nrlmsise-00.h

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/* -------------------------------------------------------------------- */
/* ---------  N R L M S I S E - 0 0    M O D E L    2 0 0 1  ---------- */
/* -------------------------------------------------------------------- */
 
/* This file is part of the NRLMSISE-00  C source code package - release
 * 20041227
 *
 * The NRLMSISE-00 model was developed by Mike Picone, Alan Hedin, and
 * Doug Drob. They also wrote a NRLMSISE-00 distribution package in 
 * FORTRAN which is available at
 * http://uap-www.nrl.navy.mil/models_web/msis/msis_home.htm
 *
 * Dominik Brodowski implemented and maintains this C version. You can
 * reach him at mail@brodo.de. See the file "DOCUMENTATION" for details,
 * and check http://www.brodo.de/english/pub/nrlmsise/index.html for
 * updated releases of this package.
 */
 
#ifndef MSIS_NRLMSISE_00_H
#define MSIS_NRLMSISE_00_H
 
/* ------------------------------------------------------------------- */
/* ------------------------------- INPUT ----------------------------- */
/* ------------------------------------------------------------------- */
 
struct nrlmsise_flags {
    int switches[24];
    double sw[24];
    double swc[24];
};
/*   
 *   Switches: to turn on and off particular variations use these switches.
 *   0 is off, 1 is on, and 2 is main effects off but cross terms on.
 *
 *   Standard values are 0 for switch 0 and 1 for switches 1 to 23. The 
 *   array "switches" needs to be set accordingly by the calling program. 
 *   The arrays sw and swc are set internally.
 *
 *   switches[i]:
 *    i - explanation
 *   -----------------
 *    0 - output in meters and kilograms instead of centimeters and grams
 *    1 - F10.7 effect on mean
 *    2 - time independent
 *    3 - symmetrical annual
 *    4 - symmetrical semiannual
 *    5 - asymmetrical annual
 *    6 - asymmetrical semiannual
 *    7 - diurnal
 *    8 - semidiurnal
 *    9 - daily ap [when this is set to -1 (!) the pointer
 *                  ap_a in struct nrlmsise_input must
 *                  point to a struct ap_array]
 *   10 - all UT/long effects
 *   11 - longitudinal
 *   12 - UT and mixed UT/long
 *   13 - mixed AP/UT/LONG
 *   14 - terdiurnal
 *   15 - departures from diffusive equilibrium
 *   16 - all TINF var
 *   17 - all TLB var
 *   18 - all TN1 var
 *   19 - all S var
 *   20 - all TN2 var
 *   21 - all NLB var
 *   22 - all TN3 var
 *   23 - turbo scale height var
 */
 
struct ap_array {
    double a[7];   
};
/* Array containing the following magnetic values:
 *   0 : daily AP
 *   1 : 3 hr AP index for current time
 *   2 : 3 hr AP index for 3 hrs before current time
 *   3 : 3 hr AP index for 6 hrs before current time
 *   4 : 3 hr AP index for 9 hrs before current time
 *   5 : Average of eight 3 hr AP indicies from 12 to 33 hrs 
 *           prior to current time
 *   6 : Average of eight 3 hr AP indicies from 36 to 57 hrs 
 *           prior to current time 
 */
 
struct nrlmsise_input {
    int year;      /* year, currently ignored */
    int doy;       /* day of year */
    double sec;    /* seconds in day (UT) */
    double alt;    /* altitude in kilometers */
    double g_lat;  /* geodetic latitude */
    double g_long; /* geodetic longitude */
    double lst;    /* local apparent solar time (hours), see note below */
    double f107A;  /* 81 day average of F10.7 flux (centered on doy) */
    double f107;   /* daily F10.7 flux for previous day */
    double ap;     /* magnetic index(daily) */
    struct ap_array *ap_a; /* see above */
};
 
/*
 *   NOTES ON INPUT VARIABLES: 
 *      UT, Local Time, and Longitude are used independently in the
 *      model and are not of equal importance for every situation.  
 *      For the most physically realistic calculation these three
 *      variables should be consistent (lst=sec/3600 + g_long/15).
 *      The Equation of Time departures from the above formula
 *      for apparent local time can be included if available but
 *      are of minor importance.
 *
 *      f107 and f107A values used to generate the model correspond
 *      to the 10.7 cm radio flux at the actual distance of the Earth
 *      from the Sun rather than the radio flux at 1 AU. The following
 *      site provides both classes of values:
 *      ftp://ftp.ngdc.noaa.gov/STP/SOLAR_DATA/SOLAR_RADIO/FLUX/
 *
 *      f107, f107A, and ap effects are neither large nor well
 *      established below 80 km and these parameters should be set to
 *      150., 150., and 4. respectively.
 */
 
 
 
/* ------------------------------------------------------------------- */
/* ------------------------------ OUTPUT ----------------------------- */
/* ------------------------------------------------------------------- */
 
struct nrlmsise_output {
    double d[9];   /* densities */
    double t[2];   /* temperatures */
};
/* 
 *   OUTPUT VARIABLES:
 *      d[0] - HE NUMBER DENSITY(CM-3)
 *      d[1] - O NUMBER DENSITY(CM-3)
 *      d[2] - N2 NUMBER DENSITY(CM-3)
 *      d[3] - O2 NUMBER DENSITY(CM-3)
 *      d[4] - AR NUMBER DENSITY(CM-3)                       
 *      d[5] - TOTAL MASS DENSITY(GM/CM3) [includes d[8] in td7d]
 *      d[6] - H NUMBER DENSITY(CM-3)
 *      d[7] - N NUMBER DENSITY(CM-3)
 *      d[8] - Anomalous oxygen NUMBER DENSITY(CM-3)
 *      t[0] - EXOSPHERIC TEMPERATURE
 *      t[1] - TEMPERATURE AT ALT
 * 
 *
 *      O, H, and N are set to zero below 72.5 km
 *
 *      t[0], Exospheric temperature, is set to global average for
 *      altitudes below 120 km. The 120 km gradient is left at global
 *      average value for altitudes below 72 km.
 *
 *      d[5], TOTAL MASS DENSITY, is NOT the same for subroutines GTD7 
 *      and GTD7D
 *
 *        SUBROUTINE GTD7 -- d[5] is the sum of the mass densities of the
 *        species labeled by indices 0-4 and 6-7 in output variable d.
 *        This includes He, O, N2, O2, Ar, H, and N but does NOT include
 *        anomalous oxygen (species index 8).
 *
 *        SUBROUTINE GTD7D -- d[5] is the "effective total mass density
 *        for drag" and is the sum of the mass densities of all species
 *        in this model, INCLUDING anomalous oxygen.
 */
 
 
 
/* ------------------------------------------------------------------- */
/* --------------------------- PROTOTYPES ---------------------------- */
/* ------------------------------------------------------------------- */
 
/* GTD7 */
/*   Neutral Atmosphere Empircial Model from the surface to lower
 *   exosphere.
 */
void gtd7 (struct nrlmsise_input *input, \
           struct nrlmsise_flags *flags, \
           struct nrlmsise_output *output);
 
 
/* GTD7D */
/*   This subroutine provides Effective Total Mass Density for output
 *   d[5] which includes contributions from "anomalous oxygen" which can
 *   affect satellite drag above 500 km. See the section "output" for
 *   additional details.
 */
void gtd7d(struct nrlmsise_input *input, \
           struct nrlmsise_flags *flags, \
           struct nrlmsise_output *output);
 
 
/* GTS7 */
/*   Thermospheric portion of NRLMSISE-00
 */
void gts7 (struct nrlmsise_input *input, \
       struct nrlmsise_flags *flags, \
       struct nrlmsise_output *output);
 
 
/* GHP7 */
/*   To specify outputs at a pressure level (press) rather than at
 *   an altitude.
 */
void ghp7 (struct nrlmsise_input *input, \
           struct nrlmsise_flags *flags, \
           struct nrlmsise_output *output, \
           double press);
 
 
 
/* ------------------------------------------------------------------- */
/* ----------------------- COMPILATION TWEAKS ------------------------ */
/* ------------------------------------------------------------------- */
 
/* "inlining" of functions */
/*   Some compilers (e.g. gcc) allow the inlining of functions into the
 *   calling routine. This means a lot of overhead can be removed, and
 *   the execution of the program runs much faster. However, the filesize
 *   and thus the loading time is increased.
 */
#ifdef INLINE
#define __inline_double static inline double
#else
#define __inline_double double
#endif
 
#endif