116,713 research outputs found

    Bibliographie Leo Perutz : Stand: 26. April 2010

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    In den gut eineinhalb Jahrzehnten, die seit der Bibliographie von Hans-Harald Müller und Wilhelm Schernus (Nr. 140) vergangen sind, hat sich die Perutz-Forschung etabliert. Dies zeigt schon ein flüchtiger quantitativer Vergleich. Der Abschnitt "Wissenschaftliche Untersuchungen" bestand damals aus einer Handvoll Magisterarbeiten und Dissertationen; in der vorliegenden Bibliographie nimmt die Sekundärliteratur mehr als die Hälfte des Raums ein. Die Rechtfertigung einer neuen Perutz-Bibliographie liegt denn auch vor allem darin, ein aktuelles, möglichst vollständiges Verzeichnis der wissenschaftlichen Literatur zu Leo Perutz (unter Einschluß der vor 1990 erschienenen Titel) vorzulegen. Der Abschnitt "Primärliteratur" schließt dagegen chronologisch an Müller und Schernus an

    Joshua Davis: Author of Spare Parts

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    Citation: K-State First (2016). Joshua Davis: Author of Spare Parts [Flier]. Manhattan, Kansas: K-State First.Flyer advertising Joshua Davis's author talk at Kansas State University

    Počemu i kak my približaemsja k anarchii?

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    D-r Leo

    Steven Johnson Author Talk Poster

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    K-State Book NetworkA poster advertising an author talk by Steven Johnson at Kansas State University on September 3, 2014. Steven Johnson's book "The Ghost Map" was the 2014-2015 common book

    No.241, Leo T. Samuels, interviews by Clarence Stover and Hans K. Jacobs

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    Transcript (67 pages) of interviews by Clarence Stover on December 15, 1969, and Hans K. Jacobs on December 18 and 22, 1970, with Dr. Leo Tolstoy Samuels, professor emeritus of biochemistry at the University of Utah medical school. This interview is no. 241 in the Everett L. Cooley Oral History Project, and tape no. U-1239. Accompanied by Samuels\u27 curriculum vitae and an obituary from 1978Samuels (b. 1894) discusses his early life and education; the establishment of the four-year College of Medicine, University of Utah; his work and research in biochemistry and endocrinology and his career at the University, 1940s-1970s. Interviewers: Hans K. Jacobs, Clarence Stove

    Gravity gradient effect on a LEO satellite with an elliptic orbit and unsymmetrical mass properties

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    Corresponding Author: Mechanical Engineering Department, College of Engineering, King Saud University, P.O. Box 800 Riyadh-11421, Saudi Arabia Telehone: +966-1-4676659 Email: [email protected] study presented in this paper investigates the dynamic behavior of a low earth orbit (LEO) satellite due to gravity gradient disturbances when the product of inertia terms of the spacecraft and the orbit eccentricity are considered. It is shown that the classical stable solution for the gravity gradient disturbance becomes unstable if at least one product of inertia term exceeds a critical value. Dimensional analysis technique is used to develop the significant dimensionless groups which were used to correlate the data generated from the response of the coupled roll, pitch and yaw dynamics. Based on the findings of these groups, stability maps are developed to predict the influence of the product of inertia terms on the long-term behavior of the spacecraft attitude dynamics. The developed stability maps are verified numerically and successful prediction of a spacecraft stability condition due to gravity gradient disturbance is achieved

    Orbit Precision Analysis of Small Man-Made Space Objects in LEO Based on Radar Tracking Measurements

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    The German Space Operations Center (GSOC) performs collision avoidance for 11 LEO and 2 GEO satellites. Risk detection and maneuver decisions strongly depend on the computed probability of collision that is driven by the anticipated orbit precision of chaser and target. While the orbits of operational satellite are well known this is usually not the case for space debris. Therefore, an improved collision assessment requires refined orbit determination of the chaser object. This paper describes the achievable orbit precision for a small object based on radar measurements. The Tracking and Imaging Radar (TIRA) of Fraunhofer FHR in Wachtberg, Germany, was used to track the Canadian nanosatellite CanX-2 over a period of five days. CanX-2 is a triple CubeSat of the size 10x10x34 cm carrying a dual frequency GPS receiver. A reference trajectory is established by precise orbit determination (POD) from GPS measurements. Radar tracking measurements and derived orbital information are evaluated by comparison against the reference orbit. Statistics of the orbit determination and orbit prediction precision using different radar measurement data arc lengths is presented leading to a better understanding of the prediction uncertainty of critical close approaches between an active satellite and a small object

    You are just the girl that I could kiss [first line of chorus]

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    strophic with choruspiano and voiceads on back cover for Chas. K. Harris stock2035-4Johns Hopkins University, Levy Sheet Music Collection, Box 154a, Item 093Lyric by Blanche Merrill. Music by Leo Edwards.[Clark & Bergman]; Jesse L. Lasky's Most Pretentious Production The Trained Nurses With Clark & Bergman.unattrib. photo of Clark & Bergman, of Lasky, and of unidentified women on stag

    You are just the girl that I could kiss [first line of chorus]

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    strophic with choruspiano and voiceads on back cover for Chas. K. Harris stock2035-4Johns Hopkins University, Levy Sheet Music Collection, Box 154a, Item 093Lyric by Blanche Merrill. Music by Leo Edwards.[Clark & Bergman]; Jesse L. Lasky's Most Pretentious Production The Trained Nurses With Clark & Bergman.unattrib. photo of Clark & Bergman, of Lasky, and of unidentified women on stag

    Discovery and Characterization of Two Ultra Faint-Dwarfs Outside the Halo of the Milky Way: Leo M and Leo K

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    We report the discovery of two ultra-faint dwarf galaxies, Leo M and Leo K, that lie outside the halo of the Milky Way. Using Hubble Space Telescope imaging of the resolved stars, we create color-magnitude diagrams reaching the old main sequence turn-off of each system and (i) fit for structural parameters of the galaxies; (ii) measure their distances using the luminosity of the Horizontal Branch stars; (iii) estimate integrated magnitudes and stellar masses; and (iv) reconstruct the star formation histories. Based on their location in the Local Group, neither galaxy is currently a satellite of the Milky Way, although Leo K is located ~26 kpc from the low-mass galaxy Leo T and these two systems may have had a past interaction. Leo M and Leo K have stellar masses of 1.8 (+0.3/-0.2) x 10^4 Msun and 1.2+/-0.2 x 10^4 Msun, and were quenched 10.6 (+2.2/-1.1) Gyr and 12.8 (+0.1/-4.2) Gyr ago, respectively. Given that the galaxies are not satellites of the MW, it is unlikely that they were quenched by environmental processing. Instead, given their low stellar masses, their early quenching timescales are consistent with the scenario that a combination of reionization and stellar feedback shut-down star formation at early cosmic times.Comment: 12 pages, 9 figures, 1 tabl
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