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DOOM BREAK!! Attention GLP!!! MSM: Hidden Magnetic Universe Begins to Come Into View! get in here! bring popcorn! :-)

 
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DOOM BREAK!! Attention GLP!!! MSM: Hidden Magnetic Universe Begins to Come Into View! get in here! bring popcorn! :-)
Anytime astronomers figure out a new way of looking for magnetic fields in ever more remote regions of the cosmos, inexplicably, they find them.

These force fields — the same entities that emanate from fridge magnets — surround Earth, the sun and all galaxies. Twenty years ago, astronomers started to detect magnetism permeating entire galaxy clusters, including the space between one galaxy and the next. Invisible field lines swoop through intergalactic space like the grooves of a fingerprint.

Last year, astronomers finally managed to examine a far sparser region of space — the expanse between galaxy clusters. There, they discovered the largest magnetic field yet: 10 million light-years of magnetized space spanning the entire length of this “filament” of the cosmic web. A second magnetized filament has already been spotted elsewhere in the cosmos by means of the same techniques. “We are just looking at the tip of the iceberg, probably,” said Federica Govoni of the National Institute for Astrophysics in Cagliari, Italy, who led the first detection.

The question is: Where did these enormous magnetic fields come from?

“It clearly cannot be related to the activity of single galaxies or single explosions or, I don’t know, winds from supernovae,” said Franco Vazza, an astrophysicist at the University of Bologna who makes state-of-the-art computer simulations of cosmic magnetic fields. “This goes much beyond that.”

One possibility is that cosmic magnetism is primordial, tracing all the way back to the birth of the universe. In that case, weak magnetism should exist everywhere, even in the “voids” of the cosmic web — the very darkest, emptiest regions of the universe. The omnipresent magnetism would have seeded the stronger fields that blossomed in galaxies and clusters.



[link to www.quantamagazine.org (secure)]


-------------------------

JULY 6, 2020!!!!

by European Space Agency!!!


A collection of intriguing images based on data from ESA's Herschel and Planck space telescopes show the influence of magnetic fields on the clouds of gas and dust where stars are forming.


The images are part of a study by astronomer Juan D. Soler of the Max Planck Institute for Astronomy in Heidelberg, Germany, who used data gathered during Planck's all-sky observations and Herschel's 'Gould Belt Survey'. Both Herschel and Planck were instrumental in exploring the cool Universe, and shed light on the many complexities of the interstellar medium – the mix of gas and dust that fills the space between the stars in a galaxy. Both telescopes ended their operational lifetime in 2013, but new discoveries continue to be made from their treasure trove of data.

Herschel revealed in unprecedented detail the filaments of dense material in molecular clouds across our Milky Way galaxy, and their key role in the process of star formation. Filaments can fragment into clumps which eventually collapse into stars. The results from Herschel show a close link between filament structure and the presence of dense clumps.

Herschel observed the sky in far-infrared and sub-millimetre wavelengths, and the data is seen in these images as a mixture of different colours, with light emitted by interstellar dust grains mixed within the gas. The texture of faint grey bands stretching across the images like a drapery pattern, is based on Planck's measurements of the direction of the polarised light emitted by the dust and show the orientation of the magnetic field.




[link to phys.org (secure)]

Last Edited by Digital mix guy Spock on 07/07/2020 10:15 AM
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Re: DOOM BREAK!! Attention GLP!!! MSM: Hidden Magnetic Universe Begins to Come Into View! get in here! bring popcorn! :-)
SUMMARY: We observed a ridge of radio emission connecting the merging galaxy clusters Abell 0399 and Abell 0401 with the Low-Frequency Array (LOFAR) telescope network at 140 megahertz. This emission requires a population of relativistic electrons and a magnetic field located in a filament between the two galaxy clusters. We performed simulations to show that a volume-filling distribution of weak shocks may reaccelerate a preexisting population of relativistic particles, producing emission at radio wavelengths that illuminates the magnetic ridge.


[link to science.sciencemag.org (secure)]

EXCERPT:

Galaxy clusters form at the intersections of the cosmic web filaments and grow by accreting substructures in a merging process, which converts most of the infall kinetic energy into thermal gas energy. A residual fraction of nonthermalized energy is expected to manifest itself in the form of turbulent gas motions, magnetic fields, and relativistic particles. Extended radio sources called radio halos and radio relics are found at the center and the periphery of galaxy clusters, respectively, visible through their emission of synchrotron radiation. Magnetic fields and relativistic particles in the large-scale structure of the Universe can be inferred from observations of these sources.

Observations show that magnetic fields are ubiquitous in galaxy clusters (1), whereas radio halos and relics are most common in merging clusters, suggesting that cluster mergers provide the acceleration of relativistic particles necessary for synchrotron emission (2). Collisions between nearly equal-mass clusters dissipate large amounts of energy within a few billion years. The merging galaxy clusters Abell 0399 and Abell 0401 are separated by a projected distance of 3 megaparsec (Mpc) and host a double radio halo (3). The presence of radio halos at the centers of both Abell 0399 and Abell 0401 was unexpected because radio halos are not common sources, and x-ray (4–7) and optical data (8) suggest that the two systems are still in the initial phase of a merger, before the bulk of kinetic energy of the collision has been dissipated. X-ray data show a hot (temperature T ≃ 6 to 7 keV) and nearly isothermal filament of plasma in the region between the two clusters (7).

There may be a weak shock (Mach number M < 2) in the outer part of the filament, at ~650 to 810 kiloparsec (kpc) from the collision axis (equivalent to an angular offset of 8 to 10 arc min). Observations with the Planck spacecraft (9, 10) detected a signal due to the Sunyaev–Zeldovich (SZ) effect, revealing a large-scale filament of gas connecting the two systems. The SZ effect is a spectral distortion caused by inverse Compton scattering of the cosmic microwave background radiation by hot electrons (T &#8764;keV), which is sensitive to the total thermal energy of the intervening medium.

We observed the region between Abell 0399 and Abell 0401 at radio wavelengths to investigate whether relativistic particles and magnetic fields exist on cosmic scales larger than those of galaxy clusters. Using the Low Frequency Array (LOFAR) telescope network at a central frequency &#957; = 140 MHz (corresponding to a wavelength &#955; = 2.14 m), we detected a filament of diffuse synchrotron emission connecting the two galaxy clusters.
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Re: DOOM BREAK!! Attention GLP!!! MSM: Hidden Magnetic Universe Begins to Come Into View! get in here! bring popcorn! :-)
Begin scanning!!


trek bridge

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Re: DOOM BREAK!! Attention GLP!!! MSM: Hidden Magnetic Universe Begins to Come Into View! get in here! bring popcorn! :-)
The beautiful mess in Abell 2255!!!!

29 June 2020


[link to www.physik.uni-hamburg.de (secure)]


An international team of astrophysicists led by Andrea Botteon from Leiden University, the Netherlands, has shed light on one of the most intricate objects of the radio sky: the galaxy cluster Abell 2255. Thanks to the incredible detailed images obtained with the European radio telescope LOFAR, the scientists have been able to observe details never seen before of the emission from the cluster. The halo in Abell 2255 is not smooth, but contains numerous filaments that have not been seen previously. The result has been presented today at the virtual annual meeting of the European Astronomical Society (EAS) and will be published in The Astrophysical Journal.

The observations carried out with the LOFAR radio telescope are changing the picture that astrophysicists had on galaxy clusters. Despite their name, clusters are not only composed by hundreds of galaxies spread over millions of light years that are bound together by gravity, but also contain particles moving at speeds close to the speed of light that are able to emit radiation in the radio band, when they interact with the cluster magnetic field. These radio emissions, that extend from cluster centers for millions of light years and are produced when two clusters of galaxies collide, have been called radio halos due to their generally spherical and smooth appearance.

The halo in Abell 2255 appears to be anything but smooth, though. First author Botteon: “We discovered the existence of numerous filaments within the halo emission that have not been seen previously. This was possible thanks to LOFAR, which has a sensitivity and angular resolution much higher than the radio telescopes that have observed galaxy clusters in the past, and also because the discovered filaments emit most of their radiation in long radio wavelengths, precisely those detected by the LOFAR antennas.”

Radio halos are still enigmatic sources for astrophysicists. One of the most accepted hypotheses on their origin is that they form due to the turbulent motions generated in the cluster gas, triggered when two clusters collide. In this framework, the new observations could provide valuable insights on radio halos.
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Re: DOOM BREAK!! Attention GLP!!! MSM: Hidden Magnetic Universe Begins to Come Into View! get in here! bring popcorn! :-)
:)

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Re: DOOM BREAK!! Attention GLP!!! MSM: Hidden Magnetic Universe Begins to Come Into View! get in here! bring popcorn! :-)
SCIENCE JOURNAL ARTICLE!!



Submission history
From: Andrea Botteon
[v1] Mon, 8 Jun 2020

We present LOFAR observations of one of the most spectacular objects in the radio sky: Abell 2255. This is a nearby (z=0.0806) merging galaxy cluster hosting one of the first radio halos ever detected in the intra-cluster medium (ICM). The deep LOFAR images at 144 MHz of the central &#8764;10 Mpc2 region show a plethora of emission on different scales, from tens of kpc to above Mpc sizes. In this work, we focus on the innermost region of the cluster. Among the numerous interesting features observed, we discover remarkable bright and filamentary structures embedded in the radio halo. We incorporate archival WSRT 1.2 GHz data to study the spectral properties of the diffuse synchrotron emission and find a very complex spectral index distribution in the halo spanning a wide range of values.

We combine the radio data with Chandra observations to investigate the connection between the thermal and non-thermal components by quantitatively comparing the radio and X-ray surface brightness and the spectral index of the radio emission with the thermodynamical quantities of the ICM. Despite the multitude of structures observed in the radio halo, we find that the X-ray and radio emission are overall well correlated. The fact that the steepest spectrum emission is located in the cluster center and traces regions with high entropy possibly suggests the presence of seed particles injected by radio galaxies that are spread in the ICM by turbulence generating the extended radio halo.
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Re: DOOM BREAK!! Attention GLP!!! MSM: Hidden Magnetic Universe Begins to Come Into View! get in here! bring popcorn! :-)
:)

bump
 Quoting: Angels 77948266


thanks, friend!!! GLP rocks!!

GLP
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Re: DOOM BREAK!! Attention GLP!!! MSM: Hidden Magnetic Universe Begins to Come Into View! get in here! bring popcorn! :-)
Anytime astronomers figure out a new way of looking for magnetic fields in ever more remote regions of the cosmos, inexplicably, they find them.

These force fields — the same entities that emanate from fridge magnets — surround Earth, the sun and all galaxies. Twenty years ago, astronomers started to detect magnetism permeating entire galaxy clusters, including the space between one galaxy and the next. Invisible field lines swoop through intergalactic space like the grooves of a fingerprint.

Last year, astronomers finally managed to examine a far sparser region of space — the expanse between galaxy clusters. There, they discovered the largest magnetic field yet: 10 million light-years of magnetized space spanning the entire length of this “filament” of the cosmic web. A second magnetized filament has already been spotted elsewhere in the cosmos by means of the same techniques. “We are just looking at the tip of the iceberg, probably,” said Federica Govoni of the National Institute for Astrophysics in Cagliari, Italy, who led the first detection.

The question is: Where did these enormous magnetic fields come from?

“It clearly cannot be related to the activity of single galaxies or single explosions or, I don’t know, winds from supernovae,” said Franco Vazza, an astrophysicist at the University of Bologna who makes state-of-the-art computer simulations of cosmic magnetic fields. “This goes much beyond that.”

One possibility is that cosmic magnetism is primordial, tracing all the way back to the birth of the universe. In that case, weak magnetism should exist everywhere, even in the “voids” of the cosmic web — the very darkest, emptiest regions of the universe. The omnipresent magnetism would have seeded the stronger fields that blossomed in galaxies and clusters.



[link to www.quantamagazine.org (secure)]
 Quoting: Digital mix guy


its about time they aknowledge the truth.

gravity..pfffffh
Digital mix guy  (OP)

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Re: DOOM BREAK!! Attention GLP!!! MSM: Hidden Magnetic Universe Begins to Come Into View! get in here! bring popcorn! :-)
Additional link!!! this article seems to be the same as the one posted above; however, this website is highly reputable.


[link to phys.org (secure)]
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Re: DOOM BREAK!! Attention GLP!!! MSM: Hidden Magnetic Universe Begins to Come Into View! get in here! bring popcorn! :-)
In a new data set on the cluster Abell 2255, a team led by Andrea Botteon captures all these effects in stunning detail using the LOFAR radio telescope. According to team member Gianfranco Brunetti: The filaments discovered by LOFAR could form exactly as a consequence of these turbulent motions. Another possibility that we are considering is that the filaments originate from the interaction between the galaxies, which move at speeds of many hundreds of km/s inside the cluster and the plasma that produces the radio emission of the halo.

The degree of emissions from shockwaves is something that had been somewhat anticipated, but this is the first study to look at how far the radio emissions extend from this cluster. According to team member Reinout van Weeren: One of the goals is to understand if the radio emission extends also beyond Abell 2255, tracing the gigantic cosmic web that connects clusters of galaxies in the Universe.




[link to cosmoquest.org (secure)]
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Re: DOOM BREAK!! Attention GLP!!! MSM: Hidden Magnetic Universe Begins to Come Into View! get in here! bring popcorn! :-)
this is from 2003!!! seems highly interesting though!!


Chandra Observations of Point Sources in Abell 2255
David S. Davis’l2
Neal A. Miller3
and
Richard F. Mushotzky4
ABSTRACT

In our search for “hidden” AGN we present results from a Chandra observation of the nearby cluster Abell 2255. Eight cluster galaxies are associated with
point-like X-ray emission, and we classify these galaxies based on their X-ray,
radio, and optical properties. At least three are associated with active galactic
nuclei (AGN) with no optical signatures of nuclear activity, with a further two
being potential AGN. Of the potential AGN, one corresponds to a galaxy with
a post-starburst optical spectrum. The remaining three X-ray detected cluster
galaxies consist of two starbursts and an elliptical with luminous hot gas.

Of the
eight cluster galaxies five are associated with luminous (massive) galaxies and the
remaining three lie in much lower luminosity systems. We note that the use of
X-ray to optical flux ratios for classification of X-ray sources is often misleading,
and strengthen the claim that the fraction of cluster galaxies hosting an AGN
based on optical data is signficantly lower than the fraction based on X-ray and
radio data.


[link to ntrs.nasa.gov (secure)]
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Re: DOOM BREAK!! Attention GLP!!! MSM: Hidden Magnetic Universe Begins to Come Into View! get in here! bring popcorn! :-)
JULY 6, 2020!!!!

by European Space Agency!!!


A collection of intriguing images based on data from ESA's Herschel and Planck space telescopes show the influence of magnetic fields on the clouds of gas and dust where stars are forming.


The images are part of a study by astronomer Juan D. Soler of the Max Planck Institute for Astronomy in Heidelberg, Germany, who used data gathered during Planck's all-sky observations and Herschel's 'Gould Belt Survey'. Both Herschel and Planck were instrumental in exploring the cool Universe, and shed light on the many complexities of the interstellar medium – the mix of gas and dust that fills the space between the stars in a galaxy. Both telescopes ended their operational lifetime in 2013, but new discoveries continue to be made from their treasure trove of data.

Herschel revealed in unprecedented detail the filaments of dense material in molecular clouds across our Milky Way galaxy, and their key role in the process of star formation. Filaments can fragment into clumps which eventually collapse into stars. The results from Herschel show a close link between filament structure and the presence of dense clumps.

Herschel observed the sky in far-infrared and sub-millimetre wavelengths, and the data is seen in these images as a mixture of different colours, with light emitted by interstellar dust grains mixed within the gas. The texture of faint grey bands stretching across the images like a drapery pattern, is based on Planck's measurements of the direction of the polarised light emitted by the dust and show the orientation of the magnetic field.




[link to phys.org (secure)]
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As a EU follower you get fivestars
All great truths begin as Blasphemies.
G.B.S.

GLP is like a diamond mine of information, in the sense that you have to shovel mountains of crap to find the diamonds, but it's still worth the pain.
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As a EU follower you get fivestars
 Quoting: Red Hot Chilean Pepe


thanks, friend!! :-)
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As a EU follower you get fivestars
 Quoting: Red Hot Chilean Pepe


thanks, friend!! :-)
 Quoting: Digital mix guy


I have seen ideas that point to the electromagnetic force as the “unified field”. There’s currently a theoretical approach being developed by an informatics PhD that has been able to accurately predict observed values of several essential particle physics properties from the model. This is mind bending stuff, it involves time as a dimension that matter “does not see”, and the author himself reckons researching the model will take decades but it applies to, and works fine, for condensed matter, something classic physics does not even dream about.

This model unifies gravity as a secondary EM effect, thus proving that the Universe is indeed electric, albeit not as simply as one might wish, as all the effects start at the particle scale, but is already there. It will take decades to get the ideas to capture the interest of mainstream, but the seed has already been planted. Problem is that this approach makes all sorts of “impossible” things possible, and you know that a paradigm refusing to die is indeed lethal to whoever challenges it.
All great truths begin as Blasphemies.
G.B.S.

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Re: DOOM BREAK!! Attention GLP!!! MSM: Hidden Magnetic Universe Begins to Come Into View! get in here! bring popcorn! :-)
Thread: The FLUFFY MAGNETIC RIBBON NEMESIS of the PLASMA UNIVERSE
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2012 Nexus Event – Unknown Form of Energy comes our way:
[link to 2012portal.myfeedportal.com]
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magnetic field
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[link to www.plasma-universe.com (secure)]

Plasma Cosmology
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Re: DOOM BREAK!! Attention GLP!!! MSM: Hidden Magnetic Universe Begins to Come Into View! get in here! bring popcorn! :-)
Anytime astronomers figure out a new way of looking for magnetic fields in ever more remote regions of the cosmos, inexplicably, they find them.

These force fields — the same entities that emanate from fridge magnets — surround Earth, the sun and all galaxies. Twenty years ago, astronomers started to detect magnetism permeating entire galaxy clusters, including the space between one galaxy and the next. Invisible field lines swoop through intergalactic space like the grooves of a fingerprint.

Last year, astronomers finally managed to examine a far sparser region of space — the expanse between galaxy clusters. There, they discovered the largest magnetic field yet: 10 million light-years of magnetized space spanning the entire length of this “filament” of the cosmic web. A second magnetized filament has already been spotted elsewhere in the cosmos by means of the same techniques. “We are just looking at the tip of the iceberg, probably,” said Federica Govoni of the National Institute for Astrophysics in Cagliari, Italy, who led the first detection.

The question is: Where did these enormous magnetic fields come from?

“It clearly cannot be related to the activity of single galaxies or single explosions or, I don’t know, winds from supernovae,” said Franco Vazza, an astrophysicist at the University of Bologna who makes state-of-the-art computer simulations of cosmic magnetic fields. “This goes much beyond that.”

One possibility is that cosmic magnetism is primordial, tracing all the way back to the birth of the universe. In that case, weak magnetism should exist everywhere, even in the “voids” of the cosmic web — the very darkest, emptiest regions of the universe. The omnipresent magnetism would have seeded the stronger fields that blossomed in galaxies and clusters.



[link to www.quantamagazine.org (secure)]
 Quoting: Digital mix guy


its about time they acknowledge the truth.

gravity..pfffffh

 Quoting: Anonymous Coward 75449616


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trek bridge
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Re: DOOM BREAK!! Attention GLP!!! MSM: Hidden Magnetic Universe Begins to Come Into View! get in here! bring popcorn! :-)
Anytime astronomers figure out a new way of looking for magnetic fields in ever more remote regions of the cosmos, inexplicably, they find them.

These force fields — the same entities that emanate from fridge magnets — surround Earth, the sun and all galaxies. Twenty years ago, astronomers started to detect magnetism permeating entire galaxy clusters, including the space between one galaxy and the next. Invisible field lines swoop through intergalactic space like the grooves of a fingerprint.

Last year, astronomers finally managed to examine a far sparser region of space — the expanse between galaxy clusters. There, they discovered the largest magnetic field yet: 10 million light-years of magnetized space spanning the entire length of this “filament” of the cosmic web. A second magnetized filament has already been spotted elsewhere in the cosmos by means of the same techniques. “We are just looking at the tip of the iceberg, probably,” said Federica Govoni of the National Institute for Astrophysics in Cagliari, Italy, who led the first detection.

The question is: Where did these enormous magnetic fields come from?

“It clearly cannot be related to the activity of single galaxies or single explosions or, I don’t know, winds from supernovae,” said Franco Vazza, an astrophysicist at the University of Bologna who makes state-of-the-art computer simulations of cosmic magnetic fields. “This goes much beyond that.”

One possibility is that cosmic magnetism is primordial, tracing all the way back to the birth of the universe. In that case, weak magnetism should exist everywhere, even in the “voids” of the cosmic web — the very darkest, emptiest regions of the universe. The omnipresent magnetism would have seeded the stronger fields that blossomed in galaxies and clusters.



[link to www.quantamagazine.org (secure)]


-------------------------

JULY 6, 2020!!!!

by European Space Agency!!!


A collection of intriguing images based on data from ESA's Herschel and Planck space telescopes show the influence of magnetic fields on the clouds of gas and dust where stars are forming.


The images are part of a study by astronomer Juan D. Soler of the Max Planck Institute for Astronomy in Heidelberg, Germany, who used data gathered during Planck's all-sky observations and Herschel's 'Gould Belt Survey'. Both Herschel and Planck were instrumental in exploring the cool Universe, and shed light on the many complexities of the interstellar medium – the mix of gas and dust that fills the space between the stars in a galaxy. Both telescopes ended their operational lifetime in 2013, but new discoveries continue to be made from their treasure trove of data.

Herschel revealed in unprecedented detail the filaments of dense material in molecular clouds across our Milky Way galaxy, and their key role in the process of star formation. Filaments can fragment into clumps which eventually collapse into stars. The results from Herschel show a close link between filament structure and the presence of dense clumps.

Herschel observed the sky in far-infrared and sub-millimetre wavelengths, and the data is seen in these images as a mixture of different colours, with light emitted by interstellar dust grains mixed within the gas. The texture of faint grey bands stretching across the images like a drapery pattern, is based on Planck's measurements of the direction of the polarised light emitted by the dust and show the orientation of the magnetic field.




[link to phys.org (secure)]
 Quoting: Digital mix guy

Have no fear, Spock is here!!! LLAP





GLP