add_config_search_dir(dir)
|
|
are_coordinate_scales_convertible(from, to)
|
|
az_el_range_to_cart(*args, **kwargs)
|
Overloaded function. |
az_el_range_to_east_north_up(*args, **kwargs)
|
Overloaded function. |
cart2coe(posvel, GM)
|
|
cart_to_az_el_range(*args, **kwargs)
|
Overloaded function. |
cart_to_classical(*args, **kwargs)
|
Overloaded function. |
cart_to_east_north_up(*args, **kwargs)
|
Overloaded function. |
cart_to_lat_lon_alt(*args, **kwargs)
|
Overloaded function. |
cart_to_stereographic(*args, **kwargs)
|
Overloaded function. |
classical_to_cart(*args, **kwargs)
|
Overloaded function. |
classical_to_delaunay(*args, **kwargs)
|
Overloaded function. |
classical_to_equinoctial(*args, **kwargs)
|
Overloaded function. |
classical_to_quasi_nonsingular(*args, **kwargs)
|
Overloaded function. |
coe2cart(coe, GM)
|
|
compute_B(t_j2000, pos_geo, config[, debug])
|
Magnetic field vector [nT] at a given ECEF position. |
compute_eop_from_spice(t_tdb)
|
Derive (x_pole [rad], y_pole [rad], UT1-UTC [s]) at t_tdb from SPICE |
compute_min_altitude(pos1, pos2, radius)
|
|
compute_ne(t_j2000, pos_geo, config[, debug])
|
Electron density [cm^-3] at a given position and time. |
compute_vis(pos1, pos2, radius, max_angle)
|
|
config_to_string(config)
|
|
convert_coordinate_time(*args, **kwargs)
|
Overloaded function. |
convert_frame(*args, **kwargs)
|
Overloaded function. |
convert_time(*args, **kwargs)
|
Overloaded function. |
coordinate_scale_factor(scale)
|
|
coordinate_scale_ratio(from, to)
|
|
create_body(*args, **kwargs)
|
Overloaded function. |
datetime_to_itime(datetime)
|
|
datetime_to_mjd(datetime)
|
|
decibel_to_decimal(*args, **kwargs)
|
Overloaded function. |
decimal_to_decibel(*args, **kwargs)
|
Overloaded function. |
deg_min_sec_to_degrees(hms)
|
|
degrees_to_deg_min_sec(deg)
|
|
delaunay_to_classical(*args, **kwargs)
|
Overloaded function. |
east_north_up_to_az_el_range(*args, **kwargs)
|
Overloaded function. |
east_north_up_to_cart(*args, **kwargs)
|
Overloaded function. |
ecc2true(E, e)
|
|
eccentric_to_mean_anomaly(*args, **kwargs)
|
Overloaded function. |
eccentric_to_true_anomaly(*args, **kwargs)
|
Overloaded function. |
equinoctial_to_classical(*args, **kwargs)
|
Overloaded function. |
find_file_in_dir(*args, **kwargs)
|
Overloaded function. |
gcpm_v24(datetime, r_RE, amlt, alatr[, akp])
|
C++ GCPM v2.4: returns [ne_cm3, H+, He+, O+]. |
gcpm_v24_fortran(datetime, r_RE, amlt, alatr)
|
Fortran GCPM v2.4: returns [ne_cm3, H+, He+, O+]. |
get_ascii_kernel_dir()
|
|
get_body_pos(*args, **kwargs)
|
Overloaded function. |
get_body_pos_vel(*args, **kwargs)
|
Overloaded function. |
get_cspice_kernel_dir()
|
|
get_data_path()
|
|
get_eop_data(mjd_utc)
|
|
get_eop_file_data()
|
|
get_file_path(arg0)
|
|
get_frame_center(frame)
|
|
get_frame_rotation_translation(t_tdb, ...)
|
|
get_frame_rotation_translation_rv(t_tdb, ...)
|
|
get_iono_params(t_j2000[, kp])
|
Returns [f107, rz12, hmf2_km] ionospheric parameters. |
get_iri_model()
|
|
get_kp_index(datetime)
|
|
get_lunar_orientation_angles(t_tdb)
|
Get lunar mantle rotation angles |
get_lupnt_epoch()
|
|
get_orbital_period(*args, **kwargs)
|
Overloaded function. |
get_physical_constants(*args, **kwargs)
|
Overloaded function. |
get_plasma_base_path()
|
Get the base path used to locate plasma runtime data (iri/, kp/). |
get_proper_time_correction_tcl(*args, **kwargs)
|
Overloaded function. |
gregorian_to_mjd(*args, **kwargs)
|
Overloaded function. |
gregorian_to_time(*args, **kwargs)
|
Overloaded function. |
init_default_config_search_dirs()
|
|
is_coordinate_time_scale(time)
|
|
itime_to_datetime(itime)
|
|
lat_lon_alt_to_cart(*args, **kwargs)
|
Overloaded function. |
lat_lon_alt_to_stereographic(*args, **kwargs)
|
Overloaded function. |
load_config(*args, **kwargs)
|
Overloaded function. |
load_eop_file_data(filepath[, force])
|
|
load_latest_eop_from_iers([force])
|
|
load_tiff(path, xlims, ], ylims, ], max_res)
|
|
long_to_lt(longitude)
|
|
lt_to_long(amlt)
|
|
mean2ecc(M, e)
|
|
mean2true(M, e)
|
|
mean_to_eccentric_anomaly(*args, **kwargs)
|
Overloaded function. |
mean_to_true_anomaly(*args, **kwargs)
|
Overloaded function. |
mjd_to_datetime(mjd)
|
|
mjd_to_gregorian(mjd)
|
|
mjd_to_gregorian_string(mjd[, precision])
|
|
mjd_to_time(mjd)
|
|
mjd_to_tj2000(mjd)
|
|
normalize_quat(*args, **kwargs)
|
Overloaded function. |
propagate_coe(coe, GM, dt)
|
|
quasi_nonsingular_to_classical(*args, **kwargs)
|
Overloaded function. |
quat_to_rot(qw)
|
|
refractive_index_neB(ne_m3, freq_Hz[, B, ...])
|
Refractive index of the ionosphere for given ne and frequency. |
roll_pitch_yaw_to_rot(rpy)
|
|
rot_to_quat(rot)
|
|
rot_to_roll_pitch_yaw(rot)
|
|
rot_x(angle)
|
|
rot_y(angle)
|
|
rot_z(angle)
|
|
rotation_angle(R)
|
|
save_config(config, path)
|
|
scalar_first_to_last(*args, **kwargs)
|
Overloaded function. |
scalar_last_to_first(*args, **kwargs)
|
Overloaded function. |
scale_gm_for_coordinate_scale(value, from, to)
|
|
scale_length_for_coordinate_scale(value, ...)
|
|
set_iri2007_option(option)
|
|
set_iri2020_option(option)
|
|
set_iri_model([model_name])
|
|
set_lupnt_epoch(arg0)
|
|
set_plasma_base_path(path)
|
Override the base path used to locate plasma runtime data. |
setup_gnss_constellation(filename)
|
|
skew(x)
|
|
solve_lt(sat, rx_pos, epoch_utc_rx)
|
|
stereographic_to_cart(*args, **kwargs)
|
Overloaded function. |
stereographic_to_lat_lon_alt(*args, **kwargs)
|
Overloaded function. |
tcb_to_tcl(*args, **kwargs)
|
Overloaded function. |
tcl_to_tcb(*args, **kwargs)
|
Overloaded function. |
time_to_gregorian_string(t[, precision])
|
|
time_to_mjd(t)
|
|
tj2000_to_mjd(t_j2000)
|
|
tle_to_classical(arg0, arg1)
|
GM |
trace_ray(epoch, pos_tx, pos_rx, config[, ...])
|
Trace a ray from pos_tx to pos_rx and return a PathProfile. |
true2mean(nu, e)
|
|
true_to_eccentric_anomaly(*args, **kwargs)
|
Overloaded function. |
true_to_mean_anomaly(*args, **kwargs)
|
Overloaded function. |
wrap2pi(angle)
|
|
wrap_to_pi(*args, **kwargs)
|
Overloaded function. |
wrap_to_two_pi(*args, **kwargs)
|
Overloaded function. |