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IEEE Aerospace Conference (AERO)

Development of the science data system for the international space station Cold Atom Lab

Chris van Harmelen, Melissa A. Soriano

Published Mar 1, 2015• 0 citations
Publisher

Abstract

Cold Atom Laboratory (CAL) is a facility that will enable scientists to study ultra-cold quantum gases in a microgravity environment on the International Space Station (ISS) beginning in 2016. The primary science data for each experiment consists of two images taken in quick succession. The first image is of the trapped cold atoms and the second image is of the background. The two images are subtracted to obtain optical density. These raw Level 0 atom and background images are processed into the Level 1 optical density data product, and then into the Level 2 data products: atom number, Magneto-Optical Trap (MOT) lifetime, magnetic chip-trap atom lifetime, and condensate fraction. These products can also be used as diagnostics of the instrument health. With experiments being conducted for 8 hours every day, the amount of data being generated poses many technical challenges, such as downlinking and managing the required data volume. A parallel processing design is described, implemented, and benchmarked. In addition to optimizing the data pipeline, accuracy and speed in producing the Level 1 and 2 data products is key. Algorithms for feature recognition are explored, facilitating image cropping and accurate atom number calculations.

DOI
10.1109/aero.2015.7118928

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Cold Atom Laboratory (CAL) is a facility that will enable scientists to study ultra-cold quantum gases in a microgravity environment on the International Space Station (ISS) beginning in 2016. The primary science data for each experiment consists of two images taken in quick succession. The first image is of the trapped cold atoms and the second image is of the background. The two images are subtracted to obtain optical density. These raw Level 0 atom and background images are processed into the Level 1 optical density data product, and then into the Level 2 data products: atom number, Magneto-Optical Trap (MOT) lifetime, magnetic chip-trap atom lifetime, and condensate fraction. These products can also be used as diagnostics of the instrument health. With experiments being conducted for 8 hours every day, the amount of data being generated poses many technical challenges, such as downlinking and managing the required data volume. A parallel processing design is described, implemented, and benchmarked. In addition to optimizing the data pipeline, accuracy and speed in producing the Level 1 and 2 data products is key. Algorithms for feature recognition are explored, facilitating image cropping and accurate atom number calculations.
Cold Atom Laboratory (CAL) is a multi-user facility that will provide the ability to study ultra-cold quantum gases in a microgravity environment. The laboratory is an internal payload that will operate on the International Space Station (ISS) in 2016. Principal Investigators from various universities will trade off in designing experiment sequences that vary different parameters, such as magnetic field strength or timing. The primary science data consists of two images of the cold atoms captured successively at the end of each experiment.
Abstract We report the status of the Cold Atom Lab (CAL) instrument to be operated aboard the International Space Station (ISS). Utilizing a compact atom chip-based system to create ultracold mixtures and degenerate samples of 87 Rb, 39 K, and 41 K, CAL is a multi-user facility developed by NASA’s Jet Propulsion Laboratory to provide the first persistent quantum gas platform in the microgravity conditions of space. Within this unique environment, atom traps can be decompressed to arbitrarily weak confining potentials, producing a new regime of picokelvin temperatures and ultra-low densities. Further, the complete removal of these confining potential allows the free fall evolution of ultracold clouds to be observed on unprecedented timescales compared to earthbound instruments. This unique facility will enable novel ultracold atom research to be remotely performed by an international group of principle investigators with broad applications in fundamental physics and inertial sensing. Here, we describe the development and validation of critical CAL technologies, including demonstration of the first on-chip Bose–Einstein condensation (BEC) of 87 Rb with microwave-based evaporation and the generation of ultracold dual-species quantum gas mixtures of 39 K/ 87 Rb and 41 K/ 87 Rb in an atom chip trap via sympathetic cooling.
With the recent production of Bose-Einstein condensates using NASA's Cold Atom Laboratory (CAL) aboard the International Space Station, research is underway focusing on the extent to which quantum mechanics can be studied in a microgravity environment. These condensates have the potential to be the coldest ever studied in experiment and in free-fall their place in orbit allows us to observe them in long time-of-flights. This thesis reports fitting analyses and trap frequency characterization of imaging data from condensates in conventional magnetic potentials. This information will be used for the calibration and design of future experiments with CAL, regarding both conventional and radio-frequency dressed traps. Of particular interest to further study are ellipsoidal shell condensates and the quasi-two-dimensional condensate that exists on its surface in the limit of low shell thickness.
BECCAL (Bose-Einstein-Condensate - Cold Atom Laboratory) is an experiment designed to be housed on the International Space Station (ISS) within a bilateral collaboration between DLR and NASA. The payload's design and operation are based on the previous quantum experiments under microgravity, QUANTUS (drop tower), MAIUS (sounding rocket), and CAL (NASA operated ISS experiment). The scienti�c capabilities, outlined here, cover a wide range of cold atom manipulation and observation. Additionally, the payload strives to pave the road for future microgravity missions housing cold atom ensembles.
Deployment of ultracold atom interferometers (AI) into space will capitalize on quantum advantages and the extended freefall of persistent microgravity to provide high-precision measurement capabilities for gravitational, Earth, and planetary sciences, and to enable searches for subtle forces signifying physics beyond General Relativity and the Standard Model. NASA’s Cold Atom Lab (CAL) operates onboard the International Space Station as a multi-user facility for fundamental studies of ultracold atoms and to mature space-based quantum technologies. We report on pathfinding experiments utilizing ultracold 87Rb atoms in the CAL AI. A three-pulse Mach–Zehnder interferometer was studied to understand the influence of ISS vibrations. Additionally, Ramsey shear-wave interferometry was used to manifest interference patterns in a single run that were observable for over 150 ms free-expansion time. Finally, the CAL AI was used to remotely measure the Bragg laser photon recoil as a demonstration of the first quantum sensor using matter-wave interferometry in space. NASA’s Cold Atom Lab has operated on the International Space Station since 2018 to study quantum gases and mature quantum technologies in Earth’s orbit. Here, Williams et al., report on a series of pathfinding experiments exploring the first quantum sensor using atom interferometry in space.
Quantum-optical experiments situated in a gravitationally bound experimental setup are fundamentally limited in numerous ways, such as the gravitational sag experienced by the trapped atoms or the limited free-evolution times of an atomic interferometer.These constraints can be overcome by deploying the experiment in a microgravity platform, such as the International Space Station (ISS).The Bose-Einstein Condensate and Cold Atom Laboratory (BECCAL), a collaboration between NASA and DLR and successor to NASA's CAL mission, aims to achieve just that.Planned as a multi-user experimental facility, it will enable numerous quantum-optical experiments with ultracold atomic clouds of different isotopes of rubidium and potassium in the microgravity environment of the ISS.The optical capabilities of this experiment will be manifold: Atoms can be cooled and trapped using a 2D-and 3D-magneto optical trap (MOT).They can then be loaded into a red-detuned crossed optical dipole trap.Using blue-detuned light, arbitrary painted optical potentials can be applied.Atom interferometry along two separate interferometry axes is also possible.Fluorescence and absorption detection are available for imaging of the atomic ensemble.In this paper, we present a compact and robust optical distribution system which is required to enable this functionality.To this end, we use a combination of fiber-to-fiber coupled optical benches, and fiber-based components.This distribution system needs to withstand the vibrational loads during launch to the ISS, and needs to retain a good fiber-to-fiber coupling efficiency under varying environmental conditions, such as temperature fluctuations, without maintenance, through the multi-year mission time.We have designed a total of ten optical benches, eight for light distribution and two as spectroscopic units.The optical benches make use of our micro-optical bench toolkit based on the glass-ceramic Zerodur, which has mechanical properties akin to aluminium and a negligible coefficient of thermal expansion.The toolkit has been