Search Results

1–37 of 37 results (0.000 seconds)

Data Sets and Information
• collection: Arizona State University Ronald Greeley Center for Planetary Studies - The Ronald Greeley 35mm Slide Collection, The Jovian System, The Jovian System Bodies and Miscellaneous Objects
  This collection, included in document_jovian_system_and_misc, consists of 245 digitized 35mm slides of Jovian System bodies and miscellaneous objects. Slides are divided into two databases, diagrams and photos, but are inventoried as a single collection. Information about each photograph, including location, description, and mission, are in the document_database in jovian_system_and_misc_diagram_database.pdf and jovian_system_and_misc_photo_database.pdf. The photographs and documentation are from the Dr. Ronald Greeley archive at the Arizona State University Ronald Greeley Center for Planetary Studies, Tempe, Arizona.
• collection: Small Main-Belt Asteroid Spectroscopic Survey (SMASS) V1.0
  The Small Main-Belt Asteroid Spectroscopic Survey (SMASS) was a wide wavelength-coverage visible spectroscopic survey of asteroids carried out primarily at the Michagan-Dartmouth-MIT (McGraw Hill) Observatory on Kitt Peak beginning in 1990. This data set covers the observations for the years 1990-1994 and includes spectra of 316 asteroids. The data have been published in Xu et al. (1995), Icarus 115, 1-35, 1995.
• collection: Galileo NIMS PDS4 Archive XML Schema Collection
  The original Galileo NIMS archived data were originally publicly available but not in a format that was readily accessible by the planetary community. This situation precludes the spectral investigation of surface and atmospheric chemistry and mineralogy for these objects. Several aspects of the NIMS data archive contribute to this circumstance, including VAX formatted data files (a platform and format abandoned by the PDS), a challenging radiometric calibration, and the absence of a rigorous camera/sensor model, and/or data products that have been orthorectified or spatially controlled relative to SSI observations or more recent Cassini data products (e.g., VIMS). NIMS data are also not easily accessible by the planetary community. Before this work, NIMS data were only compatible with ISIS2, a program no longer supported by the USGS and no longer functions on some modern computer operating systems (e.g., Apple OS X). Galileo NIMS data were also not compatible with mainstream planetary software, including ENVI/IDL or ISIS3. This effort transitioned the data set to ISIS3 and thereby ISIS3 support interfaces. The NIMS PDS archive contains tube and g-cube data derived from the EDRs. Considering the relatively small scope of this effort only the NIMS tube and g-cube product data are the focus of this work. The objective of this work is to reformat and re-archive the Galileo NIMS data set into a more easily accessible data format. In order to do this we outlined three basic objectives: Objective 1: Create an ISIS3 application that reads and converts the NIMS data cubes into native ISIS3 cubes. NIMS data in the PDS is stored in VAX FLOAT format which is mostly obsolete and not widely used in the community any longer. This objective would ential adding support for conversion of VAX FLOAT to IEEE FLOAT in ISIS; advantageous to the pursuit is existing code in ISIS2 that provided a basis for this work. Here we also sought to seek out problems with the NIMS labels in PDS archive that are not compliant with PDS4 standards. These labels errors are to then be corrected and exported with properly formed labels to the PDS archive. Objective 2: Provide the ability to project NIMS tubes using the existing NIMS latitude, longitude tube backplanes. Objective 3: Derivation of a PDS4 compliant archive of the results of our study and provide it to the PDS for general distribution. These basic initial steps will make NIMS more user friendly and provide active support through ISIS help interfaces.
• bundle: Galileo NIMS PDS4 Archive
  The original Galileo NIMS archived data were originally publicly available but not in a format that was readily accessible by the planetary community. This situation precludes the spectral investigation of surface and atmospheric chemistry and mineralogy for these objects. Several aspects of the NIMS data archive contribute to this circumstance, including VAX formatted data files (a platform and format abandoned by the PDS), a challenging radiometric calibration, and the absence of a rigorous camera/sensor model, and/or data products that have been orthorectified or spatially controlled relative to SSI observations or more recent Cassini data products (e.g., VIMS). NIMS data are also not easily accessible by the planetary community. Before this work, NIMS data were only compatible with ISIS2, a program no longer supported by the USGS and no longer functions on some modern computer operating systems (e.g., Apple OS X). Galileo NIMS data were also not compatible with mainstream planetary software, including ENVI/IDL or ISIS3. This effort transitioned the data set to ISIS3 and thereby ISIS3 support interfaces. The NIMS PDS archive contains tube and g-cube data derived from the EDRs. Considering the relatively small scope of this effort only the NIMS tube and g-cube product data are the focus of this work. The objective of this work is to reformat and re-archive the Galileo NIMS data set into a more easily accessible data format. In order to do this we outlined three basic objectives: Objective 1: Create an ISIS3 application that reads and converts the NIMS data cubes into native ISIS3 cubes. NIMS data in the PDS is stored in VAX FLOAT format which is mostly obsolete and not widely used in the community any longer. This objective would ential adding support for conversion of VAX FLOAT to IEEE FLOAT in ISIS; advantageous to the pursuit is existing code in ISIS2 that provided a basis for this work. Here we also sought to seek out problems with the NIMS labels in PDS archive that are not compliant with PDS4 standards. These labels errors are to then be corrected and exported with properly formed labels to the PDS archive. Objective 2: Provide the ability to project NIMS tubes using the existing NIMS latitude, longitude tube backplanes. Objective 3: Derivation of a PDS4 compliant archive of the results of our study and provide it to the PDS for general distribution. These basic initial steps will make NIMS more user friendly and provide active support through ISIS help interfaces.
• bundle: Dawn RSS Raw Data Bundle For Asteroid 4 Vesta
  This bundle contains raw radio data that can be used to determine the position and velocity of the DAWN spacecraft during its encounter with 4 Vesta. The bundle also contains the calibration data for the effects of Earth's ionosphere and troposphere, meteorological conditions at stations of the NASA Deep Space Network, thruster activity, spacecraft mass history, and changes in spacecraft antenna selection. The data were used to determine the gravity field and shape of 4 Vesta. Documents describing these data are also included in the bundle. The bundle is a migration of data from the original PDS3 archive.
• bundle: Galileo Photopolarimeter Radiometer Pre-Jupiter Raw Bundle
  This Bundle includes raw (R_EDR) data for the Galileo Orbiter PPR instrument for the period corresponding to the Galileo Pre-Jupiter observations between December 1989 and August 1993.
• bundle: Galileo Photopolarimeter Radiometer Pre-Jupiter Derived Bundle
  This Bundle includes derived data for the Galileo Orbiter PPR instrument for the period corresponding to the Galileo Pre-Jupiter observations between December 1989 and July 1994.
• bundle: Arizona State University Ronald Greeley Center for Planetary Studies - The Ronald Greeley 35mm Slide Collection, The Jovian System
  This bundle contains the digitized products generated from Dr. Ronald Greeley's 35mm Slide Collection, the Jovian System, housed at the RGCPS, ASU, Tempe, AZ. Included is a User’s Guide for a further description of the products.
• collection: Galileo PLS Asteroid Averaged Ida Calibrated Data Collection
  This collection contains a listing of particle energy spectra from the Galileo Plasma Instrument (PLS) during the Ida Flyby
• collection: Small Main-Belt Asteroid Spectroscopic Survey, Phase II V1.0
  This data set contains visible-wavelength (0.435-0.925 micron) spectra for 1341 main-belt asteroids observed during the second phase of the Small Main-belt Asteroid Spectroscopic Survey (SMASSII) between August 1993 and March 1999. The purpose of the SMASSII survey was to provide a new basis for studying the compositional diversity and structure of the asteroid belt. Based on experiences gained from the earlier SMASS survey, SMASSII focused on producing an even larger, internally consistent set of CCD spectra for small (D < 20 km) main-belt asteroids. The observing strategies and procedures used during SMASSII roughly parallel those used in the first survey (Xu et al. Icarus 115 1-35, 1995), though several minor changes were made in instrumentation and in portions of the data reduction process.
• collection: Dawn Radio Science Orbit Data File (ODF) Product Collection
  This is the collection of Radio Science Orbit Data File (ODF) data products acquired during the Dawn mission. These ODF files were produced by the NASA/JPL Multi-Mission Navigation Radio Metric Data Conditioning Team for use in determining spacecraft trajectories, gravity fields affecting them, and radio propagation conditions.
• collection: Galileo Solar System MAG Averaged Cruise RTN Coordinates Calibrated Data Collection
  This collection contains data acquired by the Galileo Magnetometer during the Interplanetary Cruise to Jupiter. The data are at varying resolution depending on the averaging constant applied to the instrument.
• collection: Small Bodies Radar Shape Models V1.0
  This data set contains radar-based shape models for small solar system bodies, prepared by various authors.
• bundle: Dawn RSS Raw Data Bundle For Dwarf Planet 1 Ceres
  This bundle contains raw radio data that can be used to determine the position and velocity of the DAWN spacecraft during its encounter with 1 Ceres. The bundle also contains the calibration data for the effects of Earth's ionosphere and troposphere, meteorological conditions at stations of the NASA Deep Space Network, thruster activity, spacecraft mass history, and changes in spacecraft antenna selection. The data were used to determine the gravity field and shape of 1 Ceres. Documents describing these data are also included in the bundle. The bundle is a migration of data from the original PDS3 archive.
• bundle: Small Main-Belt Asteroid Spectroscopic Survey (SMASS) V1.0
  The Small Main-Belt Asteroid Spectroscopic Survey (SMASS) was a wide wavelength-coverage visible spectroscopic survey of asteroids carried out primarily at the Michagan-Dartmouth-MIT (McGraw Hill) Observatory on Kitt Peak beginning in 1990. This data set covers the observations for the years 1990-1994 and includes spectra of 316 asteroids. The data have been published in Xu et al. (1995), Icarus 115, 1-35, 1995.
• bundle: NEAR EARTH ASTEROID LIGHTCURVES
  This data set is a collection of photometric lightcurves for 42 near-earth asteroids obtained at Ondrejov Observatory from 1984 through 1998.
• bundle: Small Bodies Radar Shape Models V1.0
  This data set contains radar-based shape models for small solar system bodies, prepared by various authors.
• bundle: Small Main-Belt Asteroid Spectroscopic Survey, Phase II V1.0
  This data set contains visible-wavelength (0.435-0.925 micron) spectra for 1341 main-belt asteroids observed during the second phase of the Small Main-belt Asteroid Spectroscopic Survey (SMASSII) between August 1993 and March 1999. The purpose of the SMASSII survey was to provide a new basis for studying the compositional diversity and structure of the asteroid belt. Based on experiences gained from the earlier SMASS survey, SMASSII focused on producing an even larger, internally consistent set of CCD spectra for small (D < 20 km) main-belt asteroids. The observing strategies and procedures used during SMASSII roughly parallel those used in the first survey (Xu et al. Icarus 115 1-35, 1995), though several minor changes were made in instrumentation and in portions of the data reduction process.
• collection: Galileo MAG RDR Gaspra High Resolution Calibrated Data Collection
  This collection contains calibrated high-resolution data from the Gaspra flyby in spacecraft, EME-50, RTN and Gaspra Solar Ecliptic (GaSE) coordinates.
• collection: Galileo PLS Pre-Jupiter Calibrated Browse Collection
  This collection includes full resolution electron, positive ion, and mass spectrometer observations obtained obtained during the period that the Galileo plasma analyzer was operated at Venus, Gaspra and Ida.
• collection: Galileo PLS Asteroid Averaged Gaspra Calibrated Data Collection
  This collection contains a listing of particle energy spectra from the Galileo Plasma Instrument (PLS) during the Gaspra Flyby
• collection: Galileo PPR Pre-Jupiter Raw Asteroid Gaspra Data Collection
  This collection contains the raw data for the Galileo Orbiter PPR instrument for the period corresponding to the Gaspra asteroid encounter observations in October 1991.
• collection: Small Main-Belt Asteroid Spectroscopic Survey, Phase II V1.0
  This data set contains visible-wavelength (0.435-0.925 micron) spectra for 1341 main-belt asteroids observed during the second phase of the Small Main-belt Asteroid Spectroscopic Survey (SMASSII) between August 1993 and March 1999. The purpose of the SMASSII survey was to provide a new basis for studying the compositional diversity and structure of the asteroid belt. Based on experiences gained from the earlier SMASS survey, SMASSII focused on producing an even larger, internally consistent set of CCD spectra for small (D < 20 km) main-belt asteroids. The observing strategies and procedures used during SMASSII roughly parallel those used in the first survey (Xu et al. Icarus 115 1-35, 1995), though several minor changes were made in instrumentation and in portions of the data reduction process.
• collection: Galileo MAG Averaged Gaspra Summary Calibrated Data Collection
  This collection contains calibrated averaged data from the Gaspra flyby in RTN coordinates. These data cover the interval 1991-10-29 06:03 to 1991-10-30 02:51.
• collection: Dawn Radio Science Tracking and Navigation (TNF) Data Products Collection
  This is the collection of Radio Science Tracking and Navigation (TNF) data products acquired during the Dawn mission. Data were originally stored as chronological records in DSN format TRK-2-34; but they have been sorted according to data type (retaining chronological order within each data type) during migration from PDS3 to PDS4.
• collection: Galileo NIMS PDS4 Archive - Data Collection
  The original Galileo NIMS archived data were originally publicly available but not in a format that was readily accessible by the planetary community. This situation precludes the spectral investigation of surface and atmospheric chemistry and mineralogy for these objects. Several aspects of the NIMS data archive contribute to this circumstance, including VAX formatted data files (a platform and format abandoned by the PDS), a challenging radiometric calibration, and the absence of a rigorous camera/sensor model, and/or data products that have been orthorectified or spatially controlled relative to SSI observations or more recent Cassini data products (e.g., VIMS). NIMS data are also not easily accessible by the planetary community. Before this work, NIMS data were only compatible with ISIS2, a program no longer supported by the USGS and no longer functions on some modern computer operating systems (e.g., Apple OS X). Galileo NIMS data were also not compatible with mainstream planetary software, including ENVI/IDL or ISIS3. This effort transitioned the data set to ISIS3 and thereby ISIS3 support interfaces. The NIMS PDS archive contains tube and g-cube data derived from the EDRs. Considering the relatively small scope of this effort only the NIMS tube and g-cube product data are the focus of this work. The objective of this work is to reformat and re-archive the Galileo NIMS data set into a more easily accessible data format. In order to do this we outlined three basic objectives: Objective 1: Create an ISIS3 application that reads and converts the NIMS data cubes into native ISIS3 cubes. NIMS data in the PDS is stored in VAX FLOAT format which is mostly obsolete and not widely used in the community any longer. This objective would ential adding support for conversion of VAX FLOAT to IEEE FLOAT in ISIS; advantageous to the pursuit is existing code in ISIS2 that provided a basis for this work. Here we also sought to seek out problems with the NIMS labels in PDS archive that are not compliant with PDS4 standards. These labels errors are to then be corrected and exported with properly formed labels to the PDS archive. Objective 2: Provide the ability to project NIMS tubes using the existing NIMS latitude, longitude tube backplanes. Objective 3: Derivation of a PDS4 compliant archive of the results of our study and provide it to the PDS for general distribution. These basic initial steps will make NIMS more user friendly and provide active support through ISIS help interfaces.
• collection: Galileo MAG RDR IDA High Resolution Solar Ecliptic Calibrated Data Collection
  This collection contains calibrated high-resolution data from the Gaspra flyby in spacecraft, EME-50, RTN and Gaspra Solar Ecliptic (GaSE) coordinates.
• collection: Galileo PPR Pre-Jupiter Derived Gaspra Asteroid Encounter Data Collection
  This collection contains the RDR data for the Galileo Orbiter PPR instrument for the period corresponding to the Gaspra asteroid encounter observations in October 1991.
• collection: Galileo MAG Averaged IDA Summary Calibrated Data Collection
  This collection contains calibrated averaged data from the Ida flyby in RTN coordinates. These data cover the interval 1993-08-28 00:56 to 1993-08-28 23:59.
• collection: Galileo Solar System MAG Averaged Cruise Inertial Rotor Coordinates (IRC) Calibrated Data Collection
  This collection contains data acquired by the Galileo Magnetometer during the Interplanetary Cruise to Jupiter. The data are at varying resolution depending on the averaging constant applied by the instrument. These data have been fully processed to remove instrument response function characteristics. The data are provided in physical units (nanoTesla) and in 2 coordinate systems. This set of data files contains data in Inertial Rotor Coordinates (IRC= despun spacecraft).
• collection: data collection for the "NEAR EARTH ASTEROID LIGHTCURVES" bundle
  This is the data collection for the gbo.ast-neo.ondrejov.lightcurves bundle. This data set is a collection of photometric lightcurves for 42 near-earth asteroids obtained at Ondrejov Observatory from 1984 through 1998.
• collection: Small Main-Belt Asteroid Spectroscopic Survey (SMASS) V1.0
  The Small Main-Belt Asteroid Spectroscopic Survey (SMASS) was a wide wavelength-coverage visible spectroscopic survey of asteroids carried out primarily at the Michagan-Dartmouth-MIT (McGraw Hill) Observatory on Kitt Peak beginning in 1990. This data set covers the observations for the years 1990-1994 and includes spectra of 316 asteroids. The data have been published in Xu et al. (1995), Icarus 115, 1-35, 1995.
• collection: Dawn Radio Science Orbit Data File (ODF) Product Collection
  This is the collection of Radio Science Orbit Data File (ODF) data products acquired during the Dawn mission. These ODF files were produced by the NASA/JPL Multi-Mission Navigation Radio Metric Data Conditioning Team for use in determining spacecraft trajectories, gravity fields affecting them, and radio propagation conditions.
• collection: Galileo PPR Pre-Jupiter Derived Ida Asteroid Encounter Data Collection
  This collection contains the RDR data for the Galileo Orbiter PPR instrument for the period corresponding to the Ida asteroid encounter observations in August 1993.
• collection: Galileo NIMS PDS4 Archive Context Collection
  The original Galileo NIMS archived data were originally publicly available but not in a format that was readily accessible by the planetary community. This situation precludes the spectral investigation of surface and atmospheric chemistry and mineralogy for these objects. Several aspects of the NIMS data archive contribute to this circumstance, including VAX formatted data files (a platform and format abandoned by the PDS), a challenging radiometric calibration, and the absence of a rigorous camera/sensor model, and/or data products that have been orthorectified or spatially controlled relative to SSI observations or more recent Cassini data products (e.g., VIMS). NIMS data are also not easily accessible by the planetary community. Before this work, NIMS data were only compatible with ISIS2, a program no longer supported by the USGS and no longer functions on some modern computer operating systems (e.g., Apple OS X). Galileo NIMS data were also not compatible with mainstream planetary software, including ENVI/IDL or ISIS3. This effort transitioned the data set to ISIS3 and thereby ISIS3 support interfaces. The NIMS PDS archive contains tube and g-cube data derived from the EDRs. Considering the relatively small scope of this effort only the NIMS tube and g-cube product data are the focus of this work. The objective of this work is to reformat and re-archive the Galileo NIMS data set into a more easily accessible data format. In order to do this we outlined three basic objectives: Objective 1: Create an ISIS3 application that reads and converts the NIMS data cubes into native ISIS3 cubes. NIMS data in the PDS is stored in VAX FLOAT format which is mostly obsolete and not widely used in the community any longer. This objective would ential adding support for conversion of VAX FLOAT to IEEE FLOAT in ISIS; advantageous to the pursuit is existing code in ISIS2 that provided a basis for this work. Here we also sought to seek out problems with the NIMS labels in PDS archive that are not compliant with PDS4 standards. These labels errors are to then be corrected and exported with properly formed labels to the PDS archive. Objective 2: Provide the ability to project NIMS tubes using the existing NIMS latitude, longitude tube backplanes. Objective 3: Derivation of a PDS4 compliant archive of the results of our study and provide it to the PDS for general distribution. These basic initial steps will make NIMS more user friendly and provide active support through ISIS help interfaces.
• collection: Galileo PPR Pre-Jupiter Raw Asteroid Ida Data Collection
  This collection contains the raw data for the Galileo Orbiter PPR instrument for the period corresponding to the Ida asteroid encounter observations in October 1993.
• collection: Small Bodies Radar Shape Models V1.0
  This data set contains radar-based shape models for small solar system bodies, prepared by various authors.