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Artykuły w czasopismach na temat "Interplanetary science"

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DONN, B. "Interplanetary Dust: Properties and Interactions of Interplanetary Dust." Science 233, nr 4764 (8.08.1986): 673. http://dx.doi.org/10.1126/science.233.4764.673.

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Exarhos, G., i X. Moussas. "On the heliolatitudinal variation of the galactic cosmic-ray intensity. Comparison with Ulysses measurements". Annales Geophysicae 21, nr 6 (30.06.2003): 1341–45. http://dx.doi.org/10.5194/angeo-21-1341-2003.

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Abstract. We study the dependence of cosmic rays with heliolatitude using a simple method and compare the results with the actual data from Ulysses and IMP spacecraft. We reproduce the galactic cosmic-ray heliographic latitudinal intensity variations, applying a semi-empirical, 2-D diffusion-convection model for the cosmic-ray transport in the interplanetary space. This model is a modification of our previous 1-D model (Exarhos and Moussas, 2001) and includes not only the radial diffusion of the cosmic-ray particles but also the latitudinal diffusion. Dividing the interplanetary region into "spherical magnetic sectors" (a small heliolatitudinal extension of a spherical magnetized solar wind plasma shell) that travel into the interplanetary space at the solar wind velocity, we calculate the cosmic-ray intensity for different heliographic latitudes as a series of successive intensity drops that all these "spherical magnetic sectors" between the Sun and the heliospheric termination shock cause the unmodulated galactic cosmic-ray intensity. Our results are compared with the Ulysses cosmic-ray measurements obtained during the first pole-to-pole passage from mid-1994 to mid-1995.Key words. Interplanetary physics (cosmic rays; interplanetray magnetic fields; solar wind plasma)
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Martin-Mur, T. J., G. L. Kruizinga, P. D. Burkhart, F. Abilleira, M. C. Wong i J. A. Kangas. "Mars Science Laboratory Interplanetary Navigation". Journal of Spacecraft and Rockets 51, nr 4 (lipiec 2014): 1014–28. http://dx.doi.org/10.2514/1.a32631.

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Martin-Mur, Tomas J., Gerard L. Kruizinga i Mau C. Wong. "Mars science laboratory interplanetary navigaton analysis". Journal of Aerospace Engineering, Sciences and Applications 4, nr 2 (1.04.2012): 107–20. http://dx.doi.org/10.7446/jaesa.0402.10.

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Zweibel, E. G. "The Solar Wind: Interplanetary Magnetohydrodynamics." Science 272, nr 5261 (26.04.1996): 495b—496b. http://dx.doi.org/10.1126/science.272.5261.495b.

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CHRISTOFFERSEN, R., i P. R. BUSECK. "Refractory Minerals in Interplanetary Dust". Science 234, nr 4776 (31.10.1986): 590–92. http://dx.doi.org/10.1126/science.234.4776.590.

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ZOLENSKY, M. E. "Reports Refractory Interplanetary Dust Particles". Science 237, nr 4821 (18.09.1987): 1466–68. http://dx.doi.org/10.1126/science.237.4821.1466.

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Hand, Eric. "Interplanetary small satellites come of age". Science 361, nr 6404 (23.08.2018): 736–37. http://dx.doi.org/10.1126/science.361.6404.736.

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Watari, S., M. Vandas i T. Watanabe. "Formation of a strong southward IMF near the solar maximum of cycle 23". Annales Geophysicae 22, nr 2 (1.01.2004): 673–87. http://dx.doi.org/10.5194/angeo-22-673-2004.

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Abstract. We analyzed observations of the solar activities and the solar wind parameters associated with large geomagnetic storms near the maximum of solar cycle 23. This analysis showed that strong southward interplanetary magnetic fields (IMFs), formed through interaction between an interplanetary disturbance, and background solar wind or between interplanetary disturbances are an important factor in the occurrence of intense geomagnetic storms. Based on our analysis, we seek to improve our understanding of the physical processes in which large negative Bz's are created which will lead to improving predictions of space weather. Key words. Interplanetary physics (Flare and stream dynamics; Interplanetary magnetic fields; Interplanetary shocks)
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Smith, D. E. "Two-Way Laser Link over Interplanetary Distance". Science 311, nr 5757 (6.01.2006): 53. http://dx.doi.org/10.1126/science.1120091.

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Rozprawy doktorskie na temat "Interplanetary science"

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Prathaban, Mahendiran. "Contributions to the performance study of interplanetary networks". Phd thesis, Institut National des Télécommunications, 2010. http://tel.archives-ouvertes.fr/tel-00538532.

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L'acquisition de connaissances sur l'espace fascine les humains depuis l'antiquité. Depuis quelques décennies, il y a augmentation significative des programmes spatiaux concernant Mars, des missions d'exploration lunaire et des projets d'exploration spatiale de plus en plus complexes, impliquant plusieurs nœuds de communication: satellites, robots (Rovers, Landers) ou "aerorobots" (ie capteurs atmosphériques). Dans ce cadre, des efforts ont été faits par les organismes de normalisation pour l'espace comme le Comité consultatif pour les systèmes de données spatiales (CCSDS) et le Delay Tolérant Networking groupe de travail au sein del' Internet Research Task Force (IRTF) pour élaborer une architecture de protocoles efficace pour des missions spatiales. Dans cette thèse, nous avons analysé quelques unes de ces propositions : (les piles de protocole CCSDS, et DTN) pour leurs performances sur la surface de Mars (une sous-section de Interplanetary Network) et obtenu les paramètres qui affectent les performances du système, comme la mémoire tampon, les limitations de puissance. Également exploré divers problèmes de réseau de routage, Transport & couches de l'application de la pile de protocole, qui doit être abordée. Pour qui s'étendent, dans cette thèse nous avons proposé un nouvel algorithme de routage prenant en compte les ressources disponibles, qui prend en considération les limitations des ressources du réseau pour le routage et transmet les décisions permettant une politique efficace de gestion des tampons. Comme il existe différentes piles de protocoles d'interopérabilité proposées par l'agence spatiale, dans nos travaux, nous avons développé un framework de QoS qui est joint à chaque application, et peut sélectionner la pile de protocoles sous-jacents adéquate, selon les exigences de qualité de service des applications, qui sont les mieux adaptés pour améliorer les performances globales de ce réseau. Comme l'analyse révèle que les performances du protocole de remise de fichiers CCSDS lequel est le plus couramment utilisé le protocole d'application dans la mission spatiale. Pour améliorer les performances du protocole, nous avons proposé un algorithme dynamique du timer qui fixe la valeur du time-out en fonction de l'état du réseau pour tous les timers du protocole, afin de réduire les retransmissions inutiles de données d'UFC, accroissant ainsi les performances de débit.
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Lindner, Patricia J. "Bundle Security: Verifying Confidentiality and Integrity for the Interplanetary Overlay Network". Ohio University / OhioLINK, 2019. http://rave.ohiolink.edu/etdc/view?acc_num=ohiou1554911833066868.

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Huff, John D. "Performance Characteristics of the Interplanetary Overlay Network in 10 Gbps Networks". Ohio University / OhioLINK, 2021. http://rave.ohiolink.edu/etdc/view?acc_num=ohiou1619115602389023.

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Losik, Len. "Using Telemetry Science, An Adaptation of Prognostic Algorithms for Predicting Normal Space Vehicle Telemetry Behavior from Space for Earth and Lunar Satellites and Interplanetary Spacecraft". International Foundation for Telemetering, 2009. http://hdl.handle.net/10150/606150.

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ITC/USA 2009 Conference Proceedings / The Forty-Fifth Annual International Telemetering Conference and Technical Exhibition / October 26-29, 2009 / Riviera Hotel & Convention Center, Las Vegas, Nevada
Prognostic technology uses a series of algorithms, combined forms a prognostic-based inference engine (PBIE) for the identification of deterministic behavior embedded in completely normal appearing telemetry from fully functional equipment. The algorithms used to define normal behavior in the PBIE from which deterministic behavior is identified can be adapted to quantify normal spacecraft telemetry behavior while in orbit about a moon or planet or during interplanetary travel. Time-series analog engineering data (telemetry) from orbiting satellites and interplanetary spacecraft are defined by harmonic and non-harmonic influences which shape it behavior. Spectrum analysis can be used to understand and quantify the fundamental behavior of spacecraft analog telemetry and relate the behavior's frequency and phase to its time-series behavior through Fourier analysis.
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Uwamahoro, Jean. "An analysis of sources and predictability of geomagnetic storms". Thesis, Rhodes University, 2011. http://hdl.handle.net/10962/d1005236.

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Solar transient eruptions are the main cause of interplanetary-magnetospheric disturbances leading to the phenomena known as geomagnetic storms. Eruptive solar events such as coronal mass ejections (CMEs) are currently considered the main cause of geomagnetic storms (GMS). GMS are strong perturbations of the Earth’s magnetic field that can affect space-borne and ground-based technological systems. The solar-terrestrial impact on modern technological systems is commonly known as Space Weather. Part of the research study described in this thesis was to investigate and establish a relationship between GMS (periods with Dst ≤ −50 nT) and their associated solar and interplanetary (IP) properties during solar cycle (SC) 23. Solar and IP geoeffective properties associated with or without CMEs were investigated and used to qualitatively characterise both intense and moderate storms. The results of this analysis specifically provide an estimate of the main sources of GMS during an average 11-year solar activity period. This study indicates that during SC 23, the majority of intense GMS (83%) were associated with CMEs, while the non-associated CME storms were dominant among moderate storms. GMS phenomena are the result of a complex and non-linear chaotic system involving the Sun, the IP medium, the magnetosphere and ionosphere, which make the prediction of these phenomena challenging. This thesis also explored the predictability of both the occurrence and strength of GMS. Due to their nonlinear driving mechanisms, the prediction of GMS was attempted by the use of neural network (NN) techniques, known for their non-linear modelling capabilities. To predict the occurrence of storms, a combination of solar and IP parameters were used as inputs in the NN model that proved to predict the occurrence of GMS with a probability of 87%. Using the solar wind (SW) and IP magnetic field (IMF) parameters, a separate NN-based model was developed to predict the storm-time strength as measured by the global Dst and ap geomagnetic indices, as well as by the locally measured K-index. The performance of the models was tested on data sets which were not part of the NN training process. The results obtained indicate that NN models provide a reliable alternative method for empirically predicting the occurrence and strength of GMS on the basis of solar and IP parameters. The demonstrated ability to predict the geoeffectiveness of solar and IP transient events is a key step in the goal towards improving space weather modelling and prediction.
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Vogt, Marissa Farland. "Analyzing the large-scale curvature of interplanetary shocks". Thesis, Massachusetts Institute of Technology, 2006. http://hdl.handle.net/1721.1/114134.

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Thesis: S.B., Massachusetts Institute of Technology, Department of Earth, Atmospheric, and Planetary Sciences, 2006.
Thesis: S.B., Massachusetts Institute of Technology, Department of Physics, 2006.
Cataloged from PDF version of thesis.
Includes bibliographical references (pages 36-37).
The 3-dimensional structure of interplanetary shock surfaces are analyzed using observations from the Wind and ACE spacecraft. Events seen by both spacecraft were selected from the available data and used to calculate the radius of curvature R, of the shock surface. The surface structure was examined within the ecliptic plane, and evidence of large-scale curvature was seen when the spacecraft separation was sufficiently large. A simulation was run to test the effects of small errors in the shock normal, and showed that these errors could affect R, calculations at small separation. The radius of curvature was studied as a function of shock strength to look for evidence of ripples on the shock surface, though no correlation was found.
by Marissa F. Vogt.
S.B.
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Bomark, David. "Den interplanetära rasismen : Star Trek Enterprise möte med världsrymden". Thesis, Södertörns högskola, Institutionen för kultur och kommunikation, 2012. http://urn.kb.se/resolve?urn=urn:nbn:se:sh:diva-16822.

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Denna studie vill undersöka om koloniala strukturer genomsyrar den senaste i raden av Star Trek-serierna, Enterprise. Med utgångspunkt i äldre forskning om just koloniala strukturer i Star Trek kommer en jämförelse göras om Enterprise först och främst har dessa strukturer och om så är fallet, göra en jämförelse med de andra serierna. Det postkoloniala forskningsfältet tillsammans med ett strukturalistiskt och post-strukturalistiskt tillvägagångssätt som innefattar semiotik och diskursanalys används för att kunna peka på hur de koloniala strukturerna genomsyrar serien. Analysen, som bland annat innefattar besättningens inbördes hierarki, hur andra främmande raser ser ut och vilka egenskaper de har och hur mötet går till med andra kulturer, visar att de koloniala strukturerna fortfarande genomsyrar Star Trek. Enterprise skiljer sig dock från de äldre serierna på ett sådant sätt att det koloniala tar mindre plats, bland annat seriens handling och även hur alla besättningsmedlemmar är med och skapar seriens handling.
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Wennergren, Oscar, Mattias Vidhall i Jimmy Sörensen. "Transparency analysis of Distributed file systems : With a focus on InterPlanetary File System". Thesis, Högskolan i Skövde, Institutionen för informationsteknologi, 2018. http://urn.kb.se/resolve?urn=urn:nbn:se:his:diva-15727.

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IPFS claims to be the replacement of HTTP and aims to be used globally. However, our study shows that in terms of scalability, performance and security, IPFS is inadequate. This is a result from our experimental and qualitative study of transparency of IPFS version 0.4.13. Moreover, since IPFS is a distributed file system, it should fulfill all aspects of transparency, but according to our study, this is not the case. From our small-scale analysis, we speculate that nested files appear to be the main cause of the performance issues and replication amplifies these problems even further.
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Souza, Carlos A. Loiola de. "Carl Sagan: a exploração e colonização de planetas - ficção científica,cência e divulgação". Pontifícia Universidade Católica de São Paulo, 2006. https://tede2.pucsp.br/handle/handle/13337.

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Made available in DSpace on 2016-04-28T14:16:25Z (GMT). No. of bitstreams: 1 CARLOS A LOIOLA DE SOUZA.pdf: 415449 bytes, checksum: d861caf6da8174df5e70f24cd0bc6748 (MD5) Previous issue date: 2006-05-29
Sci - fi books depending on how they are structured by their authors, might be in our case, the astronomer Carl Sagan, be used as reference texts in Science History by his indisciplinity. The specific case of interplanetary trips, theorized and thought scientificaly and advertised under a sci - fi language in books of Carl Sagan, is what this dissertation talks about.The authors of fiction texts, such as Sagan Arthur Charles Clarke and Issac Asimov, try to found their extrpolate in careful notes of trends that happen in society and science, and develop the ( narration, in Asmov and Clarke´s case ) implication or advertising with rigidity and consistency.On the other hand, part of the futuristic literature would be an important History of Science analysis instrument, for it to be possible of thinking in alternative proposals for a scientific policy and taught which may have a social reach. A kind of experiment or imaginary exercise. In other words, what is studied here, is the relation between sci - fi and science, which talks about interplanetary trips, and how they are explained in Sagan´s books. However, the dissertation, delimitates, in the first instance, must be considered about interplanetary trips, its dissimilation from the 30´s to the 60´s and the adverstising through two of the best sci - fi writers of the twentieth century, whose work was to advertise scientific ideas or Astronautic for a better understanding of the science, its role and the impact of science and technology, in a society which moves really fast, but without many details. After all, as it was a relevant realization of some of these realized fantasies by Carl Sagan´s commitment, initially, with the American industial military complexduring the Cold War against USSR, and after that by NASA.And what we have learned scientifically from the exploration of the Solar Sistem and the nearest planets, in a way that the results of this spacial exploration could be advertised with the help from literature and fiction, in a type of alert about the problems that we will have to face in a near future. At last, the mankind destiny, imagined by Sagan in a kind of manifest advertised by himself in his main books and analysed here for it to be possible to keep its parallelism of contents and trends between sci - fi books and the academic literatureabout the development of science and technology and the destiny of mankind and the individuals that make itself. This is a conclusion that History students having a beginning or complementary graduation in humanities, will be able to find on the shelves of science history, a worthy manifest for an unexpective reflection or for a militancy
Obras de ficção científica podem, dependendo de como estiverem estruturadas por seus autores, em nosso caso, o astrônomo Carl Sagan, ser usadas como textos de referência em História da Ciência por sua interdisciplinaridade. O caso específico das viagens interplanetárias, pensadas e teorizadas cientificamente e divulgadas sob a linguagem da ficção científica nos livros de Carl Sagan, é o de que se ocupa esta dissertação. Os autores de textos de ficção, como os colegas de Sagan Arthur Charles Clarke e Isaac Asimov, procuram, como acontece com textos teóricos acadêmicos, assim como também eram alguns dos textos de Sagan, fundamentar suas extrapolações em observações cuidadosas de tendências em ação na sociedade e na ciência e desenvolver sua (narração, no caso de Asimov e Clarke) implementação ou divulgação com rigor e consistência. Ou seja, parte da literatura futurística seria um instrumento importante de análise de História da Ciência para que esta possa pensar em propostas alternativas para uma política científica e de ensino científico que tenha um alcance social. Uma espécie de experimento ou exercício imaginário. Em outras palavras, o que aqui se estuda é a relação entre ficção científica e ciência que fale das viagens interplanetárias e como elas estão expressas nas obras de Sagan. Portanto, a dissertação delimita o que, em primeiro lugar, deve-se considerar sobre as viagens interplanetárias, sua disseminação nos anos de 1930 a 1960 e sua divulgação através de dois dos melhores escritores de ficção científica do século XX, que se empenharam em divulgar idéias científicas ou de Astronáutica para uma melhor compreensão da ciência, do papel da ciência e do impacto da ciência e tecnologia numa sociedade com uma velocidade em movimento rápido, mas sem muitos detalhes. Depois, como foi a realização primordial de algumas dessas fantasias realizadas pelo envolvimento de Carl Sagan, inicialmente, com o complexo militar industrial dos Estados Unidos da América durante a Guerra Fria com a URSS e depois pela NASA. E o que se aprendeu, cientificamente, com a exploração de nosso sistema solar e de nossos planetas mais próximos, de maneira que esses resultados da exploração espacial pudessem ser divulgados com a ajuda da literatura de ficção em forma de alerta sobre os problemas que teremos de enfrentar num futuro bem próximo. E, por último, o destino da humanidade imaginado por Sagan numa espécie de manifesto divulgado por ele mesmo em seus principais livros e aqui analisado para que se pudesse manter o paralelismo de conteúdo e tendências entre as obras de ficção e a literatura acadêmica sobre o desenvolvimento da ciência e da tecnologia e o destino da humanidade e dos indivíduos que a compõem. Isto nos leva a concluir que o estudante de História da Ciência, tendo uma formação inicial ou complementar em humanidades, poderá encontrar na estante de História da Ciência um valioso manifesto para uma reflexão despretensiosa ou para a militância
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Andersson, Oscar. "Securing Electronic Health Records : A Blockchain Solution". Thesis, Linnéuniversitetet, Institutionen för datavetenskap och medieteknik (DM), 2021. http://urn.kb.se/resolve?urn=urn:nbn:se:lnu:diva-107330.

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Blockchain is an interesting technology, with different projects developing every day since it first gained its light back in 2008. More and more research finds blockchain useful in several different sectors. One of the sectors being healthcare, specifically for electronic health records (EHR). EHR contains highly sensitive data which is critical to protect and, just in the year 2019, 41,232,527 records were deemed stolen. Blockchain can provide several benefits when it comes to EHR, such as increased security, availability, and privacy, however, it needs to be done correctly. Due to blockchain being a rather novel technology, there is room for improvement when it comes to integrating blockchain with EHR. In this thesis a framework for EHR in the healthcare sector is proposed, using Ethereum based smart contracts together with decentralized off-chain storage using InterPlanetary File System (IPFS) and strong symmetric encryption. The framework secures the records and provides a scalable solution. Furthermore, a discussion and evaluation regarding several security aspects that the framework excels on as well as what the framework could improve on.
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Książki na temat "Interplanetary science"

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Daniel, Tony. Metaplanetary: A novel of interplanetary civil war. New York: EOS, 2001.

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V, Papkov Oleg, i Sukhanov Konstantin G, red. Multiple gravity assist interplanetary trajectories. Australia: Gordon and Breach Science Publishers, 1998.

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Daniel, Tony. Superluminal: A novel of interplanetary civil war. New York: Eos, 2005.

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Daniel, Tony. Superluminal: A novel of interplanetary civil war. New York: Eos, 2005.

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Vulpetti, Giovanni. Solar sails: A novel approach to interplanetary travel. New York: Copernicus Books, 2008.

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Battlestar Galactica: The miniseries : a novel. New York: Tor, 2006.

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The voyage. New York: T. Doherty Associates, 1994.

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Hamilton, Peter F. Pandora's star. New York: Del Rey/Ballantine Books, 2004.

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Figueroa, Acton. Cosmic cake. New York: Grosset & Dunlap, 2005.

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1945-, Chapleau Serge, red. Les geants de Blizzard. Montreal: Editions La Courte echelle, 1985.

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Części książek na temat "Interplanetary science"

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Hu, Y. Q. "Interplanetary Physics*". W Space Science in China, 89–115. London: Routledge, 2022. http://dx.doi.org/10.1201/9780203739082-10.

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Watari, Shinichi, Yukio Kozuka i Takashi Watanabe. "Yohkoh Observations and Interplanetary Disturbances". W Astrophysics and Space Science Library, 375–78. Dordrecht: Springer Netherlands, 1998. http://dx.doi.org/10.1007/978-94-011-5220-4_66.

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Bhonsle, R. V., S. K. Alurkar, S. S. Degaonkar, H. O. Vats i A. K. Sharma. "Exploration of Heliosphere by Interplanetary Scintillation". W Astrophysics and Space Science Library, 153–58. Dordrecht: Springer Netherlands, 1986. http://dx.doi.org/10.1007/978-94-009-4612-5_20.

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Aran, Angels, Neus Agueda, Alexandr Afanasiev i Blai Sanahuja. "Charged Particle Transport in the Interplanetary Medium". W Astrophysics and Space Science Library, 63–78. Cham: Springer International Publishing, 2017. http://dx.doi.org/10.1007/978-3-319-60051-2_4.

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Vainio, Rami, Neus Agueda, Angels Aran i David Lario. "Modeling of Solar Energetic Particles in Interplanetary Space". W Astrophysics and Space Science Library, 27–37. Dordrecht: Springer Netherlands, 2007. http://dx.doi.org/10.1007/1-4020-5446-7_4.

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Schwenn, Rainer. "Relationship of Coronal Transients to Interplanetary Shocks: 3D Aspects". W Astrophysics and Space Science Library, 119–21. Dordrecht: Springer Netherlands, 1986. http://dx.doi.org/10.1007/978-94-009-4612-5_15.

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Giese, R. H., i G. Kinateder. "The 3-Dimensional Structure of the Interplanetary Dust Cloud". W Astrophysics and Space Science Library, 441–54. Dordrecht: Springer Netherlands, 1986. http://dx.doi.org/10.1007/978-94-009-4612-5_52.

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Morfill, G. E., E. Grün i C. Leinert. "The Interaction of Solid Particles with the Interplanetary Medium". W Astrophysics and Space Science Library, 455–74. Dordrecht: Springer Netherlands, 1986. http://dx.doi.org/10.1007/978-94-009-4612-5_53.

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Coles, W. A., i B. J. Rickett. "Interplanetary Scintillation Observations of the Solar Wind at High Latitudes". W Astrophysics and Space Science Library, 143–51. Dordrecht: Springer Netherlands, 1986. http://dx.doi.org/10.1007/978-94-009-4612-5_19.

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Watanabe, Takashi, Takakiyo Kakinuma i Masayoshi Kojima. "Three-Dimensional Configurations of Interplanetary Disturbances Associated with Coronal Mass Ejections". W Astrophysics and Space Science Library, 123–28. Dordrecht: Springer Netherlands, 1986. http://dx.doi.org/10.1007/978-94-009-4612-5_16.

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Streszczenia konferencji na temat "Interplanetary science"

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Gong-Liang Zhang. "Interplanetary disturbance structures and geomagnetic storm". W Basic space science. AIP, 1992. http://dx.doi.org/10.1063/1.41724.

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Bhaskaran, Shyam, Joseph E. Riedel i Stephen P. Synnott. "Autonomous optical navigation for interplanetary missions". W SPIE's 1996 International Symposium on Optical Science, Engineering, and Instrumentation, redaktorzy E. Kane Casani i Mark A. Vander Does. SPIE, 1996. http://dx.doi.org/10.1117/12.255151.

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Toquinho Campana, C. "Interplanetary trajectory design in high-fidelity model: Application to deep-space CubeSats’ cruises". W Aerospace Science and Engineering. Materials Research Forum LLC, 2023. http://dx.doi.org/10.21741/9781644902677-27.

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Streszczenie:
Abstract. This paper tackles the problem of first guess trajectory generation for interplanetary missions flying in chaotic environments. Simplified dynamical models are first exploited to perform the preliminary design of deep-space trajectories which leverage orbital perturbations. A real trajectory is then obtained by a refinement procedure in a high-fidelity model. A description of tools and methodologies which will be developed during this PhD research is provided.
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Zubrin, Robert M. "Maximizing the science return of interplanetary missions using nuclear electric power". W Proceedings of the 12th symposium on space nuclear power and propulsion: Conference on alternative power from space; Conference on accelerator-driven transmutation technologies and applications. AIP, 1995. http://dx.doi.org/10.1063/1.47227.

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Hemmati, H., A. Biswas i D. M. Boroson. "30-dB data rate improvement for interplanetary laser communication". W Lasers and Applications in Science and Engineering, redaktor Steve Mecherle. SPIE, 2008. http://dx.doi.org/10.1117/12.767696.

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Krupar, V., O. Santolik, M. Maksimovic, J. Soucek i O. Kruparova. "Interplanetary type II radio bursts and Coronal Mass Ejections". W 2015 1st URSI Atlantic Radio Science Conference (URSI AT-RASC). IEEE, 2015. http://dx.doi.org/10.1109/ursi-at-rasc.2015.7303147.

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Kruparova, O., V. Krupar, J. Safrankova, Z. Nemecek, O. Santolik, M. Maksimovic i J. Soucek. "Turbulent spectra of the solar wind near interplanetary shocks". W 2015 1st URSI Atlantic Radio Science Conference (URSI AT-RASC). IEEE, 2015. http://dx.doi.org/10.1109/ursi-at-rasc.2015.7303148.

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Yan, Yihua, Wei Wang, Linjie Chen, Fei Liu, Lihong Geng i Zhijun Chen. "Future prospects in China for the observations of interplanetary scintillations". W 2019 URSI Asia-Pacific Radio Science Conference (AP-RASC). IEEE, 2019. http://dx.doi.org/10.23919/ursiap-rasc.2019.8738762.

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Afzal, Muhammad Imran, i Abdul Majid. "An aero-capture strategy for human rated interplanetary exploration missions". W 2013 International Conference on Space Science and Communication (IconSpace). IEEE, 2013. http://dx.doi.org/10.1109/iconspace.2013.6599426.

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Haoliang, Sun, Hu Xiaohui i Liu Lixiang. "A Hop-by-Hop Transport Protocol for Interplanetary Backbone Networks". W 2012 International Conference on Computer Science and Service System (CSSS). IEEE, 2012. http://dx.doi.org/10.1109/csss.2012.322.

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