Simulating energetic particle losses in JET plasmas with a reverse integration biasing scheme

2021 ◽  
Author(s):  
Phillip Bonofiglo ◽  
Mario Podesta ◽  
Roscoe B White ◽  
Vasily Kiptily ◽  
Victor Goloborodko ◽  
...  

Abstract An integrated energetic particle transport model has been constructed in JET plasmas constrained by experimental fast ion loss measurements. The model incorporates a synthetic fast ion loss detector identical to JET's thin-foil Faraday cup fast ion loss detector array. The loss model combines analyses from the TRANSP and ORBIT-kick codes with enhanced features for producing the synthetic diagnostic. Extensions to the ORBIT code framework allow a full-orbit representation within the vacuum region that can map particles directly to an installed detector geometry. Since synthetic fast ion loss detectors are plagued by weak loss statistics, a novel reverse integration biasing scheme has been implemented to boost computational efficiency. The model is validated against experimental loss measurements induced by long-lived kink modes and is found to be in good agreement. This confirms the development of a fully integrated transport/loss model which can be quantitatively verified against experiment allowing for future validation and predictive studies. The model is particularly useful for more complicated plasma scenarios that involve multiple fast ion species such as JET's 2021 DT-campaign.

2010 ◽  
Vol 17 (5) ◽  
pp. 467-479 ◽  
Author(s):  
B. T. Tsurutani ◽  
G. S. Lakhina ◽  
O. P. Verkhoglyadova ◽  
E. Echer ◽  
F. L. Guarnieri

Abstract. We discuss two different physical processes that create localized high β plasma regions. One is nonlinear wave-steepening, generating magnetic decreases (MDs) by a ponderomotive force. The other is the mirror instability generating alternating high and low β plasma regions. It is demonstrated that MDs and mirror modes are observationally quite different structures. MDs spatially occur in interplanetary space and mirror modes primarily in planetary magnetosheaths. MDs are characterized by: 1) variable (exponentially decreasing number with increasing) angular changes, 2) variable (exponentially decreasing) thicknesses, and 3) no characteristic inter-event spacings. In sharp contrast, mirror modes are characterized by: 1) little or no angular changes across the structures, 2) a characteristic scale size, and 3) are quasiperiodic in nature. Arguments are presented for the recently observed magnetic dips in the heliosheath being mirror mode structures. The sources of free energy for instability are discussed. Both structures are important for energetic particle transport in astrophysical and heliospheric plasmas.


2009 ◽  
Vol 8 (4) ◽  
pp. 858-872 ◽  
Author(s):  
Sorab Panday ◽  
Nathan Brown ◽  
Terry Foreman ◽  
Vivek Bedekar ◽  
Jagjit Kaur ◽  
...  

1999 ◽  
Vol 39 (9Y) ◽  
pp. 1309-1319 ◽  
Author(s):  
B.C Stratton ◽  
R.V Budny ◽  
D.S Darrow ◽  
R.K Fisher ◽  
E.D Fredrickson ◽  
...  

1995 ◽  
Vol 35 (12) ◽  
pp. 1697-1705 ◽  
Author(s):  
L.C Appel ◽  
H.L Berk ◽  
D Borba ◽  
B.N Breizman ◽  
T.C Hender ◽  
...  

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