The ozone layer is formed in the stratosphere when solar radiation breaks oxygen molecules into oxygen atoms below 240nm wavelengths. The oxygen atoms then combine with oxygen molecules to form ozone molecules in an exothermic reaction where an inert substance absorbs excess energy to prevent ozone decomposition. Ozone is an unstable blue gas that decomposes into oxygen at high temperatures but acts as a powerful oxidizer and reducer in chemical reactions due to its unstable nature.
Atmospheric ozone protects the Earth and its inhabitants from the harmful ultraviolet radiation of the Sun. Without this protective layer, more ultraviolet radiation would reach the surface of the Earth and cause damage to plant, animal and human life. This module explains the importance of ozone, the causes of its depletion and the effects expected on earth's systems.
This presentation is about Ozone Layer and chemicals known to cause its depletion.
It also covers information about Ozone Hole and Correlation between Ozone depletion and skin diseases due to Ultra Violet light.It also contains no. of ways to limit ozone deterioration.
The PPT Brief About the Ozone Layer?,
Where it is located?,
Why It is Important?
Why it is depleting?,
What are the effects of the Ozone Depletion?,
What to be done to save the ozone layer ?.
Stratosphere System Overview Big Data Beers Berlin. 20.11.2013Robert Metzger
Stratosphere is the next generation big data processing engine.
These slides introduce the most important features of Stratosphere by comparing it with Apache Hadoop.
For more information, visit stratosphere.eu
Based on university research, it is now a completely open-source, community driven development with focus on stability and usability.
Atmospheric ozone protects the Earth and its inhabitants from the harmful ultraviolet radiation of the Sun. Without this protective layer, more ultraviolet radiation would reach the surface of the Earth and cause damage to plant, animal and human life. This module explains the importance of ozone, the causes of its depletion and the effects expected on earth's systems.
This presentation is about Ozone Layer and chemicals known to cause its depletion.
It also covers information about Ozone Hole and Correlation between Ozone depletion and skin diseases due to Ultra Violet light.It also contains no. of ways to limit ozone deterioration.
The PPT Brief About the Ozone Layer?,
Where it is located?,
Why It is Important?
Why it is depleting?,
What are the effects of the Ozone Depletion?,
What to be done to save the ozone layer ?.
Stratosphere System Overview Big Data Beers Berlin. 20.11.2013Robert Metzger
Stratosphere is the next generation big data processing engine.
These slides introduce the most important features of Stratosphere by comparing it with Apache Hadoop.
For more information, visit stratosphere.eu
Based on university research, it is now a completely open-source, community driven development with focus on stability and usability.
this ppt is mainly for the students of grade 7 igcse
go ahead,have a look!
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just comment whichever ppt you want next and it will be ready for u!
-proud dsrvian
Dr. Kostas Tzoumas: Big Data Looks Tiny From Stratosphere at Big Data Beers (...stratosphere_eu
Presentation by Dr. Kostas Tzoumas at the Big Data Beers Meetup [1] (Nov. 20, 2013) introducing the Stratosphere Platform for Big Data Analytics.
Check out http://stratosphere.eu for more information.
[1] http://www.meetup.com/Big-Data-Beers/events/147397982/
Montreal Protocol and Ozone Layer DepletionBaral Pradeep
This presentation provides comprehensive information about Ozone, Ozone Layer, Ozone Layer Depletion, International Initiatives and Analysis of Montreal Protocol.
exotic breeds
.Based on the place of origin (Standard or official classification)
.Based on utility, economics or commercial value
Turkey breeds, quail varieties, duck breeds, comb types
In the stratosphere ozone molecules are absorbing the uvlight. The.pdfakshay1213
In the stratosphere ozone molecules are absorbing the uvlight.
The Oxygen molecules present in the stratosphere will dissociatedto two O atoms by absorbing
uv light photon
O2 + hv ----> O + O
These atomic oxygen then combines with O2to form O3.
This ozone molecules absorb UV light between 300 - 200nm
Now this ozone splits into O2 and anoxygen atom.
O3 + hv ---> O2 + O
The formed oxygen atom then reacts with an oxygen molecule toregenerate ozone.
O2 + O ---> O3
which is a continous process
So the answer is B (O3 )
Solution
In the stratosphere ozone molecules are absorbing the uvlight.
The Oxygen molecules present in the stratosphere will dissociatedto two O atoms by absorbing
uv light photon
O2 + hv ----> O + O
These atomic oxygen then combines with O2to form O3.
This ozone molecules absorb UV light between 300 - 200nm
Now this ozone splits into O2 and anoxygen atom.
O3 + hv ---> O2 + O
The formed oxygen atom then reacts with an oxygen molecule toregenerate ozone.
O2 + O ---> O3
which is a continous process
So the answer is B (O3 ).
Model Attribute Check Company Auto PropertyCeline George
In Odoo, the multi-company feature allows you to manage multiple companies within a single Odoo database instance. Each company can have its own configurations while still sharing common resources such as products, customers, and suppliers.
How to Split Bills in the Odoo 17 POS ModuleCeline George
Bills have a main role in point of sale procedure. It will help to track sales, handling payments and giving receipts to customers. Bill splitting also has an important role in POS. For example, If some friends come together for dinner and if they want to divide the bill then it is possible by POS bill splitting. This slide will show how to split bills in odoo 17 POS.
The Art Pastor's Guide to Sabbath | Steve ThomasonSteve Thomason
What is the purpose of the Sabbath Law in the Torah. It is interesting to compare how the context of the law shifts from Exodus to Deuteronomy. Who gets to rest, and why?
Instructions for Submissions thorugh G- Classroom.pptxJheel Barad
This presentation provides a briefing on how to upload submissions and documents in Google Classroom. It was prepared as part of an orientation for new Sainik School in-service teacher trainees. As a training officer, my goal is to ensure that you are comfortable and proficient with this essential tool for managing assignments and fostering student engagement.
The Roman Empire A Historical Colossus.pdfkaushalkr1407
The Roman Empire, a vast and enduring power, stands as one of history's most remarkable civilizations, leaving an indelible imprint on the world. It emerged from the Roman Republic, transitioning into an imperial powerhouse under the leadership of Augustus Caesar in 27 BCE. This transformation marked the beginning of an era defined by unprecedented territorial expansion, architectural marvels, and profound cultural influence.
The empire's roots lie in the city of Rome, founded, according to legend, by Romulus in 753 BCE. Over centuries, Rome evolved from a small settlement to a formidable republic, characterized by a complex political system with elected officials and checks on power. However, internal strife, class conflicts, and military ambitions paved the way for the end of the Republic. Julius Caesar’s dictatorship and subsequent assassination in 44 BCE created a power vacuum, leading to a civil war. Octavian, later Augustus, emerged victorious, heralding the Roman Empire’s birth.
Under Augustus, the empire experienced the Pax Romana, a 200-year period of relative peace and stability. Augustus reformed the military, established efficient administrative systems, and initiated grand construction projects. The empire's borders expanded, encompassing territories from Britain to Egypt and from Spain to the Euphrates. Roman legions, renowned for their discipline and engineering prowess, secured and maintained these vast territories, building roads, fortifications, and cities that facilitated control and integration.
The Roman Empire’s society was hierarchical, with a rigid class system. At the top were the patricians, wealthy elites who held significant political power. Below them were the plebeians, free citizens with limited political influence, and the vast numbers of slaves who formed the backbone of the economy. The family unit was central, governed by the paterfamilias, the male head who held absolute authority.
Culturally, the Romans were eclectic, absorbing and adapting elements from the civilizations they encountered, particularly the Greeks. Roman art, literature, and philosophy reflected this synthesis, creating a rich cultural tapestry. Latin, the Roman language, became the lingua franca of the Western world, influencing numerous modern languages.
Roman architecture and engineering achievements were monumental. They perfected the arch, vault, and dome, constructing enduring structures like the Colosseum, Pantheon, and aqueducts. These engineering marvels not only showcased Roman ingenuity but also served practical purposes, from public entertainment to water supply.
Students, digital devices and success - Andreas Schleicher - 27 May 2024..pptxEduSkills OECD
Andreas Schleicher presents at the OECD webinar ‘Digital devices in schools: detrimental distraction or secret to success?’ on 27 May 2024. The presentation was based on findings from PISA 2022 results and the webinar helped launch the PISA in Focus ‘Managing screen time: How to protect and equip students against distraction’ https://www.oecd-ilibrary.org/education/managing-screen-time_7c225af4-en and the OECD Education Policy Perspective ‘Students, digital devices and success’ can be found here - https://oe.cd/il/5yV
The Indian economy is classified into different sectors to simplify the analysis and understanding of economic activities. For Class 10, it's essential to grasp the sectors of the Indian economy, understand their characteristics, and recognize their importance. This guide will provide detailed notes on the Sectors of the Indian Economy Class 10, using specific long-tail keywords to enhance comprehension.
For more information, visit-www.vavaclasses.com
1. The formation of the ozone layer
The formation of the ozone in the stratosphere region begins with the
photodissociation of oxygen molecules by the solar radiation at
.wavelengths below 240 nm
O2 O + O
The highly reactive O atoms combine with oxygen molecules to form ozone as
follows :
O3 + MO + O2 + M
M : Some inert substance.
The role of M in this exothermic reaction is to absorb some of the excess
energy released and prevent the spontaneous decomposition of the O3
.molecule
O3 O + O2
UV < 240 nm
UV
2. Some physical properties of ozone
Pure ozone is a blue gas with a strong
irritating smell.
It is more soluble than oxygen in water.
It gets liquefied to a deep blue color liquid,
when cooled in liquid air.
It boils at 161 K and solidifies to violet-black
crystals, which melts at 81 K.
3. Some chemical properties of
ozoneDecomposition:
Ozone is unstable compound. Pure ozone decompose instantaneously at 573
K.
2O3 3O2
Oxidizing property :
Ozone acts as a powerful oxidizing agent due to the reaction :
O3 O2 + O
Reducing property :
Ozone reduces peroxides to oxides and in turn gets reduced to oxygen
H2O2 + O3 H2O + 2O2
573 K