timed/guvi data for iri r. demajistre, l.j. paxton, d. bilitza and h.kil
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TIMED/GUVI Data for IRI R. DeMajistre, L.J. Paxton, D. Bilitza and H.Kil. IRI 2005. GUVI for the ionosphere. What is TIMED/GUVI Measurement methods for the nighttime ionosphere Ionosonde validation Application – Calibration transfer GUVI and IRI. - PowerPoint PPT PresentationTRANSCRIPT
TIMED/GUVI Data for IRIR. DeMajistre, L.J. Paxton, D. Bilitza and H.Kil
IRI 2005
GUVI for the ionosphere
• What is TIMED/GUVI
• Measurement methods for the nighttime ionosphere
• Ionosonde validation
• Application – Calibration transfer
• GUVI and IRI
Motivation for future work and collaboration rather than final results
GUVI - Global UV Imager
• Scanning Spectrographic Imager
• Covers 115-180 nm in 160 nm spectral bins
• 14 cross track spatial pixels act as a linear array
TIMED Spacecraft
• High inclination circular orbit, ~625 km altitude
• Covers all local times in 60 days
• Nightside passes ~25 degrees apart
Nightside measurements
Dayside radiance
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GUVI Colors
• GUVI ‘colors’ summed on board – 5 bright FUV spectral features
• Only 2 colors are usually detected at night
• Color 3, 135.6 nm, due almost entirely from F region recombination
Disk MeasurementsGUVI
F Layer
• GUVI down-looking pixels yield slant column brightness through the F Layer
• Can be converted to TEC with some assumptions about profile shape
• Very high spatial resolution (~ 25x25 km) reveals bubbles and irregularities
Composite 135.6 nm image for day 82, 2002
Limb Measurements
• First 32 steps of each scan are on the limb (100 – 520 km)
• Constrained linear inversion yields volume emission rate/electron densities
Systematic monitoring of the nighttime F Region
Monitoring the IonosphereCoverage• Altitude – Each scan, 150 – 500 km• Latitude – Each orbit• Longitude – Each day• Local time – 60 days• Over 3 years of data yields seasonal coverage as well
Limits• Low signal levels away from the anomalies• Assumption of spherical symmetry• Recombination rate is uncertain• Assumes one constituent ionosphere (O+)
Global Observations
• Electron densities can be used to estimate NMF2
• Coverage allows global maps
• Orbit precession rate allows inter-annual comparisons
• Can be compared directly with ionosonde data or IRI
Ionosonde Comparisons
• GUVI electron density profile fit with a Chapman layer
• NMF2 and HMF2 taken directly from the fit
• Same process can be used with IRI
Ionosonde DataStation Lat. Long.
Juliusruh, Germany 54.6 13.4
Wakkanai, Japan 45 141
Ebro, Spain 40.8 0.5
Kokubunji, Japan 35 139
Yamagawa, Japan 31 130
Delhi, India 28.6 77.2
Okinawa, Japan 26 128
Waltair, India 17 83
Trivandrum, India 8.3 76.6
Sao Luis, Brazil -2.3 315.8
Fortaleza, Brazil -3.9 321.5
C. Paulista, Brazil -22.7 315
B. Aires, Argentina -34.6 301.7
Concepcion, Chile* -36.8 287
Cachimbo, Brazil -9.5 305.2
• Ionosonde Data Supplied to from the various stations
• Data from other stations was supplied but had no suitable GUVI coincident measurement
GUVI Selections
Criteria for selecting coincidences
• Within 200 km and 20 minutes
• Chapman layer fit successful– Good fit to data– Realistic HMF2 and NMF2
• No ‘qualifying letters’ on ionosonde data
427of 1112 observations met these criteria
• GUVI and IRI have similar spread (~30-40%)
• GUVI compares well between 0.5 and 1.0 (106 cm-3)
• IRI bias similar in shape to GUVI
• Both GUVI and IRI show ‘discontinuity’ at 1.0 (106 cm-3)
IRI/GUVI comparison
• Similar spread as (~30%)
• At higher NMF2, GUVI systematically low
• Slope of bias is constant (suggests calibration of GUVI is reasonable)
Conclusion of comparisons
• At moderate NMF2, GUVI predicts ionosonde measurements with 30% or so
• In the same range, IRI behaves the same way with a fairly large positive bias
• At larger NMF2 both under-predict
Calibration Transfer
• The issue – Ionosonde intercalibration– Various instrument designs– Separate calibrations– Independently operated
• Example solution – Ozone monitors– ‘Standard instrument’ carried from site to site– Makes simultaneous measurements
• Suggested approach – Orbiting UV monitoring– Use GUVI (and/or its successors) to transfer
calibration
Regional Analysis - significant geographic differences
Inter-ionosonde Comparisons
• Significant differences between stations
• Significant regional differences
• GUVI statistics can be used to identify areas that may need attention– In principle, GUVI measurements should
have little geographic dependence– Geographic differences in profile shapes and
horizontal gradients may have some influence
GUVI and IRI - Conclusions
• GUVI can provide systematic observations– Can be used to compare with IRI– Once differences are understood,
observations can be included in IRI
• GUVI can be used to refine ionosonde measurements– Provide better IRI validation– Provide better IRI input