Components of Earth's angular velocity vector

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SUMMARY

The discussion focuses on calculating the components of the Earth's angular velocity vector (ω) using a coordinate system where x and y represent east and north directions, respectively, and z is the radial distance from the Earth's center. The latitude of the city is given as λ = 34 degrees. The relevant equations include the apparent gravitational acceleration and its relationship with ω, specifically g* = g - ω × (ω × r) and the derived expressions for gh* and gv*. The solution involves projecting ω onto the x, y, and z axes, leading to the conclusion that ω can be expressed as ω = ωsin(λ)j + ωcos(λ)k.

PREREQUISITES
  • Understanding of angular velocity vector components
  • Familiarity with coordinate systems in physics
  • Knowledge of gravitational acceleration equations
  • Basic trigonometry involving sine and cosine functions
NEXT STEPS
  • Study the derivation of angular velocity components in spherical coordinates
  • Learn about the effects of latitude on gravitational acceleration
  • Explore vector projection techniques in physics
  • Investigate the implications of Earth's rotation on local gravitational fields
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Students studying physics, particularly those focusing on mechanics and gravitational forces, as well as educators seeking to clarify concepts related to angular velocity and coordinate systems.

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Homework Statement


Using a coordinate system in whic x and y are due east and nort of the city and z is the radial distance outwards from te centre of te earth, find the compnents of w the Earth's angular velocity vector. You may assume that the latitude of the city is lamdba = 34degrees.


Homework Equations


I know that apparent gravitational acceleration g*=g-w x (w x r) and that gh* = w^2 rsin(lambda)cos(lambda) and gv* = g-w^2 r sin(lambda)^2. But I am not sure how to fit this all together to find w


The Attempt at a Solution


Any suggestions or help much appreciated!
 
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the diagram for this is in the notes. chapter 5 page 4. w is going vertically upward, mark on the x,y and z axes (into the page, toward north pole and radially outward respectively). now its just a case of projecting w onto the relative axes.
 
So is it just w= wsin(lambda)j +wcos(lamdba)k as stated in section 6.3? How is writing this down worth 4 marks?
 
More Edinburgh people! It's only 2 marks. But yeah it's that easy.
 

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