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283 results for “orbital data”
Lunar Orbiter Laser Altimeter (LOLA) one-way Laser Ranging Full Rate Data (all ranges collected, ground stations, aggregate of normal points daily) from NASA CDDIS
Lunar Orbiter Laser Altimeter (LOLA) one-way laser ranging full rate data. These files contain the full rate data (all ranges collected) as delivered from the ground stations participating in one way ranging. Each file is an aggregate of full rate data collected for every station on a particular day. Note that this does not constitute the official data delivered by the LOLA mission; for these data, please visit the LOLA Planetary Data System listed in the reference. The ground station only data may be useful for those who wish to do their own transmit-receive pairing from onboard spacecraft data.
OMI/Aura Level 2 Sulphur Dioxide (SO2) Trace Gas Column Data 1-Orbit Subset and Collocated Swath along CloudSat V003 (OMSO2_CPR) at GES DISC
This is a CloudSat-collocated subset of the original product OMSO2, for the purposes of the A-Train mission. The goal of the subset is to select and return OMI data that are within +/-100 km across the CloudSat track. The resultant OMI subset swath is sought to be about 200 km cross-track of CloudSat. Even though collocated with CloudSat, this subset can serve many other A-Train applications. (The shortname for this CloudSat-collocated subset of the original product OMSO2 Product is OMSO2_CPR_V003) This document describes the original OMI SO2 product (OMSO2) produced from global mode UV measurements of the Ozone Monitoring Instrument (OMI). OMI was launched on July 15, 2004 on the EOS Aura satellite, which is in a sun-synchronous ascending polar orbit with 1:45pm local equator crossing time. The data collection started on August 17, 2004 (orbit 482) and continues to this day with only minor data gaps. The minimum SO2 mass detectable by OMI is about two orders of magnitude smaller than the detection threshold of the legacy Total Ozone Mapping Spectrometer (TOMS) SO2 data (1978-2005) [Krueger et al 1995]. This is due to smaller OMI footprint and the use of wavelengths better optimized for separating O3 from SO2. The product file, called a data granule, covers the sunlit portion of the orbit with an approximately 2600 km wide swath containing 60 pixels per viewing line. During normal operations, 14 or 15 granules are produced daily, providing fully contiguous coverage of the globe. Currently, OMSO2 products are not produced when OMI goes into the "zoom mode" for one day every 452 orbits (~32 days). For each OMI pixel we provide 4 different estimates of the column density of SO2 in Dobson Units (1DU=2.69x10^16 molecules/cm2) obtained by making different assumptions about the vertical distribution of the SO2. However, it is important to note that in most cases the precise vertical distribution of SO2 is unimportant. The users can use either the SO2 plume height, or the center of mass altitude (CMA) derived from SO2 vertical distribution, to interpolate between the 4 values: 1)Planetary Boundary Layer (PBL) SO2 column (ColumnAmountSO2_PBL), corresponding to CMA of 0.9 km. 2)Lower tropospheric SO2 column (ColumnAmountSO2_TRL), corresponding to CMA of 2.5 km. 3)Middle tropospheric SO2 column, (ColumnAmountSO2_TRM), usually produced by volcanic degassing, corresponding to CMA of 7.5 km, 4)Upper tropospheric and Stratospheric SO2 column (ColumnAmountSO2_STL), usually produced by explosive volcanic eruption, corresponding to CMA of 17 km. The accuracy and precision of the derived SO2 columns vary significantly with the SO2 CMA and column amount, observational geometry, and slant column ozone. OMI becomes more sensitive to SO2 above clouds and snow/ice, and less sensitive to SO2 below clouds. Preliminary error estimates are discussed below (see Data Quality Assessment). OMSO2 files are stored in EOS Hierarchical Data Format (HDF-EOS5). Each file contains data from the day lit portion of an orbit (53 minutes). There are approximately 14 orbits per day. The maximum file size for the OMSO2 data product is about 9 Mbytes.
Expression data from human brain orbital ventral prefrontal cortex - including control samples and samples with major depression disorders (24 samples NY_BA47)
GEO Series GSE54575. Homo sapiens. 24 samples. Type: Expression profiling by array.
PVO V SUPP EXPERIMENTER DATA RECORD SC ORBIT/ATTITUDE V1.0
This dataset contains the Supplemental Experimenter Data Records (SEDR) as provided by the Pioneer project to the Magnetometer team (C.T. Russell - PI). The dataset covers the entire period of orbital operations, orbits 1-5055 (1978-12-05 to 1992-10-07). Each orbit was originally provided on a separate IBM 9-track 800 bpi tape which contained 6 files: 1) Standard Label file [sl] , 2) Ephemeris file [ep], 3) S/C Attitude file [at], 4) Pulse Time file [pt], 5) Selected Roll Reference file [sr], 6) Spin period file [sp]. The original structure has been preserved within the limitations of the CD-ROM media, and the PDS data archive rules. The data remain in individual orbit files in IBM binary and EBCDIC representations.
ROSETTA-ORBITER COMET PRELANDING OSINAC 3 RDR DATA MTP 002
This data set contains calibrated images acquired by the OSIRIS Narrow Angle Camera during the prelanding phase of the Rosetta mission at the comet 67P, covering the period from 2014-04-06 to 2014-05-07.
ROSETTA-ORBITER LUTETIA FLY-BY OSIWAC 2 EDR data
This data set contains images acquired by the OSIRIS Wide Angle Camera during the LUTETIA FLY-BY mission phase
SSC 4D Orbit Viewer Web Services API at the Space Physics Data Facility (SPDF)
This API allows any web application to offer an interactive 4D display of the trajectories of satellites known to SSCweb (Satellite Situation Center). The Space Physics Data Facility (SPDF) is the archive of non-solar data for the Heliospheric Science Division (HSD) at NASA's Goddard Space Flight Center.
ROSETTA-ORBITER CRUISE 4-2 OSIWAC 2 EDR data
This data set contains images acquired by the OSIRIS Wide Angle Camera during the CRUISE 4-2 mission phase
GALILEO ORBITER JUPITER RAW MAGNETOMETER DATA V1.0
This data set contains raw magnetic field data acquired by the Galileo Orbiter magnetometer at Jupiter. The data set covers the time period from 1995-11-06T00:21:30 UT (Jupiter approach) until the end of mission (March 2003). The raw magnetometer data set includes various forms of data: recorded high time resolution, real-time survey (RTS), optimal averager (opt/avg), snapshot, and the calibration parameters required to generate processed data products. In addition corrected rotor angles and spacecraft relative clock and cone angles are provided to simplify future calibration and reprocessing of the data.
ROSETTA-ORBITER COMET PRELANDING OSINAC 2 EDR DATA MTP 003
This data set contains raw EDR images acquired by the OSIRIS Narrow Angle Camera during the prelanding phase of the Rosetta mission at the comet 67P, covering the period from 2014-05-07 to 2014-06-04.
ROSETTA-ORBITER CRUISE 5 OSIWAC 2 EDR data
This data set contains images acquired by the OSIRIS Wide Angle Camera during the CRUISE 5 mission phase
SSCweb orbit locations at the Space Physics Data Facility (SPDF)
Display and download orbit and trajectory data for most heliophysics missions. The Satellite Situation Center (SSC) also enables complex queries between spacecraft and ground locations, tracing along magnetic field lines, and geophysical regions of space. The Space Physics Data Facility (SPDF) is the archive of non-solar data for the Heliospheric Science Division (HSD) at NASA's Goddard Space Flight Center.
ROSETTA-ORBITER CRUISE 5 OSIWAC 3 RDR data
This data set contains images acquired by the OSIRIS Wide Angle Camera during the CRUISE 5 mission phase
ROSETTA-ORBITER COMET PRELANDING OSIWAC 2 EDR DATA MTP 004
This data set contains raw EDR images acquired by the OSIRIS Wide Angle Camera during the prelanding phase of the Rosetta mission at the comet 67P, covering the period from 2014-06-04 to 2014-06-18.
Pioneer Venus Orbiter (PVO) Magnetometer, OMAG, Plasma Analyzer, OPA, Merged Solar Wind Data, 10 min Data
Pioneer Venus Orbiter, PVO, was the first orbiter mission designed to conduct a comprehensive and long term investigation of the planet Venus. PVO measured the detailed structure of the upper atmosphere and ionosphere of Venus and investigated the interaction of the solar wind with the Venusian ionosphere. Over the years from 1978 to 1992, PVO provided nearly continuous measurements of the solar wind from its highly eccentric orbit around Venus. * PI, magnetic field instrument: C.T. Russell, University of California, Los Angeles * PI, plasma instrument: A. Barnes, Ames Research Center, NASA This merged data includes 10-minute averages for selected parameters of the interplanetary magnetic field, solar wind plasma, and spacecraft trajectory. The data were taken when the spacecraft was outside the bow shock of the Venusian ionosphere and was in the solar wind. Venus Solar Orbital (VSO) coordinates are defined with respect to the orbital plane of Venus which is tilted about two degrees from the Ecliptic. The VSO system is Venus-centered with the X axis towards the Sun, the Z axis northward and perpendicular to the orbital plane, and the Y axis completing the right hand system. Time coverage of merged data: 1978-12-06 to 1988-08-07. PVO data were converted to CDF based on the flatfiles from UCLA.
MAVEN Magnetometer (MAG) Magnetic Field and Orbital Position, Sun-State and Payload Coordinates, Level 2 (L2), 1 s Data
The MAVEN Magnetic Field Investigation is Part of a comprehensive Particles and Fields Subsystem that will measure the Magnetic and Electric Fields and Plasma Environment of Mars and its Interaction with the Solar Wind. This Data Product includes Magnetic Field Observations in Sun-State and Payload Coordinates. Sun-State, SS, Coordinate System wherein the Primary Reference Vector, the X-axis, points from the Object, in this case Mars, to the Sun and the Secondary Reference Vector, the Y-axis, is in the Mars Orbit Plane, which is approximately opposite to Orbital Motion Direction, such that the Z-axis is Northward. The Observations Spacecraft Payload, PL, Coordinates are suitable for use in association with Measurements obtained by other Instruments on the Spacecraft. The Spacecraft Payload Coordinate System and the MAG Sensor Coordinate Systems are illustrated in Figure 21 of Connerney et al., 2015. The Text appearing here is also adapted from Connerney et al., 2015.
ROSETTA-ORBITER CRUISE 4-2 OSINAC 2 EDR data
This data set contains images acquired by the OSIRIS Narrow Angle Camera during the CRUISE 4-2 mission phase
ROSETTA-ORBITER COMET PRELANDING OSINAC 2 EDR data
This data set contains images acquired between 2014-06-04 and 2014-06-18 by the OSIRIS Narrow Angle Camera during the prelanding phase of the Rosetta mission at the comet 67P
ROSETTA-ORBITER CRUISE 5 OSINAC 3 RDR data
This data set contains images acquired by the OSIRIS Narrow Angle Camera during the CRUISE 5 mission phase
ROSETTA-ORBITER LUTETIA FLY-BY OSINAC 3 RDR data
This data set contains images acquired by the OSIRIS Narrow Angle Camera during the LUTETIA FLY-BY mission phase
ScienceDex guides
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These curated guides explain access requirements, typical timelines, costs, and reuse considerations for widely used research datasets.
Allen Brain Atlas
Allen Brain Atlas is an Allen Institute collection of brain map atlases, datasets, APIs, and analysis tools covering mouse, human, and non-human primate brain resources.
Annotated Behaviour and Observability Dataset (ABODe)
ABODe is a University of Edinburgh DataShare dataset for behavior classification in group-housed mice using home-cage video, identities, bounding boxes, ground-plate positions, and annotator labels.
DANDI Archive for NWB datasets
DANDI is a BRAIN Initiative archive for publishing and sharing neurophysiology data, including electrophysiology, optophysiology, and behavioral data packaged as NWB and related standards.
International Brain Laboratory public data
The International Brain Laboratory public data releases expose standardized mouse decision-making experiments, including Neuropixels recordings, widefield calcium imaging, behavior, and session metadata accessed through the ONE API.
OpenNeuro
OpenNeuro is a free, open platform for sharing neuroimaging datasets, with public search, dataset pages, and download paths for web, S3, DataLad, and the OpenNeuro CLI.