Icarus
ISSN: 0019--1035
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Datasets associated with articles published in Icarus
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Observations of small NEOs from SST while operating in New Mexico.
Data Types:
  • Dataset
  • Text
MATLAB software used to perform plate tectonics force balance for ocean world ice shells.
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  • Dataset
  • File Set
Tabulation of Taxonomic and Principal Component Analysis for near-Earth objects observed in the MIT-Hawaii Near-Earth Object Spectroscopic Survey (MITHNEOS)
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  • Tabular Data
  • Dataset
  • Document
LVL 0 magnetometer data product description: The data is given in 24 hour frames with the decimal DOY (day of year) as the title, and is further split into half orbits, exploiting the nearly polar orbit of the LP spacecraft. Each struct contains the following: Col 1: LP LVL0 magnetometer data and position array (data)* Col 2: start of half-orbit in julian-time (jdstart) Col 3: end of half-orbit in julian-time (jdstop) Col 4: start of half-orbit in decimal doy (doystart) Col 5: end of half-orbit in decimal doy (doystop) Col 6: longitude at equator crossing (eqlon) * The description for the mag data arrays is as follows: Col 1: julian date Col 2: decimal doy Col 3: B_x (nT) Col 4: B_y (nT) Col 5: B_z (nT) Col 6: |B| (field magnitude) (nT) Col 7: julian date corresponding to spacecraft position/trajectory (Col 8-12)(redundant) Col 8: radius of spacecraft relative to fixed lunar center (km) Col 9: spacecraft translational velocity (km/s) Col 10: latitude (deg) Col 11: longitude (deg) Col 12: altitude (km)
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  • Dataset
Visible to near infrared reflectance spectra measured at the University of Winnipeg and thermal infrared emissivity spectra measured at the University of Oxford of the blind test samples. The samples and their measurements are described in the submitted manuscript.
Data Types:
  • Tabular Data
  • Dataset
Compositional and spectral data associated with this project.
Data Types:
  • Tabular Data
  • Dataset
Data files each contain a single abundance profile of HC3N, C3H4, CH3CN, or one of the two HCN isotopes: HC15N or H13CN; the latter two profiles have not been scaled by an isotope ratio value to represent HCN, as in the manuscript. Each file corresponds to either disk-averaged (_da) results, or spatially resolved profiles from North (48 N), Center (21 N), or South (16 S) retrievals (_n, _c, and _s, respectively). Abundance profiles cover the approximate altitudes where ALMA sensitivity allows for accurate retrievals: 50-550 km for HC3N, C3H4, and HCN isotopes, and 150-550 km for CH3CN. File column format is as follows: altitude (km), pressure (mbar), abundance.
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The dataset is collected by ChangE-1, which can be downloaded from Ground application system (http://moon.bao.ac.cn/) for lunar exploration project. The data ID of the research area is CE1_BMYK_IIM_SCI_N_20081204081022_20081204101804_4458, and the image concludes 2843 rows with 128 lines. The dataset includes 32 bands from 0.48 μm to 0.96 μm, the spectral resolution is 15nm.
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  • Text
The dataset is 2 Level collected by Chandrayaan-1 includes 85 contiguous bands from 460 nm to 2970 nm with 140-280 m spatial resolution for global observations. The data ID of the research area is M3G20090118T022705-V01-RFL, which can be downloaded from (http://pds-imaging.jpl.nasa.gov/data/m3).
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  • Software/Code
  • Dataset
Surface deposition profiles for the Enceladus plume.
Data Types:
  • Other
  • Dataset
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