{VERSION 5 0 "IBM INTEL NT" "5.0" } {USTYLETAB {CSTYLE "Maple Input" -1 0 "Courier" 0 1 255 0 0 1 0 1 0 0 1 0 0 0 0 1 }{CSTYLE "2D Math" -1 2 "Times" 0 1 0 0 0 0 0 0 2 0 0 0 0 0 0 1 }{CSTYLE "2D Comment" 2 18 "" 0 1 0 0 0 0 0 0 0 0 0 0 0 0 0 1 } {CSTYLE "" -1 256 "" 1 24 0 0 0 0 0 0 0 0 0 0 0 0 0 1 }{CSTYLE "" -1 257 "" 1 18 0 0 0 0 0 0 0 0 0 0 0 0 0 1 }{CSTYLE "" -1 258 "" 1 24 0 0 0 0 0 0 0 0 0 0 0 0 0 1 }{PSTYLE "Normal" -1 0 1 {CSTYLE "" -1 -1 " " 0 1 0 0 0 0 0 0 0 0 0 0 0 0 0 1 }0 0 0 -1 -1 -1 0 0 0 0 0 0 -1 0 } {PSTYLE "Heading 1" 0 3 1 {CSTYLE "" -1 -1 "" 1 18 0 0 0 0 0 1 0 0 0 0 0 0 0 1 }1 0 0 0 6 6 0 0 0 0 0 0 -1 0 }{PSTYLE "Heading 2" 3 4 1 {CSTYLE "" -1 -1 "" 1 14 0 0 0 0 0 0 0 0 0 0 0 0 0 1 }0 0 0 -1 4 4 0 0 0 0 0 0 -1 0 }} {SECT 0 {EXCHG {PARA 4 "" 0 "" {TEXT 256 14 "Ejercicios de " }}{PARA 4 "" 0 "" {TEXT 258 44 "(2) Ecuaciones escalares: el m\351todo de EULE R" }}{PARA 4 "" 0 "" {TEXT -1 0 "" }}{PARA 4 "" 0 "" {TEXT 257 15 "Eje rcicio 02-02" }{TEXT -1 72 "\n\nSiendo y(x) la soluci\363n exacta de l problema tipo y'=f(x,y) , y(a)= " }{XPPEDIT 18 0 "eta" "6#%$etaG" } {TEXT -1 3 " , " }}{PARA 4 "" 0 "" {TEXT -1 50 "se recuerda que se ver ifica por la Regla de BARROW" }}{PARA 4 "" 0 "" {TEXT -1 19 " y(x+h) - y(x) = " }{XPPEDIT 18 0 "Int(y(t),t=x..x+h)" "6#-%$IntG6$-%\"yG6#% \"tG/F);%\"xG,&F,\"\"\"%\"hGF." }{TEXT -1 6 " = " }{XPPEDIT 18 0 "I nt(f(t,y(t)),t=x..x+h)" "6#-%$IntG6$-%\"fG6$%\"tG-%\"yG6#F)/F);%\"xG,& F/\"\"\"%\"hGF1" }{TEXT -1 2 " " }}{PARA 4 "" 0 "" {TEXT -1 76 "D\355 gase qu\351 aproximaci\363n hay que tomar en la integral para obtener \+ el m\351todo " }}{PARA 4 "" 0 "" {TEXT -1 74 "de EULER. D\355gase tamb i\351n qu\351 m\351todo se crea cuando se aproxima la integral" }} {PARA 4 "" 0 "" {TEXT -1 34 "empleando el 'm\351todo del trapecio'" }} }{EXCHG {PARA 0 "> " 0 "" {MPLTEXT 1 0 8 "restart:" }}}{EXCHG {PARA 0 "> " 0 "" {MPLTEXT 1 0 26 "interface(labeling=false):" }}}}{MARK "0 0 \+ 0" 0 }{VIEWOPTS 1 1 0 3 4 1802 1 1 1 1 }{PAGENUMBERS 0 1 2 33 1 1 }