Investigating the Magnus Effect on Solar Wind

Click For Summary
SUMMARY

The discussion centers on the applicability of the Magnus effect to solar wind dynamics. Participants assert that the solar wind, primarily composed of particles rather than a fluid medium, does not exhibit the Magnus effect as it would require conditions beyond the ballistic limit. The conversation highlights that the mean free path of solar wind particles is pressure-dependent, and significant hydrodynamic effects would only manifest with sails larger than thousands of kilometers. Additionally, the dominant pressure influencing solar sails is radiation pressure, with solar wind contributing minimally.

PREREQUISITES
  • Understanding of the Magnus effect and its principles
  • Knowledge of solar wind composition and behavior
  • Familiarity with concepts of mean free path and pressure in plasma physics
  • Basic grasp of radiation pressure and its impact on solar sails
NEXT STEPS
  • Research the principles of the Magnus effect in fluid dynamics
  • Explore the characteristics and behavior of solar wind in astrophysics
  • Study the concept of mean free path in different mediums
  • Investigate the design and efficiency of solar sails in space exploration
USEFUL FOR

Astronomers, astrophysicists, aerospace engineers, and anyone interested in the dynamics of solar sails and the interaction of solar wind with spacecraft.

d3mm
Messages
140
Reaction score
1
I can't find authorative sources on whether the magnus effect works on the solar wind.

I thought the solar wind was mostly particles, not a fluid medium, and therefore it would not.

I thought this was the reason for the flat nature of solar sails. If the solar wind acted like a fluid medium, solar sails ought to be aerofoils like boat sails or airplane wings.
 
Last edited:
Physics news on Phys.org


First of all the Magnus effect should only work if we are not in the ballistic limit. The mean free path of the molecules is pressure dependent and I don't know what the pressure distribution is. But in interstellar medium hydrodynamic effects should not show until your sail is much larger than thousands of kilometres. You might find the pressure and thus the mean free path in the heliosphere somewhere on the web. The wikipedia article on the Magnus effect states that it probably has an effect on the planets. The solar wind is extremely fast, so some effect should be expected (it is also supersonic but I have no idea what that means).
 


The dominant fraction of the pressure is radiation - catch it, reflect it or lose it, shape does not really matter. Solar wind is just a small bonus to the pressure.
 

Similar threads

  • · Replies 5 ·
Replies
5
Views
3K
  • · Replies 5 ·
Replies
5
Views
2K
  • · Replies 4 ·
Replies
4
Views
3K
  • · Replies 3 ·
Replies
3
Views
2K
  • · Replies 69 ·
3
Replies
69
Views
17K
  • · Replies 1 ·
Replies
1
Views
3K
  • · Replies 46 ·
2
Replies
46
Views
12K
  • · Replies 3 ·
Replies
3
Views
2K
  • · Replies 4 ·
Replies
4
Views
3K
  • · Replies 9 ·
Replies
9
Views
1K