Explore
For Enterprise
Join for Free
Log In

artes y humanidades
Negocios
Ciencias de la Computación
Ciencia de Datos
Tecnología de información
salud
Matemáticas y Lógica
Desarrollo Personal
Ciencias Físicas e Ingeniería
Ciencias sociales
Aprendizaje de un idioma
Grados
Certificados

Explorar todo lo que Coursera tiene para ofrecer

Explorar
Buscar
For Enterprise
Inicia Sesión
Únete de forma gratuita

Video 3.3.2: What Controls the Temperature Profile of the Atmosphere?

Loading...

Our Earth: Its Climate, History, and Processes

Universidad de Mánchester

4.6 (95 calificaciones) | 6.4K estudiantes inscritos

Develop a greater appreciation for how the air, water, land, and life formed and have interacted over the last 4.5 billion years.

Revisiones

4.6 (95 calificaciones)

5 stars
67 ratings
4 stars
19 ratings
3 stars
9 ratings

SS

Jun 02, 2019

So informative and well-prepared learning materials for students. Thank you very much for your course.

PG

Oct 27, 2017

Excellent broad content. Ideal for the learner or someone wanting to get to grips with the basics.

De la lección

Water in Earth’s Climate System: Oceans, Atmosphere, and Cryosphere

Video 3.1.1: Where Did the Oceans Come From?6:55

Video 3.1.2: Are the Oceans in Steady State?13:36

Video 3.2.1: How the oceans work - Dr. Gregory Lane-Serff9:36

Video 3.2.2: The oceanic conveyor belt - Dr. Gregory Lane-Serff12:57

Video 3.3.1: What is the Atmosphere Made Of?6:41

Video 3.3.2: What Controls the Temperature Profile of the Atmosphere?5:49

Video 3.3.3: Three Radiation Laws4:48

Video 3.3.4: What if the Earth had no Atmosphere?7:37

Video 3.4.1: How does the Atmosphere Work?9:04

Video 3.4.2: How do the Jet Streams Control the Weather?7:05

Video 3.5: Extratropical cyclones8:11

Video 3.6: The Rise and Fall of Ice on Earth12:44

Video 3.7: How do Glaciers Control the Height of Mountains? – Dr. Simon Brocklehurst10:46

Video 3.8: Why the Arctic is Crucial to Earth's Climate - Dr. Bart Van Dongen and Dr. Robert Sparks 7:48

Impartido por:

Prof. David M. Schultz
Professor of Synoptic Meteorology
Dr Rochelle Taylor
Postdoctoral Research Associate
Dr Jonathan Fairman
Postdoctoral Research Associate

Transcripción

So we talked about this E shaped temperature profile.

And what I want to do now is look at why this temperature profile exists.

It's actually relatively simple to explain.

And the approach that I want to take to explain it, is simply to say

there are three areas in this temperature profile that are warm.

And why is that region of high temperature present in each one of these locations.

And so what I've done here is broken down what the cause of that heating is.

Let's start at the bottom in the troposphere.

Within the troposphere,

we see relatively warm air near the ground and the temperature

decreasing with height until we get to the top of the troposphere.

This heating comes from the greenhouse effect.

Solar radiation comes down, is absorbed by the ground.

The ground having a high temperature

then emits infrared radiation into the lower part of the atmosphere.

Which the atmosphere then absorbs.

So.

In the bottom, we have the greenhouse effect.

Heating from the ground, and we'll talk more about this in a later lecture.

Why is it warm here at the stratopause,

the boundary between the stratosphere and the mesosphere?

It's warm here because of the presence of ozone.

We have ultraviolet radiation that's coming down, coming from the sun.

It encounters this ozone, and it breaks apart the ozone into molecular

oxygen plus atomic oxygen, so O2 + O.

This process of breaking the bonds that construct the ozone

leads to the release of heat.

And although the ozone is concentrated mostly in the stratosphere,

this ultraviolet radiation encounters it in the upper part of the stratosphere and

lower mesosphere.

So that's why it's warm in this region here around 50 kilometers.

Why is it warm in the thermosphere?

Well much more, a few more reactions going on here.

When we get up high in the atmosphere,

we start to encounter more intense radiation coming from the sun.

We have x-rays and extreme short wave ultra-violet radiation, radiation

that would be damaging to cells had it made it all the way down to the ground.

Both the oxygen and the nitrogen absorb this radiation and

it causes them to break apart into their atomic components, oxygen and nitrogen.

Then this radiation interacts with the oxygen and nitrogen and

in it's atomic state and kicks out electrons from

these atoms leaving ions.

And, you may also hear this area being referred to as the ionosphere,

this is where the aurora occur.

These regions are releasing heat because of the ionization of these atoms,

and the result is a relatively warm thermosphere.

So, the way I like to think about the thermo structure of the atmosphere

is one that would be relatively uniform with height,

except there are three areas of warmth.

One, in the troposphere, due to the greenhouse effect.

One near the stratopause, due to the heating

of ozone and the breakup of ozone by ultraviolet light.

And then one in the thermosphere that is the result of the ionization

of the gases in the atmosphere.

So, what I want to do now is summarize this lecture in a way that illustrates

why this temperature profile is important and why I'm making a big deal out of it.

Here, we have this inverted W, this tilted W shape.

To the earth's temperature profile.

And we know this area here in the middle, in the stratopause, why it's warm.

It's due to the breakup of ozone, O3.

Well obviously, if there wasn't any oxygen in the earth's atmosphere,

then there wouldn't be any ozone, either and this warming

in the upper part of the stratosphere and lower mesosphere would not be occurring.

And indeed, if we look at other planets that don't have a lot of molecular oxygen

in them, such as Mars and

Venus, then we see temperature profiles that look more like this.

They are warming near the surface.

Because of whatever greenhouse effect they have.

Venus has a very strong one.

Mars has a very weak one.

But they both have warming near the ground.

Both planets have warming in the upper part of the atmosphere due to

the ionization of the gasses in the atmosphere.

But neither of these planets have a strong stratopause.

And we know that because there's no oxygen in these atmospheres.

Explora nuestro catálogo

Inscríbete de manera gratuita y obtén recomendaciones personalizadas, actualizaciones y ofertas.

Coursera brinda acceso universal a la mejor educación del mundo, al asociarse con las mejores universidades y organizaciones, para ofrecer cursos en línea.

© 2019 Coursera Inc. Todos los derechos reservados.

Descargar en la App Store

Consíguelo en Google Play

Coursera
Acerca de
Liderazgo
Empleo
Catálogo
Certificados
Certificados MasterTrack™
Grados
For Enterprise
For Government

Comunidad
Learners
Partners
Developers
Beta Testers
Translators

Conectar
Blog
Facebook
LinkedIn
Twitter
Instagram
Youtube
Blog de Tecnología

Más
Términos
Privacidad
Ayuda
Accesibilidad
Prensa
Contacto
Directorio
Afiliados