Calculating Solar Rotation Using Sunspot Observations

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To calculate solar rotation using sunspot observations, one must determine the longitudinal angles of sunspots from a series of images taken over time. The process involves using angular displacement equations, specifically θ = s/r and θ = ωt, to derive angular velocity. Key to this calculation is identifying the x,y coordinates of sunspots in the images and translating these to positions on the sun's surface. The tilt of the sun's rotational axis, approximately 7.5° to the ecliptic, must also be considered, as it affects the apparent latitude of sunspots based on the time of year. Ultimately, calculating the difference in angle between two sunspots over time will yield the angular velocity of the sun's rotation.
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Homework Statement


Calculating solar of the sun through observing sunspots. We are given a series of photos of the sun over a period of time where we can see sun spots.

I am assuming the way to calculate would be to work out the longitudinal angles of the sun spots in the different photos and then use Angular Displacement to figure it out. The problem is I have no idea how to calculate longitude, or how to get the longitudinal values into something I can plug into the Angular Displacement equation.

Homework Equations



from what I understand θ=s/r. θ= ωt. But I have no idea how to use the data to get quantities I can plug into this.
 

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Did you draw a sketch?

For a given latitude and longitude, can you determine where you would see a sunspot? Then you just have to reverse the direction of the calculation.
 
sketch it out like this you mean? how would I find the quantative values from this?
 

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What data accompanies each observation? Presumably a time stamp of some form, but anything else? What's the timeframe for the whole series?

The reason I ask is that the Sun's rotational axis actually has a tilt (inclination) of about 7.5° to the ecliptic, so the time of year when the snapshot is taken, presuming an Earth-based platform for capturing the photos, will influence the apparent latitude -- spots won't track horizontally unless the viewing position has the rotation axis vertical and is located in the plane of the Sun's equator.
 
magnanimousto said:
sketch it out like this you mean?
That's not the direction I had in mind, but it can be useful as well.
how would I find the quantative values from this?
Well first you have to find the position in the image (like x,y-coordinates), and afterwards you have to translate this to a position on the actual (curved) surface of sun.

@gneill: I guess we can neglect this here.
 
mfb said:
@gneill: I guess we can neglect this here.
Could be. I can't tell the course level that the question pertains to from the given info, that's why I threw that out to see what the response might be. Carry on...
 
OK I get it. Thanks guys. I use the measurement of the x,y co-ordinates and then sin(inverse) to find angle. Then calculate difference in angle between the two spots per difference in time which would give me the angular velocity.
 
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