Planetary and Space Science

We share the photometric and spectroscopic observation data about (3200) Phaethon used in our paper. The photometric observations were conducted at Mt. Lemon Optical Astronomy Observatory (LOAO) in Arizona, USA using the 1m telescope and the 4K x 4K e2v CCD from November 11 to 13, 2017. The spectroscopic data was observed at Mt. Bohyunsan Optical Astronomy Observatory (BOAO) in Korea using the 1.8m telescope, with the 4K x 4K e2v CCD and long-slit spectrograph on December 7, 2017. This data is including the raw file, calibrations and processed data.

Digital elevation model,the models of illumination and communication conditions at landing region for the Chang’E-5 mission based on LOLA data

These two excel data tables contain the reduced CODEX LARIMS data required to reproduce our Zagami isochron diagrams for February and September 2019 data acquisitions. Each excel file has a header explaining each column. Each spot measurement on Zagami is recorded as a row, with a filename to allow us to identify the original raw data if needed, the date acquired, the measurement position on the sample, the integrated peak areas, the 1-sigma standard error uncertainties, and correlation coefficients.

HRSC Level 2 Product IDs used as Inputs to produce a New South Polar Digital Terrain Model of Mars

1) Set stimulation settings and run the script 2) Tune Advanced Model and run the script 3) run save_results to save the results

The field of In Situ Resource Utilisation (ISRU) is expanding rapidly with a particular focus on developing ISRU technologies and applications to support a longer-term surface exploration of the Moon. In this respect, microwave sintering is proposed to be one of the potential fabrication methods for developing a 3D printing technique for construction processes on the Moon. Thus, understanding the behaviour of lunar regolith, available at different locations on the Moon (e.g. mare versus highlands regions), under microwave heating is crucial for developing an optimal method for microwave sintering. As the availability of real lunar regolith on Earth is highly limited, developing an appropriate numerical model of microwave heating behaviour of lunar regolith is urgently required. In this paper, three representative lunar regolith samples (selected from the database of Apollo sample collections) with pre-defined material properties have been simulated under seven input powers and three specimen sizes. This paper discusses the outcomes of these simulations and the potential contribution of the model for developing a desired 3D printing technique utilising microwave sintering of lunar regolith.

Sodium velocity profiles reported by Yakshinskiy and Madey (2000, 2004)

Sample video used when testing the convolutional neural network (CNN) on real data. The video is in a raw binary format (unit16 greyscale). To generate all the necessary training data for the CNN, over 2TB of data was processed to find samples, thus only a small segment is shown here.

Comparison of different reported anaerobic growth and metal reduction experiments with Shewanella oneidensis. Used electron donors and acceptors are listed and important aspects of the experimental designs are noted. In some cases, reported parameters are combined to obtain missing values.

Event_list.txt: List of events used in the statistical analysis section. G_correction_coefficients.txt: Tables of correction factors to the geometric factor of the RPC-IES electron sensor.