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1 Generation and Evaluation of Systematic CRISM Mineral Indicator Maps Frank Seelos, Olivier Barnouin David Humm, Howard Taylor, Chris Hash, Frank Morgan, Kim Seelos, Debra Buczkowski, Scott Murchie, and Anne Sola 4 th MSL Landing Site Selection Workshop MSL CDP 09/27/2010
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Generation and Evaluation of Systematic CRISM Mineral Indicator Maps

Frank Seelos, Olivier BarnouinDavid Humm, Howard Taylor, Chris Hash, Frank Morgan,

Kim Seelos, Debra Buczkowski, Scott Murchie, and Anne Sola

4th MSL Landing Site Selection WorkshopMSL CDP

09/27/2010

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Outline

• CRISM data processing and product description– Updated radiometric calibration (TRR2 TRR3)– Systematic spectral processing– Revised summary parameters and browse products

• MSL candidate landing sites – CRISM web site– Active online community resource– 170 targeted observations of the MSL candidate landing sites presented

• CRISM prototype TRR3 I/F image cubes• Systematic browse products, false color composites, etc.

• Representative observations and derived analysis products– Mawrth Vallis– Holden Crater– Ebserswalde Crater– Gale Crater

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CRISM Data Processing Upgrade Overview

• A major upgrade of the CRISM data processing pipeline is nearing completion– Non-map projected hyperspectral data, calibration version 3 (TRR3s)

Radiance (‘RA’) cubes – output from radiometric calibration version 3 I/F cubes – TRR3’s processed though custom filtering procedures

o IR: kernel filter to remove stochastic noise o VNIR+IR: mitigation of systematic column-oriented noise

– Map-projected filtered hyperspectral dataUpgraded atmospheric correction Correction for observation geometric/photometric effectsCorrection for spectral smile effect

– Browse versions of the data with the above correctionsReformulated to show more phases, reduce artifacts

• 1st release for MSL candidate landing sites - via CRISM web site• Redelivery of other data will begin with next PDS delivery

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Next Steps for Post TRR3 ProcessingCa

Calibration upgrade and noise filtering

Revised summary products

PNG versions of summary product composites (browse products)

Upgraded atmospheric correction

Empirical correction of systematic calibration residual

Map projection using MRO conventions

Combine VNIR+IR remove bad channels

Empirical normalization of geometric dependencies

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Post-Calibration Empirical Corrections

The TRR3 data still exhibit two effects• Along-track brightness variations Due to continuously varying gimbal angle Processing fits variation as a function of observing geometry in

the central scan and accompanying EPF segments Data is normalized to minimum emission angle

• Cross-track brightness variations (optical artifact) Fits cross-track variations using a function constrained in form

to follow spectral smile Data is normalized to center of the FOV

VNIR RGB Corrected VNIR RGB

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Current I/F PDS deliverable

False color IR RGB composite; 0.5% linear stretch on each displayed band; spectral median plot with interquartile envelope and RGB wavelengths indicated; boxplots show data distribution of RGB bands

Note IR spectral slope and noise components

TRR2

CRISM Data Processing Progression: Heimdal

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CRISM Data Processing Progression: Heimdal

Spectral artifact at < 1.7 µm corrected

Improved flat-field

Minor change to systematic noise component; stochastic component effectively unchanged

TRR3 – Unfiltered

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CRISM Data Processing Progression: Heimdal

Systematic and stochastic noise removed - spectral shape intact

TRR3 I/F PDS deliverable

Prototype TRR3 data for MSL candidate landing sites available as an early release

Note photometric effects at the top and bottom of the scene

TRR3 – Filtered

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CRISM Data Processing Progression: Heimdal

TRR3 – Filtered & Corrected

Simple photometric (cos(i)) and atmospheric (“volcano scan”) corrections

Empirical normalization of the data to the minimum sampled emission angle observing geometry

Empirical spectral smile residual correction

Corrected data used in the calculation of spectral summary parameters and browse products

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Spectral Summary Parameters / Browse Products -Targeted Observation Hyperspectral Sampling

Previous: Use only 72 channels present in both multispectral and

hyperspectral data for spectral parameter calculationSpectral noise propagated into parameter

Current:Evaluate spectral data in channels near wavelengths

used in parameter calculationsMitigates propagation of spectral artifacts

MAF -Red: OLINDEX Green: LCPINDEXBlue: HCPINDEX

FRT00007D87 - TRR2

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False positive strong olivine detection

Bright dust

MAF (previous) -Red: OLINDEX Green: LCPINDEXBlue: HCPINDEX

IRA - Corrected brightness at 1.3 µm

OLINDEX2 – Mitigates spectral continuum effects in parameter calculation

No false positive

Spectral Summary Parameters / Browse Products -Improved Parameter Functions

MAF (current) -Red: OLINDEX2 Green: LCPINDEXBlue: HCPINDEX

FRT00007D87 - TRR2

Salvatore, M. R., J. F. Mustard, M. B. Wyatt, and S. L. Murchie (2010), Definitive evidence of Hesperian basalt in Acidalia and Chryseplanitiae, J. Geophys. Res., 115, E07005,

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New MSL candidate landing site CRISM browse products

Brief explanation of systematic data processing

Product overview

http://crism.jhuapl.edu/msl_landing_sites/

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Detailed information on the browse products, parameter stretches, products interpretation, and caveats

Click on the site name to access product the library

http://crism.jhuapl.edu/msl_landing_sites/

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Observations organized into tabs by type and time order

1 column = 1 observation

1 row = 1 product type

Data quality metrics –IR detector temperature Atmospheric opacity

http://crism.jhuapl.edu/msl_landing_sites/

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Each product type emphasizes one way to visualize the observation information content: context image showing footprint, Fe minerals, maficminerals, phyllosilicates, etc.

Click on a thumbnail to access full-resolution version

http://crism.jhuapl.edu/msl_landing_sites/

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Separate ‘global’ and regional stretches for site-to-site comparison and to highlight local heterogeneity

Links to full resolution versions of the browse products with and without geographic grid

Links to version of data already in the PDS (TRR2)

Links to early release of TRR3s

Detailed breakdown of observation and data set characteristics: lat/lon/Ls, i/e/g, lines/samples/bands, etc.

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Mawrth Vallis – FRT0000B141

FRTHRLHRS

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Mawrth Vallis – FRT0000B141

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Mawrth Vallis – FRT0000B141

VNIR RGB VNIR FM2

VNIR spectral variability – Fe mineralogy

R: BD530G: BD920B: BDI1000

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IR RGB IR PHY

Mawrth Vallis – FRT0000B141

R: D2300G: BD2210B: BD1900

Western portion of the ellipse dominated by Al-phyllosilicate signatures

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FRTHRLHRS

Holden Crater – FRT0000C1D1

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Holden Crater – FRT0000C1D1

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IR RGB IR PHY

Light toned deposits in IR RGB image correspond to enhanced D2300 and BD1900 spectral indices (magenta pixels – Fe/Mg phyllosilicate) in IR PHY browse product

Holden Crater – FRT0000C1D1

R: D2300G: BD2210B: BD1900

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FRTHRLHRS

Eberswalde Crater – FRT0000AADE

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Eberswalde Crater – FRT0000AADE

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Fe/Mg-Phyllosilicate detection - magenta pixels in IR PHY brose product –restricted to small knobs/outcrops

IR RGB IR PHY

Eberswalde Crater – FRT0000AADE

R: D2300G: BD2210B: BD1900

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FRTHRLHRS

Gale Crater – FRT0000B6F1

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Gale Crater – FRT0000B6F1

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Gale Crater – FRT0000B6F1

VNIR RGB VNIR FM2 R: BD530G: BD920B: BDI1000

Distribution of ferric/ferrous iron phases

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IR RGB IR HYD

Gale Crater – FRT0000B6F1

Hydrated sulfate signature correlated with pyroxene signature

R: SINDEXG: BD2100B: BD1900

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Summary

CRISM support for MSL landing site selection:http://crism.jhuapl.edu/msl_landing_sites/

• The systematic set of derived CRISM analysis products provides an objective framework for the evaluation and comparison of the spectral signatures at each candidate site

• CRISM prototype TRR3 I/F data available for MSL candidate landing sites via the website

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Future Attractions – Systematic Product Mosaics

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CRISM TRR3 Calibration - Additional Material

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2 of 6 intermediate versions that were rejected (too-large spectral slopes, organized artifacts, etc.)

TRR3 – new- spectral artifacts fixed- less high-frequency spectral noiseTRR2 – old version has issues:

- time-drift of calibration at 1-1.7 µm- artifacts at 1.9, 2.5, 3.2 µm- systematic spectral noise

TRR3 vs. TRR2

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Unfiltered vs. Filtered Spectral Comparison

Polynomial form of the interpolation through noisy pixels preserves high spectral-frequency information

Random noise from elevated detector operating temp. greatly reduced

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TRR2 vs. TRR3

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TRR2 vs. TRR3

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2.3-µm Phyllosilicate Band TRR2 vs. TRR3(1% stretch)

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2.3-µm Phyllosilicate Band TRR2 vs. TRR3(1% stretch)

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MSL Systematic CRISM Browse Products Gallery

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45IR RGB IR PHY IR MAF

VNIR RGB VNIR FEM VNIR FM2

Mawrth Vallis – FRT0000B141 Gallery

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46IR RGB IR PHY IR MAF

VNIR RGB VNIR FEM VNIR FM2

Holden Crater – FRT0000C1D1 Gallery

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47IR RGB IR PHY IR MAF

VNIR RGB VNIR FEM VNIR FM2

Eberswalde Crater – FRT0000AADE Gallery

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48IR RGB IR HYD IR MAF

VNIR RGB VNIR FEM VNIR FM2

Gale Crater – FRT0000B6F1 Gallery


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