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Getting and Using SSUSI Data f rom the SSUSI Website, and Website Features. Robert Schaefer and Giuseppe Romeo for the SSUSI team Robert Schaefer Giuseppe Romeo Robert.Schaefer@jhuapl.edu Giuseppe.Romeo@jhuapl.edu 240-228-2740 240-228-5905. Overview.
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Getting and Using SSUSI Data from the SSUSI Website, and Website Features Robert Schaefer and Giuseppe Romeo for the SSUSI team Robert Schaefer Giuseppe Romeo Robert.Schaefer@jhuapl.eduGiuseppe.Romeo@jhuapl.edu 240-228-2740 240-228-5905
Overview • How to do analysis with SSUSI data • SSUSI Web and features
How to Analyze SSUSI data • So you have an idea to investigate some upper atmospheric phenomenon – what do you do now? • First, Identify time period of the data you want. • Second, identify the appropriate data product(s) you need. • Third, Retrieve the data • Fourth, identify Variables that have the information you want • Fifth, identify any quality issues • Sixth, Read and access the data
1. Identify the Time Period • If you have a pre-defined time period, see discussion of data availability page coming up later to determine what data exist for the period • If not, the SSUSI Website can help • L1B Daily Summaries – found in the SSUSI Gallery • http://ssusi.jhuapl.edu/images_daily_l1b • 3 color images to represent 3 UV color images • Red = LBH Short • Green = 1356 Å • Blue = 1304 Å • Variety of perspectives
SSUSI L1B daily Summary Gallery • Time frame, satellite, date • Slideshow • Perspective • GUVI web site will soon look like this, too. • Can see many features of interest
Features in Summary image • Brightness of color corresponds to UV color intensity • Equatorial Ionosphere • White means all three colors are bright.
Other perspectives available in Summary • Stacked Limb Plots • Stacked Disk Plots • Polar view plots • Orthographic perspectives • Can go browsing for features Stacked Limb Plot Equatorial ionosphere Aurora Dayglow Aurora Polar Perspective Plot
If you need want higher time resolution browse Google Earth galleries • Require Google Earth plugin (freely downloadable from Google)
2. Identify Data Products You need • Electron Density • Low Latitude Electron Density Profiles • Nightside • 3D density cube: EDR-IONO • Bubbles and Characteristics: EDR-IONO • Mutual neutralization corrected profile: EDR-NIGHT-LIMB • Dayside • Topside density (only above 400 km): EDR-DAY-LIMB • Disk F-region NmF2, HmF2 is an unvalidated product – use at your own risk: EDR-DAY-DISK • High Latitude Electron Density Profiles • E-Region densities: EDR-AURORAL • Dayside Neutral Densities: • O/N2: EDR-DAY-DISK • Solar Extreme UV Flux • Qeuv: EDR-DAY-DISK
Identify Products (for the polar region analysis) • Auroral Zone products - All are in the: EDR-AURORAL • Precipitating electron energy flux (Q) and mean energy (E0) (conductances!) • Hemispheric Power • Regions of proton precipitation • Auroral boundaries (poleward, equatorward),(global/pixelated) • Discrete arc locations • Magnetic field lines from the auroral boundary • Auroral Oval predition –EDR-AURORA-PRED • New product (not validated) gives predicted auroral energy flux, mean energy and boundary
3 Retrieve the Data • Single files are clickable • Case where you want more than one file will be discussed later
Data Availability – for the future • DMSP program is winding down – one more SSUSI to launch (2016?) • Long term data support> • NASA: Space Physics Data Facility – http://spdf.gsfc.nasa.gov • CDAwebhttp://cdaweb.gsfc.nasa.gov/istp_public/ • Virtual ITM Observatory – http://vitmo.jhuapl.edu
4. Identify Variables Needed • Separate Document discusses this - Here we give an overview • Coordinates • Low latitude Disk – PiercepointLatitude, Longitude at • Night Altitude 350 km • Day Altitude: 150 km • Auroral Altitude: 110 km • Low Latitude Limb – Tangentpoint Latitude, Longitude, and Altitude • Auroral Zone – Geographic and Magnetic Coordinates available • Magnetic Latitude and Magnetic Local Time • Time • Year, DOY, and Seconds of the day • Note seconds of the day called “TIME” in all files except AURORAL files where it is called UT (actually UT_N for northern hemisphere magnetic coordinates and UT_S for southern hemisphere coordinates) • Other variables more specific to the product and type of analysis
Example DQI • EDR-NIGHT-LIMB • DATA_QUALITY variable is an array – 1 per pixel Bit # Meaning if set to true (1) 0 VER fit unsuccessful (chi squared test: rchi2v>10) • Chapman fit unsuccessful (chi squared test: rchi2c>10) • NmF2 uncertainty > 50% • HmF2 < 0 km • HmF2 > 500 km • HmF2 uncertainty > 50% • NRP < 7 • SZA < 105 degrees • MeV contamination 9-15 Spare
5. Data Quality Issues • Data Quality Indices – Integers used as bit fields • Individual bits have meaning for different failure conditions • Designed so that 0=good, 1=bad • Simplest thing to do: • Evaluate as integers • Throw away anything that is not 0 • Other Data indicators • Aurora – sometimes files only cover one hemisphere • SOUTH_DATA, NORTH_DATA are set to 1 if Data exists for the SOUTH, NORTH hemispheres, 0 if no data. • Variables can be checked to see if any useful data exists • Also Pixels with no data are set to IEEE NaN value to prevent accidental use in averages • no problem for IDL programmers • Good_data_indices= where(finite(variable_arrary))
6. Read and Access Data • IDL Software tools available (http://ssusi.jhuapl.edu/software_tools) • These allow you to read and plot data • Libraries in many computer language for reading NetCDF available from Unidata UCAR web site (http://www.unidata.ucar.edu/software/netcdf/index.html) • Most useful utility we have found: read_ncdf.pro • Reads in everything in the file and populates an idl structure with a single call • Variable names become tags in the structure • Reads in all global header information, including geophysical indices supplied by the Air Force in realtime • Plotting routines show examples of reading and manipulating most useful variables
SSUSI Website • Most of the content is available to the general public, some is restricted to registered users • New interface/New tools
New Features for SSUSI website • Data Availability • Data Retriever • Image Galleries (including Google Earth KMZ file) • Enhanced Data Retriever (registered users ONLY) • Software tools
SSUSI Data Availability(http://ssusi.jhuapl.edu/data_availability)
Daily Data Retriever (http://ssusi.jhuapl.edu/daily_data_retriever) • To prevent abuse by robots, only registered users can retrieve data for periods longer than 1 orbit. • For Longer Periods than a day, need to request them by e-mail to one of us on the SSUSI team • Compressed files covering a range of dates can be downloaded by registered users.
User Requested Data Archive(http://ssusi.jhuapl.edu/data_archive)
Daily Summary Images(http://ssusi.jhuapl.edu/images_daily_l1b)
EDR-AURORAL KMZ gallery(http://ssusi.jhuapl.edu/gal_edr-aur)
GUVI New Data Products • Thermospheric O/N2 Gallery • Level 1B Spectrograph Gallery • Thermospheric O/N2 Gallery and Total Electron Control • SSUSI-Like EDR-AURORAL, EDR-IONOSPHERE, SDR
GUVI Thermospheric O/N2 Gallery(http://guvi.jhuapl.edu/site/gallery/guvi-galleryl3on2.shtml)
GUVI Level 1B Spectrograph Gallery(http://guvi.jhuapl.edu/site/gallery/guvi-galleryl1bspec.shtml)
GUVI Thermospheric O/N2 Gallery and TEC(http://guvi.jhuapl.edu/site/gallery/guvi-galleryl3on2tec.shtml)
SSUSI Like EDR-AURORAL(http://guvi.jhuapl.edu/site/gallery/NewProduct/edr-aur/guvi-gallery.shtml)
SSUSI Like EDR-IONOSPHERE(http://guvi.jhuapl.edu/site/gallery/NewProduct/edr-iono/guvi-gallery.shtml)
SSUSI Like SDR(http://guvi.jhuapl.edu/site/gallery/NewProduct/sdr/guvi-gallery.shtml)
What’s to come, funding permitting! • New web interface for GUVI • NetCDF 4 (compressed and browseable format) • Simpler Filenaming scheme • Solar Storm alert based on Auroral SSUSI data