Last change
on this file since 3436 was
3175,
checked in by emillour, 11 months ago
|
Pluto PCM:
Add the old Pluto LMDZ for reference (required prior step to making
an LMDZ.PLUTO using the same framework as the other physics packages).
TB+EM
|
File size:
1.2 KB
|
Line | |
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1 | c ******************************************************** |
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2 | subroutine call_dayperi(Lsperi,e_elips,dayperi,year_day) |
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3 | IMPLICIT NONE |
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4 | |
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5 | c======================================================================= |
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6 | c |
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7 | c Objet: |
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8 | c ------ |
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9 | c Computing the Plutonian date (number of sols since Ls=0 = spring |
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10 | c equinox) at perihelion. Called by testphys1D only |
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11 | c |
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12 | c Arguments: |
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13 | c ---------- |
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14 | c |
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15 | c Input: |
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16 | c ------ |
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17 | c Lsperi solar longitude (Ls) of perohelion (rad) |
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18 | c e_elips Excentricity |
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19 | c |
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20 | c output |
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21 | c ------ |
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22 | c dayperi Plutonian date at perihelion (sol) |
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23 | c real year_day ! number of sols per Pluto year |
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24 | c----------------------------------------------------------------------- |
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25 | |
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26 | c arguments: |
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27 | c ---------- |
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28 | real Lsperi,e_elips,dayperi |
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29 | real year_day ! number of sols per Pluto year ~ 14164.46 |
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30 | |
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31 | |
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32 | c Local |
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33 | real x1, x2,pi |
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34 | |
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35 | |
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36 | pi=2.*asin(1.) |
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37 | |
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38 | x1 = sqrt((1.-e_elips)/(1.+e_elips)) |
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39 | x2 = e_elips*sqrt(1.-e_elips**2.) |
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40 | |
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41 | dayperi = 0.5*(year_day/pi)* |
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42 | & ( 2.*atan(x1*tan(0.5*Lsperi)) |
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43 | & -x2*sin(Lsperi)/(1.+e_elips*cos(Lsperi)) ) |
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44 | if(dayperi.lt.0) dayperi=dayperi+year_day |
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45 | return |
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46 | end |
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