gma 1.x 气候气象指数计算源代码（分享）

本文主要是介绍gma 1.x 气候气象指数计算源代码（分享），希望对大家解决编程问题提供一定的参考价值，需要的开发者们随着小编来一起学习吧！

本模块的主要内建子模块如下：

如何获得完整代码：回复博主或者留言/私信。

注意：本代码完全开源，可随意修改使用。 但如果您的成果使用或参考了本段代码，给予一定的引用说明（非强制），包括但不限于：

1.作者：洛
2.网站：gma.luosgeo.com
3.PyPI：https://pypi.org/project/gma/
3.GitHub：https://github.com/LiChongrui

其中：

clindex：气候指标计算函数
cmana：气候诊断函数
et0：蒸散计算函数
static：气候常量
utils：通用工具

示例代:1：

from ..core.arraypro import *
from .utils import *#################################### 累积概率计算
def GammaCP(Data, Axis):'''gamma 分布累积概率'''if np.nanmin(Data) < 0:Data = Data + np.abs(np.nanmin(Data)) * 2    # Data = Data + 1000PF = ParameterFitting(Data, Axis = Axis)Data = PF.DataAxis = PF.Axis# 计算 0 值概率并填充 0 值 为 NaNZeros = (Data == 0).sum(axis = Axis, keepdims = True)ProbabilitiesOfZero = Zeros / Data.shape[Axis]Data[Data == 0] = np.nanAlphas, Betas = ParameterFitting(Data, Axis = Axis).MLE()# 使用gamma CDF 查找 gamma 概率值GammaProbabilities = stats.gamma.cdf(Data, a = Alphas, scale = Betas)Probabilities = ProbabilitiesOfZero + (1 - ProbabilitiesOfZero) * GammaProbabilitiesreturn Probabilities def LogLogisticCP(Data, Axis):'''Log-Logistic 分布累积概率'''PF = ParameterFitting(Data, Axis)Alpha, Beta, Gamma1 = PF.LMoment()Probabilities = 1 / (1 + (Alpha / (PF.Data - Gamma1)) ** Beta)# 由于 scipy 对 non 值处理过于简单，这里不使用 scipy 的函数# Probabilities = stats.fisk.cdf(PF.Data, Beta, loc = Gamma1, scale = Alpha)return Probabilitiesdef Pearson3CP(Data, Axis):'''pearson III 分布累积概率'''if np.nanmin(Data) < 0:Data = Data + np.abs(np.nanmin(Data)) * 2    PF = ParameterFitting(Data, Axis)Data = PF.DataAxis = PF.Axis  Loc, Scale, Skew = PF.LMoment2()Alpha = 4.0 / (Skew ** 2)MINPossible = Loc - ((Alpha * Scale * Skew) / 2.0)Zeros = (Data == 0).sum(axis = Axis, keepdims = True)ProbabilitiesOfZero = Zeros / Data.shape[Axis]Probabilities = stats.pearson3.cdf(Data, Skew, Loc, Scale)Probabilities[(Data < 0.0005) & (ProbabilitiesOfZero > 0.0)] = 0.0Probabilities[(Data < 0.0005) & (ProbabilitiesOfZero <= 0.0)] = 0.0005Probabilities[(Data <= MINPossible) & (Skew >= 0)] = 0.0005Probabilities[(Data >= MINPossible) & (Skew < 0)] = 0.9995Probabilities = ProbabilitiesOfZero + (1.0 - ProbabilitiesOfZero) * Probabilitiesreturn Probabilitiesdef _ReshapeAndExtend(Data, Axis, Periodicity):'''更改输入数据维度为 （Axis / Periodicity, Periodicity, N），并补充末尾缺失数据'''# 交换设置轴到 0 if Data.ndim > 1:Data = np.swapaxes(Data, 0, Axis)S = Data.shapeS0, S1 = S[0], np.prod(S[1:], dtype = int)Data = Data.reshape((S0, S1))else:Data = np.expand_dims(Data, -1)# 填充不足 Data.shape[0] / PeriodicityB = Data.shape[0] % PeriodicityPW = 0 if B == 0 else Periodicity - BData = np.pad(Data, ((0, PW), (0,0)), mode = "constant", constant_values = np.nan)# 更改为目标维度（3维）PeriodicityTimes = Data.shape[0] // Periodicity return Data.reshape(PeriodicityTimes, Periodicity, Data.shape[1])def _RestoreReshapeAndExtend(Data, Axis, Shape):'''对 _ReshapeAndExtend 修改的维度和数据进行还原'''# 还原为原始维度（2维）Data = Data.reshape(np.prod(Data.shape[:2]), *Data.shape[2:])# 去除尾部填充值Data = Data[:Shape[Axis]]# 还原到初始状态SHP = list(Shape)SHP.pop(Axis)SHP = [Shape[Axis]] + SHPData = Data.reshape(SHP)Data = np.swapaxes(Data, Axis, 0)return Data############### 不同的计算方式
def _Fit(WBInScale, Periodicity, Distribution):'''计算标准化指数'''# 1.计算累积概率Probabilities = eval(f'{Distribution}CP')(WBInScale, 0)if Periodicity == 1:Probabilities = np.expand_dims(Probabilities, 1)# 2.生成结果OutInScale = stats.norm.ppf(Probabilities)return OutInScaledef _API(WBInScale, Axis):'''计算距平指数'''# 1.计算平均值或趋势值Mean = np.nanmean(WBInScale, axis = Axis, dtype = np.float64, keepdims = True)# 4.生成结果OutInScale = (WBInScale - Mean) / Meanreturn OutInScale############### 计算结果
def _Compute(Data, Axis, Scale, Periodicity, Distribution):'''自动计算'''   Periodicity = ValueType(Periodicity, 'pint')# 0.数据准备DP = DataPreparation(Data, Axis) Data = DP.DataSHP = Data.shapeAxis = DP.Axis# 1.计算尺度WBInScale = DP.SumScale(Scale)if not (SHP[Axis] > Periodicity) and (SHP[Axis] > Scale):return np.full(WBInScale.shape, np.nan)# 2.更改输入数据维度为 （Axis / Periodicity, Periodicity, N）WBInScale = _ReshapeAndExtend(WBInScale, Axis, Periodicity)# 3.生成结果if Distribution == 'API':OutInScale = _API(WBInScale, Axis)else:OutInScale = _Fit(WBInScale, Periodicity, Distribution)# 4.还原数据OutInScale = _RestoreReshapeAndExtend(OutInScale, Axis, SHP)    return OutInScale

示例代码2：

#################################### SPEI
def SPEI(PRE, PET, Axis = None, Scale = 1, Periodicity = 12, Distribution = 'LogLogistic'):'''计算SPEI'''Distribution = GetDistribution(Distribution)PRE, PET = INITArray(PRE, PET)WB = np.subtract(PRE, PET, dtype = PRE.dtype)SPEIInScale = _Compute(WB, Axis, Scale, Periodicity, Distribution)return SPEIInScale#################################### SPI
def SPI(PRE, Axis = None, Scale = 1, Periodicity = 12, Distribution = 'Gamma'):'''计算 SPI'''Distribution = GetDistribution(Distribution)SPIInScale = _Compute(PRE, Axis, Scale, Periodicity, Distribution)return SPIInScale#################################### PAP
def PAP(PRE, Axis = None, Scale = 1, Periodicity = 12):'''降水距平百分率'''PAPInScale = _Compute(PRE, Axis, Scale, Periodicity, 'API') return PAPInScale