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Cristian Bota 3Socf5x9eyz6
Cristian Bota https://www.facebook.com/index.php?lh=Ac- _3sOcf5X9eyz6 Das Imperium Talent Agency Berlin (D.I.T.A.) Georg Georgi Phone: +49 151 6195 7519 Email: [email protected] Website: www.dasimperium.com © b Information Acting age 25 - 35 years Nationality Romanian Year of birth 1992 (29 years) Languages English: fluent Height (cm) 180 Romanian: native-language Weight (in kg) 68 French: medium Eye color green Dialects Resita dialect: only when Hair color Brown required Hair length Medium English: only when required Stature athletic-muscular Accents Romanian: only when required Place of residence Bucharest Instruments Piano: professional Cities I could work in Europe, Asia, America Sport Acrobatics, Aerial yoga, Aerobics, Aikido, Alpine skiing, American football, Archery, Artistic cycling, Artistic gymnastics, Athletics, Backpacking, Badminton, Ballet, Baseball, Basketball, Beach volleyball, Biathlon, Billiards, BMX, Body building, Bodyboarding, Bouldering, Bowling, Boxing, Bujinkan, Bungee, Bycicle racing, Canoe/Kayak, Capoeira, Caster board, Cheerleading, Chinese martial arts, Climb, Cricket, Cross-country skiing, Crossbow shooting, CrossFit, Curling, Dancesport, Darts, Decathlon, Discus throw, Diving, Diving (apnea), Diving (bottle), Dressage, Eskrima/Kali, Fencing (sports), Fencing (stage), Figure skating, Finswimming, Fishing, Fistball, Fitness, Floor Exercise, Fly fishing, Free Climbing, Frisbee, Gliding, Golf, Gymnastics, Gymnastics, Hammer throw, Handball, Hang- Vita Cristian Bota by www.castupload.com — As of: 2021-05-10 -
Using Kepler Systems to Constrain the Frequency and Severity of Dynamical Effects on Habitable Planets Alexander James Mustill Melvyn B
Using Kepler systems to constrain the frequency and severity of dynamical effects on habitable planets Alexander James Mustill Melvyn B. Davies Anders Johansen Dynamical instability bad for habitability • Excitation of eccentricity can shift HZ or cause extreme seasons (Spiegel+10, Dressing+10) • Planets may be scattered out of HZ • Planet-planet collisions may remove biospheres, atmospheres, water • Earth-like planets may be eaten by Neptunes/Jupiters Strong dynamical effects: scattering and Kozai • Scattering: closely-spaced giant planets excite each others’ eccentricities (Chatterjee+08) • Kozai: inclined external perturber (e.g. binary) can cause very large eccentricity fluctuations (Kozai 62, Lidov 62, Naoz 16) Relevance of inner systems to HZ • If you can • form a hot Jupiter through high-eccentricity migration • damage a Kepler system at few tenths of an au • you will damage the habitable zone too Relevance of inner systems intrinsically • Large number of single-candidate systems found by Kepler relative to multiples • Is this left over from formation? Or do the multiples evolve into singles through dynamics? (Johansen+12) • Informs models of planet formation • all the Kepler systems are interestingly different to the Solar system, but do we have two interestingly different channels of planet formation or only one? What do we know about the prevalence of strong dynamical effects? • So far know little about planets in HZ • What we do know: • Violent dynamical history strong contender for hot Jupiter migration • Many giants have high -
Dynamics of the Terrestrial Planets from a Large Number of N-Body Simulations ∗ Rebecca A
Earth and Planetary Science Letters 392 (2014) 28–38 Contents lists available at ScienceDirect Earth and Planetary Science Letters www.elsevier.com/locate/epsl Dynamics of the terrestrial planets from a large number of N-body simulations ∗ Rebecca A. Fischer , Fred J. Ciesla Department of the Geophysical Sciences, University of Chicago, 5734 S Ellis Ave, Chicago, IL 60637, USA article info abstract Article history: The agglomeration of planetary embryos and planetesimals was the final stage of terrestrial planet Received 6 September 2013 formation. This process is modeled using N-body accretion simulations, whose outcomes are tested by Received in revised form 26 January 2014 comparing to observed physical and chemical Solar System properties. The outcomes of these simulations Accepted 3 February 2014 are stochastic, leading to a wide range of results, which makes it difficult at times to identify the full Availableonline25February2014 range of possible outcomes for a given dynamic environment. We ran fifty high-resolution simulations Editor: T. Elliott each with Jupiter and Saturn on circular or eccentric orbits, whereas most previous studies ran an Keywords: order of magnitude fewer. This allows us to better quantify the probabilities of matching various accretion observables, including low probability events such as Mars formation, and to search for correlations N-body simulations between properties. We produce many good Earth analogues, which provide information about the mass terrestrial planets evolution and provenance of the building blocks of the Earth. Most observables are weakly correlated Mars or uncorrelated, implying that individual evolutionary stages may reflect how the system evolved even late veneer if models do not reproduce all of the Solar System’s properties at the end. -
How Doc Draper Became the Father of Inertial Guidance
(Preprint) AAS 18-121 HOW DOC DRAPER BECAME THE FATHER OF INERTIAL GUIDANCE Philip D. Hattis* With Missouri roots, a Stanford Psychology degree, and a variety of MIT de- grees, Charles Stark “Doc” Draper formulated the basis for reliable and accurate gyro-based sensing technology that enabled the first and many subsequent iner- tial navigation systems. Working with colleagues and students, he created an Instrumentation Laboratory that developed bombsights that changed the balance of World War II in the Pacific. His engineering teams then went on to develop ever smaller and more accurate inertial navigation for aircraft, submarines, stra- tegic missiles, and spaceflight. The resulting inertial navigation systems enable national security, took humans to the Moon, and continue to find new applica- tions. This paper discusses the history of Draper’s path to becoming known as the “Father of Inertial Guidance.” FROM DRAPER’S MISSOURI ROOTS TO MIT ENGINEERING Charles Stark Draper was born in 1901 in Windsor Missouri. His father was a dentist and his mother (nee Stark) was a school teacher. The Stark family developed the Stark apple that was popular in the Midwest and raised the family to prominence1 including a cousin, Lloyd Stark, who became governor of Missouri in 1937. Draper was known to his family and friends as Stark (Figure 1), and later in life was known by colleagues as Doc. During his teenage years, Draper enjoyed tinkering with automobiles. He also worked as an electric linesman (Figure 2), and at age 15 began a liberal arts education at the University of Mis- souri in Rolla. -
Collectspace List of Items Stolen from Kansas Cosmosphere
CollectSpace list of items stolen from Kansas Cosmosphere What follows is a list of artifacts that were identified as missing from the Kansas Cosmosphere in a December 2003 search warrant. It is presented here as transcribed from a copy of the warrant. Due to the condition of the document, it is possible that errors were introduced as it was transcribed. Item Description Part Number Serial Number Main Hatch Latch V36-553010-21 Main Hatch Latch V36-553010-32 Main Hatch Swing Assembly V36-591122 Main Hatch Pressure Dump Assembly V36-591062-3 306908 Main Hatch Pressure Dump Assembly V36-59106162-3 306908 3 each Urine Hoses A10694-1 4 each Communication Control Unit Adapters V36-715103-11 3 each Flown Apollo 9 16MM Camera Mounts V36-752028 Machined Parts (Unknown, Possibly Main Hatch) 2 each [indiscernible] Filters 14116-501 1.02661E+11 Fecal Management Subsystem CL-501000 001-F Urine Collection/Sampling System 24-0105 Collins' In-Flight Coveralls Boot Assembly 8N-1062-801 113 Apollo Helmet Neck Ring A6L-101038-12 1146 Conrad Glove Molds T1594-01/02 A205 5 each Food Samples N-P-73 FDAI Flight Director Altitude Indicator FDAI Flight Director Altitude Indicator AGC DSKY Assembly 200395071 RAY20 Flown Apollo 14 Ring Set V36-000002-141 VCA4948 Knife EC-30045 Communication Control Unit V36-7130031 06352AAG4729 Defecation Collection Device V36-JS501-397 2302 Main Hatch Cylinder V36-000002-901 1.0106E+11 Strap Assembly V36-000002-131 109 Sensors MSC BM 01 001, 005, 007 Bio-Belt Assembly SEC13100148-301 1068 Flown Apollo 7 Communication Control Unit -
2013 Annual Report
2012-13 Annual Accountability Report FLORIDA INTERNATIONAL UNIVERSITY STATE UNIVERSITY SYSTEM of FLORIDA Board of Governors Annual Accountability Report FLORIDA INTERNATIONAL UNIVERSITY 2012-2013 TABLE OF CONTENTS EXECUTIVE SUMMARY DASHBOARD p. 2 KEY ACHIEVEMENTS p. 5 NARRATIVE p. 6 DATA TABLES SECTION 1. FINANCIAL RESOURCES p. 16 SECTION 2. PERSONNEL p. 20 SECTION 3. ENROLLMENT p. 21 SECTION 4. UNDERGRADUATE EDUCATION p. 23 SECTION 5. GRADUATE EDUCATION p. 32 SECTION 6. RESEARCH & ECONOMIC DEVELOPMENT p. 35 1 Annual Accountability Report FLORIDA INTERNATIONAL UNIVERSITY 2012-2013 Dashboard Headcount Fall % 2007-2012 Degree Programs Offered 2012 Carnegie Classifications Enrollments 2012 Total % Change TOTAL 50,394 100% 31% TOTAL (as of Spring 2013) 178 Research Universities Basic: White 6,259 12% -5% Baccalaureate 63 (high research activity) Hispanic 31,037 62% 36% Master’s 81 Undergraduate Professions plus arts & Black 6,639 13% 37% Research& Specialist’s Doctorate 30 Instructional Program: sciences, high graduate Doctorate Other 6,459 13% 50% Professional Doctorate 4 Graduate Comprehensive doctoral Full-Time 30,094 60% 31% Faculty Full- Part- Instructional Program: (no medical/veterinary) Part-Time 20,300 40% 30% (Fall 2012) Time Time Large four-year, primarily Size and Setting: Undergraduate 36,217 72% 22% TOTAL 1,116 34 nonresidential Graduate 8,414 17% 35% Tenure & Ten. Track 687 6 Community Curricular Engagement and T. Track Unclassified 5,763 11% 114% Non-Tenured Faculty 429 28 Engagement: Outreach and Partnerships DEGREE PRODUCTIVITY -
Aquarius Fact Sheet
Fact Sheet: 2019 Designer: Perry Submarine Builders (Florida) Construction: Victoria Machine Works (Texas); start: 1986 | complete: 1987 Estimated construction cost: $5.5M Operational Timeline: St. Croix Deployment: Deployment in Salt River Canyon, St. Croix: 1987 Owner: NOAA Operator: Farleigh Dickenson University Interim Period: Recovered: 1990 by the University of North Carolina Wilmington Refurbished: 1990-1993 at North Carolina State Ports, Wilmington, NC Owner: NOAA Operator: University of North Carolina Wilmington Florida Keys Deployment: Initial deployment on Conch Reef, Florida Keys: 1993 (baseplate deployed 1992) Recovered for refurbishment: 1996-1998 - Harbor Branch Oceanographic Institution, Ft. Pierce, FL Redeployment on Conch Reef, Florida Keys: 1998 – present Owner: NOAA: 1986-2014; Florida International University: 2014 – present Operator: FDU: 1987-1989; UNCW: 1990-2012; Florida International University: 2013 - present Aquarius Siting: Conch Reef, Florida Keys (Florida Keys National Marine Sanctuary): Distance From Islamorada shore base: 15.4 km (8.5 nm) Distance offshore: 9 km (5.4 nm) Hatch depth/storage depth: 14 m (46 fsw) 35 psi Depth of bottom directly below Aquarius: 18 m (60 fsw) (updated: 09.15.19) Habitat Specifications: Aquarius weight: 82-ton double-lock pressure vessel Baseplate weight: 120 tons Dimensions: 14-meters long by 3-meters in diameter (46 ft x 10 ft) Crew: 4 scientists and 2 technicians Amenities: kitchen facilities that include a microwave, instant hot water dispenser, refrigerator, sink, dining -
New Romanian Cinema
NOVEMBer 29–DECEMBer 3, 2013 Romanian Film Initiative NEW ROMANIAN CINEMA EMA N I C MAKING WAVES: New Romanian Cinema is MAKING WAVES 2013 is made possible with the N IA N co-presented by the Film Society of Lincoln Center leading support of the Trust for Mutual Understand- and the Romanian Film Initiative, in partnership ing, Alexandre Almăjeanu and Gentica Foundation, OMA R with the Jacob Burns Film Center and Transilvania Adrian Porumboiu, HBO Romania, Adrian Giurgea, International Film Festival. Colgate University & Christian A. Johnson Founda- S: NEW Launched in 2006 at the initiative of Corina tion, Blue Heron Foundation, Mica Ertegun, Marie WAVE Șuteu, MAKING WAVES has become a fixture in France Ionesco, Lucian Pintilie, Dr. Daiana Voiculescu NG New York City’s cultural scene. The festival offers and Renzo Cianfanelli, and other generous sponsors I K every year the best selection of contemporary and donors, including visual artists Șerban Savu, Dan MA Romanian filmmaking, and introduces American Perjovschi, Adrian Ghenie, and Mircea Cantor. audiences to films and filmmakers who laid the Special support from ICON Production, Lark ground for the new Romanian cinema. Play Development Center, Șapte Seri, Dilema For the second consecutive year, MAKING veche, Radio Guerilla, and filmmaker Mona WAVES is now a fully independent festival of Nicoară, joined by more than 250 supporters. Romanian contemporary cinema and culture, made The “Creative Freedom through Cinema” spe- possible solely through the support of private funders cial program is presented in partnership with the and individual donations, including a large number of Romanian National Film Center, Czech Center New Romanian artists who believe that audiences at home York and the Slovak Film Institute. -
INVESTIGATING ACTIVE GALACTIC NUCLEI with LOW FREQUENCY RADIO OBSERVATIONS By
INVESTIGATING ACTIVE GALACTIC NUCLEI WITH LOW FREQUENCY RADIO OBSERVATIONS by MATTHEW LAZELL A thesis submitted to The University of Birmingham for the degree of DOCTOR OF PHILOSOPHY School of Physics & Astronomy College of Engineering and Physical Sciences The University of Birmingham March 2015 University of Birmingham Research Archive e-theses repository This unpublished thesis/dissertation is copyright of the author and/or third parties. The intellectual property rights of the author or third parties in respect of this work are as defined by The Copyright Designs and Patents Act 1988 or as modified by any successor legislation. Any use made of information contained in this thesis/dissertation must be in accordance with that legislation and must be properly acknowledged. Further distribution or reproduction in any format is prohibited without the permission of the copyright holder. Abstract Low frequency radio astronomy allows us to look at some of the fainter and older synchrotron emission from the relativistic plasma associated with active galactic nuclei in galaxies and clusters. In this thesis, we use the Giant Metrewave Radio Telescope to explore the impact that active galactic nuclei have on their surroundings. We present deep, high quality, 150–610 MHz radio observations for a sample of fifteen predominantly cool-core galaxy clusters. We in- vestigate a selection of these in detail, uncovering interesting radio features and using our multi-frequency data to derive various radio properties. For well-known clusters such as MS0735, our low noise images enable us to see in improved detail the radio lobes working against the intracluster medium, whilst deriving the energies and timescales of this event. -
Go for Lunar Landing Conference Report
CONFERENCE REPORT Sponsored by: REPORT OF THE GO FOR LUNAR LANDING: FROM TERMINAL DESCENT TO TOUCHDOWN CONFERENCE March 4-5, 2008 Fiesta Inn, Tempe, AZ Sponsors: Arizona State University Lunar and Planetary Institute University of Arizona Report Editors: William Gregory Wayne Ottinger Mark Robinson Harrison Schmitt Samuel J. Lawrence, Executive Editor Organizing Committee: William Gregory, Co-Chair, Honeywell International Wayne Ottinger, Co-Chair, NASA and Bell Aerosystems, retired Roberto Fufaro, University of Arizona Kip Hodges, Arizona State University Samuel J. Lawrence, Arizona State University Wendell Mendell, NASA Lyndon B. Johnson Space Center Clive Neal, University of Notre Dame Charles Oman, Massachusetts Institute of Technology James Rice, Arizona State University Mark Robinson, Arizona State University Cindy Ryan, Arizona State University Harrison H. Schmitt, NASA, retired Rick Shangraw, Arizona State University Camelia Skiba, Arizona State University Nicolé A. Staab, Arizona State University i Table of Contents EXECUTIVE SUMMARY..................................................................................................1 INTRODUCTION...............................................................................................................2 Notes...............................................................................................................................3 THE APOLLO EXPERIENCE............................................................................................4 Panelists...........................................................................................................................4 -
Orthoptera: Tristiridae), En La Zona Costera Sur De La Región De Antofagasta
Boletín del Museo Nacional de Historia Natural, Chile, 57: 133-138 (2008) REGISTRO EN ALTURA DE ENODISOMACRIS CURTIPENNIS CIGLIANO, 1989 (ORTHOPTERA: TRISTIRIDAE), EN LA ZONA COSTERA SUR DE LA REGIÓN DE ANTOFAGASTA MARIO ELGUETA¹ y CONSTANZA BARRÍA² ¹ Entomología, Museo Nacional de Historia Natural, Casilla 787, Santiago, Chile; [email protected] ² Instituto de Geografía, Universidad Católica de Chile, Av. Vicuña Mackenna 4860, Santiago, Chile. [email protected] RESUMEN Se documenta el hallazgo de ejemplares de Enodisomacris curtipennis Cigliano, 1989 (Tristiridae: Elasmoderini) a una altitud de 2.700 m en el Cerro Armazones en 24º34’53”S; 70º11’56”O (Datum PSAD 56) equivalente a 378.600 E y 7.280.850 S (UTM); este constituye un nuevo registro altitudinal y a la vez es la máxima altura reportada para esta especie. El Cerro Armazones forma parte de la sierra Vicuña Mackenna y se ubica al NE de la localidad costera de Paposo, a 37 km hacia el interior, en la zona sur de la Provincia de Antofagasta. Se entregan además algunos antecedentes del ambiente en que se encuentra este ortóptero. ————— Palabras clave: Tristiridae, Enodisomacris curtipennis, distribución geográfica. ABSTRACT A high altitude record for Enodisomacris curtipennis Cigliano, 1989 (Orthoptera: Tristiridae), in the Southern coastal area of Antofagasta Region. The grasshopper Enodisomacris curtipennis Cigliano, 1989 is reported for the first time at 2,700 meters of altitude in the Cerro Armazones, 24º34’53” S; 70º11’56” W (Datum PSAD 56) or 378.600 E; 7.280.850 S (UTM). This is the highest altitudinal record for this species. The hill belongs to the Vicuña Mackenna range and is located at NE of Paposo locality, in the Southern coastal area of Antofagasta Province of Chile. -
50 Years of Existence of the European Southern Observatory (ESO) 30 Years of Swiss Membership with the ESO
Federal Department for Economic Affairs, Education and Research EAER State Secretariat for Education, Research and Innovation SERI 50 years of existence of the European Southern Observatory (ESO) 30 years of Swiss membership with the ESO The European Southern Observatory (ESO) was founded in Paris on 5 October 1962. Exactly half a century later, on 5 October 2012, Switzerland organised a com- memoration ceremony at the University of Bern to mark ESO’s 50 years of existence and 30 years of Swiss membership with the ESO. This article provides a brief summary of the history and milestones of Swiss member- ship with the ESO as well as an overview of the most important achievements and challenges. Switzerland’s route to ESO membership Nearly twenty years after the ESO was founded, the time was ripe for Switzerland to apply for membership with the ESO. The driving forces on the academic side included the Universi- ty of Geneva and the University of Basel, which wanted to gain access to the most advanced astronomical research available. In 1980, the Federal Council submitted its Dispatch on Swiss membership with the ESO to the Federal Assembly. In 1981, the Federal Assembly adopted a federal decree endorsing Swiss membership with the ESO. In 1982, the Swiss Confederation filed the official documents for ESO membership in Paris. In 1982, Switzerland paid the initial membership fee and, in 1983, the first year’s member- ship contributions. High points of Swiss participation In 1987, the Federal Council issued a federal decree on Swiss participation in the ESO’s Very Large Telescope (VLT) to be built at the Paranal Observatory in the Chilean Atacama Desert.