Epochs
AstroTime.Epochs.Epoch
— TypeEpoch(str[, format])
Construct an Epoch
from a string str
. Optionally a format
definition can be passed as a DateFormat
object or as a string. In addition to the character codes supported by DateFormat
the character code D
is supported which is parsed as "day of year" (see the example below) and the character code t
which is parsed as the time scale. The default format is yyyy-mm-ddTHH:MM:SS.sss ttt
.
Note: Please be aware that this constructor requires that the time scale is part of str
, e.g. 2018-02-06T00:00 TAI
. Otherwise use an explicit constructor, e.g. Epoch{TAI}
.
Example
julia> Epoch("2018-02-06T20:45:00.0 TAI")
2018-02-06T20:45:00.000 TAI
julia> Epoch("2018-037T00:00 TAI", "yyyy-DDDTHH:MM ttt")
2018-02-06T00:00:00.000 TAI
AstroTime.Epochs.Epoch
— MethodEpoch{S}(str[, format]) where S
Construct an Epoch
with time scale S
from a string str
. Optionally a format
definition can be passed as a DateFormat
object or as a string. In addition to the character codes supported by DateFormat
the code D
can be used which is parsed as "day of year" (see the example below). The default format is yyyy-mm-ddTHH:MM:SS.sss
.
Example
julia> Epoch{InternationalAtomicTime}("2018-02-06T20:45:00.0")
2018-02-06T20:45:00.000 TAI
julia> Epoch{InternationalAtomicTime}("February 6, 2018", "U d, y")
2018-02-06T00:00:00.000 TAI
julia> Epoch{InternationalAtomicTime}("2018-037T00:00", "yyyy-DDDTHH:MM")
2018-02-06T00:00:00.000 TAI
AstroTime.Epochs.Epoch
— MethodEpoch{S2}(ep::Epoch{S1}) where {S1, S2}
Convert ep
, an Epoch
with time scale S1
, to an Epoch
with time scale S2
.
Examples
julia> ep = TTEpoch(2000,1,1)
2000-01-01T00:00:00.000 TT
julia> TAIEpoch(ep)
1999-12-31T23:59:27.816 TAI
AstroTime.Epochs.Epoch
— MethodEpoch{S}(year, month, day, hour=0, minute=0, second=0.0) where S
Construct an Epoch
with time scale S
from date and time components.
Example
julia> Epoch{InternationalAtomicTime}(2018, 2, 6, 20, 45, 0.0)
2018-02-06T20:45:00.000 TAI
julia> Epoch{InternationalAtomicTime}(2018, 2, 6)
2018-02-06T00:00:00.000 TAI
AstroTime.Epochs.Epoch
— MethodEpoch{S}(Δtai, ep::TAIEpoch) where S
Convert ep
, a TAIEpoch
, to an Epoch
with time scale S
by overriding the offset between S2
and TAI
with Δtai
.
Examples
julia> ep = TAIEpoch(2000,1,1)
2000-01-01T00:00:00.000 TAI
julia> TTEpoch(32.184, ep)
2000-01-01T00:00:32.184 TT
AstroTime.Epochs.Epoch
— MethodEpoch(ep::Epoch{S1}, scale::S2) where {S1, S2}
Convert ep
, an Epoch
with time scale S1
, to an Epoch
with time scale S2
.
Examples
julia> ep = TTEpoch(2000,1,1)
2000-01-01T00:00:00.000 TT
julia> Epoch(ep, TAI)
1999-12-31T23:59:27.816 TAI
AstroTime.Epochs.Epoch
— MethodEpoch{S}(jd1::T, jd2::T=zero(T); origin=:j2000) where {S, T<:AstroPeriod}
Construct an Epoch
with time scale S
from a Julian date (optionally split into jd1
and jd2
). origin
determines the variant of Julian date that is used. Possible values are:
:j2000
: J2000 Julian date, starts at2000-01-01T12:00
:julian
: Julian date, starts at-4712-01-01T12:00
:modified_julian
: Modified Julian date, starts at1858-11-17T00:00
Examples
julia> Epoch{InternationalAtomicTime}(0.0days, 0.5days)
2000-01-02T00:00:00.000 TAI
julia> Epoch{InternationalAtomicTime}(2.451545e6days, origin=:julian)
2000-01-01T12:00:00.000 TAI
AstroTime.Epochs.TAIEpoch
— MethodTAIEpoch(str[, format])
Construct a TAIEpoch from a string str
. Optionally a format
definition can be passed as a DateFormat
object or as a string. In addition to the character codes supported by DateFormat
the code D
is supported which is parsed as "day of year" (see the example below). The default format is yyyy-mm-ddTHH:MM:SS.sss
.
Example
julia> TAIEpoch("2018-02-06T20:45:00.0")
2018-02-06T20:45:00.000 TAI
julia> TAIEpoch("February 6, 2018", "U d, y")
2018-02-06T00:00:00.000 TAI
julia> TAIEpoch("2018-37T00:00", "yyyy-DDDTHH:MM")
2018-02-06T00:00:00.000 TAI
AstroTime.Epochs.TAIEpoch
— MethodTAIEpoch(year, month, day, hour=0, minute=0, second=0.0)
Construct a TAIEpoch from date and time components.
Example
julia> TAIEpoch(2018, 2, 6, 20, 45, 0.0)
2018-02-06T20:45:00.000 TAI
julia> TAIEpoch(2018, 2, 6)
2018-02-06T00:00:00.000 TAI
AstroTime.Epochs.TAIEpoch
— MethodTAIEpoch(jd1::T, jd2::T=zero(T); origin=:j2000) where T<:AstroPeriod
Construct a TAIEpoch from a Julian date (optionally split into jd1
and jd2
). origin
determines the variant of Julian date that is used. Possible values are:
:j2000
: J2000 Julian date, starts at2000-01-01T12:00
:julian
: Julian date, starts at-4712-01-01T12:00
:modified_julian
: Modified Julian date, starts at1858-11-17T00:00
Examples
julia> TAIEpoch(0.0days, 0.5days)
2000-01-02T00:00:00.000 TAI
julia> TAIEpoch(2.451545e6days, origin=:julian)
2000-01-01T12:00:00.000 TAI
AstroTime.Epochs.TCBEpoch
— MethodTCBEpoch(str[, format])
Construct a TCBEpoch from a string str
. Optionally a format
definition can be passed as a DateFormat
object or as a string. In addition to the character codes supported by DateFormat
the code D
is supported which is parsed as "day of year" (see the example below). The default format is yyyy-mm-ddTHH:MM:SS.sss
.
Example
julia> TCBEpoch("2018-02-06T20:45:00.0")
2018-02-06T20:45:00.000 TCB
julia> TCBEpoch("February 6, 2018", "U d, y")
2018-02-06T00:00:00.000 TCB
julia> TCBEpoch("2018-37T00:00", "yyyy-DDDTHH:MM")
2018-02-06T00:00:00.000 TCB
AstroTime.Epochs.TCBEpoch
— MethodTCBEpoch(year, month, day, hour=0, minute=0, second=0.0)
Construct a TCBEpoch from date and time components.
Example
julia> TCBEpoch(2018, 2, 6, 20, 45, 0.0)
2018-02-06T20:45:00.000 TCB
julia> TCBEpoch(2018, 2, 6)
2018-02-06T00:00:00.000 TCB
AstroTime.Epochs.TCBEpoch
— MethodTCBEpoch(jd1::T, jd2::T=zero(T); origin=:j2000) where T<:AstroPeriod
Construct a TCBEpoch from a Julian date (optionally split into jd1
and jd2
). origin
determines the variant of Julian date that is used. Possible values are:
:j2000
: J2000 Julian date, starts at2000-01-01T12:00
:julian
: Julian date, starts at-4712-01-01T12:00
:modified_julian
: Modified Julian date, starts at1858-11-17T00:00
Examples
julia> TCBEpoch(0.0days, 0.5days)
2000-01-02T00:00:00.000 TCB
julia> TCBEpoch(2.451545e6days, origin=:julian)
2000-01-01T12:00:00.000 TCB
AstroTime.Epochs.TCGEpoch
— MethodTCGEpoch(str[, format])
Construct a TCGEpoch from a string str
. Optionally a format
definition can be passed as a DateFormat
object or as a string. In addition to the character codes supported by DateFormat
the code D
is supported which is parsed as "day of year" (see the example below). The default format is yyyy-mm-ddTHH:MM:SS.sss
.
Example
julia> TCGEpoch("2018-02-06T20:45:00.0")
2018-02-06T20:45:00.000 TCG
julia> TCGEpoch("February 6, 2018", "U d, y")
2018-02-06T00:00:00.000 TCG
julia> TCGEpoch("2018-37T00:00", "yyyy-DDDTHH:MM")
2018-02-06T00:00:00.000 TCG
AstroTime.Epochs.TCGEpoch
— MethodTCGEpoch(year, month, day, hour=0, minute=0, second=0.0)
Construct a TCGEpoch from date and time components.
Example
julia> TCGEpoch(2018, 2, 6, 20, 45, 0.0)
2018-02-06T20:45:00.000 TCG
julia> TCGEpoch(2018, 2, 6)
2018-02-06T00:00:00.000 TCG
AstroTime.Epochs.TCGEpoch
— MethodTCGEpoch(jd1::T, jd2::T=zero(T); origin=:j2000) where T<:AstroPeriod
Construct a TCGEpoch from a Julian date (optionally split into jd1
and jd2
). origin
determines the variant of Julian date that is used. Possible values are:
:j2000
: J2000 Julian date, starts at2000-01-01T12:00
:julian
: Julian date, starts at-4712-01-01T12:00
:modified_julian
: Modified Julian date, starts at1858-11-17T00:00
Examples
julia> TCGEpoch(0.0days, 0.5days)
2000-01-02T00:00:00.000 TCG
julia> TCGEpoch(2.451545e6days, origin=:julian)
2000-01-01T12:00:00.000 TCG
AstroTime.Epochs.TDBEpoch
— MethodTDBEpoch(str[, format])
Construct a TDBEpoch from a string str
. Optionally a format
definition can be passed as a DateFormat
object or as a string. In addition to the character codes supported by DateFormat
the code D
is supported which is parsed as "day of year" (see the example below). The default format is yyyy-mm-ddTHH:MM:SS.sss
.
Example
julia> TDBEpoch("2018-02-06T20:45:00.0")
2018-02-06T20:45:00.000 TDB
julia> TDBEpoch("February 6, 2018", "U d, y")
2018-02-06T00:00:00.000 TDB
julia> TDBEpoch("2018-37T00:00", "yyyy-DDDTHH:MM")
2018-02-06T00:00:00.000 TDB
AstroTime.Epochs.TDBEpoch
— MethodTDBEpoch(year, month, day, hour=0, minute=0, second=0.0)
Construct a TDBEpoch from date and time components.
Example
julia> TDBEpoch(2018, 2, 6, 20, 45, 0.0)
2018-02-06T20:45:00.000 TDB
julia> TDBEpoch(2018, 2, 6)
2018-02-06T00:00:00.000 TDB
AstroTime.Epochs.TDBEpoch
— MethodTDBEpoch(jd1::T, jd2::T=zero(T); origin=:j2000) where T<:AstroPeriod
Construct a TDBEpoch from a Julian date (optionally split into jd1
and jd2
). origin
determines the variant of Julian date that is used. Possible values are:
:j2000
: J2000 Julian date, starts at2000-01-01T12:00
:julian
: Julian date, starts at-4712-01-01T12:00
:modified_julian
: Modified Julian date, starts at1858-11-17T00:00
Examples
julia> TDBEpoch(0.0days, 0.5days)
2000-01-02T00:00:00.000 TDB
julia> TDBEpoch(2.451545e6days, origin=:julian)
2000-01-01T12:00:00.000 TDB
AstroTime.Epochs.TTEpoch
— MethodTTEpoch(str[, format])
Construct a TTEpoch from a string str
. Optionally a format
definition can be passed as a DateFormat
object or as a string. In addition to the character codes supported by DateFormat
the code D
is supported which is parsed as "day of year" (see the example below). The default format is yyyy-mm-ddTHH:MM:SS.sss
.
Example
julia> TTEpoch("2018-02-06T20:45:00.0")
2018-02-06T20:45:00.000 TT
julia> TTEpoch("February 6, 2018", "U d, y")
2018-02-06T00:00:00.000 TT
julia> TTEpoch("2018-37T00:00", "yyyy-DDDTHH:MM")
2018-02-06T00:00:00.000 TT
AstroTime.Epochs.TTEpoch
— MethodTTEpoch(year, month, day, hour=0, minute=0, second=0.0)
Construct a TTEpoch from date and time components.
Example
julia> TTEpoch(2018, 2, 6, 20, 45, 0.0)
2018-02-06T20:45:00.000 TT
julia> TTEpoch(2018, 2, 6)
2018-02-06T00:00:00.000 TT
AstroTime.Epochs.TTEpoch
— MethodTTEpoch(jd1::T, jd2::T=zero(T); origin=:j2000) where T<:AstroPeriod
Construct a TTEpoch from a Julian date (optionally split into jd1
and jd2
). origin
determines the variant of Julian date that is used. Possible values are:
:j2000
: J2000 Julian date, starts at2000-01-01T12:00
:julian
: Julian date, starts at-4712-01-01T12:00
:modified_julian
: Modified Julian date, starts at1858-11-17T00:00
Examples
julia> TTEpoch(0.0days, 0.5days)
2000-01-02T00:00:00.000 TT
julia> TTEpoch(2.451545e6days, origin=:julian)
2000-01-01T12:00:00.000 TT
AstroTime.Epochs.UT1Epoch
— MethodUT1Epoch(str[, format])
Construct a UT1Epoch from a string str
. Optionally a format
definition can be passed as a DateFormat
object or as a string. In addition to the character codes supported by DateFormat
the code D
is supported which is parsed as "day of year" (see the example below). The default format is yyyy-mm-ddTHH:MM:SS.sss
.
Example
julia> UT1Epoch("2018-02-06T20:45:00.0")
2018-02-06T20:45:00.000 UT1
julia> UT1Epoch("February 6, 2018", "U d, y")
2018-02-06T00:00:00.000 UT1
julia> UT1Epoch("2018-37T00:00", "yyyy-DDDTHH:MM")
2018-02-06T00:00:00.000 UT1
AstroTime.Epochs.UT1Epoch
— MethodUT1Epoch(year, month, day, hour=0, minute=0, second=0.0)
Construct a UT1Epoch from date and time components.
Example
julia> UT1Epoch(2018, 2, 6, 20, 45, 0.0)
2018-02-06T20:45:00.000 UT1
julia> UT1Epoch(2018, 2, 6)
2018-02-06T00:00:00.000 UT1
AstroTime.Epochs.UT1Epoch
— MethodUT1Epoch(jd1::T, jd2::T=zero(T); origin=:j2000) where T<:AstroPeriod
Construct a UT1Epoch from a Julian date (optionally split into jd1
and jd2
). origin
determines the variant of Julian date that is used. Possible values are:
:j2000
: J2000 Julian date, starts at2000-01-01T12:00
:julian
: Julian date, starts at-4712-01-01T12:00
:modified_julian
: Modified Julian date, starts at1858-11-17T00:00
Examples
julia> UT1Epoch(0.0days, 0.5days)
2000-01-02T00:00:00.000 UT1
julia> UT1Epoch(2.451545e6days, origin=:julian)
2000-01-01T12:00:00.000 UT1
AstroTime.AstroDates.fractionofday
— Methodfractionofday(ep::Epoch)
Get the time of the day of the epoch ep
as a fraction.
AstroTime.AstroDates.fractionofsecond
— Methodfractionofsecond(ep::Epoch)
Get the fraction of the current second of the epoch ep
.
AstroTime.AstroDates.j2000
— Methodj2000(ep)
Return the J2000 Julian Date for epoch ep
.
Example
julia> j2000(TAIEpoch(2000, 1, 1, 12))
0.0 days
AstroTime.AstroDates.julian
— Methodjulian(ep)
Return the Julian Date for epoch ep
.
Example
julia> julian(TAIEpoch(2000, 1, 1, 12))
2.451545e6 days
AstroTime.AstroDates.julian_twopart
— Methodjulian_twopart(ep)
Return the two-part Julian Date for epoch ep
, which is a tuple consisting of the Julian day number and the fraction of the day.
Example
julia> julian_twopart(TAIEpoch(2000, 1, 2))
(2.451545e6 days, 0.5 days)
AstroTime.AstroDates.subsecond
— Methodsubsecond(ep::Epoch, n)
Get the number of fractional seconds with the unit $s * \frac{1}{10^n}$, e.g. subsecond(ep, 3)
for milliseconds, of the epoch ep
. n
must be divisible by 3.
AstroTime.Epochs.from_utc
— Functionfrom_utc(str::AbstractString, dateformat::Dates.DateFormat; scale=TAI)
from_utc(dt::Dates.DateTime; scale=TAI)
from_utc(year, month, day, hour=0, minute=0, second=0, fraction=0.0; scale=TAI)
from_utc(year, month, day, hour, minute, seconds; scale=TAI)
Create an Epoch
in scale
based on a UTC timestamp, Dates.DateTime
or date and time components.
Examples
julia> from_utc(2016, 12, 31, 23, 59, 60, 0.0)
2017-01-01T00:00:36.000 TAI
julia> from_utc(2016, 12, 31, 23, 59, 60.0)
2017-01-01T00:00:36.000 TAI
julia> from_utc("2016-12-31T23:59:60.0")
2017-01-01T00:00:36.000 TAI
julia> from_utc("2016-12-31T23:59:60.0", scale=TDB)
2017-01-01T00:01:08.183 TDB
AstroTime.Epochs.getoffset
— Functiongetoffset(UT1, TAI, second, fraction[, eop])
Return the offset between UT1
and TAI
for the current epoch (second
after J2000 and fraction
) in seconds. Optionally, a custom Earth orientation data struct eop
can be provided, see EarthOrientation.jl.
Example
julia> getoffset(UT1, TAI, 0, 0.0)
31.644974965344606
AstroTime.Epochs.getoffset
— Functiongetoffset(TAI, UT1, second, fraction[, eop])
Return the offset between TAI
and UT1
for the current epoch (second
after J2000 and fraction
) in seconds. Optionally, a custom Earth orientation data struct eop
can be provided, see EarthOrientation.jl.
Example
julia> getoffset(TAI, UT1, 0, 0.0)
-31.644974644349812
AstroTime.Epochs.getoffset
— Methodgetoffset(TCB, TDB, second, fraction)
Return the linear offset between TCB
and TDB
for the current epoch (second
after J2000 and fraction
) in seconds.
Example
julia> getoffset(TCB, TDB, 0, 0.0)
-11.253721593757295
AstroTime.Epochs.getoffset
— Methodgetoffset(TDB, TCB, second, fraction)
Return the linear offset between TDB
and TCB
for the current epoch (second
after J2000 and fraction
) in seconds.
Example
julia> getoffset(TDB, TCB, 0, 0.0)
11.253721768248475
AstroTime.Epochs.getoffset
— Methodgetoffset(TDB, TT, second, fraction[, eop])
Return the offset between TDB
and TT
for the current epoch (second
after J2000 and fraction
) for an observer on earth in seconds.
Arguments
second
,fraction
: Current epochelong
: Longitude (east positive, radians)u
: Distance from Earth's spin axis (km)v
: Distance north of equatorial plane (km)
Example
julia> getoffset(TDB, TT, 0, 0.0, π, 6371.0, 0.0)
9.928419814106208e-5
References
AstroTime.Epochs.getoffset
— Methodgetoffset(TDB, TT, second, fraction[, eop])
Return the offset between TDB
and TT
for the current epoch (second
after J2000 and fraction
) in seconds. This routine is accurate to ~40 microseconds over the interval 1900-2100.
An accurate transformation between TDB and TT depends on the trajectory of the observer. For two observers fixed on Earth's surface the quantity TDB-TT can differ by as much as ~4 microseconds. See here
.
Example
julia> getoffset(TDB, TT, 0, 0.0)
7.273677616693264e-5
References
AstroTime.Epochs.getoffset
— Methodgetoffset(TCG, TT, second, fraction)
Return the linear offset between TCG
and TT
for the current epoch (second
after J2000 and fraction
) in seconds.
Example
julia> getoffset(TCG, TT, 0, 0.0)
-0.5058332856685995
AstroTime.Epochs.getoffset
— Methodgetoffset(TAI, TT, args...)
Return the fixed offset between TAI
and TT
in seconds.
Example
julia> getoffset(TAI, TT)
32.184
AstroTime.Epochs.getoffset
— Methodgetoffset(TT, TDB, second, fraction[, eop])
Return the offset between TT
and TDB
for the current epoch (second
after J2000 and fraction
) for an observer on earth in seconds.
Arguments
second
,fraction
: Current epochelong
: Longitude (east positive, radians)u
: Distance from Earth's spin axis (km)v
: Distance north of equatorial plane (km)
Example
julia> getoffset(TT, TDB, 0, 0.0, π, 6371.0, 0.0)
-9.928419818977206e-5
References
AstroTime.Epochs.getoffset
— Methodgetoffset(TT, TDB, second, fraction[, eop])
Return the offset between TT
and TDB
for the current epoch (second
after J2000 and fraction
) in seconds. This routine is accurate to ~40 microseconds over the interval 1900-2100.
An accurate transformation between TDB and TT depends on the trajectory of the observer. For two observers fixed on Earth's surface the quantity TDB-TT can differ by as much as ~4 microseconds. See here
.
Example
julia> getoffset(TT, TDB, 0, 0.0)
-7.273677619130569e-5
References
AstroTime.Epochs.getoffset
— Methodgetoffset(TT, TCG, second, fraction)
Return the linear offset between TT
and TCG
for the current epoch (second
after J2000 and fraction
) in seconds.
Example
julia> getoffset(TT, TCG, 0, 0.0)
0.5058332860211293
AstroTime.Epochs.getoffset
— Methodgetoffset(TT, TAI, args...)
Return the fixed offset between TT
and TAI
in seconds.
Example
julia> getoffset(TT, TAI)
-32.184
AstroTime.Epochs.getoffset
— Methodgetoffset(ep::Epoch, scale::TimeScale)
For a given epoch ep
return the offset between its time scale and another time scale
in seconds.
Example
julia> tai = TAIEpoch(2000, 1, 1)
2000-01-01T00:00:00.000 TAI
julia> getoffset(tai, TT)
32.184
AstroTime.Epochs.julian_period
— Methodjulian_period([T,] ep::Epoch; origin=:j2000, scale=timescale(ep), unit=days)
Return the period since Julian Epoch origin
within the time scale scale
expressed in unit
for a given epoch ep
. The result is an AstroPeriod
object by default. If the type argument T
is present, the result is converted to T
instead.
Example
julia> ep = TAIEpoch(2018, 2, 6, 20, 45, 0.0)
2018-02-06T20:45:00.000 TAI
julia> julian_period(ep; scale=TT)
6611.364955833334 days
julia> julian_period(ep; unit=years)
18.100929728496464 years
julia> julian_period(Float64, ep)
6611.364583333333
AstroTime.Epochs.modified_julian
— Methodmodified_julian(ep)
Return the Modified Julian Date for epoch ep
.
Example
julia> modified_julian(TAIEpoch(2000, 1, 1, 12))
51544.5 days
AstroTime.Epochs.timescale
— Methodtimescale(ep)
Return the time scale of epoch ep
.
Example
julia> ep = TTEpoch(2000, 1, 1)
2000-01-01T00:00:00.000 TT
julia> timescale(ep)
TT
AstroTime.Epochs.to_utc
— Functionto_utc(ep)
to_utc(::Type{DateTime}, ep)
to_utc(::Type{Dates.DateTime}, ep)
to_utc(::Type{String}, ep, dateformat=Dates.default_format(DateTime))
Create a UTC timestamp or Dates.DateTime
from an Epoch
ep
.
Examples
julia> tai = from_utc(Dates.DateTime(2018, 2, 6, 20, 45, 0, 0))
2018-02-06T20:45:37.000 TAI
julia> to_utc(tai)
"2018-02-06T20:45:00.000"
julia> to_utc(String, tai, Dates.dateformat"yyyy-mm-dd")
"2018-02-06"
julia> to_utc(Dates.DateTime, tai)
2018-02-06T20:45:00
Base.:-
— Method-(a::Epoch, b::Epoch)
Return the duration between epoch a
and epoch b
.
Examples
julia> TAIEpoch(2018, 2, 6, 20, 45, 20.0) - TAIEpoch(2018, 2, 6, 20, 45, 0.0)
20.0 seconds
Dates.day
— Methodday(ep::Epoch)
Get the day of the epoch ep
.
Dates.dayofyear
— Methoddayofyear(ep::Epoch)
Get the day of the year of the epoch ep
.
Dates.hour
— Methodhour(ep::Epoch)
Get the hour of the epoch ep
.
Dates.microsecond
— Methodmicrosecond(ep::Epoch)
Get the number of microseconds of the epoch ep
.
Dates.millisecond
— Methodmillisecond(ep::Epoch)
Get the number of milliseconds of the epoch ep
.
Dates.minute
— Methodminute(ep::Epoch)
Get the minute of the epoch ep
.
Dates.month
— Methodmonth(ep::Epoch)
Get the month of the epoch ep
.
Dates.nanosecond
— Methodnanosecond(ep::Epoch)
Get the number of nanoseconds of the epoch ep
.
Dates.now
— Methodnow(::Type{Epoch})
now(::Type{Epoch{S}}) where S<:TimeScale
Get the current date and time as an Epoch
. The default time scale is TAI.
Example
julia> now(Epoch)
2021-04-11T13:20:29.160 TAI
julia> now(TDBEpoch)
2021-04-11T13:21:21.518 TDB
Dates.second
— Methodsecond(type, ep::Epoch)
Get the second of the epoch ep
as a type
.
Dates.second
— Methodsecond(ep::Epoch) -> Int
Get the second of the epoch ep
as an Int
.
Dates.year
— Methodyear(ep::Epoch)
Get the year of the epoch ep
.
Dates.yearmonthday
— Methodyearmonthday(ep::Epoch)
Get the year, month, and day of the epoch ep
as a tuple.
AstroTime.AstroDates.DateTime
— TypeDateTime(ep::Epoch)
Convert the epoch ep
to an AstroDates.DateTime
.
AstroTime.AstroDates.Date
— TypeDate(ep::Epoch)
Get the Date
of the epoch ep
.
AstroTime.AstroDates.Time
— TypeTime(ep::Epoch)
Get the Time
of the epoch ep
.