‫׷ֶֽח'‪+1"3$.-‬‬‫‪䱱稊‬ظٔز‪ُ٦‬صٕ؎ٓذأ‬‫‪灇瑔⠓!+1"3$‬يذأء‪ 鎘庠‬‬‫‪ٝ㣐㷕‬ؖءى ➂‪䀵❁խ榪‬‬‫‪1‬‬‫ُصٕ؎ٓذأ‬٦‫ظٔز‬䱱稊˖ 䎃⟃勻ծ傀濼‫ُصך‬٦‫ظٔز‬䮶⹛‫כד‬铡僇‫ְזֹד‬ծ幉尔‫׋׃ה‬㹋꿀✲㹋ָ֮‫׷‬կ
-4/%

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‫ُص‬٦‫ظٔز‬彁

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tEFDBZBUSFTU

ğt̔ğFĤ

.F7N.JOJ#PP/&(BMMJVN4"(&
⾱㶨拜

FDBQUVSF
Ĕ䄶㠨ğt̔ğF

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5

.F7N
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L/Eν (meters/MeV)˖ -&1㹋꿀‫׶״‬ծ颵ꆀ.[⟃♴‫ך‬䓲ְ湱✼⡲欽;‫ٕفحؕה‬‫ׅ‬‫ُص׷‬٦‫כظٔز‬珏겲‫׫ך‬
FIG. 24:

The Lν /Eν distribution for events with Rγ > 10 and 20 < Ee < 6

the distance travelled by the neutrino in meters and Eν is the neutrino energ

agree well with the expectation from neutrino background and neutrino oscilԸ䓲ְ湱✼⡲欽‫ُصְז׃׾‬٦‫ظٔز‬Ԩ✲㹋‫ַךז‬ծ꟦麩ְ‫ַךז‬ծ㸣Ⰻ寸滠 Ĥ⟃♳ ‫׾‬湡䭷‫ׅ‬2+1"3$&+4/4 BU.-'Material and Life
science Facility3.-'‫⚥ך‬䚍㶨彁3$4 )(UBSHFUJO.-'˖ 3$4‫ך‬㣐䓼䏝ꤿ㶨‫ؽ‬٦‫⚅׷״חي‬歲‫ךأؙٓ‬㣐䓼䏝⚥䚍㶨彁‫ُص‬٦‫ظٔز‬彁 ‫ؽ‬٦‫ؘٕطؒي‬٦(F7 ‫ؽ‬٦‫ػي‬ٙ٦鏣鎘⦼.8 鸬竲ⵃ欽麊鯄L8˖ ‫ؽ‬٦‫׵ַي‬tT⟃꣬‫׾‬鼅‫׶״חהֿע‬ծ꫼姺‫ُى‬٦ؔٝ䄶㠨歋勻‫ُصך‬٦‫׾׫ךظٔز‬錁庠‫׷ֹדָהֿ׷ׅ‬#ν/10ns/POT

80ns

540ns

80ns
time

M. Harada et al,arXiv:1310.1437[physics.ins-det]

10-2
-3

10

10-4

total
from µfromfrom K

-5

10

-6

10

mercury target（neutron＆neutrino source）

3GeV
proton beam

10-7
-8

10

0

500

1000

1500

2000

time[ns]4庠㹀⾱椚
protonbeam+
μtargetνμprompt : e+νe(µ+ decay-at-rest)(up to 50 MeV)n

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delayed : γsdetector(total 8MeV)˖ ‫ٕشؚء‬ğt ̔ğ ̔ğF˖ ‫ُص‬٦‫ظٔز‬彁ğtGSPNĢ ̔t ̔F EFDBZBUSFTU
 JOUSJOTJDğFĢ̔t̔F‫ؑث‬٦ٝ‫כ‬Ģt䯲栻‫׶״ח‬呞䫇ⵖ˖ 鷞Ĕ䄶㠨 *#%ğF Q̔F  O ‫ך‬鹼䒀ず儗鎘庠 倖꬗琎ծؒ‫ؘٕط‬٦ⱄ圓䧭ָ‫ֻ״‬椚鍑ׁ‫׷ְג׸‬ 䖓涪✲韋‫כ‬ծ(E‫⚥׷״ח‬䚍㶨䯲栻ַ‫ ך׵‬醱侧‫ ך‬ĕ简‫׃ה‬‫ג‬錁庠˖ -4/%‫ך‬湫䱸涸‫ז‬鷄嗚鏾ָ〳腉5

嗚⳿㐻

MLF 3rd ﬂoor
(maintenance area)

２
ﬁducial: 50 tonnes in total˖ ‫ك‬٦‫؎ٓأ‬ٝN

mercury target（neutron＆neutrino source）

3GeV
proton beam

˖ 剣⸬⡤琎‫ز‬ٝ˖ ؒ‫ؘٕط‬٦ⴓ鍑腉Ĥ&&<>_TRSU <.F7>˖ ⚥䚍㶨䯲栻‫׷״ח‬䖓涪✲韋
 (EⰅ‫׶‬巉⡤‫ء‬ٝ‫ٖث‬٦‫ ة‬%BZB#BZ %PVCMF$IPP[ 3&/0 䪮遭䩛岀‫כ‬然甧ׁ‫׷ְג׸‬˖ 14%BOEPS$IFSFOLPW‫׷״ח‬磛㶨陎ⴽ ĕO˖ 倜‫ؽ‬٦‫؎ٓي‬ٝ 倜㹋꿀啥 䒉鏣ַ‫׵‬䎃‫رד‬٦‫《ة‬䖤Ꟛ㨣‫פ‬
˖ 3FBTPOBCMFDPTU ։⭙EFUFDUPS 鎘⭙6

∆ m2[eV

JSNS2 5σ
LSND 90%C.L.
LSND 99%C.L.
OPERA(2013) 90%C.L.
IceCube combined* 90%C.L.
IceCube combined* 99%C.L.
(* arXiv 1607.00011v2)⥋〾䬄⳿‫ה‬䠬䏝
10˖ ⥋〾✲韋‫⚺ה‬銲‫ُصז‬٦‫ظٔز‬歋勻‫ך‬胜兝✲韋 JOUSJOTJDğF ‫ؘٕطؒכ‬٦ⴓ䋒‫ך‬麩ְ‫׾‬欽ְ‫ג‬䬄⳿‫׷ֹד‬
10
1

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10
10
10
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Total
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a)

35

20

15

Events/MeV

102

40

15

10

10

5

5

45
40

10

20

30

40

50

60
E[MeV]

LSND best ﬁt
Total
i e from i µ Oscillationi e from µ-−11
sin22θJSNS2 90%C.L.
JSNS2 3σ
JSNS2 5σ
LSND 90%C.L.
LSND 99%C.L.
OPERA(2013) 90%C.L.
IceCube combined* 90%C.L.
IceCube combined* 99%C.L.
(* arXiv 1607.00011v2)

25

20

on

45

30

25

50

Total
i e from i µ Oscillationi e from µ-

35

30

0
0

−2

50t, 5MWyr@24m

50∆ m2[eV 2Events/MeV/c 4]

Events/MeV

−4

10

0
0

10

20

30

40

1

50

60
E[MeV]

b)
10− 1

35
30
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40
50
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E[MeV]

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10

10
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10

20

30

40

50

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E[MeV]

10

−3

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1
sin22θ
7

5JNFMJOF‣ 剢։剢.-'㹋꿀‫م‬٦ٕ ' ‫ךד‬胜兝✲韋庠㹀‣ 剢㹋꿀‫هٗف‬٦‫׾ٕؠ‬䲿⳿UI+1"3$1"$‣ 剢։剢㹋꿀⦪酡㖑㹋㖑‫ךד‬胜兝✲韋庠㹀 .-''‣ 剢+1"3$3$4.8USJBM‣ 剢4UBHFBQQSPWBM‣ 㢙3$43'14،‫ؚٖفح‬٦‫ س‬.8鸬竲麊鯄‫׭׋ך‬





‣ 剢։剢巉‫ء‬ٝ‫׾‬欽ְ‫׋‬胜兝✲韋庠㹀BU.-''‣ 〴湡嗚⳿㐻‫ך‬頿彁㛇湍‣ 䪮遭鏣鎘剅 5FDIOJDBM%FTJHO3FQPSU ‫ך‬䲿⳿‣ ‫ر‬٦‫《ة‬䖤Ꟛ㨣䎃䏝劣
8

5JNFMJOF‣ 剢։剢.-'㹋꿀‫م‬٦ٕ ' ‫ךד‬胜兝✲韋庠㹀‣ 剢㹋꿀‫هٗف‬٦‫׾ٕؠ‬䲿⳿UI+1"3$1"$‣ 剢։剢㹋꿀⦪酡㖑㹋㖑‫ךד‬胜兝✲韋庠㹀 .-''‣ 剢+1"3$3$4.8USJBM‣ 剢4UBHFBQQSPWBM‣ 㢙3$43'14،‫ؚٖفح‬٦‫ س‬.8鸬竲麊鯄‫׭׋ך‬





‣ 剢։剢巉‫ء‬ٝ‫׾‬欽ְ‫׋‬胜兝✲韋庠㹀BU.-''‣ 〴湡嗚⳿㐻‫ך‬頿彁㛇湍‣ 䪮遭鏣鎘剅 5FDIOJDBM%FTJHO3FQPSU ‫ך‬䲿⳿‣ ‫ر‬٦‫《ة‬䖤Ꟛ㨣䎃䏝劣
9

UBSHFU#(CBDLHSPVOET

elsewhere in the world. These include OscSNS at SNS in the US, STEREO at
ILL in Europe, NEUTRINO-4 in Gatchina, Russia, and others. However, none ofthese other experiments have been approved yet. The PAC invites the proponents㹋꿀⦪酡㖑‫ךד‬胜兝✲韋庠㹀

of P56 to address the relative time scales and sensitivities of their proposal
compared to these potential competitors.

The most critical technical issue is a detailed estimate of the actual background rate
at the 3rd floor of the MLF. The PAC recommends a direct measurement of thisbackground with a small-scale prototype detector. If the background levels are aspredicted (based on an extrapolation from rates measured at BL13 using asimulation), the experiment would be technically feasible and could receive stage-I
approval.

UI+1"3$1"$

DPNQBSFCFBN0/0''

15. Hall planning after renovation

CFBNPO.JDIFMFO

Gd.JDIFMFeexperimental area to the K1.1 experimental area in FY2013. However, the PAC
GBLFQSPNQU
understands that this scheduled work has to be rearranged. The PAC endorses thedecision that the renovation work of the hadron hall has to be started first and has
higher priority than high-p/COMET construction
and moving the SKS.
EFMBZFETJHOBMTXFSFIn the Hadron hall in May, experiments with secondary kaon beams at 25kW
OPUSFRVJSFE
primary proton intensity, E15 at the K1.8BR beam line, and E14 at the KL beamline, were acquiring data, and E13 at the K1.8 beam line and E31 at the K1.8BR
beam line were preparing for the beam time in June. The PAC understands that thebeam time for these experiments will be fully re-allocated when the Hadron hall

UJNF

_tTUJNFµ

DPNNFOU

Before the accident, the high-p and the COMET beam lines planned to start
construction and the SKS spectrometer was scheduled to move from the K1.8

GBLFEFMBZFEγˑPOCVODI˒DPTNJDtµˑPOCVODI˒

CZCFBNGBTU
OFVUSPO

CFBNPThe PAC heard a presentation on the work plan for renovation of the hadron hall.

e

ӧ

19

IVHF SFKFDUFECZWFUP

GSPNDPTNJDt

UJNF

ӧ

SFKFDUFECZEFUFDUJOHNPUIFSt

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ӧ

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10㹋꿀⦪酡㖑‫ךד‬胜兝✲韋庠㹀˖ 垥涸‫ء‬ٝ‫ٖثث‬٦‫ة‬ QJFDFT 鎘LH˖ 㾴ַ‫زك׷ז׵‬٦‫يذأء‬MLF 3rd ﬂoor
(maintenance area)

 JOOFSBOEPVUFS‫زك‬٦ 嗚⳿⸬桦
mercury target（neutron＆neutrino source）

front view

3GeV
proton beamside view
side
view

11

-5

10

㹋꿀⦪酡㖑‫ךד‬胜兝✲韋庠㹀
-6

10

10-7
-8

10

100ns 100ns

0

50

100

time

102

3

10

102

10

#events/spillenergy[MeV]

600ns
10-2

beam ON w/o vetobeam OFF w/o veto

-3

10

-4

10

beam ON w/ vetobeam OFF w/ veto

-5

10

-6

10
10

10-7

QSPKFDUJPO
10

1

-8

0

TQJMML8
103

102

XPWFUPXWFUP

2000

1

4000

time[ns]

0/

0

0''

hTimeTest

Entries 69028p
Yp
Y
Mean
569.5 ± 1.272
RMS
Integral

333.4


6.87e+04

p Yp Y50

þ 0/0''p Y

100

energy[MeV]
4"KJNVSBFUBM
1SPH5IFPS&YQ1IZT $p Y

12

beam-on-510胜兝✲韋庠㹀

nµ“on bunch”-6

10 Target BG

Gd“beam Michel-e”-7-8 cosmic µ

10100ns 100ns

0 Michel-efrom cosmic µ

3

10

102

10

#events/spill

102

-5

10

time

○

time

○

time

○

e

POCVODIIJU

600ns

delayed signals

were not observed

time~2.2µsOther cosmic related

time

e

γ

µ
50

comment

fake prompt

fake delayed

10“on bunch”

energy[MeV]beam-oﬀ

huge, rejected by vetosuppressed by100
checking timing of
mother µ

accidental hit on bunch
timingbeam
beam unrelated-6

FTUJNBUJPO

10

10-7
10
-8

10

QSPKFDUJPO

10TQJMML8
103

102

XPWFUPXWFUPˑPOCVODIDVU˒

2000

1

4000

time[ns]

0/

0

0''

hTimeTest

Entries 69028p
Yp
Y
Mean
569.5 ± 1.272
RMS
Integral

333.4


6.87e+04

p Yp Y

50

þ 0/0''p Y

100

energy[MeV]
4"KJNVSBFUBM
1SPH5IFPS&YQ1IZT $p Yp Y

p Y

p Y ̤ZS.8U˟FTUJNBUJPO$-13

"DDJEFOUBM#( 巉‫ء‬ٝ /& /B*‫׾‬欽ְ‫ⴽ׋‬庠㹀 ⟃ⰻ‫♧ד‬荜˖ ‫ؽ‬٦‫ي‬歋勻ĕ简‫׷״ח‬䖓涪✲韋#( 䎮‫؝‬ٝ‫ؙٔ‬٦‫ך׵ַز‬ĕ简 嗚⳿㐻♴‫ח‬ꊊ‫׾ؙحٗـ‬侲ֻ✲‫ד‬䫇姺

10-2

10-2

data
cosmicγ
neutronMichel-e
env.γ

-3

10-3
10

10-4-4
10
-5

10

-5

10-6
10

10-7-6
10
-8

10 0
0

#events/2.5µs ‫ؽ‬٦‫ي‬搀‫׃‬儗‫⯓ך‬涪✲韋‫ؘٕطؒך‬٦걄㚖鋵‫ُى‬٦ؔٝ嗚⳿‫׷״ח‬.JDIFMFꤐ⿠#events/2.5µs

˖ 㸘㸾简饯彁‫⯓ך‬涪✲韋#(

4"KJNVSBFUBM
1SPH5IFPS&YQ1IZT $

20

5
50 40

10100
60

80

15 100150

energy[MeV]

data
gamma
env.γ
cosmic ray

-3

10

10-4
-5

10

-6

10

0

5

10

15

energy[MeV]14

series of background measurements on the 3rd floor of the MLF using a 500 kg array of 24

5JNFMJOF

plastic scintillators surrounded by cosmic veto scintillators. They made measurements at points
with 3 different baselines: 17 m, 20 m, and 40 m. Only the results from 20 m were reported.
For comparison with the rates quoted in their proposal, Monte Carlo was used to extrapolate thefor the 500 kg detector to a 25-ton
liquid scintillator detector at 24 m. They
20 m ‣results剢։剢.-'㹋꿀‫م‬٦ٕ' ‫ךד‬胜兝✲韋庠㹀
investigated two sources of beam-related background: beam fast neutrons and accidentals. They‣ 剢㹋꿀‫هٗف‬٦‫׾ٕؠ‬䲿⳿UI+1"3$1"$

saw no evidence for beam-related fast neutrons and set a limit of < 8 events/ 4 years/ 50 ton /MW. A‣ 30剢։剢㹋꿀⦪酡㖑㹋㖑‫ךד‬胜兝✲韋庠㹀.-''
times larger accidental rate of photons than expected was observed,
originating from‣ 剢+1"3$3$4.8USJBM

the large flux of neutrons striking the concrete below the experiment area. To reduce thisbackground they propose to use a 12.5 cm layer of lead under the detector: the effect of thisshielding‣ 剢4UBHFBQQSPWBM
has already been tested and will reduce the gamma flux to 1/10 of the proposal rate.

‣ 㢙3$43'14،‫ؚٖفح‬٦‫س‬
.8鸬竲麊鯄‫׭׋ך‬Basedon the background measurements presented,
the PAC is convinced that thebackgroundrates described in the proposal are achievable. The PAC recommends stage-1 status‣ 剢։剢巉‫ء‬ٝ‫׾‬欽ְ‫׋‬胜兝✲韋庠㹀BU.-''for P56.




‣ 〴湡嗚⳿㐻‫ך‬頿彁㛇湍
15‣ 䪮遭鏣鎘剅 5FDIOJDBM%FTJHO3FQPSU‫ך‬䲿⳿‣ ‫ر‬٦‫《ة‬䖤Ꟛ㨣䎃䏝劣
15

5JNFMJOF‣ 剢։剢.-'㹋꿀‫م‬٦ٕ ' ‫ךד‬胜兝✲韋庠㹀‣ 剢㹋꿀‫هٗف‬٦‫׾ٕؠ‬䲿⳿UI+1"3$1"$‣ 剢։剢㹋꿀⦪酡㖑㹋㖑‫ךד‬胜兝✲韋庠㹀 .-''‣ 剢+1"3$3$4.8USJBM‣ 剢4UBHFBQQSPWBM‣ 㢙3$43'14،‫ؚٖفح‬٦‫ س‬.8鸬竲麊鯄‫׭׋ך‬





‣ 剢։剢巉‫ء‬ٝ‫׾‬欽ְ‫׋‬胜兝✲韋庠㹀BU.-''‣ 〴湡嗚⳿㐻‫ך‬頿彁㛇湍‣ 䪮遭鏣鎘剅 5FDIOJDBM%FTJHO3FQPSU ‫ך‬䲿⳿‣ ‫ر‬٦‫《ة‬䖤Ꟛ㨣䎃䏝劣16⦪酡㖑‫ךד‬巉‫ء‬ٝ‫׾‬欽ְ‫׋‬庠㹀˖ 杆ְ ‫ؽ‬٦‫⚥׷ֻג׏װח⚥ي‬䚍磛㶨‫ך‬陎ⴽ Oĕ  ⦪酡㖑‫ךד‬巉‫ء‬ٝ麊欽 㸜Ⰻ꬗‫✮ךד‬遤怴统ビームオンバン
Veto

Pictures for setups

Preliminary

15 MeV以上の事象を横軸方向に射影• 擬似的に2 Bunchイベントを作成
し、先発信号開始後に染み出す事象数を見積もる。
17•

5JNFMJOF‣ 剢։剢.-'㹋꿀‫م‬٦ٕ ' ‫ךד‬胜兝✲韋庠㹀‣ 剢㹋꿀‫هٗف‬٦‫׾ٕؠ‬䲿⳿UI+1"3$1"$‣ 剢։剢㹋꿀⦪酡㖑㹋㖑‫ךד‬胜兝✲韋庠㹀 .-''‣ 剢+1"3$3$4.8USJBM‣ 剢4UBHFBQQSPWBM‣ 㢙3$43'14،‫ؚٖفح‬٦‫ س‬.8鸬竲麊鯄‫׭׋ך‬





‣ 剢։剢巉‫ء‬ٝ‫׾‬欽ְ‫׋‬胜兝✲韋庠㹀BU.-''‣ 〴湡嗚⳿㐻‫ך‬頿彁㛇湍̒剣⸬⡤琎‫ز‬ٝ‣ 䪮遭鏣鎘剅 5FDIOJDBM%FTJHO3FQPSU ‫ך‬䲿⳿‣ ‫ر‬٦‫《ة‬䖤Ꟛ㨣䎃䏝劣
18

4JHOBMBOE#(T#($POUFOUTUZS.8/PUFT

ğFGSPNt⚺‫ז‬#(ğF $̔F /HT‫ؽ‬٦‫ي‬넝鸞⚥䚍㶨 $-ַ‫ך׵‬.JDIFMF㹋庠㹀‫ח‬㛇‫ֻב‬㸘㸾简넝鸞⚥䚍㶨㹋庠㹀‫ח‬㛇‫ֻב‬ꤐ⿠‫⟎׾‬㹀

"DDJEFOUBM㹋庠㹀‫ח‬㛇‫ֻב‬⥋〾ğt̔ğF



m2 = 2.5 eV2 , sin2 2 = 0.003+4/4CFTUTFOTJUJWJUZ
m2 = 1.2 eV2 , sin2 2 = 0.003-4/%CFTUU
19

Events/MeV

ov or/and PSD5%3䲿⳿‫ח‬ぢֽ‫ג‬
50

Total
i e from i µ Oscillationi e from µ-4540• Left；with small˖ 嗚⳿㐻3%
amount of‣ 葺ְؒ‫ؘٕط‬٦ⴓ鍑腉
scintillation light,‣ 葺ְ넝鸞⚥䚍㶨ꤐ⿠腉⸂
Cherenkov light can
Ը1VMTF4IBQF%JTDSJNJOBUJPObe seen with timing. 14% BOEPS$IFSFOLPW
35
30
25
20
15
10
5

0
0

10

20

30

40

50

60
E[MeV]

˖ 14%
0.24

Neutrino

0.22

NeutronArbitrary

TailQ/TotalQPSD#F简彁̔+4/4
variable Æ tailQ/totalQԨ• "N걄㚖‫ךד‬䚍腉鋅琎1
Neutrino

0.8

Neutron

0.2
0.6

0.18
0.16

.$
&<.F7>

0.4

0.14
0.2

0.12
0.1
0

Preliminary
6
2000

4000

6000

8000

10000 12000
Num_Of_PEs

Preliminary
00.1

0.12 0.14 0.16

0.18

0.2

0.22 0.24
TailQ/TotalQ

20

$IFSFOLPW‫׷״ח‬磛㶨陎ⴽ˖ 湡涸 Oĕ磛㶨陎ⴽ 14%‫سحٔـ؎عךה‬ ꨵ煁‫ٍء‬ٙ٦鹌遤倯ぢ‫ⱄך‬圓䧭˖ Ꟛ涪銲稆 巉⡤‫ء‬ٝ‫ٖث‬٦‫ة‬涪⯔‫ؙؚؐٓحغ׷״ח‬ٝ‫س‬ؒ‫ؘٕط‬٦ⴓ鍑腉 14%‫ך‬錁挿ַ‫כ׵‬ծ‫ء‬ٝ‫⯔ث‬ꆀ‫כ‬㢳ְ倯ָ劄‫ְ׃ת‬ 1.5‫׷״ח‬剣ꣲ‫ך‬QIPUPDPWFSBHF‫ךزأ؝‬錁挿ַ‫ֻץ׷זכ׵‬1.5‫ך‬侧‫כ‬幾‫ְ׋׃׵‬observed
Cherenkov=

Scintillation+˟⡚涪⯔巉⡤‫ء‬ٝ‫ٖث‬٦‫הة‬DPWFSBHF‫ךד‬嚊䙀㔳 .$21巉⡤‫ء‬ٝ‫ٖث‬٦‫ךة‬暴䚍
PPO$concentraGon$dependences$$of$light$yield$and$waveform$of$LAB$based$LS$˖ 慬䏝WT⯔ꆀLight*yield*ra9o*of*each*PPO*concentra9on*to*PPO3g/L*˖ 慬䏝WT儗㹀侧

Mean*waveform*around*100P.E.s*of*each*PPO*concentra9on

There$is$a$tendency$that$waveform$becomes$wider$as$PPO$concentraGon$is$d
There$is$a$possibility$that$PSD$capability$of$diluted$LS$becomes$worse.$
22

$IFSFOLPW‫׷״ח‬磛㶨陎ⴽ
Cherenkov vs scinti (LAB+0.03g/l b-PBD )Relative hit timing w.r.t. cosmic trigger
scintillation
Cherenkov

2” PMT
Cosmic µ

Scinti+Cherenkov
Scinti only

Blue; diluted scinti
Red ; scinti for trigger

scintillation
Cherenkov

Cosmic µ2” PMT(ns)•BS9JW
Clear excess around fast timing from direct Cherenkov light are seen.
23

8
25
6

20

4

15

$IFSFOLPW‫׷״ח‬磛㶨陎ⴽ
10

2
0

5

0

0

50

0

50

˖ 굲騊倯ぢ‫⟎׾‬㹀‫ג׃‬ծ錁庠ׁ‫׋׸‬岚䕎䞔㜠‫׾‬鐰⣣‫׷ׅ‬62

0.882628

SBXIJUUJNF
$IFSFOLPW
12
SBXIJUUJNF
TDJOUJMMBUJPO10PCTFSWFEHFOFSBUFE8UFNQMBUFGPSUSVFEJSFDUJPO
6

30
25
20
15

4

5

2
0

67

50
0.004046

̥χO144.5, -147.9 : g=323, n=449

0

150

0

50

550

100

25
20
15

0

50

500

50
450

0

− 50

10

− 100

5

− 150

0

0
0

50

χĕ

0

BTTVNFEħ<EFH>

10

0.028032

0.867077

14

35

47

37

400

.$USVF
50

100

−
350

−

150

BTTVNFEĚ<EFH>

135.9, -69.5 : g=423, n=1589
42

0.043176

177

0.00462624넝ְ넝鸞⚥䚍㶨ꤐ⿠腉⸂‫׾‬䖤‫ח׭׋׷‬˖ 岚䕎鐰⣣儗‫ח‬$IFSFOLPW‫גִ⸇ח‬14%‫⸇׾‬㄂‫ֿ׷ׅ‬‫דה‬ծOĕ‫ⴓך‬ꨄ‫ח׵ׁכ‬葺ֻ‫׷ז‬
Ը$IFSFOLPW 14%‫חⰟכ‬岚䕎䞔㜠ָꅾ銲˖ 넝礵䏝 넝⥋걾䏝‫ז‬XBWFGPSNEJHJUJ[FSָ䗳銲˖ &,050㹋꿀‫ך‬.)['"%$ USJHHFSCPBSE
˖ $"&/.)['"%$25

‫‪圓䟝‬ךٖؗؒז‪⦐➂涸‬‬‫‪鯄欽‬ךٖؗؒך‪̔,050‬׋ג׏װ׮ٖؗؒד‪˖ ,050‬‬‫‪ٕ侧_ +4/4 խխ_ ,050‬ط‪ٍٝ‬ث ‬‫‪ .)[ CJU‬‬‫‪٦‬زك ‪٦‬ؖٔز‪٦ㄤ‬ؘٕطؒחⰟ‪٦‬ؖٔز‪ -‬‬‫ח‪٦ٝ‬ةػכְ‪侧䧴‬زحؼ׾زحؽ‪♧鿇‬ך‪٦ㄤ‬ؘٕطؒ‪ծ‬ח׵ׁ ‣‬‫‪̔UPUBM&WTIJU1.5‬ג‪䔲‬׶ⶴ‬‫‪ؐؑ،‬س‪٦‬ع‪‬׮‪-‬גׄ‪䘔‬ח‪ 䗳銲‬‬‫‪ğ‬‬‫‪O ĕ‬‬‫‪26‬‬

4VNNBSZ
˖ +1"3$.-'‫ُصٕ؎ٓذأךד‬٦‫ظٔز‬䱱稊
 3$4.8‫ؽך‬٦‫׾ي‬欽ְ‫׋‬㣐䓼䏝‫ُص‬٦‫ظٔز‬彁 -4/%㹋꿀‫ך‬湫䱸涸‫ז‬鷄嗚鏾
 'MBTI"%$ (EⰅ‫׶‬巉‫ء‬ٝ‫וז‬嫰鯰涸倜‫ְ׃‬䪮遭‫׾‬欽ְ‫׋‬嗚⳿㐻˖ 넝ְ넝鸞⚥䚍㶨ꤐ⿠腉⸂‫׋ִ⪒׾‬嗚⳿㐻
 14% $IFSFOLPWְ‫׮׸׆‬岚䕎䞔㜠ָꅾ銲

27