Exploring Orbital Velocity vs RMS of Eddy Velocities

In summary, there is a difference between the orbital velocity of an eddy and the root mean square of the velocity fluctuations in a turbulent flow. The characteristic eddy velocity is the orbital velocity, and the turnover time of an eddy is the time needed for it to complete one revolution. However, there is debate over whether the orbital velocity is the same as the root mean square of the velocity fluctuations. Many books make this assumption to derive equations, but it may not accurately represent the large scales dominated by low frequencies.
  • #1
rdemyan
4
0
Is there a difference between the orbital velocity of an eddy and the root mean square of the velocity fluctuations? I'm particularly interested in understanding the eddy turnover time of the largest eddies in a turbulent flow, which is given by the characteristic eddy size and the characteristic eddy velocity. As I understand it, this characteristic eddy velocity is the orbital velocity. The turnover time is the time needed for the spinning eddy to complete one revolution; so the orbital velocity should be used. Frankly I'm not convinced that the orbital velocity is the same as the root mean square of the velocity fluctuations. It seems that many books derive equations based on this assumption, but the authors are usually careful to state that the velocities are "of the order of" which then allows for the derivation of relatively simple equations. I would greatly appreciate thoughts on this.
 
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  • #2
I've never heard it called orbital velocity before. I'll preface this by saying I'm not super well-versed in turbulence theory.

If you look at a turbulent power spectrum, it is highly biased toward low frequencies representing the largest eddies. This implies that the rms of the fluctuations technically contains all scales but is overwhelmingly dominated by the large scales. If an author makes the assumption you discuss, it's basically equivalent to making the assumption that the power contained in the large scales is much larger than small scales so the rms of the fluctuations are a good stand-in for the large scales.
 

Related to Exploring Orbital Velocity vs RMS of Eddy Velocities

What is the difference between orbital velocity and RMS of eddy velocities?

Orbital velocity refers to the speed at which an object needs to travel to maintain a stable orbit around a celestial body, such as a planet or star. RMS (Root Mean Square) of eddy velocities refers to a statistical measure of the magnitude of velocity fluctuations within a turbulent flow, often used in fluid dynamics to describe the intensity of turbulence.

How is orbital velocity calculated?

Orbital velocity is calculated using the formula \( v = \sqrt{\frac{GM}{r}} \), where \( G \) is the gravitational constant, \( M \) is the mass of the celestial body being orbited, and \( r \) is the radius of the orbit. This formula assumes a circular orbit and neglects other forces such as atmospheric drag.

What factors influence the RMS of eddy velocities?

The RMS of eddy velocities is influenced by factors such as the scale of turbulence, the viscosity of the fluid, and the energy input into the system. It is often calculated from velocity measurements at various points within the flow and provides insight into the intensity and distribution of turbulent fluctuations.

Why is it important to compare orbital velocity with RMS of eddy velocities?

Comparing orbital velocity with RMS of eddy velocities can be important in contexts such as satellite operations and atmospheric science. For satellites in low Earth orbit, understanding the turbulence in the upper atmosphere can help in predicting drag forces and potential impacts on orbital stability. In planetary atmospheres, this comparison can aid in understanding the dynamics of atmospheric circulation and weather patterns.

Can RMS of eddy velocities affect the stability of an orbit?

Yes, RMS of eddy velocities can affect the stability of an orbit, particularly for low Earth orbit satellites. Turbulent eddies in the upper atmosphere can create variations in atmospheric density and drag forces, potentially leading to changes in the satellite's velocity and trajectory. This can necessitate adjustments to maintain a stable orbit.

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