Calculating tangential velocity of an air parcel circulating a tornado

Click For Summary
SUMMARY

The discussion focuses on calculating the tangential velocity of an air parcel in a tornado, specifically when the parcel is 2000m and then 100m from the tornado center. The key equations used are v = rω and ω = v/r, where ω represents angular velocity. The calculated angular velocity is 0.005 radians/sec, leading to a tangential velocity of 0.5 m/s at 100m from the center. The conclusion drawn is that tangential velocity decreases as the radius decreases due to the nature of circular motion, contrasting with planetary motion influenced by gravitational forces.

PREREQUISITES
  • Understanding of circular motion principles
  • Familiarity with angular velocity and tangential velocity concepts
  • Basic knowledge of physics equations related to motion
  • Ability to perform unit conversions and calculations
NEXT STEPS
  • Study the relationship between angular velocity and tangential velocity in circular motion
  • Explore the effects of gravitational forces on planetary motion
  • Learn about the dynamics of tornadoes and their impact on air parcel movement
  • Investigate real-world applications of circular motion in meteorology
USEFUL FOR

Students studying physics, meteorologists analyzing tornado dynamics, and anyone interested in the principles of circular motion and its applications in atmospheric science.

Timebomb3750
Messages
59
Reaction score
0

Homework Statement



If an air parcel 2000m from a tornado center has a tangential velocity of 10 m/s, what is the resultant tangential velocity if the parcel is 100m from the tornado center.

Homework Equations



v = rω, where r = radius, and ω = angular velocity
ω = v/r

The Attempt at a Solution



I understand that the tangential velocity of the air parcel should be much faster as radius drops. But how am I supposed to calculate tangential velocity of it requires the calculation of angular velocity which requires velocity. I'm really lost.
 
Physics news on Phys.org
Angular Velocity is not dependent on radius, therefore, it will be the same for each radius. You can find angular velocity with the equation ω = v/r. Use that value to find the tangential velocity at the new radius.
 
NewtonsHead said:
Angular Velocity is not dependent on radius, therefore, it will be the same for each radius. You can find angular velocity with the equation ω = v/r. Use that value to find the tangential velocity at the new radius.

Okay, here's my work.

ω = 10 (m/s)/ 2000m = .005 radians/sec

Then I put that into the tangential velocity question:

v = rω = 100m*.005 radians/sec = .5 m/s

Why is it that the tangential velocity got slower as radius decreased? I thought it was the other way around as I mentioned in my first post.
 
The tangential velocity is slower near the center of the disk because it doesn't have to circle around as big of a radius as the outside. Imagine running around a circular track... the people on the outside have to run faster to keep up with the people on the inside lanes. This is not true for planets though, because the inner planets are affected by the sun's gravity more and travel faster in the tangential direction to maintain their orbits.
 

Similar threads

Replies
12
Views
2K
  • · Replies 11 ·
Replies
11
Views
2K
Replies
9
Views
2K
  • · Replies 2 ·
Replies
2
Views
2K
  • · Replies 7 ·
Replies
7
Views
2K
Replies
4
Views
2K
  • · Replies 2 ·
Replies
2
Views
2K
  • · Replies 13 ·
Replies
13
Views
1K
  • · Replies 10 ·
Replies
10
Views
2K
  • · Replies 1 ·
Replies
1
Views
3K