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	English	Chinese (Simplified)	Actions
	Astrometry	天体测量
	Astrometry is the science dealing with the positions and motions of celestial objects. Astrometry is essential in modern astrophotography where capture software like N.I.N.A, Ekos, APT or others, plate solve the images in order to obtain an astrometric solution, meaning they will precisely know the position of the frame with regards to the sky. Astrometry can also be used at processing stage, like in photometric color calibration tool for example.	天体测量学着重于天体的位置和运动，是现代天文观测软件如N.I.N.A，Ekos，APT中的重要组成部分。解析（Plate Solving）图像可以获知图像的精确位置。在图像处理阶段，如测光色彩校准工具中也需要用到天体测量。
	Color Management	色彩管理
	Siril now offers a fully color managed workflow using ICC profiles. By ensuring accurate and consistent color reproduction across different devices, Siril enables you to edit your images with confidence, knowing that the colors you see on your screen will translate faithfully to prints or other displays. You can edit your images in color spaces better matched to the capabilities of a wide gamut professional photo printer, thus allowing production of prints with richer colors than are possible when working in the standard sRGB color space, and you can produce images that your audience will be able to view consistently with how you see them during editing, regardless of their display device.
	There are several pages in this section of the documentation: between them they aim to provide a basic outline of what color management does, how it can help you and how it works in Siril.
	Back to index	回到索引
	Scriptable	可编程的
	Non scriptable	不可编程的
	Commands	指令
	The following page lists all the commands available in Siril \|release\|.	此页面中列出了Siril \|release\| 中的可用指令。
	You can access an index by clicking this icon \|indexlink\|.	使用 \|indexlink\| 查看索引。
	Commands marked with this icon \|scriptable\| can be used in scripts while those marked with this one \|nonscriptable\| cannot.	用 \|scriptable\| 标记的指令可以被用在脚本中，而 \|nonscriptable\| 则不行。
	For all the sequence commands, you can replace argument sequencename with a ``.`` if the sequence to be processed is already loaded.	对于所有指令，如果序列已经加载，你可以将参数sequencename设置为``.``。
	If you want to provide an argument that includes a string with spaces, for example a filename, you need to quote the entire argument not just the string. So for example you should use ``command "-filename=My File.fits"``, not ``command -filename="My File.fits"``.	如果您想提供一个包含空格的字符串参数，例如文件名，您需要引用整个参数，而不仅仅是字符串。因此，例如，您应该使用command“-filename=My File.fits”，而不是command-filename=“My File.fts”。
	:commandname:`addmax` \|nonscriptable\| \|indexlink\|	:commandname:`addmax` \|nonscriptable\| \|indexlink\|
	Computes a new image combining the image in memory with the image filename. At each pixel location, the new value is determined as the max of value in current image and in filename	将内存中的图像与filename合并成新图像。每个像素是当前图像和filename同样位置像素的最大值
	:commandname:`asinh` \|scriptable\| \|indexlink\|	:commandname:`asinh` \|scriptable\| \|indexlink\|
	Stretches the image to show faint objects using an hyperbolic arcsin transformation. The mandatory argument stretch, typically between 1 and 1000, will give the strength of the stretch. The black point can be offset by providing an optional offset argument in the normalized pixel value of [0, 1]. Finally the option -human enables using human eye luminous efficiency weights to compute the luminance used to compute the stretch value for each pixel, instead of the simple mean of the channels pixel values. This stretch method preserves lightness from the L\a\b\* color space	使用双曲arcsin函数拉伸图像，使暗淡的星点可见。必填选项stretch（一般于1到1000之间）描述了拉伸强度。黑点可由可选选项offset指定（在归一化后的[0, 1]之间）。-human选项使用人眼亮度感知权重代替简单的各通道亮度平均值。拉伸在L\a\b\*颜色空间中保持亮度
	:commandname:`autoghs` \|scriptable\| \|indexlink\|	:commandname:`autoghs` \|scriptable\| \|indexlink\|
	Application of the generalized hyperbolic stretch with a symmetry point SP defined as k.sigma from the median of each channel (the provided shadowsclip value is the k here and can be negative). By default, SP and the stretch are computed per channel; SP can be computed as a mean of image channels by passing -linked. The stretch amount D is provided in the second mandatory argument.
	Implicit values of 13 for B, making it very focused on the SP brightness range, 0.7 for HP, 0 for LP are used but can be changed with the options of the same names
	:commandname:`autostretch` \|scriptable\| \|indexlink\|	:commandname:`autostretch` \|scriptable\| \|indexlink\|
	Auto-stretches the currently loaded image, with different parameters for each channel (unlinked) unless -linked is passed. Arguments are optional, shadowclip is the shadows clipping point, measured in sigma units from the main histogram peak (default is -2.8), targetbg is the target background value, giving a final brightness to the image, range [0, 1], default is 0.25. The default values are those used in the Auto-stretch rendering from the GUI.	自动拉伸当前加载的图像，每个通道具有不同的参数（unlinked），除非传递 -linked 。参数是可选的，shadowclip是阴影剪切点，以西格玛单位从主直方图峰值测量（默认为-2.8），targetbg是目标背景值，为图像提供最终亮度，范围 [0, 1]，默认为 0.25。默认值是 GUI 中自动拉伸渲染中使用的值。
	Do not use the unlinked version after color calibration, it will alter the white balance
	:commandname:`bg` \|scriptable\| \|indexlink\|	:commandname:`bg` \|scriptable\| \|indexlink\|
	Returns the background level of the loaded image	返回载入图像的背景值
	:commandname:`bgnoise` \|scriptable\| \|indexlink\|	:commandname:`bgnoise` \|scriptable\| \|indexlink\|
	Returns the background noise level of the loaded image	返回载入图像的背景噪声级别
	For more information, see the :ref:`statistics documentation <Statistics:Background noise>`
	:commandname:`binxy` \|scriptable\| \|indexlink\|	:commandname:`binxy` \|scriptable\| \|indexlink\|

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	English	Chinese (Simplified)	Actions
	Astrometry	天体测量
	Astrometry is the science dealing with the positions and motions of celestial objects. Astrometry is essential in modern astrophotography where capture software like N.I.N.A, Ekos, APT or others, plate solve the images in order to obtain an astrometric solution, meaning they will precisely know the position of the frame with regards to the sky. Astrometry can also be used at processing stage, like in photometric color calibration tool for example.	天体测量学着重于天体的位置和运动，是现代天文观测软件如N.I.N.A，Ekos，APT中的重要组成部分。解析（Plate Solving）图像可以获知图像的精确位置。在图像处理阶段，如测光色彩校准工具中也需要用到天体测量。
	Color Management	色彩管理
	Siril now offers a fully color managed workflow using ICC profiles. By ensuring accurate and consistent color reproduction across different devices, Siril enables you to edit your images with confidence, knowing that the colors you see on your screen will translate faithfully to prints or other displays. You can edit your images in color spaces better matched to the capabilities of a wide gamut professional photo printer, thus allowing production of prints with richer colors than are possible when working in the standard sRGB color space, and you can produce images that your audience will be able to view consistently with how you see them during editing, regardless of their display device.
	There are several pages in this section of the documentation: between them they aim to provide a basic outline of what color management does, how it can help you and how it works in Siril.
	Back to index	回到索引
	Scriptable	可编程的
	Non scriptable	不可编程的
	Commands	指令
	The following page lists all the commands available in Siril \|release\|.	此页面中列出了Siril \|release\| 中的可用指令。
	You can access an index by clicking this icon \|indexlink\|.	使用 \|indexlink\| 查看索引。
	Commands marked with this icon \|scriptable\| can be used in scripts while those marked with this one \|nonscriptable\| cannot.	用 \|scriptable\| 标记的指令可以被用在脚本中，而 \|nonscriptable\| 则不行。
	For all the sequence commands, you can replace argument sequencename with a ``.`` if the sequence to be processed is already loaded.	对于所有指令，如果序列已经加载，你可以将参数sequencename设置为``.``。
	If you want to provide an argument that includes a string with spaces, for example a filename, you need to quote the entire argument not just the string. So for example you should use ``command "-filename=My File.fits"``, not ``command -filename="My File.fits"``.	如果您想提供一个包含空格的字符串参数，例如文件名，您需要引用整个参数，而不仅仅是字符串。因此，例如，您应该使用command“-filename=My File.fits”，而不是command-filename=“My File.fts”。
	:commandname:`addmax` \|nonscriptable\| \|indexlink\|	:commandname:`addmax` \|nonscriptable\| \|indexlink\|
	Computes a new image combining the image in memory with the image filename. At each pixel location, the new value is determined as the max of value in current image and in filename	将内存中的图像与filename合并成新图像。每个像素是当前图像和filename同样位置像素的最大值
	:commandname:`asinh` \|scriptable\| \|indexlink\|	:commandname:`asinh` \|scriptable\| \|indexlink\|
	Stretches the image to show faint objects using an hyperbolic arcsin transformation. The mandatory argument stretch, typically between 1 and 1000, will give the strength of the stretch. The black point can be offset by providing an optional offset argument in the normalized pixel value of [0, 1]. Finally the option -human enables using human eye luminous efficiency weights to compute the luminance used to compute the stretch value for each pixel, instead of the simple mean of the channels pixel values. This stretch method preserves lightness from the L\a\b\* color space	使用双曲arcsin函数拉伸图像，使暗淡的星点可见。必填选项stretch（一般于1到1000之间）描述了拉伸强度。黑点可由可选选项offset指定（在归一化后的[0, 1]之间）。-human选项使用人眼亮度感知权重代替简单的各通道亮度平均值。拉伸在L\a\b\*颜色空间中保持亮度
	:commandname:`autoghs` \|scriptable\| \|indexlink\|	:commandname:`autoghs` \|scriptable\| \|indexlink\|
	Application of the generalized hyperbolic stretch with a symmetry point SP defined as k.sigma from the median of each channel (the provided shadowsclip value is the k here and can be negative). By default, SP and the stretch are computed per channel; SP can be computed as a mean of image channels by passing -linked. The stretch amount D is provided in the second mandatory argument.
	Implicit values of 13 for B, making it very focused on the SP brightness range, 0.7 for HP, 0 for LP are used but can be changed with the options of the same names
	:commandname:`autostretch` \|scriptable\| \|indexlink\|	:commandname:`autostretch` \|scriptable\| \|indexlink\|
	Auto-stretches the currently loaded image, with different parameters for each channel (unlinked) unless -linked is passed. Arguments are optional, shadowclip is the shadows clipping point, measured in sigma units from the main histogram peak (default is -2.8), targetbg is the target background value, giving a final brightness to the image, range [0, 1], default is 0.25. The default values are those used in the Auto-stretch rendering from the GUI.	自动拉伸当前加载的图像，每个通道具有不同的参数（unlinked），除非传递 -linked 。参数是可选的，shadowclip是阴影剪切点，以西格玛单位从主直方图峰值测量（默认为-2.8），targetbg是目标背景值，为图像提供最终亮度，范围 [0, 1]，默认为 0.25。默认值是 GUI 中自动拉伸渲染中使用的值。
	Do not use the unlinked version after color calibration, it will alter the white balance
	:commandname:`bg` \|scriptable\| \|indexlink\|	:commandname:`bg` \|scriptable\| \|indexlink\|
	Returns the background level of the loaded image	返回载入图像的背景值
	:commandname:`bgnoise` \|scriptable\| \|indexlink\|	:commandname:`bgnoise` \|scriptable\| \|indexlink\|
	Returns the background noise level of the loaded image	返回载入图像的背景噪声级别
	For more information, see the :ref:`statistics documentation <Statistics:Background noise>`
	:commandname:`binxy` \|scriptable\| \|indexlink\|	:commandname:`binxy` \|scriptable\| \|indexlink\|