Determine the number of times the magnetic field has wound around the Sun

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Homework Help Overview

The problem involves determining the number of times the magnetic field has wound around the Sun at a heliocentric distance of 70 AU. The context includes concepts related to magnetic fields and their behavior in relation to celestial bodies.

Discussion Character

  • Exploratory, Assumption checking, Conceptual clarification

Approaches and Questions Raised

  • The original poster attempts to relate the circumference of the Sun to a distance of 70 AU, questioning the relevance of the magnetic field source's location. Other participants suggest investigating the interplanetary magnetic field and its connection to the Sun's rotation, as well as considering the angular velocity of charged particles in a magnetic field.

Discussion Status

The discussion is ongoing, with participants exploring various aspects of the problem. Some guidance has been offered regarding the investigation of the interplanetary magnetic field and its dynamics, but no consensus has been reached on the approach to the problem.

Contextual Notes

Participants are considering the implications of the magnetic field's source location and the relationship between the Sun's radius and the distance of 70 AU. There is an acknowledgment of the complexity of the problem and the need for further exploration of relevant concepts.

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Homework Statement



Hi,
I know that this probably is easy to calculate, but I have the ability to thing the opposite about problems, therefore I'm stuck with this one. The question is

Determine the number of times the magnetic field has wound around the Sun by a heliocentric distance of 70 AU.

Homework Equations



I guess that I have to find a relation between the circumference of the Sun (or a circle generally) and the length of something, in this case L=70 AU. But as I mentioned, I really don't know what to do.

Is it relevant to determine where the magnetic field source is located? If yes, then R=10Rs (Rs = radius of the Sun).

The Attempt at a Solution

 
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You'll want to do some investigation on the topic of the interplanetary magnetic field. Find out where its base is "locked" to the rotation of the Sun, and how the field lines are carried outwards (what entrains the field lines?). Hint: find the radial speed.
 
I assume that the angular velocity for a charged particle in a magnetic field is:
T=2*π*m/qB ; m should be the mass of an electron (?) , q=the charge , B = magnetic field strength, which I have. And where it is "locked", isn't it the 10*Rs that I mentioned?
Thanks btw!
 
Take a look here to begin with.
 

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