The document discusses ozone depletion and the ozone layer. It begins with an overview of the earth's atmosphere and ultraviolet radiation. It then discusses ozone, its physical properties, types (stratospheric and tropospheric), and effects on human health. The document outlines how CFCs and other ozone depleting substances cause ozone layer depletion, leading to formation of the ozone hole over Antarctica. This in turn causes effects like increased skin cancer and damage to marine life. The Montreal Protocol was adopted to phase out ozone depleting substances and protect the ozone layer. Individual actions and use of substitutes can also help mitigate ozone depletion.
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 ?.
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 ?.
very easy and best ppt on ozone layer..
you ca understand easily about ozone layer..
it will be some what helpful for you..
i have describe about each basic points accoring to me..
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.
Ozone (O3) is a molecule made up of three atoms of oxygen (O), and very reactive gas.
Bluish gas that harmful to breathe.
Is mostly found in the stratosphere, where it protects us from the Sun’s harmful ultraviolet (UV) radiation.
Although it represents only a tiny fraction of the atmosphere, ozone is essential for life on Earth.
Ozone in the stratosphere— a layer of the atmosphere between 15 and 50 kilometers (10 and 31 miles) above us—acts as a shield to protect Earth’s surface from the sun’s harmful ultraviolet radiation.
This is PPT was presented by Mr. Girishwar of 9th std, JNV Lepakshi, to the INOVIT-2015 organised by Vellore Institute of Technology, Vellore, Tamilnadu on 24-25th Jan 2015.
very easy and best ppt on ozone layer..
you ca understand easily about ozone layer..
it will be some what helpful for you..
i have describe about each basic points accoring to me..
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.
Ozone (O3) is a molecule made up of three atoms of oxygen (O), and very reactive gas.
Bluish gas that harmful to breathe.
Is mostly found in the stratosphere, where it protects us from the Sun’s harmful ultraviolet (UV) radiation.
Although it represents only a tiny fraction of the atmosphere, ozone is essential for life on Earth.
Ozone in the stratosphere— a layer of the atmosphere between 15 and 50 kilometers (10 and 31 miles) above us—acts as a shield to protect Earth’s surface from the sun’s harmful ultraviolet radiation.
This is PPT was presented by Mr. Girishwar of 9th std, JNV Lepakshi, to the INOVIT-2015 organised by Vellore Institute of Technology, Vellore, Tamilnadu on 24-25th Jan 2015.
THE IMPORTANCE OF MARTIAN ATMOSPHERE SAMPLE RETURN.Sérgio Sacani
The return of a sample of near-surface atmosphere from Mars would facilitate answers to several first-order science questions surrounding the formation and evolution of the planet. One of the important aspects of terrestrial planet formation in general is the role that primary atmospheres played in influencing the chemistry and structure of the planets and their antecedents. Studies of the martian atmosphere can be used to investigate the role of a primary atmosphere in its history. Atmosphere samples would also inform our understanding of the near-surface chemistry of the planet, and ultimately the prospects for life. High-precision isotopic analyses of constituent gases are needed to address these questions, requiring that the analyses are made on returned samples rather than in situ.
Observation of Io’s Resurfacing via Plume Deposition Using Ground-based Adapt...Sérgio Sacani
Since volcanic activity was first discovered on Io from Voyager images in 1979, changes
on Io’s surface have been monitored from both spacecraft and ground-based telescopes.
Here, we present the highest spatial resolution images of Io ever obtained from a groundbased telescope. These images, acquired by the SHARK-VIS instrument on the Large
Binocular Telescope, show evidence of a major resurfacing event on Io’s trailing hemisphere. When compared to the most recent spacecraft images, the SHARK-VIS images
show that a plume deposit from a powerful eruption at Pillan Patera has covered part
of the long-lived Pele plume deposit. Although this type of resurfacing event may be common on Io, few have been detected due to the rarity of spacecraft visits and the previously low spatial resolution available from Earth-based telescopes. The SHARK-VIS instrument ushers in a new era of high resolution imaging of Io’s surface using adaptive
optics at visible wavelengths.
Introduction:
RNA interference (RNAi) or Post-Transcriptional Gene Silencing (PTGS) is an important biological process for modulating eukaryotic gene expression.
It is highly conserved process of posttranscriptional gene silencing by which double stranded RNA (dsRNA) causes sequence-specific degradation of mRNA sequences.
dsRNA-induced gene silencing (RNAi) is reported in a wide range of eukaryotes ranging from worms, insects, mammals and plants.
This process mediates resistance to both endogenous parasitic and exogenous pathogenic nucleic acids, and regulates the expression of protein-coding genes.
What are small ncRNAs?
micro RNA (miRNA)
short interfering RNA (siRNA)
Properties of small non-coding RNA:
Involved in silencing mRNA transcripts.
Called “small” because they are usually only about 21-24 nucleotides long.
Synthesized by first cutting up longer precursor sequences (like the 61nt one that Lee discovered).
Silence an mRNA by base pairing with some sequence on the mRNA.
Discovery of siRNA?
The first small RNA:
In 1993 Rosalind Lee (Victor Ambros lab) was studying a non- coding gene in C. elegans, lin-4, that was involved in silencing of another gene, lin-14, at the appropriate time in the
development of the worm C. elegans.
Two small transcripts of lin-4 (22nt and 61nt) were found to be complementary to a sequence in the 3' UTR of lin-14.
Because lin-4 encoded no protein, she deduced that it must be these transcripts that are causing the silencing by RNA-RNA interactions.
Types of RNAi ( non coding RNA)
MiRNA
Length (23-25 nt)
Trans acting
Binds with target MRNA in mismatch
Translation inhibition
Si RNA
Length 21 nt.
Cis acting
Bind with target Mrna in perfect complementary sequence
Piwi-RNA
Length ; 25 to 36 nt.
Expressed in Germ Cells
Regulates trnasposomes activity
MECHANISM OF RNAI:
First the double-stranded RNA teams up with a protein complex named Dicer, which cuts the long RNA into short pieces.
Then another protein complex called RISC (RNA-induced silencing complex) discards one of the two RNA strands.
The RISC-docked, single-stranded RNA then pairs with the homologous mRNA and destroys it.
THE RISC COMPLEX:
RISC is large(>500kD) RNA multi- protein Binding complex which triggers MRNA degradation in response to MRNA
Unwinding of double stranded Si RNA by ATP independent Helicase
Active component of RISC is Ago proteins( ENDONUCLEASE) which cleave target MRNA.
DICER: endonuclease (RNase Family III)
Argonaute: Central Component of the RNA-Induced Silencing Complex (RISC)
One strand of the dsRNA produced by Dicer is retained in the RISC complex in association with Argonaute
ARGONAUTE PROTEIN :
1.PAZ(PIWI/Argonaute/ Zwille)- Recognition of target MRNA
2.PIWI (p-element induced wimpy Testis)- breaks Phosphodiester bond of mRNA.)RNAse H activity.
MiRNA:
The Double-stranded RNAs are naturally produced in eukaryotic cells during development, and they have a key role in regulating gene expression .
Seminar of U.V. Spectroscopy by SAMIR PANDASAMIR PANDA
Spectroscopy is a branch of science dealing the study of interaction of electromagnetic radiation with matter.
Ultraviolet-visible spectroscopy refers to absorption spectroscopy or reflect spectroscopy in the UV-VIS spectral region.
Ultraviolet-visible spectroscopy is an analytical method that can measure the amount of light received by the analyte.
Richard's entangled aventures in wonderlandRichard Gill
Since the loophole-free Bell experiments of 2020 and the Nobel prizes in physics of 2022, critics of Bell's work have retreated to the fortress of super-determinism. Now, super-determinism is a derogatory word - it just means "determinism". Palmer, Hance and Hossenfelder argue that quantum mechanics and determinism are not incompatible, using a sophisticated mathematical construction based on a subtle thinning of allowed states and measurements in quantum mechanics, such that what is left appears to make Bell's argument fail, without altering the empirical predictions of quantum mechanics. I think however that it is a smoke screen, and the slogan "lost in math" comes to my mind. I will discuss some other recent disproofs of Bell's theorem using the language of causality based on causal graphs. Causal thinking is also central to law and justice. I will mention surprising connections to my work on serial killer nurse cases, in particular the Dutch case of Lucia de Berk and the current UK case of Lucy Letby.
Slide 1: Title Slide
Extrachromosomal Inheritance
Slide 2: Introduction to Extrachromosomal Inheritance
Definition: Extrachromosomal inheritance refers to the transmission of genetic material that is not found within the nucleus.
Key Components: Involves genes located in mitochondria, chloroplasts, and plasmids.
Slide 3: Mitochondrial Inheritance
Mitochondria: Organelles responsible for energy production.
Mitochondrial DNA (mtDNA): Circular DNA molecule found in mitochondria.
Inheritance Pattern: Maternally inherited, meaning it is passed from mothers to all their offspring.
Diseases: Examples include Leber’s hereditary optic neuropathy (LHON) and mitochondrial myopathy.
Slide 4: Chloroplast Inheritance
Chloroplasts: Organelles responsible for photosynthesis in plants.
Chloroplast DNA (cpDNA): Circular DNA molecule found in chloroplasts.
Inheritance Pattern: Often maternally inherited in most plants, but can vary in some species.
Examples: Variegation in plants, where leaf color patterns are determined by chloroplast DNA.
Slide 5: Plasmid Inheritance
Plasmids: Small, circular DNA molecules found in bacteria and some eukaryotes.
Features: Can carry antibiotic resistance genes and can be transferred between cells through processes like conjugation.
Significance: Important in biotechnology for gene cloning and genetic engineering.
Slide 6: Mechanisms of Extrachromosomal Inheritance
Non-Mendelian Patterns: Do not follow Mendel’s laws of inheritance.
Cytoplasmic Segregation: During cell division, organelles like mitochondria and chloroplasts are randomly distributed to daughter cells.
Heteroplasmy: Presence of more than one type of organellar genome within a cell, leading to variation in expression.
Slide 7: Examples of Extrachromosomal Inheritance
Four O’clock Plant (Mirabilis jalapa): Shows variegated leaves due to different cpDNA in leaf cells.
Petite Mutants in Yeast: Result from mutations in mitochondrial DNA affecting respiration.
Slide 8: Importance of Extrachromosomal Inheritance
Evolution: Provides insight into the evolution of eukaryotic cells.
Medicine: Understanding mitochondrial inheritance helps in diagnosing and treating mitochondrial diseases.
Agriculture: Chloroplast inheritance can be used in plant breeding and genetic modification.
Slide 9: Recent Research and Advances
Gene Editing: Techniques like CRISPR-Cas9 are being used to edit mitochondrial and chloroplast DNA.
Therapies: Development of mitochondrial replacement therapy (MRT) for preventing mitochondrial diseases.
Slide 10: Conclusion
Summary: Extrachromosomal inheritance involves the transmission of genetic material outside the nucleus and plays a crucial role in genetics, medicine, and biotechnology.
Future Directions: Continued research and technological advancements hold promise for new treatments and applications.
Slide 11: Questions and Discussion
Invite Audience: Open the floor for any questions or further discussion on the topic.
The increased availability of biomedical data, particularly in the public domain, offers the opportunity to better understand human health and to develop effective therapeutics for a wide range of unmet medical needs. However, data scientists remain stymied by the fact that data remain hard to find and to productively reuse because data and their metadata i) are wholly inaccessible, ii) are in non-standard or incompatible representations, iii) do not conform to community standards, and iv) have unclear or highly restricted terms and conditions that preclude legitimate reuse. These limitations require a rethink on data can be made machine and AI-ready - the key motivation behind the FAIR Guiding Principles. Concurrently, while recent efforts have explored the use of deep learning to fuse disparate data into predictive models for a wide range of biomedical applications, these models often fail even when the correct answer is already known, and fail to explain individual predictions in terms that data scientists can appreciate. These limitations suggest that new methods to produce practical artificial intelligence are still needed.
In this talk, I will discuss our work in (1) building an integrative knowledge infrastructure to prepare FAIR and "AI-ready" data and services along with (2) neurosymbolic AI methods to improve the quality of predictions and to generate plausible explanations. Attention is given to standards, platforms, and methods to wrangle knowledge into simple, but effective semantic and latent representations, and to make these available into standards-compliant and discoverable interfaces that can be used in model building, validation, and explanation. Our work, and those of others in the field, creates a baseline for building trustworthy and easy to deploy AI models in biomedicine.
Bio
Dr. Michel Dumontier is the Distinguished Professor of Data Science at Maastricht University, founder and executive director of the Institute of Data Science, and co-founder of the FAIR (Findable, Accessible, Interoperable and Reusable) data principles. His research explores socio-technological approaches for responsible discovery science, which includes collaborative multi-modal knowledge graphs, privacy-preserving distributed data mining, and AI methods for drug discovery and personalized medicine. His work is supported through the Dutch National Research Agenda, the Netherlands Organisation for Scientific Research, Horizon Europe, the European Open Science Cloud, the US National Institutes of Health, and a Marie-Curie Innovative Training Network. He is the editor-in-chief for the journal Data Science and is internationally recognized for his contributions in bioinformatics, biomedical informatics, and semantic technologies including ontologies and linked data.
2. TOPICS TO BEDISCUSSED
What is Ozone?
Types of Ozone.
Effects of Ozone.
Physical and Chemical Properties of Ozone.
Source of Ozone.
Ozone Depletion.
Ozone Hole.
Effects of Ozone Depletion.
How can we protect Ozone?
How can we protect ourselves?
3. Overview of Earth’sAtmosphere
An atmosphere is a layer or layers of gases surrounding a planet
material body of sufficient mass. The earth’s atmosphere is comprised of gases
consisting mostly of nitrogen and oxygen. It also contains lesser amounts of
argon, carbon dioxide, and many other trace gases.
From bottom to top, the layers are:
• The Troposphere
• The Stratosphere
• The Mesosphere
• The Thermosphere
• The Exosphere
The different layers of the atmosphere have contrasting characteristics.
4.
5.
6. Ultraviolet Radiation
• Ultra-violet means “beyond violet” in
Latin since violet is the shortest
wavelength of visible light and UV
light is the next shortest. They are high
energy electromagnetic wave emitted
from the sun. It is made up of
wavelengths ranging from 100nm to
400nm.
• UV radiation include:
iii.
i. UV-A, the least dangerous form of
UV radiation, with a wavelength
range between 315nm to 400nm.
ii. UV-B with a wavelength range
between 280nm to 315nm.
UV-C which is the most dangerous
between 100nm to 280nm. UV-C is
unable to reach Earth’s surface due
to stratospheric ozone’s ability to
absorb it.
• Shorter wavelength meanshigher frequency.
• Higher frequency means higher energy.
7. OZONE
Ozone (O3) is a highly reactive gas composed of
three oxygen atoms. It is both a natural and a
man-made product that occurs in the Earth's
upper atmosphere (the stratosphere) and lower
atmosphere (the troposphere). Depending on
where it is in the atmosphere, ozone affects life
on Earth in either good or bad ways.
Ozone is present in low concentrations
throughout the Earth's atmosphere. In total,
ozone makes up only 0.6 ppm (parts per million)
of the atmosphere.
8. PHYSICAL PROPERTIES
Standard State: Gas
Boling temperature: -111.9 °C
Melting temperature: -195.5 °C
Specific Gravity: 2.144
Color: Colorless OR Pale Blue
Odor: Pungent Smell
• Ozone levels are reported in in Dobson Units (DU)
& 300 DU is an average value.
9. TYPESOF OZONE
Stratospheric Ozone
Stratospheric ozone is formed naturally through the interaction of solar
ultraviolet (UV) radiation with molecular oxygen (O2). The "ozone layer“,
approximately 6 through 30 miles OR 10 through 50 km above the Earth's
surface, reduces the amount of harmful UV radiation reaching the Earth's
surface.
10. TYPESOF OZONE
Tropospheric Ozone
Ozone is also found much nearer the ground, in the troposphere, the lowest level
of Earth’s atmosphere. Unlike the ozone that occurs naturally in the stratosphere,
tropospheric ozone (what webreathe) is man-made.
It is an indirect result of air pollution
created by photochemical reactions
between two major classes of air
pollutants, volatile organic compounds
(VOC) and nitrogen oxides (NOx) which
are present in automobile exhaust and
emissions from factories andpower plants.
11. EFFECTS OF OZONE
Effect of Ozone on Human Health:
1. Stratospheric ozone absorbs UV
light, reducing human exposure to
harmful UV radiation that causes skin
cancer and cataracts.
2. Tropospheric ozone, when inhaled,
reacts chemically with many
biological molecules in the respiratory
tract, leading to a number of adverse
health effects. This makes ozone a
potent respiratory hazard and
pollutant near ground level.
12. STRATOSPHERE OZONE
Ozone Layer
The ozone layer ismainly found in the lower portion of the stratosphere
from approximately 20 to 30 kilometers (12 to 19 miles) above Earth,
though the thickness varies seasonally and geographically. It prevents the
harmful ultraviolet radiations of the sun from reaching the Earth's surface,
and benefits both plants and animals.
The ozone layer can absorb 97–99%of the Sun's medium-frequency
ultraviolet light (from about 200 nm to 315 nm wavelength).
13. Ozone Layer Depletion
• Normal ozone concentration is about 300 to 350 DU
• The term “Ozone hole” is applied over region when stratospheric ozone depletion
is so severe that levels fall below 200 DU.
• Special meteorological conditions and very low air temperatures accelerate and
enhance the destruction of ozone loss by man-made ozone depleting chemicals
(ODCs).
• Ozone loss now occurs every late winter and spring time above Antarctica (South
pole), and to a lesser extent the Arctic (North pole).
19. Net Reaction: O3 + O 2O2
• One chlorine atom from CFC can destroy up to 100,000 ozone atoms in a
catalytic process.
• As a result, continuous deplition of the ozone in the stratospere created the
hole in ozone layer “OZONE HOLE“
Cl+O3
ClO+O
ClO+O2
Cl+O2
23. • Why is an ozone hole formed only above Antarctica and
not over developed countries that emit a lot of CFCs?
CFCs gases takes 6 to 7 years to move up to the stratosphere and the
wind spreads them all around the world. Extreme cold, a freezing
wind, frozen stratospheric clouds and 6-months darkness over Antarctica,
all provides ideal conditions for Chlorine to break from the CFC . The
Chlorine (or Bromine) gasses, then destroy the ozone during spring(Dec)
and causes the formation of ozone holes above Antarctica more than
otherplaces.
24. Effects Of OzoneLayer Depletion
Harm to humanhealth:
Skin cancers, sunburns and premature aging of the skin.
DNA absorbs UV-B radiation and changes its shape. This changes in the DNA results in
mutated cells or the cells die and then cancer.
Note: Scientific evidence suggests that 1%depletion in ozone layer results in 5%increasein skin cancer.
25. Effects OfOzone Layer Depletion
Cataracts, blindness and other eye diseases.
Weakening of the human immune system
26. Effects OfOzone Layer Depletion
Damage tomarine life
Inparticular, plankton (tiny organisms in
the surface layer of oceans) are
threatened by increased UV radiation.
Plankton are the first vital step in aquatic
food chains.
27. Effects OfOzone Layer Depletion
Animals
In domestic animals, UV overexposure may cause eye and skin cancers. Species
of marine animals in their developmental stage (e.g. young fish, shrimp larvae and
crab larvae) have been threatened in recent years by the increased UV radiation
under the Antarctic ozonehole.
Materials
Wood, plastic, rubber, fabrics and many construction materials are degraded by
UV radiation.
The economic impact of replacing and protecting materials could be
significant.
28. MONTREAL PROTOCOL
• After the discovery of ozone depletion in the late 1970’s, many countries agreed
that something must be done worldwide to stop the production of man-
made,ozone harmful products.
• The international community adopted the Vienna Convention in 1985 followed by
the Montreal Protocol in 1987.
• Protocol on substances that deplete the ozone layer was adopted on
16/09/1987,Governments recognized the need for stronger measures to reduce the
production and consumption of CFCs.
• The latest reports confirm that it has led to the phasing out of about 95% of the
consumption of ozone depleting substances (ODS) listed in the
agreement.Inturn,this has led to the prospect of the ozone layer recovering by 2050
to 2075.
29. PROTECT THEENVIRONMENT
What You Can Do about Ozone Layer Depletion?
Established policies that prevent future use of certain
types of chemicals.
Know the rules: It is illegal to recharge refrigerators,
freezers and home/vehicle air conditioners with CFCs.
If you have an older refrigerator or an older vehicle with
an air conditioner, have it serviced by a qualified
technician, and make sure the CFC is recaptured and
recycled by technician who is specifically certified to do
this work.
Don't buy or use portable fire extinguishers that contain
Halogens
Chlorofluorocarbons (CFCs)
Carbon tetrachloride
Methyl chloroform
Hydrochlorofluorocarbons (HCFCs)
30. CFC SUBSTITUTES
• As a safeguard against ozone deplition the recommended CFC substitutes are
1.Hydroalkanes
2.HCFC-22, HCFC -142,HFC 134a, HFC-152a
They have low ozone deplition potential,short tropospheric lifetime.
31. The world started promoting and
adopting products that are ozone
friendly, today we can see that
refrigerators and air conditioners are now
coming with coolant made up of
hydrocarbon and not CFCs. Also in the
aerosol sprays we can find written as
ozone safe, ozone friendly etc
International Ozone day is celebrated
on September 16 every year.
32. There is no doubt that the problem of ozone depletion exists
and deserves extensive research and attention. With the
release of each and every CFC, our ozone layer takes one small
step towards its destruction. The decision to ban completely
CFCs sooner than later cannot be decided by the United States
or even the United Nations. The entire world must unite in
order to expel this problem forever. What can we do, as concerned
citizens, to ensure that our children have a viable planet to inhabit.
CONCLUSIONCONCLUSION