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WMAP polarization data has had the odd characteristic of being aligned with the geometry of the solar system. If the CMB is purely cosmological, which is expected, the meaning of this continues to be unexpected and wanting for a reasonable correction or explanation. The authors try 4 possible sources of error and rule them out. This leaves it up to you, the reader. Surprise!
Note that their improved analysis is not close to the poles, but right over them in figure 1's color diagram.(see page 4 in the link) That's the 9 sigma result. They are suspecting some systematic error which is being overlooked here. SEE:http://arxiv.org/PS_cache/arxiv/pdf/...911.0150v1.pdf
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A third rate theory forbids. A second rate theory explains after the fact. A first rate theory predicts. A. Lomonosov Last edited by trinitree88; 10-November-2009 at 03:07 PM.. Reason: link,typo |
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Why not something like a galactic microwave corona stimiluated by a galactic bipolar flow from a magnetic pole 5.5 deg from the rotational pole?
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A third rate theory forbids. A second rate theory explains after the fact. A first rate theory predicts. A. Lomonosov |
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![]() It is interesting to note that iron is found in the remnant of supernova 1006, a type 1a remnant. SEE:http://adsabs.harvard.edu/abs/2007PThPS.169..150W Winkler. pete There's strong iron in 1a"s, but at least some weak iron in type 2's. see:http://www.solstation.com/x-objects/tycho-s.htm, and we live inside at least one very old type 2, more likely, a cumulative bubble of about six of them from the Centaurus-Sco Association. How the sun's magnetosphere cannot be influencing the polarization of iron needles as we plow through that stuff, and causing what we are seing in the CMB remains a mystery to me. It is clear from the iron-60 in terrestrial marine sediments that we have bathed the solar system at least as deep as Earth's orbit in iron during the last several million years. (Fields) SEE:http://www.space.com/scienceastronom...xtinction.html and SEE:http://arxiv.org/ftp/arxiv/papers/0709/0709.4197.pdf
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A third rate theory forbids. A second rate theory explains after the fact. A first rate theory predicts. A. Lomonosov Last edited by trinitree88; 11-November-2009 at 07:12 PM.. Reason: links typo |
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I hope I remember my freshman astronomy correctly-- but iron is usually found in supernova of larger stars--- not of the IA type-- Type IA is associated with stars of or --around the mass of the our Sun.
One governing prinicple of stars is their mass and therefore: possibly their ultimate fate-- IA types do nott have an iron core at the end of their lifetimes-- whereas our Sun will probably follow suit to a carbon core at the end of its lifecycle -- a type IA... then a black dwarf.. after it cools down. Pure speculation: It is possible that there may be more than one supernova remnant here-- but I am not fully qualified to add authority to that notion. The following link to wikipedia has some fairly basic answers to your question: Type IA N.B. Note to the mods & experts in the forum-- please excuse my oversimplifications. Last edited by jaksichj; 12-November-2009 at 01:17 AM.. Reason: Correction on wording, grammar and spelling |
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The current model for Type Ia supernovae involves a carbon-oxygen white dwarf undergoing complete thermonuclear combustion. That means that the nuclei of the elements in the white dwarf (carbon and oxygen, for the most part) undergo a series of reactions until they reach iron-group nuclei.
Hence, a great deal of the material -- different explosion models predict up to 0.6 or 0.8 solar masses -- in the white dwarf is turned into iron-group elements. You could look it up at ADS .... |
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It has been shown that the kinematics of an expanding remnant can generate microwaves, and that the energetics are order of magnitude from some of the radio data. What would enhance the view is isotopic sediment studies indicating whether a series of nearby supernovae were all type 1a's, all type 2's or a mixture of them , and in which sequence they occurred. That might point more assuredly to a Local component of the CMB that has not been cleared as a "foreground". We are only talking a small percentage of the entire signal causing the polarization effect. You can check out some of my older threads on CMB, Local Bubble, Star of Bethlehem, etc. I won't hijack or link them here. I think I laid a theoretical basis for a physical effect, and the work of Dr. Katherine Kielty on late phase evolution of supernovae indicates they can not only contain iron whiskers, but grains coated in carbon nanotubes. Both radiate pretty blackbody at low temperatures. pete
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Since the result is bipolar, however, could it be that our galaxy is attenuating the microwaves, similar to our atmospheric air mass values increasing and causing greater extinctions as the observing angle increases toward the horizon. The size of the hot spots (fig. 5 of your OP link) and the temp. gradient seems to support this conjecture, or maybe not since I'm over my head in this thing. ![]()
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pghnative. Because iron, being a metal, is a good absorber of radiation when it is colder than the ambient surroundings, and emits pretty blackbody as it cools down in interstellar space when it is warmer than it's surroundings. Eli Dwek, one of the premier dust?ISM experts has shown that the spectra of some remnants are best fit by emission from iron needles. These, in a magnetic field will polar align, giving polarized emission. Dwek has also shown that at temperatures less than ~ 20 Kelvins, the radiation is predominantly in microwave. Eventually this should come to equilibrium at the approximate temperature of space....~2.725 K.
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A third rate theory forbids. A second rate theory explains after the fact. A first rate theory predicts. A. Lomonosov |
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and Ap. J 607:848-854, 2004, June 1....sorry can't link, school library computer has blocking software
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Furthermore, he says in the abstract: "However, expelled into the intergalactic medium, their abundance is too low to cause any dimming of cosmological sources, and their length is too short to make them a significant source of submillimeter emission." But I'm not sure if you were implying that they had some connection to the CMB or not, so I apologize if I've made any incorrect assumptions. |
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The 9 sigma result is the non-zero measure of the anisotropy, not its closeness to the poles of the ecliptic. (g = 0.29 ± 0.031, and 0.29/0.031 is 9.4) From that Figure 1, they don't even look "right over" the poles, I'd estimate a couple degrees off or more. In fact, table 1 seems to say it's over 4 degrees, ± 4. Now that I've had a look at it, I have some more questions, which I can't answer right now. The authors result is a re-work, which incorporates a "previously neglected factor" in the signal covariance matrix. They reference another work, so I'm not doubting them, but it is interesting that a change to the scaling produces a much stronger signal along the axis of the reference system. I'll have to look into it closer. I've seen this sort of thing before. ![]() |
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