scholarly journals Quantification of the Adjacency Effect on Measurements in the Thermal Infrared Region

2019 ◽  
Vol 57 (12) ◽  
pp. 9674-9687 ◽  
Author(s):  
Xiaopo Zheng ◽  
Zhao-Liang Li ◽  
Xia Zhang ◽  
Guofei Shang
2014 ◽  
Vol 2014 ◽  
pp. 1-16 ◽  
Author(s):  
Hui Xu ◽  
Tianhai Cheng ◽  
Donghai Xie ◽  
Jiaguo Li ◽  
Yu Wu ◽  
...  

Asia dust generated in northern China exerts significant influences on regional air quality, weather, and climate. In this study, a dust identification algorithm over arid and semiarid regions of Asia was proposed based on the thermal observations of atmospheric infrared sounder (AIRS). Firstly, a combination of the line-by-line (LBL) and discrete ordinates radiative transfer (DISORT) model was utilized to investigate the thermal infrared signatures of dust and cloud in 800–1250 cm−1region. Secondly, six channels in the thermal infrared region were selected from AIRS to monitor dust from space, and a further sensitivity analysis for dust and cloud under different conditions was also performed. Then, the description of the detailed identification method was provided based on distinct thermal infrared signature of dust. At last, several dust events that observed in northern China between the period of 2008 and 2012 were analyzed, and the usefulness of monitoring the outbreaks of Asian dust was emphasized through the comparison with moderate resolution imaging spectroradiometer (MODIS) visible observations and cloud aerosol lidar with orthogonal polarization (CALIOP) data in this study.


2002 ◽  
Vol 572 (1) ◽  
pp. 276-287 ◽  
Author(s):  
Miwa Goto ◽  
Naoto Kobayashi ◽  
Hiroshi Terada ◽  
A. T. Tokunaga

2000 ◽  
Vol 197 ◽  
pp. 461-470 ◽  
Author(s):  
J. Crovisier

The Infrared Space Observatory (ISO) offered us the opportunity to observe celestial bodies from 2.4 to 196 μm, which is of particular interest for comets. We present here spectroscopic observations with ISO of comets C/1995 O1 (Hale-Bopp) and 103P/Hartley 2. Fluorescence emissions of H2O, CO2 and (for comet Hale-Bopp only) CO and CH4 are observed, yielding the production rates of these species. High-resolution spectra of water permit the study of the rotational and spin temperatures of this molecule. In comet Hale-Bopp, the thermal infrared region of the spectra shows specifically, in addition to continuum-like emission, the signatures of crystalline, Mg-rich olivine (forsterite), and signs of crystalline pyroxenes, amorphous silicates and water ice. The presence of crystalline silicates is also suggested in the Jupiter-family comet P/Hartley 2.


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