scholarly journals Stratospheric Aerosol and Gas Experiment (SAGE) from SAGE III on the ISS to a Free Flying SAGE IV Cubesat

2021 ◽  
Vol 13 (22) ◽  
pp. 4664
Author(s):  
John P. Leckey ◽  
Robert Damadeo ◽  
Charles A. Hill

The Stratospheric Aerosol and Gas Experiment III (SAGE III) on the International Space Station (ISS) is widely accepted as a stable source for high-quality stratospheric ozone, aerosol, and water vapor measurements since it was installed on the ISS in 2017. The ISS is a unique platform that provides access for hosted payloads while furnishing infrastructure for power, uplink, downlink, etc. for instrument operations. The opportunities, risks, and challenges from operating on the ISS are described in addition to comprehensive lessons learned. In addition, SAGE IV is presented as an option for the future of the SAGE lineage where the lessons learned from SAGE III and technological advances have enabled the instrument to fit into a 6U CubeSat yielding a significantly smaller and cheaper form-factor to preserve the continuity of critical atmospheric measurements.

Author(s):  
Koji INAKA ◽  
Saori ICHIMIZU ◽  
Izumi YOSHIZAKI ◽  
Kiyohito KIHIRA ◽  
Elena G. LAVRENKO ◽  
...  

A series of space experiments aboard the International Space Station (ISS) associated with high-quality Protein Crystal Growth (PCG) in microgravity conditions can be considered as a unique and one of the best examples of fruitful collaboration between Japanese and Russian scientists and engineers in space, which includes also other ISS International Partners. X-ray diffraction is still the most powerful tool to determine the protein three dimensional structure necessary for Structure based drug design (SBDD). The major purpose of the experiment is to grow high quality protein crystals in microgravity for X-ray diffraction on Earth. Within one and a half decade, Japan and Russia have established an efficient process over PCG in space to support latest developments over drug design and structural biology. One of the keys for success of the experiment lies in how precisely pre-launch preparations are made. Japanese party provides flight equipment for crystallization and ensures the required environment to support the experiment aboard of the ISS’s Kibo module, and also mainly takes part of the experiment ground support such as protein sample characterization, purification, crystallization screening, and solution optimization for microgravity experiment. Russian party is responsible for integration of the flight items equipped with proteins and precipitants on board Russian transportation space vehicles (Soyuz or Progress), for delivery them at the ISS, transfer to Kibo module, and returning the experiments’ results back on Earth aboard Soyuz manned capsule. Due to close cooperation of the parties and solid organizational structure, samples can be launched at the ISS every half a year if the ground preparation goes smoothly. The samples are crystallized using counter diffusion method at 20 degree C for 1–2.5 months. After samples return, the crystals are carefully taken out from the capillary, and frozen for X-ray diffraction at SPring8 facility in Japan. Extensive support of researchers from both countries is also a part of this process. The paper analyses details of the PCG experiment scheme, unique and reliable technology of its execution, and contains examples of the application. Key words: International Space Station, Protein crystals, Microgravity, International collaboration.


2021 ◽  
Author(s):  
Susan Kizer ◽  
David Flittner ◽  
Marilee Roell ◽  
Robert Damadeo ◽  
Carrie Roller ◽  
...  

<p>The Stratospheric Aerosol and Gas Experiment III (SAGE III) instrument installed on the International Space Station (ISS) has completed over three and a half years of data collection and production of science data products. The SAGE III/ISS is a solar and lunar occultation instrument that scans the light from the Sun and Moon through the limb of the Earth’s atmosphere to produce vertical profiles of aerosol, ozone, water vapor, and other trace gases. It continues the legacy of previous SAGE instruments dating back to the 1970s to provide data continuity of stratospheric constituents critical for assessing trends in the ozone layer. This presentation shows the validation results of comparing SAGE III/ISS ozone and water vapor vertical profiles from the newly released v5.2 science product with those of in situ and satellite data .</p>


2014 ◽  
Author(s):  
Michael Cisewski ◽  
Joseph Zawodny ◽  
Joseph Gasbarre ◽  
Richard Eckman ◽  
Nandkishore Topiwala ◽  
...  

2012 ◽  
Vol 134 (10) ◽  
Author(s):  
Rishi Raj ◽  
Jungho Kim ◽  
John McQuillen

The relatively poor understanding of gravity effects on pool boiling heat transfer can be attributed to the lack of long duration high-quality microgravity data, g-jitter associated with ground-based low gravity facilities, little data at intermediate gravity levels, and a poor understanding of the effect of important parameters even at earth gravity conditions. The results of over 200 pool boiling experiments with n-perfluorohexane as the test fluid performed aboard the International Space Station (ISS) are presented in this paper. A flat, transparent, constant temperature microheater array was used to perform experiments over a wide range of temperatures (55 °C < Tw < 107.5 °C), pressures (0.58 atm < P < 1.86 atm), subcoolings (1 °C ≤ ΔTsub ≤ 26 °C), and heater sizes (4.2 mm ≤ Lh ≤ 7.0 mm). The boiling process was visualized from the side and bottom. Based on this high quality microgravity data (a/g<10−6), the recently reported gravity scaling parameter for heat flux, which was primarily based on parabolic flight experiments, was modified to account for these new results. The updated model accurately predicts the experimental microgravity data to within ±20%. The robustness of this framework in predicting low gravity heat transfer is further demonstrated by predicting many of the trends in the pool boiling literature that cannot be explained by any single model.


Author(s):  
Gloria Hernandez ◽  
Joseph M. Zawodny ◽  
Michael S. Cisewski ◽  
Brooke Thornton ◽  
Andrew Panetta ◽  
...  

Life ◽  
2021 ◽  
Vol 11 (6) ◽  
pp. 492
Author(s):  
Christina L. M. Khodadad ◽  
Cherie M. Oubre ◽  
Victoria A. Castro ◽  
Stephanie M. Flint ◽  
Monsi C. Roman ◽  
...  

Closed environments such as the International Space Station (ISS) and spacecraft for other planned interplanetary destinations require sustainable environmental control systems for manned spaceflight and habitation. These systems require monitoring for microbial contaminants and potential pathogens that could foul equipment or affect the health of the crew. Technological advances may help to facilitate this environmental monitoring, but many of the current advances do not function as expected in reduced gravity conditions. The microbial monitoring system (RAZOR® EX) is a compact, semi-quantitative rugged PCR instrument that was successfully tested on the ISS using station potable water. After a series of technical demonstrations between ISS and ground laboratories, it was determined that the instruments functioned comparably and provided a sample to answer flow in approximately 1 hour without enrichment or sample manipulation. Post-flight, additional advancements were accomplished at Kennedy Space Center, Merritt Island, FL, USA, to expand the instrument’s detections of targeted microorganisms of concern such as water, food-borne, and surface microbes including Salmonella enterica serovar Typhimurium, Pseudomonas aeruginosa, Escherichia coli, and Aeromonas hydrophilia. Early detection of contaminants and bio-fouling microbes will increase crew safety and the ability to make appropriate operational decisions to minimize exposure to these contaminants.


1999 ◽  
Author(s):  
Lorelei S. Szatkowski ◽  
Obie H. Bradley, Jr. ◽  
Lemuel E. Mauldin III ◽  
Mary B. Wusk ◽  
William P. Chu ◽  
...  

2015 ◽  
Vol 10 (6) ◽  
pp. 1031-1034 ◽  
Author(s):  
Takashi Sugita ◽  
◽  
Otomi Cho

A wide variety of microorganisms colonize the human skin and are important to maintaining human health. However, this community is highly sensitive to perturbations, and diseases can develop when the skin microbiome is disrupted by a change in host or environmental conditions. The International Space Station (ISS) is a closed environment, and astronauts on the ISS do not wash their bodies as frequently as when they are on the ground. The maintenance of a balanced skin microbiome is important to overall health, disease prevention, and a high quality of life while on the ISS. The skin fungal microbiome is dominated by Malassezia sp. These lipophilic fungi are ubiquitous across different skin types, whereas changes in the levels of M. globosa and M. restricta are correlated with the formation of seborreich dermatitis/dandruff. The Malassezia microbiome on the skin of astronauts staying on the ISS changed, and there was a reduction in skin fungal microbial diversity. These findings provide useful information about temporal changes in the hygiene of astronauts who are on the ISS for an extended period and indicate that Malassezia microbiome as microbiological markers of skin hygiene.


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