This page summarizes information about the selected resource and its origin based on SPASE metadata.
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The Ultraviolet Imager (UVI) is a small camera that detected and produced images of the ultraviolet light of the aurora, day and night. Using any of five specially designed filters the UVI camera imaged an eight degree circular field of view. Images are generated once every 37 seconds with a nominal pixel angular resolution of 0.036 degrees.
The Polar Ultraviolet Imager (UVI) Home Page contains links that describe the instrument, its operation, allow the user to view 36 second images and key parameter mosaics from the mission and download software, plus links to the UVI data archive, to lists of UVI publications and presentations, and several miscellaneous mission sites.
| Role | Person | |
|---|---|---|
| 1. | Principal investigator | Prof. George K. Parks |
| 2. | Metadata contact | Peggy Sloan |
FTP repository of Polar Level 1 UVI image data in CDF format at CDAWeb. This repository mirrors data from NSSTC.
The image array with instrument CCD pixel values.
All elements contain image pixel values.
| Bin | Band name | Low wavelength | High wavelength |
|---|---|---|---|
| 1 | 1304 filter | 125 | 135 |
| 2 | 1356 filter | 128 | 142 |
| 3 | LBHS filter | 135 | 160 |
| 4 | LBHL filter | 160 | 190 |
| 5 | SOLR filter | 175 | 190 |
Timestamp of first major frame of image
Spacecraft truncated Julian date
Spacecraft time
Microchannel plate voltage
Baseplate temperature
Primary detector electronics temperature
Secondary detector electronics temperature"
Optical bench temperature
Baffle temperature (spacecraft)
Radiator temperature
Stack housing temperature (spacecraft)
Stack electronics temperature (spacecraft)
Metering panel temperature
Top panel temperature
Secondary sensor panel temperature
Bottom panel temperature
Baffle temperature (operational)
Filter wheel motor temperature
CCD temperature
Detector case temperature
Stack housing temperature (operational)
Stack electronics temperature (operational)
High voltage power supply temperature
+5 voltage monitor
+5 current monitor
+15 voltage monitor
-15 voltage monitor
+15 current monitor
-15 current monitor
Data quality suspect flag
0=OK 1=Suspect
System ID
0=PRIMARY, 1=SECONDARY
Filter
0=HOME 1=1304 2=1356 3=LBHS 4=LBHL 5=SOLR 6=SHUTTER 7=UNK
Mirror position
0=NOTFULL 1=FULLEXT
Aperture door position
0=UNK 1=FULLEX 2=OPEN 3=CLOSED
Gain step
High voltage power supply enable
0=DISABLED 1=ENABLED
Instrument operating mode
0=UNK 1=NORMAL 2=STAR 3=IDLE 64-67=SYNC
Actual integration period
Valid numbers: 1, 2, 4
Observation sequence number
Sequence step number
Number of images to record with current gain/filter
Sequence pass count (loop counter)
Nominal integration period
Valid numbers: 1, 2, 4, 5, 6
UVI Telemetry Mode
0=Science 1=Maneuver 2=Contingency 3=Engineering
Safe mode enable
0=Disabled 1=Enabled
Platform Lock
0=Locked 1=Out of lock
Image number
Valid numbers: 1,2
Mode table in use
# frames summed for image
# spin pulse per image acquisition
# of frames to sum
# images every 4 major frames
Valid numbers: 1,2
# detector rows per image
Starting detector row
# detector rows per line readout
Valid numbers: 1,2,3
Structure padding
Structure padding
Integration time = msec/10
Delta time offset from spin pulse=msec/2
Delta time from top of major frame 1=msec/10
Spacecraft spin rate=msec/2
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The ultraviolet imager is an ultraviolet imaging camera designed to obtain global images of the aurora at several selected wavelengths with a time resolution of 60 s, a spatial resolution of 10 km at a spacecraft altitude of 9 RE, and sensitivities of 100-300 rayleighs per count in each pixel. The objective is to provide coherent information on the total energy influx to the atmosphere, the characteristic energy of the precipitating particles, their spatial extent and structure, and various other parameters such as activity indices. This investigation utilizes two UV optical channels, one in the near ultraviolet (NUV) and one in the vacuum ultraviolet (VUV). The electronics subsystem is shared with the Visible Imaging System (VIS) investigation, as is the front-optics system used to point the instrument and to avoid the sunlit limb of the earth which is very bright in the visible. The combined instrument comprises primary and secondary optics, electromechanical devices for mirror and aperture control and filter selection, optical filters, image-intensified CCD sensor arrays with thermoelectric cooling, power converters and distribution circuits, and data, attitude and command processors. The instrument is mounted on the despun platform and normally directed in or near the nadir direction. The imaging field of view is directed by the earth-finding mirror to different sectors within the 20 x 36 degree instrument observing field. The VUV (vacuum ultraviolet) covers six wavelengths from 120.0 to 180.0 nm, and the NUV (near ultraviolet) covers five wavelengths from 247.0 to 337.1 nm.
Information about the Ultraviolet Imager (UVI) experiment on the Polar mission.
| Role | Person | |
|---|---|---|
| 1. | Principal investigator | Prof. George K. Parks |
SPASE version 2.0.0
POLAR is one of four spacecraft in the Global Geospace Science (GGS) program. These are among the six spacecraft in the International Solar Terrestrial Physics (ISTP) program. POLAR provides multi-wavelength imaging of the aurora, measuring plasma entry into the polar magnetosphere and geomagnetic tail, the flow of plasmas to and from the ionosphere, and the deposition of particle energy in the ionosphere and upper atmosphere. POLAR has on-board propulsion systems and a design lifetime of three to five years, with redundant subsystems. POLAR is cylindrical, approximately 2.8 m in diameter by 1.25 m high (plus 1.25 m for its two despun platforms), with body-mounted solar cells, weighs 1250 kg and uses 333 W of power. The spin rate is 10 rpm around an axis approximately normal to the orbital plane. It has long wire spin-plane antennas, inertial booms, and spin-plane appendages to support sensors. POLAR has two despun gimbaled instrument platforms, and booms are deployed along both Z axes. Data are stored using on-board tape recorders and are relayed to the Deep Space Network at 600 kbps maximum (250 kbps nominal) although the average real-time data rate for POLAR is 41.6 kbps. POLAR has a 22.6-h polar orbit (90 deg inclination), with perigee and apogee of 11,500 and 57,000 km. Polar was launched to observe the polar magnetosphere and, as its orbit has precessed with time, has observed the equatorial inner magnetosphere and is now carrying out an extended period of southern hemisphere coverage. Details on the POLAR mission and instrumentation are provided in Space Science Reviews (Vol. 71, Nos. 1-4, 1995) and reprinted in The Global Geospace Mission, edited by C. T. Russell (Kluwer, 1995).
Web site of NASA Polar Mission, including overview, data products, FTP to the data, publications, educational outreach, orbits, instrument descriptions, contacts, news archive, and ISTP archive.
Information about the Polar mission
| Role | Person | |
|---|---|---|
| 1. | Project scientist | Dr. John B. Sigwarth |
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Polar UVI Resident Archive web server and data archive located at the National Space Science and Technology Center (NSSTC) in Huntsville, Alabama.
The Polar Ultraviolet Imager (UVI) Home Page contains links that describe the instrument, its operation, allow the user to view 36 second images and key parameter mosaics from the mission and download software, plus links to the UVI data archive, to lists of UVI publications and presentations, and several miscellaneous mission sites.
| Role | Person | |
|---|---|---|
| 1. | Principal investigator | Prof. George K. Parks |
| 2. | General contact | Dr. Paul D. Craven |
| 3. | Metadata contact | Peggy Sloan |
The UVI Data Archive contains UVI data and plot files including level-one (l1), orbit (or), attitude (at), and pitch angle (pa) CDF files, and the 36-second UVI Image gif files (gifs). The files are stored by year/doy-of-year in the subdirectories in parentheses. All of the CDFs are also available at the CDAWeb. The archive also contains the key parameter mosaic gif/png files and software.
SPASE version 1.2.0
Coordinated Data Analysis Web (CDAWeb) supports not only interactive plotting of variables from multiple instruments on multiple investigations simultaneously on arbitrary, user-defined time-scales. It also supports data retrieval in various formats using its interactive web interface or ftp service.
Coordinated Data Analysis Web (CDAWeb) home page at Space Physics Data Facility of the NASA Goddard Space Flight Center.
| Role | Person | |
|---|---|---|
| 1. | Project scientist | Dr. Robert E. McGuire |