Hydrogen line observation frequency range and space Hydrogen speed?

In summary, the hydrogen line observation frequency range primarily focuses on the 21 cm wavelength, which corresponds to a frequency of approximately 1.42 GHz. This spectral line is crucial for studying interstellar hydrogen and cosmic structures. The speed of hydrogen in space can vary based on local conditions, but it typically moves at significant fractions of the speed of light, influenced by factors such as gravitational fields and thermal energy. Understanding these parameters is essential for astrophysical research and the study of the universe's evolution.
  • #1
Jaaanosik
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TL;DR Summary
What is the relationship between Hydrogen (21cm) line observation frequency range 200MHz to 15MHz and Hydrogen speed in space?
Including the redshift, this line will be observed at frequencies from 200 MHz to about 15 MHz on Earth.
From Hydrogen line in cosmology

Is it possible to calculate Hydrogen speed in the outer space based on the observed frequency range considering the mix of Doppler effect and the gravitational redshift?
 
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  • #3
PeterDonis said:
Speed relative to what?
The Earth, as per the quote from the link, that's where the measurement is being done.
 
  • #4
To expand slightly on Peter's comment, you can always look at a received frequency and say that the wave was stretched x amount by cosmological redshift, compressed y amount by gravitational blueshift, and stretched z amount by kinematic Doppler. Assuming you think you know the emitted frequency then you immediately know the total effect, but the breakdown into the three components largely depends on your choice of what "at rest" means.

Unfortunately "at rest relative to the Earth" doesn't work as a definition because it doesn't define "at rest over there", only "at rest at Earth".
 
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  • #5
Jaaanosik said:
The Earth
Then the answer is that the "speed" of a distant hydrogen gas cloud relative to Earth in an expanding universe is not well-defined.

Note that the "redshift" in your reference is not gravitational redshift, it's cosmological redshift, due to the expansion of the universe.
 
  • #6
If we go with Ibix's naming:
x - cosmological redshift
y - gravitational blueshift
z - kinetic Doppler effect
If we take hydrogen somewhere from our galaxy the same distance from the center of galaxy then wouldn't be z value dominating?
 
  • #7
Jaaanosik said:
If we go with Ibix's naming
Then you are assuming a particular breakdown of the total effect, which is what is actually observed, into three components--but as @Ibix told you, that breakdown depends on your choice of what "at rest" means--and that's not the only thing it depends on. There is no invariant way of making such a breakdown.

Jaaanosik said:
If we take hydrogen somewhere from our galaxy the same distance from the center of galaxy
Then the reference you gave in the OP is irrelevant, since that reference, at least the part that you quoted, is talking about clouds of hydrogen gas at cosmological distances, not in our own galaxy. For hydrogen gas clouds in our own galaxy, the total effect would be very small.
 
  • #8
Jaaanosik said:
If we take hydrogen somewhere from our galaxy the same distance from the center of galaxy then wouldn't be z value dominating?
That would depend on your choice of coordinates. There isn't an absolute answer.

As Peter notes, you don't seem to be interested in the same things you cited in your opening post. Are you interested in gas clouds in our galaxy or ones far out in the universe?
 
  • #9
I am interested in 21cm line because I would like to find out how fast hydrogen atoms fly through the space in relation to the Earth.
Is 200MHz to 15MHz range only related to intergalactic hydrogen?
Do we measure some other frequencies of 21cm line?
Do we observe hydrogen moving for example at >0.5c?
 
  • #10
Jaaanosik said:
I am interested in 21cm line because I would like to find out how fast hydrogen atoms fly through the space in relation to the Earth.
And, as has already been explained to you, there is no invariant answer to that question.

Jaaanosik said:
Is 200MHz to 15MHz range only related to intergalactic hydrogen?
As a simple calculation will show you, the base frequency of the 21 cm hydrogen line is about 1400 MHz. That is the frequency observed in the lab. So 200 MHz is already redshifted by a factor of about 7 (more precisely, ##1 + z = 7##), and 15 MHz is redshifted by a factor of almost 100. So those frequencies are not just for "intergalactic hydrogen", they are for hydrogen that is far enough away to have cosmological redshifts in that range.

Jaaanosik said:
Do we measure some other frequencies of 21cm line?
See above. And I shouldn't have had to tell you what I said above. You should have checked yourself to see what the base frequency of the 21 cm hydrogen line is. Anyone with "I" level knowledge of this subject should be able to do that.

Jaaanosik said:
Do we observe hydrogen moving for example at >0.5c?
You have already been told that there is no invariant answer to your "speed" question. For hydrogen gas clouds close enough that cosmological redshifts are not an issue, such as in our own galaxy, where we can come up with reasonable definitions of "relative speed", no, we don't see relative speeds anywhere even close to that. You should be able to figure that out too by looking up data on the orbital speeds of stars around the center of the galaxy.
 
  • #11
Why do you feel cosmological redshift of hydrogen represents the speed it flies through space ? That's not what the 21 cm line tells you. Cosmological redshift is not Doppler redshift. As others have mentioned the redshift is primarily cosmological and not doppler.
 
  • #12
Mordred said:
Why do you feel cosmological redshift of hydrogen represents the speed it flies through space ? That's not what the 21 cm line tells you. Cosmological redshift is not Doppler redshift. As others have mentioned the redshift is primarily cosmological and not doppler.
Understood, and I knew the 21cm line measurement has multiple factors.
Looking for the Doppler contribution though.
For example, the first part of this paper The Hydrogen 21-cm Line and Its Applications to Radio Astrophysics talks about measurement of the Sun.
The result is ##T_{sun}=3.5\times10^4K.##
What is the hydrogen velocity in the Sun corona?
Using thermal velocity calculator the speed is ~30km/s.
It appears surprisingly low speed.
I am confused though, how did the above mentioned paper measure the galactic speed?
 
  • #13
Local group objects that are gravitstionally bound are not affected by universe expansion for starters.
So in this specific case you do get strictly Doppler redshift. There is some gravitational redshift but likely that is already factored out by knowing the mass of the Earth and sun.

Far away objects outside our gravitationally bound local group you must now use cosmological redshift but you can have a combination of all 3 forms of redshift.

The trick is you must also recognize that recessive velocity due to expansion is not a true ,kinetic motion velocity but a peculiar velocity due to separation distance and expansion
$$ V_{rec}=H_o zd$$
Further calculations are needed for proper distance.
That still does not give the proper velocity for hydrogen you must factor out the cosmological redshift as well as any potential gravitational redshift to get the Dopler shift portion to get the proper velocity.
The cosmological redshift is only useful for determining distance but as mentioned above you need further calculation for proper distance or alternately commoving distance and conformal distance.
 
  • #14
Mordred said:
Local group objects that are gravitstionally bound are not affected by universe expansion for starters.
...
Thanks!
I am curious, if the space is filled with hydrogen and plasma (free electrons and free protons) why they do not recombine at higher velocities and emit 21cm line at higher velocities?
 
  • #15
There is a temperature dependency the spin temperature of the neutral hydrogen must be higher or lower than the blackbody temperature (radiation temperature) at the location and also the gas temperature is involved. Also in late times after recombination you don't have free electrons and protons so the 21 cm line involves other processes such as those occurring in stars as well as star formation in plasma clouds.
 
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  • #17
Mordred said:
Here is an article describing the details on the temperature dependency
https://www.mso.anu.edu.au/~krumholz/teaching/astr8007_s1_2021/notes5.pdf
Thank you, the article helps but it also says this:
1717508027194.png

I do not see any connection to the question why free electrons and free protons do not recombine in space at higher velocities.
 
  • #18
I take it you missed the previous excitation temperature?

as to your question the 21 cm line does nothing to describe recombination of protons and electrons to form hydrogen. That process requires that the temperature required depends on the baryon to photon ratio and the ionization potential of the species and process involved.
see here
https://people.ast.cam.ac.uk/~pettini/Intro Cosmology/Lecture09.pdf
 
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  • #19
Jaaanosik said:
Looking for the Doppler contribution though.
For distant hydrogen clouds that have a significant cosmological redshift, as you have already been told multiple times now, there is no invariant way to separate out a "Doppler contribution".

Jaaanosik said:
measurement of the Sun
Which obviously has no cosmological redshift relative to the Earth.

Jaaanosik said:
What is the hydrogen velocity in the Sun corona?
Using thermal velocity calculator the speed is ~30km/s.
Thermal velocity has nothing to do with Doppler shift, or indeed with any redshift or blueshift at all.

You seem very, very confused.
 
  • #20
Another confusion I see is not recognizing that there is in regards to the 21 cm line you need to look into the difference between neutral hydrogen and ionized hydrogen. Not free protons and electrons to form hydrogen which is a different process
 
  • #21
Mordred said:
neutral hydrogen and ionized hydrogen. Not free protons and electrons to form hydrogen
Um, ionized hydrogen is free protons and electrons. (Or, rarely, free deuterons and electrons.)

The 21-cm line has nothing to do with ionized hydrogen any more than it has to do with free protons and electrons. It is an emission line associated with the electron in a hydrogen atom making a transition between energy levels. The atom can't be ionized because then there would be no electron in the first place: the electron would be free.
 
  • #22
really isn't ionized hydrogen a hydrogen atom that has lost an electron and is now positively charged ?
https://en.wikipedia.org/wiki/Hydrogen_ion

never mind I understand what your stating D'oh too early in the am. Forgot the nucleus only requires a single proton silly me
 
  • #23
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  • #24
Jaaanosik said:
Yes, measurements are in Kelvins, yet somehow it represents Doppler shift.
https://physicsopenlab.org/2020/09/08/measurement-of-the-milky-way-rotation/

30K is 522Hz.
Is this the reason you actually started this thread? Because if so, you could have (and should have) given this particular reference and asked the question you just asked in your OP of the thread. Which would have saved us more than a day of trying to figure out what your actual question is.
 
  • #26
Jaaanosik said:
30K is 522Hz.
Says who? It looks like your "temperature to frequency calculator" is on a different web page that you have not provided a link to. Please provide a link.
 
  • #27
PeterDonis said:
Where on the physicsopenlab page does it say anything about temperature?
1717528762350.png
 
  • #28
PeterDonis said:
Is this the reason you actually started this thread? Because if so, you could have (and should have) given this particular reference and asked the question you just asked in your OP of the thread. Which would have saved us more than a day of trying to figure out what your actual question is.
The reason for the OP is to determine why we do not measure 'fast' hydrogen atoms.
 
  • #29
Jaaanosik said:
The reason for the OP is to determine why we do not measure 'fast' hydrogen atoms.
But until post #23, you did not tell us what "hydrogen atoms" you were even talking about. Not until post #23 did you actually give us a reference that showed specific measurements of particular hydrogen gas clouds--and then they turn out to be hydrogen gas clouds in our own galaxy, whose measured power spectrum, as shown in the "previous post" on physicsopenlab (linked to at the top of the one you referenced), peaks at about 1420 MHz, exactly as expected for the 21 cm hydrogen line with no cosmological redshift. Yet in your OP, you talked about frequencies ranging from 200 MHz down to 15 MHz, which cannot possibly be from the measurements discussed in the physicsopenlab article.
 
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  • #30
Jaaanosik said:
The "Signal" in degrees K in this graph appears to actually represent received power. The "previous post" says "The y axis shows the equivalent temperature of the signal in degrees °K." This temperature itself cannot correspond to a frequency, since frequency is shown on the X axis, as given in the first graph in the "previous post"--and then, as the "previous post" explains, the frequency is converted to velocity by assuming that the "base" frequency is the 1420 MHz expected frequency of the 21 cm hydrogen line, and that all shifts in frequency are due to Doppler shift. So we have a spectrum of received power vs. frequency, which is then used to infer Doppler shifts and hence relative velocities. The articles do not explain how received power is converted into a temperature, which seems to me to be a significant omission; but the "previous post" uses the term "power spectrum" explicitly, indicating that the "signal" is received power.
 
  • #31
Jaaanosik said:
why we do not measure 'fast' hydrogen atoms.
Because the hydrogen atoms being measured are in gas clouds in our own galaxy, whose velocities relative to Earth are not going to be very fast when compared with the speed of light.
 
  • #32
PeterDonis said:
But until post #23, you did not tell us what "hydrogen atoms" you were even talking about. Not until post #23 did you actually give us a reference that showed specific measurements of particular hydrogen gas clouds--and then they turn out to be hydrogen gas clouds in our own galaxy, whose measured power spectrum, as shown in the "previous post" on physicsopenlab (linked to at the top of the one you referenced), peaks at about 1420 MHz, exactly as expected for the 21 cm hydrogen line with no cosmological redshift. Yet in your OP, you talked about frequencies ranging from 200 MHz down to 15 MHz, which cannot possibly be from the measurements discussed in the physicsopenlab article.
My understanding was the measurements in the 200MHz-15MHz as per wiki page include Doppler effect in combination with the other factors.
If that's not the case then I stand corrected.
The title: "Hydrogen line observation frequency range and space Hydrogen speed?
points towards the question trying to resolve the speed of hydrogen in space.
 
  • #33
Jaaanosik said:
the measurements in the 200MHz-15MHz as per wiki page
Have nothing to do with the actual measurements you referenced in post #23.
 
  • #34
Jaaanosik said:
The title: "Hydrogen line observation frequency range and space Hydrogen speed?
points towards the question trying to resolve the speed of hydrogen in space.
And at this point that question has been sufficiently answered, and enough time has been spent on it. Thread closed.
 

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