USERS GUIDE, CONSTANTS, AND SYMBOLS

The first input card is the program card. The format is as follows:

verbatim3#

All times are in minutes since epoch and can be positive or negative. The second and third input cards consist of either a 2-card transmission or 2-card G type element set. Either type can be used with the only condition being that the two cards must be in the correct order. For reference a format sheet for the T-card and G-card element sets follows this section.

The values of the physical and mathematical constants used in the program are given below.



Variable name ;SPMnbsp;;SPMnbsp;;SPMnbsp;;SPMnbsp;distance units/Earth radii ;SPMnbsp;;SPMnbsp;;SPMnbsp;;SPMnbsp;
Variable name 		 Definition 		 Value

CK2 #math394##tex2html_wrap_inline4798#J2aE2 5.413080E-4

CK4 #math395#- #tex2html_wrap_inline4802#J4aE4 .62098875E-6

E6A 10-6 1.0 E-6

QOMS2T #math396#(qo - s)4<#1#> (er)<#1#>4 1.88027916E-9

S #math397#s<#1#> (er)<#1#> 1.01222928

TOTHRD 2/3 .66666667

XJ3 J3 -.253881E-5

XKE #math398#ke#tex2html_wrap_inline4810##tex2html_wrap_inline4811##tex2html_wrap_inline4812# .743669161E-1

XKMPER kilometers/Earth radii 6378.135

XMNPDA time units/day 1440.0

AE distance units/Earth radii 1.0

DE2RA radians/degree .174532925E-1

PI π 3.14159265

PIO2 π/2 1.57079633

TWOPI 2π 6.2831853

X3PIO2 3π/2 4.71238898

where er = Earth radii. Except for the deep-space models, all ephemeris models are independent of units. Thus, units input or output as well as physical constants can be changed by making the appropriate changes in only the DRIVER program.

Following is a list of symbols commonly used in this report.

no = the SGP type ``mean'' mean motion at epoch

eo = the ``mean'' eccentricity at epoch

io = the ``mean'' inclination at epoch

Mo = the ``mean'' mean anomaly at epoch

ωo = the ``mean'' argument of perigee at epoch

Ωo = the ``mean'' longitude of ascending node at epoch

#tex2html_wrap_inline4824# = the time rate of change of ``mean'' mean motion at epoch

#math399##tex2html_wrap_inline4826# = the second time rate of change of ``mean'' mean motion at epoch

B* = the SGP4 type drag coefficient

ke = #tex2html_wrap_inline4829#

aE = the equatorial radius of the Earth

J2 = the second gravitational zonal harmonic of the Earth

J3 = the third gravitational zonal harmonic of the Earth

J4 = the fourth gravitational zonal harmonic of the Earth

(t - to) = time since epoch

#math400#k2 = #tex2html_wrap_inline4836#J2aE2

#math401#k4 = - #tex2html_wrap_inline4840#J4aE4

#math402#A3, 0 = - J3aE3

qo = parameter for the SGP4/SGP8 density function

s = parameter for the SGP4/SGP8 density function

B = #tex2html_wrap_inline4849#