1) The document describes the key features of planets in our solar system from Mercury to Pluto. Mercury is the closest planet to the sun and has extreme temperature variations. Venus has a dense atmosphere that causes a strong greenhouse effect. Earth has water and atmosphere that supports life. Mars has the largest volcano and seasons due to its tilt. Jupiter is the largest planet and has many moons including the volcanic Io. Saturn has rings composed of ice and rock and over 47 moons including Titan, larger than Mercury. Uranus has rings and its atmosphere gives it a blue-green color. Neptune also appears blue-green and has the Great Dark Spot storm. Pluto is the smallest and most distant planet from the sun.
Grade 8 Integrated Science Chapter 11 Lesson 3 on the outer planets. This lesson discusses the four outer planets. It gives details on their composition, atmosphere, rings, moons, and other identifying details.
Grade 8 Integrated Science Chapter 11 Lesson 2 on the inner planets. Discusses the four inner planets, their atmosphere, interior, surface, weather, and other defining features. Includes individual slides on Mercury, Venus, Earth and Mars.
SPACE IS AMAZING!! PLANETS ARE A PART OF IT! LETS LEARN ABOUT IT.PrishaGupta4
> Earth a 'Planet' is what we live in! So we should know about it completely!
> Lets know about each planet a little bit in detail that would amaze you a lot!!!!
>This ppt even tells you about Pluto!
> So lets start!!!
Grade 8 Integrated Science Chapter 11 Lesson 3 on the outer planets. This lesson discusses the four outer planets. It gives details on their composition, atmosphere, rings, moons, and other identifying details.
Grade 8 Integrated Science Chapter 11 Lesson 2 on the inner planets. Discusses the four inner planets, their atmosphere, interior, surface, weather, and other defining features. Includes individual slides on Mercury, Venus, Earth and Mars.
SPACE IS AMAZING!! PLANETS ARE A PART OF IT! LETS LEARN ABOUT IT.PrishaGupta4
> Earth a 'Planet' is what we live in! So we should know about it completely!
> Lets know about each planet a little bit in detail that would amaze you a lot!!!!
>This ppt even tells you about Pluto!
> So lets start!!!
Generative AI Deep Dive: Advancing from Proof of Concept to ProductionAggregage
Join Maher Hanafi, VP of Engineering at Betterworks, in this new session where he'll share a practical framework to transform Gen AI prototypes into impactful products! He'll delve into the complexities of data collection and management, model selection and optimization, and ensuring security, scalability, and responsible use.
Communications Mining Series - Zero to Hero - Session 1DianaGray10
This session provides introduction to UiPath Communication Mining, importance and platform overview. You will acquire a good understand of the phases in Communication Mining as we go over the platform with you. Topics covered:
• Communication Mining Overview
• Why is it important?
• How can it help today’s business and the benefits
• Phases in Communication Mining
• Demo on Platform overview
• Q/A
Pushing the limits of ePRTC: 100ns holdover for 100 daysAdtran
At WSTS 2024, Alon Stern explored the topic of parametric holdover and explained how recent research findings can be implemented in real-world PNT networks to achieve 100 nanoseconds of accuracy for up to 100 days.
In his public lecture, Christian Timmerer provides insights into the fascinating history of video streaming, starting from its humble beginnings before YouTube to the groundbreaking technologies that now dominate platforms like Netflix and ORF ON. Timmerer also presents provocative contributions of his own that have significantly influenced the industry. He concludes by looking at future challenges and invites the audience to join in a discussion.
Removing Uninteresting Bytes in Software FuzzingAftab Hussain
Imagine a world where software fuzzing, the process of mutating bytes in test seeds to uncover hidden and erroneous program behaviors, becomes faster and more effective. A lot depends on the initial seeds, which can significantly dictate the trajectory of a fuzzing campaign, particularly in terms of how long it takes to uncover interesting behaviour in your code. We introduce DIAR, a technique designed to speedup fuzzing campaigns by pinpointing and eliminating those uninteresting bytes in the seeds. Picture this: instead of wasting valuable resources on meaningless mutations in large, bloated seeds, DIAR removes the unnecessary bytes, streamlining the entire process.
In this work, we equipped AFL, a popular fuzzer, with DIAR and examined two critical Linux libraries -- Libxml's xmllint, a tool for parsing xml documents, and Binutil's readelf, an essential debugging and security analysis command-line tool used to display detailed information about ELF (Executable and Linkable Format). Our preliminary results show that AFL+DIAR does not only discover new paths more quickly but also achieves higher coverage overall. This work thus showcases how starting with lean and optimized seeds can lead to faster, more comprehensive fuzzing campaigns -- and DIAR helps you find such seeds.
- These are slides of the talk given at IEEE International Conference on Software Testing Verification and Validation Workshop, ICSTW 2022.
Securing your Kubernetes cluster_ a step-by-step guide to success !KatiaHIMEUR1
Today, after several years of existence, an extremely active community and an ultra-dynamic ecosystem, Kubernetes has established itself as the de facto standard in container orchestration. Thanks to a wide range of managed services, it has never been so easy to set up a ready-to-use Kubernetes cluster.
However, this ease of use means that the subject of security in Kubernetes is often left for later, or even neglected. This exposes companies to significant risks.
In this talk, I'll show you step-by-step how to secure your Kubernetes cluster for greater peace of mind and reliability.
GraphSummit Singapore | The Art of the Possible with Graph - Q2 2024Neo4j
Neha Bajwa, Vice President of Product Marketing, Neo4j
Join us as we explore breakthrough innovations enabled by interconnected data and AI. Discover firsthand how organizations use relationships in data to uncover contextual insights and solve our most pressing challenges – from optimizing supply chains, detecting fraud, and improving customer experiences to accelerating drug discoveries.
GraphSummit Singapore | The Future of Agility: Supercharging Digital Transfor...Neo4j
Leonard Jayamohan, Partner & Generative AI Lead, Deloitte
This keynote will reveal how Deloitte leverages Neo4j’s graph power for groundbreaking digital twin solutions, achieving a staggering 100x performance boost. Discover the essential role knowledge graphs play in successful generative AI implementations. Plus, get an exclusive look at an innovative Neo4j + Generative AI solution Deloitte is developing in-house.
Epistemic Interaction - tuning interfaces to provide information for AI supportAlan Dix
Paper presented at SYNERGY workshop at AVI 2024, Genoa, Italy. 3rd June 2024
https://alandix.com/academic/papers/synergy2024-epistemic/
As machine learning integrates deeper into human-computer interactions, the concept of epistemic interaction emerges, aiming to refine these interactions to enhance system adaptability. This approach encourages minor, intentional adjustments in user behaviour to enrich the data available for system learning. This paper introduces epistemic interaction within the context of human-system communication, illustrating how deliberate interaction design can improve system understanding and adaptation. Through concrete examples, we demonstrate the potential of epistemic interaction to significantly advance human-computer interaction by leveraging intuitive human communication strategies to inform system design and functionality, offering a novel pathway for enriching user-system engagements.
Smart TV Buyer Insights Survey 2024 by 91mobiles.pdf91mobiles
91mobiles recently conducted a Smart TV Buyer Insights Survey in which we asked over 3,000 respondents about the TV they own, aspects they look at on a new TV, and their TV buying preferences.
LF Energy Webinar: Electrical Grid Modelling and Simulation Through PowSyBl -...DanBrown980551
Do you want to learn how to model and simulate an electrical network from scratch in under an hour?
Then welcome to this PowSyBl workshop, hosted by Rte, the French Transmission System Operator (TSO)!
During the webinar, you will discover the PowSyBl ecosystem as well as handle and study an electrical network through an interactive Python notebook.
PowSyBl is an open source project hosted by LF Energy, which offers a comprehensive set of features for electrical grid modelling and simulation. Among other advanced features, PowSyBl provides:
- A fully editable and extendable library for grid component modelling;
- Visualization tools to display your network;
- Grid simulation tools, such as power flows, security analyses (with or without remedial actions) and sensitivity analyses;
The framework is mostly written in Java, with a Python binding so that Python developers can access PowSyBl functionalities as well.
What you will learn during the webinar:
- For beginners: discover PowSyBl's functionalities through a quick general presentation and the notebook, without needing any expert coding skills;
- For advanced developers: master the skills to efficiently apply PowSyBl functionalities to your real-world scenarios.
The Art of the Pitch: WordPress Relationships and SalesLaura Byrne
Clients don’t know what they don’t know. What web solutions are right for them? How does WordPress come into the picture? How do you make sure you understand scope and timeline? What do you do if sometime changes?
All these questions and more will be explored as we talk about matching clients’ needs with what your agency offers without pulling teeth or pulling your hair out. Practical tips, and strategies for successful relationship building that leads to closing the deal.
A tale of scale & speed: How the US Navy is enabling software delivery from l...sonjaschweigert1
Rapid and secure feature delivery is a goal across every application team and every branch of the DoD. The Navy’s DevSecOps platform, Party Barge, has achieved:
- Reduction in onboarding time from 5 weeks to 1 day
- Improved developer experience and productivity through actionable findings and reduction of false positives
- Maintenance of superior security standards and inherent policy enforcement with Authorization to Operate (ATO)
Development teams can ship efficiently and ensure applications are cyber ready for Navy Authorizing Officials (AOs). In this webinar, Sigma Defense and Anchore will give attendees a look behind the scenes and demo secure pipeline automation and security artifacts that speed up application ATO and time to production.
We will cover:
- How to remove silos in DevSecOps
- How to build efficient development pipeline roles and component templates
- How to deliver security artifacts that matter for ATO’s (SBOMs, vulnerability reports, and policy evidence)
- How to streamline operations with automated policy checks on container images
GraphRAG is All You need? LLM & Knowledge GraphGuy Korland
Guy Korland, CEO and Co-founder of FalkorDB, will review two articles on the integration of language models with knowledge graphs.
1. Unifying Large Language Models and Knowledge Graphs: A Roadmap.
https://arxiv.org/abs/2306.08302
2. Microsoft Research's GraphRAG paper and a review paper on various uses of knowledge graphs:
https://www.microsoft.com/en-us/research/blog/graphrag-unlocking-llm-discovery-on-narrative-private-data/
GDG Cloud Southlake #33: Boule & Rebala: Effective AppSec in SDLC using Deplo...James Anderson
Effective Application Security in Software Delivery lifecycle using Deployment Firewall and DBOM
The modern software delivery process (or the CI/CD process) includes many tools, distributed teams, open-source code, and cloud platforms. Constant focus on speed to release software to market, along with the traditional slow and manual security checks has caused gaps in continuous security as an important piece in the software supply chain. Today organizations feel more susceptible to external and internal cyber threats due to the vast attack surface in their applications supply chain and the lack of end-to-end governance and risk management.
The software team must secure its software delivery process to avoid vulnerability and security breaches. This needs to be achieved with existing tool chains and without extensive rework of the delivery processes. This talk will present strategies and techniques for providing visibility into the true risk of the existing vulnerabilities, preventing the introduction of security issues in the software, resolving vulnerabilities in production environments quickly, and capturing the deployment bill of materials (DBOM).
Speakers:
Bob Boule
Robert Boule is a technology enthusiast with PASSION for technology and making things work along with a knack for helping others understand how things work. He comes with around 20 years of solution engineering experience in application security, software continuous delivery, and SaaS platforms. He is known for his dynamic presentations in CI/CD and application security integrated in software delivery lifecycle.
Gopinath Rebala
Gopinath Rebala is the CTO of OpsMx, where he has overall responsibility for the machine learning and data processing architectures for Secure Software Delivery. Gopi also has a strong connection with our customers, leading design and architecture for strategic implementations. Gopi is a frequent speaker and well-known leader in continuous delivery and integrating security into software delivery.
2. Mercury Mercury is the closest planet to the Sun. Mercury was photographed by Mariner 10 it photographed 45% of its surface, and it showed us that Mercury had a lot of craters just like our moon. It has cliffs as high as 3 km, it was formed when mercury shrank. Mercury does not have an atmosphere either.So without an atmosphere and since it is so close to the Sun the temperatures can go from 425C to -174C.
3. Venus The second nearest to the Sun is Venus. They call Venus “Earth’s twin”, because the size and mass of Venus is around the same as Earth’s. Maat Mons is the highest volcano on Venus, lava flows across hundreds of kilometers. The clouds on Venus are so dense little of the sunlight reaches the surface of Venus. The light that does get through, heats up the surface and gives off heat to the atmosphere, a lot of the heat is absorbed by carbon dioxide in Venus’ atmosphere. So this causes a greenhouse effect like the one on Earth. Since the greenhouse effect is so serious, the temperatures go from 450C to 475C.
4. Earth Earth is the third closest planet to the Sun. It is about 150 million km from the Sun. It has water, which can support life. Earth’s atmosphere causes most meteors to burn up in the atmosphere before reaching the surface. It’s ozone layer protects life from the Sun’s radiation.
5. Mars The reason why Mars is red, because the iron oxide in the soil give a reddish color. Mariner 9 showed canals most likely carved by flowing water. It also discovered the largest volcano in the solar system, a volcano called Olympus Mons, but it probably extinct. They also discovered large rift valleys. Mars’ atmosphere is thinner than Earth’s, it is made up of mostly carbon dioxide with some nitrogen and argon. The temperatures go from -125C to 35C. Mars has a 25 degree tilt, so that means like Earth it has a seasonal variation.
6. Jupiter Callisto Ganymede Europa Io Jupiter is the largest planet in our solor system. It’s atmosphere is mostly made of hydrogen, helium, ammonia, methane, and water vapor. The clouds on Earth are very colorful, it also has continuous storms, such as the “Great Red Spot”. It also has 63 different moons but the biggest four are: Io, Europa, Ganymede, Callisto. Io gets heat up by the gravitational pull that it is known as the most active volcano in our solar system. Europa is mostly made of rock and a thick crust of ice. Under the ice might be a ocean as deep as 50 km. Ganymede is the largest moon in the solar system, it is even larger than Mercury. Callisto is mostly made up off ice and rock, it also has many craters inside it too.
7. Saturn Saturn is the second largest planet in the solar system. Saturn’s atmosphere is mostly composed of hydrogen and helium. Much like Jupiter’s atmosphere it also contains ammonia, methane, and water vapor. When you get deeper into the atmosphere the gases become liquid hydrogen and liquid helium. Saturn has several rings, each large ring is made up of thousands of smaller rings. Saturn’s rings are composed of thousands of ice and rock particles. There are around 47 moons orbiting Saturn. The largest moon on Saturn is a moon called Titan, it is larger than Mercury.
8. Uranus Uranus is a large planet, it has 27 moons with dark rings. It’s largest moon is Titania, it has many deep valleys and craters. Uranus has 11 rings surrounding it’s equator. The atmosphere there is composed up of hydrogen, helium, and a little methane. Methane give the turquoise color that we see on Uranus. It is blue because the methane absorbs the red and yellow light, and the clouds reflect the green and blue light. Uranus is mostly made up of rocks and ices. It’s axis is very different than other planets, its axis is tiled on the side, some scientists believe that it collided with something which caused it to be tilted like this.
9. Neptune Neptune’s atmosphere is composed of hydrogen and helium, with small amounts of methane, just like Uranus.Also like Uranus, the methane gives Neptune its turquoise color. Also like Jupiter it has dark colored storms, one of them is called the Great Dark Spot. Neptune’s surface is mostly composed of rock and different types of ices made from methane and ammonia. Neptune has at least 13 moons, it’s biggest one is called Triton. Neptune has dark rings which are pretty young and won’t last very long either.
10. Pluto Pluto is the smallest planet within the other planets, it also is the farthest away from the Sun too. It has a diameter of 2,300 km, it also takes about 248 years for one orbit around the Sun. It has a thin atmosphere, it also has a solid, icy/rocky surface. Pluto has 3 moons: Charon,, Hydra, and Nix.The largest of the 3 is Charon, it has a diameter of 1,200 km and orbits Pluto from 19,500 km away.