Re: [EVGRAY] Re: Magnetic flux annihilation-reconnect phenom

Database ID: 111641
2019-01-10T15:21:30+00:00
Warren Keillor <[email protected]>

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Norman,Alfen waves must require some kind of exotic detection apparatus, as opposed to an oscilloscope, for instance? There is a certain frequency threshold below which, it was normally disregarded, as something in the nature of Johnson Noise.I wonder if there is some kind of transducer to alter the apparent frequency to some more familiar detector?When I was with my biologist friend in Trinidad, he produced a device that made it possible to hear the sounds of earth worms, and bats, not normally audible to the human ear, where you could identify the creatures by the sounds they emitted, in the jungle, at night.Listening to this device, the landscape developed a whole new dimension around you, on every side, as you trecked through it.It simply shifted the frequency ranges, not normally heard, into the human range.I expect many animals perceive sound in a much different manner from humans, with our very limited frequency range.Since we have no detection, it dosen't exist for us, without prosthetic devices of some sort, except as an intellectual concept.Now let's get down to earth.What kind of machine do we need to simply use thus information for energy purposes?Sent from Yahoo Mail on Android 
 
  On Thu, 10 Jan 2019 at 8:22 AM, Norman Wootan [email protected] [EVGRAY]<[email protected]> wrote:       
 

Moray, Jon Gentry and Warren asked pertinent questions regarding velocities, magnetic flux etc. in plasma events so I did a search as to whether Alfven waves have a frequency.  This site pretty well defines a lot of plasma info that we need.   See:  https://www.britannica.com/science/plasma-state-of-matter#ref507092
 
 On 1/10/2019 6:29 AM, Warren Keillor [email protected] [EVGRAY] wrote:
  
     Norman Hooper's work looks very compelling. At his time of experimentation, super conductors were not a reality as they are now. The fact that a resistance free conductor might accelerate  a potential's velocity, after going through a resistor, suggests an analogy to fluid dynamics, much like Bernuili's principle application of a venturi to gases. The idea of dielectric conductors is a mind smasher, inverting our entire circuit thoughts. Generally, pretty radical concepts, in a zone to set us up for quantum physics thinking. Whew! Cheers Warren
 
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   On Wed, 9 Jan 2019 at 3:17 PM, Norman Wootan [email protected] [EVGRAY] <[email protected]> wrote:          
 
 
Good question Warren!   Nobody really knows how the potential and current manifest in the conductor passing through a flux field. Your question is valid cause there very well may be some sort of reconnect  occurring here. Theory was, that the flux field was photon stream which enabled pairing to produce electrons and attending current.  There is still so much that we don't know but things are getting interesting.   Read that last doc that I posted for it is very enlightening on this subject.  See:  http://www.tfcbooks.com/mall/more/temp/x565-hen.htm   This is one of Oles  favorites.
 
  On 1/9/2019 9:09 AM, Warren Keillor [email protected] [EVGRAY] wrote:
  
    
Norman
 I wonder if, in a down to earth , practical manner, the connect/re-connect plays a role in, for instance, the Kromery, where one slides the  magnets at right angles to their locked together state. Initially, I need both hands to grasp the flywheel to turn my Kromery. Once turning, one finger's friction on the rim, easily rotates the flywheel, regardless of the load.
 Too fast, then eddy currents start warming the magnetic coil cores. Are we cutting those magnetic lines? Cheers Warren
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  On Wed, 9 Jan 2019 at 9:25 AM, Norman Wootan [email protected] [EVGRAY] <[email protected]> wrote:          
 
 
http://young.caltech.edu/Collisionless_Magnetic_Reconnection.html
 
  On 1/9/2019 8:21 AM, Norman Wootan wrote:
  
 
https://phys.org/news/2017-10-hidden-mechanics-magnetic-field-reconnection.html
 
 On 1/9/2019 8:14 AM, Norman Wootan wrote:
  
 
https://gss.pppl.gov/talks/reconnection%20lecture%201.pdf
 
 On 1/9/2019 8:09 AM, Norman Wootan wrote:
  
 
 
                         
 https://link.springer.com/chapter/10.1007%2F978-94-009-0545-0_14
 

 
 

 

 
 

 
           Recent  Developments  in  the  Theory  of  Magnetic  Reconnection  Dieter  Biskamp  Max-Planck-Institut  fiir  Plasmaphysik  8046  Garching  bei  Miinchen,  Federal  Republic  of  Germany  Abstract  The  talk  briefly  reviews  previous  stationary  models,  mainly  configurations  of  the  Petschek  type,  pointing  out  their  shortcomings  and  basic  failure  in  accounting  for  fast  magnetic  reconnection  in  the  limit  of  large  magnetic  Reynolds  number.  It  is  shown  that  in  this  limit  no  relevant  stationary  states  exist.  Instead  strong  small-scale  MHD  turbulence  develops  even  in  2D  geometry,  giving  rise  to  energy  dissipation  and  reconnection  rates  independent  of  the  value  of  the  collisional  re- sistivity.  I  Introduction  In  the  last  decade  it  has  been realized  that  the  presence  of  magnetic  fields  is  a  ubiquitous  phenomenon  in  cosmic  systems.  On  the  one  hand,  magnetic  fields  serve  as  a large  energy  reservoir  which  may  be  tapped  in  a fast  dynamic  process  leading  to  various  kinds  of  explosive  events  such  as  flares.  On  the  other  hand,  magnetic  fields  tend  to  be  compressed  in  processes  such  as  protostar  formation  and  are  computed  to  dominate  the  dynamics  in  the  later  phases  in  a nonrealistic  way  if  not  dissipated  sufficiently  fast.  To  account  for  such  processes of  fast  magnetic  field  annihilation  is  the  main  objective  of  the  theory  of  magnetic  reconnect  ion.  The  term  magnetic  reconnect  ion  refers  to  the  picture  of  magnetic  field  lines.  These  have  a well-defined  meaning  in  a highly  conducting  fluid,  viz.  thin  magnetic  flux  tubes  which  are  carried  along  with  the  fluid,  maintaining  their  individuality,  though  they  may  be  wound  in  a very  complex  manner.  Only  owing  to  finite  electrical  resistivity  or  some  equivalent  process  may  two  field  lines  coming  close  together  lose  their  identities  by  being  cut  and  reconnected  in  a different  way.  Though  this  is  a local  process,  it  leads  to  a change  of  field  topology  permitting  new  types  of  large-scale  plasma  motions  that  would  otherwise  be  inhibited.  The  255  w.  BrinbMnn  et  al.  (eds.J,  Physical  Processes  in  Hot  Cosmic  PlIlsmas,  255-269.  e  1990  Kluwer  Academic  Publishers.  256  change  of  the  magnetic  field  is described  by  Faraday's  law:  oB  (  ...  )  2'"  7it=VX  iixB  +  'IV  B.  (1)  Here  the  ratio  of  the  diffusion  term  and  the  convection  term  (2)  is  a convenient  dimensionless  measure  of  the  resistivity,  Rm  being  the  magnetic  Reynolds  number.  In  practically  all  astrophysical  plasmas  Rm  is large,  essentially  because  of  the  large  scales  L.  Hence  magnetic  diffusion  is  in  general  a very  weak  process.  Magnetic  processes  such  as  solar  flares,  however,  seem  to  require  fast  reconnection  with  time  scales  practically  independent  of  Rm.  The  main  theoretical  problem  therefore  is  to  find  models  allowing  sufficiently  high  reconnect  ion  rates.  Fast  reconnection  is  not  a diffuse  process,  but  is  strongly  localized  in  current  sheets.  Such  current  sheets  may  arise  at  any  point  with  non-vanishing  magnetic  shear  and  a velocity  gradient  along  the  direction  of  the  shear  perpendicular  to  the  field,  i.e.  virtually  everywhere  in  the  plasma,  as  visualized  in  Fig.  1.  The  simplest  models  are  quasi-stationary  configurations  with  one  current  sheet  at  a well  defined  location  determined  by  the  overall  geometry,  which  have  been  investigated  in  the  conventional  theory  of  magnetic  reconnection.  The  basic  assumption  in  these  theoretical  approaches is  the  existence  of  atwo-dimensional  subsystem  around  an  X-type  magnetic  neutral  point  which  is  small  compared  with  the  global  magnetic  configuration  but  large  compared  with  the  so-called  diffusion  region  around  the  neutral  point,  where  the  diffusion  term  in  (1)  is  important.  In  this  subsystem  conditions  would  rapidly  adjust  to  changes  in  the  global  configuration,  so  that  the  evolution  of  the  latter  would  correspond  to  a sequence  of  stationary  states  in  the  former  which  are  steady-state  solutions  with  the  boundary  conditions  determined  by  the  global  system.  This  is  the  idea  of  stationary  forced  reconnection.  The  prototype  of  such  configurations  is Petschek's  reconnection  model  1),  which  is given  schematically  in  Fig.  2.  In  fact,  much  of  the  theoretical  work  on  magnetic  reconnection 2 ),3)  consists  of  modifications  and  refinements  of  this  model.  The  theory  is based  on  the  effect  that  the  motion  of  a plasma  may  be  supersonic  at  arbitrarily  low  speed  with  respect  to  the  slow  mode . Hence,  by  analogy  with  a system  of  two  supersonic  gas  jets      
 
 
        
   
         
     
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