spectrometer visibleΒΆ
| Path | Dimensions | Type | Units | Description |
|---|---|---|---|---|
spectrometer_visible (alpha) | Spectrometer in visible light range diagnostic | |||
spectrometer_visible.channel (alpha) | [1...N] | STRUCT_ARRAY | Set of channels (detector or pixel of a camera) | |
spectrometer_visible.channel[:].active_spatial_resolution (alpha) | [spectrometer_visible.channel[:].active_spatial_resolution[:].time] | STRUCT_ARRAY | In case of active spectroscopy, describes the spatial resolution of the measurement, calculated as a convolution of the atomic smearing, magnetic and beam geometry smearing and detector projection, for a set of time slices | |
spectrometer_visible.channel[:].active_spatial_resolution[:].centre (alpha) | STRUCTURE | Position of the centre of the spatially resolved zone | ||
spectrometer_visible.channel[:].active_spatial_resolution[:].centre.phi (alpha) | FLT_0D (uncertain) | rad | Toroidal angle (oriented counter-clockwise when viewing from above) | |
spectrometer_visible.channel[:].active_spatial_resolution[:].centre.r (alpha) | FLT_0D (uncertain) | m | Major radius | |
spectrometer_visible.channel[:].active_spatial_resolution[:].centre.z (alpha) | FLT_0D (uncertain) | m | Height | |
spectrometer_visible.channel[:].active_spatial_resolution[:].time (alpha) | FLT_0D | s | Time | |
spectrometer_visible.channel[:].active_spatial_resolution[:].width (alpha) | STRUCTURE | Full width of the spatially resolved zone in the R, Z and phi directions | ||
spectrometer_visible.channel[:].active_spatial_resolution[:].width.phi (alpha) | FLT_0D (uncertain) | rad | Toroidal angle (oriented counter-clockwise when viewing from above) | |
spectrometer_visible.channel[:].active_spatial_resolution[:].width.r (alpha) | FLT_0D (uncertain) | m | Major radius | |
spectrometer_visible.channel[:].active_spatial_resolution[:].width.z (alpha) | FLT_0D (uncertain) | m | Height | |
spectrometer_visible.channel[:].aperture (alpha) | [1...N] | STRUCT_ARRAY | Description of a set of collimating apertures | |
spectrometer_visible.channel[:].aperture[:].centre (alpha) | STRUCTURE | If geometry_type=2, coordinates of the centre of the circle. If geometry_type=1 or 3, coordinates of the origin of the local coordinate system (X1,X2,X3) describing the plane detector/aperture. This origin is located within the detector/aperture area. | ||
spectrometer_visible.channel[:].aperture[:].centre.phi (alpha) | FLT_0D (uncertain) | rad | Toroidal angle (oriented counter-clockwise when viewing from above) | |
spectrometer_visible.channel[:].aperture[:].centre.r (alpha) | FLT_0D (uncertain) | m | Major radius | |
spectrometer_visible.channel[:].aperture[:].centre.z (alpha) | FLT_0D (uncertain) | m | Height | |
spectrometer_visible.channel[:].aperture[:].geometry_type (alpha) | INT_0D | Type of geometry used to describe the surface of the detector or aperture (1:'outline', 2:'circular', 3:'rectangle'). In case of 'outline', the surface is described by an outline of point in a local coordinate system defined by a centre and three unit vectors X1, X2, X3. Note that there is some flexibility here and the data provider should choose the most convenient coordinate system for the object, respecting the definitions of (X1,X2,X3) indicated below. In case of 'circular', the surface is a circle defined by its centre, radius, and normal vector oriented towards the plasma X3. In case of 'rectangle', the surface is a rectangle defined by its centre, widths in the X1 and X2 directions, and normal vector oriented towards the plasma X3. | ||
spectrometer_visible.channel[:].aperture[:].outline (alpha) | STRUCTURE | Irregular outline of the detector/aperture in the (X1, X2) coordinate system. Do NOT repeat the first point. | ||
spectrometer_visible.channel[:].aperture[:].outline.x1 (alpha) | [1...N] | FLT_1D (uncertain) | m | Positions along x1 axis |
spectrometer_visible.channel[:].aperture[:].outline.x2 (alpha) | [spectrometer_visible.channel[:].aperture[:].outline.x1] | FLT_1D (uncertain) | m | Positions along x2 axis |
spectrometer_visible.channel[:].aperture[:].radius (alpha) | FLT_0D (uncertain) | m | Radius of the circle, used only if geometry_type = 2 | |
spectrometer_visible.channel[:].aperture[:].surface (alpha) | FLT_0D (uncertain) | m^2 | Surface of the detector/aperture, derived from the above geometric data | |
spectrometer_visible.channel[:].aperture[:].x1_unit_vector (alpha) | STRUCTURE | Components of the X1 direction unit vector in the (X,Y,Z) coordinate system, where X is the major radius axis for phi = 0, Y is the major radius axis for phi = pi/2, and Z is the height axis. The X1 vector is more horizontal than X2 (has a smaller abs(Z) component) and oriented in the positive phi direction (counter-clockwise when viewing from above). | ||
spectrometer_visible.channel[:].aperture[:].x1_unit_vector.x (alpha) | FLT_0D (uncertain) | m | Component along X axis | |
spectrometer_visible.channel[:].aperture[:].x1_unit_vector.y (alpha) | FLT_0D (uncertain) | m | Component along Y axis | |
spectrometer_visible.channel[:].aperture[:].x1_unit_vector.z (alpha) | FLT_0D (uncertain) | m | Component along Z axis | |
spectrometer_visible.channel[:].aperture[:].x1_width (alpha) | FLT_0D (uncertain) | m | Full width of the aperture in the X1 direction, used only if geometry_type = 3 | |
spectrometer_visible.channel[:].aperture[:].x2_unit_vector (alpha) | STRUCTURE | Components of the X2 direction unit vector in the (X,Y,Z) coordinate system, where X is the major radius axis for phi = 0, Y is the major radius axis for phi = pi/2, and Z is the height axis. The X2 axis is orthonormal so that uX2 = uX3 x uX1. | ||
spectrometer_visible.channel[:].aperture[:].x2_unit_vector.x (alpha) | FLT_0D (uncertain) | m | Component along X axis | |
spectrometer_visible.channel[:].aperture[:].x2_unit_vector.y (alpha) | FLT_0D (uncertain) | m | Component along Y axis | |
spectrometer_visible.channel[:].aperture[:].x2_unit_vector.z (alpha) | FLT_0D (uncertain) | m | Component along Z axis | |
spectrometer_visible.channel[:].aperture[:].x2_width (alpha) | FLT_0D (uncertain) | m | Full width of the aperture in the X2 direction, used only if geometry_type = 3 | |
spectrometer_visible.channel[:].aperture[:].x3_unit_vector (alpha) | STRUCTURE | Components of the X3 direction unit vector in the (X,Y,Z) coordinate system, where X is the major radius axis for phi = 0, Y is the major radius axis for phi = pi/2, and Z is the height axis. The X3 axis is normal to the detector/aperture plane and oriented towards the plasma. | ||
spectrometer_visible.channel[:].aperture[:].x3_unit_vector.x (alpha) | FLT_0D (uncertain) | m | Component along X axis | |
spectrometer_visible.channel[:].aperture[:].x3_unit_vector.y (alpha) | FLT_0D (uncertain) | m | Component along Y axis | |
spectrometer_visible.channel[:].aperture[:].x3_unit_vector.z (alpha) | FLT_0D (uncertain) | m | Component along Z axis | |
spectrometer_visible.channel[:].detector (alpha) | STRUCTURE | Detector description | ||
spectrometer_visible.channel[:].detector.centre (alpha) | STRUCTURE | If geometry_type=2, coordinates of the centre of the circle. If geometry_type=1 or 3, coordinates of the origin of the local coordinate system (X1,X2,X3) describing the plane detector/aperture. This origin is located within the detector/aperture area. | ||
spectrometer_visible.channel[:].detector.centre.phi (alpha) | FLT_0D (uncertain) | rad | Toroidal angle (oriented counter-clockwise when viewing from above) | |
spectrometer_visible.channel[:].detector.centre.r (alpha) | FLT_0D (uncertain) | m | Major radius | |
spectrometer_visible.channel[:].detector.centre.z (alpha) | FLT_0D (uncertain) | m | Height | |
spectrometer_visible.channel[:].detector.geometry_type (alpha) | INT_0D | Type of geometry used to describe the surface of the detector or aperture (1:'outline', 2:'circular', 3:'rectangle'). In case of 'outline', the surface is described by an outline of point in a local coordinate system defined by a centre and three unit vectors X1, X2, X3. Note that there is some flexibility here and the data provider should choose the most convenient coordinate system for the object, respecting the definitions of (X1,X2,X3) indicated below. In case of 'circular', the surface is a circle defined by its centre, radius, and normal vector oriented towards the plasma X3. In case of 'rectangle', the surface is a rectangle defined by its centre, widths in the X1 and X2 directions, and normal vector oriented towards the plasma X3. | ||
spectrometer_visible.channel[:].detector.outline (alpha) | STRUCTURE | Irregular outline of the detector/aperture in the (X1, X2) coordinate system. Do NOT repeat the first point. | ||
spectrometer_visible.channel[:].detector.outline.x1 (alpha) | [1...N] | FLT_1D (uncertain) | m | Positions along x1 axis |
spectrometer_visible.channel[:].detector.outline.x2 (alpha) | [spectrometer_visible.channel[:].detector.outline.x1] | FLT_1D (uncertain) | m | Positions along x2 axis |
spectrometer_visible.channel[:].detector.radius (alpha) | FLT_0D (uncertain) | m | Radius of the circle, used only if geometry_type = 2 | |
spectrometer_visible.channel[:].detector.surface (alpha) | FLT_0D (uncertain) | m^2 | Surface of the detector/aperture, derived from the above geometric data | |
spectrometer_visible.channel[:].detector.x1_unit_vector (alpha) | STRUCTURE | Components of the X1 direction unit vector in the (X,Y,Z) coordinate system, where X is the major radius axis for phi = 0, Y is the major radius axis for phi = pi/2, and Z is the height axis. The X1 vector is more horizontal than X2 (has a smaller abs(Z) component) and oriented in the positive phi direction (counter-clockwise when viewing from above). | ||
spectrometer_visible.channel[:].detector.x1_unit_vector.x (alpha) | FLT_0D (uncertain) | m | Component along X axis | |
spectrometer_visible.channel[:].detector.x1_unit_vector.y (alpha) | FLT_0D (uncertain) | m | Component along Y axis | |
spectrometer_visible.channel[:].detector.x1_unit_vector.z (alpha) | FLT_0D (uncertain) | m | Component along Z axis | |
spectrometer_visible.channel[:].detector.x1_width (alpha) | FLT_0D (uncertain) | m | Full width of the aperture in the X1 direction, used only if geometry_type = 3 | |
spectrometer_visible.channel[:].detector.x2_unit_vector (alpha) | STRUCTURE | Components of the X2 direction unit vector in the (X,Y,Z) coordinate system, where X is the major radius axis for phi = 0, Y is the major radius axis for phi = pi/2, and Z is the height axis. The X2 axis is orthonormal so that uX2 = uX3 x uX1. | ||
spectrometer_visible.channel[:].detector.x2_unit_vector.x (alpha) | FLT_0D (uncertain) | m | Component along X axis | |
spectrometer_visible.channel[:].detector.x2_unit_vector.y (alpha) | FLT_0D (uncertain) | m | Component along Y axis | |
spectrometer_visible.channel[:].detector.x2_unit_vector.z (alpha) | FLT_0D (uncertain) | m | Component along Z axis | |
spectrometer_visible.channel[:].detector.x2_width (alpha) | FLT_0D (uncertain) | m | Full width of the aperture in the X2 direction, used only if geometry_type = 3 | |
spectrometer_visible.channel[:].detector.x3_unit_vector (alpha) | STRUCTURE | Components of the X3 direction unit vector in the (X,Y,Z) coordinate system, where X is the major radius axis for phi = 0, Y is the major radius axis for phi = pi/2, and Z is the height axis. The X3 axis is normal to the detector/aperture plane and oriented towards the plasma. | ||
spectrometer_visible.channel[:].detector.x3_unit_vector.x (alpha) | FLT_0D (uncertain) | m | Component along X axis | |
spectrometer_visible.channel[:].detector.x3_unit_vector.y (alpha) | FLT_0D (uncertain) | m | Component along Y axis | |
spectrometer_visible.channel[:].detector.x3_unit_vector.z (alpha) | FLT_0D (uncertain) | m | Component along Z axis | |
spectrometer_visible.channel[:].detector_image (alpha) | STRUCTURE | Image of the detector or pixel on the focal plane of the optical system | ||
spectrometer_visible.channel[:].detector_image.circular (alpha) | STRUCTURE | Description of circular or elliptic image | ||
spectrometer_visible.channel[:].detector_image.circular.ellipticity (alpha) | FLT_0D (uncertain) | - | Ellipticity | |
spectrometer_visible.channel[:].detector_image.circular.radius (alpha) | FLT_0D (uncertain) | m | Radius of the circle | |
spectrometer_visible.channel[:].detector_image.geometry_type (alpha) | INT_0D | Type of geometry used to describe the image (1:'outline', 2:'circular') | ||
spectrometer_visible.channel[:].detector_image.outline (alpha) | STRUCTURE | Coordinates of the points shaping the polygon of the image | ||
spectrometer_visible.channel[:].detector_image.outline.phi (alpha) | [spectrometer_visible.channel[:].detector_image.outline.r] | FLT_1D (uncertain) | rad | Toroidal angle (oriented counter-clockwise when viewing from above) |
spectrometer_visible.channel[:].detector_image.outline.r (alpha) | [1...N] | FLT_1D (uncertain) | m | Major radius |
spectrometer_visible.channel[:].detector_image.outline.z (alpha) | [spectrometer_visible.channel[:].detector_image.outline.r] | FLT_1D (uncertain) | m | Height |
spectrometer_visible.channel[:].etendue (alpha) | FLT_0D (uncertain) | m^2.str | Etendue (geometric extent) of the channel's optical system | |
spectrometer_visible.channel[:].etendue_method (alpha) | STRUCTURE | Method used to calculate the etendue. Index = 0 : exact calculation with a 4D integral; 1 : approximation with first order formula (detector surface times solid angle subtended by the apertures); 2 : other methods | ||
spectrometer_visible.channel[:].etendue_method.description (alpha) | STR_0D | Verbose description | ||
spectrometer_visible.channel[:].etendue_method.index (alpha) | INT_0D | Integer identifier (enumeration index within a list). Private identifier values must be indicated by a negative index. | ||
spectrometer_visible.channel[:].etendue_method.name (alpha) | STR_0D | Short string identifier | ||
spectrometer_visible.channel[:].fibre_bundle (alpha) | STRUCTURE | Description of the fibre bundle | ||
spectrometer_visible.channel[:].fibre_bundle.fibre_positions (alpha) | STRUCTURE | Individual fibres centres positions in the (X1, X2) coordinate system | ||
spectrometer_visible.channel[:].fibre_bundle.fibre_positions.x1 (alpha) | [1...N] | FLT_1D (uncertain) | m | Positions along x1 axis |
spectrometer_visible.channel[:].fibre_bundle.fibre_positions.x2 (alpha) | [spectrometer_visible.channel[:].fibre_bundle.fibre_positions.x1] | FLT_1D (uncertain) | m | Positions along x2 axis |
spectrometer_visible.channel[:].fibre_bundle.fibre_radius (alpha) | FLT_0D (uncertain) | m | Radius of a single fibre | |
spectrometer_visible.channel[:].fibre_bundle.geometry (alpha) | STRUCTURE | Geometry of the fibre bundle entrance | ||
spectrometer_visible.channel[:].fibre_bundle.geometry.centre (alpha) | STRUCTURE | If geometry_type=2, coordinates of the centre of the circle. If geometry_type=1 or 3, coordinates of the origin of the local coordinate system (X1,X2,X3) describing the plane detector/aperture. This origin is located within the detector/aperture area. | ||
spectrometer_visible.channel[:].fibre_bundle.geometry.centre.phi (alpha) | FLT_0D (uncertain) | rad | Toroidal angle (oriented counter-clockwise when viewing from above) | |
spectrometer_visible.channel[:].fibre_bundle.geometry.centre.r (alpha) | FLT_0D (uncertain) | m | Major radius | |
spectrometer_visible.channel[:].fibre_bundle.geometry.centre.z (alpha) | FLT_0D (uncertain) | m | Height | |
spectrometer_visible.channel[:].fibre_bundle.geometry.geometry_type (alpha) | INT_0D | Type of geometry used to describe the surface of the detector or aperture (1:'outline', 2:'circular', 3:'rectangle'). In case of 'outline', the surface is described by an outline of point in a local coordinate system defined by a centre and three unit vectors X1, X2, X3. Note that there is some flexibility here and the data provider should choose the most convenient coordinate system for the object, respecting the definitions of (X1,X2,X3) indicated below. In case of 'circular', the surface is a circle defined by its centre, radius, and normal vector oriented towards the plasma X3. In case of 'rectangle', the surface is a rectangle defined by its centre, widths in the X1 and X2 directions, and normal vector oriented towards the plasma X3. | ||
spectrometer_visible.channel[:].fibre_bundle.geometry.outline (alpha) | STRUCTURE | Irregular outline of the detector/aperture in the (X1, X2) coordinate system. Do NOT repeat the first point. | ||
spectrometer_visible.channel[:].fibre_bundle.geometry.outline.x1 (alpha) | [1...N] | FLT_1D (uncertain) | m | Positions along x1 axis |
spectrometer_visible.channel[:].fibre_bundle.geometry.outline.x2 (alpha) | [spectrometer_visible.channel[:].fibre_bundle.geometry.outline.x1] | FLT_1D (uncertain) | m | Positions along x2 axis |
spectrometer_visible.channel[:].fibre_bundle.geometry.radius (alpha) | FLT_0D (uncertain) | m | Radius of the circle, used only if geometry_type = 2 | |
spectrometer_visible.channel[:].fibre_bundle.geometry.surface (alpha) | FLT_0D (uncertain) | m^2 | Surface of the detector/aperture, derived from the above geometric data | |
spectrometer_visible.channel[:].fibre_bundle.geometry.x1_unit_vector (alpha) | STRUCTURE | Components of the X1 direction unit vector in the (X,Y,Z) coordinate system, where X is the major radius axis for phi = 0, Y is the major radius axis for phi = pi/2, and Z is the height axis. The X1 vector is more horizontal than X2 (has a smaller abs(Z) component) and oriented in the positive phi direction (counter-clockwise when viewing from above). | ||
spectrometer_visible.channel[:].fibre_bundle.geometry.x1_unit_vector.x (alpha) | FLT_0D (uncertain) | m | Component along X axis | |
spectrometer_visible.channel[:].fibre_bundle.geometry.x1_unit_vector.y (alpha) | FLT_0D (uncertain) | m | Component along Y axis | |
spectrometer_visible.channel[:].fibre_bundle.geometry.x1_unit_vector.z (alpha) | FLT_0D (uncertain) | m | Component along Z axis | |
spectrometer_visible.channel[:].fibre_bundle.geometry.x1_width (alpha) | FLT_0D (uncertain) | m | Full width of the aperture in the X1 direction, used only if geometry_type = 3 | |
spectrometer_visible.channel[:].fibre_bundle.geometry.x2_unit_vector (alpha) | STRUCTURE | Components of the X2 direction unit vector in the (X,Y,Z) coordinate system, where X is the major radius axis for phi = 0, Y is the major radius axis for phi = pi/2, and Z is the height axis. The X2 axis is orthonormal so that uX2 = uX3 x uX1. | ||
spectrometer_visible.channel[:].fibre_bundle.geometry.x2_unit_vector.x (alpha) | FLT_0D (uncertain) | m | Component along X axis | |
spectrometer_visible.channel[:].fibre_bundle.geometry.x2_unit_vector.y (alpha) | FLT_0D (uncertain) | m | Component along Y axis | |
spectrometer_visible.channel[:].fibre_bundle.geometry.x2_unit_vector.z (alpha) | FLT_0D (uncertain) | m | Component along Z axis | |
spectrometer_visible.channel[:].fibre_bundle.geometry.x2_width (alpha) | FLT_0D (uncertain) | m | Full width of the aperture in the X2 direction, used only if geometry_type = 3 | |
spectrometer_visible.channel[:].fibre_bundle.geometry.x3_unit_vector (alpha) | STRUCTURE | Components of the X3 direction unit vector in the (X,Y,Z) coordinate system, where X is the major radius axis for phi = 0, Y is the major radius axis for phi = pi/2, and Z is the height axis. The X3 axis is normal to the detector/aperture plane and oriented towards the plasma. | ||
spectrometer_visible.channel[:].fibre_bundle.geometry.x3_unit_vector.x (alpha) | FLT_0D (uncertain) | m | Component along X axis | |
spectrometer_visible.channel[:].fibre_bundle.geometry.x3_unit_vector.y (alpha) | FLT_0D (uncertain) | m | Component along Y axis | |
spectrometer_visible.channel[:].fibre_bundle.geometry.x3_unit_vector.z (alpha) | FLT_0D (uncertain) | m | Component along Z axis | |
spectrometer_visible.channel[:].fibre_image (alpha) | STRUCTURE | Image of the optical fibre on the focal plane of the optical system | ||
spectrometer_visible.channel[:].fibre_image.circular (alpha) | STRUCTURE | Description of circular or elliptic image | ||
spectrometer_visible.channel[:].fibre_image.circular.ellipticity (alpha) | FLT_0D (uncertain) | - | Ellipticity | |
spectrometer_visible.channel[:].fibre_image.circular.radius (alpha) | FLT_0D (uncertain) | m | Radius of the circle | |
spectrometer_visible.channel[:].fibre_image.geometry_type (alpha) | INT_0D | Type of geometry used to describe the image (1:'outline', 2:'circular') | ||
spectrometer_visible.channel[:].fibre_image.outline (alpha) | STRUCTURE | Coordinates of the points shaping the polygon of the image | ||
spectrometer_visible.channel[:].fibre_image.outline.phi (alpha) | [spectrometer_visible.channel[:].fibre_image.outline.r] | FLT_1D (uncertain) | rad | Toroidal angle (oriented counter-clockwise when viewing from above) |
spectrometer_visible.channel[:].fibre_image.outline.r (alpha) | [1...N] | FLT_1D (uncertain) | m | Major radius |
spectrometer_visible.channel[:].fibre_image.outline.z (alpha) | [spectrometer_visible.channel[:].fibre_image.outline.r] | FLT_1D (uncertain) | m | Height |
spectrometer_visible.channel[:].filter_spectrometer (alpha) | STRUCTURE | Quantities measured by the channel if connected to a filter spectrometer | ||
spectrometer_visible.channel[:].filter_spectrometer.exposure_time (alpha) | FLT_0D (uncertain) | s | Exposure time | |
spectrometer_visible.channel[:].filter_spectrometer.filter (alpha) | STRUCTURE | Filter description | ||
spectrometer_visible.channel[:].filter_spectrometer.filter.wavelength_central (alpha) | FLT_0D (uncertain) | m | Central wavelength of the filter | |
spectrometer_visible.channel[:].filter_spectrometer.filter.wavelength_width (alpha) | FLT_0D (uncertain) | m | Filter transmission function width (at 90% level) | |
spectrometer_visible.channel[:].filter_spectrometer.output_voltage (alpha) | STRUCTURE | V | Raw voltage output of the whole acquisition chain | |
spectrometer_visible.channel[:].filter_spectrometer.output_voltage.data (alpha) | [spectrometer_visible.channel[:].filter_spectrometer.output_voltage.time] | FLT_1D (uncertain) | V | Data |
spectrometer_visible.channel[:].filter_spectrometer.output_voltage.time (alpha) | [1...N] | FLT_1D_TYPE | s | Time |
spectrometer_visible.channel[:].filter_spectrometer.photoelectric_voltage (alpha) | STRUCTURE | V | Gain corrected and background subtracted voltage | |
spectrometer_visible.channel[:].filter_spectrometer.photoelectric_voltage.data (alpha) | [spectrometer_visible.channel[:].filter_spectrometer.photoelectric_voltage.time] | FLT_1D (uncertain) | V | Data |
spectrometer_visible.channel[:].filter_spectrometer.photoelectric_voltage.time (alpha) | [1...N] | FLT_1D_TYPE | s | Time |
spectrometer_visible.channel[:].filter_spectrometer.photon_count (alpha) | STRUCTURE | s^-1 | Detected photon count | |
spectrometer_visible.channel[:].filter_spectrometer.photon_count.data (alpha) | [spectrometer_visible.channel[:].filter_spectrometer.photon_count.time] | FLT_1D (uncertain) | s^-1 | Data |
spectrometer_visible.channel[:].filter_spectrometer.photon_count.time (alpha) | [1...N] | FLT_1D_TYPE | s | Time |
spectrometer_visible.channel[:].filter_spectrometer.processed_line (alpha) | [1...N] | STRUCT_ARRAY | Set of processed spectral lines (normally a single line is filtered out, but it may happen in some cases that several lines go through the filter). | |
spectrometer_visible.channel[:].filter_spectrometer.processed_line[:].label (alpha) | STR_0D | String identifying the processed line. To avoid ambiguities, the following syntax is used : element with ionization state_wavelength in Angstrom (e.g. WI_4000) | ||
spectrometer_visible.channel[:].filter_spectrometer.processed_line[:].wavelength_central (alpha) | FLT_0D (uncertain) | m | Central wavelength of the processed line | |
spectrometer_visible.channel[:].filter_spectrometer.radiance_calibration (alpha) | [spectrometer_visible.channel[:].filter_spectrometer.wavelengths] | FLT_1D (uncertain) | m^-3.sr^-1 | Radiance calibration |
spectrometer_visible.channel[:].filter_spectrometer.radiance_calibration_date (alpha) | STR_0D | Date of the radiance calibration (yyyy_mm_dd) | ||
spectrometer_visible.channel[:].filter_spectrometer.sensitivity (alpha) | [spectrometer_visible.channel[:].filter_spectrometer.wavelengths] | FLT_1D (uncertain) | V.W^-1 | Photoelectric sensitivity of the detector. This is the conversion factor from the received power on the detector into electric voltage depending on the wavelength |
spectrometer_visible.channel[:].filter_spectrometer.wavelengths (alpha) | [1...N] | FLT_1D (uncertain) | m | Array of wavelengths for radiance calibration |
spectrometer_visible.channel[:].geometry_matrix (alpha) | STRUCTURE | Description of geometry matrix (ray transfer matrix) | ||
spectrometer_visible.channel[:].geometry_matrix.emission_grid (alpha) | STRUCTURE | Grid defining the light emission cells | ||
spectrometer_visible.channel[:].geometry_matrix.emission_grid.dim1 (alpha) | [1...N] | FLT_1D (uncertain) | mixed | First dimension values |
spectrometer_visible.channel[:].geometry_matrix.emission_grid.dim2 (alpha) | [1...N] | FLT_1D (uncertain) | mixed | Second dimension values |
spectrometer_visible.channel[:].geometry_matrix.emission_grid.dim3 (alpha) | [1...N] | FLT_1D (uncertain) | mixed | Third dimension values |
spectrometer_visible.channel[:].geometry_matrix.emission_grid.grid_type (alpha) | STRUCTURE | Grid type | ||
spectrometer_visible.channel[:].geometry_matrix.emission_grid.grid_type.description (alpha) | STR_0D | Verbose description | ||
spectrometer_visible.channel[:].geometry_matrix.emission_grid.grid_type.index (alpha) | INT_0D | Integer identifier (enumeration index within a list). Private identifier values must be indicated by a negative index. | ||
spectrometer_visible.channel[:].geometry_matrix.emission_grid.grid_type.name (alpha) | STR_0D | Short string identifier | ||
spectrometer_visible.channel[:].geometry_matrix.interpolated (alpha) | STRUCTURE | Interpolated geometry matrix for reflected light | ||
spectrometer_visible.channel[:].geometry_matrix.interpolated.data (alpha) | [spectrometer_visible.channel[:].geometry_matrix.interpolated.r] | FLT_1D (uncertain) | m^-2 | Interpolated Ray Transfer Matrix (RTM, or geometry matrix), which provides transformation of the reflected light from each interpolation knot to the receiver (detector or head of an optic fibre). When convolving with an emission profile, the values must be interpolated to the emission grid and multiplied by the volume of the grid cells. The interpolated matrix is given on an array of interpolation knots of coordinates r, z and phi |
spectrometer_visible.channel[:].geometry_matrix.interpolated.phi (alpha) | [spectrometer_visible.channel[:].geometry_matrix.interpolated.r] | FLT_1D (uncertain) | rad | Toroidal angle (oriented counter-clockwise when viewing from above) of interpolation knots |
spectrometer_visible.channel[:].geometry_matrix.interpolated.r (alpha) | [1...N] | FLT_1D (uncertain) | m | Major radius of interpolation knots |
spectrometer_visible.channel[:].geometry_matrix.interpolated.z (alpha) | [spectrometer_visible.channel[:].geometry_matrix.interpolated.r] | FLT_1D (uncertain) | m | Height of interpolation knots |
spectrometer_visible.channel[:].geometry_matrix.voxel_map (alpha) | [spectrometer_visible.channel[:].geometry_matrix.emission_grid.dim1, | INT_3D | Voxel map for geometry matrix. The cells with same number are merged in the computation into a single emission source meta-cell (the voxel). Cells with number -1 are excluded. Voxel count starts from 0. | |
spectrometer_visible.channel[:].geometry_matrix.voxels_n (alpha) | INT_0D | Number of voxels defined in the voxel_map. | ||
spectrometer_visible.channel[:].geometry_matrix.with_reflections (alpha) | STRUCTURE | Geometry matrix with reflections | ||
spectrometer_visible.channel[:].geometry_matrix.with_reflections.data (alpha) | [1...N] | FLT_1D (uncertain) | m | The Ray Transfer Matrix (RTM, or geometry matrix) here provides transformation of the signal from each individual unit light source (voxel) to the receiver (detector or head of an optic fibre). The emission profile has [photons.m^-3.s^-1.sr^-1] units and radiance signal has [photons.m^-2.s^-1.sr^-1] units. So the RTM has [m] units. This data is stored in a sparse form, i.e. the array contains only the non-zero element of the Ray transfer matrix. The voxel index corresponding to an element of this array can be found in voxel_indices |
spectrometer_visible.channel[:].geometry_matrix.with_reflections.voxel_indices (alpha) | [spectrometer_visible.channel[:].geometry_matrix.with_reflections.data] | INT_1D | List of voxel indices (defined in the voxel map) used in the sparse data array | |
spectrometer_visible.channel[:].geometry_matrix.without_reflections (alpha) | STRUCTURE | Geometry matrix without reflections | ||
spectrometer_visible.channel[:].geometry_matrix.without_reflections.data (alpha) | [1...N] | FLT_1D (uncertain) | m | The Ray Transfer Matrix (RTM, or geometry matrix) here provides transformation of the signal from each individual unit light source (voxel) to the receiver (detector or head of an optic fibre). The emission profile has [photons.m^-3.s^-1.sr^-1] units and radiance signal has [photons.m^-2.s^-1.sr^-1] units. So the RTM has [m] units. This data is stored in a sparse form, i.e. the array contains only the non-zero element of the Ray transfer matrix. The voxel index corresponding to an element of this array can be found in voxel_indices |
spectrometer_visible.channel[:].geometry_matrix.without_reflections.voxel_indices (alpha) | [spectrometer_visible.channel[:].geometry_matrix.without_reflections.data] | INT_1D | List of voxel indices (defined in the voxel map) used in the sparse data array | |
spectrometer_visible.channel[:].grating_spectrometer (alpha) | STRUCTURE | Quantities measured by the channel if connected to a grating spectrometer | ||
spectrometer_visible.channel[:].grating_spectrometer.exposure_time (alpha) | FLT_0D (uncertain) | s | Exposure time | |
spectrometer_visible.channel[:].grating_spectrometer.grating (alpha) | FLT_0D (uncertain) | m^-1 | Number of grating lines per unit length | |
spectrometer_visible.channel[:].grating_spectrometer.instrument_function (alpha) | [1...2, | FLT_2D (uncertain) | m | Array of Gaussian widths and amplitudes which as a sum make up the instrument function. The instrument function is the shape that would be measured by a grating spectrometer if perfectly monochromatic line emission would be used as input. F(lambda) = 1 / sqrt (2*pi) * sum( instrument_function(1,i) / instrument_function(2,i) ) * exp( -lambda^2 / (2 * instrument_function(2,i)^2) ) ), whereby sum( instrument_function(1,i) ) = 1 |
spectrometer_visible.channel[:].grating_spectrometer.intensity_spectrum (alpha) | [spectrometer_visible.channel[:].grating_spectrometer.wavelengths, | STRUCTURE | (counts) s^-1 | Intensity spectrum (not calibrated), i.e. number of photoelectrons detected by unit time by a wavelength pixel of the channel, taking into account electronic gain compensation and channels relative calibration |
spectrometer_visible.channel[:].grating_spectrometer.intensity_spectrum.data (alpha) | [1...N, | FLT_2D (uncertain) | (counts) s^-1 | Data |
spectrometer_visible.channel[:].grating_spectrometer.intensity_spectrum.time (alpha) | [1...N] | FLT_1D_TYPE | s | Time |
spectrometer_visible.channel[:].grating_spectrometer.processed_line (alpha) | [1...N] | STRUCT_ARRAY | Set of processed spectral lines | |
spectrometer_visible.channel[:].grating_spectrometer.processed_line[:].intensity (alpha) | STRUCTURE | s^-1 | Non-calibrated intensity (integrated over the spectrum for this line) | |
spectrometer_visible.channel[:].grating_spectrometer.processed_line[:].intensity.data (alpha) | [spectrometer_visible.channel[:].grating_spectrometer.processed_line[:].intensity.time] | FLT_1D (uncertain) | s^-1 | Data |
spectrometer_visible.channel[:].grating_spectrometer.processed_line[:].intensity.time (alpha) | [1...N] | FLT_1D_TYPE | s | Time |
spectrometer_visible.channel[:].grating_spectrometer.processed_line[:].label (alpha) | STR_0D | String identifying the processed line. To avoid ambiguities, the following syntax is used : element with ionization state_wavelength in Angstrom (e.g. WI_4000) | ||
spectrometer_visible.channel[:].grating_spectrometer.processed_line[:].radiance (alpha) | STRUCTURE | m^-2.s^-1.sr^-1 | Calibrated, background subtracted radiance (integrated over the spectrum for this line) | |
spectrometer_visible.channel[:].grating_spectrometer.processed_line[:].radiance.data (alpha) | [spectrometer_visible.channel[:].grating_spectrometer.processed_line[:].radiance.time] | FLT_1D (uncertain) | m^-2.s^-1.sr^-1 | Data |
spectrometer_visible.channel[:].grating_spectrometer.processed_line[:].radiance.time (alpha) | [1...N] | FLT_1D_TYPE | s | Time |
spectrometer_visible.channel[:].grating_spectrometer.processed_line[:].wavelength_central (alpha) | FLT_0D (uncertain) | m | Central wavelength of the processed line | |
spectrometer_visible.channel[:].grating_spectrometer.radiance_calibration (alpha) | [spectrometer_visible.channel[:].grating_spectrometer.wavelengths] | FLT_1D (uncertain) | m^-3.sr^-1 | Radiance calibration |
spectrometer_visible.channel[:].grating_spectrometer.radiance_calibration_date (alpha) | STR_0D | Date of the radiance calibration (yyyy_mm_dd) | ||
spectrometer_visible.channel[:].grating_spectrometer.radiance_spectral (alpha) | [spectrometer_visible.channel[:].grating_spectrometer.wavelengths, | STRUCTURE | (photons).m^-2.s^-1.sr^-1.m^-1 | Calibrated spectral radiance (radiance per unit wavelength) |
spectrometer_visible.channel[:].grating_spectrometer.radiance_spectral.data (alpha) | [1...N, | FLT_2D (uncertain) | (photons).m^-2.s^-1.sr^-1.m^-1 | Data |
spectrometer_visible.channel[:].grating_spectrometer.radiance_spectral.time (alpha) | [1...N] | FLT_1D_TYPE | s | Time |
spectrometer_visible.channel[:].grating_spectrometer.slit_width (alpha) | FLT_0D (uncertain) | m | Width of the slit (placed in the object focal plane) | |
spectrometer_visible.channel[:].grating_spectrometer.wavelength_calibration (alpha) | STRUCTURE | Wavelength calibration data. The wavelength is obtained from the pixel index k by: wavelength = k * gain + offset. k is starting from 1. | ||
spectrometer_visible.channel[:].grating_spectrometer.wavelength_calibration.gain (alpha) | FLT_0D (uncertain) | m | Gain | |
spectrometer_visible.channel[:].grating_spectrometer.wavelength_calibration.offset (alpha) | FLT_0D (uncertain) | m | Offset | |
spectrometer_visible.channel[:].grating_spectrometer.wavelength_calibration_date (alpha) | STR_0D | Date of the wavelength calibration (yyyy_mm_dd) | ||
spectrometer_visible.channel[:].grating_spectrometer.wavelengths (alpha) | [1...N] | FLT_1D (uncertain) | m | Measured wavelengths |
spectrometer_visible.channel[:].isotope_ratios (alpha) | STRUCTURE | Isotope ratios and related information | ||
spectrometer_visible.channel[:].isotope_ratios.isotope (alpha) | [1...N] | STRUCT_ARRAY | Set of isotopes | |
spectrometer_visible.channel[:].isotope_ratios.isotope[:].cold_neutrals_fraction (alpha) | [spectrometer_visible.channel[:].isotope_ratios.isotope[:].time] | FLT_1D (uncertain) | - | Fraction of cold neutrals for this isotope (n_cold_neutrals/(n_cold_neutrals+n_hot_neutrals)) |
spectrometer_visible.channel[:].isotope_ratios.isotope[:].cold_neutrals_temperature (alpha) | [spectrometer_visible.channel[:].isotope_ratios.isotope[:].time] | FLT_1D (uncertain) | eV | Temperature of cold neutrals for this isotope |
spectrometer_visible.channel[:].isotope_ratios.isotope[:].density_ratio (alpha) | [spectrometer_visible.channel[:].isotope_ratios.isotope[:].time] | FLT_1D (uncertain) | - | Ratio of the density of neutrals of this isotope over the summed neutral densities of all other isotopes described in the ../isotope array |
spectrometer_visible.channel[:].isotope_ratios.isotope[:].element (alpha) | [1...N] | STRUCT_ARRAY | List of elements forming the atom or molecule | |
spectrometer_visible.channel[:].isotope_ratios.isotope[:].element[:].a (alpha) | FLT_0D (uncertain) | Atomic Mass Unit | Mass of atom | |
spectrometer_visible.channel[:].isotope_ratios.isotope[:].element[:].atoms_n (alpha) | INT_0D | Number of atoms of this element in the molecule | ||
spectrometer_visible.channel[:].isotope_ratios.isotope[:].element[:].multiplicity (obsolescent) | FLT_0D (uncertain) | Elementary Charge Unit | Multiplicity of the atom | |
spectrometer_visible.channel[:].isotope_ratios.isotope[:].element[:].z_n (alpha) | FLT_0D (uncertain) | Elementary Charge Unit | Nuclear charge | |
spectrometer_visible.channel[:].isotope_ratios.isotope[:].hot_neutrals_fraction (alpha) | [spectrometer_visible.channel[:].isotope_ratios.isotope[:].time] | FLT_1D (uncertain) | - | Fraction of hot neutrals for this isotope (n_hot_neutrals/(n_cold_neutrals+n_hot_neutrals)) |
spectrometer_visible.channel[:].isotope_ratios.isotope[:].hot_neutrals_temperature (alpha) | [spectrometer_visible.channel[:].isotope_ratios.isotope[:].time] | FLT_1D (uncertain) | eV | Temperature of hot neutrals for this isotope |
spectrometer_visible.channel[:].isotope_ratios.isotope[:].label (alpha) | STR_0D | String identifying the species (H, D, T, He3, He4) | ||
spectrometer_visible.channel[:].isotope_ratios.isotope[:].time (alpha) | [1...N] | FLT_1D_TYPE | s | Timebase for dynamic quantities at this level of the data structure |
spectrometer_visible.channel[:].isotope_ratios.method (alpha) | STRUCTURE | Fitting method used to calculate isotope ratios | ||
spectrometer_visible.channel[:].isotope_ratios.method.description (alpha) | STR_0D | Verbose description | ||
spectrometer_visible.channel[:].isotope_ratios.method.index (alpha) | INT_0D | Integer identifier (enumeration index within a list). Private identifier values must be indicated by a negative index. | ||
spectrometer_visible.channel[:].isotope_ratios.method.name (alpha) | STR_0D | Short string identifier | ||
spectrometer_visible.channel[:].isotope_ratios.signal_to_noise (alpha) | [spectrometer_visible.channel[:].isotope_ratios.time] | FLT_1D (uncertain) | dB | Log10 of the ratio of the powers in two bands, one with the spectral lines of interest (signal) the other without spectral lines (noise). |
spectrometer_visible.channel[:].isotope_ratios.time (alpha) | [1...N] | FLT_1D_TYPE | s | Timebase for dynamic quantities at this level of the data structure |
spectrometer_visible.channel[:].isotope_ratios.validity (alpha) | INT_0D | Indicator of the validity of the isotope ratios for the whole acquisition period (0 means valid, negative values mean non-valid) | ||
spectrometer_visible.channel[:].isotope_ratios.validity_timed (alpha) | [spectrometer_visible.channel[:].isotope_ratios.time] | INT_1D | Indicator of the validity of the isotope ratios as a function of time (0 means valid, negative values mean non-valid) | |
spectrometer_visible.channel[:].light_collection_efficiencies (alpha) | STRUCTURE | Light collection efficiencies (fraction of the local emission detected by the optical system) for a list of points defining regions of interest. To be used for non-pinhole optics. | ||
spectrometer_visible.channel[:].light_collection_efficiencies.positions (alpha) | STRUCTURE | List of positions for which the light collection efficiencies are provided | ||
spectrometer_visible.channel[:].light_collection_efficiencies.positions.phi (alpha) | [spectrometer_visible.channel[:].light_collection_efficiencies.positions.r] | FLT_1D (uncertain) | rad | Toroidal angle (oriented counter-clockwise when viewing from above) |
spectrometer_visible.channel[:].light_collection_efficiencies.positions.r (alpha) | [1...N] | FLT_1D (uncertain) | m | Major radius |
spectrometer_visible.channel[:].light_collection_efficiencies.positions.z (alpha) | [spectrometer_visible.channel[:].light_collection_efficiencies.positions.r] | FLT_1D (uncertain) | m | Height |
spectrometer_visible.channel[:].light_collection_efficiencies.values (alpha) | [spectrometer_visible.channel[:].light_collection_efficiencies.positions.r] | FLT_1D (uncertain) | - | Values of the light collection efficiencies |
spectrometer_visible.channel[:].line_of_sight (alpha) | STRUCTURE | Description of the line of sight of the channel, given by 2 points | ||
spectrometer_visible.channel[:].line_of_sight.first_point (alpha) | STRUCTURE | Position of the first point | ||
spectrometer_visible.channel[:].line_of_sight.first_point.phi (alpha) | FLT_0D (uncertain) | rad | Toroidal angle (oriented counter-clockwise when viewing from above) | |
spectrometer_visible.channel[:].line_of_sight.first_point.r (alpha) | FLT_0D (uncertain) | m | Major radius | |
spectrometer_visible.channel[:].line_of_sight.first_point.z (alpha) | FLT_0D (uncertain) | m | Height | |
spectrometer_visible.channel[:].line_of_sight.second_point (alpha) | STRUCTURE | Position of the second point | ||
spectrometer_visible.channel[:].line_of_sight.second_point.phi (alpha) | FLT_0D (uncertain) | rad | Toroidal angle (oriented counter-clockwise when viewing from above) | |
spectrometer_visible.channel[:].line_of_sight.second_point.r (alpha) | FLT_0D (uncertain) | m | Major radius | |
spectrometer_visible.channel[:].line_of_sight.second_point.z (alpha) | FLT_0D (uncertain) | m | Height | |
spectrometer_visible.channel[:].name (alpha) | STR_0D | Name of the channel | ||
spectrometer_visible.channel[:].object_observed (alpha) | STR_0D | Main object observed by the channel | ||
spectrometer_visible.channel[:].optical_element (alpha) | [1...N] | STRUCT_ARRAY | Set of optical elements | |
spectrometer_visible.channel[:].optical_element[:].back_surface (alpha) | STRUCTURE | Curvature of the front surface | ||
spectrometer_visible.channel[:].optical_element[:].back_surface.curvature_type (alpha) | STRUCTURE | Curvature of the surface | ||
spectrometer_visible.channel[:].optical_element[:].back_surface.curvature_type.description (alpha) | STR_0D | Verbose description | ||
spectrometer_visible.channel[:].optical_element[:].back_surface.curvature_type.index (alpha) | INT_0D | Integer identifier (enumeration index within a list). Private identifier values must be indicated by a negative index. | ||
spectrometer_visible.channel[:].optical_element[:].back_surface.curvature_type.name (alpha) | STR_0D | Short string identifier | ||
spectrometer_visible.channel[:].optical_element[:].back_surface.x1_curvature (alpha) | FLT_0D (uncertain) | m | Radius of curvature in the X1 direction, to be filled only for curvature_type/index = 2, 4 or 5 | |
spectrometer_visible.channel[:].optical_element[:].back_surface.x2_curvature (alpha) | FLT_0D (uncertain) | m | Radius of curvature in the X2 direction, to be filled only for curvature_type/index = 3 or 5 | |
spectrometer_visible.channel[:].optical_element[:].front_surface (alpha) | STRUCTURE | Curvature of the front surface | ||
spectrometer_visible.channel[:].optical_element[:].front_surface.curvature_type (alpha) | STRUCTURE | Curvature of the surface | ||
spectrometer_visible.channel[:].optical_element[:].front_surface.curvature_type.description (alpha) | STR_0D | Verbose description | ||
spectrometer_visible.channel[:].optical_element[:].front_surface.curvature_type.index (alpha) | INT_0D | Integer identifier (enumeration index within a list). Private identifier values must be indicated by a negative index. | ||
spectrometer_visible.channel[:].optical_element[:].front_surface.curvature_type.name (alpha) | STR_0D | Short string identifier | ||
spectrometer_visible.channel[:].optical_element[:].front_surface.x1_curvature (alpha) | FLT_0D (uncertain) | m | Radius of curvature in the X1 direction, to be filled only for curvature_type/index = 2, 4 or 5 | |
spectrometer_visible.channel[:].optical_element[:].front_surface.x2_curvature (alpha) | FLT_0D (uncertain) | m | Radius of curvature in the X2 direction, to be filled only for curvature_type/index = 3 or 5 | |
spectrometer_visible.channel[:].optical_element[:].geometry (alpha) | STRUCTURE | Further geometrical description of the element | ||
spectrometer_visible.channel[:].optical_element[:].geometry.centre (alpha) | STRUCTURE | If geometry_type=2, coordinates of the centre of the circle. If geometry_type=1 or 3, coordinates of the origin of the local coordinate system (X1,X2,X3) describing the plane detector/aperture. This origin is located within the detector/aperture area. | ||
spectrometer_visible.channel[:].optical_element[:].geometry.centre.phi (alpha) | FLT_0D (uncertain) | rad | Toroidal angle (oriented counter-clockwise when viewing from above) | |
spectrometer_visible.channel[:].optical_element[:].geometry.centre.r (alpha) | FLT_0D (uncertain) | m | Major radius | |
spectrometer_visible.channel[:].optical_element[:].geometry.centre.z (alpha) | FLT_0D (uncertain) | m | Height | |
spectrometer_visible.channel[:].optical_element[:].geometry.geometry_type (alpha) | INT_0D | Type of geometry used to describe the surface of the detector or aperture (1:'outline', 2:'circular', 3:'rectangle'). In case of 'outline', the surface is described by an outline of point in a local coordinate system defined by a centre and three unit vectors X1, X2, X3. Note that there is some flexibility here and the data provider should choose the most convenient coordinate system for the object, respecting the definitions of (X1,X2,X3) indicated below. In case of 'circular', the surface is a circle defined by its centre, radius, and normal vector oriented towards the plasma X3. In case of 'rectangle', the surface is a rectangle defined by its centre, widths in the X1 and X2 directions, and normal vector oriented towards the plasma X3. | ||
spectrometer_visible.channel[:].optical_element[:].geometry.outline (alpha) | STRUCTURE | Irregular outline of the detector/aperture in the (X1, X2) coordinate system. Do NOT repeat the first point. | ||
spectrometer_visible.channel[:].optical_element[:].geometry.outline.x1 (alpha) | [1...N] | FLT_1D (uncertain) | m | Positions along x1 axis |
spectrometer_visible.channel[:].optical_element[:].geometry.outline.x2 (alpha) | [spectrometer_visible.channel[:].optical_element[:].geometry.outline.x1] | FLT_1D (uncertain) | m | Positions along x2 axis |
spectrometer_visible.channel[:].optical_element[:].geometry.radius (alpha) | FLT_0D (uncertain) | m | Radius of the circle, used only if geometry_type = 2 | |
spectrometer_visible.channel[:].optical_element[:].geometry.surface (alpha) | FLT_0D (uncertain) | m^2 | Surface of the detector/aperture, derived from the above geometric data | |
spectrometer_visible.channel[:].optical_element[:].geometry.x1_unit_vector (alpha) | STRUCTURE | Components of the X1 direction unit vector in the (X,Y,Z) coordinate system, where X is the major radius axis for phi = 0, Y is the major radius axis for phi = pi/2, and Z is the height axis. The X1 vector is more horizontal than X2 (has a smaller abs(Z) component) and oriented in the positive phi direction (counter-clockwise when viewing from above). | ||
spectrometer_visible.channel[:].optical_element[:].geometry.x1_unit_vector.x (alpha) | FLT_0D (uncertain) | m | Component along X axis | |
spectrometer_visible.channel[:].optical_element[:].geometry.x1_unit_vector.y (alpha) | FLT_0D (uncertain) | m | Component along Y axis | |
spectrometer_visible.channel[:].optical_element[:].geometry.x1_unit_vector.z (alpha) | FLT_0D (uncertain) | m | Component along Z axis | |
spectrometer_visible.channel[:].optical_element[:].geometry.x1_width (alpha) | FLT_0D (uncertain) | m | Full width of the aperture in the X1 direction, used only if geometry_type = 3 | |
spectrometer_visible.channel[:].optical_element[:].geometry.x2_unit_vector (alpha) | STRUCTURE | Components of the X2 direction unit vector in the (X,Y,Z) coordinate system, where X is the major radius axis for phi = 0, Y is the major radius axis for phi = pi/2, and Z is the height axis. The X2 axis is orthonormal so that uX2 = uX3 x uX1. | ||
spectrometer_visible.channel[:].optical_element[:].geometry.x2_unit_vector.x (alpha) | FLT_0D (uncertain) | m | Component along X axis | |
spectrometer_visible.channel[:].optical_element[:].geometry.x2_unit_vector.y (alpha) | FLT_0D (uncertain) | m | Component along Y axis | |
spectrometer_visible.channel[:].optical_element[:].geometry.x2_unit_vector.z (alpha) | FLT_0D (uncertain) | m | Component along Z axis | |
spectrometer_visible.channel[:].optical_element[:].geometry.x2_width (alpha) | FLT_0D (uncertain) | m | Full width of the aperture in the X2 direction, used only if geometry_type = 3 | |
spectrometer_visible.channel[:].optical_element[:].geometry.x3_unit_vector (alpha) | STRUCTURE | Components of the X3 direction unit vector in the (X,Y,Z) coordinate system, where X is the major radius axis for phi = 0, Y is the major radius axis for phi = pi/2, and Z is the height axis. The X3 axis is normal to the detector/aperture plane and oriented towards the plasma. | ||
spectrometer_visible.channel[:].optical_element[:].geometry.x3_unit_vector.x (alpha) | FLT_0D (uncertain) | m | Component along X axis | |
spectrometer_visible.channel[:].optical_element[:].geometry.x3_unit_vector.y (alpha) | FLT_0D (uncertain) | m | Component along Y axis | |
spectrometer_visible.channel[:].optical_element[:].geometry.x3_unit_vector.z (alpha) | FLT_0D (uncertain) | m | Component along Z axis | |
spectrometer_visible.channel[:].optical_element[:].material_properties (alpha) | STRUCTURE | Material properties of the optical element | ||
spectrometer_visible.channel[:].optical_element[:].material_properties.extinction_coefficient (alpha) | [spectrometer_visible.channel[:].optical_element[:].material_properties.wavelengths] | FLT_1D (uncertain) | - | Extinction coefficient (for metal) |
spectrometer_visible.channel[:].optical_element[:].material_properties.refractive_index (alpha) | [spectrometer_visible.channel[:].optical_element[:].material_properties.wavelengths] | FLT_1D (uncertain) | - | Refractive index (for metal and dielectric) |
spectrometer_visible.channel[:].optical_element[:].material_properties.roughness (alpha) | [spectrometer_visible.channel[:].optical_element[:].material_properties.wavelengths] | FLT_1D (uncertain) | - | Roughness parameter of the material. Varies in range [0, 1]. 0 is perfectly specular, 1 is perfectly rough |
spectrometer_visible.channel[:].optical_element[:].material_properties.transmission_coefficient (alpha) | [spectrometer_visible.channel[:].optical_element[:].material_properties.wavelengths] | FLT_1D (uncertain) | - | Transmission coefficient (for dielectric) |
spectrometer_visible.channel[:].optical_element[:].material_properties.type (alpha) | STRUCTURE | Type of optical element material. In case of 'metal' refractive_index and extinction_coefficient are used. In case of 'dielectric' refractive_index and transmission_coefficient are used. | ||
spectrometer_visible.channel[:].optical_element[:].material_properties.type.description (alpha) | STR_0D | Verbose description | ||
spectrometer_visible.channel[:].optical_element[:].material_properties.type.index (alpha) | INT_0D | Integer identifier (enumeration index within a list). Private identifier values must be indicated by a negative index. | ||
spectrometer_visible.channel[:].optical_element[:].material_properties.type.name (alpha) | STR_0D | Short string identifier | ||
spectrometer_visible.channel[:].optical_element[:].material_properties.wavelengths (alpha) | [1...N] | FLT_1D (uncertain) | m | Wavelengths array for refractive_index, extinction_coefficient and transmission_coefficient |
spectrometer_visible.channel[:].optical_element[:].thickness (alpha) | FLT_0D (uncertain) | m | Distance between front_surface and back_surface along the X3 vector | |
spectrometer_visible.channel[:].optical_element[:].type (alpha) | STRUCTURE | Type of optical element. In case of 'mirror' and 'diaphragm', the element is described by one 'front_surface'. In case of 'lens', the element is described by 'front_surface' and 'back_surface'. | ||
spectrometer_visible.channel[:].optical_element[:].type.description (alpha) | STR_0D | Verbose description | ||
spectrometer_visible.channel[:].optical_element[:].type.index (alpha) | INT_0D | Integer identifier (enumeration index within a list). Private identifier values must be indicated by a negative index. | ||
spectrometer_visible.channel[:].optical_element[:].type.name (alpha) | STR_0D | Short string identifier | ||
spectrometer_visible.channel[:].polarization_spectroscopy (alpha) | STRUCTURE | Physics quantities measured from polarized light spectroscopy | ||
spectrometer_visible.channel[:].polarization_spectroscopy.b_field_modulus (alpha) | [spectrometer_visible.channel[:].polarization_spectroscopy.time] | FLT_1D (uncertain) | T | Modulus of the magnetic field (always positive, irrespective of the sign convention for the B-field direction), obtained from Zeeman effect fit |
spectrometer_visible.channel[:].polarization_spectroscopy.e_field_lh_r (alpha) | [spectrometer_visible.channel[:].polarization_spectroscopy.time] | FLT_1D (uncertain) | V.m^-1 | Lower Hybrid electric field component in the major radius direction |
spectrometer_visible.channel[:].polarization_spectroscopy.e_field_lh_tor (alpha) | [spectrometer_visible.channel[:].polarization_spectroscopy.time] | FLT_1D (uncertain) | V.m^-1 | Lower Hybrid electric field component in the toroidal direction |
spectrometer_visible.channel[:].polarization_spectroscopy.e_field_lh_z (alpha) | [spectrometer_visible.channel[:].polarization_spectroscopy.time] | FLT_1D (uncertain) | V.m^-1 | Lower Hybrid electric field component in the vertical direction |
spectrometer_visible.channel[:].polarization_spectroscopy.n_e (alpha) | [spectrometer_visible.channel[:].polarization_spectroscopy.time] | FLT_1D (uncertain) | m^-3 | Electron density, obtained from Stark broadening fit |
spectrometer_visible.channel[:].polarization_spectroscopy.temperature_cold_neutrals (alpha) | [spectrometer_visible.channel[:].polarization_spectroscopy.time] | FLT_1D (uncertain) | eV | Fit of cold neutrals temperature |
spectrometer_visible.channel[:].polarization_spectroscopy.temperature_hot_neutrals (alpha) | [spectrometer_visible.channel[:].polarization_spectroscopy.time] | FLT_1D (uncertain) | eV | Fit of hot neutrals temperature |
spectrometer_visible.channel[:].polarization_spectroscopy.time (alpha) | [1...N] | FLT_1D_TYPE | s | Timebase for dynamic quantities at this level of the data structure |
spectrometer_visible.channel[:].polarization_spectroscopy.velocity_cold_neutrals (alpha) | [spectrometer_visible.channel[:].polarization_spectroscopy.time] | FLT_1D (uncertain) | m.s^-1 | Projection of the cold neutral velocity along the line of sight, positive when going from first point to second point of the line of sight |
spectrometer_visible.channel[:].polarization_spectroscopy.velocity_hot_neutrals (alpha) | [spectrometer_visible.channel[:].polarization_spectroscopy.time] | FLT_1D (uncertain) | m.s^-1 | Projection of the hot neutral velocity along the line of sight, positive when going from first point to second point of the line of sight |
spectrometer_visible.channel[:].polarizer (alpha) | STRUCTURE | Polarizer description | ||
spectrometer_visible.channel[:].polarizer.centre (alpha) | STRUCTURE | If geometry_type=2, coordinates of the centre of the circle. If geometry_type=1 or 3, coordinates of the origin of the local coordinate system (X1,X2,X3) describing the plane detector/aperture. This origin is located within the detector/aperture area. | ||
spectrometer_visible.channel[:].polarizer.centre.phi (alpha) | FLT_0D (uncertain) | rad | Toroidal angle (oriented counter-clockwise when viewing from above) | |
spectrometer_visible.channel[:].polarizer.centre.r (alpha) | FLT_0D (uncertain) | m | Major radius | |
spectrometer_visible.channel[:].polarizer.centre.z (alpha) | FLT_0D (uncertain) | m | Height | |
spectrometer_visible.channel[:].polarizer.geometry_type (alpha) | INT_0D | Type of geometry used to describe the surface of the detector or aperture (1:'outline', 2:'circular', 3:'rectangle'). In case of 'outline', the surface is described by an outline of point in a local coordinate system defined by a centre and three unit vectors X1, X2, X3. Note that there is some flexibility here and the data provider should choose the most convenient coordinate system for the object, respecting the definitions of (X1,X2,X3) indicated below. In case of 'circular', the surface is a circle defined by its centre, radius, and normal vector oriented towards the plasma X3. In case of 'rectangle', the surface is a rectangle defined by its centre, widths in the X1 and X2 directions, and normal vector oriented towards the plasma X3. | ||
spectrometer_visible.channel[:].polarizer.outline (alpha) | STRUCTURE | Irregular outline of the detector/aperture in the (X1, X2) coordinate system. Do NOT repeat the first point. | ||
spectrometer_visible.channel[:].polarizer.outline.x1 (alpha) | [1...N] | FLT_1D (uncertain) | m | Positions along x1 axis |
spectrometer_visible.channel[:].polarizer.outline.x2 (alpha) | [spectrometer_visible.channel[:].polarizer.outline.x1] | FLT_1D (uncertain) | m | Positions along x2 axis |
spectrometer_visible.channel[:].polarizer.radius (alpha) | FLT_0D (uncertain) | m | Radius of the circle, used only if geometry_type = 2 | |
spectrometer_visible.channel[:].polarizer.surface (alpha) | FLT_0D (uncertain) | m^2 | Surface of the detector/aperture, derived from the above geometric data | |
spectrometer_visible.channel[:].polarizer.x1_unit_vector (alpha) | STRUCTURE | Components of the X1 direction unit vector in the (X,Y,Z) coordinate system, where X is the major radius axis for phi = 0, Y is the major radius axis for phi = pi/2, and Z is the height axis. The X1 vector is more horizontal than X2 (has a smaller abs(Z) component) and oriented in the positive phi direction (counter-clockwise when viewing from above). | ||
spectrometer_visible.channel[:].polarizer.x1_unit_vector.x (alpha) | FLT_0D (uncertain) | m | Component along X axis | |
spectrometer_visible.channel[:].polarizer.x1_unit_vector.y (alpha) | FLT_0D (uncertain) | m | Component along Y axis | |
spectrometer_visible.channel[:].polarizer.x1_unit_vector.z (alpha) | FLT_0D (uncertain) | m | Component along Z axis | |
spectrometer_visible.channel[:].polarizer.x1_width (alpha) | FLT_0D (uncertain) | m | Full width of the aperture in the X1 direction, used only if geometry_type = 3 | |
spectrometer_visible.channel[:].polarizer.x2_unit_vector (alpha) | STRUCTURE | Components of the X2 direction unit vector in the (X,Y,Z) coordinate system, where X is the major radius axis for phi = 0, Y is the major radius axis for phi = pi/2, and Z is the height axis. The X2 axis is orthonormal so that uX2 = uX3 x uX1. | ||
spectrometer_visible.channel[:].polarizer.x2_unit_vector.x (alpha) | FLT_0D (uncertain) | m | Component along X axis | |
spectrometer_visible.channel[:].polarizer.x2_unit_vector.y (alpha) | FLT_0D (uncertain) | m | Component along Y axis | |
spectrometer_visible.channel[:].polarizer.x2_unit_vector.z (alpha) | FLT_0D (uncertain) | m | Component along Z axis | |
spectrometer_visible.channel[:].polarizer.x2_width (alpha) | FLT_0D (uncertain) | m | Full width of the aperture in the X2 direction, used only if geometry_type = 3 | |
spectrometer_visible.channel[:].polarizer.x3_unit_vector (alpha) | STRUCTURE | Components of the X3 direction unit vector in the (X,Y,Z) coordinate system, where X is the major radius axis for phi = 0, Y is the major radius axis for phi = pi/2, and Z is the height axis. The X3 axis is normal to the detector/aperture plane and oriented towards the plasma. | ||
spectrometer_visible.channel[:].polarizer.x3_unit_vector.x (alpha) | FLT_0D (uncertain) | m | Component along X axis | |
spectrometer_visible.channel[:].polarizer.x3_unit_vector.y (alpha) | FLT_0D (uncertain) | m | Component along Y axis | |
spectrometer_visible.channel[:].polarizer.x3_unit_vector.z (alpha) | FLT_0D (uncertain) | m | Component along Z axis | |
spectrometer_visible.channel[:].polarizer_active (alpha) | INT_0D | Indicator of whether a polarizer is present and active in the optical system (set to 1 in this case, set to 0 or leave empty ottherwise) | ||
spectrometer_visible.channel[:].type (alpha) | STRUCTURE | Type of spectrometer the channel is connected to (index=1: grating, 2: filter) | ||
spectrometer_visible.channel[:].type.description (alpha) | STR_0D | Verbose description | ||
spectrometer_visible.channel[:].type.index (alpha) | INT_0D | Integer identifier (enumeration index within a list). Private identifier values must be indicated by a negative index. | ||
spectrometer_visible.channel[:].type.name (alpha) | STR_0D | Short string identifier | ||
spectrometer_visible.channel[:].validity (alpha) | INT_0D | Indicator of the validity of the channel for the whole acquisition period (0 means valid, negative values mean non-valid) | ||
spectrometer_visible.channel[:].validity_timed (alpha) | STRUCTURE | Indicator of the validity of the channel as a function of time (0 means valid, negative values mean non-valid) | ||
spectrometer_visible.channel[:].validity_timed.data (alpha) | [spectrometer_visible.channel[:].validity_timed.time] | INT_1D | Data | |
spectrometer_visible.channel[:].validity_timed.time (alpha) | [1...N] | FLT_1D_TYPE | s | Time |
spectrometer_visible.code (alpha) | STRUCTURE | Generic decription of the code-specific parameters for the code that has produced this IDS | ||
spectrometer_visible.code.commit (alpha) | STR_0D | Unique commit reference of software | ||
spectrometer_visible.code.description (alpha) | STR_0D | Short description of the software (type, purpose) | ||
spectrometer_visible.code.library (alpha) | [1...N] | STRUCT_ARRAY | List of external libraries used by the code that has produced this IDS | |
spectrometer_visible.code.library[:].commit (alpha) | STR_0D | Unique commit reference of software | ||
spectrometer_visible.code.library[:].description (alpha) | STR_0D | Short description of the software (type, purpose) | ||
spectrometer_visible.code.library[:].name (alpha) | STR_0D | Name of software | ||
spectrometer_visible.code.library[:].parameters (alpha) | STR_0D | List of the code specific parameters in XML format | ||
spectrometer_visible.code.library[:].repository (alpha) | STR_0D | URL of software repository | ||
spectrometer_visible.code.library[:].version (alpha) | STR_0D | Unique version (tag) of software | ||
spectrometer_visible.code.name (alpha) | STR_0D | Name of software generating IDS | ||
spectrometer_visible.code.output_flag (alpha) | [spectrometer_visible.time] | INT_1D | Output flag : 0 means the run is successful, other values mean some difficulty has been encountered, the exact meaning is then code specific. Negative values mean the result shall not be used. | |
spectrometer_visible.code.parameters (alpha) | STR_0D | List of the code specific parameters in XML format | ||
spectrometer_visible.code.repository (alpha) | STR_0D | URL of software repository | ||
spectrometer_visible.code.version (alpha) | STR_0D | Unique version (tag) of software | ||
spectrometer_visible.detector_layout (alpha) | STR_0D | Layout of the detector grid employed. Ex: '4x16', '4x32', '1x18' | ||
spectrometer_visible.ids_properties (alpha) | STRUCTURE | Interface Data Structure properties. This element identifies the node above as an IDS | ||
spectrometer_visible.ids_properties.comment (alpha) | STR_0D | Any comment describing the content of this IDS | ||
spectrometer_visible.ids_properties.creation_date (alpha) | STR_0D | Date at which this data has been produced | ||
spectrometer_visible.ids_properties.homogeneous_time (alpha) | INT_0D | This node must be filled (with 0, 1, or 2) for the IDS to be valid. If 1, the time of this IDS is homogeneous, i.e. the time values for this IDS are stored in the time node just below the root of this IDS. If 0, the time values are stored in the various time fields at lower levels in the tree. In the case only constant or static nodes are filled within the IDS, homogeneous_time must be set to 2 | ||
spectrometer_visible.ids_properties.name (alpha) | STR_0D | User-defined name for this IDS occurrence | ||
spectrometer_visible.ids_properties.occurrence | INT_0D | |||
spectrometer_visible.ids_properties.occurrence_type (alpha) | STRUCTURE | Type of data contained in this occurrence | ||
spectrometer_visible.ids_properties.occurrence_type.description (alpha) | STR_0D | Verbose description | ||
spectrometer_visible.ids_properties.occurrence_type.index (alpha) | INT_0D | Integer identifier (enumeration index within a list). Private identifier values must be indicated by a negative index. | ||
spectrometer_visible.ids_properties.occurrence_type.name (alpha) | STR_0D | Short string identifier | ||
spectrometer_visible.ids_properties.plugins (alpha) | STRUCTURE | Information about the plugins used to write/read this IDS. This structure is filled automatically by the Access Layer at GET/PUT time, no need to fill it via a user program. | ||
spectrometer_visible.ids_properties.plugins.infrastructure_get (alpha) | STRUCTURE | Plugin infrastructure used to GET the data | ||
spectrometer_visible.ids_properties.plugins.infrastructure_get.commit (alpha) | STR_0D | Unique commit reference of software | ||
spectrometer_visible.ids_properties.plugins.infrastructure_get.description (alpha) | STR_0D | Short description of the software (type, purpose) | ||
spectrometer_visible.ids_properties.plugins.infrastructure_get.name (alpha) | STR_0D | Name of software used | ||
spectrometer_visible.ids_properties.plugins.infrastructure_get.repository (alpha) | STR_0D | URL of software repository | ||
spectrometer_visible.ids_properties.plugins.infrastructure_get.version (alpha) | STR_0D | Unique version (tag) of software | ||
spectrometer_visible.ids_properties.plugins.infrastructure_put (alpha) | STRUCTURE | Plugin infrastructure used to PUT the data | ||
spectrometer_visible.ids_properties.plugins.infrastructure_put.commit (alpha) | STR_0D | Unique commit reference of software | ||
spectrometer_visible.ids_properties.plugins.infrastructure_put.description (alpha) | STR_0D | Short description of the software (type, purpose) | ||
spectrometer_visible.ids_properties.plugins.infrastructure_put.name (alpha) | STR_0D | Name of software used | ||
spectrometer_visible.ids_properties.plugins.infrastructure_put.repository (alpha) | STR_0D | URL of software repository | ||
spectrometer_visible.ids_properties.plugins.infrastructure_put.version (alpha) | STR_0D | Unique version (tag) of software | ||
spectrometer_visible.ids_properties.plugins.node (alpha) | [1...N] | STRUCT_ARRAY | Set of IDS nodes for which a plugin has been applied | |
spectrometer_visible.ids_properties.plugins.node[:].get_operation (alpha) | [1...N] | STRUCT_ARRAY | Plugins actually used to read back a node (potentially, multiple plugins can be applied, listed in reverse order of application). This information is filled by the plugin infrastructure during the GET operation. | |
spectrometer_visible.ids_properties.plugins.node[:].get_operation[:].commit (alpha) | STR_0D | Unique commit reference of software | ||
spectrometer_visible.ids_properties.plugins.node[:].get_operation[:].description (alpha) | STR_0D | Short description of the software (type, purpose) | ||
spectrometer_visible.ids_properties.plugins.node[:].get_operation[:].name (alpha) | STR_0D | Name of software used | ||
spectrometer_visible.ids_properties.plugins.node[:].get_operation[:].parameters (alpha) | STR_0D | List of the code specific parameters in XML format | ||
spectrometer_visible.ids_properties.plugins.node[:].get_operation[:].repository (alpha) | STR_0D | URL of software repository | ||
spectrometer_visible.ids_properties.plugins.node[:].get_operation[:].version (alpha) | STR_0D | Unique version (tag) of software | ||
spectrometer_visible.ids_properties.plugins.node[:].path (alpha) | STR_0D | Path of the node within the IDS, following the syntax given in the link below. If empty, means the plugin applies to the whole IDS. | ||
spectrometer_visible.ids_properties.plugins.node[:].put_operation (alpha) | [1...N] | STRUCT_ARRAY | Plugins used to PUT a node (potentially, multiple plugins can be applied, if so they are listed by order of application) | |
spectrometer_visible.ids_properties.plugins.node[:].put_operation[:].commit (alpha) | STR_0D | Unique commit reference of software | ||
spectrometer_visible.ids_properties.plugins.node[:].put_operation[:].description (alpha) | STR_0D | Short description of the software (type, purpose) | ||
spectrometer_visible.ids_properties.plugins.node[:].put_operation[:].name (alpha) | STR_0D | Name of software used | ||
spectrometer_visible.ids_properties.plugins.node[:].put_operation[:].parameters (alpha) | STR_0D | List of the code specific parameters in XML format | ||
spectrometer_visible.ids_properties.plugins.node[:].put_operation[:].repository (alpha) | STR_0D | URL of software repository | ||
spectrometer_visible.ids_properties.plugins.node[:].put_operation[:].version (alpha) | STR_0D | Unique version (tag) of software | ||
spectrometer_visible.ids_properties.plugins.node[:].readback (alpha) | [1...N] | STRUCT_ARRAY | Plugins to be used to read back a node (potentially, multiple plugins can be applied, listed in reverse order of application) | |
spectrometer_visible.ids_properties.plugins.node[:].readback[:].commit (alpha) | STR_0D | Unique commit reference of software | ||
spectrometer_visible.ids_properties.plugins.node[:].readback[:].description (alpha) | STR_0D | Short description of the software (type, purpose) | ||
spectrometer_visible.ids_properties.plugins.node[:].readback[:].name (alpha) | STR_0D | Name of software used | ||
spectrometer_visible.ids_properties.plugins.node[:].readback[:].parameters (alpha) | STR_0D | List of the code specific parameters in XML format | ||
spectrometer_visible.ids_properties.plugins.node[:].readback[:].repository (alpha) | STR_0D | URL of software repository | ||
spectrometer_visible.ids_properties.plugins.node[:].readback[:].version (alpha) | STR_0D | Unique version (tag) of software | ||
spectrometer_visible.ids_properties.provenance (alpha) | STRUCTURE | Provenance information about this IDS | ||
spectrometer_visible.ids_properties.provenance.node (alpha) | [1...N] | STRUCT_ARRAY | Set of IDS nodes for which the provenance is given. The provenance information applies to the whole structure below the IDS node. For documenting provenance information for the whole IDS, set the size of this array of structure to 1 and leave the child "path" node empty | |
spectrometer_visible.ids_properties.provenance.node[:].path (alpha) | STR_0D | Path of the node within the IDS, following the syntax given in the link below. If empty, means the provenance information applies to the whole IDS. | ||
spectrometer_visible.ids_properties.provenance.node[:].sources (alpha) | [1...N] | STR_1D | List of sources used to import or calculate this node, identified as explained below. In case the node is the result of of a calculation / data processing, the source is an input to the process described in the "code" structure at the root of the IDS. The source can be an IDS (identified by a URI or a persitent identifier, see syntax in the link below) or non-IDS data imported directly from an non-IMAS database (identified by the command used to import the source, or the persistent identifier of the data source). Often data are obtained by a chain of processes, however only the last process input are recorded here. The full chain of provenance has then to be reconstructed recursively from the provenance information contained in the data sources. | |
spectrometer_visible.ids_properties.provider (alpha) | STR_0D | Name of the person in charge of producing this data | ||
spectrometer_visible.ids_properties.source (obsolescent) | STR_0D | Source of the data (any comment describing the origin of the data : code, path to diagnostic signals, processing method, ...). Superseeded by the new provenance structure. | ||
spectrometer_visible.ids_properties.version_put (alpha) | STRUCTURE | Version of the access layer package used to PUT this IDS | ||
spectrometer_visible.ids_properties.version_put.access_layer (alpha) | STR_0D | Version of Access Layer used to PUT this IDS | ||
spectrometer_visible.ids_properties.version_put.access_layer_language (alpha) | STR_0D | Programming language of the Access Layer high level API used to PUT this IDS | ||
spectrometer_visible.ids_properties.version_put.data_dictionary (alpha) | STR_0D | Version of Data Dictionary used to PUT this IDS | ||
spectrometer_visible.latency (alpha) | FLT_0D (uncertain) | s | Upper bound of the delay between physical information received by the detector and data available on the real-time (RT) network. | |
spectrometer_visible.time (alpha) | [1...N] | FLT_1D_TYPE | s | Generic time |