# From the motion on carousels to cyclones and the Gulf Stream

A guided tour full of surprises

## An interactive material for secondary school students

for assisted or individual learning

Questions and tasks are set in shaded boxes. Those marked by an ? are recommended for particularly motivated readers.

### I Introduction

Watch the video:

What do you think of an effect like this, is it realistic?

To gain a better insight, let us start with a more straightforward video.

You might want to carry out analogous table-top experiments with balls on rotating platforms (e.g. an LP player or potter’s wheel). Using a web camera rotating with the platform, you can observe motions like this.

Can you decide by comparing the last two videos, whether the platform is turning in a clockwise or in a counter-clockwis direction in the second case?

Why do you think the balls follow such a curved path rather than a straight course after tossing? You might have had similar experiences e.g., in science centers.

### The basic effect: deflection of moving bodies

If interested, carry out a simple home-experiment with a pencil, a sheet of paper and a ruler. Fix the center of the paper disk to a board with a pin. First draw a straight line with constant speed on the non-moving sheet across this center point. Repeat the same motion with someone rotating the sheet clockwise with an approximately constant angular velocity while you are drawing the line. You might obtain a curved path, deflecting from the straight line, similar to this.

It is clear that the motion in the carousel (the path traced out on the rotated paper sheet) is deflected from its initial direction. Note that the deflection is to the left if the rotation is clockwise. The same kind of deflection is observed in the deflection of the ball in the second and third video.

Note: the straight line on the non-rotated paper sheet corresponds to a uniform motion as seen from stationary reference frame. The deflection is thus a consequence of the fact that an otherwise simple motion is observed from a rotating frame.

The curved path traced out on the rotated paper sheet resembles a parabola, at least for short distances. The
motion on the carousel is thus similar to motion with a **constant** acceleration.

In the curve drawn in your experiment, consider the part that belongs to short times (i.e. the part near the beginning). Measure the amount of deflection from the straight line at a few points. Using the motion along the straight line as a measure of time (in arbitrary units), show that the dependence is parabolic for short times at least, and determine the acceleration.

Using the fact that a point of distance $r$ from the center is rotated along an arc of length $r \Omega t$, where $\Omega$ is the angular velocity of the sheet, express the acceleration in terms of $\Omega$ and the pencil’s velocity $v$. What force can cause this acceleration?

The force used to describe the deviation is the Coriolis force. Its magnitude is $$ {F_C=m 2 v \Omega}, $$ and it points perpendicular to the direction of velocity $\boldsymbol{v}$, to the left and to the right in the case of clockwise and counter-clockwise rotation, respectively.

For a deeper insight, carry out a slightly more advanced experiment. Repeat the first experiment so that you start drawing the pencil line at a distance of $r_0$ away from the center of rotation and radially outwards. Do you obtain a different expression for the acceleration or the force acting perpendicular to velocity?

The force remains $F_C=m 2 v \Omega$ but $v$ turns out to be the velocity of the body relative to the rotating system. Another force also appears acting radially outwards, this is the centrifugal force $F_{cf}=m r_0 \Omega^2$. Both forces are important in the motion of a ball on the carousel, but only the Coriolis force is responsible for the deflection from the original velocity.

### A basic quantitative measure: the strength of deflection

Consider a body which would move in a non-rotating system with a velocity of $U$ and estimate the deflection $D$ from the direction of this initial velocity after traveling a distance $L$, provided the deflection is weak: $D \ll L$. The acceleration $2 v \Omega$ is then constant and can be approximated by $2 U \Omega$. With this approximation, the distance $D$ traveled perpendicular to the initial velocity is, after time $t$, $(1/2)a_C t^2$, i.e., $(1/2) 2 U \Omega t^2$. The time needed to travel a distance $L$ is approximately $L/U$, and we obtain $$D=U \Omega L^2 /U^2 = \Omega L^2 /U.$$ The relative deflection, the distance $D$ compared to the total distance $L$, i.e. $D/L$ is also worth considering: $$ \boxed{D/L = \Omega L/U.} $$ This is a useful simple expression which enables us to estimate the magnitude of deflection. Therefore the expression $D/L=\Omega L/U$ for the relative deflection is generally considered the quantitative measure of the strength of deflection. Note that is is inversely proportional to $U$ since the time during which the Coriolis force acts is also important for the deflection.

Check your knowledge acquired: Quiz I

### II The rotating Earth as a carousel

Our paper sheet experiment clearly illustrates that deflection is due to a rotation the axis of which is perpendicular to the plane in which the deflection takes place. If the plane of deflection is not perpendicular to the rotational axis, it is the angular velocity component perpendicular to this plane that determines the rate of deflection.

It must be surprising to learn that angular velocity may have components. In fact, it is useful to consider angular velocity as a vector. The angular velocity vector is parallel to the axis of rotation, and its direction is obtained as the direction of the thumb of one’s right hand if the fingers are curved in the direction of the rotation. Besides directionality, angular velocity is a vector also in the sense that it can be decomposed into perpendicular components. This implies that a rotation through a small angle, with an angular velocity vector ${\bf \Omega}$ is equivalent to carrying out rotation around one axis with angular velocity ${\bf \Omega_1}$ and, another rotation around a perpendicular axis with angular velocity ${\bf \Omega_2}$, where $\Omega^2=\Omega_1^2+\Omega_2^2$. This is illustrated by means of a simple animation. (Note that the animation is not to scale since the decomposition of angular displacement into two components about two perpendicular axes holds true for low angles only which would not be visible otherwise.)

When applied to the rotating Earth, the angular velocity ${\bf \Omega_E}$ of the planet directed along the axis from south to north can be decomposed into arbitrary perpendicular components ${\bf \Omega_1}$ and ${\bf \Omega_2}$, as shown here

When dealing with the deflection effect of the Coriolis force on the Earth - which is always observed in the local
*horizontal* plane - it is most natural to decompose ${\bf \Omega_E}$ into horizontal and vertical components with
magnitudes denoted by $\Omega_H$ and $\Omega_V$, respectively.

If you are interested to see that the resultant angular velocity is indeed the vectorial sum of the horizontal and vertical components in this particular decomposition, too, consult this page

At a location on latitude $\phi$, the angle between the horizontal plane and the rotational axis is also $\phi$,
therefore the angular velocity of Earth, $\Omega_E$, projected onto the local **vertical** component is
$$ {\Omega_V = \Omega_E \sin \phi} . $$

The deflection expression $D=\Omega L^2 /U$ can safely be applied to any motion on the Earth, you just have to replace $\Omega$ with $\Omega_V$. The relative deflection can then be given as $$ \boxed{D/L = \Omega_V L/U.} $$ Note that the Earth's angular velocity is 1 rotation / 1 day = $2 \pi/ 86400 \text{ s}$, i.e., $$ \Omega_E=7.3\ 10^{-5} \text{ 1/s}. $$ At mid latitudes, at $\phi \sim 45 \text{ degrees} (=\pi/4)$, $$ \Omega_V=5\ 10^{-5} \text{ 1/s}, $$ a value easy to remember. Note that on the Southern Hemisphere $\phi$ is negative, and thus $\Omega_V$ is negative, too.

Remark: A simplifying feature in motions on the Earth compared to those on a carousel is that the centrifugal force need not be taken into account explicitly since it is included in the acceleration of gravity ${\bf g}$ which is the vector sum resulting from the gravitational and the (small) centrifugal acceleration.

From the gun in the picture, estimate the deflection of a cannon ball over a distance of an L=100 km shot During World War I, given that the average horizontal velocity of the canon ball from the gun was about 500 m/s.

$$ \Omega_V = 5\ 10^{-5} \text{ 1/s},\ L=10^5 \text{ m},\ U=500 \text{ m/s},\quad \text{thus}\quad D=\Omega_V L^2/U = 1 \text{ km}. $$ Coriolis compensators letting the canon shoot a little left of the target on the Northern Hemisphere (by approximately 1/100 radians, about 0.6 degrees in this case) were used during World War I.

### Does water drain in different directions on the Northern and Southern Hemispheres?

If the Coriolis force was acting alone, it would be reasonable to think that water drains differently on the two hemispheres, since the sign of $\Omega_E$ is different as seen above. When draining starts, water parcels start to move towards the sink, but become deflected due to the Coriolis force. The figure corresponds to the Northern Hemisphere where a counter-clockwise spin is expected while water is going down in a plughole.

Before becoming fully convinced, estimate the deflection $D$ at mid latitudes using realistic values for a plughole: $L=10 \text{ cm},\ U=10 \text{ cm/s}$.

$$ \Omega_V = 5\ 10^{-5} \text{ 1/s},\ L=0.1 \text{ m},\ U=0.1 \text{ m/s},\quad \text{thus}\quad D=\Omega_V L^2 /U = 5\ 10^{-6} \text{ m}\ (D/L= 5\ 10^{-5} ).$$ This value equals 5 micrometers, which cannot be perceived by the naked eye! The fact that this number is so small is the reason why our laboratories can be considered inertial reference frames in which Newton’s law hold, since the Coriolis force is practically negligble.

To see how strong other effects can be in the draining process, estimate the acceleration of a small cube of edge $\Delta r=1 \text{ cm}$ of water caused by the difference in the hydrostatic pressure generated by a tiny height difference: $\Delta h=1\text{ mm}$ on the surfaces of the opposite vertical planes of the cube.

The pressure difference on the vertical planes of area $A=\Delta r^2$ is $$ F = \rho g \Delta h A, $$ where $\rho$ denotes the density of water. The mass of the water cube is $\rho \Delta r A$, its horizontal acceleration is thus $$ a=g \Delta h/\Delta r = 1 \text{ m/s}^2 $$ This is to be compared with the Coriolis acceleration which is, when $U=0.1 \text{ m/s}$, $$ a_C=2\ 5\ 10^{-5}\ 10^{-1} \text{ m/s}^2 = 10^{-5} \text{ m/s}^2 $$ A difference of 5 orders of magnitude!

The Coriolis deflection is so small, due to the small magnitude of Earth’s angular velocity, that this effect is typically suppressed in our bath tubs by other effects (residual fluid motion, waves on the surface, asymmetry of the container, etc.) and in practice, either direction of the plughole vertex may be observed on either hemisphere. In carefully planned experiments, however, where all the disturbances are ruled out, the expected direction of spin can indeed be observed. The first such experiment was carried out by A. Perrot in Paris in 1859. Later experiments with sinks.

Considering these, how can you explain the events seen in the very first video? Hint: What is the magnitude of $\Omega_V$ on the Equator (where the local horizontal plane is parallel to the rotational axis), which is responsible for the deflection.

Since the total angular velocity vector points to the North, it has no vertical component here: $\Omega_V=0$. Therefore, no deflection occurs at the Equator! The effect seen in the video must be due to a clever way of pouring the water into the vessel.

Estimate the tilt angle of an aircraft moving at a speed of 1080 km/h by which the Coriolis deflection can be compensated.

On the Northern Hemisphere the aircraft should tilt to the left under some
angle $\alpha$ (as if it intended to turn left) to compensate the Coriolis force pointing to the right of its
direction of flight.

The magnitude of the lift acting perpendicular to the aircraft is practically the weight $mg$ of the craft
under this weak tilt, too. Since the aircraft is tilted, the horizontal component of this force is
$mg \sin\alpha$. This should balance the deflecting force to the right:
$$ mg \sin\alpha = 2 m \Omega_V U. $$
From here $\sin\alpha \approx \alpha = 2 \Omega_V U/g$. When $U=300 \text{ m/s}$,
$\alpha=3\ 10^{-3} \text{ rad} = 0.17 \text{ degrees}$, hardly discernible.

**Historical experiments:** Foucault and
Eötvös

Other weak deflection effects which, occasionally, may have long-lasting consequences.

On the Northern Hemisphere, the right bank of rivers is eroding faster than the left one. This rule was formulated (in a somewhat restricted form) by the Estonian scientist K. E. Baer in 1860.

On geological time scales, the Coriolis force might cause a drift of hundreds of kilometers of river beds to the right of the overall direction of the river.

On the Northern Hemispheres, the wear on the right rail of railway tracks is stronger than that on the left rail.

In sports, like hammer or javelin throw deflection due to the Coriolis force can be on the order of a few cm.

**In summary**, on the human scale, from a few meters up to hundreds of meters, the Coriolis effect is weak:
in certain situations it cannot even be perceived, while in others one has to use special equipment to prove it in
experiments.

Evaluate the ratio $\Omega_V L/U$ at mid latitude for a typical horizontal speed of $U=10$ m/s on increasing length scales of the size of $L=10, 100, 1000$ and $10000$ km. Express the ratio as a percentage. What is your conclusion regarding the importance of the deflection on these scales?

$L$ | $\Omega_V L/U$ | ($\Omega_V=5 \cdot 10^{-5} \text{ 1/s},\quad U=10 \text{ m/s}$) |
---|---|---|

1 km | 0,5% | deflection effect is very weak |

10 km | 5% | deflection effect becomes noticable |

100 km | 50% | deflection effect is considerable |

1000 km | 500% | deflection effect dominates |

We see that Coriolis deflection becomes more relevant with **increasing** scales.

Check your knowledge acquired: Quiz II

### III Strong Coriolis deflections

A remarkable feature of the deflection effect is, however, that on geographical scales it can become **strong**.
When the deflection $D$ is not much smaller than the extension in space, $L$, of the phenomenon. the estimated $D$
cannot be considered a true measure of deflection. However, the ratio
$$ \boxed{\Omega_V L /U} $$
can still serve as a suitable number measuring the strength of of the Coriolis deflection (with $\Omega_V$ replaced
by $\Omega$ when dealing with motions on carousels). Indeed, if this ratio is of order unity, we can be sure that
the deflection is comparable to the total displacement. The deflection effect proves to be strong **if this ratio
is larger than 1**.

Estimate the strength $\Omega L /U$ of deflection a) for our paper sheet experiment and b) in the carousel video.

The ratio $\Omega L /U$ is $5\pi/2=7.9$ in a), and $2\pi=6.3$ in b). The fact that we consider the deflection strong if the ratio is larger than unity is in accordance with the carousel video since deflection may result in a complete return of the ball there. The effect is strong even in our paper sheet experiment (otherwise it would have been very difficult to see the difference between the two lines drawn).

Consider the case when the ball returns to the kid rolling the ball in the carousel video, and assume that the path of the ball (friction is negligible) goes through the center of rotation when observed from outside the carousel. Assuming the distance of the kid is $r$ from the center and the angular velocity is $\Omega$, what should be the tangential initial velocity of the ball on the carousel (in which direction?) in order to make the ball move like that? How should the radial velocity be chosen in order to ensure a full return of the ball, after half a revolution?

The tangential velocity of the ball should cancel the tangential velocity of the carousel, it should be $r \Omega$ to the right. A stationary observer can see a uniform motion of velocity $v$, along a diameter $2r$ in time $2r/v$. For full return after half a revolution, $t=\pi/\Omega$ and this yields $v=2/\pi r \Omega$.

A rather remarkable property of the expression for the strength is its **increase** with the length. With
a given velocity, the greater the extension of the motion in space, the larger the strength of the effect. This
shows that, in spite of the slow rotation of Earth, strong deflections are present on large, geographical scales.
**In the large-scale motion of the atmosphere and of the ocean Coriolis deflections are never negligible**.
In fact, the Coriolis force overcomes most of the other forces.

Estimate the strength of deflection on the Earth at mid latitudes a) for a wind blowing with $U=10 \text{ m/s}$ in a cyclone of size $L=1000 \text{ km}$ and b) for an oceanic eddy with a radius of $L=100 \text{ km}$ in which water moves with velocity $U=1 \text{ m/s}$.

The ratio $\Omega_V L /U$ is $5\ 10^{-5}\ 10^6/10=5$ in a cyclone (a), and $5\ 10^{-5}\ 10^5/1=5$ in an oceanic eddy (b). The fact that the numbers are equal, indicates that the effect of the Coriolis force is of equal importance in the atmosphere and in the oceans.

### Cyclones as atmospheric sinks

Mid-latitude cyclones are known to bring rain. This is due to a low pressure region in their center, causing the upwelling of wet air from the surface which then leads to precipitation.

Upwelling can only be present if there is a flow toward the center in the lower layers. Thus the figures

used when discussing water draining from a bathtub, is perfectly valid for the air flow towards the center of cyclones. Air parcels are exposed to the Coriolis effect and turn, on the Northern Hemisphere, to the right (on the Southern to the left). The consequence is a huge air vortex spinning in counter-clockwise (clockwise) direction. It can be considered a gigantic plughole vortex draining upward.

All cyclones follow this rule **without** any exception! This is so since, as we saw, hardly any other effects
can compete with the Coriolis effect on large scales. What was found to be negligible in our plugholes, is **robustly
present** in our every-day weather forecasts dominated by cyclones. Cyclones always rotate as the Coriolis force dictates.
(Anticyclones rotate, of course, in opposite directions but - lacking the clouds to trace out the spiraling motion - they
are not visible in weather maps.) At the Equator, without an $\Omega_V$ and, therefore, withut a deflection effect, cyclones
do not exist! (Note that tropical cyclones, or hurricanes, are not equatorial cyclones: they occur above 15 degrees to
the North or the the South only.) How could then the plughole vortices seen in the very first video be caused by the Coriolis
effect? This deceptive video, and many others of the same kind on the internet, are fake demonstrations.

### Air does not blow in the direction it is pushed but at right angles to it

There is a single force which is comparable to the horizontal component of the Coriolis force on large scales. This is the pressure force arising from horizontal pressure differences. The direction of this force (from higher to lower pressure) is the direction in which the material is pushed. Acceleration is brought about by the resultant force acting on air (or fluid) masses. Since velocity changes are rather slow in the atmosphere and in the ocean, the acceleration can practically be neglected. Accordingly, the Coriolis force $\boldsymbol{F}_C$ and the pressure force $\boldsymbol{F}$ originating from horizontal pressure differences balance each other. The vectors $\boldsymbol{F}_C$ and $\boldsymbol{F}$ are opposite to each other, as the figure shows for the Northern Hemisphere (the straight lines represent curves of constant pressure, isobars, and force $\boldsymbol{F}$ points from larger to lower pressure).

The velocity vector $\boldsymbol{v}$ is, however, perpendicular to the Coriolis force, and therefore velocity is perpendicular to the pressure force, too. As a result, the air or the water masses do not move in the direction they are pushed, but at right angles to the direction of the pressue difference. This is in conflict with everyday experience, e.g. flow in a pipe, where the fluid moves in the direction it is pushed. No wonder, the Coriolis force is very weak on small scales.

The tendency of moving perpendicular to the driving force can be seen in a simple ball experiment on a carousel. Take a slope with a low tilt angle and release a ball on it from rest. Initially, only gravity acts (the analogue of the pressure force) and the ball starts moving down the slope. With increasing velocity the Coriolis force increases and a motion evolves along a spiral-like path in which the resultant displacement is practically horizontal, i.e., perpendicular to the pressure force. In this video the slope is tilted towards the bottom of the picture.

### The weather map

As a surprising consequence of the orthogonality of the velocity and the pressure force, the isobars of a weather
map, lines of constant pressure, run **parallel to the wind** arrows so that higher pressure values are on the
right of the arrows on the Northern Hemisphere. A historical predecessor: Buys Ballot rule.

### Buys Ballot's rule

For winds in the Northern Hemisphere, the Dutch meteorologist formulated the following rule in 1857: if you turn your back to the wind, the low pressure will be to your left.

On the left and along the upper edge of the figure, two cyclones can be seen: closed isobars with the lowest values in the middle, and wind blowing in counter-clockwise direction.

### Water surface is tilted above oceanic currents

For oceanic currents a surprising consequence of the balance between the Coriolis and the pressure forces is
that the water surface is not horizontal above currents, it is slightly tilted. The reason for this is that in
slow flowing motions, pressure at some depth basically equals hydrostatic pressure which, in turn, is proportional
to the height of the water column. The horizontal pressure difference is thus accompanied by a **height difference**.
If an oceanic current is present with a certain velocity, the height of water should be larger on the right side
in the Northern Hemisphere.

The figure shows the average elevation of the sea level (over a month's period, during which waves are, of course, averaged out) above the Gulf Stream. Arrows indicate flow velocities and colors indicate the elevation above sea level relative to a reference value (given in m above mean sea level or mamsl). On the right of the Gulf Stream (longest arrows) elevation is about 60 cm, and -40 cm on the left. The total level difference is thus 1 m across an approximately 100 km wide current. Eddies turning counter-clockwise are clearly discernible as orange patches within the red region since they have a pressure minimum in their centers.

### Laboratory experiments with fluids to demonstrate strong Coriolis deflection in nature

We have seen that the strength of deflection in the plugholes of our homes is on the order of $10^{-4}$.
The low value is derived from the slowness of the Earth's rotation which is just 1 turn over a full day.
Strong deflections may be achieved with laboratory equipment rotating about 10 000 times faster. Since one
day is 1440 minutes, such a rotational speed is not irrealistic, you just have to produce a few revolutions
per minute (a lot slower than a CD player). In fact, experiments carried out with **rotating tanks**
filled with fluids not only show strong deflections but, with properly chosen parameters, can **faithfully
imitate the essence of large scale atmospheric or oceanic flows**.

Show that if you see a fluid pattern of size $L=10$ cm due to a fluid velocity of $U=1 \text{ cm/s}$ in a tank rotating with 5 revolutions per minute (rpm), the strength of deflection is exactly the same value as in a cylone or in an oceanic eddy.

In such a case the rotation period is $T=12$ s. The angular velocity $\Omega = 2 \pi/T \approx 0.5$ 1/s. The ratio $\Omega L /U$ is thus $0.5 \ 0.1/0.01=5$.

To illustrate the strong analogy with nature, let us take a cylinder with a radius of 25 cm, fill it with water up to a height of 10 cm, and rotate it with a speed of a few rpm. When injecting blue dye abruptly from above, penetrating in a few cm depth, an interesting pattern evolves as this video shows.

One sees a dye curtain evolving (non-existent in stationary fluids!). The identical motion of the dye at any height is a consequence of the Coriolis deflection which only depends on the horizontal dye velocity (the same for any dye particles right after injection, and at any time later), and is thus independent of the height. The dye curtain persists and becomes wavy (when observed from above) due to emerging vortices next to each other, rotating in counter-clockwise or clockwise direction, the analog of cyclones and anticyclones. The appearance of the phenomenon is rather similar to that of Polar Light (Aurora Borealis).

This is no accident, the motion of light emitting molecules is also governed by strong horizontal Coriolis deflection in the stratosphere. For other similar experimental observations see here and here.

Other experiments in rotating tanks can be designed to model the essense of the general circulation of the atmosphere, including its change due to a decrease of the temperature contrast between the Equator and the Polar Region (i.e. in the presence of a climate change).

### Summary

This short introduction to the Coriolis force demonstrated that on the scale of our buildings (meters) the rotation of Earth is hardly detectable without carefully designed experiments. This force has the peculiar feature of increasing the strength of the deflection it causes with the extension. On the planetary scales (100 to 1000 kilometers) the horizontal component of the Coriolis force is dominant and only the pressure force can compete with it. This leads to surprising effects, since nothing like it is experienced in every-day life (except carousels and rotating tank experiments). You can't comprehend the elements of the Earth System without knowing about the Coriolis force (let alone the great challenge of our age, climate change). You can get an impression of the global dynamics of the atmosphere and of the oceans by looking at these NASA videos:

note that no spiraling motion, no cyclones and no deflection effect are present at the Equator!

note that no eddies are present at the Equator!

Check your knowledge acquired: Quiz III

### Recommended further materials:

A. Persson: Is the Coriolis effect an ‘optical illusion’?

http://marshallplumb.mit.edu/experiments

http://www.karman.elte.hu/index_eng.php

Copyright: A. Gróf, Á. Szeidemann, T. Tél

This study was funded by the Content Pedagogy Research Program of the Hungarian Academy of Sciences.