[38] | 1 | SUBROUTINE iniorbit |
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| 2 | $ (paphelie,pperiheli,pyear_day,pperi_day,pobliq) |
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[1382] | 3 | use planete_h, only: aphelie, periheli, year_day, peri_day, |
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| 4 | & obliquit, unitastr, e_elips, p_elips, |
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| 5 | & timeperi |
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| 6 | use comcstfi_h, only: pi |
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[38] | 7 | IMPLICIT NONE |
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| 8 | |
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[1382] | 9 | !======================================================================= |
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| 10 | ! Initialisation of orbital parameters (stored in planete_h module) |
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| 11 | !======================================================================= |
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[38] | 12 | |
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[1382] | 13 | ! Arguments: |
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| 14 | ! ---------- |
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[38] | 15 | |
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[1382] | 16 | REAL,INTENT(IN) :: paphelie,pperiheli,pyear_day,pperi_day,pobliq |
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[38] | 17 | |
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[1382] | 18 | ! Local: |
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| 19 | ! ------ |
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[38] | 20 | |
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| 21 | REAL zxref,zanom,zz,zx0,zdx |
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| 22 | INTEGER iter |
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| 23 | |
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[1382] | 24 | !----------------------------------------------------------------------- |
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[38] | 25 | |
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| 26 | pi=2.*asin(1.) |
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| 27 | |
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| 28 | aphelie =paphelie |
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| 29 | periheli=pperiheli |
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| 30 | year_day=pyear_day |
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| 31 | obliquit=pobliq |
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| 32 | peri_day=pperi_day |
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| 33 | |
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[1382] | 34 | PRINT*,'iniorbit: Perihelion in Mkm ',periheli |
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| 35 | PRINT*,'iniorbit: Aphelion in Mkm ',aphelie |
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| 36 | PRINT*,'iniorbit: Obliquity in degrees :',obliquit |
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| 37 | unitastr=149.597927 ! 1 UA, in Mkm |
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[38] | 38 | e_elips=(aphelie-periheli)/(periheli+aphelie) |
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| 39 | p_elips=0.5*(periheli+aphelie)*(1-e_elips*e_elips)/unitastr |
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| 40 | |
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[1382] | 41 | print*,'iniorbit: e_elips',e_elips |
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| 42 | print*,'iniorbit: p_elips',p_elips |
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[38] | 43 | |
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[1382] | 44 | !----------------------------------------------------------------------- |
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| 45 | ! compute polar angle and distance to the Sun: |
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| 46 | ! ------------------------------------------------------- |
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[38] | 47 | |
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[1382] | 48 | ! compute mean anomaly zanom |
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[38] | 49 | |
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| 50 | zz=(year_day-pperi_day)/year_day |
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| 51 | zanom=2.*pi*(zz-nint(zz)) |
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| 52 | zxref=abs(zanom) |
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[1382] | 53 | PRINT*,'iniorbit: zanom ',zanom |
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[38] | 54 | |
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[1382] | 55 | ! solve equation zx0 - e * sin (zx0) = zxref for eccentric anomaly zx0 |
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| 56 | ! using Newton method |
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[38] | 57 | |
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| 58 | zx0=zxref+e_elips*sin(zxref) |
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[1382] | 59 | DO iter=1,100 |
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[38] | 60 | zdx=-(zx0-e_elips*sin(zx0)-zxref)/(1.-e_elips*cos(zx0)) |
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[1382] | 61 | if(abs(zdx).le.(1.e-12)) exit |
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[38] | 62 | zx0=zx0+zdx |
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[1382] | 63 | ENDDO |
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| 64 | |
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[38] | 65 | zx0=zx0+zdx |
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| 66 | if(zanom.lt.0.) zx0=-zx0 |
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[1382] | 67 | PRINT*,'iniorbit: zx0 ',zx0 |
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[38] | 68 | |
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| 69 | timeperi=2.*atan(sqrt((1.+e_elips)/(1.-e_elips))*tan(zx0/2.)) |
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[1382] | 70 | PRINT*,'iniorbit: Perihelion solar long. Ls (deg)=', |
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| 71 | & 360.-timeperi*180./pi |
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[38] | 72 | |
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| 73 | END |
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