This data set contains tables of time ordered, hourly-averaged plasma parameters, mainly of the solar wind, as observed on the Moon at the Apollo 12 ALSEP site by the Apollo 12 Solar Wind Spectrometer from 19 November 1969 through 25 March 1976.

This data collection consists of archived Space Weather Follow On Lagrange 1 (SOL-1) Level 1b data from the Solar Wind Plasma Sensor (SWiPS). The archival process includes daily files. The SWiPS instrument generates 1 file per day per level in the netCDF-4 format. These data are produced by the SWiPS instrument aboard the SOL-1 spacecraft. SWiPS monitors the solar wind for abrupt changes, which can result from interplanetary shocks, coronal mass ejections, corotating interaction regions or high speed solar wind, because these can cause geomagnetic storms that are harmful to life and technology. SOL-1 will launch in 2025. Other products available are auxiliary files (frm-rt-l0_sol1, frm-st-l0_sol1, pkt-l0_sol1, orb-pr_sol1, sc-att_sol1); SWiPS files (swips-l0b_sol1, swips-l1a_sol1, swips-l2_sol1, and swips-l3-avg1m_sol1); and, National Centers for Environmental Data (NCEI) Retrospective Science products (sci_swips-l1a_sol1, sci_swips-l1b_sol1, sci_swips-l2_sol1, and sci_swips-l3-avg1m_sol1).

**Overview** The dataset includes 15-minute average wind speed and direction records from 10 m to 250 m above ground level (AGL) in 5-m range gates. Data were collected by a Scintec SFAS wind profiler installed at the Condon State Airport in Oregon, about 1.8 km northeast of the center of Condon, Ore., and are intended for validating WFIP2 model improvements. **Data Details** Instrument location: * N 45° 14’ 41.58” (N 45.244885) * W 120° 10’ 06.58” (W 120.168495) Instrument clock and computer system time set to UTC. **Data Quality** The Scintec SFAS wind profiler instrument installed at the Decker Ranch is capable of measuring at heights up to 500 m. For this study, the maximum height was set to 250 m. The instrument was oriented to true north, so no corrections to the wind direction should be made. Scintec wind profilers come with the APRun software package, which performs data collection and quality control (QC), among other functions. Version 1.46 of APRun was used in this study. The APRun manual states: *The primary results are checked against local signal quality criteria, combined signal quality criteria and two-dimensional spatial/temporal consistency tests. Any data that does not pass all quality control tests is devalidated and removed*. Devalidation means replacing the value with an error value, usually a series of ‘9’s, such as 99.99 or 999.99. Not all devalidated data are actually removed from the *.mnd files, so the user must filter them out. There are some error flags that indicate the type of error, but these are not included in the *.mnd files, and we have no access to them. Because QC already has been performed by APRun, our QC procedures consisted of removing samples with error values and performing a visual inspection of the data to see if larger patterns indicated any kind of problem. There are 515 gaps of two hours or less and 26 gaps of more than two hours. The longest gaps are: * 47.78 days, from 2016-03-16 18:00Z to 2016-05-03 12:45Z * 40.20 days, from 2016-06-04 13:15Z to 2016-07-14 18:00Z All gaps that exceed two hours are listed in file: Condon_gaps.txt.

Solar wind observations collected from Faraday Cup on DSCOVR satellite - 20-second average of cycle peaks

This data set contains solar wind plasma data upstream of Jupiter before the Voyager 2 encounter. Fit and moment parameters are given; the fit parameters assume a convected isotropic proton Maxwellian distribution. Use of fit parameters is recommended as these are normally more accurate. Since only the first 72 or last 72 energy/charge channels are telemetered to Earth from each M-mode spectra, derived parameters change significantly only every other set of spectra so the effective time resolution is 196 s.

**Overview** Scaled Wind Farm Technology (SWiFT) Facility meteorological tower (MET), turbine, and Technical University of Denmark (DTU) SpinnerLidar data acquired on 20161216 UTC during a neutral atmospheric boundary layer inflow at a single focus distance of 2.5 D (D=27 m). **Data Quality** Data information is provided in uploaded documentation: *SWiFT Wake Steering Instrumentation and Data Processing* (PDF).

THIS DATA SET CONTAINS THE DERIVED VALUES FOR THE ELECTRON MOMENT DENSITY AND TEMPERATURE AT JUPITER IN THE PLS ENERGY RANGE (10-5950 EV) DURING THE VOYAGER 2 ENCOUNTER. ADJACENT LOW AND HIGH ENERGY ELECTRON MEASUREMENTS ARE COMBINED TO FORM A COMPOSITE SPECTRA WHICH IS USED FOR THE MOMENT CALCULATION. THE MOMENT CALCULATIONS ARE PERFORMED AS DESCRIBED IN SCUDDER ET AL. (1981). THESE ASSUME ISOTROPIC DISTRIBUTIONS AND CORRECT FOR POSITIVE SPACECRAFT CHARGE WHEN APPLICABLE AND INTERPOLATE ELECTRON SPECTRA BELOW THE 10 EV INSTRUMENT THRESHOLD BEFORE PERFORMING THE INTEGRATION OVER VELOCITY. DATA FORMAT: COLUMNS 1-6 ARE TIME (YEAR, DAY, HOUR, MIN, SEC, MSEC) COLUMN 7 IS THE MOMENT DENSITY IN CM-3, COLUMN 8 THE TEMPERATURE IN EV. EACH ROW HAS FORMAT (6I4, 2E12.3). VALUES OF 1.E32 INDICATE THAT THE PARAMETER COULD NOT BE OBTAINED FROM THE DATA USING THE STANDARD ANALYSIS TECHNIQUE. ADDITIONAL INFORMATION ABOUT THIS DATASET AND THE INSTRUMENT WHICH PRODUCED IT CAN BE FOUND ELSEWHERE IN THIS CATALOG. AN OVERVIEW OF THE DATA IN THIS DATA SET CAN BE FOUND IN SCUDDER ET AL. (1981) AND A COMPLETE INSTRUMENT DESCRIPTION CAN BE FOUND IN BRIDGE (1977).

Solar wind observations collected from Faraday Cup on DSCOVR satellite - 1-minute average of cycle peaks

**Overview** The dataset includes 15-minute average wind speed and direction records from 30 m to 330 m above ground level (AGL) in 10-m range gates. Data were collected by a Scintec MFAS wind profiler installed at the Decker Ranch in Oregon, about 4.4 km southeast of Kent, Ore., and are intended for validating WFIP2 model improvements. **Data Details** Instrument location: * N 45°09'54.42" (N 45.165117) * W120°39'20.87" (W 120.655799) Instrument clock and computer system time set to UTC. **Data Quality** The Scintec MFAS wind profiler instrument installed at the Decker Ranch is capable of measuring at heights up to 1000 m. For this study, the maximum height was set to 330 m. The instrument was oriented to true north, so no corrections to the wind direction should be made. Scintec wind profilers come with the APRun software package, which performs data collection and quality control (QC), among other functions. Version 1.46 of APRun was used in this study. The APRun manual states: *The primary results are checked against local signal quality criteria, combined signal quality criteria and two-dimensional spatial/temporal consistency tests. Any data that does not pass all quality control tests is devalidated and removed*. Devalidation means replacing the value with an error value, usually a series of ‘9’s, such as 99.99 or 999.99. Not all devalidated data are actually removed from the *.mnd files, so the user must filter them out. There are some error flags that indicate the type of error, but these are not included in the *.mnd files, and we have no access to them. Because QC already has been performed by APRun, our QC procedures consisted of removing samples with error values and performing a visual inspection of the data to see if larger patterns indicated any kind of problem. There are 623 gaps of two hours or less and 61 gaps of more than two hours. The longest gap is 15.31 days, from 2016-12-07 03:00Z to 2016-12-22 10:30Z. All gaps that exceed two hours are listed in file: Decker_Ranch_gaps.txt.

This dataset contains wind direction and speed, air temperature, and light intensity (solar irradiance) from two weather stations along the West Antarctic Peninsula. These weather stations collected data from the Joubin (64.787836 S, 64.351674 W) and Wauwerman (64.911416 S, 64.013430 W) islands around Palmer Deep Canyon between 11/2014 and 06/2016. These data were collected as part of NSF-funded Project CONVERGE, which examined the effect of physical oceanographic processes on penguin foraging dynamics. The data are uploaded as Comma Separated Values (CSV).