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501 results for “Charging”
ACE Solar Wind Ion Composition Spectrometer (SWICS) Solar Wind Plasma Elemental Charge State Distributions with Statistical Uncertainties and Data Quality Flags, Level 2 (L2), 2 h Data
This ACE SWICS/SWIMS Data Set contains actual Charge State, Q, Distributions of Carbon, Oxygen, Neon, Magnesium, Silicon and Iron as opposed to the averaged Charge States that have been available on CDAWeb for some time. The Solar Wind Ion Composition Spectrometer (SWICS), prior to August 23, 2011 and denoted as SWICS Version 1.1, determines uniquely the Chemical and Ionic Charge State Composition of the Solar Wind, the Temperatures and Mean Speeds of major Solar Wind Ions at all Speeds above 300 km/s for Protons and 170 km/s for Fe+16, and resolves Protons and Helium Isotopes of Solar and Interstellar Sources. SWICS 1.1 measures the Distribution Functions of Interstellar Cloud Pick-Up Ions and Interplanetary Dust Cloud Pick-Up Ions up to Energies of 100 keV/e. The ACE SWICS 1.1 Data Products represent a new Release of the Data with significantly improved Time Series Measurements for the Elemental Abundance, Charge State Composition, and Kinetic Properties of Heavy Ions in the Solar Wind. It is a major new Update produced with completely redesigned Analysis Methods to account more rigorously for Instrumental and Statistical Effects (Shearer et al., 2014). Rare Elements are now identified more reliably and Estimates of Statistical Error are provided. Release Notes are available that describe the Data, the Methods used to determine the Data Values, and Issues concerning Data Quality and Measurement Uncertainty. The Quality of ACE Level 2 Data is such that it is suitable for serious Scientific Study. However, to avoid Confusion and Misunderstanding, it is recommended that Users consult with the appropriate ACE Team Members before publishing Work derived from the Data. The ACE Team has worked hard to ensure that the Level 2 Data are free from Errors, but the Team cannot accept Responsibility for Erroneous Data, or for Misunderstandings about how the Data may be used. This is especially true if the appropriate ACE Team Members are not consulted before Publication. At the very least, Preprints should be forwarded to the ACE Team before Publication. For more Information about the SWICS Instrument, visit the SWICS Home Page at http://solar-heliospheric.engin.umich.edu/ace.
Wind Hot Plasma and Charged Particles (3DP) Electron Electrostatic Analyzer (EESA) Low, Omnidirectional Flux Spectra, 5 eV to 1100 eV, 24 s Data
Wind Three-Dimensional Particle, 3DP, instrument, Electron Electrostatic Analyzer, EESA, Low Energy Spectra, ELSP, omni directional electron differential number flux spectra, 3 eV to 30 keV.
SOHO Charge, Element, and Isotope Analysis System (CELIAS) Solar Extreme-Ultra-Violet Monitor (SEM) Daily Data in CDF Format
The data include daily average raw count rates in Channels 1 - 3 and First Order (26 - 34 nm, average of Ch1 and Ch3) and Central Order (0.1 - 50 nm, Ch2) photon fluxes, as well as SOHO Heliocentric location and distance. This CDF dataset was converted from the original ASCII dataset at the SOHO Archive https://soho.nascom.nasa.gov/data/archive.html. The original ASCII dataset Version 4 Science Product Release Notes are available at https://lasp.colorado.edu/eve/data_access/eve_data/lasp_soho_sem_data/long/LASP_SOHO_SEM_release_notes_v4.pdf. Description of the CELIAS-SEM instrument and scientific scope can befound on the CELIAS home page http://www2.physik.uni-kiel.de/SOHO-CELIAS/ and on the SOHO mission home page https://sohowww.nascom.nasa.gov/. CELIAS Instrument Publication: Hovestadt, D., Hilchenbach, M., Bürgi, A. et al. CELIAS - Charge, Element and Isotope Analysis System for SOHO, Sol Phys 162, 441–481 (1995), https://doi.org/10.1007/BF00733436.
SOHO Charge, Element, and Isotope Analysis System (CELIAS) Solar Extreme-Ultra-Violet Monitor (SEM) 15-second Data in CDF Format
The data include 15-second average raw count rates in Channels 1 - 3 and First Order (26 - 34 nm, average of Ch1 and Ch3) and Central Order (0.1 - 50 nm, Ch2) photon fluxes, as well as SOHO Heliocentric location and distance. This CDF dataset was converted from the original ASCII dataset at the SOHO Archive https://soho.nascom.nasa.gov/data/archive.html. The original ASCII dataset Version 4 science product release notes are available at https://lasp.colorado.edu/eve/data_access/eve_data/lasp_soho_sem_data/long/LASP_SOHO_SEM_release_notes_v4.pdf. Description of the CELIAS-SEM instrument and scientific scope can be found on the CELIAS home page http://www2.physik.uni-kiel.de/SOHO-CELIAS/ and on the SOHO home page https://sohowww.nascom.nasa.gov/. CELIAS Instrument Publication: Hovestadt, D., Hilchenbach, M., Bürgi, A. et al. CELIAS - Charge, Element and Isotope Analysis System for SOHO, Sol Phys 162, 441–481 (1995), https://doi.org/10.1007/BF00733436.
Battery Charge Depletion Prediction on an Electric Aircraft
Validation of prognostic technologies through ground and flight tests is an important step in maturing these novel technologies and deploying them on real-world systems. To this end, a series of flight tests have been conducted using an unmanned electric vehicle during which the motor system batteries were monitored by a prognostic algorithm. The research presented here endeavors to produce and validate a technology for predicting the remaining time until end-ofdischarge of the batteries on an electric aircraft as a function of an expected future flight and online estimates of the charge contained in the batteries. Flight data and flight experiment results are presented along with an assessment of model and algorithm performance
SOHO Charge, Element, and Isotope Analysis System (CELIAS) Proton Monitor (PM) 30-second Solar Wind Data in CDF Format
The data include 30-second proton speed, density, most probable thermal speed, and arrival direction, as well as predicted alpha-particle speed. Also included are the SOHO spacecraft predicted positon in GSE coordinates, Heliocentric Range, Heliographic Latitude and Longitude, and Earth Carrington Rotation Number. This CDF dataset was converted from the original ASCII dataset at the SOHO Archive https://soho.nascom.nasa.gov/data/archive.html. Description of the CELIAS-PM instrument and scientific scope can be found on the CELIAS instrument home page http://www2.physik.uni-kiel.de/SOHO-CELIAS/ and on the SOHO mission home page https://sohowww.nascom.nasa.gov/. CELIAS Instrument Publication: Hovestadt, D., Hilchenbach, M., Bürgi, A. et al. CELIAS - Charge, Element and Isotope Analysis System for SOHO, Sol Phys 162, 441–481 (1995), https://doi.org/10.1007/BF00733436.
ACE Solar Energetic Particle Ionic Charge Analyzer (SEPICA) Energetic Ion Flux Intensities Values and Uncertainties, Level 2 (H2), 1 h Data
This Data Product contains Measurements from the ACE Solar Energetic Particle Ionic Charge Analyzer (SEPICA) Instrument. SEPICA is used to determine the Charge State Distribution of Energetic Particle Distributions. SEPICA is designed to measure the Ionic Charge State, Q, the Kinetic Energy, E, and the Nuclear Charge, Z, of Energetic Ions above 0.2 MeV/n. This includes Ions accelerated in Solar Flares as well as in Interplanetary Space during Energetic Storm Particle (ESP) Events and Co-rotating Interaction Region (CIR) Events. For low Mass Numbers, SEPICA also separates Isotopes such as 3He and 4He. The Quality of the ACE Level 2 Data are such that it is suitable for serious Scientific Study. However, to avoid Confusion and Misunderstanding, it is recommended that Users consult with the appropriate ACE Team Members before publishing Work derived from the Data. The ACE Team has worked hard to ensure that the Level 2 Data are free from Errors, but the Team cannot accept Responsibility for erroneous Data, or for Misunderstandings about how the Data may be used. This is especially true if the appropriate ACE Team Members are not consulted before Publication. At the very least, Preprints should be forwarded to the ACE Team before Publication.
Humanized and Charge-Optimized CSPG4-Specific CAR-T Cells Show Enhanced Efficacy Against Head and Neck Squamous Cell Carcinoma
GEO Series GSE315646. Homo sapiens. 10 samples. Type: Expression profiling by high throughput sequencing.
Role of CRP K100 positive charge on Escherichia coli global transcriptome
GEO Series GSE97406. Escherichia coli. 12 samples. Type: Expression profiling by high throughput sequencing.
Chromatin Remodeler CHD7 mutated in CHARGE Syndrome Interacts with Sox10 to Regulate Timing of CNS Myelination and Remyelination [ChIP-seq]
GEO Series GSE72725. Rattus norvegicus. 2 samples. Type: Genome binding/occupancy profiling by high throughput sequencing.
Charged tRNA profiling of mcf10a, HCC1806 cells, polysome profiling, RNA-Seq and Ribo-Seq in 4T07 cells upon LARS knockdown by shRNA, and RNA-Seq of ribosome-associated RNAs in Lars depleted PyMT tumo
GEO Series GSE176130. Homo sapiens; Mus musculus. 43 samples. Type: Expression profiling by high throughput sequencing; Other.
Dataset Package for the Manuscript "Antiferromagnetic skyrmion lattice order with alternating topological charges"
<p>The attached files include data presented in the respective manuscript. In the filenames "FigureXY...", XY is a placeholder and indicates the figure in that the data are presented.</p> <p>In File "Figure2e.dat", the colorcoding is presented terms of three 57 x 22 (rows x colums) matrices. The first matrix (rows 1-57) present the values for the momentum-transfers, the second matrix (rows 58-115) the values for the temperature, and the last matrix (rows 116-171) the respective values for the neutron diffraction intensity.</p> <p>File "Figure3b.dat" presents the colorcoding, also in terms of three matrices, where the first matrix (rows 1-15001) presents values for magnetic field, the second matrix (rows 15002-30002) values for temperature, and the third matrix (30003-45003) values for the topological Hall effect.</p> <p>"Figure3c_M.dat" and "Figure3c_THE.dat", present data of magnetization and topological Hall effect, respectively. The first column in each file contains field-values and the second column the quantity indicated in the filename.</p> <p>The files "Figure4b....dat" present integrated intensities of neutron diffraction data as a function of field. The filename indicates the respective propagation vector star. In each file, the first column corresponds to magnetic field, the second column to integrated intensity, and the third column to the uncertainty derived from Poisson counting statistics.</p> <p>The colorcoding in file "Figure4dColorcoding.dat" is presented analogously to the previous files. "Figure4dMaxima.dat" contains the locations of Maxima drawn into the figure. The structure of the files for figures 4e, 4f, 4g, 5a, 5b, and 5c is analogous to the previous files.</p> <p>For Figures 5d, 5e, and 5f, the files present spin structures obtained from our theory. The first two colums describe the unit cell of the magnetic Cerium ion in conventional coordinates (the third coordinate is omitted). Colums 3-5, colums 6-8, colums 9-11, and colums 12-14 include the direction of the spins in the layers at coordinates z=0.241, z=1-0.241, z=1+0.241, and z=2-0.241 in cartesian coordinates, respectively.</p> <p>The files *.col present integrated intensities of magnetic Bragg reflections. In these files, the first column corresponds to a numeration, columns 2 - 4 correspond to the Miller Indizes of the respective magnetic Bragg peaks in conventional tetragonal coordinates, column 5 corresponds to the integrated intensity, and column 6 to the uncertainty due to statistical errors.</p> <p>Files "ExportHallEffectXpYK.dat" present Hall effect data from the Supplementary Material. The last positions of the filename indicate the temperature, where data were analyzed. Therein, the first column corresponds to magnetic field, the second column to the transverse Hall resistivity and the last column to the sum of normal Hall effect and anomalous Hall effect that is linear in the field-induced magnetization.</p> <p> </p> <p> </p>
Data files for the publication "Dissecting the hydrogen bond network of water: charge transfer and nuclear quantum effects"
<p>This dataset includes text/dat files for all the data included in the manuscript "Dissecting the hydrogen bond network of water: charge transfer and nuclear quantum effects".</p>
RNA delivery to the corneal endothelium using charge-altering releasable transporters
GEO Series GSE295750. Mus musculus. 16 samples. Type: Expression profiling by high throughput sequencing.
Adaptive Design for Controllability of a System of Electric Vehicle Charging Stations
<p>ADP - Data supporting this research, including supplementary materials.</p>
Data for "A Fast-Charging Study on the Lifetime of Power-Optimized Lithium Titanite Batteries By Electrochemical Impedance Spectroscopy"
Open the record for dataset details and reuse information.
Simulating the impact of charge exchange on beam ions in MAST-U
<p>Dataset used in paper "Simulating the impact of charge exchange on beam ions in MAST-U" to be submitted to PPCF</p>
DHI-DHICA_DIC-charg
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DHI-DHICA-LFX-charg
Open the record for dataset details and reuse information.
DHI-DHICA-OTX-charg
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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.
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DANDI Archive for NWB datasets
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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.