R1i xdZddlZddlZddlmZmZGddejZeZ dZ dZ da d d Z y) zVarious conveniences. Higher-level libraries like Skyfield that use this one usually have their own date and time handling. But for folks using this library by itself, native Python datetime handling could be convenient. N) days2mdhmsjdaycLeZdZdZej dZdZdZdZ dZ y)_UTCUTCrcyNr)selfs U/home/cursorai/projects/iching/venv/lib/python3.12/site-packages/sgp4/conveniences.py__repr__z _UTC.__repr__c|jSNzeror datetimes r dstz_UTC.dst yyrcyr r rs r tznamez _UTC.tznamerrc|jSrrrs r utcoffsetz_UTC.utcoffsetrrN) __name__ __module__ __qualname____doc__dt timedeltarrrrrr rr rr s( 2<<?Drrc|jt}|j}|j}|j}|j }|j }|j|jdzz}t||||||S)aReturn two floats that, when added, produce the specified Julian date. The first float returned gives the date, while the second float provides an additional offset for the particular hour, minute, and second of that date. Because the second float is much smaller in magnitude it can, unlike the first float, be accurate down to very small fractions of a second. >>> jd, fr = jday(2020, 2, 11, 13, 57, 0) >>> jd 2458890.5 >>> fr 0.58125 Note that the first float, which gives the moment of midnight that commences the given calendar date, always carries the fraction ``.5`` because Julian dates begin and end at noon. This made Julian dates more convenient for astronomers in Europe, by making the whole night belong to a single Julian date. The input is a native `datetime` object. Timezone of the input is converted internally to UTC. gư>) astimezoneryearmonthdayhourminutesecond microsecondr)rur%monr'hrr)secs r jday_datetimer0sm2 C A 66D ''C %%C B XXF ((Q]]T) )C c3FC 00rc .|j}|d|dkdzzz }|j}t||\}}}}}|dk(r|dkDr |dz }d}|dz}t|d\}}t |}t |dz} t j ||||||| tS) z=Return the epoch of the given satellite as a Python datetime.il9d rg?g.A)epochyr epochdaysrdivmodintr!rr) satr%daysr&r'r(r)r*fractionmicros r sat_epoch_datetimer>=s ;;DDD2I$ $$D ==D'1$'=$E3ff {sRx   r fc*FH [F 3 E ;;tUCvvuc JJrc#KtgatjjD]}|j dr'|j d}tj |;|jdsM|jd}tj |dd}||dk(stj ||dz|dz }||dk(r)tD]}|djr|}d d j|0|}t||d }d j||}|,t||d } || k(rd nd} dj|dd| | }|yw)z>Yield lines that list the attributes of one or two satellites.N*z| ``z``rz, r z# -------- {0} -------- z (not set)z {0} = {1!r} z==z!=z{0:39} {1} {2!r} ) _ATTRIBUTESsgp4r splitlinesendswithstripappend startswithsplitisupperformatgetattr) r:sat2linetitlepiecesiitemnamevaluevalue2verdicts r dump_satrecrYNsU LL++-D}}S! 3""5)(D)""6!9-Qi4'&&vac{3FAQi4'. 7?? EJ-44U; ;DC{3E"))$6D t[9#(F?$+2249gvNJsA3E!63E!*(E!BE!r)r rr!rE functionsrrtzinforrr0r>rDrYr rr r\sF ' 299  f!1F K r