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NASA HQ Update Ken Jucks, Aura Program Scientist Earth Science Division, Science Mission Directorate 11 March 2014

NASA HQ Update Ken Jucks, Aura Program Scientist Earth Science Division, Science Mission Directorate 11 March 2014

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Page 1: NASA HQ Update Ken Jucks, Aura Program Scientist Earth Science Division, Science Mission Directorate 11 March 2014

NASA HQ Update

Ken Jucks, Aura Program ScientistEarth Science Division, Science Mission Directorate 11 March 2014

Page 2: NASA HQ Update Ken Jucks, Aura Program Scientist Earth Science Division, Science Mission Directorate 11 March 2014

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NASA Operating MissionsOn-Orbit Flight Missions – Partnerships

Bi-annual Senior ReviewCompleted Summer 2013

Page 3: NASA HQ Update Ken Jucks, Aura Program Scientist Earth Science Division, Science Mission Directorate 11 March 2014

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Operating Instrument StatusINSTRUMENT INSTRUMENT MISSION STATUS       Spectral Irradiance Monitor SIM SORCE Operating in daylight onlySolar-Stellar Irradiance Comparison Experiment SOLSTICE SORCE Operating in daylight onlyTotal Irradiance Monitor TIM SORCE Operating in daylight onlyXUV Photometer System XPS SORCE Operating in daylight onlyClouds and the Earth's Radiation Energy System CERES Terra Operating nominallyModerate Resolution Imaging Spectroradiometer MODIS Terra Operating nominallyMulti-Angle Imaging Spectrometer MISR Terra Operating nominallyMeasuerment of Pollution in the Troposphere MOPITT Terra Operating nominallyAdvanced Spaceborne Thermal Emission & Reflection Radiometer ASTER Terra SWIR failed (VNIR & TIR operational)

High Resolution Dynamics Limb Sounder HIRDLS Aura FailedOzone Monitoring Instrument OMI Aura Row anomaly Microwave Limb Sounder MLS Aura Operating nominally with Band 13

powered off & THz channel in standby; on redundant mirror switching mechanism electronics

Troposphere Emission Spectrometer TES Aura Interferometer Control System currently working

Cloud-Aerosol Lidar with orthogonal Polarization CALIOP CALIPSO Operating nominally second laser unit

Imaging Infrared Radiometer IIR CALIPSO Operating nominallyWide Field Camera WFC CALIPSO Operating nominallyActive Cavity Radiometer Irradiance Monitor-III ACRIM-III ACRIMSAT Battery problemsAtmospheric Infrared Sounder AIRS Aqua Operating nominallyAdvanced Microwave Scanning Radiometer for EOS AMSR-E Aqua Operating at 2rpm for cross-calibration

with GCOM-W1 AMSR2Advanced Microwave Sounding Unit-A AMSU-A Aqua 10 of 15 channels performing wellHumidity Sounder-Brazil HSB Aqua FailedClouds and the Earth's Radiation Energy System CERES Aqua Operating nominallyModerate Resolution Imaging Spectroradiometer MODIS Aqua Operating nominallyCloud Profiling Radar CPR Cloudsat Daylight Only operationsVisible Infrared Imaging Radiometer Suite VIIRS Suomi-NPP Operating nominallyCross-track Infrared Sounder CrIS Suomi-NPP Operating nominallyClouds and the Earth's Radiation Energy System CERES Suomi-NPP Operating nominallyAdvanced Technology Microwave Sounder ATMS Suomi-NPP Operating nominallyOzone Mapping and Profiler Suite OMPS Suomi-NPP Operating nominally

Page 4: NASA HQ Update Ken Jucks, Aura Program Scientist Earth Science Division, Science Mission Directorate 11 March 2014

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Near-Term Formulation & Development Missions

SMAP5 Nov 2014

w/CSASoil Moist., Frz/Thaw

Delta II

ICESat-2Dec 2016 (TBR)

Ice DynamicsDelta II

OCO-21 July 2014Global CO2

Delta II

GRACE FOAug 2017

w/Germany; Global Mass & Water Variation

German-supplied Dnepr LV

GPMEarly CY2014

w/ JAXA; PrecipH-IIA

CYGNSS2016-2017

Tropical CycloneGeneration, Air-sea

Interaction in ExtremeConditions

SAGE IIINET Mar 2015 (TBR)Ozone & Trace Gases

Falcon-9

CATSAug 2014

w/ ISSAerosol & Cloud

Falcon-9

Page 5: NASA HQ Update Ken Jucks, Aura Program Scientist Earth Science Division, Science Mission Directorate 11 March 2014

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Venture Class Activities

• EVS (“EV-1” - Suborbital, Airborne; solicited every 4 years)– All 5 investigations are well into their sustained field campaigns– All EV-1 investigations flew during 2013– Second EV-S solicitation released June 2013, proposals due 10 Jan 2014

• EVM (“EV-2” - Small-sat; solicited every 4 years)– CYGNSS successful KDP-B in July 2013, planned LRD October 2016 – April 2017– FY14 budget proposal includes EV-M/2 solicitation on-schedule in June 2015

• EVI (Instrument; solicited every 18 months)– TEMPO selected for GEO hosted payload opportunity (early FY18 launch)– ESD making progress on formal host selection– Second “EV-I/2” solicitation released July 2013, proposals received 25

November 2013– FY14 budget proposal includes EVI-3 and subsequent solicitations on-

schedule

Page 6: NASA HQ Update Ken Jucks, Aura Program Scientist Earth Science Division, Science Mission Directorate 11 March 2014

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NASA ESD Flight Portfolio 2013 - 2022 GPM (2/2014) – Global Precipitation mapping, w/JAXA OCO-2 (7/2014) – Atmospheric CO2 monitoring, recovery mission CATS (8/2014) – Aerosol and Cloud vertical profile SMAP (10/2014) – Soil Moisture and Freeze/Thaw cycling, w/CSA (minor) SAGE-III/ISS (3/2015) – Ozone, Temp, Humidity profiles, w/HEOMD, ESA ICESat-2 (12/2016) – Precision Ice Topography, Ecosystem monitoring CYGNSS [EVM-1] (late 2016) GRACE-FO (8/2017) – Gravity/Ice Mass/Ground Water, w/GFZ & DLR OCO-3/ISS (Fall 2017) – CO2 continuity, from ISS, OCO-2 spares TEMPO [EVI-1] (2019) – Tropospheric Emissions from geosynchronous vantage SWOT (2020) – Wide-swath ocean altimetry, land water, w/CNES EVI-2 Venture-Class (NLT 2020) PACE (2020) – Ocean Color, possibly Aerosols L-band SAR (2021?) – Solid Earth, Cryosphere, Ecosystems, w/ISRO CLARREO (2022?) – Precise global radiation balance, possibly w/UK EVM-2 (NLT 2022) EVI-3 (NLT 2022)

Significant studies ongoing for all other Tier-2 Decadal Survey missions And on the horizon: Sustained Land Imaging program for the U.S. for 2018 – 2038 Solar Irradiance, Ozone profiles, and Earth Radiation Budget measurements

for beyond 2020

Page 7: NASA HQ Update Ken Jucks, Aura Program Scientist Earth Science Division, Science Mission Directorate 11 March 2014

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Aura/OMI and Senior Review

The Senior Review for all NASA missions beyond Prime Operating Mission was completed last year.

Results and guidance were delivered to the projects this past November.

Aura “Science Summary” score was “Excellent”. Aura “Utility” score was “High”. This was mostly

due to the high resolution mapping ability of OMI for air quality.

Aura “Technical Risk” was “Medium-High”. TES has some significant issues, OMI has a blockage, that while stable of late, does change. MLS has parts near end of predicted lifetime.

Page 8: NASA HQ Update Ken Jucks, Aura Program Scientist Earth Science Division, Science Mission Directorate 11 March 2014

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OMI and new Aura Science Team selections

The competitively selected Aura Science Team is reselected every 3 years.

The most recent set of proposals were due September 2013, and selections were made in December 2013.

68 proposals were received, and 27 were selected.

A total of $5M/year is currently available on that budget line.

16 of the selected proposals will use OMI data. Numerous ACMAP studies also use OMI and

other Aura data sets.

Page 9: NASA HQ Update Ken Jucks, Aura Program Scientist Earth Science Division, Science Mission Directorate 11 March 2014

TEMPO EVI-1 selected

Investigation Kelly Chance, Principal

Investigator

Other organizations include LaRC, GSFC, Ball Aerospace,

and many universities

TEMPO is about to have it’s KDP-B

NASA’s plan is to procure space and communications on a commercial

GEO satellite.

Page 10: NASA HQ Update Ken Jucks, Aura Program Scientist Earth Science Division, Science Mission Directorate 11 March 2014

Why geostationary? High temporal and spatial resolution

Hourly NO2 surface concentration and integrated column calculated by CMAQ air quality model: Houston, TX, June 22-23, 2005

June 22 Hour of Day (UTC) June 23

LEO observations provide limited information on rapidly varying emissions, chemistry, & transport

GEO will provide observations at temporal and spatial scales highly relevant to air quality processes12-13 November 2013 11TEMPO SRR/MDR

Page 11: NASA HQ Update Ken Jucks, Aura Program Scientist Earth Science Division, Science Mission Directorate 11 March 2014

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TropOMI and OCO-2, OMI, OMPS

The atmospheric science community in the US, particularly those working with NASA data, are anticipating the data from TropOMI to advance the science beyond what can be done with the NASA missions alone.

The OMPS instrument on NPP will continue on the JPSS-1 satellite, that is part of NOAA’s budget, but with strong NASA contributions.

OMI should continue as long as Aura remains operating in orbit (~2023??), and the combined data should produce interesting science results.

OCO-2 launches in July 2014. It does NOT get CH4 and CO! TropOMI will!

Page 12: NASA HQ Update Ken Jucks, Aura Program Scientist Earth Science Division, Science Mission Directorate 11 March 2014

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NASA HQ Perspective

Questions?