Perform dayofyear-based calculations according to UTC, not local time #2055
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| Original file line number | Diff line number | Diff line change |
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@@ -23,7 +23,7 @@ | |
| import scipy.optimize as so | ||
| import warnings | ||
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| from pvlib import atmosphere, tools | ||
| from pvlib.tools import datetime_to_djd, djd_to_datetime | ||
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@@ -199,11 +199,7 @@ | |
| raise ImportError('Could not import built-in SPA calculator. ' + | ||
| 'You may need to recompile the SPA code.') | ||
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| time_utc = tools._pandas_to_utc(time) | ||
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| spa_out = [] | ||
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@@ -378,7 +374,9 @@ | |
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| spa = _spa_python_import(how) | ||
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| if not delta_t: | ||
| time_utc = tools._pandas_to_utc(time) | ||
| delta_t = spa.calculate_deltat(time_utc.year, time_utc.month) | ||
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| app_zenith, zenith, app_elevation, elevation, azimuth, eot = \ | ||
| spa.solar_position(unixtime, lat, lon, elev, pressure, temperature, | ||
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@@ -452,12 +450,13 @@ | |
| raise ValueError('times must be localized') | ||
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| # must convert to midnight UTC on day of interest | ||
| times_utc = times.tz_convert('UTC') | ||
| unixtime = _datetime_to_unixtime(times_utc.normalize()) | ||
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| spa = _spa_python_import(how) | ||
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| if not delta_t: | ||
| delta_t = spa.calculate_deltat(times_utc.year, times_utc.month) | ||
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| transit, sunrise, sunset = spa.transit_sunrise_sunset( | ||
| unixtime, lat, lon, delta_t, numthreads) | ||
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@@ -581,12 +580,11 @@ | |
| sunrise = [] | ||
| sunset = [] | ||
| trans = [] | ||
| for thetime in tools._pandas_to_utc(times): | ||
| # older versions of pyephem ignore timezone when converting to its | ||
| # internal datetime format, so convert to UTC here to support | ||
| # all versions. GH #1449 | ||
| obs.date = ephem.Date(thetime) | ||
| sunrise.append(_ephem_to_timezone(rising(sun), tzinfo)) | ||
| sunset.append(_ephem_to_timezone(setting(sun), tzinfo)) | ||
| trans.append(_ephem_to_timezone(transit(sun), tzinfo)) | ||
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@@ -644,11 +642,7 @@ | |
| except ImportError: | ||
| raise ImportError('PyEphem must be installed') | ||
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| time_utc = tools._pandas_to_utc(time) | ||
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| sun_coords = pd.DataFrame(index=time) | ||
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@@ -765,11 +759,7 @@ | |
| # the SPA algorithm needs time to be expressed in terms of | ||
| # decimal UTC hours of the day of the year. | ||
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| time_utc = tools._pandas_to_utc(time) | ||
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| # strip out the day of the year and calculate the decimal hour | ||
| DayOfYear = time_utc.dayofyear | ||
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@@ -956,7 +946,10 @@ | |
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| sun = ephem.Sun() | ||
| earthsun = [] | ||
| for thetime in tools._pandas_to_utc(time): | ||
| # older versions of pyephem ignore timezone when converting to its | ||
| # internal datetime format, so convert to UTC here to support | ||
| # all versions. GH #1449 | ||
| sun.compute(ephem.Date(thetime)) | ||
| earthsun.append(sun.earth_distance) | ||
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@@ -1013,7 +1006,9 @@ | |
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| spa = _spa_python_import(how) | ||
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| if not delta_t: | ||
| time_utc = tools._pandas_to_utc(time) | ||
| delta_t = spa.calculate_deltat(time_utc.year, time_utc.month) | ||
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| dist = spa.earthsun_distance(unixtime, delta_t, numthreads) | ||
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@@ -1386,22 +1381,26 @@ | |
| equation_of_time_spencer71 | ||
| equation_of_time_pvcdrom | ||
| """ | ||
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| # times must be localized | ||
| if not times.tz: | ||
| raise ValueError('times must be localized') | ||
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| # hours - timezone = (times - normalized_times) - (naive_times - times) | ||
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Comment on lines
+1385
to
-1391
There was a problem hiding this comment. I'm not sure I agree with this change. The docstring says the input timestamps "must be localized to the timezone for the longitude", which is inconsistent with the previous behavior (localize to UTC if not already localized), so I can see some change being needed here. But why is this the correct change? There was a problem hiding this comment. It was added in accordance with pvlib-python/pvlib/solarposition.py Lines 448 to 452 in 524fa55 pvlib-python/pvlib/solarposition.py Lines 560 to 564 in 524fa55 |
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| tzs = np.array([ts.utcoffset().total_seconds() for ts in times]) / 3600 | ||
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| hrs_minus_tzs = _times_to_hours_after_local_midnight(times) - tzs | ||
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| return 15. * (hrs_minus_tzs - 12.) + longitude + equation_of_time / 4. | ||
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| def _hour_angle_to_hours(times, hourangle, longitude, equation_of_time): | ||
| """converts hour angles in degrees to hours as a numpy array""" | ||
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| # times must be localized | ||
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| if not times.tz: | ||
| raise ValueError('times must be localized') | ||
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| tzs = np.array([ts.utcoffset().total_seconds() for ts in times]) / 3600 | ||
| hours = (hourangle - longitude - equation_of_time / 4.) / 15. + 12. + tzs | ||
| return np.asarray(hours) | ||
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@@ -1411,18 +1410,26 @@ | |
| """ | ||
| converts hours since midnight from an array of floats to localized times | ||
| """ | ||
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| # times must be localized | ||
| if not times.tz: | ||
| raise ValueError('times must be localized') | ||
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| # normalize local times to previous local midnight and add the hours until | ||
| # sunrise, sunset, and transit | ||
| return times.normalize() + pd.to_timedelta(hours, unit='h') | ||
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| def _times_to_hours_after_local_midnight(times): | ||
| """convert local pandas datetime indices to array of hours as floats""" | ||
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| # times must be localized | ||
| if not times.tz: | ||
| raise ValueError('times must be localized') | ||
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| hrs = (times - times.normalize()) / pd.Timedelta('1h') | ||
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| # ensure array return instead of a version-dependent pandas <T>Index | ||
| return np.array(hrs) | ||
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@@ -1468,6 +1475,11 @@ | |
| CRC Press (2012) | ||
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| """ | ||
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| # times must be localized | ||
| if not times.tz: | ||
| raise ValueError('times must be localized') | ||
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| latitude_rad = np.radians(latitude) # radians | ||
| sunset_angle_rad = np.arccos(-np.tan(declination) * np.tan(latitude_rad)) | ||
| sunset_angle = np.degrees(sunset_angle_rad) # degrees | ||
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