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Seen from Space 2005

Landscape of Taiki-cho Region Observed from Airship

  Station-keeping flight tests (*1) of the stratospheric platform (SPF) project were conducted at Taiki-cho, Hokkaido, from July to November 2004. As one objective for the tests, we successfully conducted several Earth-observation experiments (*2) such as vegetation observation and temperature monitoring.
Fig. 1(a) WAMS-VNIR Image
(around the Taiki-cho test site)
-678 nm (red) band-
Fig. 1(b) WAMS-VNIR Image
(around the Taiki-cho test site)
-865 nm (near infrared) band-

Figures 1(a) and (b) are WAMS-VNIR images from the Station-keeping test airship flying around the Taiki-cho test site at an altitude of 850 m. WAMS-VNIR can take images of several wavelength bands including red (678nm) and near-infrared (865nm). Comparing (a) and (b), near-infrared radiance in the vegetation region is higher than that in other coverage regions. Using such multiband characteristics, we are able to understand the distribution and conditions of vegetation around the test site.

Fig. 2 WAMS-TIR Image(around the Taiki-cho test site)
-Wide (7-12 μm) band-
(Click here to see animation of images taken at 5-second intervals)

Figure 2 presents WAMS-TIR images from the airship flying around the Taiki-cho test site at an altitude of 850 m. Generally, anything radiates invisible light (thermal infrared light) whose intensity is greater when its temperature is higher. By measuring the intensity of the infrared light, we can monitor the distribution of land-surface temperatures. For example, Fig. 2 illustrates a high temperature over an asphalt-covered region (such as a landing field) warmed up by sunshine. We can also distinguish buildings and undulations from the thermal infrared image.

Note that the WAMS-VNIR and WAMS-TIR were equipped with distorted optical systems (like fish-eye lens) so that after geometric correction the images are "pin-cushion" shape, as you can see in Figs. 1 and 2.

Fig. 3 HRS Image (around Hamataiki village)
(Click the image to see animation)

Figure 3 is an HRS image with few score centimeter resolution taken from the airship flying around Hamataiki village at an altitude of 500 m. As a traffic observation experiment, the HRS took moving images of vehicles passing, stopping, and turning. By computer processing the images, we can recognize a run pattern of the vehicles and accumulate statistics data of traffic streams. We expect this method to be applied to future traffic control systems.

Earth observation from the SPF has several advantages over the traditional airborne or spaceborne observations. We can continuously monitor a specific area over a long period of time with high spatial resolution and accuracy. In the future, we expect SPF observation to be used for various applications such as remote-sensing for agriculture, forestry, fishery, traffic monitoring, and disaster monitoring.



(*1) The Station-keeping flight test is conducted by the Japan Aerospace Exploration Agency (JAXA) in collaboration with the National Institute of Information and Communications Technology (NICT). The Stratospheric Platform (SPF) was selected as "The Millennium Project," which conceives new ventures, and attempts to resolve problems faced by mankind. This project was initiated by the Prime Minister in October 1999.

(*2) October 5, 2004 Flight characteristics acquisition flight test: maximum altitude 600 m
        November 5, 2004 Mid-altitude flight test:maximum altitude 2,000 m


Explanation of the images
(Figs. 1 to 3)
Platform: Station-keeping test plane (airship)
Sensor: Earth Observation System for SPF-II (EOSS)
(See appendix for detailed information of EOSS.)
Time and Date: November 5, 2004 12:06(JST) (Figs. 1 and 2)
November 5, 2004 14:07(JST) (Fig. 3)

Related sites:
Station-keeping flight test of the Stratospheric Platform (SPF) Project(Japanese only)

Appendices:
Earth-observation mission objectives in the station-keeping flight test:
1) To examine the feasibility of observation missions from the SPF.
2) To demonstrate sensor technologies for future remote sensing projects.

Three Sensors:
A) Wide-Angle Multi-band Sensor - Visible and Near-Infrared (WAMS-VNIR)
  ・ A sensor that contains an optical system with a wide view and makes multi-band measurements of visible and near-infrared light.
  ・ Vegetation and atmospheric observation.
B) Wide-Angle Multi-band Sensor - Thermal Infrared (WAMS-TIR)
  ・ A sensor that contains an optical system with a wide view and makes multi-band measurements of thermal infrared light.
  ・ Observation of ground-surface temperature.
C) High-Resolution Sensor (HRS)
  ・ CCD cameras to obtain moving images with less than 50 cm resolution.
  ・ Basic traffic observation test.

EOSS Specifications:
  WAMS-VNIR WAMS-TIR HRS
Spectral band 545, 678, 763, 865, 940 nm
(Polarization: 678, 865nm)
8.6, 10.8, 12.0 μm,
Wide (7-12μm)
Visible (RGB)
FOV
(@ 4 km)
8kmx8km 8kmx6km 0.36 kmx0.33 km
Spatial resolution
(@ 4 km)
4.6 m
(at image center)
16 m (at image center) 30 cm
Detector
(Pixel Format)
CCD
(1024 x 1024 pixels)
Uncooled microbolometer
(320 x 240 pixels)
3 CCD Camera
(0.38 Mega pixels)
S/N
NEdT
>200 0.1 K (wide band)
0.5 K (narrow band)
N/A

Photograph of EOSS:
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