Three indoor phenotyping experiments were completed to study Arabidopsis thalianagrowth using advanced imaging systems. The first to use a high-resolution RGB camera to capture top-view images under controlled lighting and temperature. Automated cropping techniques ensured precise data preparation and organisation. The third experiment employed multiple stereo cameras for comprehensive plant monitoring. Data underwent preprocessing to enhance quality, including colour correction and noise reduction. These structured datasets support research in plant segmentation, stress detection, and growth modelling.
Two large-scale phenotyping experiments were conducted at La Trobe University at AgriBio, the Centre for AgriBioscience, during 2022. The experiments took place in a controlled growth chamber equipped with a movable X-Y (horizontal-vertical) high-throughput plant phenotyping (HTPP) platform designed by Photon System Instruments (PSI). The indoor HTPP system features a high-resolution digital RGB camera capable of moving along a gantry, performing top-view RGB screening of plants placed on an adjustable height table, as displayed in video 1. Illumination consisted of three LED light sources, including far red, red, and cold white, ranging from 400 to 750 nm. Prior to both experiments, the light intensity was measured and varied between 184 and 228 µE (micro Einsteins). The temperature of the growth chamber was set to 22°C during the daytime and 19°C during the nighttime for the planned experiments. The HTPP system has built-in auto-correction of colour and lens distortion. The design of the first experiment included 38 Arabidopsis thaliana ecotypes, each having 10 replicates, totalling 400 plants. Arabidopsis ecotypes such as Bch-4, Can-0, Col-0, Cvi-0, Sav-0, and other related ecotypes were grown in 5x5 trays under a 10 h light / 14 h dark cycle. Plants were randomly shuffled in a tray, ensuring that each tray contained a unique arrangement of ecotypes. Top-view (canopy-based) RGB images were acquired 12 days after sowing (DAS) in a sequence, i.e., twice a day, with a 6-hour interval between each screening time. Before conducting the second experiment, the growth rate of the ecotypes used in the first experiment was analysed, and the eight best-performing ecotypes were selected for the second experiment. During the second experiment, the following Arabidopsis ecotypes were grown in 4x5 trays, each containing 40 replicates: Col-0, Cvi-0, Is-1, Kz-9, Ler-1, TOU-I-17, Uk-1, and Zdr-1. The photoperiod was identical to that in the first experiment, however, four RGB images per day were collected, the same screening interval difference and 13 DAS. During both experiments, plants were constantly monitored, and if their leaves grew out of the camera scene, the corresponding pots were removed from the tray.
Video 1. Example of one screening round in a controlled growth chamber during both phenotyping experiments.
Since the camera system scans trays of plants from a top view, aside from the main tray, the raw RGB images may include parts of other trays or the floor of the growth chamber. Data preparation, including auto-tray and -pot cropping, as well as file organisation, is necessary to ensure adequate quality. Auto-tray cropping was established by using a set of coordinates (top-left and bottom-right parts of the image) that belong to the main tray visible in the RGB image. After that, cropped tray images were stored and organised based on the unique TRAY_ID in the growth chamber. Auto-pot cropping was established by randomly generating coordinates in the form of bounding boxes and manually positioning them around the pots of 5x5 or 4x5 experimental trays. Upon successful pot detection, a set of coordinates corresponding to each POT_ID was stored in a metadata file. Subsequently, the generated coordinates were loaded to execute the auto-pot cropping for each cropped tray image. Cropped pot images were stored into the following directory format Ecotype_name -> Rep_YY -> sequence of pot images, where YY is a double-digit number corresponding to a replicate number. After removing empty pot images and replicates that did not germinate, the total number of raw RGB images in the plant_ds1 dataset was 14,108, whereas the plant_ds2 dataset contained 18,559 structured images. Generated cropped RGB images were stored as PNG files, which allows lossless compression. The process of automating the cropping of trays and pots, as well as storing raw images in the database, is illustrated in Figure 2.
Figure 2. Automated cropping of trays and individual pots from raw RGB images, including the proper organisation of files within directories.
Another Arabidopsis dataset was generated at La Trobe University in 2019 to investigate temporal differences during plant development. Data acquisition was performed using an indoor HTPP growth chamber composed of 30 fixed stereo cameras installed to synchronously screen plants from different angles. Two of the most common Arabidopsis ecotypes, Col-0 and Cvi-0, were grown under a 14-hour light/10-hour dark cycle to simulate long-day conditions and 20⁰C with 50% humidity and watered every four days. The quality of the collected images required pre-processing, and then noise reduction and colour correction were performed manually by applying image processing algorithms. The experimental setup is demonstrated in Figure 3. More details about the experiment and aims can be found here.
Figure 3. Growth chamber with a multiple-camera indoor phenotyping systems design for extensive screening of Arabidopsis ecotypes.
Table 1. For the first two experiments, the day temperature was 22°C and night 19°C, while the average light intensity during the day varied between 184 to 228 (µE). In the third experiment, the day/night temperature was 20°C and light intensity during the day varied between 150 to 180 µE.
Ecotypes | Total | Images per day | Acquired images | |
---|---|---|---|---|
Experiment 1 | Ba4-1, Ba5-1, Bch-4, Br-0, C24, Cap-0, Col-0, Cvi-0, Ede-1, Edi-1, Et-6, Go-0, Hovdala-2, Hs-0, Hsm, Is-1, Jm-0, Kz-0, Ler-1, Li-5-2, Lz-0, MIB-28, Ot-0, Oy-0, PHW-2, Pro-0, Ren-11, Sav-0, TOU-1-17, TOU-J-3, Udu-1-34, Uk-1, Uk-4, Utrecht, Wil-2, Ws-2, Wt-5, and Zdr-1 | 38 | 2 | 14,108 |
Experiment 2 | Col-0, Cvi-0, Is-1, Kz-9, Ler-1, TOU-1-17, Uk-1, and Zdr-1 | 8 | 4 | 18,559 |
Experiment 3 | Col-0 and Cvi-0 | 2 | 18 | 70,927 |