Where Does Wind Come From? Crash Course Geography #8 - Free Educational videos for Students in K-12 | Lumos Learning

Where Does Wind Come From? Crash Course Geography #8 - Free Educational videos for Students in k-12


Where Does Wind Come From? Crash Course Geography #8 - By Math and Science



Transcript
00:0-1 there's an invisible force shaping our lives affecting the weather
00:02 , climate , land economy and whether a flag looks
00:05 majestic or just kind of sits there . I'm talking
00:08 of course about the wind . Large parts of the
00:10 globe are brought warmth and water thanks to wind In
00:13 europe , wind energy is one of the most popular
00:15 renewable energies , thanks to wind turbines that harness its
00:17 power . Ships with sails have followed the path of
00:19 the wind for centuries , bringing trade and entire empires
00:22 along with them . Fierce winds can also bring destruction
00:25 , stripping soil away from the ground or even ripping
00:27 apart buildings trying to protect ourselves from the wind might
00:29 feel like we're battling an imaginary foe , but wind
00:32 is definitely not imaginary . Geographers have defined it and
00:35 have tools to measure it , whether it's a gentle
00:37 sea breeze or gale force gusts . Wind is any
00:40 horizontal movement of air and there is a mixture of
00:43 nitrogen , oxygen and other gases that blend together so
00:46 well . They tend to act as one winds are
00:47 named based on what direction they come from . And
00:50 some people are even named after winds . My name
00:52 Elise means the north easterly trade winds in french or
00:55 live analyses the alleys winds with a french sailor .
00:58 For a father who used to love sailing the warm
01:00 north easterly trade winds . It's no surprise where this
01:03 came from . So let's get deeper into the science
01:05 of where wind comes from . It will be a
01:07 whirlwind of an adventure . I'm al is a career
01:09 and this is crash course geography . Mhm . Yeah
01:19 . If we zoom out and look at the globe
01:20 as a whole , we can see that there are
01:22 global wind patterns , just like there are global air
01:24 temperature patterns and these are intimately linked . We know
01:26 that insulation from the sun doesn't get distributed evenly and
01:29 ends up heating places differently . The temperature of a
01:32 place is tied to several key factors like latitude elevation
01:35 , how far it is from the ocean or sea
01:37 and even what type of surface it is and how
01:39 much of the sun's energy it absorbs . No matter
01:41 where we are though , air that's warm is lighter
01:43 , less dense and tends to rise . Cool air
01:46 on the other hand , is heavier , more dense
01:48 and tends to sink . And you did hear me
01:49 correctly , there's lighter air and heavier air because air
01:52 molecules all have weight , not a lot , but
01:55 still weight . The weight of air then leads to
01:57 atmospheric pressure , which comes from all the air above
02:00 that's pressing down on whatever air there is below .
02:02 So the pressure is much higher where I'm standing in
02:04 Miami than if we were filming this close to outer
02:06 space Down here , there's all 480 km of atmosphere
02:10 squishing down on us . In fact , it's likely
02:12 close to standard sea level pressure , which is exactly
02:15 what it sounds like the average atmospheric pressure at sea
02:17 level . We don't crumple like aluminum cans under this
02:20 enormous pressure because the air and water inside us exert
02:23 an equal amount of pressure outwards , and the exact
02:25 atmospheric pressure in other places will be different depending on
02:27 where we are the season or even the time of
02:29 day . Wind is actually the atmosphere's way of smoothing
02:32 out pressure differences , which can be created by the
02:35 daily and seasonal air temperature patterns across Earth's surface .
02:37 Meteorologists who studied the atmosphere use air pressure measurements to
02:41 forecast the weather . Like a weather report on tv
02:44 might show a map full of H . S .
02:45 And L's . Which is actually a map tracking air
02:47 pressure . A giant L . Stands for low pressure
02:50 or a low on a global scale . A low
02:52 area is where the pressure near the surface is less
02:54 than standard sea level pressure . But on a local
02:56 scale , like on your local weather report , a
02:58 low can also be an area where the pressure is
03:00 less than in the surrounding area because there's actually slightly
03:03 less air pressing down on that part of the earth
03:05 . Lows go buy lots of names . Like you
03:07 might hear it called a depression or even a cyclone
03:09 though it's not the giant spinning vortex of air we
03:11 might think of that's a specific weather event that only
03:14 forms and tropical oceans . But we'll come back to
03:16 that in upcoming episodes to keep it simple . We'll
03:18 just call it a low . Lows exist either because
03:21 air is being heated and expands up and out or
03:23 air higher up in the atmosphere is spreading out so
03:26 there's less air pressing down on Earth's surface down on
03:28 the ground . We might even be able to tell
03:30 we're in a low as their expands and rises ,
03:32 winds are drawn toward the center , the rising air
03:34 cools and moisture in the air condenses into droplets .
03:37 So if we happen to be in the center of
03:38 a low , the weather would often be pretty cloudy
03:40 and rainy . The giant H is on the map
03:42 mark . High pressure areas which we call a high
03:44 or anti cyclone in a high pressure cell , either
03:47 the air is cooling and becoming denser so it sinks
03:49 , or the atmosphere high above is piling up ,
03:51 pushing the air below it downward , sinking , compresses
03:54 air molecules together and makes them warm so any water
03:57 vapor in the air won't cool to condense into liquid
03:59 water . That means high pressure systems bring weather that's
04:02 clear and sunny , which I remember as a church
04:04 stands for happy high and low pressure cells are usually
04:06 large like they can be 1000 km across and air
04:10 moving between these vast areas to balance out energy in
04:12 the atmosphere helps us understand and identify the winds .
04:15 The key is the difference or change in pressure between
04:17 highs and lows which is called a pressure gradient .
04:20 Like any fluid air wants to flow from high to
04:22 low pressure . Let's start on a small scale and
04:25 look at an island . When the beaches and land
04:26 warm up faster during the day than the surrounding sea
04:29 , the air over the island expands , rises and
04:31 lowers the pressure at the surface . That leaves room
04:33 for air from the sea to rush onto the land
04:35 and wanna any windsurfer a son tanner will get a
04:38 cool sea breeze in the afternoon and similar things happen
04:40 at a bigger scale . Across the globe . Air
04:42 . The equator is consistently warmed by the sun and
04:45 tends to expand and rise . So we get a
04:46 belt of low pressure around the Earth called the equatorial
04:49 trough . And we'd expect the polls to experience high
04:51 pressure because the air there is cold and sinking ,
04:54 but winds don't just blow north and south . This
04:56 is because the earth rotates to see what really happens
04:59 to these winds . Let's imagine we're flying an airplane
05:01 from the north pole to the south pole with a
05:03 layover in Ecuador on the equator . Let's go to
05:05 the thought bubble . Hello , this is Captain Career
05:08 speaking . If you look out the windows , you'll
05:10 see the surface of the earth slowly rotating eastwards .
05:12 So in order to stay on a straight path ,
05:14 we'd have to constantly make little turns . This phenomenon
05:17 that causes moving objects like our plane or air or
05:20 water to seem like they curve as they travel over
05:23 the rotating Earth is known as the Coriolis effect .
05:25 The Earth is rotating beneath our plane , but also
05:28 as we travel towards the equator . The Earth actually
05:30 rotates faster because the Earth is bigger at the equator
05:33 and it has to move faster to keep up .
05:35 It's like a marching band turning a corner . If
05:37 they want to stay together in a straight line ,
05:39 The marches on the inside of the circle take much
05:41 smaller steps and moves slower than the marchers on the
05:43 outside . So if we're at the polls , we
05:45 just kind of spin in place . But as latitude
05:48 decreases , our rotational speed increases until we get to
05:50 the equator and the Earth's surface practically zooms by its
05:54 1600 km/h , which is about twice as fast as
05:57 our plane . Then , as our plane gets closer
05:59 and closer to Ecuador and the equator are rotational momentum
06:03 comes from the slow speeds at the north pole ,
06:04 not the rapidly rotating equator , which means we end
06:07 up getting deflected to the right into the pacific ocean
06:10 and have to make little left turns to get to
06:12 Ecuador . Something similar happens on our second flight towards
06:15 the south Pole , but this time we started out
06:17 rotating faster than our final destination . So as we
06:20 make our final approach to the South sandwich Islands ,
06:22 we'd get deflected left and end up east of where
06:25 we want to be . If we didn't correct ,
06:26 Please make sure your seatbelts are fastened and your tray
06:29 tables are stowed as we prepare for landing . Thanks
06:31 , that bubble in general , the Coriolis effect deflect
06:34 objects to the right in the Northern Hemisphere and to
06:36 the left in the southern hemisphere , which is how
06:38 we get those winds spirals around the low and high
06:40 pressure areas on our weather map , and why they're
06:42 also called Cyclones and anti cyclones . The air wants
06:45 to rush directly from the center of the high to
06:47 the center of the low but gets deflected . So
06:49 in our model , the heated air at the equator
06:51 first rises upward towards the trope a pause which is
06:53 the boundary between the troposphere and stratosphere as it tries
06:56 to move poll word high up in the atmosphere .
06:58 Then , as it moves away from the equator ,
07:00 the coriolis effect causes air traveling northwards to turn right
07:03 , speeding faster east . The further north it gets
07:05 , the air is also cooling and by the time
07:07 it sinks back to the surface , it's only reached
07:09 around 30 degrees latitude . So instead of one big
07:11 circulation cycle , as proposed by George Hadley , an
07:14 english lawyer and amateur meteorologist who first described it in
07:17 17 35 we get a more complicated circulation system containing
07:20 the Hadley Cell . Had we wanted to understand why
07:23 surface winds that should have blown straight south towards the
07:25 equator , along the pressure gradient from high pressure to
07:27 low pressure , took a turn west , solving that
07:30 mystery would help ensure european trading ships would safely reach
07:33 the shores and goods of the Americas . This isn't
07:36 the first time our understanding of the winds has gone
07:38 hand in hand with exploration and trade , wealth and
07:40 power were driven by the winds . For instance ,
07:42 new technologies created in the 14 hundreds , like the
07:44 quadrant and the astrolabe enabled accurate navigation and mapping of
07:48 ocean currents , winds and trade routes . Over the
07:50 years , many more scientific minds have explored the implications
07:53 of Hadley's theory , and we're still learning more as
07:55 we explore the movement of energy between the atmosphere and
07:57 the biosphere . We now know that in reality ,
07:59 air in both hemispheres converges in the narrow band around
08:02 the equator called the intertropical convergence zone and rises the
08:05 surface winds , or doldrums that form here as air
08:08 converges and rises upwards are light and not super reliable
08:11 sailing ships could get stuck in the doldrums for days
08:14 . Similarly weak winds are found on the pole word
08:16 edges of the Hadley cells where air is being forced
08:18 down , creating high pressure zone centered at about 30
08:20 degrees latitude . Called the subtropical high pressure belts .
08:23 Sailors of Your were often forced to eat their horses
08:26 or throw them overboard in these horse latitudes to conserve
08:29 drinking water and lighten the weight . While the sailing
08:31 ships waited for the week winds at the center of
08:33 these highs to pick up , wow , that's pretty
08:36 dark in between these high and low pressure belts ,
08:39 there are strong and reliable winds spiraling outward from the
08:41 subtropical high pressure belt towards the equator . These are
08:45 the easterly trade winds and they're my favorite winds .
08:48 Obviously many ships have depended on the trade winds like
08:51 early spanish sailing ships as they sought God glory and
08:53 gold . In what we now call central and south
08:55 America , of course , making the return trip was
08:57 another matter . The ancient Mariners of the spanish galleons
09:00 , going home from the Americas plotted a course using
09:02 the winds blowing poll Word from the subtropical high pressure
09:05 belt , these westerly are strongly deflected to the right
09:08 and blow from the southwest . These strong winds blow
09:10 towards another low pressure belt called the sub polar lows
09:13 , where they clashed with the polar easterly blowing from
09:15 the frigid , very high pressure polls in the southern
09:18 hemisphere . They blow with greater strength as there's very
09:21 little land in these latitudes to interrupt their flow .
09:23 So all together on our idealized Earth , we've seen
09:26 that there are actually seven pressure belts to polar highs
09:29 , to sub polar lows to subtropical highs and one
09:32 equatorial low . And winds flow between these belts of
09:34 high and low pressure on the real earth . The
09:37 belts are not so organized , they form cells of
09:40 pressure and we see more complex patterns of pressure and
09:42 wind as the cells shift with the seasons and vary
09:44 between land and water . So our idealized Earth is
09:47 kind of like a wind and pressure map . It's
09:49 a simplified model that helps us understand what's happening on
09:52 the real earth , just like the atmosphere works like
09:54 a cell membrane . The winds are like earth circulatory
09:56 system , so many things vital to our planet flow
09:59 through the winds during the voyages of discovery in the
10:02 15th to 18th centuries , which we now recognize weren't
10:04 really discoveries at all the knowledge of winds , ocean
10:07 currents , natural harbors and more was an essential foundation
10:10 for circumnavigating the globe and we continue to rely on
10:13 the winds to power our economies as a renewable energy
10:16 source . This silent force will continue to shape our
10:18 lives in the future . I hope , wherever you
10:20 are , is in the center of a sunny high
10:22 pressure area , which will be perfect weather to go
10:24 with the flow in the ocean , which is what
10:26 we'll talk about next week . Many maps and borders
10:28 represent modern geopolitical divisions that have often been decided without
10:31 the consultation , permission or recognition of the land's original
10:34 inhabitants . Many geographical place names also don't reflect the
10:38 indigenous or aboriginal peoples languages . So we have crash
10:41 course , want to acknowledge these people's traditional and ongoing
10:43 relationship with that land and all the physical and human
10:46 geographical elements of it . We encourage you to learn
10:48 about the history of the place you call home through
10:50 resources like native land dot C . A . And
10:52 by engaging with your local indigenous and aboriginal nations through
10:55 the websites and resources . They provide thanks for watching
10:58 this episode of Crash Course Geography . If you want
11:00 to help keep all crash Course free for everyone forever
11:03 , you can join our community on Patreon .
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