A public domain quality assurance software package that facilitates the assessment of multiplex short tandem repeat (STR) DNA profiles based on laboratory-specific protocols.

The Odin OSIRIS (Optical Spectrograph and Infra-Red Imaging System) data provides vertical profiles measures of spectrally dispersed, limb scattered sunlight from the upper troposphere into the lower mesosphere. The data products are regularly processed and provide Ozone density vertical profiles (both Level 2 and Level 3), vertical profiles of stratospheric Aerosol (both Level 2 and Level 3), slant column densities of nitrogen dioxide NO2 profiles (Level 2), stratospheric BrO profiles (Level 2)

This collection contains the raw interferograms acquired by the OSIRIS-REx Thermal Emission Spectrometer (OTES).

The cores and dredges described at this site were taken on the OSIRIS III cruise from 6 May until 3 June 1977 by the Muséum National d'Histoire Naturelle from the R/V Marion Dufresne. A total of 9 cores, dredges and camera stations were recovered and are available at MNHN for sampling and study.From 1983 until 1989 NOAA-NCEI compiled the NOAA-MMS Marine Minerals Geochemical Database from journal articles, technical reports and unpublished sources from other institutions. At the time it was the most extended data compilation on ferromanganese deposits world wide. Initially published in a proprietary format incompatible with present day standards it was jointly decided by AWI and NOAA to transcribe this legacy data into PANGAEA. This transfer is augmented by a careful checking of the original sources when available and the encoding of ancillary information (sample description, method of analysis...) not present in the NOAA-MMS database.

This collection contains the converted (processing level 1) instrument housekeeping data products produced by the OVIRS instrument onboard the OSIRIS-REx spacecraft.

The Odin satellite is a joint project bewteen Sweden, Canada, France and Finland that has been in space since Feb 2001 and still in operation. The OSIRIS datasets comprises profiles of Ozone, Nitrogen Dioxide, Bromine Monoxide and Stratospheric Aerosol from the cloud tops to 60 km depending on species

Canada's Optical Spectrograph and InfraRed Imaging System (OSIRIS) is the optical payload on Sweden's Odin satellite. It works in synergy with Sweden's advanced radiometer and measures atmospheric composition. Since 2001, OSIRIS has obtained valuable information on the upper atmosphere. It focuses its attention on altitudes from 7 to 90 km—between the highest mountains and the edge of space—and measures concentrations of ozone, aerosols and nitrogen dioxide. Data provided by OSIRIS helps scientists better understand the impact of human activities and natural phenomena on the environment and climate.

This dataset provides information about the number of properties, residents, and average property values for Osiris Street cross streets in Alexandria, LA.

Canada's Optical Spectrograph and InfraRed Imaging System (OSIRIS) is the optical payload on Sweden's Odin satellite. It works in synergy with Sweden's advanced radiometer and measures atmospheric composition. Since 2001, OSIRIS has obtained valuable information on the upper atmosphere. It focuses its attention on altitudes from 7 to 90 km—between the highest mountains and the edge of space—and measures concentrations of ozone, aerosols and nitrogen dioxide. Data provided by OSIRIS helps scientists better understand the impact of human activities and natural phenomena on the environment and climate.

This bundle contains OSIRIS-REx SPICE kernels and related documentation.

This dataset contains three spreadsheets of heuristic evaluations conducted by experts and also the prototypes they used. The evaluations assess the usability and effectiveness of various systems based on established heuristic principles. Each spreadsheet includes detailed assessments, observations, and ratings provided by the experts, offering valuable insights into the user interface and experience. These evaluations are intended to support research and improvement of usability practices in the context of the evaluated systems.

Subscribers can find out export and import data of 23 countries by HS code or product’s name. This demo is helpful for market analysis.

Osiris Inc Company Export Import Records. Follow the Eximpedia platform for HS code, importer-exporter records, and customs shipment details.

This bundle collects all the operational data products produced by the OSIRIS-REx Laser Altimeter (OLA). OLA is used for the topographic characterization of the surface of (101955) Bennu.

This bundle collects all the mission wide information needed to use and understand the scientific data products produced by the Origins, Spectral Interpretation, Resource Identification, Security, Regolith Explorer (OSIRIS-REx) mission.

This bundle collects all the operational data products produced by the OSIRIS-REx Visible and InfraRed Spectrometer (OVIRS). OVIRS is used for the spectral characterization of the surface of (101955) Bennu.

This data set collects shape models and their associated coordinate systems for the Rosetta target 67P/1969 R1 (Churyumov- Gersimenko). These were produced by the mission teams based on data obtained at the comet.

Data Set Overview This data set contains science, calibration and checkout images acquired by the OSIRIS Narrow Angle Camera system on the Rosetta mission. The images were acquired during the prelanding mission phase covering the period from 20140916 to 20140923. The images are CODMAC level 3. The PRL mission phase covers the the approach to comet 67P/ ChuryumovGerasimenko prior to the landing of Philae Essential Reading The following documents, located on the dataset DOCUMENT folder, are essential for the understanding and interpretation of this data set: OSIRIS_SSR.PDF: Gives an overview of the science goals of the OSIRIS instrument and an overview of the instrument hardware. OSIRIS_SIS.PDF: Describes the OSIRIS PDS header Related Data Sets The following PDS data sets are related: ROCOSINAC2PRL67PCHURYUMOVM07BV1.0 ROCOSIWAC2PRL67PCHURYUMOVM07BV1.0 ROCOSIWAC3PRL67PCHURYUMOVM07BV1.0 Processing The PDS images in this data set were generated using the OSIRIS telemetry processing facility at the Max Planck Institute for Solarsystem Research from the raw telemetry stream sent down from the rosetta spacecraft. The decoded telemetry stream was initially saved as Level 1 PDS images (raw telemetry header and raw image data). These raw Level 1 image files were then passed through a level 1 to level 2 processing pipeline. This pipeline converts the raw telemetry header into calibrated physical values and appends additional information collected from external data sources (SPICE, sequence library ...) Given that the calibration database is considered a single product even if it can be used separately to calibrate images from the NAC and the WAC, it is delivered in its entirety on the NAC and WAC datasets. Data CCD Images The OSIRIS images are stored as PDS images (meaning data files with embedded label where the image data is sto truncated!, Please see actual data for full text [truncated!, Please see actual data for full text]

Dataset Overview This CODMAC level 2 data set contains uncalibrated image data in DN unit, acquired by the OSIRIS Narrow Angle Camera on the Rosetta spacecraft during the CRUISE 42 mission phase, covering the period from 20081006T00:00:00.000 to 20090913T23:59:59.000 All header keywords are defined and described in the OSIRIS SIS: DOCUMENTSISOSIRIS_SIS_V08.PDF. Note that the data part of the FITs files in the /DATA/FIT directory is identical to the data part of the PDS files in the /DATA/IMG directory. FITs files are delivered only for CODMAC levels 2,3, and 4 datasets. No FITs files are delivered for CODMAC level 5 datasets. Credit Line To be used for image display (presentations, public exposure, etc.) and figure captions (e.g., in scientific articles). ESA/Rosetta/MPS for OSIRIS Team MPS/UPD/LAM/IAA/SSO/INTA/UPM/DASP/IDA Acknowledgment Full acknowledgment (e.g., in acknowledgment section of scientific article). The authors acknowledge the OSIRIS Principal Investigator H. Sierks (MPS, Goettingen, Germany) and the OSIRIS Team for providing images and related datasets and the ESA Rosetta Project to enable the science of the mission. Essential Reading The following documents, located on the dataset DOCUMENT folder, are essential for the understanding and interpretation of this dataset: KELLER_ET_AL_2007_V01.PDF: Gives an overview of the science goals of the OSIRIS instrument and an overview of the instrument hardware. OSIRIS_SIS_V08.PDF: Describes the OSIRIS PDS header SCIENCE_USER_GUIDE_V07.PDF: Describes the intention behind the acquisition of each image and its planned scientific purpose. Related Datasets The following PDS datasets are related: ROXOSIWAC2CR4BCHECKOUTV3.0 Please note that different datasets can contain different number of images. For details see OSIRIS_CAL_PIPELINE_V10.PDF and SCIENCE_USER_GUIDE_V07. truncated!, Please see actual data for full text [truncated!, Please see actual data for full text]

SMR: Contains one file for each processed tomographic orbit with SMR for July 16 2010. For a description of the processing see Christensen et.al. 2015. Each file has the following fields:aao: the angle along orbit axisfmode: the frequency mode used along the orbitgamma: Values of the Marquard-Levenberg parameter for each batchgamma_min: Values of the smallest Marquard-Levenberg parameterH2O: Retrieved water vapour (vmr)lat: latitude along orbitlon: longitude along orbitlst: local solar time along orbitmjd: Modified Julian Date along orbitodinorbit: odin orbit numberpressure: pressure axis (Pa)T: Temperature retrieved (K)Z: Altitude field (m)OSIRIS data: Data for all orbits in NH 2010 and NH 2011 are contained within the matlab file 'tom_gauss_B_alpha4.4_v1_6b.mat'. For description of the processing see Hultgren et al. (2014).The file has the following data fields: A: Column albedo at 90 deg angleAAO: angle along orbitIMD: Ice mass density (ng m^-3)IWC: Integrated ice column (ug m^-2)N: Ice particle number density (cm^-3)alpha: fitted Angstrom exponent () beta: retrieved scattering coefficient (m^-1 sr^-1)beta90: retrieved scattering coefficient at scattering angle of 90 degreesdalpha: rms of the residuals of the Angstrom fitlambda: wavelength of OSIRIS channels (nm)lat: latitude along orbitlon: logitude along orbitmjd: Modified Julian Date along orbitorbit: Odin orbit numberrm: Mode radius of the fitted gaussian PSD. ssa: Solar scattering angle (degrees)sza: Solar zenith angle (degrees)z: Altitude (km)