Research on the Influence of Solar Radiation, Sky Background Radiation and Sea Surface Emission to Infrared Search

2012 ◽  
Vol 463-464 ◽  
pp. 975-979 ◽  
Author(s):  
Yu Chen ◽  
Yun An Hu ◽  
Yong Tao Zhao ◽  
Yong Xing Xie ◽  
Chun Hua Cheng

Sea background radiation is influenced by solar radiation, sky background radiation and sea surface emission radiation. On the basis of studying the simple sea radiation model, analyze the influence of atmospheric transmittance and sea background radiation to infrared detector, emphasis on influence of solar, sky and sea surface emission radiation to infrared search in analyze Sea background radiation, emphasis on influence of aerosol to infrared search under troposphere in analyze atmospheric transmittance.

2018 ◽  
Vol 81 ◽  
pp. 93-106 ◽  
Author(s):  
Antonio J. Gutiérrez-Trashorras ◽  
Eunice Villicaña-Ortiz ◽  
Eduardo Álvarez-Álvarez ◽  
Juan M. González-Caballín ◽  
Jorge Xiberta-Bernat ◽  
...  

PeerJ ◽  
2021 ◽  
Vol 9 ◽  
pp. e12373
Author(s):  
Lili Jin ◽  
Sasa Zhou ◽  
Qing He ◽  
Alim Abbas

The characteristics of solar radiation and the influence of sand and dust on solar radiation in the northern margin of Taklimakan Desert were analyzed using radiation observation data from 2018. The results showed that the annual total radiation, direct radiation, and scattered radiation at Xiaotang were 5,781.8, 2,337.9, and 3,323.8 MJ m−2, respectively. The maximum monthly total radiation, direct radiation, and scattered radiation were observed in July (679.8 MJ m−2), August (317.3 MJ m−2), and May (455.7 MJ m−2), respectively. The aerosol optical depth corresponded well with the scattered radiation, and the maximum value was in May. Further analysis showed a significant correlation between the total radiation and solar height angle under different weather conditions. Under the same solar height angle, total radiation was higher during clear days but lower on sandstorm days. Calculation of atmospheric transmittance showed that the average atmospheric transmittance on a clear day was 0.67; on sand-and-dust days, it was 0.46. When the atmospheric transmittance was 0.5, the increase in scattering radiation by aerosol in the air began to decrease. Probability analysis of radiation indicated the following probabilities of total radiation <500 W m−2 occurring on clear, floating-dust, blowing-sand, and sandstorm days: 67.1%, 76.3%, 76.1%, and 91.8%, respectively. Dust had the greatest influence on direct radiation; the probabilities of direct radiation <200 W m−2occurring on clear, floating-dust, blowing-sand, and sandstorm days were 44.5%, 93.5%, 91.3%, and 100%, respectively, whereas those of scattered radiation <600 W m−2were 100%, 99.1%, 98.1%, and 100%, respectively. Therefore, the presence of dust in the air will reduce scattered radiation.


2007 ◽  
Vol 152 (2) ◽  
pp. 351-361 ◽  
Author(s):  
Stefano Goffredo ◽  
Erik Caroselli ◽  
Elettra Pignotti ◽  
Guido Mattioli ◽  
Francesco Zaccanti

2020 ◽  
Vol 40 (2) ◽  
pp. 0201001
Author(s):  
李建玉 Li Jianyu ◽  
黄尧 Huang Yao ◽  
黄宏华 Huang Honghua ◽  
朱文越 Zhu Wenyue ◽  
魏合理 Wei Heli

IEEE Access ◽  
2019 ◽  
Vol 7 ◽  
pp. 64758-64766 ◽  
Author(s):  
Hamza Abunima ◽  
Jiashen Teh ◽  
Hussein Jumma Jabir

2020 ◽  
Vol 24 (2) ◽  
pp. 423-441 ◽  
Author(s):  
Mingxi Zhang ◽  
Bin Wang ◽  
De Li Liu ◽  
Jiandong Liu ◽  
Hong Zhang ◽  
...  

2020 ◽  
Vol 101 (2) ◽  
pp. E146-E166 ◽  
Author(s):  
Christian Stolle ◽  
Mariana Ribas-Ribas ◽  
Thomas H. Badewien ◽  
Jonathan Barnes ◽  
Lucy J. Carpenter ◽  
...  

Abstract The sea surface microlayer (SML) at the air–sea interface is &lt;1 mm thick, but it is physically, chemically, and biologically distinct from the underlying water and the atmosphere above. Wind-driven turbulence and solar radiation are important drivers of SML physical and biogeochemical properties. Given that the SML is involved in all air–sea exchanges of mass and energy, its response to solar radiation, especially in relation to how it regulates the air–sea exchange of climate-relevant gases and aerosols, is surprisingly poorly characterized. MILAN (Sea Surface Microlayer at Night) was an international, multidisciplinary campaign designed to specifically address this issue. In spring 2017, we deployed diverse sampling platforms (research vessels, radio-controlled catamaran, free-drifting buoy) to study full diel cycles in the coastal North Sea SML and in underlying water, and installed a land-based aerosol sampler. We also carried out concurrent ex situ experiments using several microsensors, a laboratory gas exchange tank, a solar simulator, and a sea spray simulation chamber. In this paper we outline the diversity of approaches employed and some initial results obtained during MILAN. Our observations of diel SML variability show, for example, an influence of (i) changing solar radiation on the quantity and quality of organic material and (ii) diel changes in wind intensity primarily forcing air–sea CO2 exchange. Thus, MILAN underlines the value and the need of multidiciplinary campaigns for integrating SML complexity into the context of air–sea interaction.


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