This PowerPoint discusses the Sun at a high school level. It talks about characteristics, solar activities/events, how energy is created, and many more.
Maybe too in-depth for most elementary students, but very good broad coverage for teacher background or more advanced students in elementary or middle school.
The Sun is by far the largest object in the solar system, containing over 99% of the mass. It has a diameter over 100 times larger than Earth and generates energy through nuclear fusion of hydrogen into helium. Light from the Sun takes approximately 8 minutes to reach Earth. While the visible surface of the Sun appears solid, it actually consists of several layers including the core, radiative zone, convective zone, photosphere, chromosphere, and corona. Solar activity like sunspots, solar flares, and coronal mass ejections can impact power grids and communication systems on Earth. Astronomers study the Sun to better understand stars and how changes in solar output impact Earth's climate and atmosphere.
The document provides information about the Moon and its exploration history. It describes the Moon's size and distance from Earth. Key events in lunar exploration included Soviet missions in 1959 and US missions in the 1960s including Rangers, Lunar Orbiters, and Surveyors. The Apollo 11 mission in 1969 was the first to land humans on the Moon. The document discusses lunar geology, noting differences from Earth like the lack of an atmosphere, water, or plate tectonics. It describes lunar features such as maria, highlands, craters, and rilles. The formation of the Moon is also summarized.
The document summarizes tides, including their causes due to the gravitational interaction between the Earth, Moon and Sun. It describes the stages of a tidal cycle from flood tide to low tide. It distinguishes between spring tides, which occur during full and new moons when gravitational forces align to produce stronger tides, and neap tides during quarter moons when forces are perpendicular and tides are weaker. Rare proxigean spring tides result from a close and aligned positioning of the Moon.
The moon orbits the Earth every 27 days on average at a distance of 384,400km. It was likely formed from debris ejected from Earth after a collision with a Mars-sized object. The different phases of the moon are caused by the illumination of its surface from the Sun as it orbits Earth. The moon's gravitational pull causes ocean tides on Earth and influences their size.
The document discusses various terms related to the moon including its phases, features, effect on tides, and history of exploration. It defines waxing as when the moon appears to grow in size, waning as when it decreases in size, and gibbous as between a half circle and full circle of illumination. It notes the moon's seas are dark patches formed by ancient lava flows and that phases refer to how much is illuminated each day. A harvest moon is a full moon near the autumn equinox that rises earlier each night. The first men on the moon were Neil Armstrong and Buzz Aldrin in 1969.
The document provides an overview of the components of the solar system, including the sun, eight planets, asteroids, comets, and satellites. It discusses the key features of terrestrial and Jovian planets, and provides brief introductions to each of the planets as well as other celestial bodies like asteroids, meteors, comets, and satellites. The document aims to teach students about the structure and composition of objects in the solar system.
The document summarizes key information about the Sun, including its interior structure, energy production through nuclear fusion, and atmospheric layers. The Sun's core produces energy through proton-proton fusion, with a small amount of mass being converted to energy. Sunspots occur in 11-year cycles and are associated with magnetic fields, while solar flares and coronal mass ejections can emit large amounts of energy and eject plasma into space.
The Sun is a middle-aged, average sized yellow star that is made up mostly of hydrogen and helium. It is about 4.6 billion years old and located 93 million miles from Earth. The Sun generates heat and light through nuclear fusion reactions in its core that convert hydrogen into helium. It is the center of our Solar System and contains over 99% of the mass in the entire system. The Solar System also includes eight official planets that orbit the Sun, along with dwarf planets, moons, asteroids, comets, and other small bodies.
The Milky Way galaxy is our home galaxy, which contains over 100 billion stars. It is a barred spiral galaxy approximately 120,000 light years in diameter. The Solar System is located in one of the galaxy's spiral arms, about 27,000 light years from the galactic core. In the future, it is expected that the Milky Way will collide and merge with the neighboring Andromeda galaxy in 3-4 billion years.
The document provides an introduction to stars, focusing on the sun. It discusses the layers of the sun's atmosphere and interior. The sun's core generates its enormous energy output through nuclear fusion. The solar wind consists of high-energy particles escaping the sun's gravity. The sun emits across the electromagnetic spectrum, including x-rays studied by orbital telescopes. The sun's total luminosity is calculated based on the energy received by a detector at Earth's distance. Sunspots occur in pairs of opposite magnetic fields and vary in a roughly 11-year solar cycle.
The solar system consists of the Sun, eight official planets, and at least three dwarf planets. It provides details about each planet's size, distance from the Sun, orbital period, rotational period, composition, and notable features. It also includes questions and answers that provide additional interesting facts about each planet.
A meteoroid is a small rocky or metallic object traveling through space. Most meteoroids range in size from small grains to 1 meter and are fragments from comets or asteroids. When meteoroids enter the Earth's atmosphere, friction and compression cause them to heat up and glow - appearing as "shooting stars" or meteors. If they survive atmospheric entry and reach the ground, they are called meteorites.
The solar system is made up of the Sun, the planets that orbit the Sun, their satellites, dwarf planets and many, many small objects, like asteroids and comets. All of these objects move and we can see these movements. We notice the Sun rises in the eastern sky in the morning and sets in the western sky in the evening. We observe different stars in the sky at different times of the year.
This document provides an overview of stars, galaxies, and the universe. It begins with definitions of key terms like stars, galaxies, and the universe. It then covers the composition of stars and how they are classified. The next sections discuss the life cycles of stars and the different types of galaxies. The document concludes with an explanation of the big bang theory of the universe and how scientists estimate the age of the universe.
The document discusses astronomy and the scientific study of celestial objects. It provides information on stars, galaxies, and the formation and components of the solar system. Specifically, it notes that astronomy is the study of matter in outer space, including the positions, dimensions, distribution, motion, composition, energy, and evolution of celestial bodies. It also summarizes that the universe started as a single point which exploded outward in the big bang and has been expanding ever since. Finally, it outlines the key parts of the solar system, including the sun, planets, asteroids, comets, and meteoroids.
This document discusses dwarf planets in the solar system. It defines dwarf planets as celestial bodies that orbit the sun, are massive enough to be rounded by their own gravity, but have not cleared their orbit of other objects. It provides details on the five officially recognized dwarf planets: Ceres, Pluto, Eris, Haumea, and Makemake. It describes their sizes, compositions, orbits, and discoveries.
1. Stars form from dense clouds of gas and dust in interstellar space.
2. Gravity causes the cloud to contract over many stages until fusion begins in the core and a new star is born on the main sequence.
3. The size and mass of a star determines its position on the HR diagram, with more massive stars being larger and hotter.
The document provides information about the Moon. It discusses the Moon's age, distance from Earth, diameter, rotation period, and average speed around Earth. Some key facts are that the Moon is about 4.6 billion years old, its diameter is about 3,476 kilometers, and it orbits Earth once every 27.3 days. The Moon reflects light from the Sun, which is what makes it visible from Earth and causes its appearance to change throughout the month.
The Sun formed around 5 billion years ago from a cloud of gas and dust. Through the process of nuclear fusion at its core, the Sun generates immense heat and light by converting hydrogen into helium. It is a common yellow star that is part of a cycle that creates convection currents within its surface and sunspots that follow an 11-year cycle. The Sun provides the energy necessary to sustain life on Earth but will eventually exhaust its hydrogen fuel in around 5 billion years.
Comets are small icy objects with two tails made of gas and dust that formed over 4.6 billion years ago in the early solar system and have highly elliptical orbits. Asteroids are small rocky or metallic objects that orbit the sun, ranging in size from meters to hundreds of kilometers wide with irregular shapes and cratered surfaces. Meteors are streaks of light seen when meteoroids - space rocks or fragments that can be from comets, asteroids, moons or Mars - enter the Earth's atmosphere. Some meteoroids survive entry and land on Earth's surface as meteorites.
The document summarizes key facts about our solar system including:
- It contains 1 star, 8 planets, many moons, asteroids, comets and meteoroids.
- Terrestrial planets like Earth are rocky while Jovian planets like Jupiter are gaseous.
- Asteroids, meteoroids and comets originate from leftover material that did not form planets.
- The nebular hypothesis and condensation theory explain how the solar system formed from a large cloud or disk of dust and gas over billions of years.
The document provides information about the solar system and the objects within it. It describes the Sun and planets Mercury through Neptune. It discusses other bodies like asteroids, comets, and the Moon. It also explains what stars, galaxies, and constellations are made of and how they relate to the solar system.
The moon revolves around Earth once every 27 days, keeping the same side facing Earth. It reflects sunlight and its illuminated half changes shape in a cycle from new moon to first quarter to full moon to third quarter over 2912 days. The moon is the closest celestial object to Earth at 384,000 km away. It has many impact craters and temperature extremes ranging from 127属C during the day to -173属C at night. Telescopes allow observation of details on the moon's surface.
The sun is the largest object in the solar system, containing over 99% of its mass. It emits light and heat that support life on Earth and influence all solar system objects. The sun has various internal layers, including the core where energy is produced through nuclear fusion, and an outer atmosphere. Sunspots, solar flares, and other features periodically appear on its surface. In a few billion years, the sun will expand and grow hotter, eventually making Earth uninhabitable.
The document provides information about stars, constellations, and other objects in the solar system. It explains that stars appear to move across the sky from east to west due to the Earth's rotation. It then discusses the units used to measure large distances in space, including light years. Finally, it describes several constellations visible in the night sky like Ursa Major, Ursa Minor, Orion, and others, and the patterns of stars that comprise each one.
The document provides information about stars and galaxies. It begins by describing characteristics of the Sun such as its size, temperature, and composition. It then discusses the structure of the Sun and phenomena on its surface like sunspots, solar flares, and prominences. The effects of solar phenomena like solar wind on Earth are also outlined. The document concludes by describing galaxies like the Milky Way and theories about the formation, evolution and potential end of the Universe.
The document discusses the structure and composition of the Sun. It has 6 layers: the core, where fusion occurs at 15 million degrees Celsius; the radiative zone, where energy moves by radiation; the convection zone, where hot gas currents transfer energy; the photosphere, the visible surface; the chromosphere, a thin pinkish layer; and the corona, the outermost low density layer. The Sun is mostly made of hydrogen and helium and produces energy through the fusion of hydrogen into helium. It contains over 99% of the mass in the solar system and has prominent features like sunspots and solar winds.
The Sun is a middle-aged, average sized yellow star that is made up mostly of hydrogen and helium. It is about 4.6 billion years old and located 93 million miles from Earth. The Sun generates heat and light through nuclear fusion reactions in its core that convert hydrogen into helium. It is the center of our Solar System and contains over 99% of the mass in the entire system. The Solar System also includes eight official planets that orbit the Sun, along with dwarf planets, moons, asteroids, comets, and other small bodies.
The Milky Way galaxy is our home galaxy, which contains over 100 billion stars. It is a barred spiral galaxy approximately 120,000 light years in diameter. The Solar System is located in one of the galaxy's spiral arms, about 27,000 light years from the galactic core. In the future, it is expected that the Milky Way will collide and merge with the neighboring Andromeda galaxy in 3-4 billion years.
The document provides an introduction to stars, focusing on the sun. It discusses the layers of the sun's atmosphere and interior. The sun's core generates its enormous energy output through nuclear fusion. The solar wind consists of high-energy particles escaping the sun's gravity. The sun emits across the electromagnetic spectrum, including x-rays studied by orbital telescopes. The sun's total luminosity is calculated based on the energy received by a detector at Earth's distance. Sunspots occur in pairs of opposite magnetic fields and vary in a roughly 11-year solar cycle.
The solar system consists of the Sun, eight official planets, and at least three dwarf planets. It provides details about each planet's size, distance from the Sun, orbital period, rotational period, composition, and notable features. It also includes questions and answers that provide additional interesting facts about each planet.
A meteoroid is a small rocky or metallic object traveling through space. Most meteoroids range in size from small grains to 1 meter and are fragments from comets or asteroids. When meteoroids enter the Earth's atmosphere, friction and compression cause them to heat up and glow - appearing as "shooting stars" or meteors. If they survive atmospheric entry and reach the ground, they are called meteorites.
The solar system is made up of the Sun, the planets that orbit the Sun, their satellites, dwarf planets and many, many small objects, like asteroids and comets. All of these objects move and we can see these movements. We notice the Sun rises in the eastern sky in the morning and sets in the western sky in the evening. We observe different stars in the sky at different times of the year.
This document provides an overview of stars, galaxies, and the universe. It begins with definitions of key terms like stars, galaxies, and the universe. It then covers the composition of stars and how they are classified. The next sections discuss the life cycles of stars and the different types of galaxies. The document concludes with an explanation of the big bang theory of the universe and how scientists estimate the age of the universe.
The document discusses astronomy and the scientific study of celestial objects. It provides information on stars, galaxies, and the formation and components of the solar system. Specifically, it notes that astronomy is the study of matter in outer space, including the positions, dimensions, distribution, motion, composition, energy, and evolution of celestial bodies. It also summarizes that the universe started as a single point which exploded outward in the big bang and has been expanding ever since. Finally, it outlines the key parts of the solar system, including the sun, planets, asteroids, comets, and meteoroids.
This document discusses dwarf planets in the solar system. It defines dwarf planets as celestial bodies that orbit the sun, are massive enough to be rounded by their own gravity, but have not cleared their orbit of other objects. It provides details on the five officially recognized dwarf planets: Ceres, Pluto, Eris, Haumea, and Makemake. It describes their sizes, compositions, orbits, and discoveries.
1. Stars form from dense clouds of gas and dust in interstellar space.
2. Gravity causes the cloud to contract over many stages until fusion begins in the core and a new star is born on the main sequence.
3. The size and mass of a star determines its position on the HR diagram, with more massive stars being larger and hotter.
The document provides information about the Moon. It discusses the Moon's age, distance from Earth, diameter, rotation period, and average speed around Earth. Some key facts are that the Moon is about 4.6 billion years old, its diameter is about 3,476 kilometers, and it orbits Earth once every 27.3 days. The Moon reflects light from the Sun, which is what makes it visible from Earth and causes its appearance to change throughout the month.
The Sun formed around 5 billion years ago from a cloud of gas and dust. Through the process of nuclear fusion at its core, the Sun generates immense heat and light by converting hydrogen into helium. It is a common yellow star that is part of a cycle that creates convection currents within its surface and sunspots that follow an 11-year cycle. The Sun provides the energy necessary to sustain life on Earth but will eventually exhaust its hydrogen fuel in around 5 billion years.
Comets are small icy objects with two tails made of gas and dust that formed over 4.6 billion years ago in the early solar system and have highly elliptical orbits. Asteroids are small rocky or metallic objects that orbit the sun, ranging in size from meters to hundreds of kilometers wide with irregular shapes and cratered surfaces. Meteors are streaks of light seen when meteoroids - space rocks or fragments that can be from comets, asteroids, moons or Mars - enter the Earth's atmosphere. Some meteoroids survive entry and land on Earth's surface as meteorites.
The document summarizes key facts about our solar system including:
- It contains 1 star, 8 planets, many moons, asteroids, comets and meteoroids.
- Terrestrial planets like Earth are rocky while Jovian planets like Jupiter are gaseous.
- Asteroids, meteoroids and comets originate from leftover material that did not form planets.
- The nebular hypothesis and condensation theory explain how the solar system formed from a large cloud or disk of dust and gas over billions of years.
The document provides information about the solar system and the objects within it. It describes the Sun and planets Mercury through Neptune. It discusses other bodies like asteroids, comets, and the Moon. It also explains what stars, galaxies, and constellations are made of and how they relate to the solar system.
The moon revolves around Earth once every 27 days, keeping the same side facing Earth. It reflects sunlight and its illuminated half changes shape in a cycle from new moon to first quarter to full moon to third quarter over 2912 days. The moon is the closest celestial object to Earth at 384,000 km away. It has many impact craters and temperature extremes ranging from 127属C during the day to -173属C at night. Telescopes allow observation of details on the moon's surface.
The sun is the largest object in the solar system, containing over 99% of its mass. It emits light and heat that support life on Earth and influence all solar system objects. The sun has various internal layers, including the core where energy is produced through nuclear fusion, and an outer atmosphere. Sunspots, solar flares, and other features periodically appear on its surface. In a few billion years, the sun will expand and grow hotter, eventually making Earth uninhabitable.
The document provides information about stars, constellations, and other objects in the solar system. It explains that stars appear to move across the sky from east to west due to the Earth's rotation. It then discusses the units used to measure large distances in space, including light years. Finally, it describes several constellations visible in the night sky like Ursa Major, Ursa Minor, Orion, and others, and the patterns of stars that comprise each one.
The document provides information about stars and galaxies. It begins by describing characteristics of the Sun such as its size, temperature, and composition. It then discusses the structure of the Sun and phenomena on its surface like sunspots, solar flares, and prominences. The effects of solar phenomena like solar wind on Earth are also outlined. The document concludes by describing galaxies like the Milky Way and theories about the formation, evolution and potential end of the Universe.
The document discusses the structure and composition of the Sun. It has 6 layers: the core, where fusion occurs at 15 million degrees Celsius; the radiative zone, where energy moves by radiation; the convection zone, where hot gas currents transfer energy; the photosphere, the visible surface; the chromosphere, a thin pinkish layer; and the corona, the outermost low density layer. The Sun is mostly made of hydrogen and helium and produces energy through the fusion of hydrogen into helium. It contains over 99% of the mass in the solar system and has prominent features like sunspots and solar winds.
This document provides an overview of Earth science and the solar system. It describes the four branches of Earth science: geology, meteorology, astronomy, and oceanography. It then explains the importance of studying Earth science, including understanding natural resources and hazards. The document continues by defining the solar system and describing how it formed based on the planetesimal and nebular theories. It outlines the layers of the Sun and solar activities like sunspots and solar flares. Finally, it characterizes the eight major planets, grouping the inner terrestrial planets and outer gas giants, and provides key details about each planetary body.
This document provides an overview of Earth science and the solar system. It describes the four branches of Earth science: geology, meteorology, astronomy, and oceanography. It then explains the importance of studying Earth science, including understanding natural resources and hazards. The document continues by defining the solar system and describing how it formed based on the planetesimal and nebular theories. It outlines the layers of the Sun and solar activities like sunspots and solar flares. Finally, it characterizes the eight major planets, grouping the inner terrestrial planets and outer gas giants, and provides key details about each planetary body.
The document summarizes key concepts about the sun and Earth's formation. It describes how the sun generates energy through nuclear fusion in its core, and how this energy reaches the surface in about 8 minutes. It also explains how Earth formed from the accretion of planetesimals, and how its core, mantle and crust layers developed as denser materials sank to the center. The oceans formed from early rainfall, and continents gradually emerged and shifted positions over billions of years.
The document discusses the big bang theory and recent efforts to recreate what it may have sounded like. According to physicist John Cramer, the big bang would have produced a deep hum rather than a bang. He analyzed cosmic microwave background radiation data from the Wilkinson Microwave Anisotropy Probe satellite to calculate the frequencies of sound waves in the early universe. Cramer then scaled these frequencies up enormously to make them audible. His recording suggests the sound became more of a bass tone as the universe expanded after the big bang.
Stars are spherical objects made of hot gases that radiate electromagnetic radiation from their hot cores. There are over 9000 billion billion stars in the universe. All stars go through similar life cycles of birth, formation from nebulae, nuclear fusion in their cores, and death depending on their mass. Low mass stars exist as red dwarfs for over 100 billion years and become white dwarfs. Intermediate mass stars like our Sun last 10 billion years and become red giants then white dwarfs. High mass stars over 12 solar masses burn quickly in 7 billion years and explode as supernovae, collapsing into neutron stars or black holes.
The document summarizes key information about astronomy and the universe:
1) The universe started as a single extremely dense point that exploded in an enormous explosion known as the Big Bang around 12-15 billion years ago and has been expanding ever since.
2) Evidence for the expansion of the universe comes from the Doppler effect observed in the redshift of light from galaxies moving away from us as the universe expands.
3) Astronomers use large units like light years to measure the vast distances between celestial objects, where one light year is the distance light travels in one year.
The document discusses the planet Mercury. It is the closest planet to the Sun and has little atmosphere. Its landscape is dominated by craters and cliffs, and it experiences extreme temperature variations between day and night. Mercury rotates around the Sun every 88 days and has no moons.
The document provides an overview of the solar system, including its origin and components. It discusses:
1) The modern view that the solar system formed from a rotating cloud of gas and dust that condensed to form the Sun and planets as it contracted.
2) The inner planets Mercury, Venus, Earth, and Mars, including characteristics such as temperatures, atmospheres, and evidence of past water on Mars.
3) The outer planets Jupiter, Saturn, Uranus, and Neptune, noting their large sizes and gaseous compositions. Moons and rings are also mentioned.
The Sun is a glowing ball of gas held together by gravity that is powered by nuclear fusion. It has a diameter of 1.392 million km and is made up primarily of hydrogen and helium. Nuclear fusion in the core converts hydrogen to helium, releasing enormous amounts of energy over billions of years. Features on the Sun include sunspots, solar flares, and prominences, which can impact Earth.
The sun is a huge glowing ball of gas at the center of our solar system that provides light, heat, and energy to Earth. It is made up primarily of hydrogen and helium and has a radius about 109 times that of Earth. The sun was formed around 4.6 billion years ago and will remain stable for another 5 billion years before expanding into a red giant. It emits electromagnetic radiation across the spectrum, including visible light and infrared that we experience as heat and light. Nuclear fusion in the sun's core converts hydrogen to helium and releases enormous amounts of energy.
The Sun is a normal G2 star that contains over 99% of the mass in the Solar System. It has a diameter of 1.39 million km and a surface temperature of 5,800 K. Energy is created in the Sun's core through nuclear fusion and radiates outward through convection and radiation zones to the surface. The Sun's 11-year activity cycle causes variations in sunspots, flares, and other magnetic phenomena. In the future, the Sun will expand into a red giant after exhausting its hydrogen fuel supply over many billions of years.
The Solar System formed from a large rotating cloud of gas and dust called a solar nebula. As the nebula condensed due to gravity, a central mass became the Sun and the remaining material formed rings that eventually became the planets. The Sun consists of an inner core where nuclear fusion occurs and surrounding layers including the photosphere, chromosphere, and corona. The eight major planets can be divided into terrestrial and Jovian planets. Smaller bodies like asteroids and comets also orbit the Sun.
The Sun is a normal G2 star that contains over 99% of the mass in the Solar System. It has a diameter of 1.39 million km and a surface temperature of 5,800 K. Energy is created in the Sun's core through nuclear fusion and radiates outward through convection and radiation zones to the surface. The Sun's 11-year activity cycle causes variations in sunspots, flares, and other magnetic phenomena. In the future, the Sun will expand into a red giant after exhausting its hydrogen fuel supply over many billions of years.
The document discusses layers of the sun and solar events. It explains that the sun has a photosphere, chromosphere, and corona. The photosphere is the visible surface with sunspots. The chromosphere has solar prominences and flares. The corona surrounds the chromosphere and extends into space. Solar magnetism and coronal holes cause solar winds. The document also discusses measuring distances to stars using parallax as the apparent shift in a star's position from different points in Earth's orbit.
Form 3 PMR Science Chapter 9 Stars and GalaxiesSook Yen Wong
油
Stars are giant balls of hot gases that produce heat and light through nuclear fusion reactions in their cores. Stars are classified according to attributes like temperature, brightness, chemical composition, size, and density. When stars die, they may leave behind white dwarfs, neutron stars, or black holes. Galaxies contain millions of stars and come in different shapes like spiral and elliptical.
The document summarizes key aspects of how scientists believe the universe began and evolved based on two major theories - the Big Bang theory and the Solar Nebula theory. It provides details on each theory, including that the Big Bang occurred approximately 13.75 billion years ago and resulted in the rapid expansion and cooling of an extremely hot and dense early universe. The Solar Nebula theory proposes that our solar system formed from a collapsing cloud of gas and dust that gave rise to the sun and orbiting bodies.
Field Device Management Market Report 2030 - TechSci ResearchVipin Mishra
油
The Global Field Device Management (FDM) Market is expected to experience significant growth in the forecast period from 2026 to 2030, driven by the integration of advanced technologies aimed at improving industrial operations.
According to TechSci Research, the Global Field Device Management Market was valued at USD 1,506.34 million in 2023 and is anticipated to grow at a CAGR of 6.72% through 2030. FDM plays a vital role in the centralized oversight and optimization of industrial field devices, including sensors, actuators, and controllers.
Key tasks managed under FDM include:
Configuration
Monitoring
Diagnostics
Maintenance
Performance optimization
FDM solutions offer a comprehensive platform for real-time data collection, analysis, and decision-making, enabling:
Proactive maintenance
Predictive analytics
Remote monitoring
By streamlining operations and ensuring compliance, FDM enhances operational efficiency, reduces downtime, and improves asset reliability, ultimately leading to greater performance in industrial processes. FDMs emphasis on predictive maintenance is particularly important in ensuring the long-term sustainability and success of industrial operations.
For more information, explore the full report: https://shorturl.at/EJnzR
Major companies operating in Global油Field Device Management Market are:
General Electric Co
Siemens AG
ABB Ltd
Emerson Electric Co
Aveva Group Ltd
Schneider Electric SE
STMicroelectronics Inc
Techno Systems Inc
Semiconductor Components Industries LLC
International Business Machines Corporation (IBM)
#FieldDeviceManagement #IndustrialAutomation #PredictiveMaintenance #TechInnovation #IndustrialEfficiency #RemoteMonitoring #TechAdvancements #MarketGrowth #OperationalExcellence #SensorsAndActuators
Computational Photography: How Technology is Changing Way We Capture the WorldHusseinMalikMammadli
油
Computational Photography (Computer Vision/Image): How Technology is Changing the Way We Capture the World
He巽 d端端nm端s端n端zm端, m端asir smartfonlar v kameralar nec bu qdr g旦zl g旦r端nt端lr yarad脹r? Bunun sirri Computational Fotoqrafiyas脹nda(Computer Vision/Imaging) gizlidirkillri 巽km v emal etm 端sulumuzu tkmilldirn, komp端ter elmi il fotoqrafiyan脹n inqilabi birlmsi.
Future-Proof Your Career with AI OptionsDianaGray10
油
Learn about the difference between automation, AI and agentic and ways you can harness these to further your career. In this session you will learn:
Introduction to automation, AI, agentic
Trends in the marketplace
Take advantage of UiPath training and certification
In demand skills needed to strategically position yourself to stay ahead
If you have any questions or feedback, please refer to the "Women in Automation 2025" dedicated Forum thread. You can find there extra details and updates.
What Makes "Deep Research"? A Dive into AI AgentsZilliz
油
About this webinar:
Unless you live under a rock, you will have heard about OpenAIs release of Deep Research on Feb 2, 2025. This new product promises to revolutionize how we answer questions requiring the synthesis of large amounts of diverse information. But how does this technology work, and why is Deep Research a noticeable improvement over previous attempts? In this webinar, we will examine the concepts underpinning modern agents using our basic clone, Deep Searcher, as an example.
Topics covered:
Tool use
Structured output
Reflection
Reasoning models
Planning
Types of agentic memory
[Webinar] Scaling Made Simple: Getting Started with No-Code Web AppsSafe Software
油
Ready to simplify workflow sharing across your organization without diving into complex coding? With FME Flow Apps, you can build no-code web apps that make your data work harder for you fast.
In this webinar, well show you how to:
Build and deploy Workspace Apps to create an intuitive user interface for self-serve data processing and validation.
Automate processes using Automation Apps. Learn to create a no-code web app to kick off workflows tailored to your needs, trigger multiple workspaces and external actions, and use conditional filtering within automations to control your workflows.
Create a centralized portal with Gallery Apps to share a collection of no-code web apps across your organization.
Through real-world examples and practical demos, youll learn how to transform your workflows into intuitive, self-serve solutions that empower your team and save you time. We cant wait to show you whats possible!
UiPath Document Understanding - Generative AI and Active learning capabilitiesDianaGray10
油
This session focus on Generative AI features and Active learning modern experience with Document understanding.
Topics Covered:
Overview of Document Understanding
How Generative Annotation works?
What is Generative Classification?
How to use Generative Extraction activities?
What is Generative Validation?
How Active learning modern experience accelerate model training?
Q/A
If you have any questions or feedback, please refer to the "Women in Automation 2025" dedicated Forum thread. You can find there extra details and updates.
Fl studio crack version 12.9 Free Downloadkherorpacca127
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https://ncracked.com/7961-2/
Note: >> Please copy the link and paste it into Google New Tab now Download link
The ultimate guide to FL Studio 12.9 Crack, the revolutionary digital audio workstation that empowers musicians and producers of all levels. This software has become a cornerstone in the music industry, offering unparalleled creative capabilities, cutting-edge features, and an intuitive workflow.
With FL Studio 12.9 Crack, you gain access to a vast arsenal of instruments, effects, and plugins, seamlessly integrated into a user-friendly interface. Its signature Piano Roll Editor provides an exceptional level of musical expression, while the advanced automation features empower you to create complex and dynamic compositions.
Technology use over time and its impact on consumers and businesses.pptxkaylagaze
油
In this presentation, I will discuss how technology has changed consumer behaviour and its impact on consumers and businesses. I will focus on internet access, digital devices, how customers search for information and what they buy online, video consumption, and lastly consumer trends.
Many MSPs overlook endpoint backup, missing out on additional profit and leaving a gap that puts client data at risk.
Join our webinar as we break down the top challenges of endpoint backupand how to overcome them.
Formal Methods: Whence and Whither? [Martin Fr辰nzle Festkolloquium, 2025]Jonathan Bowen
油
Alan Turing arguably wrote the first paper on formal methods 75 years ago. Since then, there have been claims and counterclaims about formal methods. Tool development has been slow but aided by Moores Law with the increasing power of computers. Although formal methods are not widespread in practical usage at a heavyweight level, their influence as crept into software engineering practice to the extent that they are no longer necessarily called formal methods in their use. In addition, in areas where safety and security are important, with the increasing use of computers in such applications, formal methods are a viable way to improve the reliability of such software-based systems. Their use in hardware where a mistake can be very costly is also important. This talk explores the journey of formal methods to the present day and speculates on future directions.
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Brave is a free Chromium browser developed for Win Downloads, macOS and Linux systems that allows users to browse the internet in a safer, faster and more secure way than its competition. Designed with security in mind, Brave automatically blocks ads and trackers which also makes it faster,
As Brave naturally blocks unwanted content from appearing in your browser, it prevents these trackers and pop-ups from slowing Download your user experience. It's also designed in a way that strips Downloaden which data is being loaded each time you use it. Without these components
The Future of Repair: Transparent and Incremental by Botond DenesScyllaDB
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Regularly run repairs are essential to keep clusters healthy, yet having a good repair schedule is more challenging than it should be. Repairs often take a long time, preventing running them often. This has an impact on data consistency and also limits the usefulness of the new repair based tombstone garbage collection. We want to address these challenges by making repairs incremental and allowing for automatic repair scheduling, without relying on external tools.
Replacing RocksDB with ScyllaDB in Kafka Streams by Almog GavraScyllaDB
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Learn how Responsive replaced embedded RocksDB with ScyllaDB in Kafka Streams, simplifying the architecture and unlocking massive availability and scale. The talk covers unbundling stream processors, key ScyllaDB features tested, and lessons learned from the transition.
World Information Architecture Day 2025 - UX at a CrossroadsJoshua Randall
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User Experience stands at a crossroads: will we live up to our potential to design a better world? or will we be co-opted by product management or another business buzzword?
Looking backwards, this talk will show how UX has repeatedly failed to create a better world, drawing on industry data from Nielsen Norman Group, Baymard, MeasuringU, WebAIM, and others.
Looking forwards, this talk will argue that UX must resist hype, say no more often and collaborate less often (you read that right), and become a true profession in order to be able to design a better world.
Inside Freshworks' Migration from Cassandra to ScyllaDB by Premkumar PatturajScyllaDB
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Freshworks migrated from Cassandra to ScyllaDB to handle growing audit log data efficiently. Cassandra required frequent scaling, complex repairs, and had non-linear scaling. ScyllaDB reduced costs with fewer machines and improved operations. Using Zero Downtime Migration (ZDM), they bulk-migrated data, performed dual writes, and validated consistency.
4. PhotosphereRadiates most of the sunlight we see surfaceGranules small, bright markings about the size of texas.
5. ChromosphereAbove photosphereThin layer of hot gasesViewed as a red rim around sunSpicules located on top of the chromosphere flaming structures. (described as trees sticking out)
6. CoronaOuter part of sun (atmosphere)Looks like a crown of bright light glowingSolar wind particles(ionized gases) escaping the corona at high speeds. Ionized referes to the gaining or losing of electrons.
12. InteriorSource of energy nuclear fusion process to fuse particles together to form heavier particles. Hydrogen Helium Proton-Proton Chain is created through nuclear fusion. Chain reaction converts 4 hydrogen protons into the nucleus of a helium atom. Some mass is converted to energy.
13. P-P Chain Cont.When hydrogen is converted to helium, this process Hydrogen burning.The energy that is released from the P-P chain is transmitted through layers of the sun.
14. What Does the Sun do for Earth?Energy light Food lifeEvents Good/BadAurorasSolar EclipsesDisruption of Radio/Satellite communications
15. AurorasEffects from strong solar flares lights up Earths atmosphereNorthern/Southern lights North/South PoleVaries in shapes, sizes, and colorsAurora AustralisAurora Borealishttp://www.itsnature.org/travel/wp-content/uploads/2010/10/p6133sv.jpghttp://geology.com/nasa/aurora-borealis.shtml
16. Solar EclipseEclipse of the sunAlignment between Earth-Moon-SunNew Moon Phase casts dark shadow on Earthhttp://en.wikipedia.org/wiki/Solar_eclipse
17. Disruption of Radio/Satellite Communications Solar flares large outburst of particles can reach Earth affecting radio and satellite communications. Very rare events
18. SummarySun has 4 major layersSolar activities may include: prominences, sunspots, and solar flaresNuclear fusion and P-P chainEvents auroras, solar eclipses, and disruption in radio or satellite communications due to solar flares