1,164 Works

OMNI, Combined Solar Wind Plasma Moments and Interplanetary Magnetic Field (IMF) Time-Shifted to the Nose of the Earth's Bow Shock, plus Geomagnetic Indices, 1 min Data

Joseph H. King & Natalia E. Papitashvili
Near-Earth Heliospheric Data, OMNI, Definitive Multispacecraft Interplanetary Parameters Data, 1 min averaged Additional information for all parameters are available from OMNI Data Documentation: https://omniweb..sci.gsfc.nasa.gov/html/HROdocum.html New data may be accesible via the Space Physics Data Facility, SPDF, OMNIWeb Service: https://omniweb.sci.gsfc.nasa.gov/ow_min.html The Modified (Level-3) High Resolution OMNI data files are made in the same format as the OMNI files based on SWE Key Parameter data. There are a few differences between old and new high resolution OMNI...

STEREO Solar Energetic Particle List

Jian Lan
This catalog has a list of the Solar Energetic Particles (SEP) Events observed by STEREO-A and/or STEREO-B. For each of the observations, the following information is given: event start time, event end time, STEREO maximum_flux fluence, and a comment. It is expected that this list, given in both PDF and Excel formats, will be updated periodically.

OMNI, Combined Solar Wind Plasma Moments and Interplanetary Magnetic Field (IMF) Time-Shifted to the Nose of the Earth's Bow Shock, plus Geomagnetic Indices, 5 min Data

Joseph H. King & Natalia E. Papitashvili
Near-Earth Heliospheric Data, OMNI, Definitive Multispacecraft Interplanetary Parameters Data, 5 min averaged Additional information for all parameters are available from OMNI Data Documentation: https://omniweb..sci.gsfc.nasa.gov/html/HROdocum.html New data may be accesible via the Space Physics Data Facility, SPDF, OMNIWeb Service: https://omniweb.sci.gsfc.nasa.gov/ow_min.html The Modified (Level-3) High Resolution OMNI data files are made in the same format as the OMNI files based on SWE Key Parameter data. There are a few differences between old and new high resolution OMNI...

OMNI Hourly Data Set

Natalia E. Papitashvili & Joseph H. King
Hourly averaged, multi-source, near-Earth solar wind magnetic field, plasma and energetic proton flux data, plus AE, AU, AL, Kp, ap, and Dst geomagnetic indices, Polar Cap (Thule) index, F10.7 index, and Rz (sunspot number). Also available at 1-day, 27-day, and 1-year resolution.

Interball Tail Wide-range 3D Ion Spectrometer (CORALL) Linearly Interpolated 60 s Resolution data in GSE Coordinates

James Weygand & Robert McPherron
Interball-1 Wide-range 3D Ion Spectrometer (CORALL) linearly interpolated to have the measurements on the minute at 60 s resolution 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...

ISEE-3 Linearly Interpolated 60 s Resolution Solar Wind Plasma data in GSM Coordinates

James Weygand & Robert McPherron
ISEE-3 linearly interpolated to have the measurements on the minute at 60 s resolution solar wind plasma 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...

ISEE 1 Fast Plasma Experiment Solar Wind Weimer Propagated 60 s Resolution Data in GSM Coordinates

James Weygand & Robert McPherron
ISEE-1 Weimer propagated solar wind data and linearly interpolated to have the measurements on the minute at 60 s resolution FPE 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...

ACE Linearly Interpolated 60 s Resolution Tri-axial Fluxgate Magnetometer in GSM Coordinates

James Weygand & Robert McPherron
ACE linearly interpolated to have the measurements on the minute at 60 s resolution tri-axial fluxgate magnetometer 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...

IMP-8 Linearly Interpolated 60 s Resolution Tri-axial Fluxgate Magnetometer in GSE Coordinates

Ronald Lepping
IMP-8 linearly interpolated to have the measurements on the minute at 60 s resolution tri-axial fluxgate magnetometer 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...

ACE Linearly Interpolated 60 s Resolution SWEPAM data in GSM Coordinates

David McComas
ACE linearly interpolated to have the measurements on the minute at 60 s resolution SWEPAM 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...

IMP-8 Weimer Propagated 60 s Resolution Tri-axial Fluxgate Magnetometer in GSM Coordinates

James Weygand & Robert McPherron
IMP-8 Weimer propagated solar wind data and linearly interpolated to have the measurements on the minute at 60 s resolution Tri-axial fluxgate magnetometer 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...

IMP-8 PLS Solar Wind Weimer Propagated 60 s Resolution Data in GSM Coordinates

James Weygand & Robert McPherron
IMP-8 PLS Weimer 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...

ISEE-3 Linearly Interpolated 60 s Resolution Tri-axial Fluxgate Magnetometer in GSE Coordinates

James Weygand & Robert McPherron
ISEE-3 linearly interpolated to have the measurements on the minute at 60 s resolution tri-axial fluxgate magnetometer 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...

ISEE-3 Linearly Interpolated 60 s Resolution Tri-axial Fluxgate Magnetometer in GSM Coordinates

James Weygand & Robert McPherron
ISEE-3 linearly interpolated to have the measurements on the minute at 60 s resolution tri-axial fluxgate magnetometer 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...

PSP Solar Wind Electrons Alphas and Protons (SWEAP) SPAN-B Full 3D Electron Spectra, Level 2 (L2), 14 s Data publisher = NASA Space Physics Data Facility

Phyllis Whittlesey, Davin E. Larson & Ali Rahmati
The SF0 products are the Full 3D Electron spectra from each individual SPAN-E instrument, SPAN-Ae and SPAN-B. Units are in differential energy flux, degrees, and eV. One spectrum comprises decreasing steps in Energy specified by the number in the filename, alternating sweeps in Theta/Deflection, also specified by the number in the filename, and a number of Phi/Anode directions, also specified by the number in the filename. The sample filename above includes 16 Anodes, 8 Deflections,...

PSP Solar Wind Electrons Alphas and Protons (SWEAP) SPAN-A Proton Distribution Function, Partial Moments, Instrument Frame, Level 3 (L3), 7 s Data

Roberto Livi, Davin E. Larson & Ali Rahmati
This data product contains measurements of partial moments of the proton distribution function in the instrument frame of reference. Users should be aware that the full ion distribution is typically not in the field of view, FOV, of the SPAN Ion instrument.

Wind Energetic Particle Acceleration, Composition and Transport (EPACT) APE-B Telescope Proton Fluxes 18.90 to 21.90 MeV, Level 2, 1 hr Data

Tycho T. Von Rosenvinge & Donald V. Reames
The Energetic Particles: Acceleration, Composition and Transport, EPACT, on Wind. The APE-B Telescope measures Proton Fluxes at Particle Energies of 18.90 MeV to 21.90 MeV.

Wind 3DP Plasma data at UCB

Robert P. Lin & Stuart D. Bale
Wind 3DP thermal and energetic ion and electron distributions and moments.

Wind Definitive Orbit, 10 min Data, Spacecraft Position and Velocity in GCI, GSE, GSM, HEC, and HG Coordinates

Robert M. Candey &
Wind Definitive Orbit, Spacecraft Position and Velocity in Geocentric Celestial Inertial, GCI, Geocentric Solar Ecliptic, GSE, Geocentric Solar Magnetospheric, GSM, Heliospheric Ecliptic, HEC, and Heliographic, HG, Coordinates.

Wind Predicted Attitude, 10 min Data, Spin Axis Orientation Angles in GCI, GSE and GSM Coordinates

Robert Candey &
Wind Predicted Attitude Body Spin Rate and Spin Axis Orientation Right Ascension and Declination Angles in Geocentric Celestial Inertial, GCI, Geocentric Solar Ecliptic, GSE, and Geocentric Solar Magnetospheric, GSE, Coordinates.

Wind Plasma and Radio Waves (WAVES) Time Domain Sampler (TDS) Dust Impact, Level 3, 1 s Data

David M. Malaspina, Lynn B. Wilson III, Keith Goetz & Robert J. Macdowall
Wind WAVES Time Domain Sampler, TDS.

PSP Solar Wind Electrons Alphas and Protons (SWEAP) SPAN-A Alpha Particle Distribution Function, Partial Moments, Instrument Frame, Level 3 (L3), 14 s Data

Roberto Livi, Davin E. Larson & Ali Rahmati
This data product contains measurements of partial moments of the alpha particle distribution function in the instrument frame of reference. Users should be aware that the full ion distribution is typicaly not in the field of view, FOV, of the SPAN Ion instrument.

PSP FIELDS Digital Fields Board (DFB) AC-coupled Differential Voltage, V3-V4 Antennae, Dipole Mode, Bandpass filtered, High Gain, Sensor coordinates, Level 2 (L2), 0.873813 s Data

Stuart D. Bale, David M. Malaspina, Alexandros Chasapis, Marc Pulupa, Timothy Quinn & Peter Schroeder
PSP FIELDS Digital Fields Board, DFB, dV34 data. The DFB is the low frequency, less than 75 kHz, component of the FIELDS experiment on the Parker Solar Probe spacecraft. DFB AC bandpass data consist of peak and average values of the absolute value of bandpassed time series waveform data over a time interval equal to the reporting cadence. The AC bandpass data have the peak response frequency of each bin reported in the metadata. The...

Parker Solar Probe, FIELDS Radio Frequency Spectrometer, RFS, High Frequency Receiver, HFR, Spectra, Level 2 (L2), 7 s and 56 s Data

Stuart D. Bale
Parker Solar Probe Electromagnetic Fields Investigation (FIELDS) Radio Frequency Spectrometer, RFS, High Frequency Receiver, HFR, Data: The RFS is the high frequency component of the FIELDS experiment on the Parker Solar Probe spacecraft, see reference [1]. For a full description of the FIELDS experiment, see reference [2]. For a description of the RFS, see reference [3]. The RFS produces auto and cross spectral data products in two frequency ranges, the Low Frequency Reciever (LFR) range...

Wind 3DP Electron Plasma Moments

Robert P. Lin, Stuart D. Bale & Lynn B. Wilson III
Electron Plasma moments (computed on-board) (NOT CORRECTED FOR S/C POTENTIAL) @ 3 second (spin) resolution (version 3), EESA LOW, Wind 3DP.

Registration Year

  • 2022
    939
  • 2021
    136
  • 2020
    15
  • 2019
    68
  • 2018
    6

Resource Types

  • Dataset
    1,161
  • Model
    1
  • Standard
    1
  • Text
    1

Affiliations

  • //ror.org/03tghng59:Southwest Research Institute
    168
  • //ror.org/01fcjzv38:Laboratory for Atmospheric and Space Physics
    69
  • //ror.org/036jqmy94:University of Iowa
    55
  • //ror.org/0171mag52:Goddard Space Flight Center
    48
  • University of California, Berkeley
    42
  • //ror.org/01rmh9n78:University of New Hampshire
    37
  • //ror.org/01e41cf67:Los Alamos National Laboratory
    36
  • //ror.org/026vcq606:Kungliga Tekniska Högskolan
    32
  • Laboratory for Atmospheric and Space Physics
    30
  • //ror.org/017zqws13:University of Minnesota
    28