Atmosphere is the blanket of air that surrounds the earth and the composition of the Atmosphere is 78% nitrogen, 21% oxygen 0.9% argon and 0.1% other gases. Earth has 6 layers of Atmosphere around it to protect us from harmful gases & maintain the suitable temperature for the life on the earth .The layers are Troposphere, Stratosphere, Mesosphere , Thermosphere , Exosphere and Ionosphere.
This presentation contains about the layers of the atmosphere which has 5 layers in atmosphere
The first layer is troposphere
The second layer is stratosphere
The third layer is mesosphere
The fourth layer is ionosphere and
The fifth layer is exosphere
Toxic effects of heavy metals : Lead and Arsenicsanjana502982
Heavy metals are naturally occuring metallic chemical elements that have relatively high density, and are toxic at even low concentrations. All toxic metals are termed as heavy metals irrespective of their atomic mass and density, eg. arsenic, lead, mercury, cadmium, thallium, chromium, etc.
This presentation contains about the layers of the atmosphere which has 5 layers in atmosphere
The first layer is troposphere
The second layer is stratosphere
The third layer is mesosphere
The fourth layer is ionosphere and
The fifth layer is exosphere
Toxic effects of heavy metals : Lead and Arsenicsanjana502982
Heavy metals are naturally occuring metallic chemical elements that have relatively high density, and are toxic at even low concentrations. All toxic metals are termed as heavy metals irrespective of their atomic mass and density, eg. arsenic, lead, mercury, cadmium, thallium, chromium, etc.
Phenomics assisted breeding in crop improvementIshaGoswami9
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.
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
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at > 2.3µm to construct an ultradeep image, reaching as deep as ≈ 31.4 AB mag in the stack and
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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
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The ability to recreate computational results with minimal effort and actionable metrics provides a solid foundation for scientific research and software development. When people can replicate an analysis at the touch of a button using open-source software, open data, and methods to assess and compare proposals, it significantly eases verification of results, engagement with a diverse range of contributors, and progress. However, we have yet to fully achieve this; there are still many sociotechnical frictions.
Inspired by David Donoho's vision, this talk aims to revisit the three crucial pillars of frictionless reproducibility (data sharing, code sharing, and competitive challenges) with the perspective of deep software variability.
Our observation is that multiple layers — hardware, operating systems, third-party libraries, software versions, input data, compile-time options, and parameters — are subject to variability that exacerbates frictions but is also essential for achieving robust, generalizable results and fostering innovation. I will first review the literature, providing evidence of how the complex variability interactions across these layers affect qualitative and quantitative software properties, thereby complicating the reproduction and replication of scientific studies in various fields.
I will then present some software engineering and AI techniques that can support the strategic exploration of variability spaces. These include the use of abstractions and models (e.g., feature models), sampling strategies (e.g., uniform, random), cost-effective measurements (e.g., incremental build of software configurations), and dimensionality reduction methods (e.g., transfer learning, feature selection, software debloating).
I will finally argue that deep variability is both the problem and solution of frictionless reproducibility, calling the software science community to develop new methods and tools to manage variability and foster reproducibility in software systems.
Exposé invité Journées Nationales du GDR GPL 2024
hematic appreciation test is a psychological assessment tool used to measure an individual's appreciation and understanding of specific themes or topics. This test helps to evaluate an individual's ability to connect different ideas and concepts within a given theme, as well as their overall comprehension and interpretation skills. The results of the test can provide valuable insights into an individual's cognitive abilities, creativity, and critical thinking skills
Travis Hills' Endeavors in Minnesota: Fostering Environmental and Economic Pr...Travis Hills MN
Travis Hills of Minnesota developed a method to convert waste into high-value dry fertilizer, significantly enriching soil quality. By providing farmers with a valuable resource derived from waste, Travis Hills helps enhance farm profitability while promoting environmental stewardship. Travis Hills' sustainable practices lead to cost savings and increased revenue for farmers by improving resource efficiency and reducing waste.
What is greenhouse gasses and how many gasses are there to affect the Earth.moosaasad1975
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Salas, V. (2024) "John of St. Thomas (Poinsot) on the Science of Sacred Theol...Studia Poinsotiana
I Introduction
II Subalternation and Theology
III Theology and Dogmatic Declarations
IV The Mixed Principles of Theology
V Virtual Revelation: The Unity of Theology
VI Theology as a Natural Science
VII Theology’s Certitude
VIII Conclusion
Notes
Bibliography
All the contents are fully attributable to the author, Doctor Victor Salas. Should you wish to get this text republished, get in touch with the author or the editorial committee of the Studia Poinsotiana. Insofar as possible, we will be happy to broker your contact.
2. Atmosphere
• The Atmosphere is the blanket
of air that surrounds the earth.
• The Atmosphere help protect us
from harmful gases and
maintain the suitable temperatur
e necessary for life.
3. Composition of
the Atmosphere
• 78 % nitrogen.
• 21 %oxygen.
• 0.9 %t argon.
• 0.1 % other gases.
• Trace amounts of carbon dioxide,
methane, water vapor, and neon are
some of the other gases that make
up the remaining 0.1 percent.
6. Troposphere
• Closest to the surface of Earth, we have
the troposphere. “Tropos” means change. This layer gets its
name from the weather that is constantly changing and mixing
up the gases in this part of our atmosphere.
• The troposphere is between 5 and 9 miles (8 and 14 kilometers)
thick depending on where you are on Earth. It’s thinnest at the
North and South Pole.
• .The air is densest in this lowest layer. In fact, the troposphere
contains three-quarters of the mass of the entire atmosphere. The
air here is 78% nitrogen and 21% oxygen. The last 1% is made
of argon, water vapor, and carbon dioxide.
7. Stratosphere
• The stratosphere is a layer of Earth’s atmosphere. The stratosphere is
located above the troposphere and below the
mesosphere. Strat” means layer. This layer of our atmosphere has its own
set of layers.
• There are no storms or turbulence here to mix up the air, so cold, heavy
air is at the bottom and warm, light air is at the top. That’s the opposite of
how the layers work in the tropospher.
• This layer is 22 miles (35 kilometers) thick. The stratosphere is where
you’ll find the very important ozone layer. The ozone layer helps protect
us from ultraviolet radiation (UV) from the sun. In fact, the ozone layer
absorbs most of the UV radiation the sun sends to us. Life as we know it
wouldn’t be possible without this layer of protection.
8. Mesosphere
• The mesosphere is a layer of Earth’s atmosphere. The
mesosphere is located above the stratosphere and below
the thermosphere.
• “Meso” means middle, and this is the highest layer of the
atmosphere in which the gases are all mixed up rather
than being layered by their mass.
• The mesosphere is 22 miles (35 kilometers) thick. The air
is still thin, so you wouldn’t be able to breathe up in the
mesosphere. But there is more gas in this layer than there
is out in the thermosphere.
9. Thermosphere
• This layer is found above mesosphere from 80 to
400 km.
• Radio waves that are transmitted from the earth are
reflected by this layer.
• The temperature starts increasing again with
increasing height in this layer.
• Aurora and satellites occur in this layer.
10. Exosphere
• The exosphere is the outermost layer of Earth’s
atmosphere. “Exo” means outside
• The exosphere is the very edge of our atmosphere. This
layer separates the rest of the atmosphere from outer
space. It’s about 6,200 miles (10,000 kilometers) thick.
That’s almost as wide as Earth itself.
• The exosphere has gases like hydrogen and helium, but
they are very spread out. There is a lot of empty space in
between. There is no air to breathe, and it’s very cold.
11. Ionosphere
• Ionosphere overlaps the mesosphere, thermosphere,
and exosphere. The ionosphere is a very active part of the
atmosphere, and it grows and shrinks depending on the energy it
absorbs from the Sun. The name ionosphere comes from the fact that
gases in these layers are excited by solar radiation to form ions,
which have an electrical charge.
• Parts of the ionosphere overlap with Earth’s magnetosphere. That’s
the area around Earth where charged particles feel Earth’s magnetic
field.
• In the ionosphere, charged particles are affected by the magnetic
fields of both Earth and the sun. This is where auroras happen.
Those are the bright, beautiful bands of light that you sometimes see
near Earth’s poles. They’re caused by high-energy particles from the
sun interacting with the atoms in this layer of our atmosphere.