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CEDAR Workshop, Boulder CO June 20-25, 2010 Statistical Analysis of COSMIC Derived Abel Profiles Jet...
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Transcript of CEDAR Workshop, Boulder CO June 20-25, 2010 Statistical Analysis of COSMIC Derived Abel Profiles Jet...
CEDAR Workshop, Boulder CO June 20-25, 2010
Statistical Analysis of COSMIC Derived Abel
Profiles
Jet Propulsion LaboratoryCalifornia Institute of Technology
M/S 238-6004800 Oak Grove DrivePasadena CA 91109
Philip Stephens, Attila Komjathy, Brian Wilson, Xiaoqing Pi and Anthony J. Mannucci
CEDAR Workshop, Boulder CO June 20-25, 2010
Outline
• Introduction• Motivation for this study
• Analysis Framework• Results• Summary
CEDAR Workshop, Boulder CO June 20-25, 2010
Abel Inversion
• With F(y) the integrate line-of-site TEC and f(r) the altitude dependent density the Abel inversion is defined as
• Major assumption: For occultation measurements we have no horizontal gradients
– This is obviously false in reality– What is the impact of this assumption for real data?
• The Abel is extremely useful, however, as it provides some estimate of 3d structure from the data alone
CEDAR Workshop, Boulder CO June 20-25, 2010
Motivation for Study
• An effort was made to try use Abel profiles to develop a climatology
• Found important structure was ‘smeared’ no matter what averaging methods were used
• Hypothesis was the spherical symmetry of Abel inversion assumption would be broken in many cases
• Can we define some filter which can effectively provide a subset of potentially bad Abel inversions, with the members not in the subset all good inversions?
CEDAR Workshop, Boulder CO June 20-25, 2010
Analysis Framework
• Built database of Abel Profiles for 05/01/2010• Derived from 1 second TEC data, ~1400 profiles• Ap: 3.0, Kp: 1- very little solar activity
• Linked to database profiles generated by assimilation of COSMIC data into JPL/USC GAIM
• Used 30 second data for these results• Linked to database VTEC generated by GIM 3-shell model
• Ground data only• Slice profiles according to three criteria
• Low/Med/High Magnetic Latitude (±20, ±50, >50)• Dawn/Midday/Dusk/Midnight (3-9 LT, 9-15 LT, 15-21 LT, 21-24/0-3 LT)• Length of arc, measured by
with short/medium/long (±5, ±30,>30)• Computed Pearson Coefficient (r) and slope of line of best fit (m)• Hypothesis: Abel will break down most often when spherical
symmetry breaks down – large gradients and long spatial tracks
CEDAR Workshop, Boulder CO June 20-25, 2010
Filtering Arcs by Magnetic Latitude
Low lat (<20 degrees)
Mid lat (20<x<50 degrees)
High lat (>50 degrees)
CEDAR Workshop, Boulder CO June 20-25, 2010
Nmf2 and Hmf2 Correlation Plots
CEDAR Workshop, Boulder CO June 20-25, 2010
VTEC at High Latitude, Pearson Coefficient
CEDAR Workshop, Boulder CO June 20-25, 2010
Correlation Plots High Latitude
Long-arc, high lat, dusk
Long-arc, high lat, midday
Medium-arc, high lat, midnight
2
2
1
1
3
3
CEDAR Workshop, Boulder CO June 20-25, 2010
High Lat Correlations, Nmf2, Hmf2
CEDAR Workshop, Boulder CO June 20-25, 2010
Case 1: Long arc, High Lat, Dusk
CEDAR Workshop, Boulder CO June 20-25, 2010
Case 2: Long arc, High Latitude, Midday
CEDAR Workshop, Boulder CO June 20-25, 2010
Case 3: High lat, medium arc, midnight
CEDAR Workshop, Boulder CO June 20-25, 2010
Mid Latitude VTEC, Pearson Coefficient
CEDAR Workshop, Boulder CO June 20-25, 2010
Mid Latitude Correlation Plots
Mid latitude, midnight long arcs, only 5 points though
44
4
4
CEDAR Workshop, Boulder CO June 20-25, 2010
Case 4: Mid Lat, Long Arc, Midnight
CEDAR Workshop, Boulder CO June 20-25, 2010
Low Latitude VTEC, Pearson Coefficient
CEDAR Workshop, Boulder CO June 20-25, 2010
Correlation Plots Low Latitude
Long-arc, low lat, dusk
Long-arc, low lat, midday
6 6
55
CEDAR Workshop, Boulder CO June 20-25, 2010
Low Lat Correlation Plots, Hmf2, Nmf2
CEDAR Workshop, Boulder CO June 20-25, 2010
Case 5: Long arc, Low lat, Dawn
CEDAR Workshop, Boulder CO June 20-25, 2010
Case 6: Long arc, Low lat, Midday
CEDAR Workshop, Boulder CO June 20-25, 2010
Conclusions
• It does appear there is significantly more variability in comparing Abel profiles versus GAIM profiles in cases where spherical symmetry approximation is likely to breakdown
• This study was a test case of a very calm day• Expect more variability for more active days
• Still to do:• Extend study to multiple days with different conditions• Develop a measure of ‘physicality’ of profiles and apply to Abel
and GAIM profiles under different filters– Possibly using fits to Vary-Chapman function
• Measure effectiveness of suggested filters– E.g. what percentage of ‘bad’ profiles are captured by filters
• Important note: vast majority of profiles appear to correlate well to GIM VTEC and GAIM 3d structure
CEDAR Workshop, Boulder CO June 20-25, 2010
Backup slides
CEDAR Workshop, Boulder CO June 20-25, 2010
High Lat NmF2, Pearson Coefficient
CEDAR Workshop, Boulder CO June 20-25, 2010
Mid Lat, Nmf2, Pearson Coefficient
CEDAR Workshop, Boulder CO June 20-25, 2010
Low Lat Nmf2, Pearson Coefficient
CEDAR Workshop, Boulder CO June 20-25, 2010
Hmf2 High Lat, Pearson Coefficient
CEDAR Workshop, Boulder CO June 20-25, 2010
Hmf2 Mid latitude, Pearson Coefficient
CEDAR Workshop, Boulder CO June 20-25, 2010
Hmf2 low lat, Pearson Coefficient