This is a printer friendly version of the RAMI website.
Original address of this page: https://rami-benchmark.jrc.ec.europa.eu/HTML/RAMI-IV/EXPERIMENTS4/ACTUAL_CANOPIES/SHORT_ROTATION_FOREST/SHORT_ROTATION_FOREST.php
Copyright © 2016 European Commission.
This page provides descriptions of the architectural, spectral and illumination related properties of a short rotation forest of poplar clones located in the Parco Ticino of northern Italy. The scene is based on data provided courtesy of Roberto Colombo, Michele Meroni, Lorenzo Busetto and colleagues (Remote Sensing of Environmental Dynamics Lab., DISAT, University of Milan-Bicocca, Milan, Italy) who, - carried out a detailed measurement campaign at this site in the frame of the EC Joint Research Centre's Kyoto experiment in 2004. Linda Hunt, from Science Systems and Applications Inc (USA), generated an L-system based model of the 1 year old poplar clones suitable for ingestion into 3D canopy RT models. Thus, potential RAMI participants are to treat the information presented on this page as actual 'inventory data', that is, they should identify/extract those parameters and characteristics that are required as input to their canopy reflectance models. In some cases this may mean that simplifications have to be made to the available information, or, that parts of the available information can not be exploited with a given radiative transfer model. Whatever the case may be, all potential RAMI participants should mimic the standard practices that they use when matching actual field measurements to the required set(s) of input parameters of their model(s). If this means that you need more information than provided, please do not hesitate in contacting us. Last but not least, for those 3D models capable of maintaining architectural fidelity down to the individual shoot and branch level a series of ASCII (text) files containing the Cartesian coordinates of various geometric primitives (triangles, spheres and cylinders) and their transformations will be given. This should facilitate the reconstruction of the short rotation forest architecture as it is described on this page.
![]() ![]() ![]() |
In order to facilitate the generation of the poplar short rotation forest the information on this page has been subdivided into four different categories. For each one of these categories the relevant descriptions will be contained within a uniquely coloured text frame and can be accessed by clicking on one of the four links below:
|
|
|
|
In case of difficulties or missing data on this page please do not hesitate in contacting us so that the problems may be resolved as fast as possible.
1) General canopy characteristicsThe Poplar short rotation forest scene is generated over an area of approximately 100×100 m² . The center of the coordinate system lies almost in the middle of the scene. The trees are planted in double rows. The distance from the center of one double row to the center of the next double row is about 3.55 m. Each tree row is about 0.375 m from the center of that double row. Within a given row, neighbouring trees are separated from each other by a distance of about 0.45 m. However, 2% of the potential tree positions are void due to missing trees. Overall, the architectural characteristics of the scene are thus as follows:
2) Foliage structureThe table below provides the structural characteristics of the leaves that feature within the poplar Short Rotation Forest. Indicated are average properties since the leaves within a single tree vary somewhat in their size and shape.
3) Tree structureThe poplar Short Rotation Forest is generated on the basis of 6 individual tree representations of the Populus Nigra species. The table below provides an overview of some structural characteristics of these 6 tree representations. For those RT models capable of representing the 3D architecture of a given trees through a series of geometric primitives, the last three lines of each table contain links to data files with detailed specifications of the foliage and wood structural properties of the poplar Short Rotation Forest trees.
4) Stand structureThe poplar Short Rotation Forest is composed of 11924 individual trees. The following table indicates how these trees are distributed among the above tree classes and specifies the respective x,y locations of the tree centers of each tree class in the scene. The last row contains an ASCII file with tree translation and rotation information for those RT models capable of ingesting the detailed 3D architecture of the tree models specified in the previous section.
![]() Tree locations for the poplar Short Rotation Forest. The origin of the coordinate system is in the center of the image. |
Each one of the ten trees in the poplar Short Rotation Forest scene features distinct foliage spectral properties. All of the foliage, wood and background components in the poplar Short Rotation Forest scene feature LAMBERTIAN scattering properties. The tables below contains various spectral characteristics for nineteen different spectral bands. The experimental identifier for the poplar Short Rotation Forest scene is given by HET16_SRF_$$$_B**_## where $$$ relates to the solar azimuth angle, B** relates to the spectral bands (B01, B02, …, B19) and ## relates to the solar zenith angle. A text file that resumes all of the information in this table can be found here.
|
Five different illumination conditions are to be simulated for the poplar Short Rotation Forest. More specifically the solar zenith angle (SZA) is 0, 20 or 50 degrees and the solar azimuth angle is equal to 0 or 90 degree. Only direct solar radiation is to be considered in these experiments. The experimental identifier <EXP> that is needed in the naming of the various measurement results files (see file naming and formatting conventions) for the poplar Short Rotation Forest scene is given by HET16_SRF_$$$_B**_## where $$$ relates to the solar azimuth angle, B** relates to the spectral bands (B01, B02, …, B19) and ## relates to the solar zenith angle. The following image shows the experimental identifiers of the various experiments (right hand side) together with the correct solar azimuth (yellow) and zenith (white) angle overlaid onto the orchard geometry (left hand side). ![]() |
Prior to the performing of any RT model simulations, please refer to the 'definitions' pages for detailed instructions regarding the angular sign conventions for BRF simulations, as well as other RT model technicalities. Also read the relevant file naming and formatting conventions that must be adhered to by all participants. In addition, RAMI-IV offers participants the possibility to test the compliance of their model-generated results files with these file-naming and formatting convention, prior to their submission via ftp: To do so follow the on-line format checker link that appears in the top navigation bar during the active submission period.