The Juno MWR RDR data set will ultimately include all calibrated MWR science data for the entire Juno mission. This volume will contain only those data obtained through the cruise phase of the Juno mission, when this phase of the mission is completed. The objective for these data is to provide calibration for the MWR instrument; however, it is anticipated that they may someday be useful for astrophysics. This volume consists of calibrated data records, each of which contains all instrumental data required for further processing. The RDR records have a one-to-one correspondence with the EDR records.

This data set contains the RDR data from the MSL Radiation Assessment Detector (RAD) instrument. The RDR data are calibrated data reconstructed from EDR data.

This dataset is developed for a research project “Humour Scandals (Hu-Sca): A cross-national analysis of humour controversies in Europe”, funded by KU Leuven, Una Europa Research Acceleration Fund. The data contains an overview of humor scandals i.e. public controversies originating from humor and dealing with the boundaries of transgressive humor in public debate and their reception in legacy media for eight European countries between 1990 and 2022. The data contains quantatively coded descriptive markers of each humor scandal (e.g. nature of norm transgression, actors involved, duration, timespan) as well as qualitative analysis of the way that the humor scandal was either justified or condemned in national legacy media. This data can be used for the analysis of the role of humor in socio-political conflict and the role of media in the creation and mediation of humor-related controversies.

The MESSENGER XRS RDR data consist of maps of the ratio of elements detected by the XRS instrument during orbital operations at Mercury.

The MESSENGER MLA calibrated and reduced observations consist of laser ranges and instrument data collected by the MLA instrument during fly-by and orbital operations of Mercury. Also included are observations of Earth and Venus for calibration purposes.

Enterprise Human Resources Integration (EHRI) Retirement Data repository is a database of standardized retirement data needed to process retirements for Federal employees in a timely and accurate manner.

This dataset contains Commercial (Comm) Radio Occultation (RO) raw data from GeoOptics, which is an established method for remote sounding of the atmosphere. The technique uses an instrument in low-Earth orbit (LEO) to track radio signals from Global Navigation Satellite System (GNSS) transmitters as they rise or set through the atmosphere. The occulting atmosphere refracts or bends the radio signals, and given the precise positions of both satellites, the bending angle can be deduced from the time delay of the signal. Collecting these measurements for a full occultation through the atmosphere provides a vertical profile of bending angles, from which profiles of physical quantities such as temperature, humidity, and ionospheric electron density can be retrieved. These data primarily feed numerical weather prediction (NWP) models that support weather forecasts, and also support space weather analysis/prediction at NOAA.

The GRaND Reduced Data Records (RDR) contain a time series of calibrated spectra, counting data, and ephemeris, pointing, and geometry (EPG) data. The EPG data are contained in a single file, with an entry for every science data record acquired by GRaND within the dataset start-stop times. Each record has a unique identifier, spacecraft clock ticks, which is used as a serial number to identify data from the same record in other files containing spectra and counting data. The RDR data set includes a time series of corrected gamma ray spectra acquired by GRaND's bismuth-germanate (BGO) scintillator.

Abstract ======== The Mercury Dual Imaging System (MDIS) consists of two cameras, a Wide Angle Camera (WAC) and a Narrow Angle Camera (NAC), mounted on a common pivot platform. This dataset include regional mosaics of targeted observations directed at specific regions of interest. Four types of targeted observations are included: (a) WAC 3-color targeted observations acquired mainly during the primary mission, to complement 1 km/pixel 8-color mapping with a higher spatial resolution 3-color product; (b) WAC observations of targets that were observed repeatedly at different photometric geometries in order to improve photometric models of Mercury; these were observed initially in 8 color and since early 2013 in 11 colors; (c) WAC 8- or 11-color science targeted observations; and (d) NAC image strips acquired either for high-resolution imaging of morphology or as context for MASCS or MLA observations. The images in each observation share a common SITE_ID in the file name and PDS label. The SITE_ID corresponds to a targeting request entered into a database, in response to which a series of images was acquired. There is one SITE_ID for each time the region of interest is observed; thus for photometry targets, the same geographic region of interest is covered by many sets of images, each set sharing a common SITE_ID and distinct photometric geometry. Each mosaic is map projected in an orthographic projection, and contains one or more image planes. NAC mosaics contain 4 backplanes: observation ID, solar incidence angle, emission angle, and phase angle. WAC color products contain 3 backplanes: solar incidence angle, emission angle, and phase angle.

The GRaND Reduced Data Records (RDR) contain a time series of calibrated spectra, counting data, and ephemeris, pointing, and geometry (EPG) data. The data set is specific to Vesta encounter. The EPG data are contained in a single file, with an entry for every science data record acquired by GRaND at Vesta. Each record has a unique identifier, spacecraft clock ticks, which is used as a serial number to identify data from the same record in other files containing spectra and counting data. The RDR data set includes a time series of corrected gamma ray spectra acquired by GRaND's bismuth-germanate (BGO) scintillator.

This database offers an overview of publicly available sources for the history of Belgian self-help groups, mainly from the twentieth century. It contains archives, publications, journals, interviews, television broadcasts and other types of sources which are available in public libraries and archives or even online. The database can be opened in Zotero or it can be accessed online: https://www.arts.kuleuven.be/cultuurgeschiedenis/en/current-projects-/self-help-in-twentieth-century-belgium-a-database-of-sources

This data set contains images acquired by the OSIRIS Narrow Angle Camera during the CRUISE 5 mission phase

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This data set contains images acquired by the OSIRIS Narrow Angle Camera during the CRUISE 4-2 mission phase

Abstract ======== This data set consists of the MESSENGER Mercury Laser Altimeter (MLA) Calibrated Data Record (CDR) and Reduced Data Record (RDR) products. The MLA is a solid-state pulsed laser that measures the distance between the spacecraft and the surface of Mercury. The CDR products contain the science and auxiliary data products calibrated to physical units. The RDR products contain the calibrated, geolocated range data as profile measurements of the planetary radius.

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added ARCHIVE_STATUS, ,This data set contains the RDR data for the Galileo Orbiter PPR instrument for the period corresponding to the Venus encounter observations in February 1990.

The Suomi NPP Climate Raw Data Record (C-RDR) developed at the NOAA NCDC is an intermediate product processing level (NOAA Level 1b) between a Raw Data Record (RDR) and a Sensor Data Record (SDR). The C-RDR is intended to simplify access to the raw data for the purpose of reprocessing using calibration and geolocation methods. The Visible Infrared Imaging Radiometer Suite (VIIRS) C-RDR has raw VIIRS measurements collected into time series variables, accompanied by the coefficients and tables needed to convert them to science units and calibrate them. Where applicable, metadata in this file follows the Climate and Forecast (CF) Conventions and Attribute Convention for Dataset Discovery (ACDD). Metadata attributes from the native Suomi NPP RDR and SDR file types are also included. These files have been compared with those generated using JPSS Application Development Library (ADL) applications. Product documentation and software are available for the dataset.

A field differential Geopositional Satellite (GPS) survey team which included Jim Garvin, Jack Bufton, Bill Krabill, and Earl B. Frederick deployed a pair of Motorola Eagle II GPS receivers to the southern flanks of the feature known as Mars Hill (an alluvial boulder field superimposed on a major lobe of alluvial and colluvial material in Eastern Death Valley) on Oct. 19, 1989. The objective was to measure the 5-20 cm scale microrelief of the boulder field at pixel scales (30-50 m long transects), with vertical control to the few cm level. These microterrain profiles were to be used to help calibrate radar scattering models, and to compare with helicopter stereo data (FEXP-E-HSTP-4 RDR-TOPOGRAPHIC-PROF-V1.0) for the same location.

Portable Field Emission Spectrometer (PFES) data were acquired on July 15 and 17, 1989. A total of 31 measurements were collected for GRSFE. Of these measurements, 13 were calibrations and 18 were of representative surfaces. The data were collected primarily to support the calibration of the TIMS data and to assist in interpreting spectral mixing in the mid-infrared. Sites were selected for calibration that covered a range of emissivities. On July 15, PFES data were collected at Kelso Dunes and the Cima Volcanic Field as part of the Calibration Team effort. Daedalus and SIRIS data were collected over the same sites. For the PFES data, the Kelso Dunes Bright Target site represented the silica-rich endmember and the Cima basalt tephra Dark Target site represented the more silica-poor endmember. On July 17, PFES data were collected at two of the modelling sites at Lunar Lake (the playa and the cobble sites). Several spectra were also collected at the playa surface next to the Lunar Lake thermistor site.