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21 results for “dust detection”
A subset of the EMARS dataset in MY24 and MY26 converted from the sigma-p hybrid coordinate to the pressure coordinate and a list of local dust storms detected during the MYs in western Arcadia Planitia
<p>This dataset includes a subset of EMARS' background mean data (Greybush et al., 2019) converted from the sigma-p hybrid coordinate to the pressure coordinate. Only MY24 and MY26 were used to generate the figures shown in Ogohara (submitted to JGR Planets). <br>Updates from the original EMARS are:</p> <ul> <li>The vertical coordinate has been converted from the sigma-p hybrid coordinate to the pressure coordinate.</li> <li>The variables expressing the Earth date (e.g., year, month, day, etc.) have been combined into one variable, earth_date.</li> <li>A new variable, emars_date, has been created from emars_sol and mars_hour.</li> </ul> <p>In addition, this dataset provides two lists of local dust storms events during MY24 and MY26 which were detected in western Arcadia Planitia using a deep learning-based method proposed by Ogohara and Gichu (2022). The lists are:</p> <ul> <li>[Data Set S1] List of global image swath files examined. Only file names of MGS/MOC red band images are listed. The list consists of 5 columns indicating image ID, observation date, orbit number, solar longitude, and filter name (RED).</li> <li>[Data Set S2] List of global image swath files containing identified dust storms, as well as some attributes of the detected dust storms. Only file names of red band images are listed. The list consists of 7 columns indicating image ID, observation date, orbit number, solar longitude, center longitude and latitude, and area (km2.)</li> </ul>
Distribution of interplanetary dust detected by the Juno spacecraft and its contribution to the Zodiacal Light
<p>The Zodiacal light is sunlight reflected by dust in the inner solar system. Variations in the Zodiacal light with ecliptic latitude reveal discrete bands of dust orbiting near the ecliptic plane. The Juno spacecraft, in transit from earth to Jupiter, recorded a sufficient number of impacts with this dust to characterize their distribution in space for the first time. </p> <p>This dataset (filename IDP_List.txt) contains a time-ordered list of all IDP impact detections along with supplementary engineering and ephemeris information. The file is an ASCII text file and the file format is described in the word document (IDP_List_Format.docx).</p>
Polarization lidar data for detecting dust orientation
<p>Polarization lidar data used in publication:</p> <p>Tsekeri, A., Amiridis, V., Louridas, A., Georgoussis, G., Freudenthaler, V., Metallinos, S., Doxastakis, G., Gasteiger, J., Siomos, N., Paschou, P., Georgiou, T., Tsaknakis, G., Evangelatos, C., and Binietoglou, I.: Polarization lidar for detecting dust orientation: System design and calibration, Atmos. Meas. Tech. Discuss. [preprint], https://doi.org/10.5194/amt-2021-30, in review, 2021.</p>
Impact ionization dust detection with compact, hollow and fluffy dust analogs
<p>Datasets for the Planetary and Space Science article "Impact ionization dust detection with compact, hollow and fluffy dust analogs" (DOI: 10.1016/j.pss.2022.105536). The data contains two folders for dust impacts on the IIT and CAT targets of CDA. The folders contain separate tables with data for each run. Each table shows the registered CDA impacts for the corresponding run with impact time in UTC (determined by CDA) and all additional information about the impact that could be reconstructed from the measurements of CDA and other detectors (impact velocity, dust mass, ...). Data that could not be reconstructed are represented by NAN values in the tables.</p>
Dust devil detection microbarometer and weather – Summer 2018 data
Open the record for dataset details and reuse information.
Remote-sensing detectability of airborne Arctic dust - code
<p>The Matlab codes employed in the generation of the figures of the paper "Remote-sensing detectability of airborne Arctic dust", submitted to Atmospheric Chemistry and Physics (https://egusphere.copernicus.org/preprints/2024/egusphere-2024-1057/).</p>
Juno Waves Detection of Dust Impacts near Jupiter
<p>This is the supporting data set for the paper by the same title published in AGU JGR Space Physics. DOI 10.1029/2019JE006367</p> <p>Abstract:</p> <p>The Juno spacecraft entered orbit at Jupiter on July 5, 2016. Since then, Juno has orbited Jupiter in high inclination orbits, crossing the ring plane near perijove 21 times. During 20 of the 21 crossings, the Waves instrument detected signals induced by dust impacts. The impact rate profiles show peaks of order 6/s around the ring plane with half width at half max ~2000-3000 km. The polarity ratio of the impact signals didn't follow the areas of the antennas exposed to dust impacts that change due to the rotation of the spacecraft, suggesting Waves detects impacts on the Juno spacecraft and not just on the Waves antennas. The impact rate profile changed during Perijove 19, when the spacecraft rotation axis was tilted to the south, increasing the area of the solar panels exposed to impacts, indicating that the detected impacts were on the spacecraft body. Grain sizes of order 1 micrometer are estimated, and the differential size distribution has a slope of -5.1.</p> <p>Notes on zip archive:</p> <p>There are subdirectories for each figure including a PDF of the figure and one or more text files with the data supporting the figure. Where the labeling in the text file is not quite complete, we've added a Fign-readme.txt file.</p> <p>Figures 9 and 10 are in the same directory as the two figures just have more of the same and all the data for both figures is in the same file.</p>
GALILEO DUST DETECTION SYSTEM V4.1
This data set contains the data from the Galileo dust detector system (GDDS) from start of mission through the end of mission. Included are the dust impact data, noise data, laboratory calibration data, and location and orientation of the spacecraft and instrument.
ULYSSES DUST DETECTION SYSTEM V2.0
Dataset Overview ================ This data set contains information on dust the dust environment in interplanetary space within the inner solar system, between Jupiter and the Sun, and at high polar latitudes of the Sun. Both interplanetary and interstellar dust particles have been detected. This information is collected with a dust impact experiment, from which may be inferred direction of motion, mass, velocity and charge (see ULYDINST.CAT). The data presented in this dataset include instrumental readouts, inferred metadata, calibration information and a calendar of events. Specifically:
GALILEO DUST DETECTION SYSTEM V2.0
This data set contains information on the dust environment in interplanetary space within the inner solar system and in the Jupiter system, within and without the Jovian magnetosphere and around the Galilean satellites.
GALILEO DUST DETECTION SYSTEM V4.0
This data set contains the data from the Galileo dust detector system (GDDS) from start of mission through the end of mission. Included are the dust impact data, noise data, laboratory calibration data, and location and orientation of the spacecraft and instrument.
ULYSSES DUST DETECTION SYSTEM V3.1
This data set contains the data from the Ulysses dust detector system (UDDS) from start of mission through the end of mission, 1990-2007. (As the dust detector was turned off after Nov. 30, 2007, this is the last date for which UDDS data is recorded.) Included are the dust impact data, noise data, laboratory calibration data, and location and orientation of the spacecraft and instrument.
ULYSSES DUST DETECTION SYSTEM V3.0
This data set contains the data from the Ulysses dust detector system (UDDS) from start of mission through the end of mission, 1990-2007. (As the dust detector was turned off after Nov. 30, 2007, this is the last date for which UDDS data is recorded.) Included are the dust impact data, noise data, laboratory calibration data, and location and orientation of the spacecraft and instrument.
GALILEO DUST DETECTION SYSTEM V3.0
Detector responses and derived quantities from the Galileo dust detector as well as spacecraft geometry information for reliable impacts from launch through 2001. See Gruen et al. (Plan. Sp. Sci. 43, 953-969, 1995) and Krueger et al. (Plan. Sp. Sci. 47, 85-106, 1999; Plan. Sp. Sci. 49, 1285-1301, 2001) for more information.
GALILEO DUST DETECTION SYSTEM V2.0
This data set contains information on the dust environment in interplanetary space within the inner solar system and in the Jupiter system, within and without the Jovian magnetosphere and around the Galilean satellites.
ULYSSES DUST DETECTION SYSTEM V3.0
This data set contains the data from the Ulysses dust detector system (UDDS) from start of mission through the end of mission, 1990-2007. (As the dust detector was turned off after Nov. 30, 2007, this is the last date for which UDDS data is recorded.) Included are the dust impact data, noise data, laboratory calibration data, and location and orientation of the spacecraft and instrument.
GALILEO DUST DETECTION SYSTEM V4.1
This data set contains the data from the Galileo dust detector system (GDDS) from start of mission through the end of mission. Included are the dust impact data, noise data, laboratory calibration data, and location and orientation of the spacecraft and instrument.
GALILEO DUST DETECTION SYSTEM V3.0
Detector responses and derived quantities from the Galileo dust detector as well as spacecraft geometry information for reliable impacts from launch through 2001. See Gruen et al. (Plan. Sp. Sci. 43, 953-969, 1995) and Krueger et al. (Plan. Sp. Sci. 47, 85-106, 1999; Plan. Sp. Sci. 49, 1285-1301, 2001) for more information.
GALILEO DUST DETECTION SYSTEM V4.0
This data set contains the data from the Galileo dust detector system (GDDS) from start of mission through the end of mission. Included are the dust impact data, noise data, laboratory calibration data, and location and orientation of the spacecraft and instrument.
ULYSSES DUST DETECTION SYSTEM V3.1
This data set contains the data from the Ulysses dust detector system (UDDS) from start of mission through the end of mission, 1990-2007. (As the dust detector was turned off after Nov. 30, 2007, this is the last date for which UDDS data is recorded.) Included are the dust impact data, noise data, laboratory calibration data, and location and orientation of the spacecraft and instrument.
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