Here are the sources formatted in APA style:
24 X 7. (n.d.). Jupiter. FactMonster. http://www.factmonster.com/dk/science/encyclopedia/jupiter.html
Baquedano, E. (1993). Aztec, Inca & Maya. Knopf.
Jet Propulsion Laboratory. (n.d.). Cassini Solstice Mission: About Saturn & Its Moons. NASA. http://saturn.jpl.nasa.gov/science/index.cfm?SciencePageID=73
Space.com Staff. (2012, May 2). Jupiter, Largest Planet of the Solar System. Space.com.
Climate Impact of Software Testing at Nordic Testing DaysKari Kakkonen
My slides at Nordic Testing Days 6.6.2024
Climate impact / sustainability of software testing discussed on the talk. ICT and testing must carry their part of global responsibility to help with the climat warming. We can minimize the carbon footprint but we can also have a carbon handprint, a positive impact on the climate. Quality characteristics can be added with sustainability, and then measured continuously. Test environments can be used less, and in smaller scale and on demand. Test techniques can be used in optimizing or minimizing number of tests. Test automation can be used to speed up testing.
In the rapidly evolving landscape of technologies, XML continues to play a vital role in structuring, storing, and transporting data across diverse systems. The recent advancements in artificial intelligence (AI) present new methodologies for enhancing XML development workflows, introducing efficiency, automation, and intelligent capabilities. This presentation will outline the scope and perspective of utilizing AI in XML development. The potential benefits and the possible pitfalls will be highlighted, providing a balanced view of the subject.
We will explore the capabilities of AI in understanding XML markup languages and autonomously creating structured XML content. Additionally, we will examine the capacity of AI to enrich plain text with appropriate XML markup. Practical examples and methodological guidelines will be provided to elucidate how AI can be effectively prompted to interpret and generate accurate XML markup.
Further emphasis will be placed on the role of AI in developing XSLT, or schemas such as XSD and Schematron. We will address the techniques and strategies adopted to create prompts for generating code, explaining code, or refactoring the code, and the results achieved.
The discussion will extend to how AI can be used to transform XML content. In particular, the focus will be on the use of AI XPath extension functions in XSLT, Schematron, Schematron Quick Fixes, or for XML content refactoring.
The presentation aims to deliver a comprehensive overview of AI usage in XML development, providing attendees with the necessary knowledge to make informed decisions. Whether you’re at the early stages of adopting AI or considering integrating it in advanced XML development, this presentation will cover all levels of expertise.
By highlighting the potential advantages and challenges of integrating AI with XML development tools and languages, the presentation seeks to inspire thoughtful conversation around the future of XML development. We’ll not only delve into the technical aspects of AI-powered XML development but also discuss practical implications and possible future directions.
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.
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.
Observability Concepts EVERY Developer Should Know -- DeveloperWeek Europe.pdfPaige Cruz
Monitoring and observability aren’t traditionally found in software curriculums and many of us cobble this knowledge together from whatever vendor or ecosystem we were first introduced to and whatever is a part of your current company’s observability stack.
While the dev and ops silo continues to crumble….many organizations still relegate monitoring & observability as the purview of ops, infra and SRE teams. This is a mistake - achieving a highly observable system requires collaboration up and down the stack.
I, a former op, would like to extend an invitation to all application developers to join the observability party will share these foundational concepts to build on:
Unlocking Productivity: Leveraging the Potential of Copilot in Microsoft 365, a presentation by Christoforos Vlachos, Senior Solutions Manager – Modern Workplace, Uni Systems
Alt. GDG Cloud Southlake #33: Boule & Rebala: Effective AppSec in SDLC using ...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.
UiPath Test Automation using UiPath Test Suite series, part 5DianaGray10
Welcome to UiPath Test Automation using UiPath Test Suite series part 5. In this session, we will cover CI/CD with devops.
Topics covered:
CI/CD with in UiPath
End-to-end overview of CI/CD pipeline with Azure devops
Speaker:
Lyndsey Byblow, Test Suite Sales Engineer @ UiPath, Inc.
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.
Sudheer Mechineni, Head of Application Frameworks, Standard Chartered Bank
Discover how Standard Chartered Bank harnessed the power of Neo4j to transform complex data access challenges into a dynamic, scalable graph database solution. This keynote will cover their journey from initial adoption to deploying a fully automated, enterprise-grade causal cluster, highlighting key strategies for modelling organisational changes and ensuring robust disaster recovery. Learn how these innovations have not only enhanced Standard Chartered Bank’s data infrastructure but also positioned them as pioneers in the banking sector’s adoption of graph technology.
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
How to Get CNIC Information System with Paksim Ga.pptxdanishmna97
Pakdata Cf is a groundbreaking system designed to streamline and facilitate access to CNIC information. This innovative platform leverages advanced technology to provide users with efficient and secure access to their CNIC details.
Essentials of Automations: The Art of Triggers and Actions in FMESafe Software
In this second installment of our Essentials of Automations webinar series, we’ll explore the landscape of triggers and actions, guiding you through the nuances of authoring and adapting workspaces for seamless automations. Gain an understanding of the full spectrum of triggers and actions available in FME, empowering you to enhance your workspaces for efficient automation.
We’ll kick things off by showcasing the most commonly used event-based triggers, introducing you to various automation workflows like manual triggers, schedules, directory watchers, and more. Plus, see how these elements play out in real scenarios.
Whether you’re tweaking your current setup or building from the ground up, this session will arm you with the tools and insights needed to transform your FME usage into a powerhouse of productivity. Join us to discover effective strategies that simplify complex processes, enhancing your productivity and transforming your data management practices with FME. Let’s turn complexity into clarity and make your workspaces work wonders!
Threats to mobile devices are more prevalent and increasing in scope and complexity. Users of mobile devices desire to take full advantage of the features
available on those devices, but many of the features provide convenience and capability but sacrifice security. This best practices guide outlines steps the users can take to better protect personal devices and information.
3. Mercury, the closest planet to the sun, has a
core made of liquid iron that surprisingly takes
up about ¾ of the planet’s diameter, it is as big
as our moon, and it takes up 70% of its weight.
Its mantle is made of silica.
It has a rocky crust made of silicate rocks. It is
about 350 miles thick and it is covered with
many craters and dents.
Mercury’s atmosphere is composed of very small
amounts of hydrogen, oxygen, helium and
sodium.
4. Core Mantle –
¾ of made of silica
Mercury’s
Total diameter.
Made of liquid iron
Crust
350 miles
Thick . Made of
Silicate rocks
5. Even though Mercury is the closest planet to the sun, it
is not the hottest. Its atmosphere is very thin and it
cannot trap solar heat.
Mercury’s hot side (the side that is facing the Sun)
experiences the most extreme temperatures. It can
reach temperatures as high as 700° Kelvin.
Mercury receives 6.5 times the amount of sunlight that
the Earth does.
6. On the dark side of the planet, temperatures can fall to
as low as 100° K, making it the coldest of all the inner
planets
Researchers think there are craters dotting the north
and south poles that have temperatures as low as 90°K.
The average temperature of Mercury averages to
around 452°K!
7.
8. Venus is one of the brightest things in the sky (besides
the sun and moon). If you know where to look, you
can see it at daytime.
Venus’ atmosphere is composed of 96% carbon dioxide
and 4% nitrogen, and is 90% denser than Earth’s.
The pressure is the same as the pressure if you were a
kilometer below sea-level on Earth, which is not
survivable for humans.
The interior of Venus is composed of a central iron
core and a molten rocky mantle, similar to the
composition of Earth.
9. The surface of Venus may have been formed by a lot of
volcanic activity. It is said to have 167 volcanoes that
measure up to 100 km across.
Venus is sometimes referred as Earth’s sister planet
because not only is Venus similar in size to Earth, but
scientists think that a long time ago, Venus had
tectonic plates and liquid water. Venus may have
become the way it is by having a massive greenhouse
gas affect, vaporizing all of the water and messing up
the tectonic plates.
10. Crust-
50 km thick.
Core-
Made of
iron.
3,000 km
across
Mantle-
3,000 km
thick
11. Venus’ atmosphere being so dense results in a severe
greenhouse affect making Venus the hottest planet in
our solar system
The average surface temperature of Venus is 735°
Kelvin
Venus’ very slight axial tilt means that it receives the
same amount of energy from the Sun no matter what
time of year it is so it is always HOT.
12. The atmosphere is covered in clouds made up of
sulfuric acid and other corrosive substances resulting
in acid rain.
Along with extreme heat and acid rain, Venus can have
winds at speeds of 100 meters per second!
13.
14. Mars lacks a magnetic field and because of this it is
constantly bombarded by radiation
The Martian core is solid and is thought to be 2,960
km in diameter.
The mantle is believed to be fairly soft, kind of like a
rock paste. No one knows how thick it is.
Its crust is basalt and contains just enough iron oxide
to give it its reddish hue.
15. Core-
Mantle- Mostly made of
Made of a Sulfur and iron
Rock paste
Crust-
Made of basalt and
iron oxide
16. Average temperature: -67 °F
On summer days, it can be around 20 degrees Celsius
then plummet to -90 C at night
Even at the equator, the night time temperatures fall
well below zero.
Has seasons because its axial tilt is similar to ours
Mars’ atmosphere is over 96% carbon dioxide. If the
planet could retain heat, the carbon dioxide would
cause a greenhouse effect and the planet would end up
like Venus
17.
18.
19. Its atmosphere resembles that of the sun, made up
mostly of hydrogen and helium.
Jupiter could hold more than 1,300 Earths.
Jupiter's gargantuan magnetic field is the strongest of
all the planets in the solar system at nearly 2,000 times
the strength of Earth’s.
Jupiter’s rocky iron core is surrounded by a helium-
rich layer of fluid metallic hydrogen, wrapped up in an
atmosphere primarily made of molecular hydrogen.
There isn’t really any terrain because it is gas
20.
21. The colorful bands of Jupiter are arranged in dark belts
and light zones that are created by strong east-west
winds in the planet's upper atmosphere , which travel
more than 400 miles per hour.
The white clouds in the zones are made of crystals of
frozen ammonia.
Darker clouds of other chemicals are found in the
belts.
The deepest visible level holds blue clouds
22. The Great Red Spot is a giant storm that has lasted
for more than 300 years. At its widest, the Great Red
Spot is 3 times the diameter of Earth. Its color which
usually varies from brick red to slightly brown, may
come from small amounts of sulfur and phosphorus in
the ammonia crystals in Jupiter's clouds.
Every now and again, the Great Red Spot seems to fade
entirely.
23.
24. Io is the most volcanically active body is the solar
system
3rd largest of Jupiter’s moons.
The volcanic plumes rise 300 km (190 miles) above the
surface
Io is constantly renewing its surface filling in any
impact craters with molten lava lakes
Know one knows what the volcanos spew out.
Sulfur dioxide is the primary thing in Io’s thin
atmosphere
It has no water.
25.
26. Slightly smaller that Earth’s moon
Europa is thought to have a iron core, a rocky mantle
and on its surface, a salt water ocean.
The ocean is deep enough to cover the surface of the
entire planet but since it is far from the sun, it is frozen
over.
The ocean could possible support life forms
27.
28. It has a inner rocky core which is surrounded by a large
icy mantle.
Callisto is twice as bright as our own Moon.
Callisto is the most heavily cratered object in our solar
system
It has a surface is 4 billion years old
It has no atmosphere or tectonics
29.
30. It’s larger than Mercury and Pluto
Thought to have a thin oxygen atmosphere. It’s not
thick enough to support life though
Its core is metallic metal. Its mantle is made of
rock, and the crust is made of ice. The ice sheet is
thought to be 800 km thick might contain some rock
as well
31.
32.
33. 96% of the planet is made of hydrogen. The other 4
percent is oxygen and other stuff.
61 moons known
Divided into layers
The first layer has ammonia crystals. Right bellow it is
water and ammonium hydro-sulfide.
Under that, pressure can so high, the hydrogen is
compressed into a liquid
Under that is metallic hydrogen
People think the core is made of rock and metal
elements, but they don’t know for sure
34.
35. Mostly made of water ice, chemicals, and dust
particles
Size of particles range from a few micrometers to a few
meters big.
5 rings:
D ring- closest ring to Saturn, 7,500 km wide
A ring- There are 2 gaps within the A ring: Encke gap
and Keeler gap
C ring-Very faint, made of darker materials
B ring-Largest and brightest, 25,500 km wide.
F ring-Outermost ring, estimated 30-500km thick
36.
37. Saturn’s largest moon
Frozen version of Earth
Occasionally forms clouds and rains
Developed an orange haze of smog
Has erosion from liquid
Surface shaped by rivers and lakes
38.
39. Surface covered with clean ice
Reflects 100% of the light that hits it
Has an atmosphere
Interior of the moon is thought to be liquid
Heated by a tidal mechanism
40.
41. Composed of water ice and a little rock
Average temperature is -305 degrees Fahrenheit
Small moon
42.
43. One side is dark and has a slight reddish color
The other side is bright
Think the dark side is material that oozed from
Iapetus’s insides
44.
45.
46. Third largest planet in the solar system
Not visible the naked eye
It doesn’t really have any terrain
Made of various ices, like water, ammonia and
methane
People think it has a solid core
Regions of the core experience pressure of 8 million
bars, and have a temperature of 5,000 Kelvin
47. If you tried to land a spaceship of Uranus you would
fall through the upper atmosphere of hydrogen and
helium, and into the liquid icy center.
Has large amounts of methane it its atmosphere
48.
49. Has an most extreme axial tilt of 98° so it has seasons
Each pole has 42 Earth years of light and 42 Earth
years of darkness
Has an unusually cold temperature
Average temperature on Uranus is -224° Celsius
Has huge wind storms, with wind speeds reaching as
much as 900 km/hr
Again, DON’T LAUGH
50.
51. The atmosphere in Neptune is composed of 80%
hydrogen 19% helium, and 1% methane.
Blue because the methane absorbs the color red
Upper-level of Neptune has methane clouds
If the pressure is more than 5 bars, ammonium
sulfide, hydrogen sulfide and water clouds may form.
Clouds of water-ice may form at 50 bars of pressure.
Has no terrain
A spaceship would sink right through Neptune and hit
its core
Has very faint rings
54. The mean temperature of the planet is 73° K (-200°
Celsius
The temperature of Neptune can reach as low as 55°
Kelvin
The temperature at South Pole are -10° C warmer than
the rest of the planet because it is currently titled
towards the Sun.
At the core temperatures reach 7000° C
The difference in temperature between the core and
the surface cause winds as fast as 2100 km/hr.
55. What do you get if you cross Santa Clause with a space
ship?
What is an astronaut's favorite part of a computer?
How do we know Saturn has married more than once?
What do you call a crazy moon?
Why did the robot cross the road
56. "24 X 7." JUPITER — FactMonster.com. Web. 02 May 2012.
<http://www.factmonster.com/dk/science/encyclopedia/jupiter.html
>.
Baquedano, Elizabeth. Aztec, Inca & Maya. New York: Knopf, 1993.
Print.
"Jet Propulsion Laboratory." Cassini Solstice Mission: About Saturn &
Its Moons. Web. 02 May 2012.
<http://saturn.jpl.nasa.gov/science/index.cfm?SciencePageID=73>.
"Jupiter, Largest Planet of the Solar System." Space.com. Web. 02 May
2012. <http://www.space.com/7-jupiter-largest-planet-solar-
system.html>.
"Planet Facts – Fun & Interesting Information About the Nine
Planets." Planet Facts – Fun & Interesting Information About the
Nine Planets. Web. 02 May 2012. <http://planetfacts.org>.
"Royal Museums Greenwich: Sea, Ships, Time and the Stars : RMG."
Royal Museums Greenwich: Sea, Ships, Time and the Stars : RMG.
Web. 02 May 2012.
<http://www.rmg.co.uk/server/show/conMediaFile.3932>.
"Space and Astronomy News." Universe Today. Web. 02 May 2012.
<http://www.universetoday.com>.
57. "Iapetus, A Moon of Saturn." Views of the Solar
System. Web. 02 May 2012.
<http://www.solarviews.com/eng/iapetus.htm>.
"Space Jokes!" Puzzle Pixies : Free Kids
Painting, Coloring, Games, Puzzles and Activities. Web.
02 May 2012.
<http://www.puzzlepixies.com/jokes/jokes/space-
jokes.html>.