What happens to coronal mass ejections?

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Discussion Overview

The discussion revolves around coronal mass ejections (CMEs), their characteristics, and their interactions with the Earth and the solar system. Participants explore the nature of CMEs, their speed, composition, and potential effects on Earth and beyond, including the auroras and detection from distant locations.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • Some participants describe CMEs as large amounts of plasma ejected from the sun due to collapsing magnetic loops, which can impact Earth’s electronics and satellites.
  • There is mention of the speed of CMEs varying significantly, typically between 800 - 3200 km/s, and that they eventually become part of the solar wind.
  • One participant suggests that some CME material may fall back to the sun, while the rest is ejected into space.
  • Concerns are raised about how far away a significant CME would be detectable, with some suggesting it could be seen from the outer reaches of the solar system.
  • There is a discussion about the interaction of CMEs with planetary magnetic fields and the heliopause, with uncertainty expressed about the outcomes of such interactions.
  • Participants debate the role of solar flares in causing auroras, with differing views on whether the auroras are primarily caused by solar particles or by particles already trapped in the Van Allen belts.
  • One participant challenges another to provide research to support claims about the auroras, indicating a lack of consensus on the mechanisms involved.

Areas of Agreement / Disagreement

Participants express multiple competing views regarding the effects of CMEs on Earth and the mechanisms behind auroras. There is no clear consensus on the primary causes of auroras or the fate of CME material once ejected from the sun.

Contextual Notes

Some claims about the detection of CMEs and their effects on auroras depend on specific conditions and assumptions that are not fully explored in the discussion. The relationship between solar activity and auroras remains complex and is subject to ongoing debate.

newjerseyrunner
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This thread got me wondering something: https://www.physicsforums.com/threads/kic-8462852-in-the-news.837900/page-5 Long story short: someone suggested starspots as a reason for it's weird variance. It had some problems with it, but it did get me wondering.

I know sunspots are caused by magnetic loops pushing plasma around and when these loops collapse, large amounts of plasma gets shot of into space in a solar flare. If that material hits Earth, it can cause problems with our electronics and satellites so we watch for them.

Other than that, I don't know much about them, what happens to all of that mass? I know that they are traveling at immense speed, and extremely hot. They're also charged and all of the particles would be charged the same way (or else they wouldn't have been stuck in the magnetic loop in the first place) so they should push themselves apart.

Then what happens? Is most of the material at escape velocity? Does it end up in the galactic wind eventually? Also, more relevant to the other thread, if the sun threw a tantrum, how far away would that be detectable from? I would think a huge mass of hot plasma being thrown from a star should produce a noticeable cloud glowing in the IR.
 
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newjerseyrunner said:
know sunspots are caused by magnetic loops pushing plasma around and when these loops collapse, large amounts of plasma gets shot of into space in a solar flare. If that material hits Earth, it can cause problems with our electronics and satellites so we watch for them.

Yes, that is correct, its gets trapped in the Earth's magnetic field, and it also causes the beautiful aurora around both the polar regions
newjerseyrunner said:
Other than that, I don't know much about them, what happens to all of that mass? I know that they are traveling at immense speed, and extremely hot. They're also charged and all of the particles would be charged the same way (or else they wouldn't have been stuck in the magnetic loop in the first place) so they should push themselves apart.
its speed varies greatly depending on the intensity anywhere between 800 - 3200 km/s. 3200 being an extreme. 1000 - 2000 km/s being the common range
As they propagate out, they will slow down and will become part of the normal solar wind
The solar wind speed and density as I type this is ...
Solar wind
speed: 386.2 km/sec
density: 2.2 protons/cm3
During a large CME, proton densities can get up to over 100 protons / cm3 which when compared to a cm3 of water is extremely low density

The CME's and solar wind in general, are primarily composed of protons and electrons
newjerseyrunner said:
Then what happens? Is most of the material at escape velocity? Does it end up in the galactic wind eventually? Also, more relevant to the other thread, if the sun threw a tantrum, how far away would that be detectable from? I would think a huge mass of hot plasma being thrown from a star should produce a noticeable cloud glowing in the IR.

some of it falls back onto the sun ( this can be seen in many of the videos of CME's), the rest gets blasted out into space.

Would be easily detected from the outer reaches of the solar system ... but from many lightyears away ... I can't answer thatDave
 
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Few CME's happen to be emitted on an intercept course with Earth [think of the odds]. Those that are, are blunted by the magnetosphere which weakens their effects at ground level. As Dave noted effects of solar emissions are most pronounced at the magnetic poles where the magnetosphere is weakest.
 
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If there was a solar storm, would it make a noticeable change in surrounding solar neighborhood that could be detected light years away?
 
I would think that any CME missing the Earth will just keep on going, unless/until it hits something like another planetary magnetic field. What would happen when it hits the heliopause and the magnetosphere ? We do not know.
 
AgentSmith said:
I would think that any CME missing the Earth will just keep on going, unless/until it hits something like another planetary magnetic field.

Any CME, regardless of if the Earth is in its path or not 99.99% of it goes right on past
CME's are huge and any that are directed in the Earths' direction, only a tiny fraction will be intercepted by the Earths' magnetic field

in this pic of a large CME, the Earth size in comparison would be about the size of that bright star centre right, just a few pixels

9729348_orig.gif
Dave
 
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davenn said:
...Its gets trapped in the Earth's magnetic field, and it also causes the beautiful aurora around both the polar regions ... Dave
Yes that is slightly true, but very little, if any, of the solar flare is trapped. The aurora is mainly caused by charged particles that have long been trapped in the Van Allen belts.

The Earth's magnetic field lines converge more at lower altitudes and the trapped particles "mirror" back and forth from the North and South field convergence zones, normally turning around still high in the rare atmosphere, with little excitation of it / weak aurora. What the solar particle discharge that hits the Earth does, is make pressure on the Earth's field lines. Then the turn-a-round points for the already trapped particle can be closer to the Earth's surface - in denser but still rarefied atmosphere.

SUMMARY: The solar flare particle pulse does not DIRECTLY cause the northern lights.

It is interesting to note that the dominate green line, is from the meta-stable (first order forbidden) decay of an excited state of oxygen. It has a very low radiative transition probably, and when it decayed is very uncertain (compare to permitted decays). Thus by the uncertainty principle its "Delta T" is large and its "Delta E" is very small. I. e. its wave length and frequency (energy) are very precise. For an EM photon to have a precise frequency, it must have many cycles. So many that the green line photons from the aurora are more than a meter long!

Most people, even some Ph. D. physicists, think of photons as small ball-like packets of energy. I have measured the length of some from a low pressure lamp (so their transition is usually completed before any significant collision occurs). They were 30cm long.

How I measured the length of photons is explained here:
https://www.physicsforums.com/threads/how-a-photon-is-created.818369/#post-5140207
 
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BillyT said:
Yes that is slightly true, but very little, if any, of the solar flare is trapped. The aurora is mainly caused by charged particles that have long been trapped in the Van Allen belts.

Sorry, but if that were true, then there would be bright aurora all the time

please provide solid research papers to support your claim
and I and dozens of others will admit error

Instead, we get strong aurora directly associated with the occurrence of flares and CME's
The Van Allen belts are too high up to be causing the aurora, which are happening at a much lower altitude ... around 50 - 150 km

Everything I have so far read over the years clearly states that the Van Allen belts are fed by the geomagnetic storms that cause the aurora, NOT the other way around where the particles in the belts cause the geomagnetic storms and then the auroraDave
 
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