This data set contains ULYSSES GSE position and velocity at 1 min resolution.

This data set contains MMS-1 SCM L1A calibration waveform. The SCM calibration is executed at least once per orbit. The calibration signal sweep is broken into 4 segments with increasing sample frequencies and the whole calibration sequence lasts less than 90 sec. The frequency of the calibration signal doubles every 4 cycles from 0.125 Hz to 4096 Hz. Each segment consist of four different frequencies.

This data set contains MMS-2 SCM uncalibrated AC magnetic field waveforms (in telemetry unit) and in the sensor frame. The data in the (spinning at 20 s) sensor frame are sampled at (survey scsrvy=32 S/s, brst scb=8192 S/s, schb=16384 S/s). For this case of commissioning data, the sample frequency can be different from the nominal modes, and is indicated in the name of the CDF files (example mms1_scm_comm_l1a_sc128_20150316_v1.1.0.cdf where the frequency corresponds to 128 Hz...

This data set contains MMS-1 SCM uncalibrated AC magnetic field waveforms (in telemetry unit) in high speed burst mode and in the sensor frame. These raw uncalibrated (telemetry units) AC magnetic field waveform data in the (spinning at 20 s) sensor frame are sampled at (survey scsrvy=32 samples/s, brst scb=8192 samples/s, schb=16384 samples/s).

This dataset provides the full ion distribution functions at the FAST cadence (4.5 s). The data is provided in units of phase space density. The reference frame is related to the instrument frame, and is called near-GSE. For more information on the FPI instruments, data set, and user guide, please see: MMS Science Data Center (https://lasp.colorado.edu/mms/sdc/public/datasets/fpi/) MMS FPI Data Users and Products Guide (https://lasp.colorado.edu/galaxy/display/MFDPG/MMS+FPI+Data+Users+and+Products+Guide) FPI Release Notes (https://lasp.colorado.edu/mms/sdc/public/datasets/fpi/mms-FPIReleaseNotes-220217.pdf)

This dataset provides the full ion distribution functions at the BURST cadence (150 ms). The data is provided in units of phase space density. The reference frame is related to the instrument frame, and is called near-GSE. For more information on the FPI instruments, data set, and user guide, please see: MMS Science Data Center (https://lasp.colorado.edu/mms/sdc/public/datasets/fpi/) MMS FPI Data Users and Products Guide (https://lasp.colorado.edu/galaxy/display/MFDPG/MMS+FPI+Data+Users+and+Products+Guide) FPI Release Notes (https://lasp.colorado.edu/mms/sdc/public/datasets/fpi/mms-FPIReleaseNotes-220217.pdf)

This data set contains MMS-2 SCM uncalibrated AC magnetic field waveforms (in telemetry unit) in burst mode and in the sensor frame. These raw uncalibrated (telemetry units) AC magnetic field waveform data in the (spinning at 20 s) sensor frame are sampled at (survey scsrvy=32 samples/s, brst scb=8192 samples/s, schb=16384 samples/s).

This data set contains auto-correlation functions (ACF) from the Tromso UHF Radar, reprocessed with french TAPANAL code.

This data sets contains MMS-1 SCM (search coil magnetometer) calibrated AC magnetic field waveforms in the survey mode and GSE frame. These waveform data are sampled at (survey scsrvy=32 samples/s, brst scb=8192 samples/s, schb=16384 samples/s). They are high-pass filtered above (scsrvy = 0.5 Hz, scb = 1 Hz, schb = 32 Hz) but not low-pass filtered.

MMS-2 SCM high-speed burst quicklooks [32-8192Hz] shows from top to bottom : color coded data quality, waveforms (nT), power spectral densities (nT^2/Hz), integrated power (nT^2), time-averaged (over the burst time period) Fourier spectra (nT^2/Hz) with SCM ground noise level (in black) for reference. All data are plotted in GSE.

MMS-1 SCM survey quicklooks [0.0625-16Hz] shows from top to bottom : color coded data quality, waveforms (nT), power spectral densities (nT^2/Hz), integrated power (nT^2), time-averaged (over the 6 hours) Fourier spectra (nT^2/Hz) with SCM ground noise level (in black) for reference. All data are plotted in GSE.

MMS-1 SCM burst quicklooks [1-4096Hz] shows from top to bottom : color coded data quality, waveforms (nT), power spectral densities (nT^2/Hz), integrated power (nT^2), time-averaged (over the burst time period) Fourier spectra (nT^2/Hz) with SCM ground noise level (in black) for reference. All data are plotted in GSE.

MMS-4 SCM burst quicklooks [1-4096Hz] shows from top to bottom : color coded data quality, waveforms (nT), power spectral densities (nT^2/Hz), integrated power (nT^2), time-averaged (over the burst time period) Fourier spectra (nT^2/Hz) with SCM ground noise level (in black) for reference. All data are plotted in GSE.

This data set contains Wind Waves RAD2, RAD1, and TNR 24h dynamic spectrogram plots with frequency in kHz on the vertical axis and time in UT on the horizontal axis. These plots present the WIND WAVES radio data in the whole nominal range of frequencies, from 4 kHz to 13.825 MHz. They are produced from the 60-s averaged data

This data set contains plots of summary and power spectra of local and solar noise as 3-min averages in the frequency range 4kHz - 14 MHz, as one file/day.Plots are in GIF format.

This data set contains electron energy flux issued from the Channel 1 ELEC-1 instrument of the Interball Auroral probe (mode 64 spectra).

This data set contains the GSE position and velocity at 1 min resolution of Interball-Auroral

This data set contains time profile parameters for ions from the 1st (1P) telescope of the DOK-2 instrument on board Interball-Tail. Three time profile parameters (total particle intensities) TP1, TP2 and TP3 were measured in 3 narrow energy intervals. Detector 1P was directed at 180° to the satellite spin axis.

This data set contains the moments of the ion distribution function from the Interball-Tail-CORALL instrument. Nearly 3D ion distribution function (without mass separation) is obtained once per spacecraft spin period (about 118 s). Distribution function moments are calculated under assumption that all particles are protons.

This data set contains ions raw count rates from the Interball-Tail-CORALL instrument. The CORALL instrument uses five sensors (microchannel plates - MCPs) corresponding to five instrument polar sectors (channels). The MCPs efficiencies are different and vary with time. This data set contains raw count rates (counts per second) obtained from five MCPs without taking into account their efficiency. In order to have more realistic picture we provide relative MCPs efficiencies depending on time. The sensitivity...

This dataset contains Oxygen+ particle energy flux issued from the Channel 1 ION-1 instrument of the Interball Auroral probe (mode 16 energy steps and 32 spectra).

This dataset contains proton energy flux issued from the Channel 1 ION-1 instrument of the Interball Auroral probe (mode 32 energy steps and 64 spectra).

This dataset contains proton energy flux issued from the Channel 1 ION-1 instrument of the Interball Auroral probe (mode 16 energy steps and 32 spectra).

This dataset contains proton energy flux issued from the Channel 1 ION-1 instrument of the Interball Auroral probe (mode 16 energy steps and 16 spectra).

This data set contains electron energy flux issued from the Channel 1 ELEC-2 instrument of the Interball Auroral probe (mode 64 spectra).