Assignment 1 Worksheet (100 points)From the Text (40 total pdesteinbrook
Assignment 1 Worksheet (100 points)
From the Text (40 total points; 4 points each):
Chapter 1: Questions for Review (pg. 26)
3) List the four most abundant gases in today’s atmosphere.
9) What are the two most abundant greenhouse gases in the atmosphere?
10)
a) Explain the concept of air pressure in terms of weight of air above some level.
b) Why does air pressure always decrease with increasing height above the surface?
19) How does weather differ from climate?
Chapter 1: Questions for Thought and Exploration (pg. 27)
3) Which of the following statements relate more to weather and which relate more to climate?
a) The summers here are warm and humid.
b) Cumulus clouds presently cover the entire sky.
c) Our lowest temperature last winter was -29 °C (-18°F).
d) The air temperature outside is 22 °C (72 °F).
e) December is our foggiest month.
f) The highest temperature ever recorded in Pheonixville, Pennsylvania, was 44 °C (111 °F)
on July 10, 1936.
g) Snow is falling at the rate of 5 cm (2 in.) per hour.
h) The average temperature for the month of January in Chicago, Illinois, is -3 °C (26 °F).
Chapter 2: Questions for Review (pg. 55-56)
1) Distinguish between temperature and heat.
3) Explain how heat is transferred in our atmosphere by:
a) Conduction
b) Convection
c) Radiation
6) How does the amount of radiation emitted by the Earth differ from that emitted by the Sun?
20) During the Northern Hemisphere’s summer, the daylight hours in northern latitudes are
longer than in middle latitudes. Explain why northern latitudes are not warmer.
Chapter 2: Questions for Thought and Exploration (pg. 56)
5) Which do you feel would have the greatest effect on the Earth’s greenhouse effect: removing
all of the CO2 from the atmosphere or removing all of the water vapor? Explain your answer.
Short Answer (40 total points; 10 points each):
1. Describe the nature of the temperature lapse rate in each of the four layers of the atmosphere (Troposphere; Stratosphere; Mesosphere; Thermosphere), and why the Tropospheric and Stratospheric temperatures change the way they do.
2. Using Figure 1.8 from your textbook, find the approximate altitude in BOTH kilometers and miles for the following atmospheric pressures
Altitude (above sea level) (km)
Altitude (above sea level) (miles)
800 mb
500 mb
250 mb
1 mb
The Tropopause and Stratopause
3. Explain how the Greenhouse Effect works and why the term ‘greenhouse’ isn’t the most representative of the process. (Hint: start reading page 39). Make sure to describe what type of radiation greenhouse gases do, and do not interact with, as well as the sources for those types of radiation.
4. Challenge question: Pretend you are the first scientist to observe the temperature of the Moon. The first thing you should do is compare the Moon’s temperature with temperatures on Earth. List units!
a. In your “log” below, list the temperature range for the Sur ...
Assignment 1 Worksheet (100 points)From the Text (40 total pdesteinbrook
Assignment 1 Worksheet (100 points)
From the Text (40 total points; 4 points each):
Chapter 1: Questions for Review (pg. 26)
3) List the four most abundant gases in today’s atmosphere.
9) What are the two most abundant greenhouse gases in the atmosphere?
10)
a) Explain the concept of air pressure in terms of weight of air above some level.
b) Why does air pressure always decrease with increasing height above the surface?
19) How does weather differ from climate?
Chapter 1: Questions for Thought and Exploration (pg. 27)
3) Which of the following statements relate more to weather and which relate more to climate?
a) The summers here are warm and humid.
b) Cumulus clouds presently cover the entire sky.
c) Our lowest temperature last winter was -29 °C (-18°F).
d) The air temperature outside is 22 °C (72 °F).
e) December is our foggiest month.
f) The highest temperature ever recorded in Pheonixville, Pennsylvania, was 44 °C (111 °F)
on July 10, 1936.
g) Snow is falling at the rate of 5 cm (2 in.) per hour.
h) The average temperature for the month of January in Chicago, Illinois, is -3 °C (26 °F).
Chapter 2: Questions for Review (pg. 55-56)
1) Distinguish between temperature and heat.
3) Explain how heat is transferred in our atmosphere by:
a) Conduction
b) Convection
c) Radiation
6) How does the amount of radiation emitted by the Earth differ from that emitted by the Sun?
20) During the Northern Hemisphere’s summer, the daylight hours in northern latitudes are
longer than in middle latitudes. Explain why northern latitudes are not warmer.
Chapter 2: Questions for Thought and Exploration (pg. 56)
5) Which do you feel would have the greatest effect on the Earth’s greenhouse effect: removing
all of the CO2 from the atmosphere or removing all of the water vapor? Explain your answer.
Short Answer (40 total points; 10 points each):
1. Describe the nature of the temperature lapse rate in each of the four layers of the atmosphere (Troposphere; Stratosphere; Mesosphere; Thermosphere), and why the Tropospheric and Stratospheric temperatures change the way they do.
2. Using Figure 1.8 from your textbook, find the approximate altitude in BOTH kilometers and miles for the following atmospheric pressures
Altitude (above sea level) (km)
Altitude (above sea level) (miles)
800 mb
500 mb
250 mb
1 mb
The Tropopause and Stratopause
3. Explain how the Greenhouse Effect works and why the term ‘greenhouse’ isn’t the most representative of the process. (Hint: start reading page 39). Make sure to describe what type of radiation greenhouse gases do, and do not interact with, as well as the sources for those types of radiation.
4. Challenge question: Pretend you are the first scientist to observe the temperature of the Moon. The first thing you should do is compare the Moon’s temperature with temperatures on Earth. List units!
a. In your “log” below, list the temperature range for the Sur ...
1 SPU 25 Energy and Climate Vision for the Future, Spri.docxhoney725342
1
SPU 25 Energy and Climate: Vision for the Future, Spring 2018
Homework Set #1 Climate Basics, DUE Monday 2/12 (1:00 pm in lecture)
Name: _____________________________________ Section: __________ TF: _____________________ Score: ______/_______
Collaborators: _________________________________________________________________________________________________
Earth’s climate is a complex reflection of the distribution and movement of energy around the planet. The
primary source of Earth’s energy is radiation from the Sun. In this problem set, you will see how this energy is
received, lost, and stored, and the role of greenhouse gases in altering the climate. You will also understand
how the distribution of energy influences climate and get some practice with basic quantitative problems and
unit conversions. (40 points total)
You will only receive credit if you show all your work and write legibly.
I. Earth’s Energy Balance
Planet Earth (including the solid earth, oceans, and atmosphere) is best described as an isolated system:
energy, but not mass, can pass from Earth to space and vice versa. In this type of system, the energy balance
may be described by: Energy gained = Energy lost – change in storage.
1. Greenhouse gases in the atmosphere prevent the radiation of energy to space, so they impact which
term in the above equation? (1 point)
2. Changing surface and ocean temperatures reflect which term in the above equation? (1 point)
II. Energy from the Sun
3. True or False: Summer is warmer than winter because the Earth is closer to the Sun. (1 point)
4. Currently, the energy from the Sun arriving at Earth’s orbital position amounts to 1,379 W m-2,
measured perpendicular to the direction of the sunlight (see figure below).
a. Given that the Earth is a circular target for this energy and has a radius of 6.38 x 103 km,
calculate the total rate at which solar energy is intercepted by the Earth. Report your answer in
Watts. Recall that the area of a circle is πr2. (2 points)
Figure 1. The shadow formed by an
illuminated sphere has a circular
shape with a radius R equal to the
radius of the sphere.
2
b. Assuming that the energy from the Sun is eventually distributed equally over the entire surface
area of the Earth, use your answer from part (a) to calculate the current average rate of
incoming solar radiation. Express your answer in Watts per meter squared. Recall that the
surface area of a sphere is 4πr2. (3 points)
III. The fate of energy from the Sun
5. Based on your answers from the previous problem and assuming a global average albedo of 0.3, how
much of the incoming solar radiation is reflected back into space? How much is absorbed? Express
your answers in Watts per meter squared. (2 points)
6. Much of the energy absorbed at the Earth’s surface is used for evaporation. The energy involved in
changing the phase of water is c ...
This presentation is based on the curriculum for K12 created by the Department of education. It includes simulation to better understand the concepts presented.
Maxwell Boltzmann Summary Answer the following questions anAbramMartino96
Maxwell Boltzmann: Summary
Answer the following questions and submit your responses as a PDF.
1. Write down one major conclusion you can draw from this week’s laboratory.
Please explain.
2. Describe the experimental evidence that supports your conclusion. Please
explain.
3. Give one example of applications/situations for the finding(s) you described
above in your everyday life outside of physics lab.
4.What
did
you
like
and
dislike
about
this
week;s
lab
Lab: The Maxwell-Boltzmann Distribution* Phys 242
*Some components of this lab are based on the activity developed by Julia Chamberlain & Ingrid Ulbrich
(PhET, UC Boulder; https://phet.colorado.edu/en/contributions/view/3687)
In this lab we will study several macroscopic quantities that can be used to describe a gas and explore the
relationships among these quantities. using a simulation from the PhET team:
https://phet.colorado.edu/sims/html/gas-properties/latest/gas-properties_en.html
This is a variant of the simulation you used for the Gas Properties lab. The simulation can be run in a
browser. If you have issues with the simulation, try using another browser. If you are unable to run the
simulation, your TA will provide you with remote assistance. When you run the simulation, choose the
“Energy” option. At the very bottom of the screen you will see the other options for the simulation,
including a home button, “Ideal,” “Explore,” “Energy,” and “Diffusion.” If you accidentally navigate to
another area, you can return to the Energy option by clicking the button.
The simulation shows a preset volume. In its initial configuration the box is empty. On the right side of
the screen there is a menu labelled “Particles.” By expanding this menu, you can choose to add so many
heavy or light particles. These particles will enter the volume at a temperature of 300 K in the initial
setup.
Once there are particles in the box, the temperature and pressure in the box can be read off the scales on
the right corner of the box. The units can be changed for these values. To adjust the temperature of the
particles in the box, move and hold the slider bar below the box.
To the left of the box is a graph showing the speed of the particles. This is a histogram. By clicking the
blue and red boxes below the graph, you can see the distributions of the heavy and light particles,
respectively. The box above this shows the average speed of the heavy and light particles.
Below the speed distribution graph is a menu that can be expanded to show the kinetic energy distribution
of the particles. Again, by clicking the blue and red boxes below the graph, you can see the distributions
of the heavy and light particles, respectively.
On the left there is a handle to change the size of the box. There is also a lever at the top of the box that
can be lifted to open the box, allowing particles to escape. Particles ...
1 SPU 25 Energy and Climate Vision for the Future, Spri.docxhoney725342
1
SPU 25 Energy and Climate: Vision for the Future, Spring 2018
Homework Set #1 Climate Basics, DUE Monday 2/12 (1:00 pm in lecture)
Name: _____________________________________ Section: __________ TF: _____________________ Score: ______/_______
Collaborators: _________________________________________________________________________________________________
Earth’s climate is a complex reflection of the distribution and movement of energy around the planet. The
primary source of Earth’s energy is radiation from the Sun. In this problem set, you will see how this energy is
received, lost, and stored, and the role of greenhouse gases in altering the climate. You will also understand
how the distribution of energy influences climate and get some practice with basic quantitative problems and
unit conversions. (40 points total)
You will only receive credit if you show all your work and write legibly.
I. Earth’s Energy Balance
Planet Earth (including the solid earth, oceans, and atmosphere) is best described as an isolated system:
energy, but not mass, can pass from Earth to space and vice versa. In this type of system, the energy balance
may be described by: Energy gained = Energy lost – change in storage.
1. Greenhouse gases in the atmosphere prevent the radiation of energy to space, so they impact which
term in the above equation? (1 point)
2. Changing surface and ocean temperatures reflect which term in the above equation? (1 point)
II. Energy from the Sun
3. True or False: Summer is warmer than winter because the Earth is closer to the Sun. (1 point)
4. Currently, the energy from the Sun arriving at Earth’s orbital position amounts to 1,379 W m-2,
measured perpendicular to the direction of the sunlight (see figure below).
a. Given that the Earth is a circular target for this energy and has a radius of 6.38 x 103 km,
calculate the total rate at which solar energy is intercepted by the Earth. Report your answer in
Watts. Recall that the area of a circle is πr2. (2 points)
Figure 1. The shadow formed by an
illuminated sphere has a circular
shape with a radius R equal to the
radius of the sphere.
2
b. Assuming that the energy from the Sun is eventually distributed equally over the entire surface
area of the Earth, use your answer from part (a) to calculate the current average rate of
incoming solar radiation. Express your answer in Watts per meter squared. Recall that the
surface area of a sphere is 4πr2. (3 points)
III. The fate of energy from the Sun
5. Based on your answers from the previous problem and assuming a global average albedo of 0.3, how
much of the incoming solar radiation is reflected back into space? How much is absorbed? Express
your answers in Watts per meter squared. (2 points)
6. Much of the energy absorbed at the Earth’s surface is used for evaporation. The energy involved in
changing the phase of water is c ...
This presentation is based on the curriculum for K12 created by the Department of education. It includes simulation to better understand the concepts presented.
Maxwell Boltzmann Summary Answer the following questions anAbramMartino96
Maxwell Boltzmann: Summary
Answer the following questions and submit your responses as a PDF.
1. Write down one major conclusion you can draw from this week’s laboratory.
Please explain.
2. Describe the experimental evidence that supports your conclusion. Please
explain.
3. Give one example of applications/situations for the finding(s) you described
above in your everyday life outside of physics lab.
4.What
did
you
like
and
dislike
about
this
week;s
lab
Lab: The Maxwell-Boltzmann Distribution* Phys 242
*Some components of this lab are based on the activity developed by Julia Chamberlain & Ingrid Ulbrich
(PhET, UC Boulder; https://phet.colorado.edu/en/contributions/view/3687)
In this lab we will study several macroscopic quantities that can be used to describe a gas and explore the
relationships among these quantities. using a simulation from the PhET team:
https://phet.colorado.edu/sims/html/gas-properties/latest/gas-properties_en.html
This is a variant of the simulation you used for the Gas Properties lab. The simulation can be run in a
browser. If you have issues with the simulation, try using another browser. If you are unable to run the
simulation, your TA will provide you with remote assistance. When you run the simulation, choose the
“Energy” option. At the very bottom of the screen you will see the other options for the simulation,
including a home button, “Ideal,” “Explore,” “Energy,” and “Diffusion.” If you accidentally navigate to
another area, you can return to the Energy option by clicking the button.
The simulation shows a preset volume. In its initial configuration the box is empty. On the right side of
the screen there is a menu labelled “Particles.” By expanding this menu, you can choose to add so many
heavy or light particles. These particles will enter the volume at a temperature of 300 K in the initial
setup.
Once there are particles in the box, the temperature and pressure in the box can be read off the scales on
the right corner of the box. The units can be changed for these values. To adjust the temperature of the
particles in the box, move and hold the slider bar below the box.
To the left of the box is a graph showing the speed of the particles. This is a histogram. By clicking the
blue and red boxes below the graph, you can see the distributions of the heavy and light particles,
respectively. The box above this shows the average speed of the heavy and light particles.
Below the speed distribution graph is a menu that can be expanded to show the kinetic energy distribution
of the particles. Again, by clicking the blue and red boxes below the graph, you can see the distributions
of the heavy and light particles, respectively.
On the left there is a handle to change the size of the box. There is also a lever at the top of the box that
can be lifted to open the box, allowing particles to escape. Particles ...
Read| The latest issue of The Challenger is here! We are thrilled to announce that our school paper has qualified for the NATIONAL SCHOOLS PRESS CONFERENCE (NSPC) 2024. Thank you for your unwavering support and trust. Dive into the stories that made us stand out!
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Power-sharing Class 10 is a vital aspect of democratic governance. It refers to the distribution of power among different organs of government, levels of government, and social groups. This ensures that no single entity can control all aspects of governance, promoting stability and unity in a diverse society.
For more information, visit-www.vavaclasses.com
Synthetic Fiber Construction in lab .pptxPavel ( NSTU)
Synthetic fiber production is a fascinating and complex field that blends chemistry, engineering, and environmental science. By understanding these aspects, students can gain a comprehensive view of synthetic fiber production, its impact on society and the environment, and the potential for future innovations. Synthetic fibers play a crucial role in modern society, impacting various aspects of daily life, industry, and the environment. ynthetic fibers are integral to modern life, offering a range of benefits from cost-effectiveness and versatility to innovative applications and performance characteristics. While they pose environmental challenges, ongoing research and development aim to create more sustainable and eco-friendly alternatives. Understanding the importance of synthetic fibers helps in appreciating their role in the economy, industry, and daily life, while also emphasizing the need for sustainable practices and innovation.
Embracing GenAI - A Strategic ImperativePeter Windle
Artificial Intelligence (AI) technologies such as Generative AI, Image Generators and Large Language Models have had a dramatic impact on teaching, learning and assessment over the past 18 months. The most immediate threat AI posed was to Academic Integrity with Higher Education Institutes (HEIs) focusing their efforts on combating the use of GenAI in assessment. Guidelines were developed for staff and students, policies put in place too. Innovative educators have forged paths in the use of Generative AI for teaching, learning and assessments leading to pockets of transformation springing up across HEIs, often with little or no top-down guidance, support or direction.
This Gasta posits a strategic approach to integrating AI into HEIs to prepare staff, students and the curriculum for an evolving world and workplace. We will highlight the advantages of working with these technologies beyond the realm of teaching, learning and assessment by considering prompt engineering skills, industry impact, curriculum changes, and the need for staff upskilling. In contrast, not engaging strategically with Generative AI poses risks, including falling behind peers, missed opportunities and failing to ensure our graduates remain employable. The rapid evolution of AI technologies necessitates a proactive and strategic approach if we are to remain relevant.
Unit 8 - Information and Communication Technology (Paper I).pdfThiyagu K
This slides describes the basic concepts of ICT, basics of Email, Emerging Technology and Digital Initiatives in Education. This presentations aligns with the UGC Paper I syllabus.
2. Standard
• Standards : MS-PS3-4 Plan an investigation to determine the
relationships among the energy transferred, the type of matter, the
mass, and the change in the average kinetic energy of the particles as
measured by the temperature of the sample.
3. Objectives:
- List the factors affecting wind formation and movement of
air.
- Explain how wind is formed.
- Model the effect of Earth’s rotation on matter in the
atmosphere.
6. Have you ever sat on the edge of a
mountain?
If you tried this dangerous
activity , then you should feel
the strong wind there
Have you ever asked yourself, from
where, how this wind is coming????
Can you suggest an answer??
7. Now, in groups, watch the following video and answer its questions
Teacher’s link:
https://edpuzzle.com/media/63ee35b04afa3640f048ccfc
8. 3- The air will be heated
4- The hot air will
expand(low pressure) and
become lighter so it will
rise
1- The cold air will
become heavy and
dense (high pressure),
so it will sink
2- The cold air will move
toward the hot region
5- The hot air will go to
the cold region area
9. In summary
There are two
reasons responsible
for producing wind
and movement of air
1-uneven heating and
cooling of the earth
(how??!)
2- Spinning of earth
the cold air around the
poles will move to the
equator where the sun
is so hot, while the hot
air will move to the
poles where it is so
cold
10. One of the reasons of why air is moving?
A –because of the sun
B – spinning of earth
C- I do not know
Checkpoints :
11. Which of the following is heavier and denser?
A –The cold air.
B – The hot air
C- They are the same
Checkpoints :
12. The cold air in the north pole will move to _________
A –The equator. B- The south pole.
C- will not move at all.
Independent
activity:
https://create.kahoot.it/details/bd13a70d-7cf3-4f92-bd56-
791a243ebae8
Checkpoints :
13. Model the effect of Earth’s rotation on matter in the
atmosphere using ballons, ink, and a dropper. (Pairwork)
1. Fill in two balloons (representing Earth) with air
and tie them.
2. With the first ballon (not rotating), place a drop of
ink and write down your observation on a piece of
paper.
3. With the second ballon (rotating), place a drop of
ink and write down your observation.
4. Write a conclusion about the effect of rotation
(spinning of the ballon) on the matter (ink).
17. Starter: Imagine you and your friend sitting like this,
and you want to throw this ball to him while
you are spinning
To which direction the ball will
move??
Think???
1- to your friend direction
2- Straight forward
3- It will deflect to one side
19. It is the effect of Earth’s rotation on
the pathway of the wind.
20. Coriolis effect
Wind deflection
because of earth
rotation
rotation direction
Deflection of air and
water because of earth
rotation
In both hemispheres,
the wind deflects
opposite to the earth
rotation direction
21. Groupwork: Relate air circulation to the Earth
system. (How can air circulation be beneficial
for the Earth system?)
Note: You may use your devices to search on the internet.
• Sample answer:
1. Cycling of matter in the atmosphere (for example: Water cycle,
carbon, nitrogen, phosphorus cycles, as well as organic matter by
carrying bacteria and microorganisms).
2. Moving clouds for hundreds of kilometers.
3. Pollination and seed dispersal of plants.
4. Flow of energy (by conduction, convection, and radiation).
22. Now is your turn to show your
intelligence
Teacher’s link:
https://quizizz.com/admin/quiz/6623ede4
a0460956cb077ff0?source=quiz_share
It’s Quizizz time
24. Standard: MS-PS3-4 Plan an investigation to
determine the relationships among the energy
transferred, the type of matter, the mass, and
the change in the average kinetic energy of the
particles as measured by the temperature of
the sample.
Essential Question: How can energy be
transferred from one material to another?
25. Objectives
List 3 ways to transfer energy
(Conduction, convection, and radiation)
-Explain how energy transfers between
hot and cold objects.
-Compare and contrast 3 ways of
transferring energy.
-Investigate the 3 ways of heat energy
transfer
27. Lab Instructions:
Students will move to the science laboratory and have their manual to use.
All instructions and procedures are found in their lab manual.
Students will work in groups and each group has one leader.
Students are not allowed to touch anything without permission (hot, harm,
dangerous objects)
All observation and questions should be answered, and all groups must
submit their lab report at the end of the class.