Full text: From pixels to sequences

  
298 
Weathering Degree Survey of MAGAI-BITSU 
by Infra-red Thermograph 
Toshihiko SAKAYAMA (OYO Corporation)* 
Masaaki SAWADA (Nara National Cultural Properties Institute)** 
Yoshito MIYATSUKA (Shin Air Survey Co.,Ltd.)*** 
*** 988, Bessho, Hachioji City, Tokyo, 192-03, JAPAN 
phone; +81-426-77-5480 
fax; +81-426-77-5030 
Key Word; Archaeology, Infra-red, Thermograpy 
1,Introduction 
The stone Buddhist image of ONO DERA temple is a great MAGAI-BUTSU (cliff image) engraved on the stonewall, 
measuring 14m in height 4m in width, and is said to have been made A.D.1207 at early KAMAKURA Era. 
For nearly 800 years, weathering and deterioration have progressed over the rock surface, while physical and chemical 
factors are interrelated in a complicated fashion. The surface of the rock has shown phenomena of becoming like an 
eardrum, floating up and peeling-off from the surface. In order to consider the countermeasures of preserving and 
repairing of the stone image, it is necessary to grasp scientifically the current weathered condition and to clarify 
progressing mechanisms of weathering and deterioration. At this time, a survey of weathering degree by remote-sensing 
using an Infra-red thermograph has been carried out in order to find out the expansion of the portion with deterioration 
such as the rock surface becoming like an eardrum and floating up. 
2,Measuring Principles of Infra-red Thermograph 
Infra-red thermograph measures the temperature of the object by measuring heat radiation, which is constantly limited 
from all objects. Thermal radiation is considered to have been generated by rotation or vibration of molecules or by 
vibration of the solid body lattice. The vibration spectrum appears in the extreme-infra-red ray area. These infra-red rays 
are electromagnetic waves longer that visible rays and shorter than the microwaves, and their wavelenght ranges from 
0.75mm to 1mm. 
Theoretical research on the relation between temperature and thermal radiation was completed by Planck as the theory 
of blackbody radiation in the early years of the 20th century, and the theoretical foundation of measuring thermal 
radiation was established. When the object is a blackbody, the relation between its radiation strength and the temperture 
is given by Planck's equation of radiation. The infra-red thermograph detected rays irradiated from the object body, using 
at detector, which has sensitivity in the limited wavelegth area, and directly indicatest the detected temperature 
obtained by nonlinear conversion on the basis of Plank's equation of radiation. The infra-red thermograph used for this 
measurement is the TH1101 (Thermo-tracer) made by Nippon Electric SAN-EI. The infra-red thermograph carries out 
optically, in the horizontal and vertical directions, the infra-red radiation energy, which is naturally irradiated from the 
surface of an object, and indicates the temperature distribution of the measured object as a color static picture. The 
infra-red detector, which converts incomming infra-red rays into electric signals, is HgCdTe (Mercury Cadmium 
Tellurium), which has a wavelength of 8 to 13um. 
3,Measured Results by the Infra-red Thermograph 
Measurements by the infra-red thermograph were carried out in winter, during mid-December. The detecting part of the 
infra-red thermograph was installed in the precincts of ONO DERA temple, which commanded the entire view of the stone 
Buddha statue, and the temperature distribution of the stone Buddha statue was continuously measured at 30-minute 
intervals from 9:30 to 18:00. At this time, the distance between the stone Buddha statue and the detector part of the 
infra-red thermograph was about 50m. Fig. 1 shows the temperature distribution on the surface of the Buddha statue at 
14:00, and Fig.2 shows the distribution of the temperature change during the period from 14:00 to 17:59. 
The external air temperature measuring day were 2.5'C at 9:30, but in the daytime, the temperature rose until it reached 
IAPRS, Vol. 30, Part 5W1, ISPRS Intercommission Workshop "From Pixels to Sequences", Zurich, March 22-24 1995 
  
  
 
	        
Waiting...

Note to user

Dear user,

In response to current developments in the web technology used by the Goobi viewer, the software no longer supports your browser.

Please use one of the following browsers to display this page correctly.

Thank you.