SPACE REMOTE SENSING IN INFRARED WAVELENGTH RANGE WHEN SEARCHING FOR HYDROCARBON DEPOSITS IN THE DOUALA BASIN OF THE REPUBLIC OF CAMEROON

Author(s):  
K.M. Karimov ◽  
◽  
A. Al Ali ◽  
T.A. Vagapov ◽  
M.A. Lonshakov ◽  
...  
2011 ◽  
Vol 9 (11) ◽  
pp. 4199 ◽  
Author(s):  
Shuji Ikeda ◽  
Hiroyuki Yanagisawa ◽  
Akiko Nakamura ◽  
Dan Ohtan Wang ◽  
Mizue Yuki ◽  
...  

2021 ◽  
Vol 65 (12) ◽  
pp. 1194-1210
Author(s):  
A. A. Ermash ◽  
S. V. Pilipenko ◽  
E. V. Mikheeva ◽  
V. N. Lukash

2020 ◽  
Vol 149 ◽  
pp. 03006 ◽  
Author(s):  
Ekaterina V. Pavlova ◽  
Anastasiia I. Volkova ◽  
Ekaterina A. Demina

Currently, the consequences which take place in Khakassia expansion of tree-shrub vegetation on fallow lands have not been properly assessed neither from an ecological nor economic point of view. Based on the analysis of the agricultural map scale 1: 100 000 decoding images Landsat 4–5, 7, 8 and Sentinel 1, and 2, as well as subsatellite ground researches were carried out the identification, the description and assessment of the qualitative state of postagrogenic lands of Khakassia exposed to the processes of overgrowth of tree-shrub vegetation. As an example, this article analyzes the processes of overgrowth of agricultural land on the example of the territory of the Moscow village council of Ust-Abakan district. A geoinformation project of spatial distribution of postagrogenic lands within the Moscow village council of Ust-Abakan district of Khakassia was developed. The results of the research showed that in the studied area in the structure of agricultural land 67204 hectares of land belongs to the fallows located at different stages of recovery of which 77 % exposed to overgrowth processes. The obtained data indicate the need for the formation of management decisions in the field of land use.


Author(s):  
Mario Christian Falconi ◽  
Dario Laneve ◽  
Caterina Clemente ◽  
Giovanna Ricchiuti ◽  
Antonella Loconsole ◽  
...  

1982 ◽  
Vol 98 ◽  
pp. 211-228
Author(s):  
L. Houziaux ◽  
Y. Andrillat

Since the time of I.A.U. Colloquium n° 70, new data have been obtained in the infrared, far less however than in the ultraviolet or in the visible. Few line spectra have been recorded but numerous results have been published in the field of spectrometry of the continuum. It is however neither easy nor very useful to report on the infrared wavelength range alone, and therefore we shall consider when appropriate other spectral regions in this review. After all, the astrophysicist nowadays has the advantage to seek for information in a spectrum which encompasses a fantastic frequency range of about 10 dex, from ν = 108s−1 up to ν = 1018s−1. This means that a contemporary astronomer will have to become familiar with a somewhat larger span of phenomena than with the rather narrow one he has been accustomed to for the last 40 or 50 years.


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