Physics calculator

Coriolis Force Calculation Example

Enter mass, velocity, latitude, travel direction, and units. View signed force, components, and SI checks. Use results for aircraft, oceans, projectiles, navigation, and experiments.

Input panel

Calculate a local Coriolis force

Bearing is measured clockwise from true north. Positive vertical velocity points upward.

Default angular velocity: 7.292115e-5 rad/s
Mass of the moving object.
Speed parallel to the local surface.
Use negative values for downward motion.
degrees
North is positive. South is negative.
degrees
0° north, 90° east, 180° south, 270° west.
rad/s
Use the default for Earth.
Reset values
Worked reference

Example data table

This example uses a one kilogram object moving eastward at 100 m/s, with no vertical velocity, at 45° north latitude.

Mass Horizontal speed Latitude Bearing East force North force Up force Total force
1 kg 100 m/s 45° 90° 0 N −0.010313 N +0.010313 N 0.014585 N
Method

Formula used

Vector equation: FC = −2m(Ω × v)

Horizontal magnitude for purely horizontal motion: |Fh| = 2mΩvh|sin φ|

  • FC is the Coriolis force in newtons.
  • m is mass in kilograms.
  • Ω is angular velocity in radians per second.
  • v is velocity in meters per second.
  • φ is latitude in degrees, converted to radians internally.
  • The calculator resolves signed east, north, and up components before finding total magnitude.
Steps

How to use this calculator

  1. Enter the moving object’s mass and choose its unit.
  2. Enter horizontal speed and select a matching speed unit.
  3. Enter vertical velocity. Use zero for level motion.
  4. Enter latitude using positive north and negative south values.
  5. Enter the travel bearing measured clockwise from true north.
  6. Keep Earth’s default angular velocity or enter another rotating system.
  7. Select Calculate force and read signed vector components above the form.
  8. Use CSV for a tabular record or PDF for a printable summary.
Physics context

Understanding Coriolis force

Why it appears

Coriolis force is an apparent force. It appears inside a rotating reference frame. Earth rotates beneath objects that move through the atmosphere, oceans, or laboratory systems. An observer fixed to Earth can see a path bend even when no sideways contact force exists. The bend does not come from a new physical interaction. It comes from describing motion on a rotating planet.

Local coordinate system

The calculator uses a local east, north, up coordinate system. East points toward increasing longitude. North points toward the geographic pole. Up points away from Earth’s center. Horizontal speed and bearing create eastward and northward velocity components. A vertical velocity can also be entered. The program then combines those components with the rotation vector.

Latitude changes the result

Latitude matters because Earth’s rotation vector has different local directions around the globe. At the equator, the vertical part of the rotation vector is zero. At the poles, it is entirely vertical. This changes the force components. For horizontal motion, the familiar horizontal effect grows with the sine of latitude. It is zero at the equator and largest near either pole.

Direction and signed components

Direction matters as much as latitude. A northbound object can receive an eastward or westward component, depending on the hemisphere and motion. An eastbound object can gain a northward or southward component. The calculator reports signed east, north, and up forces. Positive values point east, north, or upward. Negative values point west, south, or downward.

Mass and speed scaling

Speed has a direct effect. Doubling speed doubles the calculated force. Mass also has a direct effect. Doubling mass doubles force, while the resulting acceleration stays unchanged. This is useful when comparing a lightweight parcel with a large aircraft. Their apparent accelerations can match when their velocities and positions match, although their forces differ.

Using another rotating system

Earth’s angular velocity is set to a standard value by default. You can replace it for a rotating platform, a centrifuge, or another planet. Use radians per second. Keep all inputs physically consistent. The calculator converts selected mass and speed units to SI values before evaluating the vector expression.

Reading the output

Results include total force, horizontal force, force components, and acceleration components. The horizontal bearing of the force is also shown when it can be determined. A small result is normal for short, slow motions. The effect becomes important for long travel times, large distances, fast vehicles, winds, ocean currents, and ballistic trajectories.

A useful test case

Use a test first. Set mass to one kilogram, horizontal speed to one hundred metres per second, vertical velocity to zero, latitude to forty-five degrees, and bearing to ninety degrees. Compare component signs after reversing the bearing. This practice makes the coordinate convention easier to trust.

Limits of a first estimate

This tool does not replace a complete trajectory model. Real systems may involve gravity, drag, pressure gradients, thrust, friction, curvature, and changing latitude. Still, the computed value gives a clear first estimate. It also helps check signs, units, and expected direction before building a more detailed model.

Common questions

FAQs

1. What is Coriolis force?

It is an apparent force seen from a rotating reference frame. On Earth, it affects the apparent path of moving air, water, vehicles, and projectiles.

2. Which equation does this calculator use?

It uses the vector equation FC = −2m(Ω × v). The calculator resolves local east, north, and up velocity components before computing force.

3. Why does mass change the force?

Force equals mass times acceleration. A heavier object has a larger Coriolis force at the same location and velocity, while its Coriolis acceleration stays the same.

4. How does latitude affect the result?

For purely horizontal motion, the horizontal effect is zero at the equator and strongest near the poles. The detailed vector components also depend on latitude.

5. What do east, north, and up mean?

They are local coordinate directions. East follows increasing longitude, north follows the geographic meridian, and up points away from Earth’s center.

6. How is travel bearing measured?

Bearing is measured clockwise from true north. Use 0° for north, 90° for east, 180° for south, and 270° for west.

7. Why can the calculator show an up component?

Earth’s rotation axis is tilted relative to local directions. Eastward or westward motion can therefore create a vertical Coriolis component in this local model.

8. Can I use another planet or platform?

Yes. Replace the angular velocity with the rotating system’s value in radians per second. Keep latitude and local direction definitions consistent with that system.

9. Which units are accepted?

Mass accepts kilograms, grams, pounds, and tonnes. Speed accepts meters per second, kilometres per hour, miles per hour, and knots.

10. Why is my result very small?

Coriolis effects are often tiny over short times and distances. They become more noticeable for fast motion, long travel, large-scale weather, and ocean currents.

11. Does this predict the whole path?

No. It estimates one rotating-frame effect under stated conditions.

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