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HARP (Hyper-Angular Rainbow Polarimeter)

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HARP is a NASA/ESTO (Earth Science Technology Office) funded CubeSat mission under the InVEST (In-Space Validation of Earth Science Technologies) Program. The HARP CubeSat mission is a joint effort between the UMBC (University of Maryland Baltimore County), Catonsville, MD, USU/SDL (Utah State University/Space Dynamics Laboratory ), North Logan, UT, STC (Science and Technology Corporation) with HQ in Hampton, VA, and NASA/GSFC (Goddard Space Flight Center) in Greenbelt, MD. The goal is to deploy the HARP CubeSat from the ISS. The desired mission life consists of three months for technology demonstration and an extended science data period of another seven months, which will total almost a year on orbit.

The HARP mission is designed to measure the microphysical properties of cloud water and ice particles in the atmosphere. HARP is a precursor for the new generation of imaging polarimeters to be used for the detailed measurements of aerosol and cloud properties. The HARP payload is a wide FOV (Field of View) imager that splits three spatially identical images into three independent polarizers and detector arrays. This technique achieves simultaneous imagery of three polarization states and is the key innovation to achieve high polarimetric accuracy with no moving parts.

The objectives of the HARP demonstration mission are: 1) 2)

• Validate the in-flight capabilities of a highly accurate and precise wide field of view hyper-angular polarimeter for characterizing aerosol and cloud properties.

• Prove that CubeSat technology can provide science-quality multi angle imaging data paving the way for lower cost aerosol-cloud instrument developments.

• Provide opportunities for student research and engineering training in implementing a space mission.

The HARP science goal is to demonstrate the ability to characterize the micro physical properties of aerosols and clouds at the scale of individual moderate-sized clouds for the ultimate purpose of narrowing uncertainties in climate change.

The PI (Principal Investigator) of the HARP mission is J. Vanderlei Martins of UMBC. The Co-Is/Partners are: Lorraine Remer, JCET-UMBC; Tim Nielsen, USU/SDL; Leroy Sparr, NASA/GSFC; Mark Schoeberl, STC. 3)

HARP is a potential precursor for the polarimeter in ACE (Aerosol-Clouds and Echosystems) and other future NASA missions.

 

Spacecraft:

The HARP CubeSat mission will be a joint effort between UMBC, the PI institution, who will provide the instrument and characterization and scientific analysis; the Space Dynamics Laboratory – Utah State University, who will provide the 3U CubeSat spacecraft and mission operations; and the Science and Technology Corporation, who will lead the science algorithm development and science application funded by NOAA. NASA Wallops will support instrument environmental testing, mission operations, and communications.

The 3U CubeSat is 3-axis stabilized designed to keep the imager pointing nadir during the data acquisition period. The hyper-angular capability is achieved by acquiring overlapping images at very fast speeds.

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Figure 1: Illustration of the HARP nanosatellite (image credit: HARP Team)

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Figure 2: HARP –full feature Earth sciences satellite (image credit: USU/SDL) 4)

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Figure 3: HARP Systems Engineer Ryan Martineau (left) and Thermal Vacuum Specialist Brittany Woytko configure HARP's spacecraft in a thermal vacuum chamber at the Space Dynamics Laboratory in Logan, Utah. Woytko is connecting several temperature sensors to the spacecraft to monitor the instrument during testing. Once the door is shut on the chamber, it loses its air and simulates the vacuum of space. The chamber also heats and cools the spacecraft through several cycles to simulate the extreme hot and cold temperatures the spacecraft will pass through on orbit (image credit: USU/SDL) 5)

 

Launch: The HARP nanosatellite was launched as part of the ELaNa-25 mission on the ISS resupply mission of Northrop Grumman (Cygnus NG-12) on 2 November 2019 (13:59.47 UTC). The launch vehicle was the Antares 230 configuration and the launch site was MARS (Mid-Atlantic Regional Spaceport) on Wallops Island, VA. USA. 6)

Orbit: Near-circular orbit, altitude of ~ 400 km, inclination of 51.6º, period of ~92 minutes.

The ISS orbit has the advantage of allowing HARP to cross many other Earth Science Satellites (including Terra, Aqua, Aura, VIIRS on Suomi NPP, CALIPSO, etc.) and produce intercomparisons and a synergistic use of the HARP data together with data from these other platforms.

Secondary CubeSat payloads of the Northrop Grumman-12 Cygnus flight

• Argus-02, a 2U CubeSat (2.5 kg) of St. Louis University, Missouri. Argus' mission is to improve the ability to model the effects of space radiation on modern electronics.

• HARP (Hyper Angular Rainbow Polarimeter), a 3U CubeSat of the University of Maryland, Baltimore County, Maryland and USU (Utah State University) - to measure the microphysical properties of cloud water and ice particles.

• Phoenix, a 3U CubeSat of ASU (Arizona State University), Tempe, AZ.

• RadSat-U (Radiation Satellite), a 3U CubeSat demonstration mission of Montana State University, Bozeman, MT.

• SOCRATES (Signal of Opportunity Cubesat Ranging and Timing Experiments), a 3U CubeSat of the University of Minnesota, Minneapolis.

External Cygnus Deployments:

• HuskySat, a 3U CubeSat technology demonstration mission (plasma propulsion) of the University of Washington, Seattle, WA.

• SwampSat II, a 3U CubeSat technology demonstration mission of the University of Florida, Gainesville, FL.

 


 

Sensor complement: (Imaging Polarimeter)

HARP will be the first US imaging polarimeter in Space. Polarization measurements are used because the technique provides new information on aerosol and cloud properties and their interaction. HARP design is an advance over POLDER's (POLarization and Directionality of the Earth's Reflectances) filter wheel system. The HARP polarimeter will provide full cloudbow retrievals from a small area (< 4 km x 4 km from space).

Cloud and aerosol processes influence climate change, which affect our oceans, weather, ecosystems, and society. The largest impediments to estimating climate change revolve around a lack of quantitative information about aerosol forcing, insufficient understanding of aerosol-cloud processes, and cloud feedbacks in the climate system. The climate community requires new observations and a better understanding of aerosol and cloud processes to narrow climate change estimate uncertainties. The aerosol community requires a multi-wavelength, multi-angle imaging polarimeter with the wide FOV imaging heritage of the POLDER mission and the high accuracy promised by the APS (Aerosol Polarimetry Sensor). Unfortunately, APS was lost when the Glory mission failed to reach orbit.

An imaging polarimeter with hyperangular capability can make a strong contribution to characterizing cloud properties, especially ice clouds. Because of their sensitivity to thin cirrus clouds, non-polarized multi-angle measurements can be used to provide climatology. Adding polarization and increasing the number of observation angles provides a much clearer picture of cloud droplet distribution, adding size and width measurements to the currently measured effective radius. The combination of hyperangular polarized measurements and short-wave infrared channels (2.1 µm) should also provide enough constraints to determine important characteristics of cloud ice crystals. In the coming decades, it will be important to have an imaging polarimeter with the capability to characterize both aerosols and clouds. Highly-capable, small, and versatile, HARP is designed to meet the needs of both the aerosol and cloud communities.

The HARP payload, a hyperangular imaging polarimeter that can see Earth from multiple viewing angles, 4 wavelengths, and three polarization angles was developed and is being built at LACO (Laboratory for Aerosol, Clouds and Optics) in the Physics Department at UMBC with support from JCET (Joint Center of Earth Systems and Technology) and NASA/GSFC (Goddard Space Flight Center). The HARP science algorithms will be developed in collaboration between UMBC and STC (Science and Technology Corporation). The main characteristics of the HARP payload are described in Table 1. 7) 8)

• One hyper-angular channel with up to 60 viewing angles per pixel at 670 nm (for cloudbow measurements)

• Three channels with up to 20 viewing angles per pixel at 440, 550, 670 nm

• Goal of one additional channel with up to 20 viewing angles at 870 nm

• 2.5 km nadir resolution (from 650 km orbit)

• 94 degree FOV in cross-track

• 110 degree FOV in along track

Table 1: Polarimeter specifications

HARP is designed to see how aerosols interact with the water droplets and ice particles that make up clouds. Aerosols and clouds are deeply connected in Earth's atmosphere – it's aerosol particles that seed cloud droplets and allow them to grow into clouds that eventually drop their precipitation (Figure 4). 9)

This interdependence implies that modifying the amount and type of particles in the atmosphere, via air pollution, will affect the type, size and lifetime of clouds, as well as when precipitation begins. These processes will affect Earth's global water cycle, energy balance and climate.

When sunlight interacts with aerosol particles or cloud droplets in the atmosphere, it scatters in different directions depending on the size, shape and composition of what it encountered. HARP will measure the scattered light that can be seen from space. We'll be able to make inferences about amounts of aerosols and sizes of droplets in the atmosphere, and compare clean clouds to polluted clouds.

In principle, the HARP instrument would have the ability to collect data daily, covering the whole globe; despite its mini size it would be gathering huge amounts of data for Earth observation. This type of capability is unprecedented in a tiny satellite and points to the future of cheaper, faster-to-deploy pathfinder precursors to bigger and more complex missions.

HARP is one of several programs currently underway that harness the advantages of CubeSats for science data collection. NASA, universities and other institutions are exploring new earth sciences technology, Earth's radiative cycle, Earth's microwave emission, ice clouds and many other science and engineering challenges.

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Figure 4: Pollution particles lead to precipitation changes (image credit: Martins, UMBC, CC BY-ND)

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Figure 5: Artist's illustration of HARP specialized to perform the delicate multi-angle, multi-spectral polarization measurements (image credit: HARP Team)

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Figure 6: Photos of the spacecraft and the actual instrument (image credit: HARP Team)

The HARP polarimeter is fully programmable and will allow for the selection of different spatial resolutions and combinations of wavelengths and viewing angles depending on the science interest and total amount of data to downlink. The different along track viewing angles from HARP will allows the observations of targets on the ground from different viewing perspectives. These different viewing observations of the same target allow for additional information from the target facilitating the quantitative retrieval of information from the atmosphere and surface properties such as the aerosol particle amount, the cloud droplet sizes, and specific characteristics of Earth's surface.

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Figure 7: Photo of the stripe filter unit (image credit: HARP Team)

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Figure 8: HARP calibration (image credit: HARP Team)

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Figure 9: A series of pictures of the coast of California taken during the PODEX (Polarimeter Definition Experiment) campaign by the PACS multi-angle imaging polarimeter taken from the NASA ER-2 aircraft (image credit: NASA)

Legend to Figure 9: The PACS (Passive Aerosol & Clouds Suite) polarimeter serves as an airborne simulator for the HARP imaging polarimeter. The different perspectives in the images emphasize the variation of the reflection of the sun on the ocean surface as a function of the viewing angle. In some along track viewing angles this reflection disappears while in other angles this reflections appear very intensively.

 


 

UMBC SOC (University of Maryland Baltimore County - Science Operations Center)

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Figure 10: UMBC SOC - HARP level 1B data production (image credit: HARP Team)

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Figure 11: UMBC SOC - Level 2 algorithm (image credit: HARP Team)

 


1) J. Vanderlei Martins, "HARP: Hyper-Angular Rainbow Polarimeter CubeSat," ESTO Science and Technology Forum, June 14, 2016, URL: https://esto.nasa.gov/forum/estf2016/PRESENTATIONS/Martins_A1P2_ESTF2016.pdf

2) "HARP Hyper-Angular Rainbow Polarimeter," USU/SDL, URL: http://www.sdl.usu.edu/downloads/harp.pdf

3) "Hyper-Angular Rainbow Polarimeter (HARP) CubeSat," Feb. 2015, URL: http://userpages.umbc.edu/~martins/laco/HARP%20QuadChart%20Feb%202015.pdf

4) J. Vanderlei Martins, Tim Nielsen, Chad Fish, Leroy Sparr, Roberto Fernandez-Borda, Mark Schoeberl, Lorraine Remer, "HARP CubeSat–An innovative Hyperangular Imaging Polarimeter for Earth Science Applications," Small Sat Pre-Conference Workshop, Logan Utah, 3 Aug 2014, URL: http://digitalcommons.usu.edu/cgi/viewcontent.cgi?filen
ame=0&article=3154&context=smallsat&type=additional

5) "Tiny NASA Satellite Will Soon See ‘Rainbows' In Clouds," NASA Feature, 28 October 2019, URL: https://www.nasa.gov/feature/goddard/2019/tiny-nasa-satellite-will-soon-see-rainbows-in-clouds

6) "NASA Science, Cargo Heads to Space Station on Northrop Grumman Mission," NASA Press Release 19-087, 2 November 2019, URL: https://www.nasa.gov/press-release/nasa-science-cargo
-heads-to-space-station-on-northrop-grumman-mission

7) "HARP Overview," UMBC/LACO, URL: http://userpages.umbc.edu/~martins/laco/harp.htm

8) Brent McBride, "Polarimetric remote sensing with the Hyper-Angular Rainbow Polarimeter, 3U CubeSat," Sept. 17, 2015, URL: http://cicsmd.umd.edu/assets/1/7/30_Brent_McBride.pdf

9) Vanderlei Martins, "Tiny satellites poised to make big contributions to essential science," UMBC, January 27, 2017, URL: https://phys.org/news/2017-01-tiny-satellites-poised-big-contributions.html
 


The information compiled and edited in this article was provided by Herbert J. Kramer from his documentation of: "Observation of the Earth and Its Environment: Survey of Missions and Sensors" (Springer Verlag) as well as many other sources after the publication of the 4th edition in 2002. - Comments and corrections to this article are always welcome for further updates (herb.kramer@gmx.net).

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