PDS_VERSION_ID = PDS3 DATA_SET_ID = "MEX-M-MARSIS-5-DDR-SS-TEC-EXT1-V1.0" PRODUCT_ID = "IONOPROCESS_REPORT3" PRODUCT_CREATION_TIME = 2009-04-22T14:00 RECORD_TYPE = FIXED_LENGTH RECORD_BYTES = 80 RELEASE_ID = 0001 REVISION_ID = 0000 ^PDF_DOCUMENT = "IONOPROCESS_REPORT3.PDF" ^ASCII_DOCUMENT = "IONOPROCESS_REPORT3.ASC" ^PNG1_DOCUMENT = "IONOPROCESS_REPORT3_EQU1.PNG" ^PNG2_DOCUMENT = "IONOPROCESS_REPORT3_EQU2.PNG" ^PNG3_DOCUMENT = "IONOPROCESS_REPORT3_FIG1.PNG" ^PNG4_DOCUMENT = "IONOPROCESS_REPORT3_FIG2.PNG" ^PNG5_DOCUMENT = "IONOPROCESS_REPORT3_FIG3.PNG" OBJECT = PDF_DOCUMENT DOCUMENT_NAME = "MARSIS DERIVED ENHANCED IONOSPHERIC CALIBRATION DATA" DOCUMENT_FORMAT = "ADOBE PDF" DESCRIPTION = "A planetary ionosphere is a perturbing environment for radar waves. Unfortunately, it is an unavoidable obstacle along the propagation path of signals emitting by orbiting radar sounders. The Mars Advanced Radar for Subsurface and Ionospheric Sounding (MARSIS) isan instrument onboard the European Space Agency's Mars Express spacecraft. In order to deeply penetrate the surface, MARSIS operates at MHz frequencies for which the perturbations due the Martian ionosphere can be significant. Therefore, prior to any analyze, MARSIS data need to be corrected from the ionospheric effects. The MARSIS derived enhanced ionospheric calibration dataset enables to correct the MARSIS signal from the ionospheric distortio. The aim of this document is to provide information on the generation and the description of the parameters forming this derive dataset, and to explain their use when needed." DOCUMENT_TOPIC_TYPE = "DERIVATION AND ANALYSIS TECHNIQUES" INTERCHANGE_FORMAT = "BINARY" PUBLICATION_DATE = 2009-04-22 END_OBJECT = PDF_DOCUMENT OBJECT = ASCII_DOCUMENT DOCUMENT_NAME = "MARSIS DERIVED ENHANCED IONOSPHERIC CALIBRATION DATA" PUBLICATION_DATE = 2009-04-22 DOCUMENT_TOPIC_TYPE = "DERIVATION AND ANALYSIS TECHNIQUES" INTERCHANGE_FORMAT = ASCII DOCUMENT_FORMAT = TEXT DESCRIPTION = "A planetary ionosphere is a perturbing environment for radar waves. Unfortunately, it is an unavoidable obstacle along the propagation path of signals emitting by orbiting radar sounders. The Mars Advanced Radar for Subsurface and Ionospheric Sounding (MARSIS) isan instrument onboard the European Space Agency's Mars Express spacecraft. In order to deeply penetrate the surface, MARSIS operates at MHz frequencies for which the perturbations due the Martian ionosphere can be significant. Therefore, prior to any analyze, MARSIS data need to be corrected from the ionospheric effects. The MARSIS derived enhanced ionospheric calibration dataset enables to correct the MARSIS signal from the ionospheric distortio. The aim of this document is to provide information on the generation and the description of the parameters forming this derive dataset, and to explain their use when needed." END_OBJECT = ASCII_DOCUMENT OBJECT = PNG1_DOCUMENT DOCUMENT_NAME = "IONOPROCESS_REPORT3_EQU1.PNG" PUBLICATION_DATE = 2009-04-22 DOCUMENT_TOPIC_TYPE = "DERIVATION AND ANALYSIS TECHNIQUES" FILES = 1 ENCODING_TYPE = PNG INTERCHANGE_FORMAT = BINARY DOCUMENT_FORMAT = PNG DESCRIPTION = "Equation (1) from the document IONOPROCESS_REPORT3" END_OBJECT = PNG1_DOCUMENT OBJECT = PNG2_DOCUMENT DOCUMENT_NAME = "IONOPROCESS_REPORT3_EQU2.PNG" PUBLICATION_DATE = 2009-04-22 DOCUMENT_TOPIC_TYPE = "DERIVATION AND ANALYSIS TECHNIQUES" FILES = 1 ENCODING_TYPE = PNG INTERCHANGE_FORMAT = BINARY DOCUMENT_FORMAT = PNG DESCRIPTION = "Equation (2) from the document IONOPROCESS_REPORT3" END_OBJECT = PNG2_DOCUMENT OBJECT = PNG3_DOCUMENT DOCUMENT_NAME = "IONOPROCESS_REPORT3_FIG1.PNG" PUBLICATION_DATE = 2009-04-22 DOCUMENT_TOPIC_TYPE = "DERIVATION AND ANALYSIS TECHNIQUES" FILES = 1 ENCODING_TYPE = PNG INTERCHANGE_FORMAT = BINARY DOCUMENT_FORMAT = PNG DESCRIPTION = "Fig. 1. Data processing executed for each frame. The results are the parameters [a1 ; a2 ; a3] and TEC." END_OBJECT = PNG3_DOCUMENT OBJECT = PNG4_DOCUMENT DOCUMENT_NAME = "IONOPROCESS_REPORT3_FIG2.PNG" PUBLICATION_DATE = 2009-04-22 DOCUMENT_TOPIC_TYPE = "DERIVATION AND ANALYSIS TECHNIQUES" FILES = 1 ENCODING_TYPE = PNG INTERCHANGE_FORMAT = BINARY DOCUMENT_FORMAT = PNG DESCRIPTION = "Fig. 2. The signal to noise ratio (down) for the MARSIS orbit 2503 (up). The red-dashed line indicates the defined SNR-threshold of 15 dB. All the frames lower than this value have a 'flag' equals to zero." END_OBJECT = PNG4_DOCUMENT OBJECT = PNG5_DOCUMENT DOCUMENT_NAME = "IONOPROCESS_REPORT3_FIG3.PNG" PUBLICATION_DATE = 2009-04-22 DOCUMENT_TOPIC_TYPE = "DERIVATION AND ANALYSIS TECHNIQUES" FILES = 1 ENCODING_TYPE = PNG INTERCHANGE_FORMAT = BINARY DOCUMENT_FORMAT = PNG DESCRIPTION = "Fig. 3. Example of the plot provided for the orbit 2503 (see text for details)." END_OBJECT = PNG5_DOCUMENT END