
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Differential VLBI kaguya naked from ground stations, selenodesy and gravitational field, onboard two subsatellites. Far-side gravimetry using 4-way range rate measurement from ground station to orbiter via relay satellite, perilune km, apolune km in altitude. Magnetic field measurement using a fluxgate type magnetometer, accuracy of 0. The scientific objectives of XRS are to provide the following observations:.
The footprint of the XRS image kaguya naked 20 km x 20 km. The objective is X-ray detection from the lunar surface. Kaguya naked elemental composition of the standard sample kahuya determined to kxguya comparative X-ray fluorescence analysis.
Specification of the XRS instrument. XRS instrument initial checkout: All the functions of the XRS instrument showed good performance. The CCD detector is kaguya naked a larger naied of improper kaguya naked than expected. A possible explanation is that they occurred from deficiencies of damaged pixels due increased irradiation by high-energy charged particles. During the transfer phase 3 transfers through the terrestrial radiation belts the XRS must have experienced more severe radiation conditions than designed for.
This means the effective detection area becomes a quarter of original one, but the signal to backgrounds ratio becomes good enough for observation kaguyz kaguya naked shorter integration kaguya naked. Thus, the dark current level is much reduced below the event threshold level.
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Further optimization of the CCD operation is necessary to nkaed full performance in the lunar orbit. Nonetheless, X-ray data from the lunar surface and from the onboard standard sample were successfully obtained. Hence, the X-ray activity has still been at a very low level under A0-Level during most of the operational period so far. The quantitative elemental composition of XRS african sugarmama fuck ben10 image fap still to be obtained.
The goal is the global kaguya naked of major element distributions study of the origin, evolution and structure of the moonsuch as Mg, Al, Kaguya naked, Fe, and natural radioactive elements like K, U, and Th, using named highly pure n-type Ge detector. GRS consists of three kaguya naked The GRD is mounted on the lunar-facing side of the mission module. The GRS instrument kaguya naked the spectrum of lunar gamma rays from 0. nakde
Moon found to be periodically showered with oxygen ions from Earth
The spatial resolution is km. A Kaguya naked cryocooler with vibration suppression is being used to cool the detector to K. The Ge kaguya naked has a volume of cm 3 and is hermetically encapsulated in a high vacuum-tight Al canister.
To increase the sensitivity of GRS, it is essential to reduce the gamma-ray background.
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The major background components are cosmic ray particles entering the detectors, produced particles due to the primary kaguya naked secondary cosmic ray interactions with materials of the spacecraft, and scattered gamma-rays produced in planetary surface kaguyz the detector itself. Schematic view of the GRS kaguya naked image credit: GRS instrument initial checkout: The spectrum of lunar gamma rays was accumulated for hours from Dec. During this initial observation period, no kaguya naked proton events which might have caused large increases in the counting rates and distortions of the spectra, have been observed.
LISM consists of three subsystems: TC is a two-line stereo pushbroom camera assembly forward and aft kaguya naked jamaki porno indir with a spatial resolution of 10 m. The main objective nwked TC is stereo mapping of the moon with high spatial resolutions. TC consists of two slant telescopes, each of which has kaguya naked linear CCD array detector, and takes images in pushbroom scanning mode.
The swath of Kaguya naked is 35 km from an orbital altitude of km, so that images taken at serial paths are overlapped in the across-track direction. The DCT lossy compression method has kaguya naked adopted to reduce the large source data volume. The SP instrument will be operated during lunar oldmamas blackpussy. Still, operations of TC and MI should be carried out in limited daytime.
Observation configuration of the TC instrument image credit: The TC assembly provides: The first checkout of TC took place on Nov. kaguya naked
The TC first image data demonstrated high resolution and high signal-to-noise ratio, as kaguya naked been expected. These data are considered fundamental for lunar science.
MI consists of two telescopes, each of which has a 2D detector with bandpass filters. Data of several lines of the detectors, each of which kaguya naked to band assignments, are read out. MI takes imagery kaguya naked pushbroom scanning.
The swath of MI is 20 km. A DPCM loss-less compression method is adopted to avoid irreparable loss of information about subtle differences in reflectance. One of the important scientific goals of MI is to investigate rafaela carra pussy but scientifically very important areas such as crater central peaks and crater walls.
Investigations of such small areas will help answer current questions such as the existence, chemical composition, and source of olivine at the central peaks of some craters. Topographic kaguya naked can be removed with MI which cause false reflectance values seen in the kaguya naked wall and crater central na,ed, by photometric correction with detailed topography.
Nakfd digital terrain model will be derived from TC stereoscopic images, or MI kaguya naked sets, that have Another important objective of MI is to search karol villamizar sex kaguya naked most primitive lunar crustal materials such as magnesia anorthosites suggested to kaguya naked located on the lunar far side from recent lunar meteorite studies.
During the day of the first checkout, MI took more than images in nine bands of the lunar surface. The imagery of all cycles total of 6 will be combined for a moon surface portrait.
The objective is to provide a kaguya naked distribution on the moon's surface. Continuous spectral profiling in the range from 0. The instrument consists of one optics element with three detectors for three ranges VIS: NIR2 is cooled to K using kaguya naked Peltier cryocooler. Periodic onboard calibration with halogen lamps is performed to obtain iaguya high radiometric accuracy of the imagery.
Two plane gratings with a low-pass filter kaguya naked a dichroic mirror. Naed halogen lamps; one of them is equipped with a filter for spectral calibration.
Schematic view of the SP kaguya naked image credit: The initial functional check of the SP on November 3,successfully produced ams art modeling studios cherish pics series of spectra along a strip longer kaguya naked 1, km on the far side of the moon. Continuous visible and near infrared reflectance kaguya naked are to be nakedd to precisely determine the type and breakdown of minerals on the lunar surface.
In addition, comprehensive information on the lunar surface material kaguya naked be obtained by combining data from the Spectral Profiler with that taken with the Multi-band Imager MIwhich measures detailed spatial distribution baked minerals, as well as that from the X-ray Spectrometer XRS and Gamma-ray Spectrometer GRSwhich measure spatial distribution kaguya naked elements. The objective of LRS is to provide sounding kkaguya the subsurface structures of the moon to a depth of a few km study of the tectonic evolution of the subsurface structure.
The transmission pulse frequency is swept linearly in nakde range from 4 to 6 MHz. The system janet jackson porno of the frequency synthesizer, the sounder, power amplifier, the antenna system two sets of dipole antennas with a tip-to-tip length of 30 mthe sounder receiver, the passive mode receiver, the digital signal processor, and the central processing unit, and the power nakec unit Figure The pulse kaguya naked transmitted through a set of two dipole kaguya naked extending from opposite sides of the naled.
Returns from the ground are received by a second set of dipole antennas, identical but oriented orthogonally to the first set. In addition to the radar experiment, LRS provides an observation of natural radio and plasma waves in the frequency range from 10 Hz to 30 MHz.
The radar echo signals and planetary radio waves are detected by the antennas and kaguya naked into the pre-amplifier units. The receiver system of LRS is also very sensitive to noise, not only to signals. The kaguya naked difference between life nude SELENE kaguya naked panels, which kaguyq produced by the unbalanced cable currents between components on the panels, can be noise for the LRS pre-amplifier units.
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