Scientific importance of total Solar eclipses?

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Discussion Overview

The discussion revolves around the scientific importance of ground-based observations of the Solar corona during total solar eclipses. Participants explore whether such observations provide unique insights that cannot be achieved with space-based telescopes, considering both historical and contemporary contexts.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • Some participants question the necessity of ground-based photographs of the Solar corona during total eclipses, suggesting that similar observations could be made with space-based telescopes using sun shields.
  • Others mention that coronal imaging is possible during an eclipse, but acknowledge that coronagraphs are typically used for such imaging in practice.
  • Historical references are made to Eddington's experiment during a total solar eclipse, which was significant for testing general relativity, highlighting the limitations of technology at that time.
  • One participant notes that ground-based observations may be better suited for imaging the closest parts of the corona to the Sun's disc, although this claim is described as unsatisfactory and lacking detail.
  • Concerns are raised about the rarity of total solar eclipses and the limited observation time, questioning whether the advantages of ground-based observations outweigh those of continuous observations from solar observatories.

Areas of Agreement / Disagreement

Participants express differing views on the scientific value of ground-based observations during total solar eclipses compared to space-based methods. There is no consensus on whether the unique conditions of an eclipse provide significant advantages for scientific study.

Contextual Notes

Participants reference historical limitations in technology and the specific conditions required for observations during eclipses, which may affect the validity of claims regarding the advantages of ground-based observations.

tarquinius
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I was wondering whether there is an actual scientific point of taking ground-based photographs of the Solar corona during total eclipses on Earth. It seems to attract a lot of attention from well equipped amateurs around the world and the pictures of the fine plasma structure surely look great, but shouldn't such conditions be routinely achievable in space by simply obscuring the Solar disc with a little sun shield?

In other words, is there any scientific aspect of a ground-based total Solar eclipse observation that would not be achievable routinely with space-based telescopes?

Thanks for answers.

-SF-
 
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tarquinius said:
In other words, is there any scientific aspect of a ground-based total Solar eclipse observation that would not be achievable routinely with space-based telescopes?
I am not an astrophysicist, but I heard the other day on the radio a solar expert who answered this very question by a resounding no!
 
My understanding would be: coronal imaging (we already see the corona naked eye during an eclipse). But then again artificial eclipses (coronographs, sample image below) blocking the light from the disk are how this is done in practice nowadays, so the resounding no sounds right.

corono1.jpg


It wasn't always the case though, wasn't an eclipse used for an early test of GR (lensing of distant stars by the Sun)?
 
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Yes, it was eddington who did the experiment with a total solar eclipse to prove einstein was correct (though I think it was heavily debated back then)
 
Ah yes, Eddington, thanks. It's strange to think that something as simple as a coronograph wasn't available yet at the time, I wonder what the issue was.

Edit. Ah yes daylight. Thanks @mathman.
 
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wabbit said:
Ah yes, Eddington, thanks. It's strange to think that something as simple as a coronograph wasn't available yet at the time, I wonder what the issue was.
Probably human error and proving Newtons theory wrong, or something like that :p
 
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Oh yes, I knew about the historical importance and the time when space telescopes simply were not an option. I was thinking of some present day applications.

While reading online, I came across an article claiming that the ground based observations during eclipses are better suited for imaging of the closest parts of the corona to the Sun disc, justifying it a bit unsatisfactorily. Do you know anything about that?
 
Maybe on earth, but I would think you could yield the same results (or similar enough) from a telescope in space using a disc to block the light in the telescope. Of course, I could be very wrong :p
 
tarquinius said:
Oh yes, I knew about the historical importance and the time when space telescopes simply were not an option. I was thinking of some present day applications.

While reading online, I came across an article claiming that the ground based observations during eclipses are better suited for imaging of the closest parts of the corona to the Sun disc, justifying it a bit unsatisfactorily. Do you know anything about that?
Interesting, although I would suspect this must be a pretty special case : there are few eclipses and each one is only visible for a few minutes, and only from a small patch of the Earth - so any advantage is limited to a couple minutes observation from a few telescopes, vs 100s of days per year from many solar observatories for coronographs, and these rare observations must trump what one can infer from a very large number of not-quite-as-good ones. But I'd be interested to hear more about it.
 
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wabbit said:
Ah yes, Eddington, thanks. It's strange to think that something as simple as a coronograph wasn't available yet at the time, I wonder what the issue was.
For Eddington it was not enough to block the sun. It was also necessary to turn off the skylight in order to see the stars.
 
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  • #11
mathman said:
For Eddington it was not enough to block the sun. It was also necessary to turn off the skylight in order to see the stars.
Gee do I feel stupid now :)
 

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