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PACS numbers: 01.30.Mn, 01.30.Pb, 02.60.Cb
Keywords: 7'>íß, q'a$íýa³ð>, ïo`¦o j˵, BÛ¼Bw, @/líH¨8
I. " e  ] Ø
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rt putH 3lwôÇ. Óüto<Ƹ[þtÉr Óüto<Æõ_ :
x&h s:r<Æ_þv,¦1pxú<Æ, (ÉÓ' áÔÐÕªÏþ<Æ_þv,þjH
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H high-leveláÔÐÕªÏþs%3 [7,8]. sH Óüto<Ƹ[þt\
>
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Ér Oregon@/<Æ_ Zimmerman§Ãº %6£§s [9]. Õª Ê
ê ´ú§Ér @/<Æ\"f &hܼР<ÊÉr ÂÒìr&hܼРBÛ¼Bw
rÛ¼%7`¦ §õîr%ò\ &h6 x ¦ Ö¸6 x H ½¨ Ö¸ µ
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rÓýtYUs õ\¦ µ1ϳðôÇ e [11]. s\
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Ð sK ½+É Ãº eHBÛ¼Bw rÓýtYUs õ\¦]jr
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Ð sK ½+É Ãº el M:ëHs. @/ÂÒìr §F_ F'p =åQÂÒìr -87-
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ÊÉréß"é¶_ F'p t} ÂÒìr\"f ÀÒ#Q t¦ e6£§Érs ]
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H<Æ, t½¨Óüto<Æ 1px¸H%ò%i\"f ïo`¦o j˵`¦ ׿כ¹
> ÀÒ¦ e [6,13–16]. ÕªX< @/ÂÒìr &³©`¦[O
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II. R å ¾ ËV R Ë Ò ÷ »4 ; c" e § S ê sU m Æ
U Ø Ò ÞU ê sX N ËÅ k Ä
t
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ü
t)a. t½¨'a$íýa³ð> (½Ó$í)\ @/ # #îîr1lxëß ô
Ç Õª|½Ótîß L0 = 12mv02− m ~W (t).~r0− U s ÷&
¦, s\ @/ôÇ Õª|½Ótîß ~½Ó&ñddtd(∂L∂~v) =∂L∂~rÉr [3]
md~v0
dt = −∂U
∂ ~r0 − m ~W (t) (1) s
)a. #l"f ~W = d ~dtVH'a$íýa³ð> K0\ @/ # îr 1
l
x H K’ýa³ð>_ #î 5Åq¸s. −m ~W (t)H |9|¾Ó m{9_ 5Åq¸ d ~dtv0ü< ~½Ó¾Ós ìøÍ@/e`¦·p. sH
Ðl j˵ (©§4,<ÊÉr'a$í§4)s 6 xHd`¦·ú ú e.
s
]j K’ýa³ð>ü< "é¶&hs °ú ¦ K’ýa³ð>\ @/ # y5Åq
Fig. 1. Change in a vector produced by an infinitesimal clockwise rotation of the vector.
¸ ~Ω(t)Ð r H K ýa³ð>\¦ 2[ôÇ. Kýa³ð>H
² D
G'a$íýa³ð>K0\ @/K"f #îîr1lxõ rîr1lx`¦ H q
'a$íýa³ð>s. K’ ýa³ð>\"f_ 5Åq¸ ~v0Hýa³ð¨8
\
_ # ~v0= ~v + ~vrot= ~v + ~Ω×~rs)a. #l"f ~vrot= Ω × ~~ rHrýa³ð>\"f ÁºôÇè 7'¨8d~r = ~dΦ × ~r`¦ tÐ pìrôÇכ s. Fig. 1\"f d~r = ~dΦ ×~r_ 7'íß`¦ SX
K Ð ~1> ·ú ú e [1–5]. Õª|½Ótîß L’_ v’@/
\ ~v+~Ω×~r\¦@/{9 # &ño Kýa³ð>\"f Õª|½Ó t
îß LÉr L = 12mv2+m~v·~Ω×+12m(Ω×~r)2−m ~W (t)·~r−U H
dܼРK ýa³ð>\"f_ Õª|½Ótîß ~½Ó&ñdÉr md~v
dt = −∂U
∂~r − m ~W + m~r ×~˙Ω+2m~v × ~Ω+m~Ω×(~r × ~Ω) (2) s
)a. 0A_ îr1lx~½Ó&ñd\"f rM:ëH\(~Ω) ÒqtlH'a
$í
§4Ér[j>h_ ½Ós. ëß{9 r y5Åq¸ {9&ñ m~r ×~Ω`˙¦Áºr½+É Ãº e. ÕªQ'a$í§4Ér 2m~v × ~Ω + m~Ω × (~r × ~Ω)s. #l\"f 2m~v × ~Ω s ïo`¦o j˵ s
¦ m~Ω × (~r × ~Ω)s "é¶d§4s. 7'd`¦ Ð ïo
`
¦o j˵Ér ~vü< ~Ω\ úf~½Ó¾Ós¦ "é¶d§4Ér ~Ω~½Ó¾Ó\ @/
# úf~½Ó¾ÓܼРH~½Ó¾Óe`¦·ú ú e. t½¨H
×
æ§4 (J$[>`¦~ÃÎ6£§Ü¼Ð d 2\"f −∂U∂~r = −m~gs. # l
"f ~Ω\ 'a>)a 'a$í§4`¦ K$3 l 0A # #î 5Åq
¸ ~W \¦Áºr d 2H
md~v
dt = −m~g + 2m~v × ~Ω + m~Ω × (~r × ~Ω) (3) s
÷&%3. ĺoHs ~½Ó&ñd`¦BÛ¼Bw rÛ¼%7\"f Ã
ºu&hܼРۦ¦ ôÇ. Óüto<Ƹ s]jt_ [O
"
î`¦ &ñSX > sK½+É Ãº e#Q ôÇ. SXs t ·ú§
H Óüto<Ƹ 7á§8 ©[jôÇ ?/6 xÉr·ú¦ H 1lqH
%
i<ƧF\¦ÃЦ l êøÍ [1–5]. {9éß Õª|½Ótîß îr
1 l
x~½Ó&ñds ½¨K &Ç 6£§Ü¼Ð s ~½Ó&ñd`¦ &h]XôÇ ~½ÓZOܼ
Ð Û¦)a. Fig. 2\"f ÐHü< °ú s ~ΩH 0A¸ θ_
<ÊúРω[t ]={−ω0Sin[θ], 0, ω0Cos[θ]}s. t½¨ y 5
Å
q¸ ω0_ ß¼lH [5,19]
ω0 = ( 2π
24 × 3600)(365.2564
365.2422) = 7.292 × 10−5sec−1. s
. 0A\"f 'Í P:Fc ñîßÉrIª\ @/ôÇ t½¨_ y
5Åq¸ s¦ ¿º P:Fc ñ îßÉrIª¸\ @/ôÇ ½Ó$í¸_ q
°úכs. t½¨³ð©_ ôÇ t&h\"f |ÃÐs #QÖ¼ ~½Ó¾Ó Ü
¼Ð #Q" [jlÐ ÂÒÖ¼\ ïo`¦o j˵s &ñ÷&
Ù
¼Ð s\¦ro # ³ðr l 0AK"fHþjèôǸ 6>h _
Ä»¸\¦°úH îr1lx`¦ ìr$3K ¦ y5Åq¸,0A¸,
| Ã
Ð_ 5Åq¸ 1px¸¹¡§Ãº[þts <Ê\ ïo`¦o j˵s
˨#Q . sp [O"îôÇX<Ð ~Ω H θ_ <Êús¦ 3>h_
$í
ìr`¦°ú¦ e¦ ~r[t], ~v[t]¸ rçß yy 3 $íìr`¦°ú¦ e
#
Q"f m~vr× ~Ωõ m~Ω × (~r × ~Ω) _ 7'>íßs ï /'îr
\Os m. sü< °ú s Ä»¸ ´ú§Érrçß_ <Êú > í
ßÉr Óüto<Ƹ[þts © 6 x l ¼#oôÇ >íßrÛ¼%7ܼ
Ð"f BÛ¼Bw\¦s6 x ¼#o [7,9,10]. #l"f 0
A_ ¿ºd`¦>íß HBÛ¼Bw "î§î#QHÐ
In[4]= fCoriolis = 2 m Cross[r’[t],ω[t]];
In[5]= fCentrifugal =
m Cross[ω[t],Cross[r[t],ω[t]]]
//Simplify]
s
. u 7'd`¦Z zH+þAIÐ "î§î#Q\¦+ ?/9
)a. BÛ¼Bw "î§î#QCross[r’[t],ω[t]]H ~r0[t]×
ω[t] \~ ¦ ³ðr ¦ e6£§`¦·ú ú e. Óüt:r ~r[t], ~r0[t][þtÉr
~
½Ó&ñd`¦ Û¦#Q"f ½¨ # ôÇ.
1. Rå¾ËVRË Ò÷»4;c"e §SêsUm UêsXNËÅkÄùp§ þsÚM
üX¢ 8080X ³zº§q
ïo`¦o j˵\¦ í<ÊôÇ 'a$í§4[þt`¦ ~ÃÎH Óüt^_ îr1lx
~
½Ód, 7£¤ d 3`¦ Û¦l0AôÇ BÛ¼Bw áÔÐÕªÏþÉrBÛ¼ B
w "î§î#Q\¦ ·ú ~½Ó&ñd`¦ Z zH dܼР$í½+É Ã
º e. ÕªQ áÔÐÕªÏþ $í\ s \Oܼ /BN>h)a MathCodes\¦Ö¸6 x Bĺ ¼#o . A_ áÔÐÕªÏþ
Ér Zimmermans $íôÇ Wolfram library (4539) [8]`¦ Õ
ªX<Ð îr~ÃÎ &h]Xy ú&ñ # $íôÇ כ s. s\
Ér>íß rÓýtYUss ro áÔÐÕªÏþÉrĺo Dh
Ð $íôÇכ s. X<s'\¦ëß[þt#Q Hõ&ñ`¦ [þt#
^
¦Ãº e> èÛ¼ áÔÐÕªÏþ_ {9ÂÒ\¦#l\ ]jr %i.
q
2¤BÛ¼Bw\ e¸nq t 3lwôÇ Óüto<Ƹ[þt¸ BÛ¼B w
"î§î#Q Óüto6 x#Qü< f¨ l M:ëH\ ~1> áÔÐÕª
Fig. 2. Rectangular coordinate system on the rotating earth with a angular velocity ~ω0.
Ïþ
ï`ç`¦°ú ú e`¦כ s. s 7HëH\"f BÛ¼Bw
"î§î#QHInputü< °ú s, ئ§4ÉrOutputü< °ú Ér W^
Ð ?/%3. áÔÐÕªÏþîrX< "î§î#Q Cross, Series, Table,Solve[þts #Q" _pt f ½+É Ãº e [11,12].
Fig. 2\"f ÐH ü< °ú s, y5Åq¸ ~ω0Ht½¨_ »¡¤
`
¦ ׿dܼРr Hrýa³ð> 0A_ 0A¸(π2− θ)©\
"
f X-Y-Z ýa³ð>\¦0Au 7'ü< y5Åq¸ 7'\¦rçß t_
<ÊúРBÛ¼Bw\"f 6£§õ °ú s &ñ_ %i.
In[1]:= r[t ]={x[t], y[t], z[t]};
In[2]:= ω[t ]={−ω0 Sin[θ], 0, ω0 Cos[θ]};
'
a$í§4 fInertial, ïo`¦o j˵ fCoriolis, "é¶d§4 fCentrifugals 6 x Hrýa³ð>\"f_ Õª|½Ótîß
~
½Ó&ñd d (3) `¦ Û¦l 0AôÇ BÛ¼Bw ï`çÉr [9]6£§ õ
°ú .
In[3]= fInertial = {0,0,-mg} ;
In[4]= fCoriolis = 2 m Cross[r’[t],ω[t]];
In[5]= fCentrifugal =
m Cross[ω[t],Cross[r[t],ω[t]]]
//Simplify]
In[6]= eq1 = - r’’[t]- fInertial -fCoriolis- fCentrifugal
In[7]= eq2 =(Series[eq1/m, {t,0,nOrder}]==0 /.initialRule//Normal//Thread //Simplify
In[8]= vars = Table[D[{x[t],y[t],z[t]},{t,i}]
,{i,2,nOrder+2}]/.t->0 //Flatten
In[9]= sol =Solve[eq2,vars]//First
In[10]= inertialRule = Thread/@r[0]->0, r’[0]->{1,0,0}//Flatten
In[11]= point[t ,θ ]=Series[r[t],{t,0,nOrder+2}]
/.sol/.initialRule//Normal]
Out[11]={t,-t2ω0 Cos[θ], −gt22 }
d
(3)`¦ ÕªX<Ð BÛ¼Bw ï׼Р` |כ s In[6]=,
In[7]s¦ s_ /åLú KH In[7]=eq2\ _K ½¨K .
s
/åLú KH t=0\ @/ # 2 t /åLú>hôÇ °úכܼ
Ð In[7]\ ³ðrôÇ ü< °ú s 2 ½Ó s©_ \Q ½ÓÉr Normal_ "î§î#QÐ Áºr ¦ H%o ôÇ כ s. íl
¸| °úכ (initialRule)õ 5Åq¸\¦ ½¨ point[t ,θ ]\ _
K 0Au 7' ~r[t] rçß_ <ÊúР½¨K . s ü
<°ú s point[t ,θ ]<Êúëß ½¨Kt In[21]=plot[θ ]:=
ParametricPlot[point[t,θ][[{1,2}]]\¦ s6 x # Fig.
3`¦ %3`¦ ú e. r[t]_ 3>h_ 7' $íìr°úכÉr Out[11]\
"
f Ð ü< °ú s{t,-t2ω0Cos[θ],-g2t2}s.
In[21]=plot[θ ]:=
ParametricPlot[point[t,θ][[{1,2}]]
/.{ω0 ->1,g->9.8}//Evaluate,{t,0,20}
,DisplayFunction->Identity];
{plot[π/4],plot[π/2,plot[3π/4]}
//GraphicsArray//Show;
{9
éßpoint[t ,θ ]s ½¨K&ܼټР0A¸ (π/2−θ)\ ,
ry5Åq¸ (ω)_ ß¼l\ , |ÃÐ_ [jlü< ~½Ó¾Ó\
Óüt^_ îr1lx`¦K$3 ¦ f'ao l 0AôÇ rÓýtYUs
s 0px > ÷&%3. Fig. 3Ér&ñzܼРÓüt^\¦Ãº¨îܼ
Ð ~|9 M: (vx=1), ·¡¤ìøÍÂÒ (π/4)ü< z ìøÍÂÒ (3π/4), Õª o
¦ &h¸©\"f Óüt^_ îr1lx &h`¦rÓýtYUsôÇ כ s
. BÛ¼Bw rÛ¼%7\"fH0A_ ÕªaË>`¦|ÃÐs '
~
½Ó¾Ó`¦ ØÔv¸2¤ ~1> EmBjs ½+É Ãº e6£§Ü¼Ð y© _
׿\ s\¦rK ÐsHכ ¸ Bĺ ´òõ&hs [17].
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¤ìøÍ½¨\"fH r>~½Ó¾ÓܼРzìøÍ½¨\"fHìøÍr> ~½Ó¾Ó Ü
¼Ð ¼#¾Ó÷& 9 &h¸©\"fH ¼#¾Ó÷&t ·ú§6£§`¦ ^¦Ãº e
. 3 "é¶ ÕªAi`¦ 0AK"fH point[t,θ][[{1,2,3}]]`¦
½
¨ # ParametricPlot3D[point[t,θ]\¦ s6 x 7á§ 8
z´&h rÓýtYUss Ð# ÅÒ ´òõ&hs.
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Table 1. Calculations of the apparent forces over the earth surface in the vector calculation The calculation parameters:
ω0 = 7.292 × 10−5sec−1,v0x = ±10.0m/s,g = 9.8m/sec2, t=5 sec.
Coriolis acceleration(m/sec2) Centrif ugal acceleration(m/sec2) Gravitational(m/sec2) θa
Xb Y Z X Y Z X Y Z
π/8 ↓ −9.0772 × 10−7 −1.3473 × 10−3 −3.7599 × 10−7 4.5386 × 10−7 0.0 1.8799 × 10−7 0.0 0.0 -9.8 2π/8 ↑ 5.3173 × 10−7 1.0312 × 10−3 5.3173 × 10−7 −2.6586 × 10−7 0.0 −2.6586 × 10−7 0.0 0.0 -9.8 3π/8 ↓ −1.5574 × 10−7 −5.5810 × 10−4 −3.7599 × 10−7 7.7870 × 10−8 0.0 1.8799 × 10−7 0.0 0.0 -9.8 4π/8 ↑ 3.9870 × 10−39 8.9288 × 10−20 6.5116 × 10−23 −1.9936 × 10−39 0.0 −3.2558 × 10−23 0.0 0.0 -9.8 5π/8 ↑ 1.5574 × 10−7 −5.5810 × 10−4 −3.7599 × 10−7 −7.7870 × 10−8 0.0 1.8799 × 10−7 0.0 0.0 -9.8 6π/8 ↓ 5.3173 × 10−7 1.0312 × 10−3 5.3173 × 10−7 2.6586 × 10−7 0.0 −2.6586 × 10−7 0.0 0.0 -9.8 7π/8 ↑ 9.0772 × 10−7 −1.3473 × 10−3 −3.7599 × 10−7 −4.5386 × 10−7 0.0 1.8799 × 10−7 0.0 0.0 -9.8
a↑wind direction to north, ↓ to south
b± deflection to east(+) or west(-) direction respectively
Fig. 4. Calculations of the Coriolis deflections on the six latitudes on the earth. The winds (a)toward the the South and (b) toward to North. The Coriolis force deflects to the right in the Northern hemisphere and to the left in the Southern hemisphere when viewed along the line of motion.
Ér ëH"f\¦ ÃЦ l êøÍ [6, 13]. ĺoH s °ú Ér 3-Cell¸4Sq\ lí # yy_ @/lݶ %ò%i\"f [O&ñ)a
|ÃÐ_ ~½Ó¾Ó`¦ l:rܼР# y %ò%i\"f ïo`¦o j˵
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Table 2. Calculations of the apparent forces varies from city to city.The calculation parameters: ω0 = 7.292 × 10−5sec−1, g = 9.8m/sec2, t=5 sec. Minus sign stand for the north direction of the wind in a the unit of m/sec at the city.
Coriolis acceleration(m/sec2 ) Centrif ugal acceleration(m/sec2 ) Gravitational(m/sec2 ) City(± v0x)
X a Y Z X Y Z X Y Z
Nome(0.902) −7.8311 × 10−8 −1.1890 × 10−4 −3.7218 × 10−8 3.9155 × 10−8 0.0 1.8605 × 10−8 0.0 0.0 -9.8 London(-0.783) 5.0997 × 10−8 8.9365 × 10−5 4.0568 × 10−8 −2.5498 × 10−8 0.0 −2.0284 × 10−8 0.0 0.0 -9.8 New York(-0.652) 2.9439 × 10−8 6.1958 × 10−5 3.4272 × 10−8 −1.4719 × 10−8 0.0 −1.7136 × 10−8 0.0 0.0 -9.8 Atlanta(-0.555) 1.8234 × 10−8 4.4989 × 10−5 2.7271 × 10−8 −9.1174 × 10−9 0.0 −1.3635 × 10−8 0.0 0.0 -9.8 Panama( 0.157) −4.0859 × 10−10 −3.5818 × 10−6 −2.5797 × 10−9 −2.0429 × 10−10 0.0 1.2898 × 10−9 0.0 0.0 -9.8 Sydney(0.559) −1.8556 × 10−8 4.5547 × 10−5 2.7546 × 10−8 9.2782 × 10−9 0.0 −1.3773 × 10−8 0.0 0.0 -9.8 Daejon(-1.50) 5.6163 × 10−8 1.2980 × 10−4 7.6189 × 10−8 −2.8081 × 10−8 0.0 −3.8094 × 10−8 0.0 0.0 -9.8
a± deflection to east(+) or west(-) direction respectively
Fig. 5. ParametricPlot3D of the deflections by the Apparent forces: (a)None Apparent force (b) with the Apparent gravity (-mg), (c) with the apparent gravity and the centrifugal forces, (d) with the gravitational,centrifugal and Coriolis force. All the cases, the angular velocity ω0 varies according to the list of {0,0.002,0.004,0.006,0.008}. All the cases of flight line are degenerated for the ω0 except of (d)case.
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Fig. 6. ParametricPlot3D of the deflections due to the Coriolis force at the latitudes of θ = π4 and θ = 3π4. The values of the angular velocity increasing with the thickness of the flight line of the winds. Both the cases, the angular velocity ω0 varies according to the list of {0,0.002,0.004,0.006,0.008}.
Fig. 7. Circulation of the atmosphere due to the Coriolis force and centrifugal and gravitational force to the earth.
In left column, the calculated wind directions in the specific region of the earth match to the winds in the region over the earth surface. Last character of the abbreviations in the figure shows the wind names: W for westerlies, T trade winds, PE polar easterlies respectively.
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[1] Keith R. Symon, Mechanics (Addison-Wesley, Reading, Massachusetts, 1971), p. 279.
[2] J. B. Marion, Classical Dynamics (Academic Press, NewYork, 1970), p. 343.
[3] L. D. Landau and E. M. Lifshitz, Mechanics 3rd ed.
(Pergamon Press, Oxford, 1976), Sec. 39.
[4] R. P. Feynmaa, R. B. Leighton and Mathew Sands, Lectures on Physics (Addison-Wesley, Read- ing, Massachusetts, 1963), Chap. 19.
[5] Herbert Goldstein, Classical Mechanics 2nd ed.
(Addison-Wesley, Reading, Massachusetts, 1980), Chap. 4.
[6] C. D. Ahrens, Essentials of Meteorology 3rd ed.
(Brooks/Cole, Pacific Grove, CA, 2001), p. 180.
[7] http://www.wolfram.com/solutions/highered/.
[8] http://library.wolfram.com/infocenter/Books/4539/.
[9] Rovert L. Zimmerman and Frederic I. Olness, Math- ematica for Physics (Addison-Wesley, San Fran- cisco, 1995), Chap. 2.
[10] Partric T. Tamm, A Physicist’s Guide to Mathemat- ica (Academic Press, San Diego, 1997), Chap. 4.
[11] H. J. Yun, SAEMULLI 40, 530 (2000).
[12] H. J. Yun, SAEMULLI 50, 1341 (2005).
[13] http://csep10.phys.utk.edu/astr161/earth/coriolis.
html/.
[14] http://www.earth.nasa.go/history/goes/goes.html/.
[15] http://helix.gatech.edu/Classes/ME3760/1998Q3/
Projects/ Fortgang/calculation.html/.
[16] Anders Person, Bull. Amer. Meteor. Soc. 79, 1373 (1988).
[17] http://home.mokwon.ac.kr/∼heejy/hanimationn82.
nb,hanimatins86.nb.
[18] http://www.kma/go.kr/kor/weather/climate/.
[19] Korea Astronomy Observatory, The Korean Al- manac for the Year 1998 (Nam San Dang, Seoul, 1998), p. 90.
Mathematica Ssimulations for the Analysis to the Coriolis Force in a Non-Inertial Frame of Reference
Hee-Joong Yun∗
Department of Optical and Electronic Physics, Mokwon University, Daejon 302-729 (Received 29 September 2005, in final form 13 January 2006)
The coriolis force is an important factor which allows calculation of the apparent effects on atmospheric flow when viewed from the rotating earth and is elemental in solving the Lagrange’s equation in a non-inertial frame of reference. To analyze the effects of apparent forces on the frame, we solved Lagrange’s equation numerically with Mathematica and visualized the vector calculations of the effects of the Coriolis force on the flow near the earth’s surface in order to improve the teaching and learning of physics in the senior year and to enhance enhancing the ingenuity of students. This forms a fundamental basis for analyzing the 3 Cell model of air circulation near the earth’s surface.
PACS numbers: 01.30.Mn, 01.30.Pb, 02.60.Cb
Keywords: Apparent forces, M athematica, Coriolis force, Atmosphere flow.
∗E-mail: [email protected]