The Coronal Heating Problem - The Hydrogen Fusion Core disappears?

In summary, the Coronal Heating Problem has been revised to only consider the discontinuity between the cool Photosphere and the Hot Corona, without taking into account the very hot Solar interior. Recent findings suggest that the heating of the corona is a result of flaring and energy transport through magnetic fields, rather than direct heat transfer from the core. This approach has been met with criticism, as it ignores the significant heat and energy produced by the core and raises questions about the applicability of the second law of thermodynamics. However, it appears that this is the current explanation for the Coronal Heating Problem, as reflected in Wikipedia's recent edits.
  • #1
Gfellow
63
0
TL;DR Summary
Edits in Wikipedia "The Coronal Heating Problem" appear to have removed the Hot Hydrogen Fusion Core as part of the problem?
In previous manifestations explaining the Coronal Heating Problem, scientists pointed out the discontinuity between a very hot Solar interior, the 'cool' Photosphere and a Hot Corona.
According to the newly modified entry in Wikipedia, they now explain the discontinuity only between a cool Photosphere and a Hot Corona.
No Solar interior.
Am I missing something?
Please let me know if I've got this wrong; I do have a slight dyslexia problem.

https://en.wikipedia.org/wiki/Stellar_corona#Coronal_heating_problem
 
Astronomy news on Phys.org
  • #2
I'm not sure why the interior details matter that much, except in so much as they might allow energy transfer via non-thermodynamic processes. The temperature discontinuity isn't between the corona and the interior, it's between the corona and the photosphere after all.
 
  • Like
Likes stefan r
  • #3
Gfellow said:
Summary:: Edits in Wikipedia "The Coronal Heating Problem" appear to have removed the Hot Hydrogen Fusion Core as part of the problem?

No Solar interior.
Am I missing something?

yes, you are.
The core doesn't have much to do with the heating of the corona ( no direct link)
The recent findings ( last few years) hint that the heating is a result of flaring and transport of energy by magnetic fields

here's 3 sites to get you started, I'm sure you can delve deeper :)
https://phys.org/news/2019-09-solar-corona.html

https://science.nasa.gov/news-articles/the-mystery-of-coronal-heating

https://www.sciencedirect.com/science/article/abs/pii/016779779090011TDAve
 
  • Informative
  • Like
Likes sophiecentaur, Klystron, berkeman and 1 other person
  • #4
Thanks for the reply and links.
Isn't it a little like taking note of the heat coming from a stove in a winter cabin, musing as to why the stove is cool, the room is warm - and ignoring the interior heat of the stove?
 
  • #5
Gfellow said:
Isn't it a little like taking note of the heat coming from a stove in a winter cabin, musing as to why the stove is cool, the room is warm - and ignoring the interior heat of the stove?

It's more like asking how the air just above the stove's surface is getting heated and ignoring the details of how the wood burns, as it isn't relevant. Exactly how the heat is transferred from the solar core to the upper layers isn't really important. It's about how the upper layers transfer heat to the corona.
 
  • Like
Likes davenn
  • #6
Isn't really important? A whopping great solar core furnace?
The magnitude temperatures such as these are hard for me to grasp, so I created this model to help me understand the problem:
Let’s pretend we can drop the temperature of the Photosphere to 0 Degrees Celsius so this shell is the temperature of a snowball:
002 Snowball registered .jpg

Then let us drop the temperatures of the inner core and outer atmospheric Corona in proportion: What one ends up with are exceedingly high temperatures from the solar core and high temperatures in the Corona - with a snowball shell sandwiched in between:
snowball inside hand freeze and if core break open.jpg


Sandwiched between this snowball shell, the core would be 2,700 C - hot enough to melt steel - and the atmospheric Corona would have a temperature that varies from 180 C to 1,800 C - a temperature so hot that you if were standing in the vicinity of this temperature-dropped snowball, you would either parboil or vaporize.
thermodynamics and rhe sun.jpg

The above image was taken from Wikipedia's page 'The Coronal heating problem' a year ago. It has now disappeared.
Is there something that has recently occurred in solar science that I am unaware of?
 
  • #7
Gfellow said:
The above image was taken from Wikipedia's page 'The Coronal heating problem' a year ago. It has now disappeared.

So? Wikipedia editors do their own thing.

Gfellow said:
Isn't really important? A whopping great solar core furnace?

Nope. Don't get me wrong. It's obviously important in the grand scheme of understanding how stars function, but the details of core fusion are not always important when you're trying to understand a specific aspect of a star. Especially on small time scales.

Gfellow said:
Sandwiched between this snowball shell, the core would be 2,700 C - hot enough to melt steel - and the atmospheric Corona would have a temperature that varies from 180 C to 1,800 C - a temperature so hot that you if were standing in the vicinity of this temperature-dropped snowball, you would either parboil or vaporize.

Well, if we scale things like you said, you'd probably be okay thanks to the extremely low density of the snowball-corona.
 
  • #8
Drakkith said:
It's about how the upper layers transfer heat to the corona.

As heat flows from hot to cold by definition, the colder upper layers cannot transfer heat to the hotter corona. There is energy transferred to the corona, but if it comes from the upper layers it is not heat.

It has already been mentioned before that there is energy transport by magnetic fields involved. Leaving the core out of the discussion would require that it has no significant impact on the generation of these magnetic fields. Is that the case?
 
  • #9
DrStupid said:
As heat flows from hot to cold by definition, the colder upper layers cannot transfer heat to the hotter corona. There is energy transferred to the corona, but if it comes from the upper layers it is not heat.

Indeed. I didn't think anyone would catch my little slip there. Shoulda known better. :wink:

DrStupid said:
It has already been mentioned before that there is energy transport by magnetic fields involved. Leaving the core out of the discussion would require that it has no significant impact on the generation of these magnetic fields. Is that the case?

I believe so. The core is obviously important in keeping the interior of the Sun hot, but beyond that I don't think it matters for understanding how the corona gets heated. If all fusion in the core ceased right now the Sun would still appear to function normally for years and years.
 
  • #10
Just seems myopic, ignoring the elephant in the room, a 15 million C solar core, that no one has as yet discovered a venting solution for heat dissipation.
Divorcing the Corona from the Photosphere and the core makes a mockery of the Coronal heating problem - the 2nd law of Thermodynamics - hot, through cold, to hot; it's a cop-out to what should be an intriguing and challenging problem.
Wikipedia is a major referencing tool for millions of people. Disengaging the Core altogether from the Coronal Heating Problem is disturbingly disappointing to say the least.
But if nobody else is bothered, I'll let the subject drop.
 
  • Skeptical
Likes weirdoguy and Motore
  • #11
Gfellow said:
Just seems myopic, ignoring the elephant in the room, a 15 million C solar core, that no one has as yet discovered a venting solution for heat dissipation.

What are you talking about? The heat dissipation is almost entirely due to radiated EM radiation from the photosphere, with heat being transferred from the core via convection and radiation transfer. This is trivial.

Gfellow said:
Divorcing the Corona from the Photosphere and the core makes a mockery of the Coronal heating problem - the 2nd law of Thermodynamics - hot, through cold, to hot; it's a cop-out to what should be an intriguing and challenging problem.

No one has divorced it from the photosphere. And no one has really divorced it from the core either. The core provides the heat that keeps the photosphere and other outer layers hot, and it is these hot layers of plasma that determine how the corona is heated.

It's quite simply that the details of fusion don't really matter when we look into how the corona is heated. If fusion ceased in the core the Sun would still behave normally for millennia, as it has an enormous amount of thermal energy in its huge mass and would still be heated by gravitational contraction. So you'd still have a very hot core that transitions to lower temperature outer layers with a surrounding corona.

And I'll say once again that time and distance scales matter here. Both dominant heating theories, magnetic reconnection and wave heating theory, take place on short time scales and are confined to the upper layers. NOTHING in the core will affect this, as changes to the core take a very long time to propagate outward and are typically constrained to relatively small temperature and density fluctuations that don't drastically change anything.

Gfellow said:
Wikipedia is a major referencing tool for millions of people. Disengaging the Core altogether from the Coronal Heating Problem is disturbingly disappointing to say the least.

Not if it doesn't matter that the two are 'disengaged'.
 
  • #12
Gfellow said:
Isn't it a little like taking note of the heat coming from a stove in a winter cabin, musing as to why the stove is cool, the room is warm - and ignoring the interior heat of the stove?

It's more like taking note of the heat in the room from an electric heater and worrying about whether the electricity comes from coal or nuclear.
 
  • Like
Likes davenn and Drakkith
  • #13
Vanadium 50 said:
It's more like taking note of the heat in the room from an electric heater and worrying about whether the electricity comes from coal or nuclear.

It's more like worrying about whether the electricity comes from a distant power plant or from batteries inside the room. My question in #8 still remains: Is Sun's core significantly involved in the generation of the mangetic field that heats the corona or not? Speculations about a suddenly stopping fusion don't answer this question.
 
  • #14
DrStupid said:
Is Sun's core significantly involved in the generation of the mangetic field that heats the corona or not?

As I've said already, I don't think so. However I'm certainly not an expert in this area, so I'd be interested in hearing from someone who is.
 
  • #15
Gfellow said:
Just seems myopic, ignoring the elephant in the room, a 15 million C solar core, that no one has as yet discovered a venting solution for heat dissipation.
You are not understanding or listening to what is being said.
Using your reasoning, the photosphere should be the same temp ( or somewhere close to) as the core
It isn't, it's millions of deg cooler at ~ 5600-6000 K (C).
But directly above the photosphere, the corona, is suddenly a million K ... so obviously the core wasn't doing it!
as the layer in between ( the photosphere) is VERY cool in comparison.
THAT was the reason why for many years it wasn't understood and a mystery as to why / how the corona could be so much hotter.
Gfellow said:
Divorcing the Corona from the photosphere and the core makes a mockery of the Coronal heating problem...

NO-ONE is divorcing the corona from the photosphere, please don't make statements that go against what is being told to you.
As I said in my very first post those 2 are closely interlinked because of the magnetic fields. I said to you in my first post that the
core wasn't directly linked in the energy transfer action and that comment still stands.
Gfellow said:
Wikipedia is a major referencing tool for millions of people. Disengaging the Core altogether from the Coronal Heating Problem is disturbingly disappointing to say the least.

and in general it is a good reference, but it can have issues, that is why it's VERY WISE to look through the lists of scientific references
at the bottom of any wiki page

It's only a disappointment to you because you refuse to listen and learn
Gfellow said:
But if nobody else is bothered, I'll let the subject drop.
well we are bothered and we are trying to help you, but you seem not to want to listen and learn.
There's nothing I or the other good people here can do about that, it's your loss :frown: Dave
 
  • #16
Drakkith said:
As I've said already, I don't think so. However I'm certainly not an expert in this area, so I'd be interested in hearing from someone who is.

I'm not en expert either and I didn't find any useful information about the generation of Sun's magnetic field. That's why I asked the question. Maybe the answer is unknown. That could at least justifiy excluding the core from the discussion because it would be speculative.
 
  • #17
DrStupid said:
I'm not an expert either and I didn't find any useful information about the generation of Sun's magnetic field. That's why I asked the question. Maybe the answer is unknown. That could at least justify excluding the core from the discussion because it would be speculative.
Globally, the Sun's magnetic field is generated by the dynamo action of the convective layer, so the core isn't directly involved, though it's energy generation is obviously the cause of the convection. Specifically, the knotting of the magnetic fields on the surface that cause sunspots and flares, are due to differential rotation. If you want to delve into the complexity of the processes, peruse the published papers of E.N. Parker.
Gfellow said:
Just seems myopic, ignoring the elephant in the room, a 15 million C solar core, that no one has as yet discovered a venting solution for heat dissipation.
Divorcing the Corona from the Photosphere and the core makes a mockery of the Coronal heating problem - the 2nd law of Thermodynamics - hot, through cold, to hot; it's a cop-out to what should be an intriguing and challenging problem.
Wikipedia is a major referencing tool for millions of people. Disengaging the Core altogether from the Coronal Heating Problem is disturbingly disappointing to say the least.
But if nobody else is bothered, I'll let the subject drop.
While the processes in the solar interior are integral to everything that occurs in the sun's subsequent evolution, the major puzzle is that the corona is hotter than the photosphere. Unless they found a link, either observational or theoretical, between the core and the corona, Wikipedia probably felt it unnecessary to include any mention of the core, not that they're ignoring it's importance but that it's inclusion wouldn't add any further insight into the problem's solution.
 
  • Like
Likes Drakkith, DrStupid and 256bits
  • #18
There is one way the core can transfer heat directly to the corona, via neutrinos. That certainly occurs but is a trivial component of the heating. A more interesting question is whether neutrinos collide with atoms in the upper layers of the sun, and produce muons. These can directly heat the corona, but more interesting is that a sufficient muon flux would create heat by muon-catalyzed fusion. Again has to occur, but the two processes may add a couple of degrees to the corona. (It would take me a month or three to simulate, but it isn't worth the effort.)
 
  • #19
eachus said:
A more interesting question is whether neutrinos collide with atoms in the upper layers of the sun, and produce muons.

They don't.
 
  • Like
Likes davenn

What is the Coronal Heating Problem?

The Coronal Heating Problem refers to the mystery of why the outer atmosphere of the Sun, known as the corona, is significantly hotter than the layers below it. According to traditional models, the temperature of the corona should decrease as you move away from the Sun's surface, but in reality, it is much hotter.

What is the Hydrogen Fusion Core?

The Hydrogen Fusion Core is the central region of the Sun where nuclear fusion reactions take place. These reactions convert hydrogen atoms into helium, releasing large amounts of energy in the process. This energy is what makes the Sun shine and provides heat and light to our planet.

Why does the Hydrogen Fusion Core disappear?

The Hydrogen Fusion Core does not actually disappear, but it becomes less efficient in producing energy. As the core uses up its hydrogen fuel, it begins to shrink and heat up, causing it to become denser. This increased density makes it more difficult for the core to sustain fusion reactions, leading to a decrease in energy production.

How does the disappearance of the Hydrogen Fusion Core relate to the Coronal Heating Problem?

The disappearance of the Hydrogen Fusion Core is believed to be one of the main factors contributing to the Coronal Heating Problem. As the core becomes less efficient, it produces less energy, which in turn leads to a decrease in the amount of energy that reaches the corona. This results in a temperature difference between the corona and the layers below it.

What are some proposed explanations for the Coronal Heating Problem?

Scientists have proposed several theories to explain the Coronal Heating Problem, including magnetic waves, nanoflares, and turbulence. These theories suggest that various mechanisms may be at play, such as the conversion of magnetic energy into heat or the release of small bursts of energy called nanoflares. However, the exact cause of the Coronal Heating Problem is still a subject of ongoing research and debate.

Similar threads

  • High Energy, Nuclear, Particle Physics
Replies
13
Views
2K
Replies
6
Views
3K
  • High Energy, Nuclear, Particle Physics
Replies
19
Views
3K
Replies
8
Views
3K
  • Astronomy and Astrophysics
Replies
2
Views
4K
  • Sci-Fi Writing and World Building
Replies
21
Views
1K
  • Cosmology
Replies
4
Views
1K
  • Beyond the Standard Models
Replies
30
Views
7K
  • Introductory Physics Homework Help
Replies
1
Views
4K
Replies
14
Views
8K
Back
Top