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#21
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One final point on CMBR
On Jul 6, 4:42 pm, (Phillip Helbig---
remove CLOTHES to reply) wrote: In article , Chalky writes: One final point on this subject: ^^^^^ ??? George Dishman pointed out some time ago that all radio telescopes radiate heat to the night sky, until thermal equilibrium is reached. Everything radiates heat to everything, until thermal equilibrium is reached (in which case it still radiates, but absorbs just as much). Ergo, a microwave dish capable of detecting black body radiation at 2.7 K, is also a 2.7 K black body radiator, whose own radiation is in thermal equilibrium with its own matter. The conclusion doesn't follow from the premises. Assume I have something which is COLDER than the surroundings. It can absorb heat, but is not in thermal equilibrium. Radio dishes are NOT colder than the night sky. Voluminous information supplied by NASA and others, via George Dishman and moderator, under "Ranging & Pioneer" and "Still Lower Noise Radio Astronomy" Therefore, we cannot say with any certainty where, and, more importantly, when, the observed CMB came from. Are you seriously suggesting this? Yes There are four interesting things about the CMB. First, there is a strong dipole, which is consistent with our motion relative to the bulk of the unuiverse. Please amplify on this Second, when the dipole is removed, one is left with a very exact black-body spectrum. This follows precisely from the relativistic principles of isotropy and homogeneity. You seem to be arguing from my corner here. Third, the signal is the same from every direction. Ditto. See above. Note, however, anisotropy in the galactic plane. Fourth, at a very low level, there are inhomogeneities consistent with theoretical predictions. Also consistent with temperature fluctuations consistent with galactic clumping. What is your point? Any alternative model would have to explain ALL four points without any ad-hoc hypotheses. I have made no ad hoc hypothesis. Please amplify on dipole objection. |
#22
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One final point on CMBR
In article , Chalky
writes: Ergo, a microwave dish capable of detecting black body radiation at 2.7 K, is also a 2.7 K black body radiator, whose own radiation is in thermal equilibrium with its own matter. The conclusion doesn't follow from the premises. Assume I have something which is COLDER than the surroundings. It can absorb heat, but is not in thermal equilibrium. Radio dishes are NOT colder than the night sky. Voluminous information supplied by NASA and others, via George Dishman and moderator, under "Ranging & Pioneer" and "Still Lower Noise Radio Astronomy" That's not what I was implying. You seem to think that if it can absorb, it is in thermal equuilibrium. I mentioned the example of a cold object as an obvious example of something which is not in thermal eqilibrium but can absorb heat. (Many radiation detectors ARE cooled, of course.) Therefore, we cannot say with any certainty where, and, more importantly, when, the observed CMB came from. Are you seriously suggesting this? Yes Extraordinary claims demand extraordinary evidence. The ball is in your court. There are four interesting things about the CMB. First, there is a strong dipole, which is consistent with our motion relative to the bulk of the unuiverse. Please amplify on this Even before the CMB was measured accurately, we had a rough idea of our own peculiar motion (look up "Great Attractor"). The CMB dipole is in the same direction. Any alternative theory would have to explain this without ad-hoc hypotheses. Second, when the dipole is removed, one is left with a very exact black-body spectrum. This follows precisely from the relativistic principles of isotropy and homogeneity. You seem to be arguing from my corner here. I'm just noting the four important things; you might not disagree with all of them. :-) Third, the signal is the same from every direction. Ditto. See above. Note, however, anisotropy in the galactic plane. That isn't the CMB, but rather the CMF ("F" as in "foreground"). Fourth, at a very low level, there are inhomogeneities consistent with theoretical predictions. Also consistent with temperature fluctuations consistent with galactic clumping. What is your point? No. Take a robust feature, such as the position of the first peak in the spectrum, and name me ANY alternative theory which predicts this. In fact, the shape of the spectrum has been used to rule out various alternative models such as topological defects. (We are talking about the power spectrum here, the amount of variation as a function of angular scale.) Any alternative model would have to explain ALL four points without any ad-hoc hypotheses. I have made no ad hoc hypothesis. I don't mean your original hypothesis, but rather that if it turns out that your hypothesis needs to explain other things, then they should follow in a natural way from your hypothesis, and not be ad-hoc additions. |
#23
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One final point on CMBR
Chalky wrote:
Radio dishes are NOT colder than the night sky. There's no reason they need to be, they are passive reflection devices, and presumably are in rough thermal equilibrium with the local atmosphere, due to conduction, not with the "night sky" due to radiation. What is kept cold is the detector electronics, as you can read about in this school science club tour writeup, with nice photos: http://www.sciencearuba.com/news/2005/topstory21.php "The box containing all the electronic parts is cooled down to 70 Kelvin that is -203 =BA Celsius." And IIUC, that's _still_ much warmer than the equivalent temperature of the CMBR, one of the reasons you need such a big concentrator to make the sky signal dominate the local noise sources.[*] Quantum valeat. xanthian. [*] Besides just that you need that much antenna due to the wavelengths you're studying. |
#24
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One final point on CMBR
"Chalky" wrote in message
... On Jun 28, 8:08 am, Richard Saam wrote: Chalky wrote: So, why wouldn't the thermal radiation from this known expanding cloud of hot transparent gas, after the surface of last scattering, produce, or, at least, contribute to, the observed CMB spectrum? If something re-absorbs that thermal radiation, why does it not simultaneously re-absorb the classically predicted CMBR, which we are taught was only released at this surface of last scattering? Possibly because most of the universe mass/energy at 1+z~1000, T~3000 was 'dark matter/energy' at temperature Td in equilibrium ~T/Td with CMBR at that time just as it is now ~T/Td at 1+z~1, T~3 One final point on this subject: George Dishman pointed out some time ago that all radio telescopes radiate heat to the night sky, until thermal equilibrium is reached. Many respondents, including George, have pointed out that any efficient radiator is also an equally efficient absorber, at the same wavelength. Ergo, a microwave dish capable of detecting black body radiation at 2.7 K, is also a 2.7 K black body radiator, You jumped a step. The electrons in the HEMT transistors reach equilibrium which means the heat being coupled to them as a result of being in a physical piece of silicon is balanced by their radiation to space. That is at an electron temperature of around 20K from memory, not 2.7K. The sensitive detectors are measuring to tiny fractions of a degree so use differential techniques, for example comparing the signal from a block at a known temperature to the antenna signal, and use chopping to so that the difference is AC while the receiver thermal noise which is always present produces DC. Much of the real scientific work in such missions as COBE is related to the instrument design. whose own radiation is in thermal equilibrium with its own matter. Therefore, we cannot say with any certainty where, and, more importantly, when, the observed CMB came from. You cannot be serious. One final point for you. Your original point relates to opacity of the neutral hydrogen gas after recombination. You may already be aware but if not I think you would find it of interest to look the characteristics and cause of the Lyman Alpha "forest". Specifically, why are there gaps between the trees ;-) George |
#25
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One final point on CMBR
On Jul 8, 8:57 pm, (Phillip Helbig---
remove CLOTHES to reply) wrote: In article , Chalky writes: Ergo, a microwave dish capable of detecting black body radiation at 2.7 K, is also a 2.7 K black body radiator, whose own radiation is in thermal equilibrium with its own matter. The conclusion doesn't follow from the premises. Assume I have something which is COLDER than the surroundings. It can absorb heat, but is not in thermal equilibrium. Radio dishes are NOT colder than the night sky. Voluminous information supplied by NASA and others, via George Dishman and moderator, under "Ranging & Pioneer" and "Still Lower Noise Radio Astronomy" That's not what I was implying. You seem to think that if it can absorb, it is in thermal equuilibrium. I mentioned the example of a cold object as an obvious example of something which is not in thermal eqilibrium but can absorb heat. (Many radiation detectors ARE cooled, of course.) Therefore, we cannot say with any certainty where, and, more importantly, when, the observed CMB came from. Are you seriously suggesting this? Yes Extraordinary claims demand extraordinary evidence. The ball is in your court. There are four interesting things about the CMB. First, there is a strong dipole, which is consistent with our motion relative to the bulk of the unuiverse. Please amplify on this Even before the CMB was measured accurately, we had a rough idea of our own peculiar motion (look up "Great Attractor"). The CMB dipole is in the same direction. I was asking you to amplify on what is meant by CMB dipole Any alternative theory would have to explain this without ad-hoc hypotheses. Second, when the dipole is removed, one is left with a very exact black-body spectrum. This follows precisely from the relativistic principles of isotropy and homogeneity. You seem to be arguing from my corner here. I'm just noting the four important things; you might not disagree with all of them. :-) OK, so we are agreed that point 2 is not a valid objection. first point to me. Third, the signal is the same from every direction. Ditto. See above. Note, however, anisotropy in the galactic plane. That isn't the CMB, but rather the CMF ("F" as in "foreground"). So what? Second point to me, I make it. Fourth, at a very low level, there are inhomogeneities consistent with theoretical predictions. Also consistent with temperature fluctuations consistent with galactic clumping. What is your point? No. Take a robust feature, such as the position of the first peak in the spectrum, I don't know what you are talking about here. Please give us a hyperlink to the pertinent graph. and name me ANY alternative theory which predicts this. In fact, the shape of the spectrum has been used to rule out various alternative models such as topological defects. (We are talking about the power spectrum here, the amount of variation as a function of angular scale.) Any alternative model would have to explain ALL four points without any ad-hoc hypotheses. I have made no ad hoc hypothesis. I don't mean your original hypothesis, but rather that if it turns out that your hypothesis needs to explain other things, then they should follow in a natural way from your hypothesis, and not be ad-hoc additions. I am in complete agreement with you there. Show me my ad hoc assumptions, and I will show you yours. C |
#26
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One final point on CMBR
On Jul 8, 9:00 pm, Kent Paul Dolan wrote:
Chalky wrote: Radio dishes are NOT colder than the night sky. There's no reason they need to be, they are passive reflection devices I was expecting the expert (DishMan) to pick up on this. I am, of course, really talking about the radio telescope, i.e. dish + antenna. , and presumably are in rough thermal equilibrium with the local atmosphere, due to conduction, not with the "night sky" due to radiation. The 'local atmosphere' of the Wilkinson Microwave Anisotropy Probe being? C |
#27
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One final point on CMBR
In article , Chalky
writes: There are four interesting things about the CMB. First, there is a strong dipole, which is consistent with our motion relative to the bulk of the unuiverse. Please amplify on this Even before the CMB was measured accurately, we had a rough idea of our own peculiar motion (look up "Great Attractor"). The CMB dipole is in the same direction. I was asking you to amplify on what is meant by CMB dipole The temperature is increased in one direction and decreased in the other. It is increased in the direction in which we are moving, which was known (but not so precisely) before the detection of the CMB dipole. No. Take a robust feature, such as the position of the first peak in the spectrum, I don't know what you are talking about here. Please give us a hyperlink to the pertinent graph. Seriously, if you are discususing the CMB and don't IMMEDIATELY know what "the position of the first peak in the spectrum" is, then you need to do some serious background research. Googling for "+CMB +peak +spectrum" gives 239 thousand hits. Take it from there. Check out http://relativity.livingreviews.org/...age=fig21.html which I got from http://relativity.livingreviews.org/...ge=node20.html which is one of the hits on the first page. We are talking about the obvious big peak near an l value of 300. (Note: this figure is 10 years old; there are MUCH more precise measurements available now.) |
#28
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One final point on CMBR
On Jul 9, 4:42 pm, (Phillip Helbig---
remove CLOTHES to reply) wrote: In article , Chalky writes: There are four interesting things about the CMB. First, there is a strong dipole, which is consistent with our motion relative to the bulk of the unuiverse. Please amplify on this Even before the CMB was measured accurately, we had a rough idea of our own peculiar motion (look up "Great Attractor"). The CMB dipole is in the same direction. I was asking you to amplify on what is meant by CMB dipole The temperature is increased in one direction and decreased in the other. I thought so! In that case, this objection, too, is groundless, and without foundation. Prediction of the CMB dipole thus follows naturally from the known fact that c = constant, and the known fact that thermal and optical radiation are both electromagnetic. When WMAP points in a given direction, it achieves thermal equilibrium with the night sky in that direction. Since this temperature information is communicated electromagnetically, it is obvious that the temperature measured by WMAP is Doppler shifted by our own peculiar motion. To conclude otherwise, you must introduce the additional ad-hoc hypothesis that thermal radiation is not electromagnetic. As I have already also posted under the other title, "Dark Matter (& Mass) of Milky Way": show me my ad hoc assumptions, and I will show you yours. Point 4 to me, too, I think. It is increased in the direction in which we are moving, which was known (but not so precisely) before the detection of the CMB dipole. Chalky |
#29
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One final point on CMBR
On Jul 9, 4:42 pm, (Phillip Helbig---
remove CLOTHES to reply) wrote: In article , Chalky writes: There are four interesting things about the CMB. First, there is a strong dipole, which is consistent with our motion relative to the bulk of the unuiverse. Please amplify on this Even before the CMB was measured accurately, we had a rough idea of our own peculiar motion (look up "Great Attractor"). The CMB dipole is in the same direction. I was asking you to amplify on what is meant by CMB dipole The temperature is increased in one direction and decreased in the other. It is increased in the direction in which we are moving, which was known (but not so precisely) before the detection of the CMB dipole. No. Take a robust feature, such as the position of the first peak in the spectrum, I don't know what you are talking about here. Please give us a hyperlink to the pertinent graph. Seriously, if you are discususing the CMB and don't IMMEDIATELY know what "the position of the first peak in the spectrum" is, then you need to do some serious background research. Googling for "+CMB +peak +spectrum" gives 239 thousand hits. Take it from there. You are the one who raised this 5th objection. If you are not prepared to disclose what the objection actually is, I do not have the spare time to wade through 239 thousand references in order to divine what it might be. Check out http://relativity.livingreviews.org/...-11&page=fig21... I have. I do not understand why this is inconsistent with the predicted black body spectrum radiated (in accordance with Planck's solution of the Ultraviolet Catastrophe) from a night sky with a temperature of ~ 2.7K Please explain. C |
#30
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One final point on CMBR
On 9 Jul, 09:54, Chalky wrote:
On Jul 8, 9:00 pm, Kent Paul Dolan wrote: Chalky wrote: Radio dishes are NOT colder than the night sky. There's no reason they need to be, they are passive reflection devices I was expecting the expert (DishMan) to pick up on this. I am, of course, really talking about the radio telescope, i.e. dish + antenna. I thought Kent had covered it but I suppose it goes back to the previous discussion about the link between transparency and emission. The same argument applies to the dish, a perfect reflector doesn't absorb any of the incident light, and if it doesn't absorb, it cannot emit either. George |
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