This is our submission for the SciChallenge project.
The topic we chose to talk about is climate change. We talk about the consequences and also how to help prevent them.
#scichallenge2017
Climate change is the current rapid warming of the Earth's climate caused by human activity. If left unchecked (and current responses are doing little to halt it) it poses an unprecedented threat to human civilisation and the ecosystems on this planet. Discover the causes and effects of climate change, but also solutions to reduce it. Find out how you can take action to save the environment. Find out how you can take action to save the environment.
Climate change is the current rapid warming of the Earth's climate caused by human activity. If left unchecked (and current responses are doing little to halt it) it poses an unprecedented threat to human civilisation and the ecosystems on this planet. Discover the causes and effects of climate change, but also solutions to reduce it. Find out how you can take action to save the environment. Find out how you can take action to save the environment.
AAUW St. George UT Branch Member Candice Hansen-Koharcheck, PhD, gave a presentation on "Climate Change: Scientific Fact vs. Political Fiction" at the March 2015 luncheon. Candice is a senior research scientist at the Planetary Science Institute who works on NASA un-manned (robotic) spacecraft missions. She has a Ph.D. in Planetary Science. Currently she is a member of the flight teams for the Cassini spacecraft, in orbit around Saturn, the Mars Reconnaissance Orbiter, at Mars, and the Juno mission, headed to Jupiter, from her office in St. George.
AAUW St. George UT Branch Member Candice Hansen-Koharcheck, PhD, gave a presentation on "Climate Change: Scientific Fact vs. Political Fiction" at the March 2015 luncheon. Candice is a senior research scientist at the Planetary Science Institute who works on NASA un-manned (robotic) spacecraft missions. She has a Ph.D. in Planetary Science. Currently she is a member of the flight teams for the Cassini spacecraft, in orbit around Saturn, the Mars Reconnaissance Orbiter, at Mars, and the Juno mission, headed to Jupiter, from her office in St. George.
This is the introduction to the course 'Climate Change and Global Environment' conducted at the Faculty of Social Sciences and Humanities, Rajarata University of Sri Lanka
a change in global or regional climate patterns, in particular a change apparent from the mid to late 20th century onwards and attributed largely to the increased levels of atmospheric carbon dioxide produced by the use of fossil fuels.
a change in global or regional climate patterns, in particular a change apparent from the mid to late 20th century onwards and attributed largely to the increased levels of atmospheric carbon dioxide produced by the use of fossil fuels.
Social climate change & water crisisIan Mohammed
this z a ppt on climate change and water crisis
well, I would actually say that a few slides in da climate change r frm other ppt's bt most dem were searched by myself.
in da water crisis also I hv done da same....
for more info;s I hv also made a page of IMPORTANT references..
thank u
hope u'd lyk it
comment below
slide 1:Topic Name[climate change(it's cause and effects)]
Presented by Bisma
slide 2: Contents
Introduction
What is climate change?
Why does our climate change?
Factors that affect climate change
What is global warming?
How will climate change affect people?
What can be done to improve our climate?
slide 3:INTRODUCTION
Have you noticed that today, everyone speaks about climate change? Learn from this presentation and be the one who knows best!
Before explaining what climate change is, do you know the difference between weather and climate?
Slide 4:WEATHER & CLIMATE
Weather describes whatever is happening outdoors in a given place at a given time. It is measured through wind, temperature, humidity, atmospheric pressure, cloudiness, and precipitation.
Climate is the average of weather over time. Climate tells us what weather is usually like in a given place.
slide 5: WHAT IS CLIMATE CHANGE?
Climate change is the change in climate over a time period from 10 to 100s of years.
Climate change involves both natural changes and changes caused by people.
slide 6: WHY DOES OUR CLIMATE CHANGE?
Over the history of the planet, the climate has changed naturally. It happened during the ice ages, and maybe also when the dinosaurs disappeared.
In addition, human activities have warmed the climate.
slide 7: FACTORS THAT AFFECT CLIMATE CHANGE:
>NATURAL FACTORS
SUN,VALCANOES
>HUMAN FACTORS
GREENHOUSE GASES,AEROSOLS,DEFORESTATION
slide 8: THE SUN
The amount of energy coming off the Sun is not constant but keeps changing
Slow changes in the Earth's distance from the Sun affect the amount of energy received from the Sun.
Those variations are believed to be one of the causes that start ice ages.
slide 9: THE VOLCANOES
Volcanoes - when a volcano erupts it throws out large amounts of sulphur dioxide (SO2), water vapour, dust, and ash into the atmosphere.
slide 10:GREENHOUSE GASES
Human activities send gases (for example methane, carbon dioxine CO2) into the atmosphere that enhance the greenhouse effect. Many of the gases come from fossil fuels such as oil, coal and natural gas to run vehicles, and generate electricity for industries or households.
When the atmosphere contains too much of those gases, the whole atmosphere and the Earth becomes hotter, like it does in a greenhouse. The atmosphere holds on to too much heat, instead of letting it escape into space.
This causes global warming !
slide 11: picture depicting green house effect
slide 12: AEROSOLS
Aerosols are tiny solid particles or liquid droplets that remain suspended in the atmosphere for a long time.
slide 13: DEFORESTATION
slide 14: WHAT IS GLOBAL WARMING
slide 15: HOW WILL CLIMATE CHANGE AFFECT PEOPLE?
slide 16: WHAT CAN WE DO TO IMPROVE OUR CLIMATE?
slide 17: Thank you slide
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.
This pdf is about the Schizophrenia.
For more details visit on YouTube; @SELF-EXPLANATORY;
https://www.youtube.com/channel/UCAiarMZDNhe1A3Rnpr_WkzA/videos
Thanks...!
Earliest Galaxies in the JADES Origins Field: Luminosity Function and Cosmic ...Sérgio Sacani
We characterize the earliest galaxy population in the JADES Origins Field (JOF), the deepest
imaging field observed with JWST. We make use of the ancillary Hubble optical images (5 filters
spanning 0.4−0.9µm) and novel JWST images with 14 filters spanning 0.8−5µm, including 7 mediumband filters, and reaching total exposure times of up to 46 hours per filter. We combine all our data
at > 2.3µm to construct an ultradeep image, reaching as deep as ≈ 31.4 AB mag in the stack and
30.3-31.0 AB mag (5σ, r = 0.1” circular aperture) in individual filters. We measure photometric
redshifts and use robust selection criteria to identify a sample of eight galaxy candidates at redshifts
z = 11.5 − 15. These objects show compact half-light radii of R1/2 ∼ 50 − 200pc, stellar masses of
M⋆ ∼ 107−108M⊙, and star-formation rates of SFR ∼ 0.1−1 M⊙ yr−1
. Our search finds no candidates
at 15 < z < 20, placing upper limits at these redshifts. We develop a forward modeling approach to
infer the properties of the evolving luminosity function without binning in redshift or luminosity that
marginalizes over the photometric redshift uncertainty of our candidate galaxies and incorporates the
impact of non-detections. We find a z = 12 luminosity function in good agreement with prior results,
and that the luminosity function normalization and UV luminosity density decline by a factor of ∼ 2.5
from z = 12 to z = 14. We discuss the possible implications of our results in the context of theoretical
models for evolution of the dark matter halo mass function.
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.
Deep Behavioral Phenotyping in Systems Neuroscience for Functional Atlasing a...Ana Luísa Pinho
Functional Magnetic Resonance Imaging (fMRI) provides means to characterize brain activations in response to behavior. However, cognitive neuroscience has been limited to group-level effects referring to the performance of specific tasks. To obtain the functional profile of elementary cognitive mechanisms, the combination of brain responses to many tasks is required. Yet, to date, both structural atlases and parcellation-based activations do not fully account for cognitive function and still present several limitations. Further, they do not adapt overall to individual characteristics. In this talk, I will give an account of deep-behavioral phenotyping strategies, namely data-driven methods in large task-fMRI datasets, to optimize functional brain-data collection and improve inference of effects-of-interest related to mental processes. Key to this approach is the employment of fast multi-functional paradigms rich on features that can be well parametrized and, consequently, facilitate the creation of psycho-physiological constructs to be modelled with imaging data. Particular emphasis will be given to music stimuli when studying high-order cognitive mechanisms, due to their ecological nature and quality to enable complex behavior compounded by discrete entities. I will also discuss how deep-behavioral phenotyping and individualized models applied to neuroimaging data can better account for the subject-specific organization of domain-general cognitive systems in the human brain. Finally, the accumulation of functional brain signatures brings the possibility to clarify relationships among tasks and create a univocal link between brain systems and mental functions through: (1) the development of ontologies proposing an organization of cognitive processes; and (2) brain-network taxonomies describing functional specialization. To this end, tools to improve commensurability in cognitive science are necessary, such as public repositories, ontology-based platforms and automated meta-analysis tools. I will thus discuss some brain-atlasing resources currently under development, and their applicability in cognitive as well as clinical neuroscience.
What is greenhouse gasses and how many gasses are there to affect the Earth.moosaasad1975
What are greenhouse gasses how they affect the earth and its environment what is the future of the environment and earth how the weather and the climate effects.
A brief information about the SCOP protein database used in bioinformatics.
The Structural Classification of Proteins (SCOP) database is a comprehensive and authoritative resource for the structural and evolutionary relationships of proteins. It provides a detailed and curated classification of protein structures, grouping them into families, superfamilies, and folds based on their structural and sequence similarities.
Multi-source connectivity as the driver of solar wind variability in the heli...Sérgio Sacani
The ambient solar wind that flls the heliosphere originates from multiple
sources in the solar corona and is highly structured. It is often described
as high-speed, relatively homogeneous, plasma streams from coronal
holes and slow-speed, highly variable, streams whose source regions are
under debate. A key goal of ESA/NASA’s Solar Orbiter mission is to identify
solar wind sources and understand what drives the complexity seen in the
heliosphere. By combining magnetic feld modelling and spectroscopic
techniques with high-resolution observations and measurements, we show
that the solar wind variability detected in situ by Solar Orbiter in March
2022 is driven by spatio-temporal changes in the magnetic connectivity to
multiple sources in the solar atmosphere. The magnetic feld footpoints
connected to the spacecraft moved from the boundaries of a coronal hole
to one active region (12961) and then across to another region (12957). This
is refected in the in situ measurements, which show the transition from fast
to highly Alfvénic then to slow solar wind that is disrupted by the arrival of
a coronal mass ejection. Our results describe solar wind variability at 0.5 au
but are applicable to near-Earth observatories.
2. What is climate
change?
Climate change is a large-scale,
long-term shift in the planet's
weather patterns or average
temperatures. This could be a
change in how much rain a place
usually gets in a year or the
change of the place's usual
temperature for a month or season.
2
3. The topics below are the main pieces of evidence for
climate change:
3
• Higher temperatures: Since the last ice
age, which ended about 11,000 years
ago, Earth's climate has been relatively
stable at about 14 °C. However, in recent
years, the average temperature has been
increasing.
• Changing Rainfall: In some areas there
has been observed an increase in winter
rainfalls and a decrease in summer.
There is also evidence that the heavy
rainfalls have become more intense in a
lot of places, especially in North America.
4. • Sea Level Rises: Since the 20th century sea levels have risen by
about 19cm globally.
• Retreating glaciers: Glaciers all over the world, Alps, Rockies, Andes,
Himalayas, Africa and Alaska are melting at a extremely fast rate
• Ice sheets: The Greenland and Antarctic ice sheets (Which store the
majority of the world's fresh water) are both shrinking at an accelerating
rate.
22 de julho de 2012 Texto de rodapé aqui4
5. The reasons behind
climate change
The main factor responsible for climate
change is the burning of fossil fuels.
Since the industrial revolution the
amount of coal and oil burnt has vastly
increased and therefore there has been
more and more greenhouse gases
released to the atmosphere (mainly
carbon dioxide).
Texto de rodapé aqui5
6. Other human activities, such as agriculture and
deforestation, directly related with
the decreased carbon storage also contribute to the
proliferation of the greenhouse gases and to the
imbalance of the CO2 we emit and the planet's
capacity to re-absorb it.
7. The amount of CO2 in the atmosphere has increased by about 38% since the Industrial Revolution. This means the
extra CO2 will absorb and emit more and more of the Earth's outgoing radiation, and this will further warm our
climate
As the atmosphere warms, the amount of water vapor it holds also increases
Which further adds to the warming effect
9. Even small increases in Earth's
temperature caused
by the climate change can have
severe effects on our planet:
• Warming ocean temperatures
are associated with stronger
and more frequent storms.
• Rising sea levels due to the
melting of the polar ice caps
contribute to the storm
damage.
• More rainfall during severe
weather events, leads to
flooding and damage.
• An increase in the number and
severity wildfires threatens
habitats, homes and lives. The
resulting heat waves contribute
to more human deaths
9
10. On a global scale, the economists agree that acting to
reduce fossil fuel emissions would be far less expensive
than dealing with the consequences of not doing so.
But how can every single one of us help to save our
planet from fatal consequences and why should we care
about doing it?
How can we stop the climate from changing so quickly?
11. • Climate change affects everyone, humans have adapted to the relatively
stable climate we have enjoyed since the last ice age. The warming of
our climate will affect our water supplies, agriculture, power and
transportation systems and even our own health and safety.
• Our decisions today will shape the world our children will live in.
Everybody can take actions to help reduce the effects. Not only does it
saves the planet but it can also save you money, some can improve our
health, therefore it's in our best interest to help:
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12. 1
1.Turn off the lights as you leave
the room and also replace the
light bulbs with energy-efficient
fluorescent bulbs.
2.Walk or bike whenever possible.
When travelling long distances, try
to take a train or bus rather than
flying or driving.
3.Conserve water by fixing drips
and leaks. Try to speed shower
and also turn off water when
brushing your teeth.
4.Wash clothes in cold water and
hang clothing to dry outside or
inside on a drying rack
13. 5. When buying appliances, look for high efficiency units.
6.Recycle and repurpose old items
7. When gardening, choose plants that require minimal watering
and better yet plant a tree!
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