Scientific importance of total Solar eclipses?

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SUMMARY

The discussion centers on the scientific significance of ground-based observations of the Solar corona during total solar eclipses compared to space-based telescopes. Participants highlight that while ground-based observations can capture unique aspects of the corona, such as imaging the closest parts to the Sun's disc, modern coronagraphs in space can achieve similar results. Historical context is provided, referencing Eddington's 1919 experiment that tested General Relativity using a total solar eclipse, emphasizing the limitations of technology at that time. Ultimately, the consensus is that while ground-based observations are valuable, they are not strictly necessary for scientific advancements in solar studies.

PREREQUISITES
  • Understanding of solar corona and its imaging techniques
  • Familiarity with coronagraphs and their function in solar observation
  • Knowledge of General Relativity and its historical experiments
  • Awareness of the limitations of observational astronomy
NEXT STEPS
  • Research the capabilities and limitations of solar coronagraphs in space
  • Explore the historical significance of Eddington's 1919 solar eclipse experiment
  • Investigate current ground-based solar observation techniques during eclipses
  • Learn about advancements in solar imaging technology and their applications
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Astronomers, astrophysicists, and students interested in solar studies, as well as enthusiasts of observational astronomy seeking to understand the relevance of total solar eclipses in scientific research.

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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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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