Extinction Rebellion House of Commons climate science presentation
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"OUR HOME IS DYING" was presented to MP's and interested parties in the House of Commons in September 2019 by Extinction Rebellion and an IPCC climate scientist. All credit to Professor Kate Jeffery
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Climate change refers to changes in weather patterns due to human activities like burning fossil fuels and deforestation, which increase greenhouse gases in the atmosphere. This warms the planet and causes the global average temperature to rise. The impacts of climate change include increased mortality rates that could match COVID-19 by 2060 and be five times worse by 2100 if emissions are not reduced. The Paris Agreement aims to limit global warming to well below 2°C by having countries commit to lowering emissions and adapting to climate impacts.
Jennie Stephens - Myra Kraft Open Classroom - October 26, 2016
The document discusses the US role in global environmental governance, with a focus on climate change. It summarizes the US's historical leadership on environmental issues but also periods of lagging behind. It then covers international climate negotiations and agreements from the UNFCCC to the Paris Agreement. It also discusses climate science, denial, and policies of Hillary Clinton and Donald Trump. Renewable energy technology advances are outlined but fossil fuels still dominate global energy.
Understanding Climate Change
Climate change is one of society's greatest threats. This was an overview presentation given on the science and solutions to a student audience at the World Bank on January 15, 2015, to inspire youth to take on climate change. The presentation was given as part of a workshop at which Lucia Grenna introduced the Connect4Climate program and Rachel Kyte, Vice President and Special Envoy for Climate Change at the World Bank, gave a personal account of what is need to take on the challenge, considering that 2015 is such an important year. The students went on do discuss their role for climate action, and brainstormed how best to enhance the Sport4Climate initiative of Connect4Climate.
Decarbonizing cement manufacture 2022.pdf
The document discusses the imperative to decarbonize cement manufacturing. It notes that cement production is a major source of CO2 emissions, which contribute to global warming. Governments and investors have determined that reducing CO2 emissions is necessary to curb rapidly rising global temperatures and the impacts of climate change. While technological solutions for capturing and storing carbon exist, they remain too expensive, and cement companies have not moved quickly enough to commit to science-based emissions reduction targets. Failure to sufficiently decarbonize cement production could deteriorate companies' credit risk as investors increasingly demand evidence of transition pathways to carbon neutrality. Overall, the cement industry must make a major contribution to peaking global greenhouse gas emissions in line with the Paris Agreement goals.
TOO4TO Module 3 / Climate Change and Sustainability: Part 1
This presentation is part of the Sustainable Management: Tools for Tomorrow (TOO4TO) learning materials. It covers the following topic: Climate Change and Sustainability (Module 3). The material consists of 3 parts. This presentation covers Part 1.
You can find all TOO4TO Modules and their presentations here: https://too4to.eu/e-learning-course/
TOO4TO was a 35-month EU-funded Erasmus+ project, running until August 2023 in co-operation with European strategic partner institutions of the Gdańsk University of Technology (Poland), the Kaunas University of Technology (Lithuania), Turku University of Applied Sciences (Finland) and Global Impact Grid (Germany).
TOO4TO aims to increase the skills, competencies and awareness of future managers and employees with available tools and methods that can provide sustainable management and, as a result, support sustainable development in the EU and beyond.
Read more about the project here: https://too4to.eu/
This project has been funded with support from the European Commission. Its whole content reflects the views only of the author, and the Commission cannot be held responsible for any use which may be made of the information contained therein. PROJECT NUMBER 2020-1-PL01-KA203-082076
Climate change
Global warming and energy are interconnected topics that work on the same basis. Generally what causes climate change is burning energy radiated from sun and stored in the earth's crust in the form of fossil fuel. We are giving earth double the amount of energy to release into space. The energy from the sun, and the sun's energy from the past; in the form of energy released from fossil fuel burning. The earth can't radiate heat out as fast as we generate energy. Thus, heat accumulates on earth and temperature rises indicating higher heat content for the planet.
We discuss:
-Day zero.
-The greenhouse effect.
-Svante Arrhenius Nobel prize winner and his discovery.
-Greenhouse gases.
-Different greenhouse gases: H2O, Carbon dioxide, Methane, Nitrous oxide, and Chlorofluorocarbons; We also discuss the difference between their effects and their concentrations.
Events caused by climate change:
-Hurricane Irma.
-South Asia floods.
-East Africa drought.
-Hurricane Harvey.
-Heat wave in India and Pakistan.
-NASA's new map for the world.
United nations legal instruments:
-Kyoto protocol.
-Paris agreement.
-Which countries emit the most greenhouse gas?
Solutions:
-Renewable energy.
-Reduce meat consumption.
-Fix devices instead of buying new one.
-Carbon Foot Print.
Hot mess
Deep Adaptation and the Anthropocene: Man-made Climate Change and the Seeming Inevitability of Near-Term Societal Collapse
Climate Change in Brief by Devashish Negi
This document provides an overview of climate change, its causes and impacts, and potential solutions. It discusses that climate change is caused by human activities like burning fossil fuels which release greenhouse gases and trap heat. This has led to the current Earth surface temperature being 1.1°C warmer than in the late 1800s. Consequences of climate change include increased droughts, fires, flooding and rising sea levels. While climate change affects everyone, vulnerable groups in developing nations face greater risks. The document stresses the need for urgent global action to cut emissions in half by 2030, transition from fossil fuels to renewables, and invest in climate change adaptation measures, in order to limit global warming to 1.5°C and shape a more
Climate change for dummies
This document provides an overview of climate change by discussing:
1. The correlation between CO2 levels and global temperatures over hundreds of thousands of years.
2. How human activities like burning fossil fuels have increased CO2 levels rapidly since the industrial era.
3. The likely effects of increased CO2 and temperatures, such as ocean acidification, rising sea levels, and more extreme weather.
4. International agreements to limit greenhouse gas emissions and actions being taken like carbon taxes and emissions trading schemes.
5. The opportunities to transition to renewable energy but also the political threats if countries do not cooperate to meaningfully address climate change.
Discussions about Climate Change, Impacts and Vulnerability
This document discusses climate change impacts and vulnerabilities in Africa according to discussions by Prof. Richard Odingo from the University of Nairobi. It summarizes that Africa is highly vulnerable to climate change due to factors like poverty, weak institutions, and lack of resources. The IPCC has found evidence that climate change is occurring and will worsen impacts like more frequent droughts and floods in Africa. This poses serious risks to African economies, health, coastlines, and future development prospects if no action is taken.
Similar to Extinction Rebellion House of Commons climate science presentation (20)
Jennie Stephens - Myra Kraft Open Classroom - October 26, 2016
Jennie Stephens - Myra Kraft Open Classroom - October 26, 2016
TOO4TO Module 3 / Climate Change and Sustainability: Part 1
TOO4TO Module 3 / Climate Change and Sustainability: Part 1
Discussions about Climate Change, Impacts and Vulnerability
Discussions about Climate Change, Impacts and Vulnerability
Recently uploaded
Sharlene Leurig - Enabling Onsite Water Use with Net Zero Water
Sharlene Leurig - Enabling Onsite Water Use with Net Zero WaterTexas Alliance of Groundwater Districts
Presented at June 6-7 Texas Alliance of Groundwater Districts Business MeetingMicronuclei test.M.sc.zoology.fisheries.
Current Ms word generated power point presentation covers major details about the micronuclei test. It's significance and assays to conduct it. It is used to detect the micronuclei formation inside the cells of nearly every multicellular organism. It's formation takes place during chromosomal sepration at metaphase.
Compexometric titration/Chelatorphy titration/chelating titration
Classification
Metal ion ion indicators
Masking and demasking reagents
Estimation of Magnisium sulphate
Calcium gluconate
Complexometric Titration/ chelatometry titration/chelating titration, introduction, Types-
1.Direct Titration
2.Back Titration
3.Replacement Titration
4.Indirect Titration
Masking agent, Demasking agents
formation of complex
comparition between masking and demasking agents,
Indicators/Metal ion indicators/ Metallochromic indicators/pM indicators,
Visual Technique,PM indicators (metallochromic), Indicators of pH, Redox Indicators
Instrumental Techniques-Photometry
Potentiometry
Miscellaneous methods.
Complex titration with EDTA.
The binding of cosmological structures by massless topological defects
Assuming spherical symmetry and weak field, it is shown that if one solves the Poisson equation or the Einstein field
equations sourced by a topological defect, i.e. a singularity of a very specific form, the result is a localized gravitational
field capable of driving flat rotation (i.e. Keplerian circular orbits at a constant speed for all radii) of test masses on a thin
spherical shell without any underlying mass. Moreover, a large-scale structure which exploits this solution by assembling
concentrically a number of such topological defects can establish a flat stellar or galactic rotation curve, and can also deflect
light in the same manner as an equipotential (isothermal) sphere. Thus, the need for dark matter or modified gravity theory is
mitigated, at least in part.
Phenomics assisted breeding in crop improvement
As the population is increasing and will reach about 9 billion upto 2050. Also due to climate change, it is difficult to meet the food requirement of such a large population. Facing the challenges presented by resource shortages, climate
change, and increasing global population, crop yield and quality need to be improved in a sustainable way over the coming decades. Genetic improvement by breeding is the best way to increase crop productivity. With the rapid progression of functional
genomics, an increasing number of crop genomes have been sequenced and dozens of genes influencing key agronomic traits have been identified. However, current genome sequence information has not been adequately exploited for understanding
the complex characteristics of multiple gene, owing to a lack of crop phenotypic data. Efficient, automatic, and accurate technologies and platforms that can capture phenotypic data that can
be linked to genomics information for crop improvement at all growth stages have become as important as genotyping. Thus,
high-throughput phenotyping has become the major bottleneck restricting crop breeding. Plant phenomics has been defined as the high-throughput, accurate acquisition and analysis of multi-dimensional phenotypes
during crop growing stages at the organism level, including the cell, tissue, organ, individual plant, plot, and field levels. With the rapid development of novel sensors, imaging technology,
and analysis methods, numerous infrastructure platforms have been developed for phenotyping.
快速办理(UAM毕业证书)马德里自治大学毕业证学位证一模一样
学校原件一模一样【微信：741003700 】《(UAM毕业证书)马德里自治大学毕业证学位证》【微信：741003700 】学位证，留信认证（真实可查，永久存档）原件一模一样纸张工艺/offer、雅思、外壳等材料/诚信可靠,可直接看成品样本，帮您解决无法毕业带来的各种难题！外壳，原版制作，诚信可靠，可直接看成品样本。行业标杆！精益求精，诚心合作，真诚制作！多年品质 ,按需精细制作，24小时接单,全套进口原装设备。十五年致力于帮助留学生解决难题，包您满意。
本公司拥有海外各大学样板无数，能完美还原。
1:1完美还原海外各大学毕业材料上的工艺：水印，阴影底纹，钢印LOGO烫金烫银，LOGO烫金烫银复合重叠。文字图案浮雕、激光镭射、紫外荧光、温感、复印防伪等防伪工艺。材料咨询办理、认证咨询办理请加学历顾问Q/微741003700
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三.真实教育部学历学位认证（教育部存档！教育部留服网站永久可查）
四.办理各国各大学文凭(一对一专业服务,可全程监控跟踪进度)
如果您处于以下几种情况：
◇在校期间，因各种原因未能顺利毕业……拿不到官方毕业证【q/微741003700】
◇面对父母的压力，希望尽快拿到；
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◇回国时间很长，忘记办理；
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◇需要报考公务员、购买免税车、落转户口
◇申请留学生创业基金
留信网认证的作用:
1:该专业认证可证明留学生真实身份
2:同时对留学生所学专业登记给予评定
3:国家专业人才认证中心颁发入库证书
4:这个认证书并且可以归档倒地方
5:凡事获得留信网入网的信息将会逐步更新到个人身份内，将在公安局网内查询个人身份证信息后，同步读取人才网入库信息
6:个人职称评审加20分
7:个人信誉贷款加10分
8:在国家人才网主办的国家网络招聘大会中纳入资料，供国家高端企业选择人才
Equivariant neural networks and representation theory
Or: Beyond linear.
Abstract: Equivariant neural networks are neural networks that incorporate symmetries. The nonlinear activation functions in these networks result in interesting nonlinear equivariant maps between simple representations, and motivate the key player of this talk: piecewise linear representation theory.
Disclaimer: No one is perfect, so please mind that there might be mistakes and typos.
dtubbenhauer@gmail.com
Corrected slides: dtubbenhauer.com/talks.html
Shallowest Oil Discovery of Turkiye.pptx
The Petroleum System of the Çukurova Field - the Shallowest Oil Discovery of Türkiye, Adana
EWOCS-I: The catalog of X-ray sources in Westerlund 1 from the Extended Weste...
Context. With a mass exceeding several 104 M⊙ and a rich and dense population of massive stars, supermassive young star clusters
represent the most massive star-forming environment that is dominated by the feedback from massive stars and gravitational interactions
among stars.
Aims. In this paper we present the Extended Westerlund 1 and 2 Open Clusters Survey (EWOCS) project, which aims to investigate
the influence of the starburst environment on the formation of stars and planets, and on the evolution of both low and high mass stars.
The primary targets of this project are Westerlund 1 and 2, the closest supermassive star clusters to the Sun.
Methods. The project is based primarily on recent observations conducted with the Chandra and JWST observatories. Specifically,
the Chandra survey of Westerlund 1 consists of 36 new ACIS-I observations, nearly co-pointed, for a total exposure time of 1 Msec.
Additionally, we included 8 archival Chandra/ACIS-S observations. This paper presents the resulting catalog of X-ray sources within
and around Westerlund 1. Sources were detected by combining various existing methods, and photon extraction and source validation
were carried out using the ACIS-Extract software.
Results. The EWOCS X-ray catalog comprises 5963 validated sources out of the 9420 initially provided to ACIS-Extract, reaching a
photon flux threshold of approximately 2 × 10−8 photons cm−2
s
−1
. The X-ray sources exhibit a highly concentrated spatial distribution,
with 1075 sources located within the central 1 arcmin. We have successfully detected X-ray emissions from 126 out of the 166 known
massive stars of the cluster, and we have collected over 71 000 photons from the magnetar CXO J164710.20-455217.
The debris of the ‘last major merger’ is dynamically young
The Milky Way’s (MW) inner stellar halo contains an [Fe/H]-rich component with highly eccentric orbits, often referred to as the
‘last major merger.’ Hypotheses for the origin of this component include Gaia-Sausage/Enceladus (GSE), where the progenitor
collided with the MW proto-disc 8–11 Gyr ago, and the Virgo Radial Merger (VRM), where the progenitor collided with the
MW disc within the last 3 Gyr. These two scenarios make different predictions about observable structure in local phase space,
because the morphology of debris depends on how long it has had to phase mix. The recently identified phase-space folds in Gaia
DR3 have positive caustic velocities, making them fundamentally different than the phase-mixed chevrons found in simulations
at late times. Roughly 20 per cent of the stars in the prograde local stellar halo are associated with the observed caustics. Based
on a simple phase-mixing model, the observed number of caustics are consistent with a merger that occurred 1–2 Gyr ago.
We also compare the observed phase-space distribution to FIRE-2 Latte simulations of GSE-like mergers, using a quantitative
measurement of phase mixing (2D causticality). The observed local phase-space distribution best matches the simulated data
1–2 Gyr after collision, and certainly not later than 3 Gyr. This is further evidence that the progenitor of the ‘last major merger’
did not collide with the MW proto-disc at early times, as is thought for the GSE, but instead collided with the MW disc within
the last few Gyr, consistent with the body of work surrounding the VRM.
The cost of acquiring information by natural selection
This is a short talk that I gave at the Banff International Research Station workshop on Modeling and Theory in Population Biology. The idea is to try to understand how the burden of natural selection relates to the amount of information that selection puts into the genome.
It's based on the first part of this research paper:
The cost of information acquisition by natural selection
Ryan Seamus McGee, Olivia Kosterlitz, Artem Kaznatcheev, Benjamin Kerr, Carl T. Bergstrom
bioRxiv 2022.07.02.498577; doi: https://doi.org/10.1101/2022.07.02.498577
8.Isolation of pure cultures and preservation of cultures.pdf
Isolation of pure culture, its various method.
Direct Seeded Rice - Climate Smart Agriculture
Direct Seeded Rice - Climate Smart AgricultureInternational Food Policy Research Institute- South Asia Office
PPT on Direct Seeded Rice presented at the three-day 'Training and Validation Workshop on Modules of Climate Smart Agriculture (CSA) Technologies in South Asia' workshop on April 22, 2024.
ESA/ACT Science Coffee: Diego Blas - Gravitational wave detection with orbita...
ESA/ACT Science Coffee: Diego Blas - Gravitational wave detection with orbita...Advanced-Concepts-Team
Presentation in the Science Coffee of the Advanced Concepts Team of the European Space Agency on the 07.06.2024.
Speaker: Diego Blas (IFAE/ICREA)
Title: Gravitational wave detection with orbital motion of Moon and artificial
Abstract:
In this talk I will describe some recent ideas to find gravitational waves from supermassive black holes or of primordial origin by studying their secular effect on the orbital motion of the Moon or satellites that are laser ranged.The use of Nauplii and metanauplii artemia in aquaculture (brine shrimp).pptx
Although Artemia has been known to man for centuries, its use as a food for the culture of larval organisms apparently began only in the 1930s, when several investigators found that it made an excellent food for newly hatched fish larvae (Litvinenko et al., 2023). As aquaculture developed in the 1960s and ‘70s, the use of Artemia also became more widespread, due both to its convenience and to its nutritional value for larval organisms (Arenas-Pardo et al., 2024). The fact that Artemia dormant cysts can be stored for long periods in cans, and then used as an off-the-shelf food requiring only 24 h of incubation makes them the most convenient, least labor-intensive, live food available for aquaculture (Sorgeloos & Roubach, 2021). The nutritional value of Artemia, especially for marine organisms, is not constant, but varies both geographically and temporally. During the last decade, however, both the causes of Artemia nutritional variability and methods to improve poorquality Artemia have been identified (Loufi et al., 2024).
Brine shrimp (Artemia spp.) are used in marine aquaculture worldwide. Annually, more than 2,000 metric tons of dry cysts are used for cultivation of fish, crustacean, and shellfish larva. Brine shrimp are important to aquaculture because newly hatched brine shrimp nauplii (larvae) provide a food source for many fish fry (Mozanzadeh et al., 2021). Culture and harvesting of brine shrimp eggs represents another aspect of the aquaculture industry. Nauplii and metanauplii of Artemia, commonly known as brine shrimp, play a crucial role in aquaculture due to their nutritional value and suitability as live feed for many aquatic species, particularly in larval stages (Sorgeloos & Roubach, 2021).
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The binding of cosmological structures by massless topological defects
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aziz sancar nobel prize winner: from mardin to nobel
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EWOCS-I: The catalog of X-ray sources in Westerlund 1 from the Extended Weste...
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The debris of the ‘last major merger’ is dynamically young
mô tả các thí nghiệm về đánh giá tác động dòng khí hóa sau đốt
mô tả các thí nghiệm về đánh giá tác động dòng khí hóa sau đốt
The cost of acquiring information by natural selection
The cost of acquiring information by natural selection
8.Isolation of pure cultures and preservation of cultures.pdf
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The use of Nauplii and metanauplii artemia in aquaculture (brine shrimp).pptx
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Extinction Rebellion House of Commons climate science presentation
- 2. GREENHOUSE GAS LEVELS ARE SKYROCKETING Industrial age began
- 3. GLOBAL TEMPERATURES ARE SKYROCKETING Source: IPCC Special report Climate change and land use (2019)
- 4. HEATING IMPACTS ARE ALREADY BEING FELT GLOBALLY
- 5. 2018: COP24 2015: Paris Agreement 2006: Stern Report 2001: US Renounces Kyoto 1997: Kyoto Protocol 1992 Rio Treaty 1990: First IPCC WORLD GOVERNMENT EFFORTS HAVE BEEN INEFFECTUAL
- 6. CLIMATE CHANGE, PESTICIDE USE AND HABITAT DESTRUCTION ARE DESTROYING THE BIOSPHERE
- 7. FOSSIL FUEL USE CONTINUES TO SKYROCKET
- 8. CONSUMER CAPITALISM MARCHES RELENTLESSLY ONWARDS
- 9. WE ARE INHERITED A RICH AND BOUNTEOUS PLANET AND WE ARE BEQUEATHING OUR DESCENDANTS A CHARRED HUSK THIS DESTRUCTION IS IRREVERSIBLE
- 10. • Formed in 2018 as part of the social-change movement Rising Up • Declaration of Rebellion in October 2018 • London Bridges blockades propelled it into public awareness • Has grown rapidly since EXTINCTION REBELLION
- 11. 1. Tell the truth about the ecological crisis and declare a climate emergency 2. Greenhouse gas net-zero & halting of biodiversity loss by 2025 3. Citizens’ assembly on climate and ecological justice EXTINCTION REBELLION’S THREE DEMANDS
- 12. 1. TELL THE TRUTH This has to stop
- 13. YEAR 1600 1800 2000 280 300 320 340 360 380 400 420 440 460 480 500 CO2 ppm (parts per million) We cannot delay 2. ACTION BY 2025
- 14. CAN’T WE JUST PLANT TREES? Annual emissions = 42 billion tons One tree removes one ton in 40 years That’s 42 billion new trees EVERY YEAR That’s 17 million hectares EVERY YEAR (Wales is 2 million hectares) And emissions are rising year on year
- 15. WE MUST URGENTLY DE-CARBONISE THE ECONOMY
- 16. ● Can take the long view ● Free from corporate influences ● Truly representative of the population ● Trusted by the public ● Has been effective before (Ireland, Poland) 3. CITIZENS’ ASSEMBLY
- 17. “Why didn’t you stop this when you still could?” WHAT WILL WE TELL OUR GRANDCHILDREN?