Carriers and sources of magnetopause current: MMS Case Study
Carriers and sources of magnetopause current: MMS Case Study
 
  We investigate the current carriers and current sources of an ion scale tangential magnetopause current layer using the Magnetospheric Multiscale four spacecraft data. Within this magnetopause current layer, ions and electrons equally contribute to the perpendicular current, while electrons carry nearly all the parallel current. The energy range of all these current carriers is predominantly from middle to high (>100 eV), where particles with higher energies are more efficient in producing the current. By comparing each term, two-fluid magnetohydrodynamic (MHD) theory is able to describe the current sources to a large degree because the sum of all the perpendicular currents from MHD theory could account for the currents observed. In addition, we find that the ion diamagnetic current is the main source of the total perpendicular current, while the curvature current can be neglected. Nevertheless, ions and electrons both carry comparable current due to the redistribution of the electric field and show features beyond the classic Chapman-Ferraro model, particularly on the front side of the boundary layer where the electric field reversal is most intense. We also show a second, comparative event in which ions do not satisfy MHD theory, while the electrons do. The small-scale, adiabatic parameter (square of curvature radius/gyroradius) supports our interpretation that this second event contains ion scale substructure. We suggest that comparing the predicted MHD current with plasma current can be a good method to judge whether the MHD theory is satisfied in each specific circumstance, especially for high-precision Magnetospheric Multiscale data.
Current carriers, Current sources, Magnetopause current, Two-fluid MHD
  
  
  5464-5475
  
    
      Dong, X. C.
      
        061141e9-b73b-43d5-aed8-b97142972657
      
     
  
    
      Dunlop, M. W.
      
        88ebb777-3e0c-43b2-9684-0ef314439ec5
      
     
  
    
      Wang, T. Y.
      
        a15c5a01-2590-4ed1-9f15-289c6a29d15f
      
     
  
    
      Cao, J. B.
      
        4fcb5435-f978-467a-93c4-11ce0d25035f
      
     
  
    
      Trattner, K. J.
      
        16c79a6f-f7b9-4be8-bf69-b64445a72f2c
      
     
  
    
      Bamford, R.
      
        f7b0d205-7772-4720-b5ba-7980b7a000b7
      
     
  
    
      Russell, C. T.
      
        0beb88bf-9d0e-4b75-80ae-61ba3776ce59
      
     
  
    
      Bingham, R.
      
        9f16ac1d-06df-4aac-bf65-aa06c2c2f55a
      
     
  
    
      Strangeway, R. J.
      
        2fd4cc7c-d923-448d-babf-ce95399ed494
      
     
  
    
      Fear, R. C.
      
        8755b9ed-c7dc-4cbb-ac9b-56235a0431ab
      
     
  
    
      Giles, B. L.
      
        eceb7be2-b272-40cb-a9af-82687b2708fd
      
     
  
    
      Torbert, R. B.
      
        dfb49866-d44d-4404-81cd-22cef59d8f03
      
     
  
  
   
  
  
    
    
  
    
    
  
  
    
      Dong, X. C.
      
        061141e9-b73b-43d5-aed8-b97142972657
      
     
  
    
      Dunlop, M. W.
      
        88ebb777-3e0c-43b2-9684-0ef314439ec5
      
     
  
    
      Wang, T. Y.
      
        a15c5a01-2590-4ed1-9f15-289c6a29d15f
      
     
  
    
      Cao, J. B.
      
        4fcb5435-f978-467a-93c4-11ce0d25035f
      
     
  
    
      Trattner, K. J.
      
        16c79a6f-f7b9-4be8-bf69-b64445a72f2c
      
     
  
    
      Bamford, R.
      
        f7b0d205-7772-4720-b5ba-7980b7a000b7
      
     
  
    
      Russell, C. T.
      
        0beb88bf-9d0e-4b75-80ae-61ba3776ce59
      
     
  
    
      Bingham, R.
      
        9f16ac1d-06df-4aac-bf65-aa06c2c2f55a
      
     
  
    
      Strangeway, R. J.
      
        2fd4cc7c-d923-448d-babf-ce95399ed494
      
     
  
    
      Fear, R. C.
      
        8755b9ed-c7dc-4cbb-ac9b-56235a0431ab
      
     
  
    
      Giles, B. L.
      
        eceb7be2-b272-40cb-a9af-82687b2708fd
      
     
  
    
      Torbert, R. B.
      
        dfb49866-d44d-4404-81cd-22cef59d8f03
      
     
  
       
    
 
  
    
      
  
  
  
  
  
  
    Dong, X. C., Dunlop, M. W., Wang, T. Y., Cao, J. B., Trattner, K. J., Bamford, R., Russell, C. T., Bingham, R., Strangeway, R. J., Fear, R. C., Giles, B. L. and Torbert, R. B.
  
  
  
  
   
    (2018)
  
  
    
    Carriers and sources of magnetopause current: MMS Case Study.
  
  
  
  
    Journal of Geophysical Research: Space Physics, 123 (7), .
  
   (doi:10.1029/2018JA025292). 
  
  
   
  
  
  
  
  
   
  
    
      
        
          Abstract
          We investigate the current carriers and current sources of an ion scale tangential magnetopause current layer using the Magnetospheric Multiscale four spacecraft data. Within this magnetopause current layer, ions and electrons equally contribute to the perpendicular current, while electrons carry nearly all the parallel current. The energy range of all these current carriers is predominantly from middle to high (>100 eV), where particles with higher energies are more efficient in producing the current. By comparing each term, two-fluid magnetohydrodynamic (MHD) theory is able to describe the current sources to a large degree because the sum of all the perpendicular currents from MHD theory could account for the currents observed. In addition, we find that the ion diamagnetic current is the main source of the total perpendicular current, while the curvature current can be neglected. Nevertheless, ions and electrons both carry comparable current due to the redistribution of the electric field and show features beyond the classic Chapman-Ferraro model, particularly on the front side of the boundary layer where the electric field reversal is most intense. We also show a second, comparative event in which ions do not satisfy MHD theory, while the electrons do. The small-scale, adiabatic parameter (square of curvature radius/gyroradius) supports our interpretation that this second event contains ion scale substructure. We suggest that comparing the predicted MHD current with plasma current can be a good method to judge whether the MHD theory is satisfied in each specific circumstance, especially for high-precision Magnetospheric Multiscale data.
        
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  More information
  
    
      Accepted/In Press date: 22 June 2018
 
    
      e-pub ahead of print date: 17 July 2018
 
    
  
  
    
  
    
  
    
  
    
  
    
  
    
     
        Keywords:
        Current carriers, Current sources, Magnetopause current, Two-fluid MHD
      
    
  
    
  
    
  
  
  
    
  
  
        Identifiers
        Local EPrints ID: 425599
        URI: http://eprints.soton.ac.uk/id/eprint/425599
        
          
        
        
        
          ISSN: 2169-9380
        
        
          PURE UUID: 3c3dd243-c00a-4472-ab60-12b046a49bef
        
  
    
        
          
        
    
        
          
        
    
        
          
        
    
        
          
        
    
        
          
        
    
        
          
        
    
        
          
        
    
        
          
        
    
        
          
        
    
        
          
            
              
            
          
        
    
        
          
        
    
        
          
        
    
  
  Catalogue record
  Date deposited: 25 Oct 2018 16:30
  Last modified: 16 Mar 2024 04:18
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      Contributors
      
          
          Author:
          
            
            
              X. C. Dong
            
          
        
      
          
          Author:
          
            
            
              M. W. Dunlop
            
          
        
      
          
          Author:
          
            
            
              T. Y. Wang
            
          
        
      
          
          Author:
          
            
            
              J. B. Cao
            
          
        
      
          
          Author:
          
            
            
              K. J. Trattner
            
          
        
      
          
          Author:
          
            
            
              R. Bamford
            
          
        
      
          
          Author:
          
            
            
              C. T. Russell
            
          
        
      
          
          Author:
          
            
            
              R. Bingham
            
          
        
      
          
          Author:
          
            
            
              R. J. Strangeway
            
          
        
      
        
      
          
          Author:
          
            
            
              B. L. Giles
            
          
        
      
          
          Author:
          
            
            
              R. B. Torbert
            
          
        
      
      
      
    
  
   
  
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