CEDAR Workshop, Boulder CO June 20-25, 2010 Statistical Analysis of COSMIC Derived Abel Profiles Jet...

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CEDAR Workshop, Boulder CO June 20-25, 2010 Statistical Analysis of COSMIC Derived Abel Profiles Jet Propulsion Laboratory California Institute of Technology M/S 238-600 4800 Oak Grove Drive Pasadena CA 91109 Philip Stephens, Attila Komjathy, Brian Wilson, Xiaoqing Pi and Anthony J. Mannucci

Transcript of CEDAR Workshop, Boulder CO June 20-25, 2010 Statistical Analysis of COSMIC Derived Abel Profiles Jet...

Page 1: CEDAR Workshop, Boulder CO June 20-25, 2010 Statistical Analysis of COSMIC Derived Abel Profiles Jet Propulsion Laboratory California Institute of Technology.

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

Page 2: CEDAR Workshop, Boulder CO June 20-25, 2010 Statistical Analysis of COSMIC Derived Abel Profiles Jet Propulsion Laboratory California Institute of Technology.

CEDAR Workshop, Boulder CO June 20-25, 2010

Outline

• Introduction• Motivation for this study

• Analysis Framework• Results• Summary

Page 3: CEDAR Workshop, Boulder CO June 20-25, 2010 Statistical Analysis of COSMIC Derived Abel Profiles Jet Propulsion Laboratory California Institute of Technology.

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

Page 4: CEDAR Workshop, Boulder CO June 20-25, 2010 Statistical Analysis of COSMIC Derived Abel Profiles Jet Propulsion Laboratory California Institute of Technology.

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?

Page 5: CEDAR Workshop, Boulder CO June 20-25, 2010 Statistical Analysis of COSMIC Derived Abel Profiles Jet Propulsion Laboratory California Institute of Technology.

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

Page 6: CEDAR Workshop, Boulder CO June 20-25, 2010 Statistical Analysis of COSMIC Derived Abel Profiles Jet Propulsion Laboratory California Institute of Technology.

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)

Page 7: CEDAR Workshop, Boulder CO June 20-25, 2010 Statistical Analysis of COSMIC Derived Abel Profiles Jet Propulsion Laboratory California Institute of Technology.

CEDAR Workshop, Boulder CO June 20-25, 2010

Nmf2 and Hmf2 Correlation Plots

Page 8: CEDAR Workshop, Boulder CO June 20-25, 2010 Statistical Analysis of COSMIC Derived Abel Profiles Jet Propulsion Laboratory California Institute of Technology.

CEDAR Workshop, Boulder CO June 20-25, 2010

VTEC at High Latitude, Pearson Coefficient

Page 9: CEDAR Workshop, Boulder CO June 20-25, 2010 Statistical Analysis of COSMIC Derived Abel Profiles Jet Propulsion Laboratory California Institute of Technology.

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

Page 10: CEDAR Workshop, Boulder CO June 20-25, 2010 Statistical Analysis of COSMIC Derived Abel Profiles Jet Propulsion Laboratory California Institute of Technology.

CEDAR Workshop, Boulder CO June 20-25, 2010

High Lat Correlations, Nmf2, Hmf2

Page 11: CEDAR Workshop, Boulder CO June 20-25, 2010 Statistical Analysis of COSMIC Derived Abel Profiles Jet Propulsion Laboratory California Institute of Technology.

CEDAR Workshop, Boulder CO June 20-25, 2010

Case 1: Long arc, High Lat, Dusk

Page 12: CEDAR Workshop, Boulder CO June 20-25, 2010 Statistical Analysis of COSMIC Derived Abel Profiles Jet Propulsion Laboratory California Institute of Technology.

CEDAR Workshop, Boulder CO June 20-25, 2010

Case 2: Long arc, High Latitude, Midday

Page 13: CEDAR Workshop, Boulder CO June 20-25, 2010 Statistical Analysis of COSMIC Derived Abel Profiles Jet Propulsion Laboratory California Institute of Technology.

CEDAR Workshop, Boulder CO June 20-25, 2010

Case 3: High lat, medium arc, midnight

Page 14: CEDAR Workshop, Boulder CO June 20-25, 2010 Statistical Analysis of COSMIC Derived Abel Profiles Jet Propulsion Laboratory California Institute of Technology.

CEDAR Workshop, Boulder CO June 20-25, 2010

Mid Latitude VTEC, Pearson Coefficient

Page 15: CEDAR Workshop, Boulder CO June 20-25, 2010 Statistical Analysis of COSMIC Derived Abel Profiles Jet Propulsion Laboratory California Institute of Technology.

CEDAR Workshop, Boulder CO June 20-25, 2010

Mid Latitude Correlation Plots

Mid latitude, midnight long arcs, only 5 points though

44

4

4

Page 16: CEDAR Workshop, Boulder CO June 20-25, 2010 Statistical Analysis of COSMIC Derived Abel Profiles Jet Propulsion Laboratory California Institute of Technology.

CEDAR Workshop, Boulder CO June 20-25, 2010

Case 4: Mid Lat, Long Arc, Midnight

Page 17: CEDAR Workshop, Boulder CO June 20-25, 2010 Statistical Analysis of COSMIC Derived Abel Profiles Jet Propulsion Laboratory California Institute of Technology.

CEDAR Workshop, Boulder CO June 20-25, 2010

Low Latitude VTEC, Pearson Coefficient

Page 18: CEDAR Workshop, Boulder CO June 20-25, 2010 Statistical Analysis of COSMIC Derived Abel Profiles Jet Propulsion Laboratory California Institute of Technology.

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

Page 19: CEDAR Workshop, Boulder CO June 20-25, 2010 Statistical Analysis of COSMIC Derived Abel Profiles Jet Propulsion Laboratory California Institute of Technology.

CEDAR Workshop, Boulder CO June 20-25, 2010

Low Lat Correlation Plots, Hmf2, Nmf2

Page 20: CEDAR Workshop, Boulder CO June 20-25, 2010 Statistical Analysis of COSMIC Derived Abel Profiles Jet Propulsion Laboratory California Institute of Technology.

CEDAR Workshop, Boulder CO June 20-25, 2010

Case 5: Long arc, Low lat, Dawn

Page 21: CEDAR Workshop, Boulder CO June 20-25, 2010 Statistical Analysis of COSMIC Derived Abel Profiles Jet Propulsion Laboratory California Institute of Technology.

CEDAR Workshop, Boulder CO June 20-25, 2010

Case 6: Long arc, Low lat, Midday

Page 22: CEDAR Workshop, Boulder CO June 20-25, 2010 Statistical Analysis of COSMIC Derived Abel Profiles Jet Propulsion Laboratory California Institute of Technology.

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

Page 23: CEDAR Workshop, Boulder CO June 20-25, 2010 Statistical Analysis of COSMIC Derived Abel Profiles Jet Propulsion Laboratory California Institute of Technology.

CEDAR Workshop, Boulder CO June 20-25, 2010

Backup slides

Page 24: CEDAR Workshop, Boulder CO June 20-25, 2010 Statistical Analysis of COSMIC Derived Abel Profiles Jet Propulsion Laboratory California Institute of Technology.

CEDAR Workshop, Boulder CO June 20-25, 2010

High Lat NmF2, Pearson Coefficient

Page 25: CEDAR Workshop, Boulder CO June 20-25, 2010 Statistical Analysis of COSMIC Derived Abel Profiles Jet Propulsion Laboratory California Institute of Technology.

CEDAR Workshop, Boulder CO June 20-25, 2010

Mid Lat, Nmf2, Pearson Coefficient

Page 26: CEDAR Workshop, Boulder CO June 20-25, 2010 Statistical Analysis of COSMIC Derived Abel Profiles Jet Propulsion Laboratory California Institute of Technology.

CEDAR Workshop, Boulder CO June 20-25, 2010

Low Lat Nmf2, Pearson Coefficient

Page 27: CEDAR Workshop, Boulder CO June 20-25, 2010 Statistical Analysis of COSMIC Derived Abel Profiles Jet Propulsion Laboratory California Institute of Technology.

CEDAR Workshop, Boulder CO June 20-25, 2010

Hmf2 High Lat, Pearson Coefficient

Page 28: CEDAR Workshop, Boulder CO June 20-25, 2010 Statistical Analysis of COSMIC Derived Abel Profiles Jet Propulsion Laboratory California Institute of Technology.

CEDAR Workshop, Boulder CO June 20-25, 2010

Hmf2 Mid latitude, Pearson Coefficient

Page 29: CEDAR Workshop, Boulder CO June 20-25, 2010 Statistical Analysis of COSMIC Derived Abel Profiles Jet Propulsion Laboratory California Institute of Technology.

CEDAR Workshop, Boulder CO June 20-25, 2010

Hmf2 low lat, Pearson Coefficient