Dersleri yüzünden oldukça stresli bir ruh haline sikiş hikayeleri bürünüp özel matematik dersinden önce rahatlayabilmek için amatör pornolar kendisini yatak odasına kapatan genç adam telefonundan porno resimleri açtığı porno filmini keyifle seyir ederek yatağını mobil porno okşar ruh dinlendirici olduğunu iddia ettikleri özel sex resim bir masaj salonunda çalışan genç masör hem sağlık hem de huzur sikiş için gelip masaj yaptıracak olan kadını gördüğünde porn nutku tutulur tüm gün boyu seksi lezbiyenleri sikiş dikizleyerek onları en savunmasız anlarında fotoğraflayan azılı erkek lavaboya geçerek fotoğraflara bakıp koca yarağını keyifle okşamaya başlar

GET THE APP

Journal of Earth Science & Climatic Change - Determination of Linke’s Turbidity Factors from Model and Measure Solar Radiations in the Tropics Over Highland of South-East Ethiopia.
ISSN: 2157-7617

Journal of Earth Science & Climatic Change
Open Access

Like us on:

Our Group organises 3000+ Global Conferenceseries Events every year across USA, Europe & Asia with support from 1000 more scientific Societies and Publishes 700+ Open Access Journals which contains over 50000 eminent personalities, reputed scientists as editorial board members.

Open Access Journals gaining more Readers and Citations
700 Journals and 15,000,000 Readers Each Journal is getting 25,000+ Readers

This Readership is 10 times more when compared to other Subscription Journals (Source: Google Analytics)

Determination of Linke’s Turbidity Factors from Model and Measure Solar Radiations in the Tropics Over Highland of South-East Ethiopia.

Ambaye C*
Madda Walabu University, Bale-Robe, Ethiopia
*Corresponding Author: Ambaye C, Madda Walabu University, Bale-Robe, Ethiopia, Tel: +251911301844, Email: janbo2012@gmail.com

Received: 05-Jun-2018 / Accepted Date: 09-Jul-2018 / Published Date: 14-Jul-2018 DOI: 10.4172/2157-7617.1000479

Keywords: Aerosols; Africa rising; Global solar radiation; Links turbidity factors; Perceptible water vapor

Introduction

The attenuation of solar radiation through a real atmosphere versus that through a clean, dry atmosphere gives an indication of the atmospheric turbidity. IT is a very suitable approximation to model the atmospheric absorption and scattering of the extraterrestrial radiation relative to dry and clean atmosphere [1]. Its study is important for monitoring atmospheric pollution trough the presence of dust aerosols in the meteorology and climatology. Atmospheric turbidity associated with aerosols from dust loads, water vapor and anthropogenic source is also an important parameter for assessing pollution trends [2].

As other published literatures, atmospheric aerosol has increased enormously over the last two decades. IT can either have nonanthropogenic or anthropogenic sources and are either emitted as primary particles (i.e. They are directly emitted to the atmosphere) or formed by secondary processes (i.e. By transformation of emitted precursor gases). IT has been rising from low concentration over the preserved forest of Amazonian because of land-use change from natural begins to biomass burning [3] may bring TL to the pollution level. According to Engelbrecht and Derbyshire [4] the pollution level of dust aerosols through the determination of TL being closer to 8.

The global source regions of dust have covered the Northern Hemisphere, including North Africa, the Middle East, the Northwest Indian subcontinent, central Asia, and Northwest China [4]. Ethiopia is not immune from the large influx of dust because of its proximity, particularly in the Sahel and Arabia Peninsula. Influx dust from these regions, particulate matter from nearby industries, and smokes from deforestations for agriculture and fuel wood combined with maritime (Red Sea and Indian Ocean) moisture may contribute the rise of a turbidity factor in the area. The study area for this purpose is an Illusanbitu District located in tropical highland of South-East Ethiopia at about 7° latitude, 40° longitudes and 2500 m altitude. The determination of Linke’s turbidity factor TL was carried out from three method data.

• The meteorological data on Global Solar Radiation (GSR) were obtained from a non-government organization called Africa Rising [5] settled there.

• The model GSR data were extracted through integrating of mathematical equations from four atmospheric parameters by MATLAB tool.

• The satellite GSR data at the location was freely logged down from a website called Atmospheric Science Data Center controlled by the National Aeronautics and Space Administration NASA.

Materials and Methods

Mathematical formulations for global solar radiation modeling

The mathematical formulations were largely reviewed from the book written by Iqbal [6], and some published journals listed in the reference. The modeling in determining GSR entirely depends upon integrating the four major classifications of atmospheric parameters discussed below:

a. Geographical Parameters: The altitude and latitude in combining solar geometry climatic and optical parameters are essential in determining the amount of solar insolation reaching the earth’s surface.

b. Solar Geometric Parameters: Under this category, the amount of solar irradiance reaching the study area are influenced by solar geometry parameters such the solar zenith angle θz , declination angle δ solar altitude angle η and solar hour angles ω . The solar geometry called declination angle δ is computed as:

Equation (1)

The orientation of a horizontally placed solar receiver towards the incident radiation related to the declination angle δ , solar zenith θz , latitude ϕ, solar altitude angle η and solar hour angle ω in degree related as:

Equation (2)

Equation (3)

Where LT is the local time from the midnight. On the other hand, IT is well known that atmospheric turbidities linked with the presence of aerosols, water vapor, and ozone are the most important extinction components affecting the direct and diffuse components of solar radiation under clear skies [7]. As a matter of fact, the effect of moist or water vapor is taken by considering the w in centimeter in terms, relative humidity Hr, ambient temperature T and partial pressure in Kelvin are expressed in Equations 4 and 5.

a. Climatic parameters: These classifications involve the measurement of ambient temperature, relative humidity, horizontal climate visibility and partial air pressure. The ambient temperature and relative humidity are also served for computing perceptible water vapor w using Equations 4 and 5. As a matter of fact, the effect of moist or water vapor is taken by considering the w in centimeter in terms, relative humidity, Hr ambient temperature T and partial pressure in Kelvin are expressed in these equations.

Equation (4)

Equation (5)

The horizontal visibility V is also a significant climate factor in computing optical air transmittance in Equation (6). The horizontal Vis of the area lies within the range of 17 km up to 22 km during winter when there are low rainfall and cloud coverage.

b. Atmospheric optical parameters: IT is the most complex atmospheric phenomena in determining the energy budget at a given location. The amount of solar energy reaching the surface is affected by optical properties of water vapor, air, ozone layer and aerosol masses. Their effects on solar irradiance are sensed by computing their optical transmittance, reflectance, absorbance, Rayleigh centeredness and turbidity coefficients that attenuate the solar irradiance reaching the surface. The ground albedo is also taken into consideration for modeling purposes. The computed value of relative optical masses of aerosol τa , air mass ma, water vapor mw and ozone mo at a given location are given under Equations (6), (7) (10) and (11) respectively. Their values are almost in closer ranges as stated by Iqbal [6]. However, an optical mass of aerosols mo is the most uncertain parameters in calculating solar radiation on the ground [6]. They are highly variable in size, distribution, composition, and optical properties. For lack of required information, the value of computing optical air mass ma can be used as a substitute for optical mass of aerosol mo in Equation (7). Therefore, the optical transmittance τa written in Eq. (6) as the presence of aerosols is calculated as

Equation (6)

Where ma is in the Equation (6) is the relative optical dry air mass for local conditions computed through Equations 7, 8, and 9.

Equation (7)

Where P and Po are the local pressure and sea level pressures in millibars respectively. The local atmospheric pressure above sea level at altitude z is evaluated as:

Equation (8)

The altitude of the study location z is around 2480 m. The relative optical air mass mr in Equation (7) may be approximated by relating to zenith angle Equation:

Equation (9)

On the other hand, the corresponding expressions for relative optical water vapor mass mw and relative optical ozone mass mo are expressed in the following two expressions by Iqbal.

Equation(10)

Equation (11)

Where Z3 measures the concentrated ozone at around 22 km and Re is the radius of the earth approximated as 6370 km. Overall spectrally integrated transmittance computation for each atmospheric constituent is necessary steps for solar radiation parameterization in modeling [7]. The total transmittance τ as a function of the ozone layer thickness Equation in cm, perceptible water vapor w in cm, turbidity coefficient β and α , and the relative mass is evaluated by Iqbal [6]:

Equation (12)

The transmittance quantities Equation and Equation for some major atmospheric constitutes such as water vapors, ozone layers and aerosols are expressed as respectively in Equations (13), (16) and (28).

Equation (13)

Where αw is the attenuation coefficient of water vapor given as:

Equation (14)

Where U1 is the pressure-corrected relative optical path length written in terms of mr and w as:

Equation (15)

The transmittance Equation due to the ozone layer is given as:

Equation (16)

Where αo is the attenuation coefficient due to direct irradiance transmission through the ozone layer. Its expression is written as:

Equation (17)

The U3 is the ozone relative optical path given by:

Equation (18)

For broad spectral range, the integrated transmittance for Rayleigh scattering Equation over the wavelength interval Equation is defined as (Iqbal, 2012)

Equation (19)

Ion is the direct irradiance on horizontal surface normal to the sun's rays (also called direct normal radiation) and Isc is the solar constant whose value is 1367 W/m2. A regression-type correlation that fits Equation (19) is given as:

Equation (20)

During parameterization of the solar radiation, the direct normal irradiance Ion on a horizontal surface at a zenith angle Equation at mean sunearth distance by including the correction factor called eccentricity Equation can be given by Iqbal [6]:

Equation (21)

Where the eccentricity Equation correction factor related to the number n of days in the year is given by:

Equation (22)

Therefore, the total global irradiance IT on a horizontal surface from direct irradiance and diffused irradiance Id from surrounding environment can be written as follows:

Equation (23)

The Id can be further written as:

Equation

The broadband diffuse irradiance Idr under a cloudless sky as the effect of Rayleigh scattering is given as

Equation (25)

On the other hand, the diffuse irradiance scattering because of aerosol-scattered diffuse radiation Ida reaching the ground after the first pass through the atmosphere is given as

Equation (26)

Where Fc is symbolized for forward scattering, Equation is symbolized for the single scattering albedo by Iqbal, which is the ratio of energy scattered by aerosol to the total attenuation under primarily incident by the direct radiation. In this paper a value of Equation [6] was taken for the computation. The determination of Equation is experimentally a troublesome, according to Iqbal [6]. However, a few amount of aerosol particles in rural environment usually scattered than those found in the urban-industrial area [6,8]. During solar irradiance modeling Equation= 0.6, by Iqbal [6] is used for urban-industrial region where as Equation= 0.9 [6,8] is used for agricultural region. Since the study location is widely known as the rural and agricultural center, so Equation= 0.9 was applied in the solar radiation modeling. The horizontal visibility (Vis) for greater than 5 km, Ångström turbidity factorβ , and wavelength exponent α are related as:

Equation (27)

The wavelength exponent α = 1.3 in Equations (27) and (28) was used in the computation according to Iqbal [6]. The aerosol transmittance τa' computed using air-mass m'a, Ångström turbidity factor β , and wavelength exponent α is:

Equation (28)

Where m'a is the relative aerosol mass at the local station calculated as:

Equation (29)

The downward irradiance Idm because of multiple reflections between the ground and the atmosphere is computed as:

Equation (30)

Where ρg is the ground albedo and ρg ′ is cloudless sky albedo. The value of ground albedo for variation of multiply reflected irradiance lies between 0.2 and 0.7 according to Iqbal [6]. On another reference, the ground albedo varied between 0.1 and 0.25 for agricultural and grassland is written in Encyclopedia of Soil Science. In this paper 0.25 ρg = was used for computing the downward irradiance Idm due to multiple reflections between the ground and the atmosphere. The cloudless sky albedo a ρ ′ is computed as Figures 1 and 2

earth-science-climatic-precipitable-water

Figure 1: The estimation of precipitable water vapor w using Equations 3 and 4.

earth-science-climatic-Ground-measurement

Figure 2: Ground measurement of GSR.

Equation (31)

Results and Discussion

Determination of linked turbidity factor TL

The influence of TL on GSR at site were evaluated by Inman and Becker [9,10]:

Equation (32)

Where Equation is the Rayleigh optical thickness. IT was employed in evaluating TL were referenced by Inman [9]:

Its equation is represented as:

Equation (33)

Equation (34)

The Equation is computed according the condition set by Wang, Chen, Niu, Salazar [11]. According to them Equation is to be greater than 100, Ion is to be greater than 200 W/m2 and the Equation is to be less than 20.

Equation (35)

The TL illustrated on Figures 3-7 is from modeled GSR oscillated between 4.2 and 8.2 with its mean value about 6.2. The TL from GSR of ground measurement is oscillated between 3.6 and 8.4 with mean value 6.16.

earth-science-climatic-Model-GSR

Figure 3: Model GSR.

earth-science-climatic-Model-GSR

Figure 4: Comparison of mean, modal, median, and 15th day (January 2016) of ground measurement with model GSR.

earth-science-climatic-ground-measurement

Figure 5: Mean daily GSR from modelling, ground measurement and satellite reading.

earth-science-climatic-ground-measurement

Figure 6: The TL from GSR modelling and ground measurement.

earth-science-climatic-Daily-determination

Figure 7: Daily determination of L T ’s with their means (model, measurement and satellite).

The statistical tools for evaluating hydrological model assessment widely discussed by Krause, Boyle, Bäse [12], where applicable for evaluating the model efficiency in determining TL . These are: Root Means Squared Error RMSE, Nash-Sutcliffe efficiency E and its relative efficiency criteria Er, index agreement d and its relative efficiency criteria dr and coefficient of determination R2.

An efficiency of 0 indicates that the model predictions are as accurate as the mean of the observed data, whereas an efficiency less than zero ( −∞ < E < 0) occurs when the observed mean is a better predictor than the model. Essentially, the closer the model efficiency is to 1; the model is becoming more accurate. On the other statistical explanation on modeling, the coefficient of determination R2 ranging between 0.33 and 0.66 would have moderate explanatory power [13].

As IT is seen in Figure 7 the daily TL from model GSR is smoothly varied between 6.02 and 6.34 with mean 6.22. However, the daily TL from ground GSR is considerably varied between 3.62 and 8.36 with the daily mean ranging between 5.77 and 6.71. The daily TL from satellite GSR is also dramatically varied between 3.51 and 8.02 with daily mean lies between 5.12 and 6.01.

Conclusion

The model GSR for the study is computed from integrated atmospheric parameters such as optical thickness, optical air mass, and ozone layer, the amount of aerosol effect, perceptible water vapor, climate data, solar geometry and geographical positions. This rise of Like’s turbidity factor is an outcome of the suspension of particulate matters, smokes and water droplet in the atmosphere. The area’s proximity to Sahel and Arabia Peninsula, large influx of dusts can stream in to IT . Maritime moisture from Red Sea and Indian Ocean combined with the dusts, particulate matters from local industries, smokes from traditional energy consumption patterns may bring the turbidity factors to the pollution level assisted through local and global wind system transport. These would have consistent pressure on the sustainability of water, air, and soil quality in the area. The TL from the model, ground and satellite GSR is approximately in a close agreement varied between 4 and 8 with the daily average 6 point. This rise of TL is approximately laid in the range between 20% to 37.5% as compared to TL of tropical warm air (continental) in 1947 as discussed by Becker [10]. The result is almost in closer agreement with the analysis made in other continent (Asia) by Wang, Chen, Niu and Salazar [11], Computing the Like’s atmospheric turbidity is an important procedure for early warning on monitoring air, water, soil quality for stability of healthy ecosystem.

Acknowledgments

The author appreciates and acknowledges heartily the teams in Africa Rising for providing meteorology data to academic researchers.

References

  1. Marif Y, Bechki D, Zerrouki M, Belhadj MM, Bouguettaia H (2017) Estimation of atmospheric turbidity over Adrar city in Algeria. Journal of King Saud 17: 1333-1317.
  2. Abdelrahman MA, Said SAM, Shuaib AN (1988) Comparison between atmospheric turbidity coefficients of desert and temperate climates. Solar Energy 40: 219-225.
  3. Fuzzi S, Baltensperger U, Carslaw K, Decesari S, Denier Van DGH (2015) Particulate matter, air quality and climate: Lessons learned and future needs. Atmospheric chemistry and physics 15: 8217-8299.
  4. Engelbrecht JP, Derbyshire E (2010) Airborne mineral dust. Elements 6: 241-246.
  5. Kemal SA (2017) Africa rising Ethiopia highlands final technical report January 2012 September 2016.
  6. Gueymard CA (2005) Importance of atmospheric turbidity and associated uncertainties in solar radiation and luminous efficacy modelling. Energy 30: 1603-1621.
  7. Fraser RS, Kaufman YJ (1985) The relative importance of aerosol scattering and absorption in remote sensing. IEEE Transactions on Geoscience and Remote Sensing 5: 625-633.
  8. Inman RH, Edson JG, Coimbra CF (2015) Impact of local broadband turbidity estimation on forecasting of clear sky direct normal irradiance. Solar Energy 117: 125-138.
  9. Becker S (2001) Calculation of direct solar and diffuse radiation in Israel. International Journal of Climatology 21: 1561-1576.
  10. Wang L, Chen Y, Niu Y, Salazar GA (2017) Analysis of atmospheric turbidity in clear skies at Wuhan, Central China. Journal of Earth Science 28: 729-738.
  11. Krause P, Boyle DP, Bäse F (2005) Comparison of different efficiency criteria for hydrological model assessment. Advances in geosciences 5: 89-97.
  12. Huang CC, Wang YM, Wu TW, Wang PA (2013) An empirical analysis of the antecedents and performance consequences of using the moodle platform. International Journal of Information and Education Technology 3: 217.

Citation: Ambaye C (2018) Determination of Linke’s Turbidity Factors from Model and Measure Solar Radiations in the Tropics Over Highland of South-East Ethiopia. J Earth Sci Clim Change 9: 479. DOI: 10.4172/2157-7617.1000479

Copyright: © 2018 Ambaye C. This is an open-access article distributed under the terms of the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original author and source are credited.

Top