Relevant bibliographies by topics / Solar cells, Extraterrestrial environments

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  2. Dissertations / Theses
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  4. Book chapters
  5. Conference papers

Academic literature on the topic 'Solar cells, Extraterrestrial environments'

Author: Grafiati
Published: 4 June 2021
Last updated: 8 February 2022

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Journal articles on the topic "Solar cells, Extraterrestrial environments"

1

Iles, Peter A. "Future use of silicon solar cells in extraterrestrial applications." Progress in Photovoltaics: Research and Applications 2, no. 2 (April 1994): 95–106. http://dx.doi.org/10.1002/pip.4670020204.

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Lage, Claudia A. S., Gabriel Z. L. Dalmaso, Lia C. R. S. Teixeira, Amanda G. Bendia, Ivan G. Paulino-Lima, Douglas Galante, Eduardo Janot-Pacheco, et al. "Mini-Review: Probing the limits of extremophilic life in extraterrestrial environment-simulated experiments." International Journal of Astrobiology 11, no. 4 (August 16, 2012): 251–56. http://dx.doi.org/10.1017/s1473550412000316.

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AbstractAstrobiology is a relatively recent scientific field that seeks to understand the origin and dynamics of life in the Universe. Several hypotheses have been proposed to explain life in the cosmic context throughout human history, but only now, technology has allowed many of them to be tested. Laboratory experiments have been able to show how chemical elements essential to life, such as carbon, nitrogen, oxygen and hydrogen combine in biologically important compounds. Interestingly, these compounds are ubiquitous. How these compounds were combined to the point of originating cells and complex organisms is still to be unveiled by science. However, our 4.5 billion years old Solar system appeared in a 10 billion years old Universe. Thus, simple cells such as micro-organisms may have had time to form in planets older than ours or in other suitable places in the Universe. One hypothesis related to the appearance of life on Earth is called panspermia, which predicts that microbial life could have been formed in the Universe billions of years ago, travelling between planets, and inseminating units of life that could have become more complex in habitable planets such as Earth. A project designed to test the viability of extremophile micro-organisms exposed to simulated extraterrestrial environments is in progress at the Carlos Chagas Filho Institute of Biophysics (UFRJ, Brazil) to test whether microbial life could withstand inhospitable environments. Radiation-resistant (known or novel ones) micro-organisms collected from extreme terrestrial environments have been exposed (at synchrotron accelerators) to intense radiation sources simulating Solar radiation, capable of emitting radiation in a few hours equivalent to many years of accumulated doses. The results obtained in these experiments reveal an interesting possibility of the existence of microbial life beyond Earth.
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Guttenberg, Nicholas, Huan Chen, Tomohiro Mochizuki, and H. Cleaves. "Classification of the Biogenicity of Complex Organic Mixtures for the Detection of Extraterrestrial Life." Life 11, no. 3 (March 12, 2021): 234. http://dx.doi.org/10.3390/life11030234.

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Searching for life in the Universe depends on unambiguously distinguishing biological features from background signals, which could take the form of chemical, morphological, or spectral signatures. The discovery and direct measurement of organic compounds unambiguously indicative of extraterrestrial (ET) life is a major goal of Solar System exploration. Biology processes matter and energy differently from abiological systems, and materials produced by biological systems may become enriched in planetary environments where biology is operative. However, ET biology might be composed of different components than terrestrial life. As ET sample return is difficult, in situ methods for identifying biology will be useful. Mass spectrometry (MS) is a potentially versatile life detection technique, which will be used to analyze numerous Solar System environments in the near future. We show here that simple algorithmic analysis of MS data from abiotic synthesis (natural and synthetic), microbial cells, and thermally processed biological materials (lab-grown organisms and petroleum) easily identifies relational organic compound distributions that distinguish pristine and aged biological and abiological materials, which likely can be attributed to the types of compounds these processes produce, as well as how they are formed and decompose. This method is independent of the detection of particular masses or molecular species samples may contain. This suggests a general method to agnostically detect evidence of biology using MS given a sufficiently strong signal in which the majority of the material in a sample has either a biological or abiological origin. Such metrics are also likely to be useful for studies of possible emergent living phenomena, and paleobiological samples.
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Abrevaya, Ximena C., Eduardo Cortón, and Pablo J. D. Mauas. "UV habitability and dM stars: an approach for evaluation of biological survival." Proceedings of the International Astronomical Union 5, S264 (August 2009): 443–45. http://dx.doi.org/10.1017/s1743921309993073.

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AbstractDwarf M stars comprise about 75 percent of all stars in the galaxy. For several years planets orbiting M stars have been discarded as suitable places for development of life. This paradigm now has changed and terrestrial-type planets within liquid-water habitable zones (LW-HZ) around M stars are reconsidered as possible hosts for life as we know it. Nevertheless, large amount of UV radiation is emitted during flares by this stars, and it is uncertain how these events could affect biological systems. In particular UV-C λ < 290nm) exhibits the most damaging effects for living organisms. To analyze the hypothesis that UV could set a limit for the development of extraterrestrial life, we studied the effect of UV-C treatment on halophile archaea cultures. Halophile archaea are extremophile organisms, they are exposed to intense solar UV radiation in their natural environment so they are generally regarded as relatively UV tolerant. Halophiles inhabits in hipersaline environments as salt lakes but also have been found in ancient salt deposits as halites and evaporites on Earth. Since evaporites have been detected in Martian meteorites, these organisms are proposed as plausible inhabitants of Mars-like planets. Our preliminary results show that even after UV damage, the surviving cells were able to resume growth with nearly normal kinetics.
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Horneck, Gerda, David M. Klaus, and Rocco L. Mancinelli. "Space Microbiology." Microbiology and Molecular Biology Reviews 74, no. 1 (March 2010): 121–56. http://dx.doi.org/10.1128/mmbr.00016-09.

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SUMMARY The responses of microorganisms (viruses, bacterial cells, bacterial and fungal spores, and lichens) to selected factors of space (microgravity, galactic cosmic radiation, solar UV radiation, and space vacuum) were determined in space and laboratory simulation experiments. In general, microorganisms tend to thrive in the space flight environment in terms of enhanced growth parameters and a demonstrated ability to proliferate in the presence of normally inhibitory levels of antibiotics. The mechanisms responsible for the observed biological responses, however, are not yet fully understood. A hypothesized interaction of microgravity with radiation-induced DNA repair processes was experimentally refuted. The survival of microorganisms in outer space was investigated to tackle questions on the upper boundary of the biosphere and on the likelihood of interplanetary transport of microorganisms. It was found that extraterrestrial solar UV radiation was the most deleterious factor of space. Among all organisms tested, only lichens (Rhizocarpon geographicum and Xanthoria elegans) maintained full viability after 2 weeks in outer space, whereas all other test systems were inactivated by orders of magnitude. Using optical filters and spores of Bacillus subtilis as a biological UV dosimeter, it was found that the current ozone layer reduces the biological effectiveness of solar UV by 3 orders of magnitude. If shielded against solar UV, spores of B. subtilis were capable of surviving in space for up to 6 years, especially if embedded in clay or meteorite powder (artificial meteorites). The data support the likelihood of interplanetary transfer of microorganisms within meteorites, the so-called lithopanspermia hypothesis.
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Ehrenfreund, Pascale, Andreas Elsaesser, and J. Groen. "Prebiotic Matter in Space." Proceedings of the International Astronomical Union 10, H16 (August 2012): 709–10. http://dx.doi.org/10.1017/s1743921314013015.

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AbstractA significant number of molecules that are used in contemporary biochemistry on Earth are found in interstellar and circumstellar regions as well as solar system environments. In particular small solar system bodies hold clues to processes that formed our solar system. Comets, asteroids, and meteorite delivered extraterrestrial material during the heavy bombardment phase ~3.9 billion years ago to the young planets, a process that made carbonaceous material available to the early Earth. In-depth understanding of the organic reservoir in different space environments as well as data on the stability of organic and prebiotic material in solar system environments are vital to assess and quantify the extraterrestrial contribution of prebiotic sources available to the young Earth.
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McKaig, Jordan, Tristan Caro, Alex Hyer, Elizabeth Delgadillo Talburt, Sonali Verma, Kaixin Cui, Anna-Sophia Boguraev, et al. "A High-Altitude Balloon Platform for Space Life Sciences Education." Gravitational and Space Research 7, no. 1 (November 27, 2019): 62–69. http://dx.doi.org/10.2478/gsr-2019-0007.

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AbstractHigh-altitude balloons (HABs) present a valuable and cost-effective tool for educators and students to access the conditions that are analogous to space and extraterrestrial environments in the Earth’s upper atmosphere. Historically, HABs have been used for meteorological measurements, observation, sampling of aerosols, and exposure of samples to upper atmosphere environments. The Earth’s stratosphere allows researchers access to a unique combination of wideband solar radiation, extreme cold, rarefied air, low humidity, and acute ionizing radiation—conditions that are relevant to space biology research. Here, we describe a reproducible payload for a HAB mission that can be constructed, launched, and retrieved for about $3,000. This general standard operating procedure can be used by educators, community scientists, and research teams working with limited resources.
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Ishii, Hope A., John P. Bradley, Hans A. Bechtel, Donald E. Brownlee, Karen C. Bustillo, James Ciston, Jeffrey N. Cuzzi, Christine Floss, and David J. Joswiak. "Multiple generations of grain aggregation in different environments preceded solar system body formation." Proceedings of the National Academy of Sciences 115, no. 26 (June 11, 2018): 6608–13. http://dx.doi.org/10.1073/pnas.1720167115.

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The solar system formed from interstellar dust and gas in a molecular cloud. Astronomical observations show that typical interstellar dust consists of amorphous (a-) silicate and organic carbon. Bona fide physical samples for laboratory studies would yield unprecedented insight about solar system formation, but they were largely destroyed. The most likely repositories of surviving presolar dust are the least altered extraterrestrial materials, interplanetary dust particles (IDPs) with probable cometary origins. Cometary IDPs contain abundant submicrona-silicate grains called GEMS (glass with embedded metal and sulfides), believed to be carbon-free. Some have detectable isotopically anomalousa-silicate components from other stars, proving they are preserved dust inherited from the interstellar medium. However, it is debated whether the majority of GEMS predate the solar system or formed in the solar nebula by condensation of high-temperature (>1,300 K) gas. Here, we map IDP compositions with single nanometer-scale resolution and find that GEMS contain organic carbon. Mapping reveals two generations of grain aggregation, the key process in growth from dust grains to planetesimals, mediated by carbon. GEMS grains, some witha-silicate subgrains mantled by organic carbon, comprise the earliest generation of aggregates. These aggregates (and other grains) are encapsulated in lower-density organic carbon matrix, indicating a second generation of aggregation. Since this organic carbon thermally decomposes above ∼450 K, GEMS cannot have accreted in the hot solar nebula, and formed, instead, in the cold presolar molecular cloud and/or outer protoplanetary disk. We suggest that GEMS are consistent with surviving interstellar dust, condensed in situ, and cycled through multiple molecular clouds.
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Varnali, Tereza, and Howell G. M. Edwards. "Raman spectroscopic identification of scytonemin and its derivatives as key biomarkers in stressed environments." Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences 372, no. 2030 (December 13, 2014): 20140197. http://dx.doi.org/10.1098/rsta.2014.0197.

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Raman spectroscopy has been identified as an important first-pass analytical technique for deployment on planetary surfaces as part of a suite of instrumentation in projected remote space exploration missions to detect extant or extinct extraterrestrial life signatures. Aside from the demonstrable advantages of a non-destructive sampling procedure and an ability to record simultaneously the molecular signatures of biological, geobiological and geological components in admixture in the geological record, the interrogation and subsequent interpretation of spectroscopic data from these experiments will be critically dependent upon the recognition of key biomolecular markers indicative of life existing or having once existed in extreme habitats. A comparison made with the characteristic Raman spectral wavenumbers obtained from standards is not acceptable because of shifts that can occur in the presence of other biomolecules and their host mineral matrices. In this paper, we identify the major sources of difficulty experienced in the interpretation of spectroscopic data centring on a key family of biomarker molecules, namely scytonemin and its derivatives; the parent scytonemin has been characterized spectroscopically in cyanobacterial colonies inhabiting some of the most extreme terrestrial environments and, with the support of theoretical calculations, spectra have been predicted for the characterization of several of its derivatives which could occur in novel extraterrestrial environments. This work will form the foundation for the identification of novel biomarkers and for their Raman spectroscopic discrimination, an essential step in the interpretation of potentially complex and hitherto unknown biological radiation protectants based on the scytoneman and scytonin molecular skeletons which may exist in niche geological scenarios in the surface and subsurface of planets and their satellites in our Solar System.
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Pavlov, Anatoly, Vladimir Cheptsov, Denis Tsurkov, Vladimir Lomasov, Dmitry Frolov, and Gennady Vasiliev. "Survival of Radioresistant Bacteria on Europa’s Surface after Pulse Ejection of Subsurface Ocean Water." Geosciences 9, no. 1 (December 25, 2018): 9. http://dx.doi.org/10.3390/geosciences9010009.

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We briefly present preliminary results of our study of the radioresistant bacteria in a low temperature and pressure and high-radiation environment and hypothesize the ability of microorganisms to survive extraterrestrial high-radiation environments, such as the icy surface of Jupiter’s moon, Europa. In this study, samples containing a strain of Deinococcus radiodurans VKM B-1422T embedded into a simulated version of Europa’s ice were put under extreme environmental (−130 °C, 0.01 mbar) and radiation conditions using a specially designed experimental vacuum chamber. The samples were irradiated with 5, 10, 50, and 100 kGy doses and subsequently studied for residual viable cells. We estimate the limit of the accumulated dose that viable cells in those conditions could withstand at 50 kGy. Combining our numerical modelling of the accumulated dose in ice with observations of water eruption events on Europa, we hypothesize that in the case of such events, it is possible that putative extraterrestrial organisms might retain viability in a dormant state for up to 10,000 years, and could be sampled and studied by future probe missions.
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Dissertations / Theses on the topic "Solar cells, Extraterrestrial environments"

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Hinks, Jonathan. "Radiation damage in copper indium diselenide." Thesis, University of Salford, 2007. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.490441.

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A study of radiation damage in copper indium diselenide (CIS) is presented. The build up of extended defects and the conditions for amorphisation have been explored. In particular, dislocation loops have been characterised and the intluence of composition and temperature on amorphisation has been investigated. CIS is a candidate for high-efficiency radiation-hard solar cells for use in extraterrestrial environments.
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Books on the topic "Solar cells, Extraterrestrial environments"

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Alexander, Dennis. 2 kWe Solar Dynamic Ground Test Demonstration Project. [Washington, DC]: National Aeronautics and Space Administration, 1997.

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Alexander, Dennis. 2 kWe Solar Dynamic Ground Test Demonstration Project. [Washington, DC]: National Aeronautics and Space Administration, 1997.

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Alexander, Dennis. 2 kWe Solar Dynamic Ground Test Demonstration Project. [Washington, DC]: National Aeronautics and Space Administration, 1997.

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Dave, Hill. Summary of solar cell data from the Long Duration Exposure Facility (LDEF): Final report, 21 July 1993 - 19 August 1994. Auburn University, AL: Space Power Institute, 1994.

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Hill, Dave. Summary of solar cell data from the Long Duration Exposure Facility (LDEF): Final report, 21 July 1993 - 19 August 1994. Auburn University, AL: Space Power Institute, 1994.

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Geoffrey, Landis, and United States. National Aeronautics and Space Administration., eds. Use of advanced solar cells for commercial communication satellites. [Washington, D.C.]: National Aeronautics and Space Administration, 1995.

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A, Landis Geoffrey, and United States. National Aeronautics and Space Administration., eds. Use of advanced solar cells for commercial communication satellites. [Washington, D.C.]: National Aeronautics and Space Administration, 1995.

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A, Xapsos M., and George C. Marshall Space Flight Center., eds. Space environment effects: Model for emission of solar protons (ESP)--cumulative and worst-case event fluences. [Marshall Space Flight Center], Ala: National Aeronautics and Space Administration, Marshall Space Flight Center, 1999.

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Center, NASA Glenn Research, ed. Effect of voltage level on power system design for solar electric propulsion missions. [Cleveland, Ohio]: National Aeronautics and Space Administration, Glenn Research Center, 2003.

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Center, NASA Glenn Research, ed. Effect of voltage level on power system design for solar electric propulsion missions. [Cleveland, Ohio]: National Aeronautics and Space Administration, Glenn Research Center, 2003.

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Book chapters on the topic "Solar cells, Extraterrestrial environments"

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McElroy, Michael B. "Power from the Sun Abundant But Expensive." In Energy and Climate. Oxford University Press, 2016. http://dx.doi.org/10.1093/oso/9780190490331.003.0015.

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As discussed in the preceding chapter, wind resources available from nonforested, nonurban, land-based environments in the United States are more than sufficient to meet present and projected future US demand for electricity. Wind resources are comparably abundant elsewhere. As indicated in Table 10.2, a combination of onshore and offshore wind could accommodate prospective demand for electricity for all of the countries classified as top- 10 emitters of CO2. Solar energy reaching the Earth’s surface averages about 200 W m– 2 (Fig. 4.1). If this power source could be converted to electricity with an efficiency of 20%, as little as 0.1% of the land area of the United States (3% of the area of Arizona) could supply the bulk of US demand for electricity. As discussed later in this chapter, the potential source of power from the sun is significant even for sun- deprived countries such as Germany. Wind and solar energy provide potentially complementary sources of electricity in the sense that when the supply from one is low, there is a good chance that it may be offset by a higher contribution from the other. Winds blow strongest typically at night and in winter. The potential supply of energy from the sun, in contrast, is highest during the day and in summer. The source from the sun is better matched thus than wind to respond to the seasonal pattern of demand for electricity, at least for the United States (as indicated in Fig. 10.5).There are two approaches available to convert energy from the sun to electricity. The first involves using photovoltaic (PV) cells, devices in which absorption of radiation results directly in production of electricity. The second is less direct. It requires solar energy to be captured and deployed first to produce heat, with the heat used subsequently to generate steam, the steam applied then to drive a turbine. The sequence in this case is similar to that used to generate electricity in conventional coal, oil, natural gas, and nuclear- powered systems. The difference is that the energy source is light from the sun rather than a carbon- based fossil fuel or fissionable uranium.
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Conference papers on the topic "Solar cells, Extraterrestrial environments"

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Anderson, Steven D., and Jekan Thangavelautham. "Solar-Powered Additive Manufacturing in Extraterrestrial Environments." In 17th Biennial International Conference on Engineering, Science, Construction, and Operations in Challenging Environments. Reston, VA: American Society of Civil Engineers, 2021. http://dx.doi.org/10.1061/9780784483374.068.

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Djordjevich, Nik. "Performance of a Flat Plate Solar Collector in Extraterrestrial Environments." In International Conference On Environmental Systems. 400 Commonwealth Drive, Warrendale, PA, United States: SAE International, 1994. http://dx.doi.org/10.4271/941270.

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Sayre, Larkin, Felix Lang, Jurgen Bundesmann, Andrea Denker, Phoebe Pearce, Andrew Johnson, and Louise Hirst. "Ultra-thin Single-junction GaAs Solar Cells For Extreme Space Environments." In 2020 IEEE 47th Photovoltaic Specialists Conference (PVSC). IEEE, 2020. http://dx.doi.org/10.1109/pvsc45281.2020.9300596.

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Boca, Andreea, Jonathan Grandidier, Paul Stella, Philip Chiu, Xing-Quan Liu, James Ermer, Claiborne McPheeters, Christopher Kerestes, and Paul Sharps. "Development of High-Performance Solar Cells for the Jupiter and Saturn Environments." In 2018 IEEE 7th World Conference on Photovoltaic Energy Conversion (WCPEC) (A Joint Conference of 45th IEEE PVSC, 28th PVSEC & 34th EU PVSEC). IEEE, 2018. http://dx.doi.org/10.1109/pvsc.2018.8548171.

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Bialic, Emilie. "Semi-transparent solar cells indifferent to ambient lighting for LiFi application." In 2016 IEEE International Conference on Wireless for Space and Extreme Environments (WiSEE). IEEE, 2016. http://dx.doi.org/10.1109/wisee.2016.7877300.

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ElMahgoub, Khaled, and Atef Z. Elsherbeni. "Analysis of nanoparticles shape for efficient absorption in nanoplasmonic solar cells." In 2013 IEEE International Conference on Wireless for Space and Extreme Environments (WiSEE). IEEE, 2013. http://dx.doi.org/10.1109/wisee.2013.6737546.

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Arumughan, J., R. Kopecek, T. Pernau, T. Buck, P. Fath, and K. Peter. "Realization of Thin MC-Silicon Pert-Type Bifacial Solar Cells in Industrial Environments." In Conference Record of the 2006 IEEE 4th World Conference on Photovoltaic Energy Conversion. IEEE, 2006. http://dx.doi.org/10.1109/wcpec.2006.279353.

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Alateeq, Ahmed, and An Chen. "Performance of Solar Cells Integrated with Rigid and Flexible Substrates under Compression." In 16th Biennial International Conference on Engineering, Science, Construction, and Operations in Challenging Environments. Reston, VA: American Society of Civil Engineers, 2018. http://dx.doi.org/10.1061/9780784481899.115.

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Masharin, Mikhail, Dmitry Gets, Grigoriy Verkhoglyadov, Sergey Makarov, and Anvar Zakhidov. "Polymer modification of perovskite solar cells to increase open-circuit voltage." In INTERNATIONAL CONFERENCE ON PHYSICS AND CHEMISTRY OF COMBUSTION AND PROCESSES IN EXTREME ENVIRONMENTS (COMPHYSCHEM’20-21) and VI INTERNATIONAL SUMMER SCHOOL “MODERN QUANTUM CHEMISTRY METHODS IN APPLICATIONS”. AIP Publishing, 2020. http://dx.doi.org/10.1063/5.0031984.

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Shimada, T., H. Toyota, A. Kukita, M. Imaizumi, K. Hirose, M. Tajima, H. Ogawa, et al. "Durability evaluation of InGaP/GaAs/Ge triple-junction solar cells in HIHT environments for Mercury exploration mission." In 2010 35th IEEE Photovoltaic Specialists Conference (PVSC). IEEE, 2010. http://dx.doi.org/10.1109/pvsc.2010.5614720.

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