def fracyear_to_date(input):
try:
# Check to see if input is array. If it is, iterate through array.
N = len(input)
year = np.zeros(N)
month = np.zeros(N)
day = np.zeros(N)
for i in range(0,N):
year[i] = np.floor(input[i])
day1 = jdcal.gcal2jd(year[i],1,1) # Get length of year
day2 = jdcal.gcal2jd(year[i]+1,1,1)
dayfrac[i] = (input[i]-year[i])*float(day2[1]+day2[0]-day1[0]-day1[1])
year[i],month[i],day[i],frac = jdcal.jd2gcal(day1[0]+day1[1],dayfrac[i])
day[i] = day[i]+frac
except:
# If input has no length (i.e., it's a float), then just calculate
# the date for that number.
year = np.floor(input)
day1 = jdcal.gcal2jd(year,1,1) # Get length of year
day2 = jdcal.gcal2jd(year+1,1,1)
dayfrac = (input-year)*float(day2[1]+day2[0]-day1[0]-day1[1])
year,month,day,frac = jdcal.jd2gcal(day1[0]+day1[1],dayfrac)
day = day+frac
return year,month,day
def test_jd2gcal_fractional_day_part():
r = jd2gcal(2400000.5, 51544.0 + 0.5)
assert round(r[-1], 12) == 0.5
r = jd2gcal(2400000.5, 51544.0 + 0.245)
assert round(r[-1], 10) == round(0.245, 10)
r = jd2gcal(2400000.5, 51544.0 + 0.75)
assert round(r[-1], 12) == 0.75
def test_jd2gcal_fractional_day_part():
r = jd2gcal(2400000.5, 51544.0 + 0.5)
assert round(r[-1], 12) == 0.5
r = jd2gcal(2400000.5, 51544.0 + 0.245)
assert round(r[-1], 10) == round(0.245, 10)
r = jd2gcal(2400000.5, 51544.0 + 0.75)
assert round(r[-1], 12) == 0.75
def gregorian_date(julianDay, mjd=False):
"""
For a given Julian Day convert to Gregorian date (YYYY, MM, DD, hh, mm,
ss). Optionally convert from modified Julian Day with mjd=True).
This function is adapted to Python from the MATLAB julian2greg.m function
(http://www.mathworks.co.uk/matlabcentral/fileexchange/11410).
Parameters
----------
julianDay : ndarray
Array of Julian Days
mjd : boolean, optional
Set to True if the input is Modified Julian Days.
Returns
-------
greg : ndarray
Array of [YYYY, MM, DD, hh, mm, ss].
Example
-------
>>> greg = gregorian_date(np.array([53583.00390625, 55895.9765625]), mjd=True)
>>> greg.astype(int)
array([[2005, 8, 1, 0, 5, 37],
[2011, 11, 30, 23, 26, 15])
"""
if not mjd:
# It's easier to use jdcal in Modified Julian Day
julianDay -= 2400000.5
try:
nt = len(julianDay)
except TypeError:
nt = 1
greg = np.empty((nt, 6))
if nt == 1:
ymdf = jdcal.jd2gcal(2400000.5, julianDay)
fractionalday = ymdf[-1]
hours = int(fractionalday * 24)
minutes = int(((fractionalday * 24) - hours) * 60)
seconds = ((((fractionalday * 24) - hours) * 60) - minutes) * 60
greg = np.asarray((ymdf[0], ymdf[1], ymdf[2], hours, minutes, seconds))
else:
for ii, jj in enumerate(julianDay):
ymdf = jdcal.jd2gcal(2400000.5, jj)
greg[ii, :3] = ymdf[:3]
fractionalday = ymdf[-1]
hours = int(fractionalday * 24)
minutes = int(((fractionalday * 24) - hours) * 60)
seconds = ((((fractionalday * 24) - hours) * 60) - minutes) * 60
greg[ii, 3:] = [hours, minutes, seconds]
return greg
def gregorian_date(julianDay, mjd=False):
"""
For a given Julian Day convert to Gregorian date (YYYY, MM, DD, hh, mm,
ss). Optionally convert from modified Julian Day with mjd=True).
This function is adapted to Python from the MATLAB julian2greg.m function
(http://www.mathworks.co.uk/matlabcentral/fileexchange/11410).
Parameters
----------
julianDay : ndarray
Array of Julian Days
mjd : boolean, optional
Set to True if the input is Modified Julian Days.
Returns
-------
greg : ndarray
Array of [YYYY, MM, DD, hh, mm, ss].
Example
-------
>>> greg = gregorianDate(np.array([53583.00390625, 55895.9765625]), mjd=True)
>>> greg.astype(int)
array([[2005, 8, 1, 0, 5, 37],
[2011, 11, 30, 23, 26, 15])
"""
if not mjd:
# It's easier to use jdcal in Modified Julian Day
julianDay = julianDay + 2400000.5
try:
nt = len(julianDay)
except TypeError:
nt = 1
greg = np.empty((nt, 6))
if nt == 1:
ymdf = jdcal.jd2gcal(2400000.5, julianDay)
fractionalday = ymdf[-1]
hours = int(fractionalday * 24)
minutes = int(((fractionalday * 24) - hours) * 60)
seconds = ((((fractionalday * 24) - hours) * 60) - minutes) * 60
greg = np.asarray((ymdf[0], ymdf[1], ymdf[2], hours, minutes, seconds))
else:
for ii, jj in enumerate(julianDay):
ymdf = jdcal.jd2gcal(2400000.5, jj)
greg[ii, :3] = ymdf[:3]
fractionalday = ymdf[-1]
hours = int(fractionalday * 24)
minutes = int(((fractionalday * 24) - hours) * 60)
seconds = ((((fractionalday * 24) - hours) * 60) - minutes) * 60
greg[ii, 3:] = [hours, minutes, seconds]
return greg
def stv_downloader(request, primary_key):
"""
Download stvs as geojson.
"""
stv = SpacetimeVolume.objects.filter(pk=primary_key)
if len(stv) == 0:
return HttpResponse(status=404)
geojson = serialize(
"geojson",
stv,
geometry_field="territory",
fields=(
"start_date",
"end_date",
"entity",
"references",
"visual_center",
"related_events",
),
)
geojson = json.loads(geojson)
for features in geojson["features"]:
features["properties"]["visual_center"] = {
"type": "Feature",
"properties": None,
"geometry": json.loads(stv[0].visual_center.json),
}
features["properties"]["entity"] = {
"label": stv[0].entity.label,
"pk": stv[0].entity.pk,
}
start_date = jd2gcal(stv[0].start_date, 0)
start_string = "{}-{}-{}".format(start_date[0], start_date[1],
start_date[2])
end_date = jd2gcal(stv[0].end_date, 0)
end_string = "{}-{}-{}".format(end_date[0], end_date[1], end_date[2])
response = JsonResponse(geojson)
response[
"Content-Disposition"] = "attachment;filename={}_{}_{}.json;".format(
stv[0].entity.label, start_string, end_string)
return response
def get_date_time(julian_day):
# take in floating Julian day and return a date and time as a single string
diff = julian_day - 240000.5
date = jdcal.jd2gcal(240000.5, diff)
year = str(date[0])
month = str(date[1])
day = str(date[2])
if len(month) == 1:
month = '0' + month
if len(day) == 1:
day = '0' + day
secs = int(round(date[3] * 86400))
hr = secs // 3600
minute = (secs - hr * 3600) // 60
sec = secs - 3600 * hr - 60 * minute
hr = str(hr)
minute = str(minute)
sec = str(sec)
if len(sec) == 1:
sec = '0' + sec
if len(minute) == 1:
minute = '0' + minute
if len(hr) == 1:
hr = '0' + hr
fulldate = month + '/' + day + '/' + year
time = hr + ':' + minute + ':' + sec
return fulldate + ' ' + time
def from_excel(value, offset=CALENDAR_WINDOWS_1900):
parts = list(jd2gcal(MJD_0, value + offset - MJD_0))
fractions = value - int(value)
diff = datetime.timedelta(days=fractions)
if 1 > value > 0 or 0 > value > -1:
return days_to_time(diff)
return datetime.datetime(*parts[:3]) + diff
def jd_2_date(julian_day):
""" Compute the date from the Julian day.
INPUT
-----
julian_day: float
The date in Julian day.
RETURN
------
t: datetime
The date.
"""
date = jd2gcal(2400000.5, julian_day - 2400000.5)
sec_day = date[3] * 24 * 3600
year = date[0]
month = date[1]
day = date[2]
hour = int(divmod(sec_day, 3600)[0])
minu = int(divmod(sec_day - hour * 3600, 60)[0])
seco = int(divmod(sec_day - hour * 3600, 60)[1])
frac = int((divmod(sec_day - hour * 3600, 60)[1] - seco) * 1E6)
t = datetime(year, month, day, hour, minu, seco, frac)
return t
def readtime(filename):
metafile = open(filename + ".meta", "r")
lines = metafile.readlines()
try:
if lines[0][0] == 'N': # Using nominal date
time = float(lines[0][15:21])
interval = 'NaN'
else: # Using Central Julian date
jdate = float(lines[0][36:47])
# Get date
year, month, day, fracday = jdcal.jd2gcal(jdate, 0)
time = datelib.date_to_fracyear(year, month, day + fracday)
# Get time interval for velocity (time of second image - time of first image)
month1 = datelib.month(lines[1][32:35])
day1 = float(lines[1][36:38])
year1 = float(lines[1][39:43])
month2 = datelib.month(lines[2][33:36])
day2 = float(lines[2][37:39])
year2 = float(lines[2][40:44])
interval = datelib.date_to_fracyear(
year2, month2, day2) - datelib.date_to_fracyear(
year1, month1, day1)
except:
time = float('nan')
interval = float('nan')
return time, interval
def from_excel(value, offset=CALENDAR_WINDOWS_1900):
parts = list(jd2gcal(MJD_0, value + offset - MJD_0))
fractions = value - int(value)
diff = datetime.timedelta(days=fractions)
if 1 > value > 0 or 0 > value > -1:
return days_to_time(diff)
return datetime.datetime(*parts[:3]) + diff
def get_date_time(julian_day):
# take in floating Julian day and return a date and time as a single string
diff = julian_day - 240000.5
date = jdcal.jd2gcal(240000.5, diff)
year = str(date[0])
month = str(date[1])
day = str(date[2])
if len(month) == 1:
month = '0' + month
if len(day) == 1:
day = '0' + day
secs = int(round(date[3]*86400))
hr = secs//3600
minute = (secs - hr * 3600) // 60
sec = secs - 3600*hr - 60*minute
hr = str(hr)
minute = str(minute)
sec = str(sec)
if len(sec) == 1:
sec = '0' + sec
if len(minute) == 1:
minute = '0' + minute
if len(hr) == 1:
hr = '0' + hr
fulldate = month + '/' + day + '/' + year
time = hr + ':' + minute + ':' + sec
return fulldate + ' ' + time
def republican_to_gregorian(y, m, d):
"""
Take a year (y>=1), a month (1<=m<=13), and a day (1<=d<=30) that represent
a day from the French Republican calendar and return a (year, month, day)
tuple that represent the same date in the Gregorian calendar.
"""
y, m, d, _ = jdcal.jd2gcal(0, _republican_ymd_to_julian_day(y, m, d))
return (y, m, d)
def getDateFromJulian(jDay):
dt = jd2gcal(2400000.5, jDay)
dayDec = dt[3] - int(dt[3])
hr = int(dayDec * 24)
minDec = dayDec - hr / 24
minute = int(minDec * 60 * 24)
sec = int((dayDec * 24 - hr - minute / 60) * 3600)
return (dt[0], dt[1], dt[2], hr, minute, sec)
def from_excel(value, offset=CALENDAR_WINDOWS_1900):
if value is None:
return
parts = list(jd2gcal(MJD_0, value + offset - MJD_0))
_, fraction = divmod(value, 1)
diff = datetime.timedelta(days=fraction)
if 0 < abs(value) < 1:
return days_to_time(diff)
return datetime.datetime(*parts[:3]) + diff
def get_end_year(self, obj): # pylint: disable=R0201
"""
Retrieves year of last narration in set
"""
if obj.narration_set.last() is not None:
return jd2gcal(
obj.narration_set.order_by("map_datetime").last().map_datetime,
0)[0]
return None
def jul_greg(jd):
d = jdcal.jd2gcal(0, jd)
g = datetime.timedelta(days=d[3])
hrs = g.seconds / 3600
min = (g.seconds % 3600) / 60
sec = g.seconds % 60
decsec = 0 # uncomment if need greater precision: g.microseconds/1E6
date = str(d[0]).zfill(4) + str(d[1]).zfill(2) + str(d[2]).zfill(2) + str(hrs).zfill(2) + str(min).zfill(2) + str(sec + decsec)
return date
def jd_to_cald(julian_day):
"""
Converts julian day into calendar day in string format.
Args:
julian_day : Julian day value to be converted to calendar day
Returns:
cal_date : Calendar date corresponding to input julian day
"""
time_tuple = jd2gcal(epoch, julian_day - epoch)
cal_date = date(*time_tuple[0:3]).strftime("%Y-%m-%d")
return cal_date
def mjd_to_time(mjd):
year, month, day, time = jdcal.jd2gcal(2400000.5, mjd)
hour = int(math.floor(time * 24.))
x = time * 24 - hour
minute = int(math.floor(x * 60))
x = x * 60 - minute
second = x * 60
return year, month, day, hour, minute, second
def mjd2000_to_date(mjd):
"""
Convert a MJD2000 date to a datetime object
:param mjd float: the MJD2000 date to convert
:return: a datetime object
:rtype: datetime.datetime
"""
dat = jdcal.jd2gcal(jdcal.MJD_0 + jdcal.MJD_JD2000, mjd)
tm = __mjd2000_fraction_to_timedelta(dat[3])
return datetime.datetime(dat[0], dat[1], dat[2],
*__split_timedelta(tm))
def mjd_to_time(mjd):
year, month, day, time = jdcal.jd2gcal(2400000.5, mjd)
hour = int(math.floor(time * 24.))
x = time*24 - hour
minute = int(math.floor(x * 60))
x = x * 60 - minute
second = x * 60
return year, month, day, hour, minute, second
def dday2timestr(yr, dday):
'''
Convert dday to str of timestamp
yr data.yearbase
dday one or more items in a list from data.dday
'''
yr1day = jdcal.gcal2jd(yr, 1, 1) # get numbers for start of the year
gcal = [jdcal.jd2gcal(yr1day[0], yr1day[1] + x) for x in np.nditer(dday)]
td = [
datetime.datetime(year=xx[0], month=xx[1], day=xx[2]) +
datetime.timedelta(days=xx[-1]) for xx in gcal
]
return [x.strftime('%H:%M:%S') for x in td]
def getDate(jDay):
jd = (
2400000.5, jDay
) # Note: This is a tuple, not a list (i.e. ordered and unchangeable)
dt = jd2gcal(*jd)
yr = dt[0]
mo = dt[1]
day = int(dt[2])
dayFrac = dt[3]
hr = int(dayFrac * 24)
mins = int((dayFrac * 24 - hr) * 60)
sec = int((dayFrac * 24 - hr - mins / 60) * 3600)
return (yr, mo, day, hr, mins, sec)
def read_ncjuld(d):
"""Convert the netcdf Julian date into a proper format"""
t_ref = parser.parse(np.unique(d['JULD_REFERENCE'])[0])
t = jdcal.jd2gcal(sum(jdcal.gcal2jd(t_ref.year, t_ref.month, t_ref.day)),np.unique(d['JULD']))
return t
# def open_erddap(dsub, i_obs):
# # WMO of the platform:
# wmo = np.asmatrix(dsub['STATION_IDENTIFIER'].isel(N_OBS=i_obs).values)[0, 0].strip()
# # Datetime of the measurement:
# jd = np.asmatrix(dsub['JULD'].isel(N_OBS=i_obs).values)[0, 0]
# ts = pd.Timestamp('1950-01-01') + pd.Timedelta(days=jd)
# # ts.to_datetime().strftime("%Y%m%d%H%M%S")
# # http://www.ifremer.fr/erddap/tabledap/ArgoFloats.htmlTable?temp%2Cpres%2Cpsal%2Ctime&platform_number=%226901047%22&time=2014-06-07T05%3A53%3A50Z
def convert_mjd_to_greg(toas):
"""
Converts MJD array to year array
:param toas: Array of TOAs in days
:return: Array of TOAs in years
"""
dates = np.zeros(len(toas))
for ct, toa in enumerate(toas):
x = jdcal.jd2gcal(2400000.5, toa)
dates[ct] = x[0] + x[1] / 12 + x[2] / 365.25 + x[3] / 365.25
return dates
def convert_mjd_to_greg(toas):
"""
Converts MJD array to year array
:param toas: Array of TOAs in days
:return: Array of TOAs in years
"""
dates = np.zeros(len(toas))
for ct, toa in enumerate(toas):
x = jdcal.jd2gcal(2400000.5, toa)
dates[ct] = x[0] + x[1] / 12 + x[2] / 365.25 + x[3] / 365.25
return dates
def from_excel(value, offset=CALENDAR_WINDOWS_1900):
if value is None:
return
if 1 < value < 60 and offset == CALENDAR_WINDOWS_1900:
value += 1
parts = list(jd2gcal(MJD_0, value + offset - MJD_0))
_, fraction = divmod(value, 1)
jumped = (parts[-1] == 0 and fraction > 0)
diff = datetime.timedelta(days=fraction)
if 0 < abs(value) < 1:
return days_to_time(diff)
if not jumped:
return datetime.datetime(*parts[:3]) + diff
else:
return datetime.datetime(*parts[:3] + [0])
def format_date(date, year):
""""""
year_jd = int(sum(gcal2jd(year, 1, 1)))
# print "year 2000", year_2000
date = date - year_jd
d = jd2gcal(year_jd, date)
print "datedate", d
# test
for i in (1, 10, 100):
print "{num:02d}".format(num=i)
date_string = "{}_{a:02d}_{b:02d}".format(d[0], a=d[1], b=d[2])
return date_string
def format_date(date, year):
""""""
year_jd = int(sum(gcal2jd(year, 1, 1)))
# print "year 2000", year_2000
date = date - year_jd
d = jd2gcal(year_jd, date)
print("datedate", d)
# test
for i in (1, 10, 100):
print("{num:02d}".format(num=i))
date_string = "{}_{a:02d}_{b:02d}".format(d[0], a=d[1], b=d[2])
return date_string
def _normalize_jd2datetime(ds: xr.Dataset) -> xr.Dataset:
"""
Convert the time dimension of the given dataset from Julian date to
datetime.
:param ds: Dataset on which to run conversion
"""
ds = ds.copy()
# Decode JD time
tuples = [jd2gcal(x, 0) for x in ds.time.values]
# Replace JD time with datetime
ds.time.values = [datetime(x[0], x[1], x[2]) for x in tuples]
# Adjust attributes
ds.time.attrs['long_name'] = 'time'
ds.time.attrs['calendar'] = 'standard'
return ds
def _normalize_jd2datetime(ds: xr.Dataset) -> xr.Dataset:
"""
Convert the time dimension of the given dataset from Julian date to
datetime.
:param ds: Dataset on which to run conversion
"""
try:
time = ds.time
except AttributeError:
return ds
try:
units = time.units
except AttributeError:
units = None
try:
long_name = time.long_name
except AttributeError:
long_name = None
if units:
units = units.lower().strip()
if long_name:
units = long_name.lower().strip()
units = units or long_name
if not units or units != 'time in julian days':
return ds
ds = ds.copy()
# Decode JD time
# noinspection PyTypeChecker
tuples = [jd2gcal(x, 0) for x in ds.time.values]
# Replace JD time with datetime
ds.time.values = [datetime(x[0], x[1], x[2]) for x in tuples]
# Adjust attributes
ds.time.attrs['long_name'] = 'time'
ds.time.attrs['calendar'] = 'standard'
return ds
def _normalize_jd2datetime(ds: xr.Dataset) -> xr.Dataset:
"""
Convert the time dimension of the given dataset from Julian date to
datetime.
:param ds: Dataset on which to run conversion
"""
try:
time = ds.time
except AttributeError:
return ds
try:
units = time.units
except AttributeError:
units = None
try:
long_name = time.long_name
except AttributeError:
long_name = None
if units:
units = units.lower().strip()
if long_name:
units = long_name.lower().strip()
units = units or long_name
if not units or units != 'time in julian days':
return ds
ds = ds.copy()
# Decode JD time
# noinspection PyTypeChecker
tuples = [jd2gcal(x, 0) for x in ds.time.values]
# Replace JD time with datetime
ds.time.values = [datetime(x[0], x[1], x[2]) for x in tuples]
# Adjust attributes
ds.time.attrs['long_name'] = 'time'
ds.time.attrs['calendar'] = 'standard'
return ds
def mjd2gcal(mjds):
"""
Calculate the Gregorian dates from a numpy-array of MJDs
@param mjds: Numpy array of MJDs
"""
nmjds = len(mjds)
gyear = np.zeros(nmjds)
gmonth = np.zeros(nmjds)
gday = np.zeros(nmjds)
gfd = np.zeros(nmjds)
# TODO: get rid of ugly for loop. Use some zip or whatever
for ii in range(nmjds):
gyear[ii], gmonth[ii], gday[ii], gfd[ii] = \
jdcal.jd2gcal(jdcal.MJD_0, mjds[ii])
return gyear, gmonth, gday, gfd
def mjd2gcal(mjds):
"""
Calculate the Gregorian dates from a numpy-array of MJDs
@param mjds: Numpy array of MJDs
"""
nmjds = len(mjds)
gyear = np.zeros(nmjds)
gmonth = np.zeros(nmjds)
gday = np.zeros(nmjds)
gfd = np.zeros(nmjds)
# TODO: get rid of ugly for loop. Use some zip or whatever
for ii in range(nmjds):
gyear[ii], gmonth[ii], gday[ii], gfd[ii] = \
jdcal.jd2gcal(jdcal.MJD_0, mjds[ii])
return gyear, gmonth, gday, gfd
def mjd2datetime(mjd):
''' convert modified Julian date to Python daytime
Uses jdcal package for dealing with modified julian dates
See https://oneau.wordpress.com/2011/08/30/jdcal/
jdcal.jd2gcal(jdcal.MJD_0,57827.5774306)
(have to pass both base date of MJD and the MJD to this function)
:param mjd: time as modified julian date
:return: equivalent datetime object
'''
jdcal_time = jdcal.jd2gcal(jdcal.MJD_0, mjd)
jdcal_time_hours = math.floor(jdcal_time[3] * 24)
jdcal_time_minutes = math.floor((jdcal_time[3] * 24 - jdcal_time_hours) * 60)
jdcal_time_seconds = math.floor(((jdcal_time[3] * 24 - jdcal_time_hours) * 60 - jdcal_time_minutes) * 60)
datetime_time = datetime(jdcal_time[0], jdcal_time[1], jdcal_time[2], int(jdcal_time_hours),
int(jdcal_time_minutes), int(jdcal_time_seconds))
return datetime_time
def nc_time_slice(width, height, timeindex, t, base_jd, output_directory,
input_filename, input_file, input_variable):
date_georg = jdcal.jd2gcal(2400000.5, t + base_jd)
year = int(date_georg[0])
month = int(date_georg[1])
day = int(date_georg[2])
date = datetime(year, month, day)
str_date = date.strftime('%Y-%m-%d')
output_file = path.join(
output_directory,
path.splitext(input_filename)[0] + '_' + str_date + '.nc')
dataset, lon_variable, lat_variable, time_variable, depth_variable = \
create_netcdf_dataset_dimensions(width, height, output_file, add_depth=True)
# input_variables = ['CHL_mean']
# output_variables = ['CHL']
# output_variables_units = ['mg/m^3']
# output_variables_long_name = ['Chlorophyll a concentration']
# output_variables_standard_name = ['CHL']
input_variables = ['chl']
output_variables = ['chl']
output_variables_units = ['mg/m^3']
output_variables_long_name = ['Chlorophyll a concentration']
output_variables_standard_name = ['chl']
create_nc_vars(dataset, input_variables, output_variables,
output_variables_units, output_variables_long_name,
output_variables_standard_name)
time_variable[0] = t
lon_variable[:] = input_file.variables['longitude'][:]
lat_variable[:] = input_file.variables['latitude'][:]
depth_variable[0] = 0.0
target_chl_variable = dataset.variables[output_variables[0]]
input_data = input_variable[timeindex:timeindex + 1, :, :]
data = input_data.reshape((1, 1, height, width))
target_chl_variable[:, :, :, :] = data
dataset.close()
def getCalDay(JD):
year, month, day, hour = jdcal.jd2gcal(JD, 0.0)
hour = hour * 24
minutes = modf(hour)[0] * 60.0
seconds = modf(minutes)[0] * 60.0
hh = int(modf(hour)[1])
mm = int(modf(minutes)[1])
ss = seconds
if (hh < 10):
hh = '0' + str(hh)
else:
hh = str(hh)
if (mm < 10):
mm = '0' + str(mm)
else:
mm = str(mm)
if (ss < 10):
ss = '0' + str(np.round(ss, 1))
else:
ss = str(np.round(ss, 1))
return year, month, day, hh, mm, ss
def gps2utc(timeOfWeek, week, cycle=0):
"""Convert GPS time to UTC, taking into account leap seconds"""
week += cycle * GPS_CYCLE_WEEKS
jd = gps2julian(timeOfWeek, week)
leap_seconds_since_gps_epoch = get_gps_utc_offset(jd)
offset = -1. * leap_seconds_since_gps_epoch / DAY_S
year, month, day, daytime = jd2gcal(jd + offset, 0)
day_seconds = daytime * DAY_S
hours = int(day_seconds // 3600)
minutes = int((day_seconds % 3600) // 60)
frac_seconds = day_seconds % 60
seconds = int(floor(frac_seconds))
microseconds = int(floor(frac_seconds % 1 * 1000000))
dt = datetime(year, month, day, hours, minutes, seconds, microseconds, pytz.utc)
return dt
def getCalDay(JD):
year, month, day, hour= jdcal.jd2gcal(JD,0.0)
hour = hour*24
minutes = modf(hour)[0]*60.0
seconds = modf(minutes)[0]*60.0
hh = int(modf(hour)[1])
mm = int(modf(minutes)[1])
ss = seconds
if(hh<10):
hh = '0'+str(hh)
else:
hh = str(hh)
if(mm<10):
mm = '0'+str(mm)
else:
mm = str(mm)
if(ss<10):
ss = '0'+str(np.round(ss,1))
else:
ss = str(np.round(ss,1))
return year,month,day,hh,mm,ss
def parseImageObservationTimeHeader(self, printInfo=False):
"""
Parses HRIT Image Observation Time header (type 131)
:param printInfo: Print info after parsing.
"""
if self.readbytes(0) == b'\x83':
self.imageObservationTimeHeader['valid'] = True
self.imageObservationTimeHeader['header_type'] = 131
self.imageObservationTimeHeader['header_len'] = int.from_bytes(
self.readbytes(1, 2), byteorder='big')
self.imageObservationTimeHeader['header_offset'] = self.byteOffset
self.imageObservationTimeHeader['mjd'] = self.readbytes(
3, self.imageObservationTimeHeader['header_len'] - 3).decode()
self.imageObservationTimeHeader['date'] = jd2gcal(
2400000.5, float(self.imageObservationTimeHeader['mjd']))
self.byteOffset += self.imageObservationTimeHeader['header_len']
if printInfo:
self.printImageObservationTimeHeader()
else:
self.imageObservationTimeHeader['valid'] = False
def parse_file(input_filepath):
output = []
with open(input_filepath) as ifile:
buf = []
d = {}
state = None
for line in [ln.strip() for ln in ifile.readlines()]:
if line.startswith('STARTMETADATA'):
state = 'METADATA'
continue
elif line.startswith('ENDMETADATA'):
state = 'DATA'
continue
elif line.startswith('ENDDATA'):
state = None
d['data'] = buf
output.append(d)
d = {}
buf = []
continue
if state == 'METADATA':
key, val = line.split('=', 1)
d[key] = val
elif state == 'DATA':
julian_date, magnitude, error_margin, airmass = line.split('=')[1].split('|')
jyear = int(julian_date[:2])*10e4
jday = float(julian_date[2:])
year, month, day, secfrac = jdcal.jd2gcal(jyear, jday)
date = datetime.datetime(year, month, day) + datetime.timedelta(0, secfrac*86400)
buf.append([str(date), float(magnitude),
str_to_float_or_None(error_margin),
str_to_float_or_None(airmass),
])
else:
raise Exception('unknown state %s! typo?' % (state))
return output
#Le format est
#Time Tau Delta_Tau
#avec Time from 31/12/1991 at 0 hs
#Ils m’ont aussi donné une valeur pour la conversion : PWV = 14.425 * Tau
#mais apparemment c’est fait avec un modèle d’atmosphère pas très sur…
import numpy as np
data = np.loadtxt('chorrillo_2009.dat')
tau = data[:,1]
dtau = data[:,2]
import jdcal as jdcal
init=np.sum(jdcal.gcal2jd(1991,12,31))
jd = init+data[:,0]
jdcal.jd2gcal(0,jd[0])
jdstart = np.sum(jdcal.gcal2jd(2009,1,1))
datestart = jdcal.jd2gcal(0,jdstart)
day = jd - jdstart
clf()
plot(day/365*12,tau)
xlim(0,12)
pwv = 14.425 * tau
clf()
plot(day/365*12,pwv)
xlim(0,12)
def func_night_time_calculator(current_date_str):
# set observation day ------------------------------------------------
# current_utc_datetime = time.gmtime()
# Op_time = current_utc_datetime.strftime( '%Y-%m-%d %H:%M:%S' )
# current_utc_datetime = "2017-05-23 21:29:38"
Op_time = time.strptime(current_date_str, "%Y-%m-%d")
gcal_y = Op_time.tm_year
gcal_m = Op_time.tm_mon
gcal_d = Op_time.tm_mday
gcal_h = Op_time.tm_hour
gcal_min = Op_time.tm_min
gcal_sec = Op_time.tm_sec
MJD_newyear = gcal2jd(gcal_y,gcal_m,gcal_d)[1]
MJD_current = MJD_newyear
print(MJD_current)
# start calculate observation sequence
time_interval = 5.0 # 2 munitues
night_number = 288 # every 2 munitues, 720 in total.
mjd = []
ut_time = []
local_time = []
solar_alt = []
for n in range(night_number):
# set mjd time ----------------------------------------
MJD_time = MJD_current + (n*time_interval/60.0/24.0)
nighttime_current = jd2gcal(2400000.5, MJD_time)
# print('night time', nighttime_current)
hh = int(nighttime_current[3] * 24.0 )
mm = int((nighttime_current[3] * 24.0 - hh)*60.0)
ss = (((nighttime_current[3] * 24.0 - hh)*60.0) - mm)*60.0
hms = "%02d:%02d:%02d" % (hh,mm,ss)
nighttime_current_cal = ('%s/%s/%s %s' % (nighttime_current[0],nighttime_current[1],nighttime_current[2],hms))
nighttime_current_str = ('%s/%02d/%02dT%s' % (nighttime_current[0],nighttime_current[1],nighttime_current[2],hms))
nighttime_current_cal_datetime = time.strptime(nighttime_current_cal, '%Y/%m/%d %H:%M:%S')
astro_parameter_night = astro_parameter_calculate(nighttime_current_cal_datetime)
local_time_str = astro_parameter_night[1]
solar_alt_dd = astro_parameter_night[3]
zenith_sun_min = astro_parameter_night[9]
if ( solar_alt_dd > zenith_sun_min ):
mjd.append(MJD_time)
local_time.append(local_time_str)
solar_alt.append(solar_alt_dd)
if (len(mjd) > 0 ):
obs_mjd_begin_index = 0
for mmm in range(len(mjd)-1):
m_gap = mjd[mmm+1] - mjd[mmm]
m_int = (2.0/24.0)
if m_gap > m_int:
obs_mjd_begin_index = mjd.index(mjd[mmm+1])
if obs_mjd_begin_index == 0:
obs_mjd_begin_index = mjd.index(min(mjd))
obs_mjd_end_index = mjd.index(max(mjd))
mjd_begin = mjd[obs_mjd_begin_index]
mjd_end = mjd[obs_mjd_end_index]
local_time_begin = local_time[obs_mjd_begin_index]
local_time_end = local_time[obs_mjd_end_index]
solar_alt_begin = solar_alt[obs_mjd_begin_index]
solar_alt_end = solar_alt[obs_mjd_end_index]
return [str(local_time_begin),str(local_time_end),\
str(solar_alt_begin),str(solar_alt_end)]
def convert_ansi_date(date, offset=0.5):
logging.info('function `convert_ansi_date` complete')
return jdcal.jd2gcal(2305812.5, date + offset) # 0.5 offset is to adjust from night to noon
def main():
""" main method """
usage = "Example: python grid_obs_calculate.py -g G0008 "
parser = OptionParser(usage, version=__version__) #"test")# __version__ )
parser.add_option( "-g", "--gridid", dest = "gridid" , type = "string", \
help = "Grid ID, default=G0001",default="G0001")
opts, args = parser.parse_args()
if len(sys.argv) == 1:
print "please use -h to see help"
print usage
sys.exit()
GridID = opts.gridid
homedir = os.getcwd()
configuration_file = './configuration.dat'
configuration_file_dev = open(configuration_file, 'rU')
lines1 = configuration_file_dev.read().splitlines()
configuration_file_dev.close()
for line1 in lines1:
word = line1.split()
if word[0] == 'griduser':
griduser = word[2]
elif word[0] == 'gridip':
gridip = word[2]
elif word[0] == 'gridmypassword':
gridmypassword = word[2]
elif word[0] == 'gridmydb':
gridmydb = word[2]
conf_obs_parameters_sys = './conf_obs_parameters_sys.dat'
conf_obs_parameters_sys_dev = open(conf_obs_parameters_sys, 'rU')
lines2 = conf_obs_parameters_sys_dev.read().splitlines()
conf_obs_parameters_sys_dev.close()
for line2 in lines2:
word = line2.split()
if word[0] == 'observatory_lat':
observatory_lat = word[2]
elif word[0] == 'observatory_lon':
observatory_lon = word[2]
elif word[0] == 'observatory_elevation':
observatory_elevation = float(word[2])
elif word[0] == 'zenith_sun_min':
zenith_sun_min = float(word[2])
elif word[0] == 'zenith_min':
zenith_min = float(word[2])
elif word[0] == 'gal_min':
gal_min = float(word[2])
elif word[0] == 'moon_dis_min_para':
moon_dis_min_str = word[2]
moon_dis_para_str = moon_dis_min_str.split('|')
moon_dis_phase_data = [[]]
for moon_dis_para in moon_dis_para_str:
moon_dis_para_phase_min = float(
moon_dis_para.split(':')[0].split('-')[0])
moon_dis_para_phase_max = float(
moon_dis_para.split(':')[0].split('-')[1])
moon_dis_para_dis = float(moon_dis_para.split(':')[1])
moon_dis_phase_data.append([
moon_dis_para_phase_min, moon_dis_para_phase_max,
moon_dis_para_dis
])
moon_dis_phase_data = filter(None, moon_dis_phase_data)
conn_gwacoc_grid = MySQLdb.connect(host=gridip,
user=griduser,
passwd=gridmypassword,
db=gridmydb)
cursor_gwacoc_grid = conn_gwacoc_grid.cursor()
grid_cmd = "select * from Grid_table where GridID = '" + GridID + "'"
#print grid_cmd
cursor_gwacoc_grid.execute(grid_cmd)
extract_grid_result = cursor_gwacoc_grid.fetchall()
print extract_grid_result
cursor_gwacoc_grid.close()
# define grid date frame ----------------------------------------
gridframe = pd.DataFrame()
if len(extract_grid_result) > 0:
gridframe['obs_date'] = 0
gridframe['Grid_ID'] = zip(*extract_grid_result)[1]
gridframe['field_ID'] = zip(*extract_grid_result)[2]
gridframe['ra_center'] = zip(*extract_grid_result)[3]
gridframe['dec_center'] = zip(*extract_grid_result)[4]
gridframe['radeg_h1'] = zip(*extract_grid_result)[5]
gridframe['decdeg_h1'] = zip(*extract_grid_result)[6]
gridframe['radeg_h2'] = zip(*extract_grid_result)[7]
gridframe['decdeg_h2'] = zip(*extract_grid_result)[8]
gridframe['radeg_l1'] = zip(*extract_grid_result)[9]
gridframe['decdeg_l1'] = zip(*extract_grid_result)[10]
gridframe['radeg_l2'] = zip(*extract_grid_result)[11]
gridframe['decdeg_l2'] = zip(*extract_grid_result)[12]
gridframe['mjd_begin'] = 0
gridframe['mjd_end'] = 0
gridframe['local_time_begin'] = 0
gridframe['local_time_end'] = 0
gridframe['lst_begin'] = 0
gridframe['lst_end'] = 0
gridframe['solar_alt_begin'] = 0
gridframe['solar_alt_end'] = 0
gridframe['lunar_ra_begin'] = 0
gridframe['lunar_dec_begin'] = 0
gridframe['lunar_phase_begin'] = 0
gridframe['lunar_ra_end'] = 0
gridframe['lunar_dec_end'] = 0
gridframe['lunar_phase_end'] = 0
#path = '/Users/han/tmp_pool/gwac_dispatch/obs_skymap/'
# set observation day ------------------------------------------------
current_utc_datetime = datetime.datetime.utcnow()
Op_time = current_utc_datetime.strftime('%Y-%m-%d')
Op_time = time.strptime(Op_time, "%Y-%m-%d")
gcal_y = Op_time.tm_year
gcal_m = Op_time.tm_mon
gcal_d = Op_time.tm_mday
MJD_newyear = gcal2jd(gcal_y, gcal_m, gcal_d)[1]
MJD_current = MJD_newyear
date_current = jd2gcal(2400000.5, MJD_current)
calendar_d_lable = "%d_%d_%d" % (date_current[0], date_current[1],
date_current[2])
calendar_d = "%d-%d-%d" % (date_current[0], date_current[1],
date_current[2])
# start calculate observation sequence
# time_interval = 40.0 # 2 munitues
# night_number = 36 # every 2 munitues, 720 in total.
time_interval = 5.0 # 2 munitues
night_number = 288 # every 2 munitues, 720 in total.
# set observatory parameters ----------------------------------------
observatory = ephem.Observer()
observatory.lat = observatory_lat
observatory.lon = observatory_lon
observatory.elevation = observatory_elevation
lat_dd = float(str(observatory.lat).split(":")[0])+\
float(str(observatory.lat).split(":")[1])/60.0+\
float(str(observatory.lat).split(":")[2])/3600.0
# define obs date frame ----------------------------------------
obsframe = pd.DataFrame()
for k in range(len(gridframe['Grid_ID'])):
#print 'field coor: ',gridframe['ra_center'][k],gridframe['dec_center'][k]
mjd = []
local_time = []
lst = []
solar_alt = []
lunar_ra = []
lunar_dec = []
lunar_phase = []
gridframe.loc[k, 'obs_date'] = calendar_d
# calculate galactic coordinate of field center and all vertexes
coor_equ_cen = ephem.Equatorial(gridframe['ra_center'][k],
gridframe['dec_center'][k],
epoch='2000')
g_cen = ephem.Galactic(coor_equ_cen)
g_cen_lat_dd = float(str(g_cen.lat).split(":")[0])+\
float(str(g_cen.lat).split(":")[1])/60.0+\
float(str(g_cen.lat).split(":")[2])/3600.0
coor_equ_h1 = ephem.Equatorial(gridframe['radeg_h1'][k],
gridframe['decdeg_h1'][k],
epoch='2000')
g_h1 = ephem.Galactic(coor_equ_h1)
g_h1_lat_dd = float(str(g_h1.lat).split(":")[0])+\
float(str(g_h1.lat).split(":")[1])/60.0+\
float(str(g_h1.lat).split(":")[2])/3600.0
coor_equ_h2 = ephem.Equatorial(gridframe['radeg_h2'][k],
gridframe['decdeg_h2'][k],
epoch='2000')
g_h2 = ephem.Galactic(coor_equ_h2)
g_h2_lat_dd = float(str(g_h2.lat).split(":")[0])+\
float(str(g_h2.lat).split(":")[1])/60.0+\
float(str(g_h2.lat).split(":")[2])/3600.0
coor_equ_l1 = ephem.Equatorial(gridframe['radeg_l1'][k],
gridframe['decdeg_l1'][k],
epoch='2000')
g_l1 = ephem.Galactic(coor_equ_l1)
g_l1_lat_dd = float(str(g_l1.lat).split(":")[0])+\
float(str(g_l1.lat).split(":")[1])/60.0+\
float(str(g_l1.lat).split(":")[2])/3600.0
coor_equ_l2 = ephem.Equatorial(gridframe['radeg_l2'][k],
gridframe['decdeg_l2'][k],
epoch='2000')
g_l2 = ephem.Galactic(coor_equ_l2)
g_l2_lat_dd = float(str(g_l2.lat).split(":")[0])+\
float(str(g_l2.lat).split(":")[1])/60.0+\
float(str(g_l2.lat).split(":")[2])/3600.0
galactic_lat_min = min([
abs(g_cen_lat_dd),
abs(g_h1_lat_dd),
abs(g_h2_lat_dd),
abs(g_l1_lat_dd),
abs(g_l2_lat_dd)
])
for n in range(night_number):
# set mjd time ----------------------------------------
MJD_time = MJD_current + (n * time_interval / 60.0 / 24.0)
nighttime_current = jd2gcal(2400000.5, MJD_time)
hh = int(nighttime_current[3] * 24.0)
mm = int((nighttime_current[3] * 24.0 - hh) * 60.0)
ss = (((nighttime_current[3] * 24.0 - hh) * 60.0) - mm) * 60.0
hms = "%02d:%02d:%02d" % (hh, mm, ss)
nighttime_current_cal = (
'%s/%s/%s %s' % (nighttime_current[0], nighttime_current[1],
nighttime_current[2], hms))
nighttime_current_str = (
'%s/%s/%sT%s' % (nighttime_current[0], nighttime_current[1],
nighttime_current[2], hms))
observatory.date = nighttime_current_cal
# set local time ----------------------------------------
local_nighttime_current = ephem.localtime(observatory.date)
local_nighttime_current_str = str(local_nighttime_current).replace(
' ', 'T')[0:22]
# calculate local sidereal time ----------------------------------------
lst_dd = float(str(observatory.sidereal_time()).split(":")[0])* 15.0+\
float(str(observatory.sidereal_time()).split(":")[1])/60.0* 15.0+\
float(str(observatory.sidereal_time()).split(":")[2])/3600.0* 15.0
# calculate altitude angle or zenith angular distance of the sun ---------------------------------
solar = ephem.Sun(observatory)
solar_alt_dd = 90 - float(str(solar.alt).split(":")[0]) + float(
str(solar.alt).split(":")[1]) / 60.0 + float(
str(solar.alt).split(":")[2]) / 3600.0
#print('solar %s' % (solar_alt_dd))
lunar = ephem.Moon(observatory)
lunar_ra_dd = float(str(lunar.ra).split(":")[0]) * 15.0 + float(
str(lunar.ra).split(":")[1]) / 60.0 * 15.0 + float(
str(lunar.ra).split(":")[2]) / 3600.0 * 15.0
lunar_dec_dd = float(str(lunar.dec).split(":")[0]) + float(
str(lunar.dec).split(":")[1]) / 60.0 + float(
str(lunar.dec).split(":")[2]) / 3600.0
#print('lunar %s %s %s' % (lunar_ra_dd, lunar_dec_dd, lunar.moon_phase))
# calculate zenith angular distance of field center and all vertexes
zenith_ang_dis_cen_dd = angular_distance(
gridframe['ra_center'][k], gridframe['dec_center'][k], lst_dd,
lat_dd)
# calculate angular distance between field center and all vertexes and moon
moon_ang_dis_cen_dd = angular_distance(gridframe['ra_center'][k],
gridframe['dec_center'][k],
lunar_ra_dd, lunar_dec_dd)
moon_ang_dis_h1_dd = angular_distance(gridframe['radeg_h1'][k],
gridframe['decdeg_h1'][k],
lunar_ra_dd, lunar_dec_dd)
moon_ang_dis_h2_dd = angular_distance(gridframe['radeg_h2'][k],
gridframe['decdeg_h2'][k],
lunar_ra_dd, lunar_dec_dd)
moon_ang_dis_l1_dd = angular_distance(gridframe['radeg_l1'][k],
gridframe['decdeg_l1'][k],
lunar_ra_dd, lunar_dec_dd)
moon_ang_dis_l2_dd = angular_distance(gridframe['radeg_l2'][k],
gridframe['decdeg_l2'][k],
lunar_ra_dd, lunar_dec_dd)
moon_ang_dis_min = min([
moon_ang_dis_cen_dd, moon_ang_dis_h1_dd, moon_ang_dis_h2_dd,
moon_ang_dis_l1_dd, moon_ang_dis_l2_dd
])
# set mini distance from the moon
for mm in range(len(moon_dis_phase_data)):
if (lunar.moon_phase >= moon_dis_phase_data[mm][0]
and lunar.moon_phase < moon_dis_phase_data[mm][1]):
moon_dis_min = moon_dis_phase_data[mm][2]
break
#print lunar.moon_phase,moon_dis_min
#print k,gridframe.loc[k,'field_ID'],zenith_ang_dis_cen_dd , zenith_min , galactic_lat_min , gal_min , moon_ang_dis_min , moon_dis_min
if (solar_alt_dd > zenith_sun_min) and (
zenith_ang_dis_cen_dd < zenith_min
): # and galactic_lat_min > gal_min and moon_ang_dis_min > moon_dis_min ):
# print 'mjd: ',MJD_current,MJD_time,nighttime_current
# print 'zenith: ',gridframe['ra_center'][k], gridframe['dec_center'][k],lst_dd,lat_dd,solar_alt_dd,zenith_ang_dis_cen_dd,zenith_min
mjd.append(MJD_time)
local_time.append(local_nighttime_current_str)
lst.append(lst_dd)
solar_alt.append(solar_alt_dd)
lunar_ra.append(lunar_ra_dd)
lunar_dec.append(lunar_dec_dd)
lunar_phase.append(lunar.moon_phase)
#print gridframe['field_ID'],MJD_time
# del mjd[0]
# del local_time[0]
# del lst[0]
# del solar_alt[0]
# del lunar_ra[0]
# del lunar_dec[0]
# del lunar_phase[0]
# mjd = filter(None,mjd)
# local_time = filter(None,local_time)
# lst = filter(None,lst)
# solar_alt = filter(None,solar_alt)
# lunar_ra = filter(None,lunar_ra)
# lunar_dec = filter(None,lunar_dec)
# lunar_phase = filter(None,lunar_phase)
if (len(mjd) > 0):
obs_mjd_begin_index = 0
for mmm in range(len(mjd) - 1):
m_gap = mjd[mmm + 1] - mjd[mmm]
m_int = (2.0 / 24.0)
if m_gap > m_int:
obs_mjd_begin_index = mjd.index(mjd[mmm + 1])
if obs_mjd_begin_index == 0:
obs_mjd_begin_index = mjd.index(min(mjd))
obs_mjd_end_index = mjd.index(max(mjd))
gridframe.loc[k, 'mjd_begin'] = mjd[obs_mjd_begin_index]
gridframe.loc[k, 'mjd_end'] = mjd[obs_mjd_end_index]
gridframe.loc[k,
'local_time_begin'] = local_time[obs_mjd_begin_index]
gridframe.loc[k, 'local_time_end'] = local_time[obs_mjd_end_index]
gridframe.loc[k, 'lst_begin'] = lst[obs_mjd_begin_index]
gridframe.loc[k, 'lst_end'] = lst[obs_mjd_end_index]
gridframe.loc[k,
'solar_alt_begin'] = solar_alt[obs_mjd_begin_index]
gridframe.loc[k, 'solar_alt_end'] = solar_alt[obs_mjd_end_index]
gridframe.loc[k, 'lunar_ra_begin'] = lunar_ra[obs_mjd_begin_index]
gridframe.loc[k, 'lunar_dec_begin'] = lunar_dec[obs_mjd_end_index]
gridframe.loc[
k, 'lunar_phase_begin'] = lunar_phase[obs_mjd_begin_index]
gridframe.loc[k, 'lunar_ra_end'] = lunar_ra[obs_mjd_end_index]
gridframe.loc[k, 'lunar_dec_end'] = lunar_dec[obs_mjd_begin_index]
gridframe.loc[k,
'lunar_phase_end'] = lunar_phase[obs_mjd_end_index]
for k in range(len(gridframe['obs_date'])):
CurrentTable = "grid_observable_timetable"
if gridframe.loc[k, 'mjd_begin'] > 0:
insert_cmd = "insert into " + CurrentTable + " values ( DEFAULT , " + \
"'" + gridframe.loc[k,'obs_date'] + "' , " + \
"'" + gridframe.loc[k,'Grid_ID'] + "' , " + \
"'" + gridframe.loc[k,'field_ID'] + "' , " + \
" " + str(gridframe.loc[k,'ra_center']) + " , " + \
" " + str(gridframe.loc[k,'dec_center']) + " , " + \
" " + str(gridframe.loc[k,'radeg_h1']) + " , " + \
" " + str(gridframe.loc[k,'decdeg_h1']) + " , " + \
" " + str(gridframe.loc[k,'radeg_h2']) + " , " + \
" " + str(gridframe.loc[k,'decdeg_h2']) + " , " + \
" " + str(gridframe.loc[k,'radeg_l1']) + " , " + \
" " + str(gridframe.loc[k,'decdeg_l1']) + " , " + \
" " + str(gridframe.loc[k,'radeg_l2']) + " , " + \
" " + str(gridframe.loc[k,'decdeg_l2']) + " , " + \
" " + str(gridframe.loc[k,'mjd_begin']) + " , " + \
" " + str(gridframe.loc[k,'mjd_end']) + " , " + \
"'" + str(gridframe.loc[k,'local_time_begin']) + "' , " + \
"'" + str(gridframe.loc[k,'local_time_end']) + "' , " + \
" " + str(gridframe.loc[k,'lst_begin']) + " , " + \
" " + str(gridframe.loc[k,'lst_end']) + " , " + \
" " + str(gridframe.loc[k,'solar_alt_begin']) + " , " + \
" " + str(gridframe.loc[k,'solar_alt_end']) + " , " + \
" " + str(gridframe.loc[k,'lunar_ra_begin']) + " , " + \
" " + str(gridframe.loc[k,'lunar_dec_begin']) + " , " + \
" " + str(gridframe.loc[k,'lunar_phase_begin']) + " , " + \
" " + str(gridframe.loc[k,'lunar_ra_end']) + " , " + \
" " + str(gridframe.loc[k,'lunar_dec_end']) + " , " + \
" " + str(gridframe.loc[k,'lunar_phase_end']) + " " + \
" " + ")"
print insert_cmd
cursor = conn_gwacoc_grid.cursor()
cursor.execute(insert_cmd)
conn_gwacoc_grid.commit()
cursor.close()
conn_gwacoc_grid.close()
import jdcal assert jdcal.gcal2jd(2000,1, 1) == (2400000.5, 51544.0) assert jdcal.gcal2jd(2001,2,30) == (2400000.5, 51970.0) assert jdcal.jd2gcal(2400000.5, 51544.75) == (2000, 1, 1, 0.75) assert jdcal.__version__ == '1.3'
def get_ymd_g(self):
"""return the year, month, and day of the instance, according to the
Gregorian calendar"""
return jdcal.jd2gcal(jdcal.MJD_0, self.date)[:3]
vals = []
for perc in percentiles:
vals.append(sd[perc*len(sd)])
truc = truc + '{0:.1f} ({1:.0f}%) - '.format(sd[perc*len(sd)], perc*100)
return truc[0:-3], vals
### Wind data
dir = '/Users/hamilton/Qubic/Sites/FromMarcelo/data_h/'
ts0, rec0, WS_ms_Avg, WS_ms_Std, WS_ms_Max, WS_ms_S_WVT, WindDir_D1_WVT, WindDir_SD1_WVT = np.loadtxt(dir+'chorrillo-t1m_cal.csv', usecols = [2,3,4,5,6,7,8,9]).T
import jdcal as jdcal
init = np.sum(jdcal.gcal2jd(1970,1,1))
jd0 = ts0/3600/24
jdcal.jd2gcal(init, jd0[0])
jdcal.jd2gcal(init, jd0[-1])
jdstartyear = np.sum(jdcal.gcal2jd(2011,1,1))
jdsince0 = init + ts0/3600/24 - jdstartyear
clf()
plot(jdsince0, WS_ms_Max, 'r,')
plot(jdsince0, WS_ms_Avg)
plot(jdsince0, WS_ms_Std)
xlabel('JD since 2011')
ylabel('Wind Speed $[m/s]$')
#### comparer avec https://science.nrao.edu/facilities/alma/aboutALMA/Technology/ALMA_Memo_Series/alma497/memo497.pdf
#### Figure 3.1
bla=hist(WS_ms_Avg, range=[0,30], bins=300, cumulative=True,normed=1, alpha=0.1)
def main(argv):
if len(argv) < 4:
print "Error: not enough arguments"
print
display_usage(argv[0])
return 1
from_date = datetime.strptime(argv[1], u"%Y-%m-%d")
to_date = datetime.strptime(argv[2], u"%Y-%m-%d")
site_abbr = argv[3]
cmd = 'wget -nv'
if len(argv) >= 5:
cmd = ' '.join(argv[4:])
#print "# Command = <%s>" % (cmd, )
list_only = None
if cmd != '-':
list_only = False
cmd = cmd + ' '
else:
list_only = True
cmd = ''
# if-else
# Convert to Julian Day numbers
from_mjday = date2mjday(from_date)
to_mjday = date2mjday(to_date)
# Compute the GPS zero day
gps_zeroday = date2mjday(datetime(1980, 1, 6))
if list_only == False:
print "#!/bin/bash"
print
print "# Automatically generated script for downloading "\
"RINEX NAV files."
print "# From date: %s" % (from_date.strftime("%Y-%m-%d"), )
print "# To date: %s (excluded)" % (to_date.strftime("%Y-%m-%d"), )
print "# Span: %d days" % (to_mjday - from_mjday, )
print
# if: not list_only
# Loop from the first day until the last day (exclusive)
for mjday in range(from_mjday, to_mjday):
gpsday = mjday - gps_zeroday
gdate = datetime(*jdcal.jd2gcal(jdcal.MJD_0, mjday)[:3])
year = gdate.year
# Compute the mjd for the first day of the year
yday_zero = date2mjday(datetime(year, 1, 1))
yday = mjday - yday_zero + 1
# Get the GPS week number
gpscycle = int(gpsday / (1024*7))
gpsweek = int(gpsday / 7) % 1024
gpsdow = gpsday % 7
# Compute day of the year
"""
print "# %s is gpsday %s (cycle %d week %d dow %d; yday %d)" % (
gdate.strftime("%Y-%m-%d"),
gpsday,
gpscycle,
gpsweek,
gpsdow,
yday,
)
"""
# Select correct base url.
urls = build_urls_for(year, yday)
print "%s%s" % (cmd, urls[site_abbr],)
def test_jd2gcal():
assert jd2gcal(*gcal2jd(2000, 1, 1)) == (2000, 1, 1, 0.0)
assert jd2gcal(*gcal2jd(1950, 1, 1)) == (1950, 1, 1, 0.0)
assert jd2gcal(*gcal2jd(1999, 10, 12)) == (1999, 10, 12, 0.0)
assert jd2gcal(*gcal2jd(2000, 2, 30)) == (2000, 3, 1, 0.0)
assert jd2gcal(*gcal2jd(2000, -2, -4)) == (1999, 9, 26, 0.0)
#
# I hope this information be useful for you.
#
# Please do not hesitate to let me know if you need anything else.
#
# Regards
#
# Emiliano
#
####### Macon tipper data
ts,tau, tau_s = np.genfromtxt('/Users/hamilton/CMB/Interfero/Sites/FromEmiliano/tipper_macon.dat',skiprows=1,invalid_raise=False).T
import jdcal as jdcal
init = np.sum(jdcal.gcal2jd(1992,1,1))
newts = init+ts
yy=[]
mm=[]
dd=[]
ut=[]
for thets in ts:
theyy, themm, thedd, theut = jdcal.jd2gcal(init,thets)
yy.append(theyy)
mm.append(themm)
dd.append(thedd)
ut.append(theut)
clf()
plot(time,tau,',')
