60 YEARS 0. Old tales 1. Ion dynamics 2. Electron dynamics 3. - - PowerPoint PPT Presentation

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60 YEARS 0. Old tales 1. Ion dynamics 2. Electron dynamics 3. - - PowerPoint PPT Presentation

Plasma particle dynamics in collisionless magnetic reconnection Seiji ZENITANI Kyoto University 60 YEARS 0. Old tales 1. Ion dynamics 2. Electron dynamics 3. Perspectives U. Tokyo, STP (Solar Terrestrial Physics) group Super Terasawa


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Seiji ZENITANI

Kyoto University

Plasma particle dynamics in collisionless magnetic reconnection

60

YEARS

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  • 0. Old tales
  • 1. Ion dynamics
  • 2. Electron dynamics
  • 3. Perspectives
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  • U. Tokyo, STP (Solar Terrestrial Physics) group
  • We initially considered:
  • Relativistic magnetic reconnection (SZ, Ph.D thesis 2006)
  • Reconnection in rotating systems (Hoshino, Shirakawa, 2013-2015)

“Super Terasawa Physics” “Masahiro Hoshino Dynamics”

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Relativistic reconnection:

Particle-in-Cell (PIC) simulation

  • Relativistic reconnection is a particle accelerator
  • SZ & Hoshino 2001-2008 (5 papers; 440 citations)

Zenitani & Hoshino 2001, 2007

Energy spectra

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Selected topics on Relativistic Particle-in-Cell Simulations

  • 1. Loading

– Loading velocity distributions by random variables
 (Sobol 1976, Swisdak 2013, Zenitani 2015) – Lorentz transformation for the spatial part (Zenitani 2015)

  • 2. Computation

– EM field (Haber 1974, Vay 2013, Ikeya & Matsumoto 2015) – Particle (Vay 2008, Zenitani & Kato 2018b, Zenitani & Umeda 2018c)

  • 3. Diagnosis & Interpretation

– Relativistic fluid decomposition (Zenitani 2018a)

  • S. Zenitani (Kyoto U), T. N. Kato (NAOJ), T. Umeda (Nagoya U)

(シミュレーション研究会スライド)

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Selected topics on Relativistic Particle-in-Cell Simulations

  • 1. Loading

– Loading velocity distributions by random variables
 (Sobol 1976, Swisdak 2013, Zenitani 2015) – Lorentz transformation for the spatial part (Zenitani 2015)

  • 2. Computation

– EM field (Haber 1974, Vay 2013, Ikeya & Matsumoto 2015) – Particle (Vay 2008, Zenitani & Kato 2018b, Zenitani & Umeda 2018c)

  • 3. Diagnosis & Interpretation

– Relativistic fluid decomposition (Zenitani 2018a)

  • S. Zenitani (Kyoto U), T. N. Kato (NAOJ), T. Umeda (Nagoya U)

(シミュレーション研究会スライド)

Poster

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Selected topics on Relativistic Particle-in-Cell Simulations

  • 1. Loading

– Loading velocity distributions by random variables
 (Sobol 1976, Swisdak 2013, Zenitani 2015) – Lorentz transformation for the spatial part (Zenitani 2015)

  • 2. Computation

– EM field (Haber 1974, Vay 2013, Ikeya & Matsumoto 2015) – Particle (Vay 2008, Zenitani & Kato 2018b, Zenitani & Umeda 2018c)

  • 3. Diagnosis & Interpretation

– Relativistic fluid decomposition (Zenitani 2018a)

  • S. Zenitani (Kyoto U), T. N. Kato (NAOJ), T. Umeda (Nagoya U)

(シミュレーション研究会スライド)

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γ = 100 v ~ +c γ = 200 v ~ -c γ = 10 v ~ +c

+X

Relativistic fluid mechanics is a nightmare…

Energy flow Number flow Eckart frame

N i = 0

Landau frame

T i0 = T 0j = 0

—> Fluid analysis in relativistic reconnection (SZ 2018 PPCF)

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Reconnection as a particle accelerator

Hoshino+ 2001, 2005 JGR SZ & Hoshino 2001 ApJL Hoshino 2012 PRL ※ Not confirmed by SZ

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Electron dynamics in reconnection

Hoshino+ 2001 EPS

Masahiro-Hoshino Dynamics (MHD) is
 very different from the standard MHD

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Beyond MHD Our recent results (SZ+ 2013,2016)

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Magnetic reconnection in near-Earth space

Burch+ 2016 Space Sci. Rev.

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Magnetospheric Multiscale (MMS) mission

2015

Burch+ 2016 Science

2016 Magnetotail reconnection region (Results coming soon) 2017~

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Electron Diffusion Region Electron Dissipation Region

electron

Ion Diffusion Region Ion Dissipation Region

ion

Central engine of magnetic reconnection

Typically, fluid properties of PIC data were analyzed

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(E+vi xB)y

Vx Vy Vx Vy Vz

Ion Velocity Distribution Functions X Z

Ion Diffusion Region?

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  • Poincaré map
  • One way to categorize

particle orbits

Buchner & Zelenyi 1989 Chen & Palmadesso 1986

Nonlinear particle dynamics

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by T. Wada (NAOJ)

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by T. Wada (NAOJ)

Confined on a hyper-surface

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By

X Z

Ion velocity distribution function (VDF)

Vy

By

X Z

Vy Vx Vx

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VDF & Poincaré map

By

X Z

Vy Vx

Two choices from 5 free parameters (x, y, Vx, Vy, Vz)

8

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First demonstration of
 8-shaped orbit in PIC simulation

Speiser orbit (known) 8-shaped orbit Speiser orbit (known) Speiser orbit (known)

X Z Y

X-line

Ion orbits in PIC simulation

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Electron VDFs in PIC simulation

Chen+ 2008 JGR

6x4

  • Many PIC studies on electron VDFs
  • Hoshino+ 2001, Pritchett 2006, Chen+ 2008, 2009, Ng+ 2011,

2012, Bessho+ 2014, Shuster+ 2014, 2015, Cheng+ 2015

Hoshino+ 2001 EPS

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6x4

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Field-aligned inflow

Dissipation region

z x y

Local Speiser orbit

  • B

B

Global Speiser

  • rbit

Egedal orbit

  • By

+By

Electron VDFs vs electron orbits

Orbits VDFs

  • In addition to VDFs,


we have to understand electron orbits, too.

Do we really understand electron orbits?

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Do we really understand electron orbits?

  • Opposite gyration
  • Small gyroradius
  • (Response to E field)

Field-aligned inflow

Dissipation region

z x y

Local Speiser orbit

  • B

B

Global Speiser

  • rbit

Egedal orbit

  • By

+By

Previous expectation Ions Electrons

  • Gyration
  • Large gyroradius

8

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Trajectory analysis in PIC simulations

Oka et al. 2010 ApJ

Memory P I C

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Trajectory analysis in PIC simulations

P I C Memory

P

Oka et al. 2010 ApJ

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Trajectory analysis in PIC simulations

P I C Memory

P P P P P

Oka et al. 2010 ApJ

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Trajectory analysis in PIC simulations

P I C

The number of self-consistent trajectories is limited

Memory

P P P P P

Oka et al. 2010 ApJ

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Our simple solution

Hard drive

P I C P I C Memory

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Our simple solution

P I C Memory

Hard drive

P I C P I C P I C P I C P I C

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PIC simulation & full Lagrange analysis

  • 2.5D
  • mi/me=100
  • 76.8 x 38.4 [di]
  • Harris sheet
  • nbg/ncs = 0.2
  • 2 x 109 particles
  • 20,000,000 electron orbits


from 1250 snapshot data

  • 3,000 orbits are inspected

with eyes

X

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Electron Speiser VDFs in PIC simulation

Vex : electron jets

  • 3
  • 2
  • 1

1 2 3 35 40 45 50

  • 20
  • 15
  • 10
  • 5

35 40 45 50 3 2 1 3

Z Y X “Global Speiser”
 via X-line region “Local Speiser”


  • f reflection type

Z

Speiser 1965 JGR

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  • 2
  • 1.5
  • 1
  • 0.5

0.5 1 1.5 2 2.5 36 38 40 42 44 46 48 2

Electron regular orbits

Z X

(b) Vex z Trapped in a figure-8 shaped orbit (κ~0.2)

Z

Chen & Palmadesso 1986 JGR Zenitani+ 2013 PoP

8

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Noncrossing electrons

  • 0.5

0.5 1 1.5 2 2.5 3 35 40 45 50 1

(a)

z

Midplane Orbits Traditional orbits

Z X

Electrostatic field Ez Midplane

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Noncrossing electrons

  • 0.5

0.5 1 1.5 2 2.5 3 35 40 45 50 1

(a)

z

Midplane Orbits Traditional orbits

Z X

Electrostatic field Ez

Ez

  • Ez

electron

ion

  • eEz

Midplane

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  • 2
  • 1.5
  • 1
  • 0.5

0.5 1 1.5 2 2.5 36 38 40 42 44 46 48 2

Z X

  • 1
  • 0.5

0.5 1

  • 10
  • 5

5 10 15

  • 1
  • 0.5

0.5 1

  • 10
  • 5

5 10

Z Vx Vz

Phase-space diagrams Trapped on flanks of the midplane

Noncrossing regular orbits

Chen & Palmadesso 1986 JGR

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  • 2
  • 1.5
  • 1
  • 0.5

0.5 1 1.5 2 2.5 36 38 40 42 44 46 48 2

Z X

  • 1
  • 0.5

0.5 1

  • 10
  • 5

5 10 15

  • 1
  • 0.5

0.5 1

  • 10
  • 5

5 10

Z Vx Vz

Trapped on flanks of the midplane

Noncrossing regular orbits

Detached from
 the midplane, due to Ez Phase-space diagrams

Chen & Palmadesso 1986 JGR

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2016

Zenitani & Nagai 2016

1965 1980’s

Speiser 1965 Chen & Palmadesso 1986, Buchner & Zelenyi 1989

Orbit theories

A related theory came out recently: Tsai+ 2017

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Noncrossing electrons in the VDF

  • Cold core is occupied by noncrossing electrons in green

vez vex

(c)

B

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Noncrossing electrons: Spatial distribution

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Noncrossing electrons: majority in number

vz

z z

vz

MRX

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State-of-art picture of electron orbits

Dissipation region

z x y

Super-Alfvénic electron jet Local Speiser orbit Noncrossing local Speiser orbit

  • B

B

Global Speiser orbit Field-aligned electron outflow Nongyrotropic electrons Egedal orbit

  • By

+By

Noncrossing regular orbit Crossing regular orbit F i e l d

  • a

l i g n e d i n fl

  • w

Noncrossing global Speiser orbit

Zenitani & Nagai, Physics of Plasmas 23, 102102 (2016)

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PIC シミュレーション研究の課題

Daughton et al. 2011 Nature Phys.

  • 2010年代 大規模PICシミュレーションで複雑かつ乱流的描像が見えてきた
  • 2015年~ MMS衛星が電子運動論スケールのプラズマ観測を開始
  • 流体量解析+粒子加速研究に行き詰まり感 → さらに進んだ解析で突破
  • 乱流、分布関数、軌道(Zenitani & Nagai 2016)
  • 粒子データを活かした解析

Karimabadi et al. 2013 Phys. Plasmas

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Mf(t0, ∆t) Mb(t0, ∆t)

1

+∆t

MR(t0, ∆t) Lagrangian Coherent Structure

Attracting boundary Repelling boundary

粒子データの活用:プラズマ混合度

Zenitani et al. 2017 JGR

電子混合度

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粒子データの活用:エントロピー

Vy Vx

− X

i

pi log pi

(Shannon) エントロピー

  • pi : 3次元速度空間内の確率密度
  • H関数(-f log f)も評価可能


→現象の不可逆性を議論するヒント

Zenitani et al. 2018d in prep.

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Summary

  • 0. M.H.D.

– Particle acceleration and electron dynamics

  • 1. Ion dynamics

– Poincaré-map analysis has revealed figure-8 shaped orbits

  • 2. Electron dynamics

– Full-Lagrange analysis has revealed many new electron orbits – Noncrossing electrons: majority in number density

  • 3. Future direction

– Better usage of PIC data: Orbits, particle mixing, and entropy…

  • References

– Zenitani, Shinohara, Nagai, & Wada, Phys. Plasmas 20, 092120 (2013) – Zenitani & Nagai, Phys. Plasmas 23, 102102 (2016)

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Thank you for your attention!