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36 results for “Sensor Calibration”
Methane sensor calibration dataset
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Development and calibration of dynamic pressure sensor for motor pressure range
<p>"Calibration results of dynamic pressure sensors.xlsx". Calibration results for VTT cylinder pressure sensor</p>
Data from: Development and calibration of a novel sensor to quantify the water content of surface soils and biological soil crusts
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Pressure Correction in the Calibration of Heat Dissipation Sensors
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Feasibility Study to Determine the Optimal Calibration Method for Glucose Sensors
ClinicalTrials.gov study NCT02155023. IPD Sharing: Not stated. Countries: 1. Publications: 0.
Calibration and Evaluation of an Audio Pulse Oximeter Sensor (AudioOx) at Ascent and Descent From Simulated Altitude
ClinicalTrials.gov study NCT01732029. IPD Sharing: Not stated. Countries: 1. Publications: 0.
Improved Calibration of Electrochemical Aptamer-Based Sensors
<p>Figure 2A raw data: titration of vancomycin into 37C rat blood</p>
CASSINI S MIMI LEMMS SENSOR CALIBRATED DATA V1.0
The Cassini Magnetospheric Imaging Instrument (MIMI) Low Energy Magnetospheric Measurements (LEMMS) measures ions and electrons in the energy range 0.03 to 18 MeV for ions and 0.015 to 0.884 MeV for electrons. The LEMMS calibrated data set includes two types of daily plots -- one presenting energy-time spectorgrams in units of intensity, and one with plots of particle pressures. There are also four types of averaged data -- minute and hourly averages for accumulator rate data and PHA data (ions and electrons). These data have been created at the Johns Hopkins University Applied Physics Laboratory by applying the calibrations and averaging. Averaging is done by first defining time periods, and then averaging all data points within those fixed intervals. The time reported is the midpoint time of the interval.
CASSINI S MIMI INCA SENSOR CALIBRATED DATA V1.0
The Ion and Neutral Camera (INCA) obtains remote images of the global distribution of energetic ions for energies from 7 keV/nucleon to 8 MeV/nucleon, discriminated according to energy and mass species (oxygen and hydrogen). To obtain the images, INCA measures the arrival directions, energy and mass species of Energetic Neutral Atoms (ENA's) using the relatively new technique of ENA imaging. INCA also can be commanded to obtain very high sensitivity ion measurements, providing the angular, energy and species distributions of in-situ O and H ions. The Cassini Magnetospheric Imaging Instrument(MIMI) Imaging Neutral Camera (INCA) calibrated data set includes all image data collected from the MIMI Data Processing Unit during the Saturn tour. The original data has been decommutated, decoded, calibrated and further processed by software at the Applied Physics Laboratory (APL). The calibrated image data is provided in three forms: an averaged form where the original image N x N pixel images pixels intensity are averaged to a single value for one species and time-of-flight (TOF) combination, browse images which display rows and columns of images for one species and TOF combination, and movies which display averaged ENA image skymaps. Calibration of INCA data has been described fully in the Cassini/MIMI Data User Guide. This data set should be among the first used by a user of any of the MIMI INCA archive as it will lead one to information required to search for more detailed or highly specialized features in the original data.
PVO VENUS MAG CALIBRATED P-SENSOR HIGH RES V1.0
This dataset contains full resolution magnetometer data from the Pioneer Venus Orbiter spacecraft beginning with orbit 3602 (Oct 16, 1988) and continuing until the orbiter was lost in the Venusian atmosphere (orbit 5055, Oct 7, 1992). The dataset differs from the high resolution magnetometer dataset from theprevious orbits due to an anomaly in the multiplexor that controlled the sampling of the magnetometer sensors. During orbit 3602, and for the remainder of the mission, the spacecraft downlink contained magnetometer data from only the P sensor. The P sensor is the sensor which is aligned with the spacecraft spin axis, nominally in the direction of the ecliptic normal.
CASSINI S MIMI CHEMS SENSOR CALIBRATED DATA V1.0
The Cassini Magnetospheric Imaging Instrument(MIMI) Charge Energy Mass Spectrometer (CHEMS) contains a deflection system and an overall field of view of 159 x 4 deg. that is comprised of three distinct energetic particle telescopes each having a field of view of 53 x 4. All telescopes share the same deflection mechanism, but each has its own start and stop microchannel plate (MCP) and its own solid-state detector (SSD). Much of the data returned by CHEMS is separated by telescope. The deflection plate power supply (DPPS) has 32 different voltages that can be applied across the deflection plates. For any single DPPS step, the electrostatic analyzer only transmits incoming ions within a narrow range of energy per charge (a 3% pass band). The CHEMS calibrated data set includes the Pulse Height Analysis (PHA) data collected during the Saturn tour. CHEMS PHA provides a list of individually detected particles, with specific detection parameters for each event, including TOF, energy deposited in the SSD, and telescope number. The energy per charge data for six ion species (H+, He+, H2+, He++, O++, W+) are presented in two forms. (The W+ water ion group includes O+, OH+, H20+ and H30+). One form is a set of tables which are of variable length and use a comma to separate various fields, and the other is a PDF file containing the energy per charge spectrograms and are based on CHEMS PHA data. The original data has been decommutated and decoded by software at the Applied Physics Laboratory (APL) and calibrated and further processed by software at the University of Maryland. This data set should be among the first used by a user of any of the MIMI CHEMS archive as it will lead one to information required to search for more detailed or highly specialized features in the original data.
MAVEN SEP Calibrated Ion and Electron Spectra Data Collection (Sensor 1)
Calibrated MAVEN Solar Energetic Particle (SEP) Instrument Sensor 1 ion and electron spectra. The data include total (integrated) and differential (as a function of 28 energy windows) ion and electron number fluxes in forward and reverse look directions. Description of the SEP instrument can be found on the SEP home page https://lasp.colorado.edu/maven/science/instrument-package/sep/ and in the SEP instrument publication https://doi.org/10.1007/s11214-015-0218-z.
CASSINI S MIMI LEMMS SENSOR CALIBRATED DATA V1.0
The Cassini Magnetospheric Imaging Instrument (MIMI) Low Energy Magnetospheric Measurements (LEMMS) measures ions and electrons in the energy range 0.03 to 18 MeV for ions and 0.015 to 0.884 MeV for electrons. The LEMMS calibrated data set includes two types of daily plots -- one presenting energy-time spectorgrams in units of intensity, and one with plots of particle pressures. There are also four types of averaged data -- minute and hourly averages for accumulator rate data and PHA data (ions and electrons). These data have been created at the Johns Hopkins University Applied Physics Laboratory by applying the calibrations and averaging. Averaging is done by first defining time periods, and then averaging all data points within those fixed intervals. The time reported is the midpoint time of the interval.
CASSINI S MIMI CHEMS SENSOR CALIBRATED DATA V1.0
The Cassini Magnetospheric Imaging Instrument(MIMI) Charge Energy Mass Spectrometer (CHEMS) contains a deflection system and an overall field of view of 159 x 4 deg. that is comprised of three distinct energetic particle telescopes each having a field of view of 53 x 4. All telescopes share the same deflection mechanism, but each has its own start and stop microchannel plate (MCP) and its own solid-state detector (SSD). Much of the data returned by CHEMS is separated by telescope. The deflection plate power supply (DPPS) has 32 different voltages that can be applied across the deflection plates. For any single DPPS step, the electrostatic analyzer only transmits incoming ions within a narrow range of energy per charge (a 3% pass band). The CHEMS calibrated data set includes the Pulse Height Analysis (PHA) data collected during the Saturn tour. CHEMS PHA provides a list of individually detected particles, with specific detection parameters for each event, including TOF, energy deposited in the SSD, and telescope number. The energy per charge data for six ion species (H+, He+, H2+, He++, O++, W+) are presented in two forms. (The W+ water ion group includes O+, OH+, H20+ and H30+). One form is a set of tables which are of variable length and use a comma to separate various fields, and the other is a PDF file containing the energy per charge spectrograms and are based on CHEMS PHA data. The original data has been decommutated and decoded by software at the Applied Physics Laboratory (APL) and calibrated and further processed by software at the University of Maryland. This data set should be among the first used by a user of any of the MIMI CHEMS archive as it will lead one to information required to search for more detailed or highly specialized features in the original data.
CASSINI S MIMI INCA SENSOR CALIBRATED DATA V1.0
The Ion and Neutral Camera (INCA) obtains remote images of the global distribution of energetic ions for energies from 7 keV/nucleon to 8 MeV/nucleon, discriminated according to energy and mass species (oxygen and hydrogen). To obtain the images, INCA measures the arrival directions, energy and mass species of Energetic Neutral Atoms (ENA's) using the relatively new technique of ENA imaging. INCA also can be commanded to obtain very high sensitivity ion measurements, providing the angular, energy and species distributions of in-situ O and H ions. The Cassini Magnetospheric Imaging Instrument(MIMI) Imaging Neutral Camera (INCA) calibrated data set includes all image data collected from the MIMI Data Processing Unit during the Saturn tour. The original data has been decommutated, decoded, calibrated and further processed by software at the Applied Physics Laboratory (APL). The calibrated image data is provided in three forms: an averaged form where the original image N x N pixel images pixels intensity are averaged to a single value for one species and time-of-flight (TOF) combination, browse images which display rows and columns of images for one species and TOF combination, and movies which display averaged ENA image skymaps. Calibration of INCA data has been described fully in the Cassini/MIMI Data User Guide. [VANDEGRIFFETAL2012] This data set should be among the first used by a user of any of the MIMI INCA archive as it will lead one to information required to search for more detailed or highly specialized features in the original data.
PVO VENUS MAG CALIBRATED P-SENSOR HIGH RES V1.0
not applicable
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Allen Brain Atlas
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Annotated Behaviour and Observability Dataset (ABODe)
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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.