urn:nasa:pds:cassini-mimi-inca-cal:browse-iionang:iionang_h_2012053_009 1.0 1.20.0.0 Product_Browse Vandegriff, Jon; Kusterer, Martha B. 2024 INCA MIMI This file contains high time-of-flight (TOF) browse ion images displayed for seven time-of-flight ranges (rows) from the INCA sensor of the Cassini MIMI instrument. Ion images are collected when no voltage is present on the INCA collimator. 2024-07-02 1.0 This product, IIONANG0_H_2012053_009_02.PNG, was originally released as part of the CO-S-MIMI-4-INCA-CALIB-V1.0 PDS3 data set. The metadata have been migrated to PDS4. The data themselves are unchanged. 2012-02-22T09:05:47.000Z 2012-02-22T10:05:47.000Z Science Calibrated Cassini MIMI INCA Extended-Extended Mission Hydrogen High TOF Browse Heliosphere Magnetosphere Particles Ions Energetic Cassini-Huygens Mission urn:nasa:pds:context:investigation:mission.cassini-huygens browse_to_investigation Cassini Orbiter Host urn:nasa:pds:context:instrument_host:spacecraft.co is_instrument_host Magnetospheric Imaging Instrument for Cassini Orbiter Instrument urn:nasa:pds:context:instrument:mimi.co is_instrument MIMI Ion Neutral Camera for Cassini Orbiter Instrument urn:nasa:pds:context:instrument:mimi-inca.co is_instrument Saturn Planet urn:nasa:pds:context:target:planet.saturn browse_to_target 1708595812.000 1708599412.000 1 161 161 5 277 Ions Flux Proton urn:nasa:pds:cassini-mimi-inca-cal:data-iangave_t:iangave_t_2012053::1.0 browse_to_data CO-S-MIMI-4-INCA-CALIB-V1.0:IIONANG0_H_2012053_009_00:IIONANG0_H_2012053_009_02.PNG data_to_calibrated_source_product 10.17189/1519607 PDS Planetary Plasma Interactions Node This is the first version converted to PDS4. The DOI references the source PDS3 data set. IIONANG0_H_2012053_009_02.PNG 2017-09-21T04:07:36 70545 8ee5f5c29c9d7e4a7da9dd53c89c8b81 IIONANG0_H_2012053_009_00 0 PNG The image species include hydrogen at TOF ranges, where the energy range for each TOF range is shown to the right of each row. The value displayed is the log of the image intensity which is counts/(centimeters squared*steradian*seconds*keV). The color bars for each row are independent and are determined by the minimum and maximum pixels in that row (i.e., for the entire day). The definition of the thumbnail frame is the primary axis X is the INCA boresight axis which goes into the page. The secondary Z axis is the Z axis of Cassini. The Y-axis completes the left-handed system. The elevation of the image goes from -60 degrees at the bottom to 60 degrees at the top of the image. The azimuth of the image goes from -45 degrees on the left to 45 degrees on the right. Each original image was 16 x 16 pixels and was expanded to 60 x 80 pixels in the PNG file. The pitch angle of INCA is displayed on top of the image as contours for the following degrees [0,30,60,90,120,150,180] in the B-field particle flow. At the top of the page, the Rsaturn=radius to Saturn, Lat=latitude in IAU_SATURN frame, LT=Saturn Local Time, L=L value, local time of Cassini relative to Saturn, Lon skr-wl= Longitude of Cassini in the Saturn Kilometric Radiation (western longitude) frame. These measurements are calculated at the start time of the first image. The seven TOF range (each one accumulated over four sectors), four sector images are displayed one above each other for the same time. The highest TOF (TOF id 0) is not a well-behaved product so it was not included in the browse product. The channel is sensitive to background, electrons, and has variable sensitivity to ions in that energy range (greater sensitivity at the edges, highly spectral slope dependent, not calibratable). Time increases from left to right. The energy ranges for the high mass TOF resolution hydrogen range from high to low: (TOF id is the value in the TOF column in the angle average files and on the plot, TOF 1 is at the top). TOF id 1 = 149-360 keV TOF id 2 = 90-149 keV TOF id 3 = 55-90 keV TOF id 4 = 35-55 keV TOF id 5 = 24-35 keV TOF id 6 = 13-24 keV TOF id 7 = 5-13 keV Images, taken when Cassini is spinning about the Z axis, may be flipped horizontally depending on the spin direction. This insures that contiguous images line up properly. All images in a column are flipped or not flipped and this is indicated by a grey bar at the bottom. Grey equals flipped.