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Found 775 dataset(s) matching "What: dust".
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The Micro-Imaging Dust Analysis System (MIDAS) is an instrument on the ROSETTA Orbiter that will provide 3D images and statistical parameters of pristine cometary particles hitting the detector....
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This archived Paleoclimatology Study is available from the NOAA National Centers for Environmental Information (NCEI), under the World Data Service (WDS) for Paleoclimatology. The associated NCEI...
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Supplemental information, excel spreadsheet of data behind figures in the paper, 11 files with code to reproduce the study. Citation information for this dataset can be found in the EDG's Metadata...
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This archived Paleoclimatology Study is available from the NOAA National Centers for Environmental Information (NCEI), under the World Data Service (WDS) for Paleoclimatology. The associated NCEI...
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Percent of size fraction and settling times
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A number of datasets from the VEGA missions were submitted by Dyachkov at IKI as FITS files (binary data) using the GROUPS form or multidimensioned arrays. In addition, little information was...
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A number of datasets from the VEGA missions were submitted by Dyachkov at IKI as FITS files (binary data) using the GROUPS form or multidimensioned arrays. In addition, little information was...
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The data from MPI for this dataset were received as text files each containing spectra of a single instrument mode (there were several files for most modes). These spectra were reformatted into...
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The data from MPI for this dataset were received as text files each containing spectra of a single instrument mode (there were several files for most modes). These spectra were reformatted into...
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The safety of the International Space Station (ISS) crewmembers and maintenance of ISS hardware are the primary rationale for monitoring microorganisms in this closed habitat. The composition of...
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Encounter data for Vega-2 consisted of two files: DSFAST27 and Dvg2CLN1. The data were submitted by the Univ of Chicago group along with hard copy versions of the operating manual and a preprint...
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Encounter data for Vega-2 consisted of two files: DSFAST27 and Dvg2CLN1. The data were submitted by the Univ of Chicago group along with hard copy versions of the operating manual and a preprint...
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The data from IKI for this dataset were received as two binary files containing data taken in all instrument modes. These files were split into separate files for each mode, preserving the...
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The data from MPI for this dataset were received as text files each containing spectra of a single instrument mode (there were several files for most modes). These spectra were reformatted into...
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The data from IKI for this dataset were received as two binary files containing data taken in all instrument modes. These files were split into separate files for each mode, preserving the...
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The PUMA data were submitted by IKI in two unique forms, a GROUPS FITS file and undocumented binary file. In one original form, the data in this set were received as 4,027 separate FITS files, one...
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Encounter Data for Vega-1 included two files: DSFAST17 and Dvega101. These files were submitted by the Univ of Chicago group with hard copy versions of the operating manual and a preprint of...
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Encounter Data for Vega-1 included two files: DSFAST17 and Dvega101. These files were submitted by the Univ of Chicago group with hard copy versions of the operating manual and a preprint of...
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The PUMA data were submitted by IKI in two unique forms, a GROUPS FITS file and undocumented binary file. In one original form, the data in this set were received as 4,027 separate FITS files, one...
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The PIA data was acquired in four modes of data compression, termed mode 0 (the least compressed), and modes 1, 2, and 3, each with increasing degrees of compression. With each spectrum are a PIA...
