<p>The jet streams in our rotating (spheroid) planet meander because they cannot maintain a straight zonal course. The atmospheric flow is effectively perturbed upon collision to large mountain ranges like the Rockies and the Himalayas; an effect that is also felt at the jet stream level (i.e., around 10km above ground; upper-troposphere). The inhomogeneous temperature field due to land-sea contrasts and the latitude-dependent insolation results in an inhomogeneous pressure field that gives rise to winds of any direction and eddies. Convection, clouds and precipitation can also affect the upper-tropospheric flow.</p>
<p>All these reasons can provide a &quot;kick&quot; in an initially zonal jet. This &quot;kick&quot; means that air masses will move toward different latitudes to the north and south maintaining the vorticity of their original position (since vorticity is conserved under certain assumptions). Cyclonic/anticyclonic rotational movement thus emerges and the jet develops the so-called Rossby waves. These waves are highly-dynamic flow features with a shape and propagation that evolve constantly and give rise to the meandering of the jet that hosts them. Since some regions in the midlatitudes are baroclinically highly unstable (i.e., the meridional temperature gradient is large and small eddies can quickly grow bigger), these meanders are often rather pronounced and the meridional component of the wind dominates the zonal one.</p>

CC BY-SA 4.0
2022-09-10T23:49:09.130Z
2022-09-10T23:49:09.130Z
geodis
<p>I wanted to explain to high school students why the jet stream meanders, I am aware of the equations describing relative vorticity and planetary vorticity, the concept of conservation of vorticity i.e. F+ζ = constant.</p>
<p>But I want to explain it without these equations in simple terms. Can anyone give a generic explanation in layman's terms.  It's ok if it's not 100% accurate but just gives a basic understanding of the concept.</p>

CC BY-SA 4.0
2022-09-11T01:21:18.563Z
Because there are continents, so the flows are perturbed.  If you look at planets with a liquid surface (e.g. Saturn) you can see the zonal patterns stay relatively isolated and unperturbed.
f.thorpe
CC BY-SA 4.0
2022-09-22T10:25:39.740Z
Think of it like a river. A river has banks that stops it from meandering. But the jet stream has only soft banks and so will be pushed upon by the jet stream itself and this will cause the 'banks' to move and hence the jet stream will meander.
Mozibur Ullah
CC BY-SA 4.0
2022-09-22T11:54:20.417Z
You don't need continents or any perturbation. Any strong flow is going to be unstable because of turbulence and it is going to start meandering. https://en.wikipedia.org/wiki/Turbulence
arkaia
<meteorology>
Why does the jet stream meander?
jai ho
# Why does the jet stream meander?

(Asked by: username_0 on 2022-06-08)

I wanted to explain to high school students why the jet stream meanders, I am aware of the equations describing relative vorticity and planetary vorticity, the concept of conservation of vorticity i.e. F+ζ = constant.

But I want to explain it without these equations in simple terms. Can anyone give a generic explanation in layman's terms. It's ok if it's not 100% accurate but just gives a basic understanding of the concept.

**Tags:** meteorology

> **Comments:**
> **username_1**: Because there are continents, so the flows are perturbed.  If you look at planets with a liquid surface (e.g. Saturn) you can see the zonal patterns stay relatively isolated and unperturbed.  
> **username_2**: Think of it like a river. A river has banks that stops it from meandering. But the jet stream has only soft banks and so will be pushed upon by the jet stream itself and this will cause the 'banks' to move and hence the jet stream will meander.  
> **username_3**: You don't need continents or any perturbation. Any strong flow is going to be unstable because of turbulence and it is going to start meandering. https://en.wikipedia.org/wiki/Turbulence  

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## 1 answers

### Answer by username_4 on 2022-09-10. Score: 1

The jet streams in our rotating (spheroid) planet meander because they cannot maintain a straight zonal course. The atmospheric flow is effectively perturbed upon collision to large mountain ranges like the Rockies and the Himalayas; an effect that is also felt at the jet stream level (i.e., around 10km above ground; upper-troposphere). The inhomogeneous temperature field due to land-sea contrasts and the latitude-dependent insolation results in an inhomogeneous pressure field that gives rise to winds of any direction and eddies. Convection, clouds and precipitation can also affect the upper-tropospheric flow.

All these reasons can provide a "kick" in an initially zonal jet. This "kick" means that air masses will move toward different latitudes to the north and south maintaining the vorticity of their original position (since vorticity is conserved under certain assumptions). Cyclonic/anticyclonic rotational movement thus emerges and the jet develops the so-called Rossby waves. These waves are highly-dynamic flow features with a shape and propagation that evolve constantly and give rise to the meandering of the jet that hosts them. Since some regions in the midlatitudes are baroclinically highly unstable (i.e., the meridional temperature gradient is large and small eddies can quickly grow bigger), these meanders are often rather pronounced and the meridional component of the wind dominates the zonal one.


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