cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.48322/rd95-b956
title: Voyager 2 Plasma Data Daily Resolution

description: Daily averages of Voyager 2 Plasma Data. The plasma investigation made use of two Faraday-cup detectors, one pointed along the earth-spacecraft line and one at right angles to this line. The earth-pointing detector determined the macroscopic properties of the plasma ions, obtaining accurate values of their velocity, density, and pressure. Three sequential energy scans were employed with (delta E)/E equal to 29, 7.2, and 1.8%, allowing a coverage from subsonic to highly supersonic flow. The side-looking Faraday cup measured electrons in the energy range from 5eV to 1 keV.
DOI: 10.22008/fk2/iw73uu/ldyzbq
title: HUM_hour.nc

description: Uploaded with pyDataverse 2024-04-10 23:44
DOI: 10.48322/ps5q-aw33
title: Voyager 2 High Resolution Plasma Data

description: The plasma investigation made use of two Faraday-cup detectors, one pointed along the earth-spacecraft line and one at right angles to this line. The earth-pointing detector determined the macroscopic properties of the plasma ions, obtaining accurate values of their velocity, density, and pressure. Three sequential energy scans were employed with (delta E)/E equal to 20, 7.2, and 1.8%, allowing a coverage from subsonic to highly supersonic flow. The side-looking Faraday cup measured electrons in the energy range from 5 eV to 1 keV. The plasma parameters are obtained by finding the best fit of a convected isotropic Maxwellian distribution to the data. One sigma errors are typically less than 0.5% in the speed and VR, less than 5% for the density and thermal speed, and vary greatly for VT and VN. Sampling times range from 12 to 192 sec., with sampling generally more frequent early in the mission. The velocity components are given in the RTN coordinate system, where R is radially outward, T is in a plane parallel to the solar equatorial plane and positive in the direction of solar rotation, and N completes a right-handed system.
DOI: 10.22008/fk2/iw73uu/7yfgzu
title: HUM_day.nc

description: Uploaded with pyDataverse 2024-04-10 23:44
DOI: 10.48322/4fwp-cw56
title: Voyager 2 Hourly Averaged Plasma Data

description: The plasma investigation made use of two Faraday-cup detectors, one pointed along the earth-spacecraft line and one at right angles to this line. The earth-pointing detector determined the macroscopic properties of the plasma ions, obtaining accurate values of their velocity, density, and pressure. Three sequential energy scans were employed with (delta E)/E equal to 20, 7.2, and 1.8%, allowing a coverage from subsonic to highly supersonic flow. The side-looking Faraday cup measured electrons in the energy range from 5 eV to 1 keV. The plasma parameters are obtained by finding the best fit of a convected isotropic Maxwellian distribution to the data. One sigma errors are typically less than 0.5% in the speed and VR, less than 5% for the density and thermal speed, and vary greatly for VT and VN. Sampling times range from 12 to 192 sec., with sampling generally more frequent early in the mission. One hour averages were produced from these samples. The velocity components are given in the RTN coordinate system, where R is radially outward, T is in a plane parallel to the solar equatorial plane and positive in the direction of solar rotation, and N completes a right-handed system.
DOI: 10.22008/fk2/iw73uu/8cbzob
title: HUM_month.nc

description: Uploaded with pyDataverse 2024-04-10 23:44
DOI: 10.22008/fk2/iw73uu/mrnnvu
title: JAR_day.csv

description: Uploaded with pyDataverse 2024-04-10 23:44
DOI: 10.48322/rtt8-v976
title: Voyager 2 PWS hr-avgd and peak plasma wave data

description: Hourly averages and peaks of calibrated electric field spectrum analyzer data from Voyager 2 PWS instrument
DOI: 10.22008/fk2/iw73uu/mrs6gc
title: JAR_hour.csv

description: Uploaded with pyDataverse 2024-04-10 23:44
DOI: 10.48322/34kg-ew57
title: Wind SWE Linearly Interpolated 60 s Resolution data in GSE Coordinates
title: Wind SWE data

description: Wind linearly interpolated to have the measurements on the minute at 60 s resolution SWE data in GSE coordinates. This data set consists of processed solar wind data that has been linearly interpolated to 1 min resolution at the position of the spacecraft using the interp1.m function in MATLAB.  This data set was originally constructed by Dr. J.M. Weygand for Prof. R.L. McPherron, who was the principle investigator of two National Science Foundation studies: GEM Grant ATM 02-1798 and a Space Weather Grant ATM 02-08501. These data were primarily used in superposed epoch studies and cross correlation studies on solar wind.
DOI: 10.48322/xzhy-d247
title: Voyager 2 PWS full resolution plasma wave data

description: Full resolution plasma wave spectrum analyzer data from Voyager 2 PWS instrument
DOI: 10.22008/fk2/iw73uu/fevrcp
title: JAR_month.csv

description: Uploaded with pyDataverse 2024-04-10 23:44
DOI: 10.48322/y111-kc38
title: Wind SWE Linearly Interpolated 60 s Resolution data in GSM Coordinates
title: Wind SWE data

description: Wind linearly interpolated to have the measurements on the minute at 60 s resolution SWE data in GSM coordinates. This data set consists of processed solar wind data that has been linearly interpolated to 1 min resolution at the position of the spacecraft using the interp1.m function in MATLAB.  This data set was originally constructed by Dr. J.M. Weygand for Prof. R.L. McPherron, who was the principle investigator of two National Science Foundation studies: GEM Grant ATM 02-1798 and a Space Weather Grant ATM 02-08501. These data were primarily used in superposed epoch studies and cross correlation studies on solar wind.
DOI: 10.22008/fk2/iw73uu/cwzdjh
title: JAR_hour.nc

description: Uploaded with pyDataverse 2024-04-10 23:44
DOI: 10.22008/fk2/iw73uu/xjj0ps
title: JAR_day.nc

description: Uploaded with pyDataverse 2024-04-10 23:45
DOI: 10.48322/8qja-p367
title: Wind SWE Weimer Propagated 60 s Resolution data in GSE Coordinates
title: Wind SWE data

description: Wind SWE propagated solar wind data and linearly interpolated to have the measurements on the minute at 60 s resolution data in GSE coordinates. This data set consists of propagated solar wind data that has first been propagated to a position just outside of the nominal bow shock (about 17, 0, 0 Re) and then linearly interpolated to 1 min resolution using the interp1.m function in MATLAB. The input data for this data set is a 1 min resolution processed solar wind data constructed by Dr. J.M. Weygand. The method of propagation is similar to the minimum variance technique and is outlined in Dan Weimer et al. [2003; 2004]. The basic method is to find the minimum variance direction of the magnetic field in the plane orthogonal to the mean magnetic field direction. This minimum variance direction is then dotted with the difference between final position vector minus the original position vector and the quantity is divided by the minimum variance dotted with the solar wind velocity vector, which gives the propagation time. This method does not work well for shocks and minimum variance directions with tilts greater than 70 degrees of the sun-earth line.   This data set was originally constructed by Dr. J.M. Weygand for Prof. R.L. McPherron, who was the principle investigator of two National Science Foundation studies: GEM Grant ATM 02-1798 and a Space Weather Grant ATM 02-08501. These data were primarily used in superposed epoch studies References: Weimer, D. R. (2004), Correction to ‘‘Predicting interplanetary magnetic field (IMF) propagation delay times using the minimum variance technique,’’ J. Geophys. Res., 109, A12104, doi:10.1029/2004JA010691. Weimer, D.R., D.M. Ober, N.C. Maynard, M.R. Collier, D.J. McComas,  N.F. Ness, C. W. Smith, and J. Watermann (2003), Predicting interplanetary magnetic field (IMF) propagation delay times using the minimum variance technique, J. Geophys. Res., 108, 1026, doi:10.1029/2002JA009405.
DOI: 10.22008/fk2/iw73uu/ucdo3z
title: JAR_month.nc

description: Uploaded with pyDataverse 2024-04-10 23:45
DOI: 10.48322/byad-w608
title: Wind SWE Weimer Propagated 60 s Resolution data in GSM Coordinates
title: Wind SWE data

description: Wind SWE propagated solar wind data and linearly interpolated to have the measurements on the minute at 60 s resolution data in GSM coordinates. This data set consists of propagated solar wind data that has first been propagated to a position just outside of the nominal bow shock (about 17, 0, 0 Re) and then linearly interpolated to 1 min resolution using the interp1.m function in MATLAB. The input data for this data set is a 1 min resolution processed solar wind data constructed by Dr. J.M. Weygand. The method of propagation is similar to the minimum variance technique and is outlined in Dan Weimer et al. [2003; 2004]. The basic method is to find the minimum variance direction of the magnetic field in the plane orthogonal to the mean magnetic field direction. This minimum variance direction is then dotted with the difference between final position vector minus the original position vector and the quantity is divided by the minimum variance dotted with the solar wind velocity vector, which gives the propagation time. This method does not work well for shocks and minimum variance directions with tilts greater than 70 degrees of the sun-earth line.   This data set was originally constructed by Dr. J.M. Weygand for Prof. R.L. McPherron, who was the principle investigator of two National Science Foundation studies: GEM Grant ATM 02-1798 and a Space Weather Grant ATM 02-08501. These data were primarily used in superposed epoch studies References: Weimer, D. R. (2004), Correction to ‘‘Predicting interplanetary magnetic field (IMF) propagation delay times using the minimum variance technique,’’ J. Geophys. Res., 109, A12104, doi:10.1029/2004JA010691. Weimer, D.R., D.M. Ober, N.C. Maynard, M.R. Collier, D.J. McComas,  N.F. Ness, C. W. Smith, and J. Watermann (2003), Predicting interplanetary magnetic field (IMF) propagation delay times using the minimum variance technique, J. Geophys. Res., 108, 1026, doi:10.1029/2002JA009405.
DOI: 10.22008/fk2/iw73uu/84hqld
title: JAR_O_day.csv

description: Uploaded with pyDataverse 2024-04-10 23:45
DOI: 10.48322/41h6-gw79
title: Wind Energetic Particle Acceleration, Composition and Transport (EPACT)/LEMT 1-Hr Spin-Sectored H,He,O,Fe Counts for Events

description: This data set contains hourly counts of H, He, O 
and Fe nuclei in 16 look directions about the spacecraft spin axis.  
Counts for each of the four species are given at 2.5-5 MeV/n, and an 
additional count is given for 5-8 MeV/n He.  As of 10/2011, the data 
cover 39 1997-2006 multi-day intervals that include energetic solar 
particle events.  ASCII data words are comma-separated.  For a given 
particle event, there are species-specific files.  File naming uses 
the convention XX_sec_YYYYMMDD, where XX = H, He2 (2.5-5 MeV/n), 
He5 (5-8 MeV/n), O or Fe, and where YYYYMMDD is the day of the first 
record of the file.  Sectoring is defined with respect to the 
ecliptic plane projection of the concurrently measured magnetic
field vector.  The edge of sector #1 is coincided with the projection 
of B on the ecliptic plane, so phi value of the center of sector i 
is phiB+11.25+(i-1)*22.5 deg, where phiB is the longitudinal angle 
of B.
DOI: 10.48322/kc69-5m68
title: Wind SMS Suite, SupraThermal Ion Composition Spectrometer (SMS/STICS) Alpha Particle Distribution Function and Differential Flux, Magnetosphere, Level 2 (L2), PT3M Data

description: The Suprathermal Ion Composition Spectrometer (STICS) is a Time of Flight (TOF) Plasma Mass Spectrometer, capable of identifying Mass and Mass per Charge for incident Ions up to 200 keV/q. It uses an Electrostatic Analyzer to admit Ions of a particular Energy per Charge (E/Q) into the TOF Chamber. The E/Q Voltage is stepped through 32 Values, sitting at each Value for approximately 24 s, to measure Ions over the full E/Q Range of 6 keV/q to 200 keV/q. Ions then pass through a Carbon Foil and TOF Chamber, before finally impacting on a Solid-State Detector (SSD) for Energy Measurement. STICS combines these three Measurements of E/Q, TOF and Residual Energy, producing PHA Words. This Triple-Coincidence Technique greatly improves the Signal to Noise Ratio in the Data. Measurements of E/Q and TOF without Residual Energy also produce PHA Words. These Double-Coincidence Measurements are characterized by better Statistics since Ions whose Energy does not allow them to be registered by the SSD can still be counted in Double-Coincidence Measurements. However, Ion Identification in Double-Coincidence Measurements are limited to a select Number of Ions that are well separated in E/Q - TOF Space. The STICS Instrument provides full 3D Velocity Distribution Functions, through a Combination of multiple Telescopes and Spacecraft Spin. The Instrument includes three separate TOF Telescopes that view three separate Latitude Sectors, as shown in Figure 1. In addition, the WIND Spacecraft Spins, allowing the three Telescopes to trace out a nearly 4π sr Viewing Area. The Longitudinal Sectors are shown in Figure 2. The Solar Direction is in Sectors 8-10 while the Earthward Direction is in Sectors 0-2.
DOI: 10.22008/fk2/iw73uu/dycg3q
title: JAR_O_hour.csv

description: Uploaded with pyDataverse 2024-04-10 23:45
DOI: 10.48322/qvy6-sk75
title: Wind SMS Suite, SupraThermal Ion Composition Spectrometer (SMS/STICS) Proton Distribution Function and Differential Flux, Magnetosphere, Level 2 (L2), PT3M Data

description: The Suprathermal Ion Composition Spectrometer (STICS) is a Time of Flight (TOF) Plasma Mass Spectrometer, capable of identifying Mass and Mass per Charge for incident Ions up to 200 keV/q. It uses an Electrostatic Analyzer to admit Ions of a particular Energy per Charge (E/Q) into the TOF Chamber. The E/Q Voltage is stepped through 32 Values, sitting at each Value for approximately 24 s, to measure Ions over the full E/Q Range of 6 keV/q to 200 keV/q. Ions then pass through a Carbon Foil and TOF Chamber, before finally impacting on a Solid-State Detector (SSD) for Energy Measurement. STICS combines these three Measurements of E/Q, TOF and Residual Energy, producing PHA Words. This Triple-Coincidence Technique greatly improves the Signal to Noise Ratio in the Data. Measurements of E/Q and TOF without Residual Energy also produce PHA Words. These Double-Coincidence Measurements are characterized by better Statistics since Ions whose Energy does not allow them to be registered by the SSD can still be counted in Double-Coincidence Measurements. However, Ion Identification in Double-Coincidence Measurements are limited to a select Number of Ions that are well separated in E/Q - TOF Space. The STICS Instrument provides full 3D Velocity Distribution Functions, through a Combination of multiple Telescopes and Spacecraft Spin. The Instrument includes three separate TOF Telescopes that view three separate Latitude Sectors, as shown in Figure 1. In addition, the WIND Spacecraft Spins, allowing the three Telescopes to trace out a nearly 4π sr Viewing Area. The Longitudinal Sectors are shown in Figure 2. The Solar Direction is in Sectors 8-10 while the Earthward Direction is in Sectors 0-2.
DOI: 10.22008/fk2/iw73uu/i9mptw
title: JAR_O_month.csv

description: Uploaded with pyDataverse 2024-04-10 23:45
DOI: 10.48322/vjrr-br96
title: Wind SMS Suite, SupraThermal Ion Composition Spectrometer (SMS/STICS) Alpha Particle Distribution Function and Differential Flux, Solar Wind, Level 2 (L2), PT3M Data

description: The Suprathermal Ion Composition Spectrometer (STICS) is a Time of Flight (TOF) Plasma Mass Spectrometer, capable of identifying Mass and Mass per Charge for incident Ions up to 200 keV/q. It uses an Electrostatic Analyzer to admit Ions of a particular Energy per Charge (E/Q) into the TOF Chamber. The E/Q Voltage is stepped through 32 Values, sitting at each Value for approximately 24 s, to measure Ions over the full E/Q Range of 6 keV/q to 200 keV/q. Ions then pass through a Carbon Foil and TOF Chamber, before finally impacting on a Solid-State Detector (SSD) for Energy Measurement. STICS combines these three Measurements of E/Q, TOF and Residual Energy, producing PHA Words. This Triple-Coincidence Technique greatly improves the Signal to Noise Ratio in the Data. Measurements of E/Q and TOF without Residual Energy also produce PHA Words. These Double-Coincidence Measurements are characterized by better Statistics since Ions whose Energy does not allow them to be registered by the SSD can still be counted in Double-Coincidence Measurements. However, Ion Identification in Double-Coincidence Measurements are limited to a select Number of Ions that are well separated in E/Q - TOF Space. The STICS Instrument provides full 3D Velocity Distribution Functions, through a Combination of multiple Telescopes and Spacecraft Spin. The Instrument includes three separate TOF Telescopes that view three separate Latitude Sectors, as shown in Figure 1. In addition, the WIND Spacecraft Spins, allowing the three Telescopes to trace out a nearly 4π sr Viewing Area. The Longitudinal Sectors are shown in Figure 2. The Solar Direction is in Sectors 8-10 while the Earthward Direction is in Sectors 0-2.
DOI: 10.22008/fk2/iw73uu/cl9oba
title: JAR_O_hour.nc

description: Uploaded with pyDataverse 2024-04-10 23:45
DOI: 10.48322/97ws-6x26
title: Wind SMS Suite, SupraThermal Ion Composition Spectrometer (SMS/STICS) Proton Distribution Function and Differential Flux, Solar Wind, Level 2 (L2), PT3M Data

description: The Suprathermal Ion Composition Spectrometer (STICS) is a Time of Flight (TOF) Plasma Mass Spectrometer, capable of identifying Mass and Mass per Charge for incident Ions up to 200 keV/q. It uses an Electrostatic Analyzer to admit Ions of a particular Energy per Charge (E/Q) into the TOF Chamber. The E/Q Voltage is stepped through 32 Values, sitting at each Value for approximately 24 s, to measure Ions over the full E/Q Range of 6 keV/q to 200 keV/q. Ions then pass through a Carbon Foil and TOF Chamber, before finally impacting on a Solid-State Detector (SSD) for Energy Measurement. STICS combines these three Measurements of E/Q, TOF and Residual Energy, producing PHA Words. This Triple-Coincidence Technique greatly improves the Signal to Noise Ratio in the Data. Measurements of E/Q and TOF without Residual Energy also produce PHA Words. These Double-Coincidence Measurements are characterized by better Statistics since Ions whose Energy does not allow them to be registered by the SSD can still be counted in Double-Coincidence Measurements. However, Ion Identification in Double-Coincidence Measurements are limited to a select Number of Ions that are well separated in E/Q - TOF Space. The STICS Instrument provides full 3D Velocity Distribution Functions, through a Combination of multiple Telescopes and Spacecraft Spin. The Instrument includes three separate TOF Telescopes that view three separate Latitude Sectors, as shown in Figure 1. In addition, the WIND Spacecraft Spins, allowing the three Telescopes to trace out a nearly 4π sr Viewing Area. The Longitudinal Sectors are shown in Figure 2. The Solar Direction is in Sectors 8-10 while the Earthward Direction is in Sectors 0-2.
DOI: 10.22008/fk2/iw73uu/3fkbpf
title: JAR_O_month.nc

description: Uploaded with pyDataverse 2024-04-10 23:45
DOI: 10.22008/fk2/iw73uu/8h1jxv
title: JAR_O_day.nc

description: Uploaded with pyDataverse 2024-04-10 23:45
DOI: 10.22008/fk2/iw73uu/of3l10
title: KAN_B_day.csv

description: Uploaded with pyDataverse 2024-04-10 23:46
DOI: 10.22008/fk2/iw73uu/2i1ur7
title: KAN_B_hour.csv

description: Uploaded with pyDataverse 2024-04-10 23:46
DOI: 10.22008/fk2/iw73uu/jtm64n
title: KAN_B_month.csv

description: Uploaded with pyDataverse 2024-04-10 23:46
DOI: 10.5517/cc9p7mt
title: CCDC 288536: Experimental Crystal Structure Determination

description: Related Article: W.Petz, C.Kutschera, B.Neumuller|2005|Organometallics|24|5038|doi:10.1021/om0580248
description: An entry from the Cambridge Structural Database, the world’s repository for small molecule crystal structures. The entry contains experimental data from a crystal diffraction study. The deposited dataset for this entry is freely available from the CCDC and typically includes 3D coordinates, cell parameters, space group, experimental conditions and quality measures.
DOI: 10.5517/cc9pggw
title: CCDC 288748: Experimental Crystal Structure Determination

description: Related Article: L.Dobrzanska, G.O.Lloyd, H.G.Raubenheimer, L.J.Barbour|2005|J.Am.Chem.Soc.|127|13134|doi:10.1021/ja054119p
description: An entry from the Cambridge Structural Database, the world’s repository for small molecule crystal structures. The entry contains experimental data from a crystal diffraction study. The deposited dataset for this entry is freely available from the CCDC and typically includes 3D coordinates, cell parameters, space group, experimental conditions and quality measures.
DOI: 10.5517/cc9phxc
title: CCDC 288793: Experimental Crystal Structure Determination

description: Related Article: M.E.Gonzalez-Nunez, J.Royo, R.Mello, M.Baguena, J.M.Ferrer, C.R.de Arellano, G.Asensio, G.K.S.Prakash|2005|J.Org.Chem.|70|7919|doi:10.1021/jo0509511
description: An entry from the Cambridge Structural Database, the world’s repository for small molecule crystal structures. The entry contains experimental data from a crystal diffraction study. The deposited dataset for this entry is freely available from the CCDC and typically includes 3D coordinates, cell parameters, space group, experimental conditions and quality measures.
DOI: 10.5517/cc8x1dl
title: CCDC 265279: Experimental Crystal Structure Determination

description: Related Article: A.Bialonska, Z.Ciunik|2005|J.Mol.Struct.|779|38|doi:10.1016/j.molstruc.2005.07.007
description: An entry from the Cambridge Structural Database, the world’s repository for small molecule crystal structures. The entry contains experimental data from a crystal diffraction study. The deposited dataset for this entry is freely available from the CCDC and typically includes 3D coordinates, cell parameters, space group, experimental conditions and quality measures.
DOI: 10.5517/cc9pj0h
title: CCDC 288796: Experimental Crystal Structure Determination

description: Related Article: M.E.Gonzalez-Nunez, J.Royo, R.Mello, M.Baguena, J.M.Ferrer, C.R.de Arellano, G.Asensio, G.K.S.Prakash|2005|J.Org.Chem.|70|7919|doi:10.1021/jo0509511
description: An entry from the Cambridge Structural Database, the world’s repository for small molecule crystal structures. The entry contains experimental data from a crystal diffraction study. The deposited dataset for this entry is freely available from the CCDC and typically includes 3D coordinates, cell parameters, space group, experimental conditions and quality measures.
DOI: 10.5517/cc8x14b
title: CCDC 265271: Experimental Crystal Structure Determination

description: Related Article: M.A.Omary, M.A.Rawashdeh-Omary, M.W.A.Gonser, O.Elbjeirami, T.Grimes, T.R.Cundari, H.V.K.Diyabalanage, C.S.P.Gamage, H.V.R.Dias|2005|Inorg.Chem.|44|8200|doi:10.1021/ic0508730
description: An entry from the Cambridge Structural Database, the world’s repository for small molecule crystal structures. The entry contains experimental data from a crystal diffraction study. The deposited dataset for this entry is freely available from the CCDC and typically includes 3D coordinates, cell parameters, space group, experimental conditions and quality measures.
DOI: 10.5517/cc91z2c
title: CCDC 270012: Experimental Crystal Structure Determination

description: Related Article: K.M.Sureshan, Y.Watanabe|2005|Carbohydr.Res.|340|2311|doi:10.1016/j.carres.2005.07.015
description: An entry from the Cambridge Structural Database, the world’s repository for small molecule crystal structures. The entry contains experimental data from a crystal diffraction study. The deposited dataset for this entry is freely available from the CCDC and typically includes 3D coordinates, cell parameters, space group, experimental conditions and quality measures.