Re . Sci. Ins um. 92, 043554 (2021); h ps://doi.o g/10.1063/5.0043768 92, 043554
© 2021 Au ho (s).
Design and simula ion o an imaging
neu al pa icle analyze o he ASDEX
Upg ade okamak
Ci e as: Re . Sci. Ins um. 92, 043554 (2021); h ps://doi.o g/10.1063/5.0043768
Submi ed: 11 Janua y 2021 • Accep ed: 25 Ma ch 2021 • Published Online: 26 Ap il 2021
J. Rueda-Rueda, M. Ga cía-Muñoz, E. Viezze , e al.
COLLECTIONS
Pape published as pa o he special opic on P oceedings o he 23 d Topical Con e ence on High-Tempe a u e
Plasma Diagnos ics
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Scien i ic Ins umen s ARTICLE sci a ion.o g/jou nal/ si
Design and simula ion o an imaging
neu al pa icle analyze o he ASDEX
Upg ade okamak
Ci e as: Re . Sci. Ins um. 92, 043554 (2021); doi: 10.1063/5.0043768
Submi ed: 11 Janua y 2021 •Accep ed: 25 Ma ch 2021 •
Published Online: 26 Ap il 2021
J. Rueda-Rueda,1,a) M. Ga cía-Muñoz,1,2 E. Viezze ,1,2 P. A. Schneide ,3J. Ga cía-Domínguez,2
J. Ayllon-Gue ola,2J. Galdón-Qui oga,1,3 A. He mann,3X. D. Du,4M. A. Van Zeeland,4P. Oyola,1
M. Rod iguez-Ramos,5and ASDEX Upg ade Teamb)
AFFILIATIONS
1Depa men o A omic, Molecula and Nuclea Physics, A . Reina Me cedes s/n, 41012 Se ille, Spain
2Cen o Nacional de Acele ado es (CNA) CSIC, 41092 Se ille, Spain
3Max Planck Ins i u e o Plasma Physics, Bol zmanns . 2, 85748 Ga ching, Ge many
4Gene al A omics, P.O. Box 85608, San Diego, Cali o nia 92186-5608, USA
5Labo a o y o Ion Beam In e ac ions, Ru--
de Boˇ
sko i´
c Ins i u e, 10000 Zag eb, C oa ia
No e: Pape published as pa o he Special Topic on P oceedings o he 23 d Topical Con e ence on High-Tempe a u e Plasma
Diagnos ics.
a)Au ho o whom co espondence should be add essed: [email p o ec ed]
b)See he au ho lis o H. Meye e al., Nucl. Fusion 59, 112014 (2019).
ABSTRACT
An Imaging Neu al Pa icle Analyze (INPA) diagnos ic has been designed o he ASDEX Upg ade (AUG) okamak. The AUG INPA
diagnos ic will measu e as neu als escaping he plasma a e cha ge exchange eac ions. The neu als will be ionized by a 20nm ca bon
oil and de lec ed owa d a scin illa o by he local magne ic ield. The use o a neu al beam injec o (NBI) as an ac i e sou ce o neu als
will p o ide adially esol ed measu emen s, while he use o a scin illa o as an ac i e componen will allow us o co e he whole plasma
along he NBI line wi h unp eceden ed phase-space esolu ion (<12 keV and 8cm) and a as empo al esponse (up o 1 kHz wi h he high
esolu ion acquisi ion sys em and abo e 100 kHz wi h he low esolu ion one), making i sui able o s udy localized as -ion edis ibu ions in
phase space.
Published unde license by AIP Publishing. h ps://doi.o g/10.1063/5.0043768
I. INTRODUCTION
A de ailed unde s anding o he as -ion (FI) beha io
in he p esence o magne ohyd odynamic (MHD) luc ua ions
is manda o y o achie ing a good as -ion con inemen in
u u e usion de ices.1Fo his pu pose, no el diagnos ic ech-
niques o measu e he FI dis ibu ion in phase space wi h
Al énic empo al esolu ion a e cu en ly being de eloped. The
Imaging Neu al Pa icle Analyze (INPA), al eady ins alled a
he DIII-D okamak,2,3 which is able o measu e he adial
posi ion and ene gy o he con ined FI popula ion wi h a
as empo al esponse, is one example among hese no el
diagnos ics.
This pape is s uc u ed as ollows: he INPA wo king p inciple
is explained in Sec. II. Sec ion III p esen s he syn he ic diagnos-
ic, while Sec. IV explains he in luence o he di e en geome i-
cal pa ame e s on he de ec o pe o mance. Sec ion Vp esen s he
esponse o he INPA o FI edis ibu ions due o magne ohyd ody-
namic (MHD) ac i i y.
II. WORKING PRINCIPLE
The INPA combines he al eady wo king p inciples o neu al
pa icle analyze s (NPAs)4and as -ion loss de ec o s (FILDs)5 o
p o ide he ene gy and loca ion o he con ined as -ion popula ion
Re . Sci. Ins um. 92, 043554 (2021); doi: 10.1063/5.0043768 92, 043554-1
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FIG.1.Schemeo heINPAwo kingp inciple.Inblueis he ajec o yo heneu al
pa icle, while in ed is he ajec o y o he ion. (a) and (b) show he side and op
iews, espec i ely, while (c) shows a 3D ske ch.
wi h a as empo al esponse. Simila o NPA sys ems, he INPA
analyzes neu al pa icles p oduced in cha ge exchange (CX) eac-
ions. These pa icles a e no con ined by he magne ic ield and
e ain all he in o ma ion o as ions, as no signi ican exchange o
ene gy o momen um occu s du ing he CX eac ion.6A e being
collima ed, neu als a e ionized by an ul a- hin [20nm, o he
ASDEX Upg ade (AUG) se up] ca bon oil and de lec ed owa d a
scin illa o pla e, as can be seen in Fig. 1. The s ike posi ion o he
pa icles in he scin illa o will be de e mined by hei ene gy and
pi ch (λ=− ∥/ , whe e ∥is he eloci y along he magne ic ield)
and he local magne ic ield o he okamak. The use o a neu al
beam injec o (NBI) as an ac i e sou ce o neu als gi es he possi-
bili y o ela ing, ia modeling, he measu ed pi ch o he neu als
o hei adial bi h posi ion and hence o he loca ion o he con-
ined FI. This is possible hanks o he geome ic ela ion be ween
he eloci y o ien a ion o he measu ed neu al and i s adial bi h
posi ion. Figu e 2 shows an example o his ela ion o he case o
AUG.The in- esselposi ioning o he diagnos icopens upa b oade
lexibili yin selec ing he lines-o -sigh (LOSs)compa ed o he con-
en ional elec omagne ic NPA ins alled ou - essel and using hei
own elec omagne ic ields.4The use o a scin illa o will enable
he simul aneous explo a ion o a wide egion o he plasma, which
FIG.2.Rela ionbe ween heline-o -sigh (LOS)and adialbi hposi ion.Asneu al
pa icles a el along a s aigh line, and assuming ha hey a e all bo n along he
NBI line, he e is a one- o-one ela ion be ween he LOS ( eloci y di ec ion o he
neu al) and i s adial bi h posi ion. In blue is he NBI line, in g een a e some o
he explo ed LOSs, and in ed is he loca ion o he INPA head.
would no be co e ed by indi idual LOSs. Ligh emi ed by he scin-
illa o is collec ed by a se ies o lenses and guided o a Phan om
came a and a se o pho omul iplie s (PMTs). The came a allows us
o ob ain high esolu ion images o he scin illa o , while he PMTs
sac i ice his esolu ion o gain a as e empo al esponse.
III. SYNTHETIC DIAGNOSTIC
A syn he ic INPA diagnos ic has been de eloped o s udy he
easibili y o he ins alla ion o an INPA a AUG and o op imize i s
design. The syn he ic INPA is based on FIDASIM7,8 ou pu and he
INPASIM code, which has been de eloped du ing his wo k. Gi en
he magne ic equilib ium, plasma p o iles, he as -ion dis ibu ion
unc ion, and he de ec o geome y, FIDASIM calcula es he lux
o neu al pa icles, coming om CX eac ions, wi h a Mon e Ca lo
(MC) app oach. To his end, a collisional- adia i e model is sol ed.7
FIDASIM has been ex ensi ely e i ied agains expe imen al da a
a he DIII-D,9AUG,10 and TCV11 okamaks, he LHD12 s ella a-
o , and o he de ices.8Using he FIDASIM ou pu ( eloci y-space
esol ed neu al densi ies) as inpu , he INPASIM code calcula es
he syn he ic signal, he esolu ion, and he ins umen unc ion
o pe o m omog aphic econs uc ions as o FILD.13 INPASIM
is di ided in o wo independen sec ions: calcula ion o he sig-
nal/ins umen unc ion and de e mina ion o he scin illa o s ike
map. In he o me , he code acks he FIDASIM ma ke s inside
hediagnos ic head un il hey collide wi h hecollima o o scin illa-
o , bo h conside ed as 3D elemen s. In he la e , MC ma ke s wi h
gi en ene gy and pi ch a e launched a he pinhole in o de o c ea e
amap,which ela es he(R,E)-space o he s ikeposi iono he pa -
icle in he scin illa o . Fo bo h sec ions, sca e ing and ene gy loss
in he ca bon oil a e modeled ollowing SRIM16 simula ions, he
ioniza ion yield in he ca bon oil ollows DIII-D INPA modeling,17
and he scin illa o yield ollows Bi k’s model as applied in absolu e
measu emen so as -ionlossesa AUG.18,19 This modelp edic s he
numbe o pho onsemi ed by hescin illa o pe inciden ion. A e
he scin illa o emission is calcula ed, INPASIM o ms he came a
image conside ing he ansmission ac o o he op ical sys em and
in oducing a 2D Gaussian unc ion o mimic he ini e ocusing o
he op ics, bo h based on Zemax simula ions.
IV. DESIGN OF THE INPA DIAGNOSTIC
A. Selec ion o he posi ion o place he INPA a AUG
The selec ion o he posi ion o he INPA diagnos ic is a com-
p omise be ween ou ac o s: phase space co e age, signal le el
(a enua ion), a ailable space inside AUG, and esolu ion. The o i-
en a ion o he diagnos ic will de e mine which eloci y di ec ions
can be measu ed and he e o e which egion o he FI phase space
canbep obed.Specialca ehasbeen akeninma ching hepi chp o-
ile o he slowing-down as -ion dis ibu ion c ea ed by NBI #8 and
#6o AUG,which a e ypicalexamples o he on- ando -axis FIdis-
ibu ions achie able in AUG ia NBI hea ing. A compa ison o he
pi ch p o iles o hese dis ibu ions and he one INPA will explo e
can be ound in Fig. 3. He e, he pi ch p o ile explo ed by he INPA
diagnos icis highligh ed wi h he whi e dashedline and he apped-
passing bounda y wi h he o ange line. No ice ha he INPA will be
mainly sensi i e o passing ions.
Re . Sci. Ins um. 92, 043554 (2021); doi: 10.1063/5.0043768 92, 043554-2
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FIG. 3. Pi ch p o ile explo ed by he INPA diagnos ic. (a) P ojec ion in he (R,λ)-
spaceo he as -iondis ibu ion,calcula edwi h heTRANSP14,15 code,usingNBI
#6 and sho #19913. The do ed (squa es) whi e line co esponds o a geome ic
calcula ion o he explo ed pi ch p o ile based on he NBI geome y and he mag-
ne ic equilib ium, and he o ange line (ci cles) co esponds o he apped-passing
bounda y a he heigh o he magne ic axis. (b) Equi alen o NBI #8 and sho
#30585. The accep ance o INPA is a ound ±0.1 on he pi ch p o ile shown.
The pinhole posi ion o achie e his good o e lapping is ound
in sec o 16 o AUG, he sec o closes o NBI #3, which p o ides
he ac i e sou ce o neu als. The e o e, he pa h ha CX neu als
should a el inside he plasma and he co esponding losses due
o e-ioniza ion a e minimized. The ansmission ac o o a high
densi y case [ne(0)=6.5 ⋅1019 m−3] can be ound in Fig. 4.
FIG. 4. F ac ion o CX neu als c ea ed in eac ions wi h he ac i e sou ce, which
each hede ec o pinhole,asa unc iono hei adialbi hposi ion.I co esponds
o a densi y o ne(0)=6.5 ⋅1019 m−3. Calcula ed wi h FIDASIM.
B. Collima o and ene gy esolu ion
The basic shape o he INPA collima o is ske ched in Fig. 1.
The collima o leng h, l, is ixed by he a ailable dis ance o he i s
wall, bu all he o he pa ame e s a e ee o be modi ied. The ape -
u e angles o he collima o , αland α , con ol i s accep ance in
he di ec ion o he NBI, as can be seen in Fig. 5. They a e 30○and
40○, espec i ely. These alues enable a co e age o he egion om
R=1.35m up o he ou e sepa a ix, app oxima ely a R =2.16m.
The accep ance o he diagnos ic in he pe pendicula di ec ion,
deno ed by βin Fig. 6(a), domina es he ene gy esolu ion. This
accep ance is con olled by he pinhole size and collima o leng h
and heigh , h. Dec easing he pinhole adius o hwill imp o e he
ene gy esolu ion bu will educe he signal le el. As dec easing he
pinhole adius educes he neu al in lux quad a ically, his he cho-
sen ac o o pu sui he desi ed alue o ene gy esolu ion, as i only
a ec s he signal le el linea ly. A de ailed compa ison o he ene gy
esolu ion o di e en alues o hcan be ound in Fig. 6(b). Val-
ues below h=3 mm a e no conside ed in o de o main ain a lux
high enough o each he Al énic ime scale wi h he PMTs, and
alues abo e h=4 mm a e a oided o keep a good ene gy esolu-
ion. The alue h=3 mm was selec ed as he inal choice, looking
o he bes ene gy esolu ion. Possible sca e ing caused by he ca -
bon oil will also de e io a e he esolu ion, bu he small hickness
o heca bon oil(20nm)makes hissca e ingunimpo an o NBI
injec ion ene gies a AUG.
C. Radial esolu ion
Two ac o s domina e he INPA adial esolu ion: he NBI
sou ce diame e , which ac s as an ac i e neu al sou ce, and
he diame e o he pinhole. Syn he ic signals calcula ed by he
INPASIM code ha e been used o es ima e he adial esolu ion. To
his end, he ac ual bi h posi ion o he ma ke s has been compa ed
wi h he posi ion gi en by he s ike map. The ull wid h hal maxi-
mum (FWHM) o he s uc u es esul ing om his compa ison can
be ound in Fig. 6(c), whe e a pa abolic i has only been included as
a guide o he eye. A p io i, he e is no model ha jus i ies ha he
adial esolu ion mus ha e a pa abolic dependence wi h he majo
adius.
D. Tempo al esolu ion
The signal- o-noise a io (SNR) a he pho o senso o he cam-
e a and PMT was es ima ed as desc ibed in Re . 20. The SNR, o
he pho on lux p edic ed by INPASIM, is plo ed in Fig. 6(d). Tak-
ing a SNR o 10 up o 1 kHz o bandwid h could be achie ed using
FIG. 5. E ec o he collima o angles in he INPA iew. In ed is a 3D ske ch o
he INPA collima o , in shaded g ay is he solid angle co e ed by he INPA, while
in blue is he NBI line.
Re . Sci. Ins um. 92, 043554 (2021); doi: 10.1063/5.0043768 92, 043554-3
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FIG. 6. INPA esolu ion. (a) in luence o he collima o heigh on he ene gy eso-
lu ion; se e al possible ajec o ies o pa icles wi h he same ene gy a e plo ed.
The la ge he heigh o he ca bon oil, he wide he dis ibu ion o impac s on
he scin illa o . (b) Ene gy esolu ion (FWHM) o INPA o di e en alues o he
collima o heigh . He e, he magne ic ield is 2.5T on he axis.(c) Radial esolu ion
o INPA. Calcula ed o sho #30585. The magne ic axisposi ion is indica edwi ha
solid black line while he ou e sepa a ix posi ion wi h a do ed one. The high ield
side (HFS) and low ield side (LFS) a e also indica ed. (d) Signal- o-noise a io o
heacquisi ionsys ems.Thecalcula ion hasbeenpe o med o acasewi haco e
plasma densi y o ne(0)=6.5 ⋅1019 m−3. Calcula ed wi h INPASIM.
FIG. 7. Sec ion o he CAD design o he AUG INPA diagnos ic. (a) In- essel
componen s and (b) ou - essel componen s.
he Phan om came a (which enables he ene gy and adial esolu-
ions p esen ed abo e) and abo e 100 kHz could be achie ed wi h
he PMTs.
E. Mechanical design
An o e iew o he mechanical design o he AUG INPA diag-
nos icisshowninFig.7.Ascanbeseen,inside hede ec o head,no
only he i s op ical elemen s and he scin illa o bu also a calib a-
ion lamp is loca ed, which allows us o check he alignmen o he
op ical componen s be ween sho days. The head is connec ed wi h
he po window wi h a pe iscope. This pe iscope no only allows us
o mee he spa ial bounda y condi ions bu also p o ides he sys-
em wi h he necessa y deg ees o eedom o accommoda e small
de ia ions be ween compu e aided design (CAD) and eali y du -
ing ins alla ion. In he ou - essel egion, a beam spli e di ides he
pho on lux and edi ec s i owa d he Phan om came a and he
PMTs.
V. RESPONSE OF THE INPA TO MHD FLUCTUATIONS
A comple e e iew o he INPA esponse o di e en plasma
scena ios and FI edis ibu ions is ou o he scope o his a icle
and will be p esen ed in a ollow-up pape . He e, we p esen only
one example o show he capabili ies o he diagnos ic. In his case,
we simula e he esponse o he INPA o a localized edis ibu ion.
An ad hoc anomalous di usion coe icien has been inse ed in o
TRANSP o mimic he e ec o a localized MHD luc ua ion in he
FI dis ibu ion. A maximum alue o he anomalous di usion coe -
icien o 0.5 m2/s21,22 has been se , wi h an ex ension o 0.3 in he
ρ space (ρ is he no malized o oidal lux adius), which is in con-
co dance wi h he size o he di e en poloidal modes o a To oidal
Al én Eigenmode (TAE) measu ed and simula ed a DIII-D.23,24
250ms was simula ed o gi e enough ime o he FI o slow down.
Re . Sci. Ins um. 92, 043554 (2021); doi: 10.1063/5.0043768 92, 043554-4
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FIG. 8. (a) Di e ences in he FI dis ibu ion due o he assumed anomalous di usion. Only he mid-plane egion (z =0) has been plo ed, which is calcula ed wi h TRANSP.
(b) Rela i e changes in he scin illa o yield. To a oid simula ion noise, only pixels ha ha e mo e han 5% signal a e plo ed. (b) Cu a 72 keV. Shaded a eas ep esen a
s anda d de ia ion o 5%, he expec ed uppe limi o measu emen noise. The g ay dashed ames indica e whe e he anomalous di usion was applied.
As men ioned in Re . 25, his simula ion scheme canno ep oduce
he p ecise in e ac ion be ween he MHD ins abili ies and as ions
bu gi es an es ima e o he pa icle anspo . The anomalous di -
usion has been selec ed o be cons an in he in e al ρ ∈(0,0.3)
and ze o o he wise. In ene gy, he coe icien akes a Gaussian shape
cen e ed a 72 keV, wi h a FWHM o 10 keV, o mimic a na ow
esonance. Anomalous di usion has only been applied o passing
pa icles. The ela i e di e ence in he dis ibu ion unc ion can be
seen in Fig. 8(a). No ice ha in he egion be ween R =1.55 and
1.85m, he FI densi y is smalle when he di usion is ac i a ed, as
expec ed ( he ange whe e he di usion was applied is highligh ed
in g ay). The di e ences in he scin illa o signal can be seen in
Fig. 8(b). No e how i ag ees wi h he di e ences in he FI dis i-
bu ion, inside he esolu ion o he diagnos ic. In Fig. 8(c), he di -
e ence along he cons an line o 72 keV can be seen. Bo h cu es
will be dis inguishable, e en wi h he assumed 5% o noise. Du ing
hiscompa ison, heplasma p o iles ha ebeen conside ed o emain
cons an .
The INPA diagnos ic is, in i s cu en con igu a ion, no
expec ed o be sensible o a edis ibu ion o apped pa icles
because he explo ed pi ch p o ile is basically always in he passing
egion o he phase space (see Fig. 3). Only o egions close o he
sepa a ix, he apped-passing bounda y en e s he egion explo ed
by he INPA and he diagnos ic becomes sensible o apped pa i-
cles. The e o e, in gene al, only passing ions o apped ions, which
become passing and en e he INPA ield o iew a e he di usion,
will be measu able.
VI. CONCLUSIONS
An imaging neu al pa icle analyze has been designed and
op imized o he ASDEX Upg ade okamak. This diagnos ic will
allow measu emen s o he dis ibu ion o sup a- he mal pa icles
in ene gy and adius wi h good esolu ion and a as empo al
esponse simul aneously, complemen ing he AUG sui e o as -ion
diagnos ics o ob ain a comple e unde s anding o he dynamics and
anspo o sup a- he mal pa icles.
The inal design o he diagnos ic ea u es an ene gy esolu ion
o 12 keV o 100 keV ions and a adial esolu ion below 8cm a he
low ield side o AUG, wi h a empo al esponse o 1 kHz. I he as
acquisi ion sys em (wi h low spa ial esolu ion) is used, he esponse
is inc eased o abo e 100 kHz.
ACKNOWLEDGMENTS
This p ojec ecei ed unding om he Eu opean Resea ch
Council (ERC) unde he Eu opean Union’s Ho izon 2020 esea ch
and inno a ion p og amme (G an Ag eemen No. 805162) and he
Spanish Minis e io de Ciencia, Inno ación y Uni e sidades (G an
No. FPU19/02486).
DATA AVAILABILITY
The da a ha suppo he indings o his s udy a e a ailable
om he co esponding au ho upon easonable eques .
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