1) Radiation transfers heat through electromagnetic waves without a medium and travels at the speed of light. The amount radiated and wavelengths depend on an object's temperature according to Stefan-Boltzmann and Planck's laws.
2) Solar radiation reaches Earth's surface through reflection, scattering, absorption and transmission in the atmosphere. Gases like ozone and oxygen absorb most harmful UV rays while scattering by air molecules causes blue skies.
3) On Earth's surface, radiation is mostly absorbed and re-emitted, with some reflected depending on surface albedo. The atmosphere emits terrestrial radiation both upwards, lost to space, and downwards to the surface.
Earth's energy budget refers to the tracking of how much energy is flowing into and out of the Earth's climate, where the energy is going, and if the energy coming in balances with the energy going out. The Earth receives energy from the Sun, and it also reflects and radiates energy back into space. All of the energy that warms the atmosphere, oceans and land must be radiated back into space in order to maintain our current climate. If the amount of energy radiating back into space is decreased by even a very small amount, it can lead to warming. It is believed that increasing levels of carbon dioxide in the atmosphere has a 'greenhouse effect' of reducing the amount of energy radiated into space.
Earth's energy budget refers to the tracking of how much energy is flowing into and out of the Earth's climate, where the energy is going, and if the energy coming in balances with the energy going out. The Earth receives energy from the Sun, and it also reflects and radiates energy back into space. All of the energy that warms the atmosphere, oceans and land must be radiated back into space in order to maintain our current climate. If the amount of energy radiating back into space is decreased by even a very small amount, it can lead to warming. It is believed that increasing levels of carbon dioxide in the atmosphere has a 'greenhouse effect' of reducing the amount of energy radiated into space.
Spectral signatures are the specific combination of emitted, reflected or absorbed electromagnetic radiation (EM) at varying wavelengths which can uniquely identify an object. Here, i have focused on the spectral signature of water and the various micro-process that are responsible for it.
Spectral signatures are the specific combination of emitted, reflected or absorbed electromagnetic radiation (EM) at varying wavelengths which can uniquely identify an object. Here, i have focused on the spectral signature of water and the various micro-process that are responsible for it.
Deals anaerobic ponds for the primary treatment of sewage, stabilization of the settled sludge and BOD removal. It also includes design and physical design of the anaerobic ponds.
Deals with primary sedimentation tanks for the primary treatment of sewage. settling column test, settling profile graph construction and use of the settling profile graph for the design of primary sedimentation tank. both circular and rectangular settling tanks are described here.
Deals with the biological removal of nitrogen and phosphorus, Nitrification-denitrification removal of nitrogen, and Phosphate accumulating organisms and poly-hydroxibutirate in the phosphorus removal.
deals with temperature, density, pressure, winds and humidity parameters of the atmosphere; Prssure gradient force, coriolis force, gravity force and friction force and winds and currents, ; pressure lows and highs, atmospheric circulation, winds.
Deals with the primary treatment of sewage specially for the removal of suspended solids and also for the stabilization of the separated solids. treatment, design and performance details of primary clarifiers, anaerobic ponds, UASB reactors, UASB ponds, and baffled anaerobic reactors are covered in this presentation..
This presentation deals with the following appurtenances: Manholes; Flushing tanks, flushing manholes and clean outs; Interceptor tanks; (Inverted) siphons; Pumping stations; Gutters, storm water inlets and catch basins, and Other appurtenances.
Deals with UASB reactors for the primary treatment of sewage, stabilization of sludge and removal of BOD. Various components of a UASB reactor are described and design details are included. Modifications to UASB such as UASB ponds, Anaerobic baffle reactors, migrating blanket reactors are also described here.
Deals with what is activated sludge, mechanisms and kinetics of treatment, design of activated sludge process, secondary clarifiers and their design and bulking sludge, raising sludge and foaming of ASP.
Willie Nelson Net Worth: A Journey Through Music, Movies, and Business Venturesgreendigital
Willie Nelson is a name that resonates within the world of music and entertainment. Known for his unique voice, and masterful guitar skills. and an extraordinary career spanning several decades. Nelson has become a legend in the country music scene. But, his influence extends far beyond the realm of music. with ventures in acting, writing, activism, and business. This comprehensive article delves into Willie Nelson net worth. exploring the various facets of his career that have contributed to his large fortune.
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Introduction
Willie Nelson net worth is a testament to his enduring influence and success in many fields. Born on April 29, 1933, in Abbott, Texas. Nelson's journey from a humble beginning to becoming one of the most iconic figures in American music is nothing short of inspirational. His net worth, which estimated to be around $25 million as of 2024. reflects a career that is as diverse as it is prolific.
Early Life and Musical Beginnings
Humble Origins
Willie Hugh Nelson was born during the Great Depression. a time of significant economic hardship in the United States. Raised by his grandparents. Nelson found solace and inspiration in music from an early age. His grandmother taught him to play the guitar. setting the stage for what would become an illustrious career.
First Steps in Music
Nelson's initial foray into the music industry was fraught with challenges. He moved to Nashville, Tennessee, to pursue his dreams, but success did not come . Working as a songwriter, Nelson penned hits for other artists. which helped him gain a foothold in the competitive music scene. His songwriting skills contributed to his early earnings. laying the foundation for his net worth.
Rise to Stardom
Breakthrough Albums
The 1970s marked a turning point in Willie Nelson's career. His albums "Shotgun Willie" (1973), "Red Headed Stranger" (1975). and "Stardust" (1978) received critical acclaim and commercial success. These albums not only solidified his position in the country music genre. but also introduced his music to a broader audience. The success of these albums played a crucial role in boosting Willie Nelson net worth.
Iconic Songs
Willie Nelson net worth is also attributed to his extensive catalog of hit songs. Tracks like "Blue Eyes Crying in the Rain," "On the Road Again," and "Always on My Mind" have become timeless classics. These songs have not only earned Nelson large royalties but have also ensured his continued relevance in the music industry.
Acting and Film Career
Hollywood Ventures
In addition to his music career, Willie Nelson has also made a mark in Hollywood. His distinctive personality and on-screen presence have landed him roles in several films and television shows. Notable appearances include roles in "The Electric Horseman" (1979), "Honeysuckle Rose" (1980), and "Barbarosa" (1982). These acting gigs have added a significant amount to Willie Nelson net worth.
Television Appearances
Nelson's char
Micro RNA genes and their likely influence in rice (Oryza sativa L.) dynamic ...Open Access Research Paper
Micro RNAs (miRNAs) are small non-coding RNAs molecules having approximately 18-25 nucleotides, they are present in both plants and animals genomes. MiRNAs have diverse spatial expression patterns and regulate various developmental metabolisms, stress responses and other physiological processes. The dynamic gene expression playing major roles in phenotypic differences in organisms are believed to be controlled by miRNAs. Mutations in regions of regulatory factors, such as miRNA genes or transcription factors (TF) necessitated by dynamic environmental factors or pathogen infections, have tremendous effects on structure and expression of genes. The resultant novel gene products presents potential explanations for constant evolving desirable traits that have long been bred using conventional means, biotechnology or genetic engineering. Rice grain quality, yield, disease tolerance, climate-resilience and palatability properties are not exceptional to miRN Asmutations effects. There are new insights courtesy of high-throughput sequencing and improved proteomic techniques that organisms’ complexity and adaptations are highly contributed by miRNAs containing regulatory networks. This article aims to expound on how rice miRNAs could be driving evolution of traits and highlight the latest miRNA research progress. Moreover, the review accentuates miRNAs grey areas to be addressed and gives recommendations for further studies.
Natural farming @ Dr. Siddhartha S. Jena.pptxsidjena70
A brief about organic farming/ Natural farming/ Zero budget natural farming/ Subash Palekar Natural farming which keeps us and environment safe and healthy. Next gen Agricultural practices of chemical free farming.
"Understanding the Carbon Cycle: Processes, Human Impacts, and Strategies for...MMariSelvam4
The carbon cycle is a critical component of Earth's environmental system, governing the movement and transformation of carbon through various reservoirs, including the atmosphere, oceans, soil, and living organisms. This complex cycle involves several key processes such as photosynthesis, respiration, decomposition, and carbon sequestration, each contributing to the regulation of carbon levels on the planet.
Human activities, particularly fossil fuel combustion and deforestation, have significantly altered the natural carbon cycle, leading to increased atmospheric carbon dioxide concentrations and driving climate change. Understanding the intricacies of the carbon cycle is essential for assessing the impacts of these changes and developing effective mitigation strategies.
By studying the carbon cycle, scientists can identify carbon sources and sinks, measure carbon fluxes, and predict future trends. This knowledge is crucial for crafting policies aimed at reducing carbon emissions, enhancing carbon storage, and promoting sustainable practices. The carbon cycle's interplay with climate systems, ecosystems, and human activities underscores its importance in maintaining a stable and healthy planet.
In-depth exploration of the carbon cycle reveals the delicate balance required to sustain life and the urgent need to address anthropogenic influences. Through research, education, and policy, we can work towards restoring equilibrium in the carbon cycle and ensuring a sustainable future for generations to come.
WRI’s brand new “Food Service Playbook for Promoting Sustainable Food Choices” gives food service operators the very latest strategies for creating dining environments that empower consumers to choose sustainable, plant-rich dishes. This research builds off our first guide for food service, now with industry experience and insights from nearly 350 academic trials.
Characterization and the Kinetics of drying at the drying oven and with micro...Open Access Research Paper
The objective of this work is to contribute to valorization de Nephelium lappaceum by the characterization of kinetics of drying of seeds of Nephelium lappaceum. The seeds were dehydrated until a constant mass respectively in a drying oven and a microwawe oven. The temperatures and the powers of drying are respectively: 50, 60 and 70°C and 140, 280 and 420 W. The results show that the curves of drying of seeds of Nephelium lappaceum do not present a phase of constant kinetics. The coefficients of diffusion vary between 2.09.10-8 to 2.98. 10-8m-2/s in the interval of 50°C at 70°C and between 4.83×10-07 at 9.04×10-07 m-8/s for the powers going of 140 W with 420 W the relation between Arrhenius and a value of energy of activation of 16.49 kJ. mol-1 expressed the effect of the temperature on effective diffusivity.
Artificial Reefs by Kuddle Life Foundation - May 2024punit537210
Situated in Pondicherry, India, Kuddle Life Foundation is a charitable, non-profit and non-governmental organization (NGO) dedicated to improving the living standards of coastal communities and simultaneously placing a strong emphasis on the protection of marine ecosystems.
One of the key areas we work in is Artificial Reefs. This presentation captures our journey so far and our learnings. We hope you get as excited about marine conservation and artificial reefs as we are.
Please visit our website: https://kuddlelife.org
Our Instagram channel:
@kuddlelifefoundation
Our Linkedin Page:
https://www.linkedin.com/company/kuddlelifefoundation/
and write to us if you have any questions:
info@kuddlelife.org
1. Radiation and Atmospheric Temperature
Dr. Akepati S. Reddy
School of Energy & Environment
Thapar University, Patiala
2. Radiation
• Electromagnetic waves (exhibit the characteristics of both electric
field and magnetic field)
– No medium is required for this mode of heat transfer (best in vacuum)
– Moves at the speed of light - spreads in all directions in straight lines
• Described by wavelength, frequency and velocity (relationship
among these: λ . V = C)
– ‘C’ speed of light: 299 792 458 m/s (3.0 x 108 m/s)
• Amount radiated and wavelength composition of the radiation
depends on the emission temperature of the object
– Stefen – Boltzmann law (radiation emitted is proportional to T4)
– Planck’s law (ideal emission spectrum or curve)
– Wein’s displacement law (λmax is object’s temperature dependent)
• Radiation spectrum: spectral distribution of radiative energy (over
different wavelengths)
• Black body (absorbs all the incident radiation) is an ideal emitter
(emissivity factor is 1.0) – grey bodies have <1.0 emissivity
3. Wein’s displacement law:
The wavelength (λmax) at which spectral radiance of a black body peaks
T
b
max
b is a constant of proportionality ( Wien's
displacement constant): 2.8977729×10−3 m K
T is absolute temperature
Stefen – Boltzman law
Total radiation emitted by a black body is proportional to the fourth
power of its absolute temperature.
I = irradiance per unit time per unit are (W/m2)
ε = Emissivity (for black body ε = 1)
σ (Stefan-Boltzmann Constant) = 5.6703 10-8 (W/m2K4)
T = absolute temperature in Kelvin (K)
I = εσ T4 A
4232
45
m
W
15
2
KhC
k
Planck’s law
Describes spectral density of radiation emitted by a black body
Bλ(λ,K) is spectral radiance at λ wavelength and K
temperature (W/m2- (λ,K))
kB (Stefan-Boltzmann Constant) = 5.6703 10-8 (W/m2K4)
C (speed of light) = 3.0 x 108 m/s
‘h’ (Planck’s constant) = 6.626196 10-34 W
4.
5. Radiation
• Radiation is divisible into shortwave and longwave radiations
– Shortwave radiation (<1500 nm) includes UV, visible and near IR
– Longwave radiation (>1.5 μm) includes far IR and microwave
• Fate of radiation includes reflection, scattering, absorption and
transmission
• Absorption of radiation increases molecular motion, heating and
increases the temperature
– Earth is almost a black body, but gases are not – gases are selective
absorbers and emitters
– A substance, which is an efficient emitter in a given wavelength range,
will also be efficient absorber at the same wavelength range
• Radiations types:
– Solar radiation (Extra-terrestrial solar radiation and solar radiation
reaching the earth surface)
– Terrestrial radiation from the earth surface
– Terrestrial radiation from the atmosphere
6.
7. Extra Terrestrial Solar Radiation
• Spectral characteristics
– Max. spectral density (λmax.) is at 480 nm (green of visible spectrum)
– 6.4% is UV radiation (<380 nm), 45.6% is Infrared radiation (>780 nm),
and the rest 48% is visible radiation (380 to 780 nm)
• Energy content
– Solar constant, GSC (extraterrestrial solar radiation received at the
mean earth-sun distance of 1.495 x 1011 m): 1367 w/m2
– The Earth – the Sun geometry is responsible for spatial and temporal
variations in the extra terrestrial solar radiation
– Varies with the time of the day (earth’s rotation), season and latitude
(tilt of the earth and Earth’s revolution around sun in the orbit)
– Earth receives 6.7% more radiation during Perihilion (3rd Jan – earth is
closest to sun) than during Aphilion (4th July – earth is farthest to sun)
– On equinox (vernal/spring & autumnal/fall) days (23rd March & 22nd
Sep.) everywhere on earth, day length and night length are equal
– Day length is maximum during the summer solstice (June 21st) and
minimum during the winter solstice (December 21st)
– On a summer solstice day, the arctic cicle (>66.5 N) experiences 24
hours day light and on winter solctice day no day light at all
8.
9.
10.
11. Fate of Solar Radiation
Solar radiation while passing through the atmosphere is affected by
reflection/scattering and absorption
Reflection and scattering
• Reflection (albedo) is redirection of radiation by surfaces
• Radiation reflection varies with cloud cover, particulate matter in
air, angle of incidence of sun rays, and types of surfaces
• Gas molecules and small particles/droplets of the atmosphere
cause scattering
• Air molcules (nitrogen and oxygen) scatter shortwave radiation in
the blue-violet region in all the directions
– Diffused radiation from scattering is responsible for the blue sky
• Particles/aerosols (water and ice crystalls of clouds) scatter all
wavelengths equally
– scattering is more forward than backward and hence clouds, fog, haze,
etc. Appear while, grey or milky
12. Fate of the Solar Radiation
Absorption and transmission
• Clouds atmospheric gases and aerosols absorb solar radiation
• Ozone and oxygen are UV absorbers
– Ozone screens all the UV-C radiation and most of the UV-B radiation
and about half of the UV-A radiation
• None of the atmospheric constituents are visible range absorbers
(atmospheric visible range window: 0.3 to 0.9 μm)
Atmosphere is considered as transparent for solar radiation
• Under clear sky conditions as much as 55% of the solar radiation is
transmitted through the atmosphere and reach earth surface
– Overcast (cloud) conditions and aerosols through reflecting reduce the
direct solar radiation reaching the earth surface to as low as 4%
• Direct solar radiation reaching the earth surface is attenuated, and
have altered spectral characteristics
– The direct radiation has mostly the red light (sun appears red during
the sunset and the sunrise)
Atmosphere emits terrestrial radiation –radiation emitted upwards is
lost to space – radiation emitted downward reaches earth surface
14. Fate of the Solar Radiation
• Earth behaves like a black body and mostly absorbs the radiation
received (some fraction is reflected – albedo)
– Direct solar radiation
– Diffused solar radiation
– Terrestrial radiation from the atmosphere above
• Surface albedoes are different for different surfaces
– Fresh snow: 75-95%; sand: 15-45%; forests: 15-55%; grass land: 10-
30%; dry plowed field: 5-20%
• Earth looses energy as
– Terrestrial radiation from the earth surface – 100% longwave radiation
(1.5 to 100 μm)
– Latent heat through evapo-transpiration
– Sensible heat (winds and rising air parcels)
• Atmosphere is opaque for terrestrial radiation (green house effect)
– Some fraction of the radiation however escapes out through an
Atmospheric longwave range window (7-13 μm wavelength range)
– Gases with absorption ranges matching with the window cause global
warming
15.
16. Name Formul a Pre-indust rial
concentration
Current
Concentration
Life-
span
Greenhous e
Potenti al
Water Vapor H2Ov Variable Variable weeks Most
impo rtant
Carbondioxid e CO2 280 ppm 375 ppm 100 yr 1
Methane CH4 700 ppb 1800 ppb 15 yr 21
Nitrous oxides NOx
N2O
275 ppb 315 ppb 100 yr 200
CFCs
Chlo ro-fluoro-carbons
CCF -12 CCl 2F2
0 0.5 ppb 100 yr 15,000
Sul fur hexafluoride SF6 0 0.03 ppb 3000 yr 24,000
17. Terrestrial Radiation and the Atmosphere
• Atmosphere is nearly opaque to terrestrial (longwave) radiation
– Atmosphere absorbs terrestrial radiation from the Earth surface and
radiates back to the earth surface – Earth’s green house effect
– Water vapour strongly absorbs terrestrial radiation at <7 μm
wavelength, carbon dioxide at >12 μm wavelength, and methane near
7 μm wavelength
– Liquid water droplets and ice crystals of clouds are excellent absorbers
of terrestrial radiation
– Earth’s actual temperature is +15C, while expected temperature in the
absence of green house effect is -18C
• Atmospheric longwave range window (7-13 μm) allows vent off of
some energy into space
– While 86% of the terrestrial radiation is absorbed, 14% of the radiation
escapes into space by atmosphere
– Upward terrestrial radiation emitted by the atmospheric gases and
clouds is also ultimately lost to space
• Clouds have net cooling effect during day time and warming effect
at nights in winter months
Heat transfer mechanisms
Radiation
Convection
Conduction
Latent heat (of vapourization)
Heat transfer mechanisms
Radiation
Convection
Conduction
Latent heat (of vapourization)
Rotation is 24 hours
Revolution is in 365.2422 days
Tilt of the earth by 23.5.
Earth receives 6.7% more solar radiation during Perihilion (3rd Jan – earth is closest to sun) than during Aphilion (4th July – earth is farthest to sun)
The axis of rotation of the earth is always in the direction of the north star or polaris.