Relevant bibliographies by topics / Cassilis (Vic )

Academic literature on the topic 'Cassilis (Vic )'

Author: Grafiati
Published: 10 December 2022
Last updated: 28 January 2023

Create a spot-on reference in APA, MLA, Chicago, Harvard, and other styles

Select a source type:

Contents

Consult the lists of relevant articles, books, theses, conference reports, and other scholarly sources on the topic 'Cassilis (Vic ).'

Next to every source in the list of references, there is an 'Add to bibliography' button. Press on it, and we will generate automatically the bibliographic reference to the chosen work in the citation style you need: APA, MLA, Harvard, Chicago, Vancouver, etc.

You can also download the full text of the academic publication as pdf and read online its abstract whenever available in the metadata.

Journal articles on the topic "Cassilis (Vic )"

1

Matson, Dennis L., Jean-Pierre Lebreton, and Linda Spilker. "Cassini/Huygens Mission To Saturn: Results And Prospects." Highlights of Astronomy 13 (2005): 904. http://dx.doi.org/10.1017/s1539299600017494.

Full text
Abstract:
The Cassini spacecraft was launched in October, 1997. Since then it has been on an interplanetary trajectory aimed toward Saturn and arriving there on July 1, 2004. En route, Cassini has flown by Venus, the Earth, and Jupiter. Each of these events yielded new scientific results, (e.g., 11 papers in J. Geophys. Res. 106, 30099-30279.) The Cassini flyby of Jupiter, with Galileo already in Jovian orbit, enabled the first-ever simultaneous measurements by two spacecraft at an outer planet. This fortuitous event provided a unique opportunity to investigate the giant planet’s magnetic field and the properties of the Jovian system. It provided a focused period for intensive observations of Jupiter and cooperation with investigators using Galileo, Hubble, Chandra, and ground-based observatories. The results achieved at Jupiter were stunning (e.g., 8 articles in Nature 415, 965-1005, February 28, 2002). Recent results and the current status of the spacecraft and mission will be discussed. Of note are the dates of July 1, 2004 when Cassini goes into orbit about Saturn and January 14, 2005 when Huygens enters the atmosphere of Titan. The Cassini/Huygens mission is a joint undertaking by NASA and ESA, with ASI as a partner via a bilateral agreement with NASA.
APA, Harvard, Vancouver, ISO, and other styles
2

Johnson, Paul, Simon Keay, and Martin Millett. "Lesser urban sites in the Tiber valley: Baccanae, Forum Cassii and Castellum Amerinum." Papers of the British School at Rome 72 (November 2004): 69–99. http://dx.doi.org/10.1017/s0068246200002671.

Full text
Abstract:
ABITATI MINORI NELLA VALLE DEL TEVERE: BACCANAE, FORUM CASSII E CASTELLUM AMERINUML'articolo presenta i risultati delle indagini geofisiche e topografiche condotte a Baccano, Forum Cassii e Castellum Amerinum, come parte del progetto ‘Città romane nella Media e Bassa Valle del Tevere’. I risultati forniscono nuove informazioni sulla struttura e sull'estensione di questi centri, integrando le evidenze raccolte in occasione degli scavi precedenti. A Baccano sono stati individuati nuovi elementi della planimetria del sito. A Forum Cassii è stato chiarito l'andamento della via Cassia in questo punto e sono state individuate nuove strutture, tra cui tombe e un possibile anfiteatro. Infine a Castellum Amerinum sono stati rintracciati il percorso della via Amerina e nuove strutture lungo la riva del Tevere. Si discute inoltre il rinvenimento da quest'ultimo sito di tre tegole con bollo.
APA, Harvard, Vancouver, ISO, and other styles
3

Lebreton, J. P., and D. L. Matson. "The Huygens Mission to Titan: Overview and status." Highlights of Astronomy 13 (2005): 905. http://dx.doi.org/10.1017/s1539299600017500.

Full text
Abstract:
Huygens is an entry probe designed to descend under parachute through the atmosphere of Titan, Saturn’s largest moon. The Huygens Probe is provided by the European Space Agency (ESA) for the Cassini/Huygens mission to Saturn and Titan. The Huygens mission will be conducted on the 3rd Orbit around Saturn. The probe will be released around December 25, 2004 for entry in Titan on January 14, 2005. This paper provided an overview of the Huygens mission. The status of the probe and of the mission was reviewed, and opportunities for Titan observations by the Orbiter during the first two orbits were discussed. The Cassini/Huygens mission is a joint undertaking by NASA and ESA, with ASI as a partner via a bilateral agreement with NASA.
APA, Harvard, Vancouver, ISO, and other styles
4

Vixie, Graham, Jason W. Barnes, Jacob Bow, Stéphane Le Mouélic, Sébastien Rodriguez, Robert H. Brown, Priscilla Cerroni, et al. "Mapping Titan's surface features within the visible spectrum via Cassini VIMS." Planetary and Space Science 60, no. 1 (January 2012): 52–61. http://dx.doi.org/10.1016/j.pss.2011.03.021.

Full text
APA, Harvard, Vancouver, ISO, and other styles
5

Woodson, A. K., H. T. Smith, F. J. Crary, and R. E. Johnson. "Ion composition in Titan's exosphere via the Cassini Plasma Spectrometer I: T40 encounter." Journal of Geophysical Research: Space Physics 120, no. 1 (January 2015): 212–34. http://dx.doi.org/10.1002/2014ja020499.

Full text
APA, Harvard, Vancouver, ISO, and other styles
6

Srama, R., and E. Grün. "The COSMIC DUST ANALYZER for the CASSINI Mission to Saturn." International Astronomical Union Colloquium 150 (1996): 227–31. http://dx.doi.org/10.1017/s0252921100501596.

Full text
Abstract:
AbstractIn October 1997 a unique mission to the Saturnian system will be launched by NASA, the CASSINI mission. One goal of this mission is to study the Saturnian dust environment, and for this task, the COSMIC DUST ANALYZER (CDA) has been developed and is currently being tested. Impact ionization is used to determine the speed (1 - 100 km/s) and the mass (1•10–15 – 1•10–9 g) of impinging particles. Furthermore, the electric charge (1•10–15 – 1•10–12 C) of the particles can be measured via the induction principle, and an integrated time-of-flight mass spectrometer will analyze the chemical composition of individual dust particles. In order to achieve sufficient sensitivity for dust fluxes as low as 10 particles/(month-m2), the sensor has a large sensitive area of 0.1 m2. This paper will describe the function of the experiment.
APA, Harvard, Vancouver, ISO, and other styles
7

Gkioulidou, Matina, M. Opher, M. Kornbleuth, K. Dialynas, J. Giacalone, J. D. Richardson, G. P. Zank, et al. "On the Energization of Pickup Ions Downstream of the Heliospheric Termination Shock by Comparing 0.52–55 keV Observed Energetic Neutral Atom Spectra to Ones Inferred from Proton Hybrid Simulations." Astrophysical Journal Letters 931, no. 2 (May 30, 2022): L21. http://dx.doi.org/10.3847/2041-8213/ac6beb.

Full text
Abstract:
Abstract We present an unprecedented comparison of ∼0.52–55 keV energetic neutral atom (ENA) heliosheath measurements, remotely sensed by the Interstellar Boundary Explorer (IBEX) mission and the Ion and Neutral Camera (INCA) on the Cassini mission, with modeled ENAs inferred from interstellar pickup protons that have been accelerated at the termination shock, using hybrid simulations, to assess the pickup ion energetics within the heliosheath. This is the first study to use hybrid simulations that are able to accurately model the acceleration of ions to tens of keV energies, which is essential in order to model ENA fluxes in the heliosheath, covering the full energy range observed by IBEX and CASSINI/INCA. The observed ENA intensities are an average value over the time period from 2009 to the end of 2012, along the Voyager 2 (V2) trajectory. The hybrid simulations upstream of the termination shock, where V2 crossed, are constrained by observations. We report an energy-dependent discrepancy between observed and simulated ENA fluxes, with the observed ENA fluxes being persistently higher than the simulated ones. Our analysis reveals that the termination shock may not accelerate pickup ions to sufficient energies to account for the observed ENA fluxes. We, thus, suggest that the further acceleration of these pickup ions is most likely occurring within the heliosheath, via additional physical processes like turbulence or magnetic reconnection. However, the redistribution of energy inside the heliosheath remains an open question.
APA, Harvard, Vancouver, ISO, and other styles
8

Willacy, Karen, SiHe Chen, Danica J. Adams, and Yuk L. Yung. "Vertical Distribution of Cyclopropenylidene and Propadiene in the Atmosphere of Titan." Astrophysical Journal 933, no. 2 (July 1, 2022): 230. http://dx.doi.org/10.3847/1538-4357/ac6b9d.

Full text
Abstract:
Abstract Titan’s atmosphere is a natural laboratory for exploring the photochemical synthesis of organic molecules. Significant recent advances in the study of the atmosphere of Titan include: (a) detection of C3 molecules: C3H6, CH2CCH2, c-C3H2, and (b) retrieval of C6H6, which is formed primarily via C3 chemistry, from Cassini Ultraviolet Imaging Spectrograph data. The detection of c-C3H2 is of particular significance as ring molecules are of great astrobiological importance. Using the Caltech/JPL KINETICS code, along with the best available photochemical rate coefficients and parameterized vertical transport, we are able to account for the recent observations. It is significant that ion chemistry, reminiscent of that in the interstellar medium, plays a major role in the production of c-C3H2 above 1000 km.
APA, Harvard, Vancouver, ISO, and other styles
9

.., Hasan G�, Selçuk Topal, and Florentin Smarandache. "Neutrosophic Number Sequences: An introductory Study." International Journal of Neutrosophic Science 20, no. 1 (2023): 27–48. http://dx.doi.org/10.54216/ijns.200103.

Full text
Abstract:
In this paper, Neutrosophic definitions and properties of some special number sequences which are frequently found in the science literature, called Neutrosophic Number Sequences (NNSq) via Horadam sequence are studied for the first time. Especially for Neutrosophic Fibonacci (NFNq) and Neutrosophic Lucas (NLNq) number sequences, fundamental properties and identities such as Ruggles, Honsberger, Cassini, Catalan, d’Ocagne, and Tagiuri are given. In addition, Neutrosophic definitions of the sequences of Pell (NPNq), Pell-Lucas (NPLNq), Jacobsthal (NJNq), Jacobsthal-Lucas (NJLNq), Mersenne (NMNq), Mersenne-Lucas (NMLNq), Balancing (NBNq), and Lucas-Balancing (NLBNq) numbers are introduced. Besides defining these numbers and their sequences, since fuzzy and intuitionistic fuzzy sets are restrictions of neutrosophic sets, sequences of numbers within these sets are naturally and indirectly revealed.
APA, Harvard, Vancouver, ISO, and other styles
10

AlDabbas, Ashraf, and Zoltan Gal. "Cassini-Huygens mission images classification framework by deep learning advanced approach." International Journal of Electrical and Computer Engineering (IJECE) 11, no. 3 (June 1, 2021): 2457. http://dx.doi.org/10.11591/ijece.v11i3.pp2457-2466.

Full text
Abstract:
Developing a deep learning (DL) model for image classification commonly demands a crucial architecture organization. Planetary expeditions produce a massive quantity of data and images. However, manually analyzing and classifying flight missions image databases with hundreds of thousands of images is ungainly and yield weak accuracy. In this paper, we speculate an essential topic related to the classification of remotely sensed images, in which the process of feature coding and extraction are decisive procedures. Diverse feature extraction techniques are intended to stimulate a discriminative image classifier. Features extraction is the primary engagement in raw data processing with the purpose of data classification; when it comes across the task of analysis of vast and varied data, these kinds of tasks are considered as time-consuming and hard to be treated with. Most of these classifiers are either, in principle, quite intricate or virtually unattainable to calculate for massive datasets. Stimulated by this perception, we put forward a straightforward, efficient classifier based on feature extraction by analyzing the cell of tensors via layered MapReduce framework beside meta-learning LSTM followed by a SoftMax classifier. Experiment results show that the provided model attains a classification accuracy of 96.7%, which makes the provided model quite valid for diverse image databases with varying sizes.
APA, Harvard, Vancouver, ISO, and other styles
More sources

Books on the topic "Cassilis (Vic )"

1

Lombardo, Robert M. The Gem of the Prairie. University of Illinois Press, 2017. http://dx.doi.org/10.5406/illinois/9780252037306.003.0003.

Full text
Abstract:
This chapter traces the history of vice and crime in Chicago from the Civil War until the beginning of Prohibition, paying special attention to the rise of machine politics under Michael Cassius McDonald, organizer of Chicago's first crime syndicate. It argues that organized crime in Chicago was not imported from the south of Italy but began because Chicago machine politicians provided political protection to vice syndicates and criminal gangs in exchange for votes and campaign contributions. The chapter reviews the history of one vice district that played a significant role in the development of organized crime in Chicago, the Levee, beginning with the original Custom House Levee and its eventual movement to the “New” Levee in the city's Near South Side. It also discusses the roles played by municipal aldermen John Coughlin and Michael Kenna as protectors of vice and crime in Chicago's First Ward. Finally, it analyzes the history of the public outcry against segregated vice and the eventual closure of the Levee vice district.
APA, Harvard, Vancouver, ISO, and other styles
2

Devic, J. F. S. Histoire de la Vie et des Travaux Scientifiques et Littéraires de J. D. Cassini Iv, Ancien Directeur de L'Observatoire. Creative Media Partners, LLC, 2018.

Find full text
APA, Harvard, Vancouver, ISO, and other styles

Book chapters on the topic "Cassilis (Vic )"

1

Coltelloni-Trannoy, Michèle. "La géographie dans l’Histoire romaine de Cassius Dion." In Histoire et géographie chez les auteurs grecs du IIe siècle avant J.-C. au VIe siècle après J.-C., 165–84. Editions de Boccard, 2019. http://dx.doi.org/10.2307/j.ctv2c3k2m7.12.

Full text
APA, Harvard, Vancouver, ISO, and other styles
2

Fant, Clyde E., and Mitchell G. Reddish. "Philippi." In A Guide to Biblical Sites in Greece and Turkey. Oxford University Press, 2003. http://dx.doi.org/10.1093/oso/9780195139174.003.0020.

Full text
Abstract:
An important city in the Roman and early Christian period, Philippi exists today only as an archaeological site. The impressive remains of this once flourishing city on the Via Egnatia, the important Roman highway in the area, are frequently visited by modern pilgrims retracing the steps of the Apostle Paul, who started a Christian church in the city. The ruins of ancient Philippi are easy to find. The archaeological site is located in the region of Macedonia, alongside highway 12 between Kavala and Drama, next to the village of Krenides. Settlement in the area occurred as early as the Middle Neolithic period (ca. 5000 B.C.E.). In 360 B.C.E., Greek colonists from the island of Thasos, led by the exiled Athenian politician Kallistratos, founded the colony of Krenides on the site of what later became Philippi. The colony at Krenides (which means “spring,” because of the abundant streams in the area) provided the Thasians with access to the rich resources of the area, particularly its silver and gold mines. Threatened by the Thracian tribes in the area, the colonists at Krenides asked Philip II of Macedonia for military assistance in 356 B.C.E. Eager to gain control of the area, and particularly its rich resources, Philip conquered the city and renamed it Philippi in his honor. Philip fortified the city with new walls, increased the city’s population with Macedonian mercenaries, and extracted large amounts of gold and silver from the mines in the area. Although little is known of the city during the Hellenistic period, this was apparently a prosperous time for Philippi. In the 2nd century B.C.E., the Romans occupied Macedonia and turned the area into a Roman province. During the Roman period, the most i important event associated with Philippi took place. In 42 B.C.E. the forces of Octavian (later known as Augustus) and Mark Antony defeated the armies of Brutus and Cassius (the murderers of Julius Caesar) on the plains just outside the west wall of Philippi. This battle brought to an end the Roman Republic.
APA, Harvard, Vancouver, ISO, and other styles

Conference papers on the topic "Cassilis (Vic )"

1

Hospodarsky, G. B. "Observations of Chorus at Saturn by Cassini (abstract)." In Planetary Radio Emissions VII. Vienna: Austrian Academy of Sciences Press, 2011. http://dx.doi.org/10.1553/pre7s127.

Full text
APA, Harvard, Vancouver, ISO, and other styles
2

Ye, S. Y. "An Overview of Saturn Narrowband Radio Emissions Observed by Cassini RPWS (invited)." In Planetary Radio Emissions VII. Vienna: Austrian Academy of Sciences Press, 2011. http://dx.doi.org/10.1553/pre7s99.

Full text
APA, Harvard, Vancouver, ISO, and other styles
3

Imai, M. "Jupiter’s Decametric and Hectometric Radio Emissions Observed by Cassini RPWS and Voyager PRA." In Planetary Radio Emissions VII. Vienna: Austrian Academy of Sciences Press, 2011. http://dx.doi.org/10.1553/pre7s167.

Full text
APA, Harvard, Vancouver, ISO, and other styles
4

Lamy, L. "AKR Diurnal, Semi-Diurnal and Shorter Term Modulations Disentangled by Cassini/RPWS Observations (abstract)." In Planetary Radio Emissions VII. Vienna: Austrian Academy of Sciences Press, 2011. http://dx.doi.org/10.1553/pre7s283.

Full text
APA, Harvard, Vancouver, ISO, and other styles
5

Moncuquet, M. "Density and Temperature of the Electron Core in the Inner Magnetosphere of Saturn from Cassini/RPWS Antennas (abstract)." In Planetary Radio Emissions VII. Vienna: Austrian Academy of Sciences Press, 2011. http://dx.doi.org/10.1553/pre7s133.

Full text
APA, Harvard, Vancouver, ISO, and other styles
6

Zuegner, Mario Andre. "Ice moon research – A phenomenon called plume." In Symposium on Space Educational Activities (SSAE). Universitat Politècnica de Catalunya, 2022. http://dx.doi.org/10.5821/conference-9788419184405.102.

Full text
Abstract:
Based on the observations of the Cassini-Huygens space exploration mission, Saturn's moon Enceladus was found to be a very promising subject in the solar system for further exploration and follow-up research, especially focusing on the potential of extraterrestrial life and its origin. Near its South Pole, fountains, specified plumes, consisting mostly of water vapor and small salt-rich ice grains with intermittent activity were observed at the surface. With supersonic speed the water vapor is exiting the trenches known as Tiger Stripes. The driving force of these plumes are not completely understood yet. In current models, Enceladus is expected to consist of a rocky core, surrounded by an ocean of liquid water and covered by a layer of ice. The observed phenomenon is assumed to be caused by the tidal forces that act upon Enceladus. However, several models try to describe the underlying physical processes. Various investigations have recognized the astrobiological potential of Enceladus, even proposed a concept for a sample return for further research in relation to the subsurface ocean. Cassini ́s existing analysis already identified CH4, CO, CO2, simple and complex organics at an altitude of approximately 190 km which allow the assumption of supersonic speeds. That said, the goal of our experiment is to gain further indices/evidence to support the current models of the plumes. Our experiment takes place on a sounding rocket which gives access to a stable vacuum and microgravity in addition. The achieved altitude with its physical environment provides almost the conditions at Enceladus related to the gravitation. The rocket module contains a pressurized and heated water reservoir which is connected via an injection system with the evaporation chamber. On the top a convergent-divergent nozzle is welded. Furthermore a nozzle cover system and a locking mechanism are integrated. At apogee, the nozzle shall be opened and the fluid stream (assumingly made up of ice, water droplets and vapor) shall exit the module at about Mach 2. The necessary fluid-dynamic data is gathered by multiple temperature and pressure measurements at different points on the module. So, the vapor stream shall be compared to the expectations based on the models. Finally it is to mention that our project is still running and waiting for its launch. Caused through the Corona crisis and the Ukraine war the launch cycle was canceled two years in succession. With much luck the rocket will launch in March 2023.
APA, Harvard, Vancouver, ISO, and other styles
You might also be interested in the extended bibliographies on the topic 'Cassilis (Vic )' for particular source types:
Journal articles
We offer discounts on all premium plans for authors whose works are included in thematic literature selections. Contact us to get a unique promo code!

To the bibliography