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Data Sets and Information
• collection: CRISM ATO S-Band LMLP Data Collection
  CRISM ATO S-Band map projected images with log maximum likelihood processing
• 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: Document collection for Arizona State University Ronald Greeley Center for Planetary Studies - The Ronald Greeley 35mm Slide Collection, The Jovian System, Ganymede
  This collection, included in document_ganymede, consists of 108 digitized 35mm slides primarily of Ganymede, Galilean Satellite of Jupiter, and other related bodies. 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 ganymede_diagram_database.pdf and ganymede_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: 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.
• collection: CRISM ATO S-Band NLML Data Collection
  CRISM ATO S-Band sensor space images without log maximum likelihood processing
• 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: 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.
• instrument host: NEW HORIZONS
  Information about the NEW HORIZONS instrument host
• instrument host: MARS EXPRESS
  Information about the MARS EXPRESS instrument host
• instrument host: GALILEO ORBITER
  Information about the GALILEO ORBITER instrument host
• collection: CRISM ATO S-Band LML Data Collection
  CRISM ATO S-Band sensor space images with log maximum likelihood processing
• collection: CRISM ATO S-Band NLMLP Data Collection
  CRISM ATO S-Band map projected images without log maximum likelihood processing
• bundle: Galileo Near-Infrared Mapping Spectrometer Encounter Guide PDF/A Bundle
  PDF/A versions of the original PostScript files from the GLL NIMS Encounter Guides.
• bundle: CRISM ATO S-Band Log Maximum Likelihood Method Bundle
  CRISM ATO S-Band Maximum Likelihood Method Bundle
• collection: CRISM ATO S-Band Browse Collection
  CRISM ATO S-Band sensor space browse images
• collection: CRISM ATO S-Band Maximum Likelihood Method Document Collection
  CRISM ATO S-Band Maximum Likelihood Method Document Collection
• collection: Document collection for Arizona State University Ronald Greeley Center for Planetary Studies - The Ronald Greeley 35mm Slide Collection, The Jovian System, Callisto
  This collection, included in document_callisto, consists of 129 digitized 35mm slides primarily of Callisto, Galilean Satellite of Jupiter, and other related bodies. 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 callisto_diagram_database.pdf and callisto_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: 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: CRISM ATO S-Band LMLP_PARAM Data Collection
  CRISM ATO S-Band map projected spectral parameters
• collection: Collection of document products: PDS4 Galileo NIMS Encounter Guides Collated into PDF/A Products
  Collection of DOCUMENT products used in this archive.
• collection: Document collection for Arizona State University Ronald Greeley Center for Planetary Studies - The Ronald Greeley 35mm Slide Collection, The Jovian System, Io
  This collection, included in document_io, consists of 292 digitized 35mm slides primarily of Io, Galilean Satellite of Jupiter, and other related bodies. 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 io_diagram_database.pdf and io_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: 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: Document collection for Arizona State University Ronald Greeley Center for Planetary Studies - The Ronald Greeley 35mm Slide Collection, The Jovian System, Europa
  This collection, included in document_europa, consists of 484 digitized 35mm slides primarily of Europa, Galilean Satellite of Jupiter, and other related bodies. 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 europa_diagram_database.pdf and europa_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: Arizona State University Ronald Greeley Center for Planetary Studies - The Ronald Greeley 35mm Slide Collection, The Jovian System
  This collection, document_database, consists of ten databases that describe information contained in the 1258 digitized 35mm slides of Jupiter, the Galilean Satellites, and miscellaneous objects. Information includes the location, subject matter, mission, and if the digitized slide was of a photograph or a diagram used for presentation/education purposes. Digitized images of the photographs are in the collections document_callisto, document_europa, document_ganymede, document_io, and document_jovian_system_and_misc also in this bundle. The digitized slides are identified whether they are a diagram or a photograph and are listed in separate descriptive databases (e.g., europa_diagram_database.pdf and europa_photo_database.pdf) but are inventoried in a single document (e.g., collection_document_europa_inventory.csv). The slides and information about them are from the Dr. Ronald Greeley archive at the Arizona State University Regional Planetary Image Facility, Tempe, Arizona.
• collection: CRISM ATO S-Band LML_PARAM Data Collection
  CRISM ATO S-Band spectral parameters in sensor space
• collection: Arizona State University Ronald Greeley Center for Planetary Studies - User's Guide for The Ronald Greeley 35mm Slide Collection, The Jovian System
  User's Guide to the ASU RGCPS Digitization of Dr. Ronald Greeley's 35mm Slide Collection, the Jovian System
• collection: CRISM ATO S-Band Maximum Likelihood Method Miscellaneous Collection
  CRISM ATO S-Band Maximum Likelihood Method Miscellaneous Collection