Commit 01596787 authored by Kelvin Rodriguez's avatar Kelvin Rodriguez
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added mars date support

parent a722d7c6
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plio/date/marstime.py

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'''
Borrowed from Dave Pawlowski.
(http://marstiming.readthedocs.io/en/latest/_modules/marstiming.html)

Mars timing information based on MARS24: http://www.giss.nasa.gov/tools/mars24/help/algorithm.html

Contains several functions for calculating Mars time parameters from Earth time and vice versa.
Probably the most useful functions are:
getMTfromTime: gets mars time data given a 6 element time list
getSZAfromTime: gets the SZA from a 6 element time list and coordinates
getLTfromTime: gets the LTST from a 6 element time list and longitude
getUTCfromLS: Estimates the Earth time from LS and a Mars year
'''

import datetime
from numpy import pi, floor,array,shape, cos, sin,ceil,arcsin,arccos,arange,abs
from collections import namedtuple


d2R = pi/180.

def getJD(iTime):
	'''Get the Julian date in seconds'''

	offset = 2440587.5 #JD on 1/1/1970 00:00:00

	year = iTime[0]
	month = iTime[1]
	day = iTime[2]
	hour = iTime[3]
	minute = iTime[4]
	sec = iTime[5]
	date = datetime.datetime(year,month,day,hour,minute,sec)

	iTime = [1970,1,1,0,0,0]
	year = iTime[0]
	month = iTime[1]
	day = iTime[2]
	hour = iTime[3]
	minute = iTime[4]
	sec = iTime[5]
	ref = datetime.datetime(year,month,day,hour,minute,sec)
	deltaTime = (date-ref)
	return deltaTime.total_seconds()/86400. + offset



def getUTC(jd):
	'''Get UTC given jd'''

	offset = 2440587.5 #JD on 1/1/1970 00:00:00

	iTime = [1970,1,1,0,0,0]
	year = iTime[0]
	month = iTime[1]
	day = iTime[2]
	hour = iTime[3]
	minute = iTime[4]
	sec = iTime[5]

	d1970 = datetime.datetime(year,month,day,hour,minute,sec)
	return d1970 + datetime.timedelta(seconds=((jd-offset)*86400.))


def getJ2000(iTime):
	'''get date in J2000 epoch.'''
	jd = getJD(iTime)
	T = (jd - 2451545.0)/36525 if iTime[0] < 1972 else 0

	conversion = 64.184 + 59* T - 51.2* T**2 - 67.1* T**3 - 16.4* T**4

	#convert to Terrestrial Time
	jdTT = jd+(conversion/86400)

	return jdTT - 2451545.0


def testJ2000():
	iTime = [2001,11,13,2,45,2]
	testJD = getJ2000(iTime)
	callibration = 58891502.000000 #test should be this value.
	diff = testJD - callibration
	print(testJD)
	print('difference = {0}s'.format(diff))

def testUTC():
	jd = 2452226.614606
	date = getUTC(jd)

	callibration = datetime.datetime(2001,11,13,2,45,2)
	diff = callibration - date
	print(date)
	print('difference = {}'.format(diff))


def testLS():

	iTime = [2000,1,6,0,0,0]
	lsdata = getMTfromTime(iTime)
	ls = lsdata.ls
	year = lsdata.year
	callibration = 277.18677
	diff = ls - callibration
	print(ls)
	print('Difference = {:f} degrees'.format(diff))

def getMarsParams(j2000):
	'''Mars time parameters'''


	Coefs = array(
	[[0.0071,2.2353,49.409],
	[0.0057,2.7543,168.173],
	[0.0039,1.1177,191.837],
	[0.0037,15.7866,21.736],
	[0.0021,2.1354,15.704],
	[0.0020,2.4694,95.528],
	[0.0018,32.8493,49.095]])

	dims = shape(Coefs)
	#Mars mean anomaly:
	M = 19.3870 + 0.52402075 * j2000

	#angle of Fiction Mean Sun
	alpha = 270.3863 + 0.52403840*j2000

	#Perturbers
	PBS = 0
	for i in range(dims[0]):
		PBS += Coefs[i,0]*cos(((0.985626* j2000 / Coefs[i,1]) + Coefs[i,2])*d2R)

	#Equation of Center
	vMinusM = ((10.691 + 3.0e-7 *j2000)*sin(M*d2R) + 0.623*sin(2*M*d2R) +
	0.050*sin(3*M*d2R) + 0.005*sin(4*M*d2R) + 0.0005*sin(5*M*d2R) + PBS)

	return M, alpha, PBS, vMinusM

def getMTfromTime(iTime):
	'''Get Mars time information.

	:param iTime: 6 element time list [y,m,d,h,m,s]
	:returns: a named tuple containing the LS value as well as
	     several parameters necessary for other calculations

	'''
	if isinstance(iTime, datetime.datetime):
		iTime = [iTime.year, iTime.month, iTime.day, iTime.hour, iTime.minute, iTime.second]

	DPY = 686.9713
	refTime = [1955,4,11,10,56,0] #Mars year 1
	rDate = getJD(refTime)
	thisTime = getJD(iTime)
	year = floor((thisTime - rDate)/DPY)+1

	j2000 = getJ2000(iTime)
	M,alpha,PBS,vMinusM = getMarsParams(j2000)

	LS = (alpha + vMinusM)

	while LS > 360:
		LS -= 360

	if LS < 0:
		LS = 360. + 360.*(LS/360. - ceil(LS/360.0))

	EOT = 2.861*sin(2*LS*d2R)-0.071*sin(4*LS*d2R)+0.002*sin(6*LS*d2R)-vMinusM

	MTC = (24*(((j2000 - 4.5)/1.027491252)+44796.0 - 0.00096 )) % 24
	subSolarLon = ((MTC+EOT*24/360.)*(360/24.)+180) % 360
	solarDec = (arcsin(0.42565*sin(LS*d2R))/d2R+0.25*sin(LS*d2R))

	data = namedtuple('data','ls year M alpha PBS vMinusM MTC EOT subSolarLon solarDec')
	d1 = data(ls = LS,year=year,M=M,alpha=alpha,PBS=PBS,vMinusM=vMinusM,MTC=MTC,EOT=EOT,
		subSolarLon=subSolarLon,solarDec=solarDec)

	return d1

def getUTCfromLS(marsyear,LS):
	'''Get a UTC starting with an estimate of LS using an orbit angle approximation
	then iteratively closing in on the correct LS by incrementing the a day first and then hour.

	:param marsyear: an int mars year
	:param ls: ls- mars solar longitude
	:returns: UTC1 (python datetime)'''

	#Get LS to within this value:
	error = 0.001
	DPY = 686.9713

	###Start with estimate

	refTime = [1955,4,11,10,56,0] #Mars year 1
	rDate = getJD(refTime)
	iTime = getUTC(rDate+(marsyear-1)*DPY) #LS 0 of given mars year

	#Now we have a guess, iterate over the day to get closer and closer.

	thisTime = [iTime.year,iTime.month,iTime.day,iTime.hour,iTime.minute,iTime.second]
	thisLS = 0

	factor = 1 #do we increment up or down?
	iTry = 0
	dt = 60 #hours.  This will get smaller as we get closer
	counter = 0
	olddiff = 1000.
	diff = 100
	while diff > error:

		iTime = iTime+factor*datetime.timedelta(hours=dt)
		thisTime = [iTime.year,iTime.month,iTime.day,iTime.hour,iTime.minute,iTime.second]
		timedata = getMTfromTime(thisTime)
		thisLS,myear = timedata.ls, timedata.year
		diff = abs(thisLS - LS)


		if diff > olddiff:
			factor = -1*factor
			counter += 1
			if counter > 1:
				dt = dt/60.

		olddiff = diff
		iTry += 1


		if iTry > 1000:
			print('Problem getting UTC from Ls in 2nd diff loop')
			print('Quitting if function getUTCfromLS...')
			exit(1)

	return iTime

def getSZAfromTime(time,lon,lat):
	'''Get SZA from Earth time and Mars coordinates.

	:param the time: [y,m,d,h,m,s] or datetime object
	:param lon: the longitude in degrees
	:param lat: the latitude in degrees
	:returns: the solar zenith angle (float)'''


	if type(time) == datetime.datetime:
		time = [time.year,time.month,time.day,time.hour,time.minute,time.second]

	timedata = getMTfromTime(time)

	SZA = arccos(sin(timedata.solarDec*d2R)*sin(lat*d2R)+
		cos(timedata.solarDec*d2R)*cos(lat*d2R)*cos((lon-timedata.subSolarLon)*d2R))/d2R

	return SZA

def SZAGetTime(sza,date, lon, lat):
	'''Find the time on a given date and location when the SZA is a given value.

	:param sza: Solar zenith angle in degrees
	:param date: [y,m,d]<
	:param lon: the longitude in degrees
	:param lat: the latitude in degrees
	:returns: A python datetime object
	'''
	thisDate = datetime.datetime(date[0],date[1],date[2])


	count = 0
	counter = 0
	error = 1
	factor = 1
	dt = 15 #minutes
	thisSza = getSZAfromTime(thisDate,lon,lat)
	diff = abs(thisSza - sza)
	while diff > error:
		thisDate += factor*datetime.timedelta(minutes=dt)
		thisSza = getSZAfromTime(thisDate,lon,lat)
		newdiff = abs(thisSza - sza)
		if newdiff > diff:
			factor = -1*factor
			counter += 1
			if counter > 1:  #Wait until counter is > 1 in case we start off going the wrong way!
				dt = dt/2.

		count += 1
		if abs(diff - newdiff)/2. < error and counter > 5:
			print('this location doesnt reach the given SZA.  Returning closest value... {:f}'.format(thisSza))
			return thisDate, thisSza

		diff = newdiff

	return thisDate, thisSza


def testSZA():
	'''test getSZAfromTime'''
	itime = [2000,1,6,0,0,0]
	lon = 0.0
	lat = 0.0
	expected = 154.26182
	sza = getSZAfromTime(itime,lon,lat)
	print(sza)
	print('Difference = {:f} degrees'.format(sza-expected))


def getLTfromTime(iTime,lon):
	'''The mars local solar time from an earth time and mars longitude.

	:param iTime: 6 element list: [y,m,d,h,m,s]
	:param lon: the longitude in degrees
	:returns: The local time (float)'''

	timedata = getMTfromTime(iTime)
	LMST = timedata.MTC-lon*(24/360.)
	LTST = LMST + timedata.EOT*(24/360.)

	return LTST

def testLTfromTime():
	'''test getLTfromTime function'''
	iTime = [2000,1,6,0,0,0]
	lon = 0.0
	LTST = getLTfromTime(iTime,lon)
	expected = 23.64847
	print(LTST)
	print('Difference = {:f} degrees'.format(LTST-expected))

def mapSZA(iTime):
	'''Create an SZA map given an Earth time

	:param iTime: 6 element list: [y,m,d,h,m,s]
	:returns: null
	'''
	import numpy as np
	from matplotlib import pyplot

	nlons = 72
	nlats = 72
	latitude = arange(nlats-1)*2.5-87.5
	longitude = arange(nlons-1)*5-175.

	SZA = np.zeros((nlats-1,nlons-1))
	for ilat in arange(nlats-1):
		for ilon in arange(nlons-1):
			SZA[ilat,ilon] = getSZAfromTime(iTime,longitude[ilon],latitude[ilat])


	pyplot.figure()
	pyplot.xlabel('Longitude')
	pyplot.ylabel('Latitude')
	levels = [0,90,180]
	cont = pyplot.contourf(longitude,latitude,SZA,30,
		cmap=pyplot.cm.gist_rainbow)
	cont2 = pyplot.contour(longitude,latitude,SZA,levels,
		linewidths=(2,),colors='black',
		linestyles=('--'))
	pyplot.clabel(cont2, fmt = '%2.1f', colors = 'black', fontsize=11)
	cb = pyplot.colorbar(cont)
	cb.set_label('Solar Zenith Angle')

	pyplot.savefig('plot.ps')
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import numpy as np
import unittest

from .. import marstime


class TestSmallJulian(unittest.TestCase):
    def runTest(self):
        earth = marstime.getUTCfromLS(24, 130)
        mars = marstime.getMTfromTime(earth)
        assert(earth.date() == marstime.getUTCfromLS(mars.year,mars.ls).date())