15,780 datasets found

The Spin-plane electric field vector, measured by the Electric Fields Instrument (EFI), in the TRACERS spinning frame (TSCS) is sampled. The sampling rate is 2048 samples/s. The...

EFI sensor potentials relative to spacecraft ground with a sampling rate of 128 samples/s (ROI) or 8 samples/s (BOR).

The ACE L2 data consist of raw measured counts and calibrated differential energy fluxes as a function of anode angle and calibrated energy. Counts are accumulated in 21...

EFI state-of-health and operational state housekeeping data (HSK). See https:/doi.org/10.1007/s11214-025-01202-5, Table 2 and supporting text for details.

TRACERS 1 Electric Field Instrument (EFI) high frequency (EHF) time-series and spectra data sampled by the EFI x-antenna, which is along the x-axis in the TRACERS Spacecraft...

The Spin-plane electric field vector, measured by the Electric Fields Instrument (EFI), in the TRACERS spinning frame (TSCS) is sampled. The sampling rate is 2048 samples/s. The...

EFI sensor potentials relative to spacecraft ground with a sampling rate of 128 samples/s (ROI) or 8 samples/s (BOR).

The ACE L2 data consist of raw measured counts and calibrated differential energy fluxes as a function of anode angle and calibrated energy. Counts are accumulated in 21...

TRACE low level data and accompanying software

TRACE satellite position and magnetic field model information.

The TIMED Doppler Interferometer, TIDI, instrument is a Fabry-Perot interferometer designed to measure zonal and meridional winds in the mesosphere and lower thermosphere. This...

Contains the TIDI Level 3 data mapped onto a fixed angle-along-the-track grid. The wind is decomposed into its zonal and meridional components. Each profile is annotated with...

Contains the TIDI Level 2 inverted profiles of wind, temperature and volume emission rates annotated with profile location and processing status. Profiles are produced at the...

Contains the TIDI Level 1B spectra corrected for instrumental effects and converted to Rayleighs/cm^-1, ancillary data and profiles of apparent LOS wind, temperature, and volume...

The SEE XPS Level 4 data are derived from the XPS Level 1 data products. The XPS Level 4 processing algorithm uses reference CHIANTI spectral models to generate a higher...

SEE Level 3A data files contain each measurements averaged solar irradiance spectrum in 1 nm intervals extracted from the EGS Level 2A and XPS Level 2A data products. Shortward...

SEE Level 3 data files contain one daily averaged solar irradiance spectrum in 1 nm intervals extracted from the EGS Level 2 and XPS Level 2 data products. Shortward of 27 nm, a...

The 12 X-Ray Photometers (XP) aboard SEE perform full-disk irradiance measurements of the Sun for about 3 minutes every orbit (97 minutes) which usually gives 14-15 measurements...

The EUV Grating Spectrograph (EGS) aboard SEE performs measurements of the Sun for about 3 minutes every orbit (97 minutes) which usually gives 14-15 measurements per day. The...

The EUV Grating Spectrograph (EGS) aboard SEE performs measurements of the Sun for about 3 minutes every orbit (97 minutes) which usually gives 14-15 measurements per day. 4x...