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Analysis of D Band Cloud Flag Jane Hurley Anu Dudhia Graham Ewen University of Oxford

Analysis of D Band Cloud Flag Jane Hurley Anu Dudhia Graham Ewen University of Oxford

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Page 1: Analysis of D Band Cloud Flag Jane Hurley Anu Dudhia Graham Ewen University of Oxford

Analysis of D Band Cloud Flag

Jane Hurley

Anu Dudhia

Graham Ewen

University of Oxford

Page 2: Analysis of D Band Cloud Flag Jane Hurley Anu Dudhia Graham Ewen University of Oxford

Background• Presence of clouds in the field of view (FOV) of remote

sensing instruments influence observations

• Retrievals can normally deal with small amounts of cloud in the FOV by fitting a continuum term in parallel with that of the retrieved species

Important to recognize and reliably be able to identify presence of clouds

• A couple of common and simple techniques for cloud detection …

Simple Radiance Thresholding (basic)Color Index Thresholding (improvement, as

reduces influence of variations in p and T)

Page 3: Analysis of D Band Cloud Flag Jane Hurley Anu Dudhia Graham Ewen University of Oxford

Colour Indices (CI) in a Nutshell• CIs work on the principle of ratios of mean radiances

between two spectral microwindows which respond differently to cloud.

• CI = Lav MW1 / Lav MW2

Large CI (ie. CI > 4) → cloud freeSmall CI (ie. CI ~ 1) → thick cloud Range of CIs represents range of optical

thicknesses of clouds present in FOV

• Presence of cloud determined by setting a threshold on the CI such that

for all CI > CIthresh → cloud free FOV

for all CI < CIthresh → cloudy FOV

Page 4: Analysis of D Band Cloud Flag Jane Hurley Anu Dudhia Graham Ewen University of Oxford

• Cautions: Definition of CI breaks down above ~ 30 km with

decreased SNRAbove threshold (“cloud free”), cloud can still occur

if the cloud is optically thin or partially filling the FOV …

• MIPAS has CIs defined for 3/5 bands:

Colour Index MW1 (cm-1) MW2 (cm-1) Threshold

CI-A

CI-B

CI-D

788.0 - 796.0

1246.3 -1249.1

1929.0 -1935.0

832.0 - 834.0

1232.3 -1234.4

1973.0 -1983.0

1.8

1.2

1.8

Page 5: Analysis of D Band Cloud Flag Jane Hurley Anu Dudhia Graham Ewen University of Oxford

Issues for Discussion

• Anomalous situations where the D band flags cloud but the A band does not – is it possible that the D band is better suited to detect certain cloud types?

• A correlation between these anomalous events (where the D band flags cloud while the A band doesn’t) and extremely low H2O volume mixing ratio (vmr)

• Day/night difference in behaviour of the D band

Page 6: Analysis of D Band Cloud Flag Jane Hurley Anu Dudhia Graham Ewen University of Oxford

Correlation of Low H2O VMR and D/A Cloud Flagging Anomaly

• Previous work (Remedios) implied a correlation between anomaly and low H2O vmr values (10-10ppmv).

Page 7: Analysis of D Band Cloud Flag Jane Hurley Anu Dudhia Graham Ewen University of Oxford

• These low H2O vmrs are markers for when retrieved H2O vmr is negative → a bad H2O vmr retrieval

• Using arbitrary day (15 August 2003), in keeping with previous work, found that in the range of definition of CI:

if D band flags and A band doesn’t, ~ 8% of the occurrences have low H2O vmr (are bad retrievals)

if have low H2O vmr, ~ 20% of the occurrences have the D band flagged but the A band unflagged.

A WEAK CORRELATION AT BEST. Not trustworthy enough to risk throwing away quite a bit of useful data …

If were to use D band as a filter for poor H2O retrieval, could potentially lose 92% of such points which could be good data

# flagging anomaly / # total points = 353 / 12041 ~ 3%# low H2O vmr / # total points = 173 / 12041 ~ 1.5%

Page 8: Analysis of D Band Cloud Flag Jane Hurley Anu Dudhia Graham Ewen University of Oxford

Day/Night Difference in D Band

• Remedios found that anomaly of D band flagging and A band not flagging occurred for winter daytime points (60-75 S day, 60 – 75 S night, 75 – 90 S day);

• Could not replicate this result – but definitely found concentration of such anomalous winter daytime points in winter south pole;

• Difference in day/night D band spectra discussed later …

Page 9: Analysis of D Band Cloud Flag Jane Hurley Anu Dudhia Graham Ewen University of Oxford

D Band Sensitive Cloud Detector?

• Mostly winter daytime points (but quite a few mid-lat nighttime points as well …)

• Polar points attributable to PSCs (A band close enough to threshold)

Page 10: Analysis of D Band Cloud Flag Jane Hurley Anu Dudhia Graham Ewen University of Oxford

Standard Spectra

• A Band Clear: level zero-magnitude baseline; day/night spectra have same relative shape.

• A Band Cloudy: slanted baseline heightened in magnitude above zero; day/night spectra have same relative shape.

• D Band Clear: level zero-magnitude baseline; day/night spectra have same relative shape.

• D Band Cloudy: slanted baseline heightened in magnitude above zero; daytime spectra exhibit large non-LTE feature at ~ 2350 cm-1.

Page 11: Analysis of D Band Cloud Flag Jane Hurley Anu Dudhia Graham Ewen University of Oxford

Anomaly Spectrum• Low altitude, mid-latitude daytime example of where D

band flags but A band doesn’t. CI-D = 0.94, CI-A = 1.88

• Both spectra exhibit cloudy features – there is cloud, but no surprise since A band quite close to threshold.

Page 12: Analysis of D Band Cloud Flag Jane Hurley Anu Dudhia Graham Ewen University of Oxford

• Pick situations where flagging anomaly occurs but can’t be attributed to cloud – ie. mid-lats, 20 – 30km altitude.

• For a period of 15 July – 15 August 2003, such anomalous points (D flagged/ A unflagged) looked clear in the A band and had strange negative feature in D band at ~ 2350 cm-1. ANOMALY NOT CAUSED BY CLOUD PRESENCE!

Page 13: Analysis of D Band Cloud Flag Jane Hurley Anu Dudhia Graham Ewen University of Oxford

• Thick cloud spectra should limit to Planck blackbody function at brightness temperature

Planck function at appropriate TB should flag as cloud

• Using ECMWF temperature profiles:

• A band reliably flags thick cloud but D band stops flagging cloud at higher altitudes/ lower brightness temperatures

15 km 18 km 22 km 25 km 28 km

CI-D 1.29 1.32 1.28 1.26 1.25

CI-A 1.15 1.17 1.14 1.13 1.12

Page 14: Analysis of D Band Cloud Flag Jane Hurley Anu Dudhia Graham Ewen University of Oxford

• D band moves away from flagging Planck function at colder temperatures.• Suggested threshold of 1.2 would fail for most atmospheric temperatures.

Page 15: Analysis of D Band Cloud Flag Jane Hurley Anu Dudhia Graham Ewen University of Oxford

RFM Atmospheric Models• Reference Forward

Model (RFM) used to simulate clear and thick cloudy atmospheric conditions

• A more realistic model than a blackbody, taking atmospheric absorptions/emissions etc into account

• Using a ‘step function’ cloud …

Page 16: Analysis of D Band Cloud Flag Jane Hurley Anu Dudhia Graham Ewen University of Oxford

• Sample spectra at a tangent height of ~ 15 km for a cloudy atmosphere

Page 17: Analysis of D Band Cloud Flag Jane Hurley Anu Dudhia Graham Ewen University of Oxford

• RFM shows range over which can confidently use CI-A and CI-D

• Clearly D band flag acts unreliably at most altitudes

Page 18: Analysis of D Band Cloud Flag Jane Hurley Anu Dudhia Graham Ewen University of Oxford

General Behaviour of CI-D & CI-A

• A band behaves as expected, detecting cloud at low altitudes (5-20km) and not at higher altitudes (20-30km);

• D band less convincing, detecting cloud even where there should be none from a statistical standpoint;

A band seems a more reliable cloud flag than the D band!!

Page 19: Analysis of D Band Cloud Flag Jane Hurley Anu Dudhia Graham Ewen University of Oxford

Conclusions• Not a high enough correlation between low H2O vmrs

(poor retrievals) and flagging anomaly to warrant using anomaly as a detection mechanism for poor data;

• Day/night difference between D band spectra due to a large non-LTE feature appearing in the daytime at ~ 2350 cm-1;

• D band more sensitive to clouds? Maybe, but probably not – and certainly not reliably so!D band flags cloud where there simply isn’t anyD band doesn’t consistently flag a blackbodyStrange features in anomalous spectra (non-LTE and

negative)

Recommendations: Stick with tried-and-true A band. D band simply not reliable.