The contribution of flux transfer events to Mercury's Dungey cycle
The contribution of flux transfer events to Mercury's Dungey cycle
 
  Bursty dayside reconnection plays a proportionally larger role in the driving of Mercury's magnetosphere than it does at Earth. Individual bursts of reconnection, called flux transfer events (FTEs), are thought to open up to 5% of Mercury's polar cap; coupled with the much higher repetition rate of FTEs at Mercury and the short Dungey cycle timescale, this makes FTEs the major driver of Mercury's magnetosphere. However, comparison between spacecraft and ionospheric observations at Earth suggests that the terrestrial contribution of FTEs may have been severely underestimated, by making implicit assumptions about FTE structure. In this study, we consider the implications of removing these assumptions at Mercury; by considering FTE mechanisms based on longer reconnection lines, we find that the contribution of FTEs to Mercury's Dungey cycle could be 5 times greater than previously thought and that FTEs may be able to provide sufficient flux transport to drive Mercury's substorm cycle.
  
  
  14239-14246
  
    
      Fear, Robert
      
        8755b9ed-c7dc-4cbb-ac9b-56235a0431ab
      
     
  
    
      Coxon, John
      
        566baea5-6a30-4855-bde3-a09c115efde4
      
     
  
    
      Jackman, Caitriona
      
        9bc3456c-b254-48f1-ade0-912c5b8b4529
      
     
  
  
   
  
  
    
    
  
    
    
  
    
      23 December 2019
    
    
  
  
    
      Fear, Robert
      
        8755b9ed-c7dc-4cbb-ac9b-56235a0431ab
      
     
  
    
      Coxon, John
      
        566baea5-6a30-4855-bde3-a09c115efde4
      
     
  
    
      Jackman, Caitriona
      
        9bc3456c-b254-48f1-ade0-912c5b8b4529
      
     
  
       
    
 
  
    
      
  
  
  
  
  
  
    Fear, Robert, Coxon, John and Jackman, Caitriona
  
  
  
  
   
    (2019)
  
  
    
    The contribution of flux transfer events to Mercury's Dungey cycle.
  
  
  
  
    Geophysical Research Letters, 46 (24), .
  
   (doi:10.1029/2019GL085399). 
  
  
   
  
  
  
  
  
   
  
    
    
      
        
          Abstract
          Bursty dayside reconnection plays a proportionally larger role in the driving of Mercury's magnetosphere than it does at Earth. Individual bursts of reconnection, called flux transfer events (FTEs), are thought to open up to 5% of Mercury's polar cap; coupled with the much higher repetition rate of FTEs at Mercury and the short Dungey cycle timescale, this makes FTEs the major driver of Mercury's magnetosphere. However, comparison between spacecraft and ionospheric observations at Earth suggests that the terrestrial contribution of FTEs may have been severely underestimated, by making implicit assumptions about FTE structure. In this study, we consider the implications of removing these assumptions at Mercury; by considering FTE mechanisms based on longer reconnection lines, we find that the contribution of FTEs to Mercury's Dungey cycle could be 5 times greater than previously thought and that FTEs may be able to provide sufficient flux transport to drive Mercury's substorm cycle.
         
      
      
        
          
            
  
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 The Contribution of Flux Transfer Events to Mercury's Dungey Cycle
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      Accepted/In Press date: 2 December 2019
 
    
      e-pub ahead of print date: 4 December 2019
 
    
      Published date: 23 December 2019
 
    
  
  
    
  
    
  
    
  
    
  
    
  
    
  
    
  
    
  
  
  
    
  
  
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        Local EPrints ID: 437449
        URI: http://eprints.soton.ac.uk/id/eprint/437449
        
          
        
        
        
          ISSN: 0094-8276
        
        
          PURE UUID: 5bf9e724-4840-44f3-bc31-021f3c31f8a5
        
  
    
        
          
            
              
            
          
        
    
        
          
            
              
            
          
        
    
        
          
            
              
            
          
        
    
  
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  Date deposited: 30 Jan 2020 17:38
  Last modified: 17 Mar 2024 05:17
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