ESTATUTO UNIVERSITARIO UNSAAC PDF

Instituto De Idiomas Unsaac in Cusco – Contact details, Address Map, Photos, Actualmente en mérito al nuevo estatuto universitario, El Centro de Idiomas. CUUNSAAC como circulo de estudios y a la fecha el CEDITER ya es por unanimidad en sesión extraordinaria del Concejo Universitario. ResolucionCDEPG-UNSAACpdf – Free download as PDF File de Ie Ley , Estatuto Universitario y el Reglamento referide se aplica, Que.

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Meteorological and seeing conditions are crucial both for uunsaac site selection and for telescope design and feasibility studies for adaptive optics. The ELTs shall be very sensitive to wind behavior when operating in open air, therefore ground level wind velocity and wind gust are also required for the feasibility of the telescope construction. Here unnsaac analyze the wind speed and wind direction, the air temperature, the relative humidity and the barometric pressure statistical results obtained from data recorded at different sites at the ORM by several Automatic Weather Stations AWS sinceday and night time separately.

Ground wind speed regimes mbar are compared with those provided by satellites from to mbar. There exists also observational evidence estafuto the correlation between the seeing and the wind speed and wind direction that will be discussed in this work. Precipitable water vapour forecasting: We have run WRF every 24 h for near two months, with a horizon of 48 hours hourly forecastsfrom Universitaroo 11 to March 4. These runs represent hourly forecast points.

The validation is carried out using different approaches: The h forecast was further improved by correcting a time lag of 2 h found in the predictions. The final errors, taking into account all the uncertainties involved, are 1.

We found linear trends in both the correlation and RMSE of the residuals measurements – forecasts as a function of the forecast range within the horizons analysed up to 48 h.

In summary, unniversitario WRF performance is excellent and accurate, thus allowing it to be implemented as an operational tool at the ORM. Directory of Open Access Journals Sweden.

Educando a los muchachos: This article draws on new social-scientific research on masculinity to develop a framework for understanding gender issues in the education of boys. Gender is constructed within institutional and cultural contexts that produce multiple forms of masculinity. Normally one form is hegemonic over others.

Schools are active players in the formation of masculinities. Masculinizing practices are concentrated at certain sites: Pupils are also active in constructing masculinities. Pupil cultures commonly emphasize heterosexual relationships and construct gender hierarchies. The Industrial Sectorial Observatories. Objectives, organization and operation; Los observatorios industriales sectoriales. Objetivos, composicion y funcionamiento. Through this systematic analysis, policies could be adapted to the true needs of each industry and its effectiveness be ensured, in order to strengthen the competitiveness of the Spanish industry.

Towards a new Mercator Observatory Control System. A new control system is currently being developed for the 1. Formerly based on transputers, the new Mercator Observatory Control System MOCS consists of a small network of Linux computers complemented by a central industrial controller and an industrial real-time data communication network. Python is chosen as the high-level language to develop flexible yet powerful supervisory control and data acquisition SCADA software for the Linux computers.

Specialized applications such as detector control, auto-guiding and middleware management are also integrated in the same Python software package. The industrial controller, on the other hand, is connected to the majority of the field devices and is targeted to run various control loops, some of which are real-time critical.

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Independently of the Linux distributed control system DCSthis controller makes sure that high priority tasks such as the telescope motion, mirror support and hydrostatic bearing control are carried out in a reliable and safe way.

As the latter is chosen as the primary platform for the lower level control, a substantial part of the software is being ported to the IEC standard programming languages. Additionally, obsolete hardware is gradually being replaced by standard industrial alternatives with fast EtherCAT communication.

In this contribution, we give an overview of the systems design, implementation details and the current status of the project. The sampling site, located on the campus of the California Institute of Technology in Pasadena, was positioned to sample a continuous afternoon influx of transported urban aerosol with a photochemical age of 1—2 h and generally free from major local contributions. Sampling spanned 5 months during the summer ofwhich were broken into 3 regimes on the basis of distinct meteorological conditions.

Regime I was characterized by a series of low pressure systems, resulting in high humidity and rainy periods with clean conditions.

Regime II typified early summer meteorology, with significant morning marine layers and warm, sunny afternoons. Regime III was characterized by hot, dry conditions with little marine layer influence. The overall oxidation state remains relatively constant on timescales of days to weeks O: C between morning and afternoon periods.

Periods characterized by significant morning marine layer influence followed by photochemically favorable afternoons displayed significantly higher aerosol mass and O: C ratio, suggesting that aqueous processes may be important in the generation of secondary eststuto and oxidized organic aerosol OOA in Los Angeles.

Sulfate and nitrate reside predominantly. Development of the quality control system of the readout electronics for the large size telescope of the Cherenkov Telescope Array observatory. The readout system for the LST prototype has been designed and around readout boards will be produced in the coming months.

In this note we describe an automated univesritario control system able to measure basic performance parameters and quickly identify faulty boards. SARA observatories comprise a 0. Remote operation offers considerable flexibility in scheduling, allowing long-term observational cadences difficult to achieve with classical observing at remote facilities, as well as obvious travel savings.

Multiple observers at different locations can share a telescope for training, educational use, or collaborative research programs.

Each telescope has a CCD system for optical imaging, using thermoelectric cooling to avoid the need for frequent local service, and a second CCD for offset guiding.

The Arizona and Chile telescopes also have fiber-fed echelle spectrographs. Switching between imaging esatuto spectroscopy is very rapid, so a night can easily accommodate mixed observing modes. We present some sample observational programs.

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For the benefit of other groups organizing similar consortia, we describe the operating univerzitario and principles of SARA, as well as some lessons learned from almost 20 years of remote operations. Spanish estatutl and competitiveness. The overview from the Industrial Observatories ; Industria espanola y competitividad.

La vision desde los observatorios industriales. This article analyzes the competitiveness of the Spanish industry. It explains the interdependencies and relations that link globalization, internationalization and international trade with competitiveness.

The main features of the Spanish industry are also studied in depth, its strengths and weaknesses. Finally, the challenges that the Spanish industry will face in the future are considered, as well as the role that the industrial observatories will play in that context.

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MOURA is a compact, miniaturized, intelligent and low cost instrument, based on two sets of triaxial magnetometers separated one centimeter from each other to do gradiometry studies. It has a resolution of 2. Also, this technology has been previously successfully employed on board Unmanned Aerial Vehicles UAV to perform geomagnetic surveys in extreme conditions areas [3], and in several space missions for different applications.

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These compensation equations have been applied to field data, which have shown to follow the daily Earth’s magnetic field variations as registered by San Pablo Geomagnetic Observatory IAGA code: SPT available at www.

CEDITER | UNSAAC

These deviations were attributed to several error factors as the different locations between MOURA and SPT and other possible different geomagnetic conditions. Due to the above, a measurement campaign on SPT installations are been done. It considers the ways in which boys attending schools in London negotiate what they see as the contradictions involved in attempting to reconcile doing schoolwork with being accepted by other boys as masculine.

The paper argues that these contradictions are emotionally charged, so that boys put effort into negotiating what they see as a middle position because this is the least problematic subject position for them to take up. The Griffith Observatoryperched atop the Hollywood Hills, is perhaps the most recognizable observatory in the world. Since opening inthis Los Angeles icon has brought millions of visitors closer to the heavens.

The astronomical community at nearby Mt. The influences of these three communities- professional astronomy, entertainment, and aerospace- persist today and continue to make Griffith Observatory one of the premiere sites of public astronomy in the country.

Private Observatories in South Africa. Descriptions of private observatories in South Africa, written by their owners.

Positions, equipment descriptions and observing programmes are given. Klein Karoo Observatory B. FosterLe Marischel Observatory L.

FerreiraSterkastaaing Observatory M. StreicherHenley on Klip B. FraserArcher Observatory B. DumasOverbeek Observatory A. OverbeekOverberg Observatory A. RobertsWeltevreden Karoo Observatory D. BullisWinobs M. By studying gamma-rays from objects like black holes, pulsars, quasars, neutron stars, and other exotic objects, scientists could discover clues to the birth, evolution, and death of stars, galaxies, and the universe.

The gamma-ray instrument was one of four major science instruments aboard the Compton. It consisted of eight detectors, or modules, located at each corner of the rectangular satellite to simultaneously scan the entire universe for bursts of gamma-rays ranging in duration from fractions of a second to minutes. In Januarythe instrument, via the Internet, cued a computer-controlled telescope at Las Alamos National Laboratory in Los Alamos, New Mexico, within 20 seconds of registering a burst.

With this capability, the gamma-ray experiment came to serve as a gamma-ray burst alert for the Hubble Space Telescope, the Chandra X-Ray Observatoryand major gound-based observatories around the world. It’s the world’s largest, sharpest, dedicated telescope array.

The Pierre Auger Observatory. The Pierre Auger Observatory is an international collaboration for the detailed study of the highest energy cosmic rays. It will operate at two similar sites, one in the northern hemisphere and one in the southern hemisphere.

The Observatory is designed to collect a statistically significant data set of events with energies greater than 10 19 eV and with equal exposures for the northern and southern skies.