dpspce |
Table of contents
ProcedureDPSPCE ( Evaluate "two-line" element data, deep-space ) SUBROUTINE DPSPCE ( ET, GEOPHS, ELEMS, STATE ) AbstractDeprecated: This routine has been superseded by the SPICELIB routine EVSGP4. *ALL* TLE evaluations should use that routine. NAIF supports DPSPCE only for backward compatibility. Evaluate NORAD two-line element data for deep-space, earth orbiting spacecraft (that is spacecraft with orbital periods greater-than 225 minutes). This evaluator uses algorithms as described in Hoots 1980 [1]. Required_ReadingNone. KeywordsDEEP SPACE PROPAGATOR EPHEMERIS TWO LINE ELEMENTS DeclarationsIMPLICIT NONE DOUBLE PRECISION ET DOUBLE PRECISION GEOPHS ( 8 ) DOUBLE PRECISION ELEMS ( 10 ) DOUBLE PRECISION STATE ( 6 ) Brief_I/OVARIABLE I/O DESCRIPTION -------- --- -------------------------------------------------- ET I Time for state evaluation in seconds past ephemeris epoch J2000. GEOPHS I The array of geophysical constants. ELEMS I Array of orbit elements. STATE O State vector at ET. Detailed_InputET is the epoch in TDB seconds past ephemeris epoch J2000 to produced a state from the input elements. GEOPHS is a collection of 8 geophysical constants needed for computing a state. The order of these constants must be: GEOPHS(1) = J2 gravitational harmonic for Earth. GEOPHS(2) = J3 gravitational harmonic for Earth. GEOPHS(3) = J4 gravitational harmonic for Earth. These first three constants are dimensionless. GEOPHS(4) = KE: Square root of the GM for Earth where GM is expressed in Earth radii cubed per minutes squared. GEOPHS(5) = QO: High altitude bound for atmospheric model in km. GEOPHS(6) = SO: Low altitude bound for atmospheric model in km. GEOPHS(7) = RE: Equatorial radius of the earth in km. GEOPHS(8) = AE: Distance units/earth radius (normally 1) Below are currently recommended values for these items: J2 = 1.082616D-3 J3 = -2.53881D-6 J4 = -1.65597D-6 The next item is the square root of GM for the Earth given in units of earth-radii**1.5/Minute KE = 7.43669161D-2 The next two items define the top and bottom of the atmospheric drag model used by the type 10 ephemeris type. Don't adjust these unless you understand the full implications of such changes. QO = 120.0D0 SO = 78.0D0 The ER value is the equatorial radius in km of the Earth as used by NORAD. ER = 6378.135D0 The value of AE is the number of distance units per Earth radii used by the NORAD state propagation software. The value should be 1 unless you've got a very good understanding of the NORAD routine SGP4 and the affect of changing this value. AE = 1.0D0 ELEMS is an array containing two-line element data as prescribed below. The elements NDD6O and BSTAR must already be scaled by the proper exponent stored in the two line elements set. Moreover, the various items must be converted to the units shown here. ELEMS ( 1 ) = NDT20 in radians/minute**2 ELEMS ( 2 ) = NDD60 in radians/minute**3 ELEMS ( 3 ) = BSTAR ELEMS ( 4 ) = INCL in radians ELEMS ( 5 ) = NODE0 in radians ELEMS ( 6 ) = ECC ELEMS ( 7 ) = OMEGA in radians ELEMS ( 8 ) = M0 in radians ELEMS ( 9 ) = N0 in radians/minute ELEMS ( 10 ) = EPOCH of the elements in seconds past ephemeris epoch J2000. Detailed_OutputSTATE is the state produced by evaluating the input elements at the input epoch ET. Units are km and km/sec relative to the TEME reference frame. ParametersNone. ExceptionsError free. FilesNone. ParticularsThis subroutine is an extensive rewrite of the SDP4 routine as described in the Spacetrack 3 report. All common blocks were removed and all variables are explicitly defined. The removal of common blocks causes the set of routines to execute slower than the original version of SDP4. However the stability improves especially as concerns memory and expanded internal documentation. Trivial or redundant variables have been eliminated. R removed, occurrence replaced with RK E6A renamed TOL THETA4 removed, relevant equation recast in Horner's form i.e. something like x^4 + x^2 -> x^2 ( x^2 + 1 ) U renamed UANG, U is now a euclidean 3 vector. Ux,Uy,Uz removed, replaced with 3-vector U Vx,Vy,Vz removed, replaced with 3-vector V OMEGAQ removed, usage replaced with OMEGAO OMGDT removed, same variable as OMGDOT, so all occurrences replaced with OMGDOT SSL,SSG replaced with the 5-vector SSX SSH,SSE SSI Three functions present in the original Spacetrack report, ACTAN, FMOD2P and THETAG, have been either replaced with an intrinsic FORTRAN function (ACTAN -> DATAN2, FMOD2P -> DMOD) or recoded using SPICELIB calls (THETAG). The code at the end of this subroutine which calculates orientation vectors, was replaced with a set of calls to SPICELIB vector routines. A direct comparison of output from the original Spacetrack 3 code and these NAIF routines for the same elements and time parameters will produce unacceptably different results. ExamplesThe numerical results shown for this example may differ across platforms. The results depend on the SPICE kernels used as input, the compiler and supporting libraries, and the machine specific arithmetic implementation. 1) Suppose that you have collected the two-line element data for the TDRS 4 geosynchronous satellite. The following example code demonstrates how you obtain its state at an epoch of interest. Use the meta-kernel shown below to load the required SPICE kernels. KPL/MK File name: dpspce_ex1.tm This meta-kernel is intended to support operation of SPICE example programs. The kernels shown here should not be assumed to contain adequate or correct versions of data required by SPICE-based user applications. In order for an application to use this meta-kernel, the kernels referenced here must be present in the user's current working directory. The names and contents of the kernels referenced by this meta-kernel are as follows: File name Contents --------- ------------------------------------ naif0012.tls Leapseconds geophysical.ker geophysical constants for evaluation of two-line element sets. \begindata KERNELS_TO_LOAD = ( 'naif0012.tls', 'geophysical.ker' ) \begintext End of meta-kernel Example code begins here. PROGRAM DPSPCE_EX1 IMPLICIT NONE C C Local parameters. C INTEGER PNAMLN PARAMETER ( PNAMLN = 2 ) INTEGER TIMSLN PARAMETER ( TIMSLN = 25 ) INTEGER TLELLN PARAMETER ( TLELLN = 69 ) C C The TDRS-4 satellite is an Earth orbiting object; set C the center ID to the Earth ID. C INTEGER CENTER PARAMETER ( CENTER = 399 ) C C Local variables. C CHARACTER*(PNAMLN) NOADPN ( 8 ) CHARACTER*(TIMSLN) TIMSTR CHARACTER*(TLELLN) TLE ( 2 ) DOUBLE PRECISION DELT DOUBLE PRECISION ELEMS ( 10 ) DOUBLE PRECISION EPOCH DOUBLE PRECISION GEOPHS ( 8 ) DOUBLE PRECISION STATE ( 6 ) DOUBLE PRECISION ET DOUBLE PRECISION TF INTEGER I INTEGER N C C These are the variables that will hold the constants C required by DPSPCE. These constants are available from C the loaded PCK file, which provides the actual values C and units as used by NORAD propagation model. C C Constant Meaning C -------- ------------------------------------------ C J2 J2 gravitational harmonic for Earth. C J3 J3 gravitational harmonic for Earth. C J4 J4 gravitational harmonic for Earth. C KE Square root of the GM for Earth. C QO High altitude bound for atmospheric model. C SO Low altitude bound for atmospheric model. C ER Equatorial radius of the Earth. C AE Distance units/earth radius. C DATA NOADPN / 'J2', 'J3', 'J4', 'KE', . 'QO', 'SO', 'ER', 'AE' / C C Define the Two-Line Element set for TDRS-4. C TLE(1) = '1 19883U 89021B 97133.05943164 -.00000277' . // ' 00000-0 10000-3 0 3315' TLE(2) = '2 19883 0.5548 86.7278 0001786 312.2904 ' . // '172.2391 1.00269108202415' C C Load the PCK file that provides the geophysical C constants required for the evaluation of the two-line C elements sets. Load also an LSK, as it is required by C GETELM to perform time conversions. Use a meta-kernel for C convenience. C CALL FURNSH ( 'dpspce_ex1.tm' ) C C Retrieve the data from the kernel, and place it on C the GEOPHS array. C DO I = 1, 8 CALL BODVCD ( CENTER, NOADPN(I), 1, N, GEOPHS(I) ) END DO C C Convert the Two Line Elements lines to the element sets. C Set the lower bound for the years to be the earliest C first year for the elements. C CALL GETELM ( 1988, TLE, EPOCH, ELEMS ) C C Define the final time past epoch, 1400 mins (in seconds), C the step size for elements output, 360 mins (in seconds), C and the start time keyed off epoch. C TF = 1440.D0 * 60.D0 DELT = 360.D0 * 60.D0 ET = EPOCH - 4.D0 * DELT C C Display the reference epoch for the elements. C CALL ET2UTC ( EPOCH, 'C', 3, TIMSTR ) WRITE(*,'(2A)') 'Reference epoch: ', TIMSTR C C Obtain the state at different epochs around the C reference epoch. C DO WHILE ( DABS(TIME - EPOCH) .LE. DABS(TF) ) CALL DPSPCE ( ET, GEOPHS, ELEMS, STATE ) CALL ET2UTC ( ET, 'C', 3, TIMSTR ) WRITE(*,*) WRITE(*,'(2A)') 'Time : ', TIMSTR WRITE(*,'(A,3F16.8)') 'Position: ', (STATE(I), I=1,3) WRITE(*,'(A,3F16.8)') 'Velocity: ', (STATE(I), I=4,6) ET = ET + DELT END DO END When this program was executed on a Mac/Intel/gfortran/64-bit platform, the output was: Reference epoch: 1997 MAY 13 01:25:34.894 Time : 1997 MAY 12 01:25:34.894 Position: -36415.06027922 -21268.27678598 324.63292275 Velocity: 1.55019424 -2.65462811 -0.01618361 Time : 1997 MAY 12 07:25:34.894 Position: 21403.92800065 -36329.04571718 -223.49047558 Velocity: 2.64861127 1.56125103 -0.02363616 Time : 1997 MAY 12 13:25:34.894 Position: 36222.44396185 21565.83478418 -323.53517502 Velocity: -1.57313376 2.64235356 0.01642601 Time : 1997 MAY 12 19:25:34.894 Position: -21736.44940088 36128.44906628 226.92953877 Velocity: -2.63481828 -1.58473777 0.02355544 Time : 1997 MAY 13 01:25:34.894 Position: -36048.19799634 -21884.57697027 322.54133293 Velocity: 1.59511867 -2.62787056 -0.01665374 Time : 1997 MAY 13 07:25:34.894 Position: 22018.52968309 -35959.79405656 -229.86590206 Velocity: 2.62168498 1.60606852 -0.02347795 Time : 1997 MAY 13 13:25:34.894 Position: 35850.58313589 22178.69474099 -321.27968318 Velocity: -1.61782447 2.61522408 0.01688604 Time : 1997 MAY 13 19:25:34.894 Position: -22347.26148339 35754.07411618 233.17456026 Velocity: -2.60750172 -1.62927167 0.02338424 Time : 1997 MAY 14 01:25:34.894 Position: -35671.56713967 -22493.50518477 320.10323846 Velocity: 1.63950543 -2.60040084 -0.01710490 RestrictionsNone. Literature_References[1] F. Hoots and R. Roehrich, "Spacetrack Report #3: Models for Propagation of the NORAD Element Sets," U.S. Air Force Aerospace Defense Command, Colorado Springs, CO, 1980. [2] F. Hoots, "Spacetrack Report #6: Models for Propagation of Space Command Element Sets," U.S. Air Force Aerospace Defense Command, Colorado Springs, CO, 1986. [3] F. Hoots, P. Schumacher and R. Glover, "History of Analytical Orbit Modeling in the U. S. Space Surveillance System," Journal of Guidance, Control, and Dynamics. 27(2):174-185, 2004. [4] D. Vallado, P. Crawford, R. Hujsak and T. Kelso, "Revisiting Spacetrack Report #3," paper AIAA 2006-6753 presented at the AIAA/AAS Astrodynamics Specialist Conference, Keystone, CO., August 21-24, 2006. Author_and_InstitutionJ. Diaz del Rio (ODC Space) W.L. Taber (JPL) E.D. Wright (JPL) VersionSPICELIB Version 2.1.0, 01-NOV-2021 (JDR) (EDW) Declared routine as deprecated. Changed input argument name "TIME" to "ET" for consistency with other routines. Corrected the description of QO and SO constants in the detailed description of the input argument GEOPHS and the input element names in ELEMS. Edited the header to comply with NAIF standard. Added complete code example based on existing fragments. SPICELIB Version 2.0.0, 23-JAN-2013 (EDW) Corrected initialization block error. The ZZDPINIT call causes a side-effect required for each DPSPCE call. The ZZDPINIT call now occurs outside the initialization block. Note from designer, side-effects are bad. Added proper citation for Hoots paper. SPICELIB Version 1.2.2, 22-AUG-2006 (EDW) Replaced references to LDPOOL with references to FURNSH. SPICELIB Version 1.2.1, 27-DEC-2000 (EDW) Corrected error in header documentation. Horner's Rule not Butcher's. SPICELIB Version 1.2.0, 24-MAR-1999 (EDW) Documentation expanded to include modifications made to private routines. Some English errors corrected. Alphabetized variable declaration lists. Temporary variable TEMP removed. OMGDOT argument added to ZZDPSEC call. SPICELIB Version 1.1.0, 05-OCT-1998 (WLT) Forced initialization section until we can figure out why it doesn't work on SUNs. SPICELIB Version 1.0.1, 11-MAR-1998 (EDW) Corrected error in header describing GEOPHS array. SPICELIB Version 1.0.0, 11-NOV-1998 (EDW) |
Fri Dec 31 18:36:14 2021