NSSDCA ID: PSSB-01122
Availability: Archived at NSSDC, accessible from elsewhere
This description was generated automatically using input from the Planetary Data System.
Dataset Overview ================= This CODMAC level 4 data set contains solar stray light corrected, radiometric calibrated and geometric distortion corrected (resampled) image data in W/m^2/sr/nm, acquired by the OSIRIS Narrow Angle Camera on the Rosetta spacecraft during the COMET ESCORT 3 mission phase, covering the period from 2015-08-25T23:25:00.000 to 2015-09-22T23:24:59.000 All header keywords are defined and described in the OSIRIS SIS: DOCUMENTSISOSIRIS_SIS_V05.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_V05.PDF: Describes the OSIRIS PDS header SCIENCE_USER_GUIDE_V03.PDF: Describes the intention behind the acquisition of each image and its planned scientific purpose. Related Datasets ================= The following PDS datasets are related: RO-C-OSINAC-2-ESC3-67PCHURYUMOV-M20-V3.0 RO-C-OSINAC-3-ESC3-67PCHURYUMOV-M20-V3.0 RO-C-OSINAC-4-ESC3-67P-M20-REFLECT-V1.0 RO-C-OSINAC-4-ESC3-67P-M20-STR-REFL-V1.0 RO-C-OSINAC-4-ESC3-67PCHURYUMOV-M20-V2.0 RO-C-OSINAC-5-ESC3-67P-M20-GEO-V1.0 RO-C-OSIWAC-2-ESC3-67PCHURYUMOV-M20-V3.0 RO-C-OSIWAC-3-ESC3-67PCHURYUMOV-M20-V3.0 RO-C-OSIWAC-4-ESC3-67P-M20-REFLECT-V1.0 RO-C-OSIWAC-4-ESC3-67P-M20-STR-REFL-V1.0 RO-C-OSIWAC-4-ESC3-67P-M20-STRLIGHT-V1.0 RO-C-OSIWAC-4-ESC3-67PCHURYUMOV-M20-V2.0 RO-C-OSIWAC-5-ESC3-67P-M20-GEO-V1.0 Please note that different datasets can contain different number of images. For details see OSIRIS_CAL_PIPELINE_V06.PDF and SCIENCE_USER_GUIDE_V03.PDF. Change log ========== V1.0 Lien corrected dataset after October 2018 PSA/PDS external peer review.
These data are available on-line from the Planetary Data System (PDS) at:
https://pdssbn.astro.umd.edu/holdings/ro-c-osinac-4-esc3-67p-m20-strlight-v1.0/
Questions and comments about this data collection can be directed to: Dr. David R. Williams
Name | Role | Original Affiliation | |
---|---|---|---|
Mr. Holger Sierks | Data Provider | Universitat Kiel | sierks@linmpi.mpg.de |
Dr. Cecilia Tubiana | General Contact | Max-Planck-Institut fur Sonnensystemforschung | tubiana@mps.mpg.de |