R1idddlmZGddejZGddejZy)) vallado_cppceZdZdZdZdZy)Satrecz=High-speed computation of satellite positions and velocities.c|jdd}|jdd}|j}|ddf}t|}||d}||d}||d}|j||||||||fS)aCompute positions and velocities for the times in a NumPy array. Given NumPy arrays ``jd`` and ``fr`` of the same length that supply the whole part and the fractional part of one or more Julian dates, return a tuple ``(e, r, v)`` of three vectors: * ``e``: nonzero for any dates that produced errors, 0 otherwise. * ``r``: position vectors in kilometers. * ``v``: velocity vectors in kilometers per second. float64Fcopyuint8)astypeshapetype_sgp4) selfjdfreshapefshapearrayervs P/home/cursorai/projects/iching/venv/lib/python3.12/site-packages/sgp4/wrapper.py sgp4_arrayzSatrec.sgp4_arraysYYyuY - YYyuY -AR &' " &) $ &) $ 2r1a#!QwN)__name__ __module__ __qualname____doc__ __slots__rrrrrrsGIrrceZdZdZdZdZy) SatrecArrayzBHigh-speed satellite array for computing positions and velocities.rc|jdd}|jdd}t|}|j\}||f}||df}t|}||d}||d} ||d} |j |||| | || | fS)aCompute positions and velocities for the satellites in this array. Given NumPy scalars or arrays ``jd`` and ``fr`` supplying the whole part and the fractional part of one or more Julian dates, return a tuple ``(e, r, v)`` of three vectors: * ``e``: nonzero for any dates that produced errors, 0 otherwise. * ``r``: position vectors in kilometers. * ``v``: velocity vectors in kilometers per second. The first dimension of each output vector has the same length as this satellite array, the second dimension the same length as the input date arrays, and the third dimension has length 3. rFr r r )rlenrrr) rrrilengthjlengthrrrrrrs rsgp4zSatrecArray.sgp4&s YYyuY - YYyuY -d)88'!'1$R &' " &) $ &) $ 2r1a#!QwrN)rrr r!r"r)rrrr$r$!sLIrr$N)rrr$rrrr+s,[  <"+))"r