$"^o7SE4"caE)9Xtbn\Vh!R (2<FzPQRSTUVWXYZ\jNUM5d n#GajMZ~SI1nucovMMM9?DLIMvMLIM[HLIMpNUCOMPPP9PPP4.P4"RIF"dAMAJAMIDMADMI,;h 6@)J/T^ArG|5lMTT9cJ0[JJ1amygBANDsSP7duPIR9?&, 0]W7A9 :B2D!B3N;A1'X3b Q7KvA5Q-M5]iWD5o{WM6u A6 A0MB0  *4>HJ6RJ5\ fpzC0#LD0)E0A/z;ocR5i$KV7R.zK5 B8tBYLXV`j~LA8C1 oA2X1 Y1J'h-3!9?EQu(W ci2<{F6 X9PZY9dnZ Z9xA3B7) ",A6@^T#^/r5|MGit G7X:r G^M SG9&0DNXblvQ F@:(>]i (L0B L1o1 R6W8u {*4 TH L7RL6\fpz@M7 C5 C64N0 V6 E7". N6:F R X Wd$ p. b N1|8 N2B wO1L O5V  L5` j n X5t : Y7~ t Y5 , Z3 Z5       X2  Y2    & X3  YY3$  *  0  < ( H 2 W5T < ` F f P l Z x d ~ n N W6 x  D9  X P1  S0    W0       BD6        d D7 "  2 6  > @  J J P T  \ ^ E8z r 8 h | S8D Q8  h   P9V     QH7  ( T9 T8  Q   n     V12 V  R1  qP8     uG0&  h H0, & 8 0 EI8> : D D J N \ I0V X b b n l t v P N8z     B G1   H1  I1       H2  I2  G2    * 4  A4 > D4 H  R " \ . f 4 p @ z R  F  L  DD1p  ^  U8v   W9  j   |  !t5  E6   $ y F6 . 86 L BM9K8 NDIAM ORADI PMASAT QaMEGAT% VI `O jnomU t ~o MOM+ m MM9< g D[ a FF6    <  s i JJ0       ( 2C J1 F P ZkKx \ ,F&g[OUD82>mys"E,6@M1JT^hr|4CB1W1nT1S1 &MT2,28>&D0J:PDVN\Xbbhlnvtz8  ,*H>Rf2pnumerito>Gnombre& hDnPxJV\}hbwGvalor ya I=1%+O7UCmx[gs         !!-!!!!!!9##'####3#!#?%KPWZcdinux]ÁÇgv}SL{hɫoͥßÙ÷ñĽ",6h@JT^ r|#)/;AGM5YekS_q}Ń&ŭ0ŏ:ʼnXŕDwNśbšlŧvŹſų % +* 4>7CHIR1 O\(=fUp[zagmsyƋƅƑƗƝƣƩƯǻǵ$.8BLV`jt ~3'!K-?9Q2W<]FcPiZEodȟnux{ȁȇȍȓșȥȫȱȷȽ/",6@JT)^ɞ LmHDIFM_DIFD;rA|MYSɦLO055 DIFLqɏeԉɛNNJ_ɧwk̓}ɡʭʳ&ʹ0ʿ:DNXblv %+17= CI O*U4[>aHgRm\sfypz˅ˋˑ˗˝˩ˣ˻˵˯$.8BLV `jt~!'-3i?EKQW]9co ú{(͇2͍<͓FP͙Z͟dͱxͥnͷͽͫ8 ",#6)@/J5T;^AhSre|w΃ΉΏΕΛιGBGAHBVHAIBIA*KTRT&6RW0:DP DrDTNZNM%X+b1l7v=CINVTOg mtUa[υysmgϋБ ЗН У*Щ4Я>еHлR\fpBzU[T550 6ЋDMES$gVIs<Нaccc*ccdymё$ѵjї.VBѣLѩ`t~ѯѻ  !'32-(9< J9$H0R<\HfTp`zflwV2} V3CQՙSQՍSPՏտPՕ I5. Z2$.8BX C3LC2 VTN` jTI&t,~28>JPLA0]io{և֓֫CV֥COE J VV׼ E2( E32׀ Q2<Q3FPw UZdnx   ױ ׫     % 70000Q 70010 tui ARRderMESARSdar_ carcar2LMAXLMINLAMAXLAMINNC 68000 ` THEN70000 mt5dt5marsup infriesriesg my5MADMI,;h 6@)J/T^ArG|5lMTT9cJ0[JJ1amygBANDsSP7{V\s6bmINFORTECNICA 2002"Nhm Lepanto 422"jnmBarcelona 08025tmTel. 934334243 / Fax. 934334239"zmWebsite - www.sadeya.orgm,INFORTECNICA SERVICIO DE CALCULO Y SOFTWARE:2m,ESTUDIOS ESTADISTICOS, ASTRONOMIA, ROBOTICA,vm8ESTUDIOS DE MERCADO, INGENIERIA, MECANICA, TEC. MILITAR,m;ARQUITECTURA, CALEFACCION, ANTENAS PARABOLICAS, MATEMATICA,"mEPROGRAMACION LINEAL, AERONAUTICA, ASTRONAUTICA, GEODESIA, TECNOLOGIA,"Zm=RESISTENCIA DE MATERIALES, FISICA, METEOROLOGIA, CARTOGRAFIA,"m&Solicite informacin sin compromiso. m5CALCULO (1) AJUSTE FECHA IMPACTO (2) AREA IMPACTO (3)" d ^ d ^ mPULSE UNA TECLA"">m EFC2000.DAT"djd"  de@Vh fts< d m: ***NEOS POSIBLE RIESGO. VALORAR SOBRETODO NO NUMERADOS***#e2 )D1m+LIMITE DE DISTANCIA ENTRE ORBITAS SUG 0.001" 7~?m!LIMITE DE MESES TIERRA-NEO SUG .8" EMmMAGNITUD H MAX. SUG 40 S[m'NUMERO DE RADIANTES A ESTUDIAR SUG 7000" a*jm/NUMERO DE EFEMERIDES PARA CADA RADIANTE SUG 750">p vd~mINTERVALO EN DIAS SUG 1=x   mAPARA EL TOTAL DEL CIELO PULSE (1). PARA UN SECTOR DETERMINADO (2)" eZ eZx ed edx " d^jm;PODRA ESTUDIAR SI EXISTEN RADIANTES EN UN SECTOR DEL CIELO."m=MARQUE LOS LIMITES DEL SECTOR. ASCENSION RECTA MAXIMA (HH.MM)" mASCENSION RECTA MINIMA (HH.MM) (mDECLINACION MAXIMA (GG.MM) ZmDECLINACION MINIMA (GG.MM) mTIEMPO DE LA EFEMERIDE INICIAL "sY     ")/ NUCOM=1505m%EFEMERIDES ECUATORIALES EQUIN. 2000,0"V;d}m;NEOS CON POSIBLE RIESGO. VALORAR SOBRETODO LOS NO NUMERADOS"AmJt.NEO A.R.(Radian)Dec. E. Moid. r. Long T. V/inf. V/imp. Mes T. D.mes Gd}mLt.NEO A.R.(Radiante)Dec. Dis.orb. r. Long T. Vinf.Vimp. MesT. D.mes EqC. M d   d SD [ PRINT #1,P ad gh m  a_]r [sr yY lPERT! @  e   d g [  eh eh&w  d%     &w   d p p  o( e : mAO=N  ` mMES=t   mDIA=  ! ' d _^- 3e  9 ? dw E K E  Q 9  - ed& W" ]d Ww Wd& cb ikC p&kA dnp& !lB:A | o lS@AA_^u {o u  c  [{ mJD="  dN mFECHA JULIANA=    k?   & J  l@}YiFoZie   Xeh Xeh&wnehp  eZ&d  eZ eZ&wneZp     Gp   M Gp  k@_^, k?@_^B k?_^L[\  l  u   p  pO G u ep   kw+2x_^!' dc^--e  X3o! X 9o?mX=0E K@QmY=TW ]dcmZ=xi ouY{mA" mB" mR" GdN{ K  ] uY X  G  o uY* X 2o\mDE POLARES A CARTESIANAS:A="p mB= ^mR= MYAmX= mY= umZ= dN  $ dxp u,o@ dxp T  dxp u\op dxp ~  uo  #  u)o/mDE GRADOS A GMS: GRD="5 ;A ;dc^GM ;& S X ; Swne<p 90^ 9& dLi 9 dwne<p ort S ded oe' zzoY/mGRD= ;mG= SmM= dmS= omGMS= zdNG ;eh ;YMdx zp zo.mG=B SRmM=f dvmS= o S de< oe ; S ded oe' zomDE GMS A GRADOS"Y,mGMS= zmGRD= ;<dN^mCOORDENADAS DEL SOL"hYrY e   " p (m1.VER.=" mR= .mAR.APR.= 4m DEC.APR.=" :dN@Y Fo2  llBAwnkG LjQljMp@l]K_A Lpky8 Ld vpw W]lp|%{q@l@ Lpkݘ9 Ld vp ci c oYu  c{lJgv@lO@ LpkRI9 Ld vpw 9 9 Y&  9^l qr@llxze; A Lpk < Ld vp kް?k ; Lpwkj7 Ld vpw  e  9Mpk,* Y{L0  6 Z<  B pH k8 A . N T k9> . Z ` e ;f YAl z r x 6 e ;~ YA z 4 ! ; YA z  B ; YA* z 2 oF dxp P [ ZY d Y n Y x Y  Y   d^  [  k?   , d  wn & 2 Y8 > v D J  P [V \ d b  h n t wn b w L.z , <  F [ P [ ^ l M  p  X G Yi   u  G X Yi   u     u"& Y6, X 2  X@8 YiN>  \D u pJ  P V  \ b  h n \ t h uz Y X @ X Yi   u  P  K ]* o4 Y{B  P  d e ;n YA| z r  ; YA b d_^  k6<; Gp b   [h ! zk8 k(Cne n p ze nMpw  @! &k?  &wnp N!" G ( !. k8 k(Cne nMp  e n w !4 ehd% : !@ e : : &wnp : !F : &k? : : &wnp E"L Y"R dc^ :"  ed !e' X z"^ . .p ( ( p pwnd .p ( pn d "j d d d pwO d p d "p d d_^v "| e d  d #v p ( ( p . .pwnd p ( pn 0# d pwO p B# d_^ V# e  # d ( 0pd)0d) 0pd)0  # d)e wnk @nvO # epd  # dd kI@p d vp $ d k333Ad vpko:pk3D ($ d g g<$ g D _^M$ d e_ )c  Ec  E_  c  _ Sd]D%  mDIAm mE MEGAT" J% d e_ )c  Ec  E_  c  _ Sd]%d}  mDIAm mE MEGAT" % d e_ )c  Ec  E_  c  _ Sd]\&d}  mDIAm mE MEGAT" *& d e_ )c  Ec  E_  c  _]&d SB& d)p&d)  P&% e d^&+ e' 1 j'6 d e_ )c  Ec  E_  c  _]'m:####.#### ##.#### +##.### ###.### ###.### ###.# ###.# ##.# X E 1 p& 1  dp& d ( dp& d dp& d d d)p&d) d)p&d) '< d)p&d) B (I d e_ )c  Ec  E_  c  _])d}m:####.#### ##.#### +##.### ###.### ###.### ###.# ###.# ##.# X E 1 p& 1  dp& d ( dp& d dp& d d d)p&d) (O   (U [[ (V Ya (g Ym (s y t ( y t ( [[ ,) m#EFEMERIDES ECUATORIALES DEL COMETA "  m EQUIN. 2000,0|) d}m#EFEMERIDES ECUATORIALES DEL COMETA "  m EQUIN. 2000,0) mT= t m PERI= m NODO= 2 m INCL= m EXC="  m Q=" , m G=" z* d}mT= t m PERI= m NODO= 2 m INCL= m EXC="  m Q=" , m G=" * m:Fecha A.R.(2000)Dec. Delta r. Elon. F.A. Mag + d}m:Fecha A.R.(2000)Dec. Delta r. Elon. F.A. Mag+[  (+  n 2+ Y <+ [\ L+sdN`+ lQm? v+ k33s?_^ + lG?_^ + d wn + Lp k?xnvp d+ dK + dd pn d$, d d&wnd p p p d6, ddc^@,[X, dd p dd,d x,  d _^&,,[2,&dx ,2 d _^8,>[D,8d p dw d,D d  J,O d 1 -U h deV--[ J  JMpw a>-g J d awK 1 p JP-m 1 d  1 `-s h f-yd nd wnO - J p J-d Jd Mp Jd  p - d  J pwnp M-[ . dd% pnd)O 4.dd wnpdd% pn ^^.dd npdd% pnO .d p p Lpd p p pO .d .  p .d  . d M d   . K /  &/ dd nv p 6/  SZ/d d Sp pd SpM ot/ ^ op op /  c/d / k>_^ /  d dvp /& d dvp 0, lm4卑? p pw $02 k5y; d vpw D08 k : dvpw d0> k9 dvpw 0D k= 9 dvpw 0J kO8 dvpw 0P  cwkw+2_^0Vd 0\ d dvp  1b kL? dvpw .1h lY  g? d vp N1n k9y< d vp n1t kl; dvp 1z ka; dvp 1 k pf: dvp 1 kk9 dvp 1d O 1  p op  2dd  p pn  42d p Z2  pd pnp Md2[v2 dc^2[2 d p 2[ 2 mFUERA DE LIMITE"2dN2[ campo nombreL2d 3m nombre.txtd (3d tH4>3d \3  ]3   p3 d |3b33d  fin campo nombre3o3m Ya 3 d _^3 e  93& dw E3, E  42 9  4 ed& W>48d Ww Wd& c~4>kC p&kA dnp& !lB:A y 4D y lS@AA_^J4Po4J y c y 4V[P campo perihelio4 d 4\mperi.txtd 5bd tH6$5hd nB5w  ]5 n V5} d b5b55d  fin campo perihelio5o campo nodop5 d 5mnodo.txtd 5d tH65d n6  ]6 n 2 (6 d 46bv6Z6d  fin campo nodo|6o campo inclinacion6 d 6m inclina.txt"d 6d tH76d n6  ]7 n 7 d  7bN787d  fin campo inclinacionP7o campo E\7 d z7m campo_e.txt"d 7d tH87d n7  ]`8 n  7  d 7b"88d  fin campo E8o campo Q&8 d D8%m campo_q.txt"d V8+d tHJ9l81d n87  ]*9 n , 8= d 8Cb88Id  fin campo Q8Oo campo magnitudes88 d 9Um magnitud.txtd *9[d tH:@9ad n^9g  ]9 n r9m d ~9sb99yd  fin campo magnitudes9o campo ao9a d 9mao.txt"d 9d tH::d n0:  ]: n D: d P:b::d  fin campo ao campo mes:d :mmes.txt"d :d tH;:d n:  ]; n ; d ;bR;D;d  fin campo mes campo diaP;d j;mdia.txt"d |;d tHp<;d n;  ]P< n !; d ;b<; d  fin campo dia;o@<m6EFEMERIDES Y ELEMENTOS DE ESTRELLAS FUGACES (EQ.2000)<d}mG OH.T.E. A.R.(2000)DEC. Dista r. LONG. VELO. MES MET/H"mANO="> 4>mMES=H> Z>mDIA=n> !> d _^>e  9> dw E> E > 9 > ed& W>d Ww Wd& c6?kC p&kA dnp& !lB:A P? lS@AA_^X?ol?  c v?[?mJD=" ?N? mFECHA JULIANA=? ? k? ? & @# l@}Lkd Cllxze; A Lpk < Ld vp nLkް?k ; Lpwkj7 Ld vpw L e  9Mpk, . Z jQ e ;tQY3Q z r Q 6 e ;QY3Q z 4Q ! ;Q Y3Q z Q B ;QY3Q! z R'oR- dxp  R3[94RimPERI="HR? \REmNODO="pRK 2 RQmINCL="RW R]mEXC=Rc  Rim DIST.PER.=Ro , Ru  d^{S[S{k?  0S , d  wn & DSmMAG G=XS bSepSe D |Sd S[Sd b S n t wn LS , S  S[S S M T p  XT GTY*T  8T u FT GTT X^TYlT   zT u  T T uT#YT) X 2  XT/YT5  T; u TA Mw GUS _w YUe  qw k,Uwk< p }BU  bU dc]vV   U dc]V d p U Qd ]V ene n U Mx }p U   }p Vk?dkL7< kX9?w pn 6Vd kB`U@wMkpΈXa ]LXg oVXmYdXs  rXy  X e ;XY3X z r X ;XY3Y zk8 k(Cne n p ze nMpw  0Y &k?  &wnp >Y G ( Y k8 k(Cne nMp  e n w Y ehd% : Ye : : &wnp : Y : &k? : : &wnp EYYZ dc^-*Z9  ed !e' X DZ  !e VZd g gjZ g D _^Z IF gv = 0 THEN PRINT nom$, K8Z" IF gv = 0 THEN PRINT #1, nom$; K8Z Ed^Z  &d](\ e  [  w ([ d_]`\e w N[$ d vk333Ad vO *Y0[6  7c E _ Sc]\d}  m H, DIAM, MAS, MEGAT V0= $\<  7c E _ Sc]\]  m H, DIAM, MAS, MEGAT V0= \Bd k0c]Bcd ec k>c]hcd i 53512 IF DT < DLIM AND MLIM > DMES AND K8 < HLIM THEN PRINT #1, USING " #. # ##. # +##.### ###.### ###.### ###.## ###.# ###.# ##.# ##.# ###.##"; T55; INT(A6 * 1 0) / 1 0; INT(D7 * 1000) / 1000; INT(DT * 1000) / 1000; INT(R1 * 1000) / 1000; INT((L * 180 / PI) * 100) / 100; INT(VT * 10) / 10; INT(VI * 10) / 10; INT(MT * 10) / 10; INT(DMES * 10) / 10; ccd0c  7c E _ Sc]xed}mBRIESGO (0-5), FECHA, # #### ## ## <## ## >## ## X & .d d_  7c E _ Sc]ed}:dd ENda   Xdgjds Qd ^ydmT.PASO PERIHELIO="dYd  t dyd ew dm  d  n dYd[ed gd D e[9"elQm? 8e k33s?_^Re lG?_^le d wn e Lp k?xnvp de dK e dd pn de d d&wnd p p p de ddc^f[f dd p d&fd :f d _^Df[ Rfdx ff  d _^pf[fd p dw df d  Jf! d 1 f' h deVhf- J  JMpw ag3 J d awK 1 p Jg9 1 d  1 "g? h fDgEd nd wnO XgK J p JgQd Jd Mp Jd  p gW d  J pwnp Mg][cgdd% pnd)O gidd wnpdd% pn ^ hodd npdd% pnO Vhud p p Lpd p p pO bh{d vh  p hd  h d M d   h K h  h dd nv p h  Sid d Sp pd SpM o6i ^ op op Di  cPid hi k>_^i d dvp i d dvp i lm4卑? p pw i k5y; d vpw j k : dvpw &j k9 dvpw Fj k= 9 dvpw fj kO8 dvpw j  cwkw+2_^jd j d dvp j  kL? dvpw j k>;= d vp  k k9y< d vp ,k kl; dvp Lk# ka; dvp lk) k pf: dvp k/ kk9 dvp k5d O k;  p op kAdd  p pn  kGd p lM  pd pnp M"lS[c4lc dc^Y>l_[eVlY d p `le[ |lmFUERA DE LIMITE"lkNl5kI@ lqd wl~l=r7@e n Jld lmA.R.h,m,s DE LA RADIANTE&m  d ozm ee  de< oenpnp mmDEC.g,m,s DE LA RADIANTEm S d o r . . Jpw DtJd D Dpw DO uPd Jd . wnpn VZu]d Jnd Vwnpnd Jwnd VnpnO cpuid cnp *uo d Td Jwnd JwnOn uu{d unp u d Jwnp u d Jnp v  J Mpw d*vk< p pO >v d  L`ve ep nw vmV= "  ep vmEXC= Jvmq= vmQ= vmINC T.=" Lv d d nv rwmPERIODO rdwmLONG. Y LAT. GEOC.ECLIPTICAS=" epkI@ ^epkI@wm VEL APAR=" 6lnաApeew[w[w0 pruwd)kA wnk @nvO w epd  $x dd kI@p d vpk,@p zx d k333Ad vpko:pk3D  &  d p&  & x ox  m4CENTRO APROXIMADO DE AREA DE IMPACTO DE UN METEORITOmT.U. ENTRADA ATMOSFERA H.FRAC= . mA.R. RADIANTE H.FRAC=" 5 mDEC. RADIANTE GRAD.= < mMES.FRACCION EFEMERIDE = C  C kl@wnd p J  5 J w Q e .  Q w X  X end X  X X &wnep X  X d)p&d) X e . w Q w _  X d g  g e_]`| g ew g  X dw o  o dc]| o e o  < eZ w  w eZ_]|eZ w  < eZw  eZxc]|eZx mLONGITUD CENTRO AREA HH= X mLONGITUD MAXIMA Y MINIMA HH= g o mLATITUD CENTRO AREA GRD= < mLATITUD MAXIMA Y MINIMA GRD= w mNUEVO CALCULO =1  d^ N z