51 research outputs found
Incidencia de los hábitos en el aprovechamiento del tiempo escolar. School - time - managment, habit - related - influence.
Esta investigación propone explorar si maestros y alumnos muestran hábitos en la escuela y si éstos inciden en el aprovechamiento del tiempo escolar, lo que permitiría inferir que su presencia optimizaría el proceso de aprendizaje y el comportamiento.
Problema: ¿Qué efecto tienen los hábitos sobre el aprovechamiento del tiempo en la escuela?
Hipótesis: La presencia de hábitos positivos en maestros y alumnos posibilita un significativo aprovechamiento del tiempo en las diversas actividades que se desarrollan en la sala de clase y en los diferentes momentos del funcionamiento escolar.
Objetivos: Determinar en qué medida la presencia/ausencia de hábitos en maestros y alumnos incide sobre el aprovechamiento del tiempo escolar.
Específicos: 1. Explorar si el currículum prescripto contempla la adquisición de hábitos como objetivo y/o contenido de aprendizaje. 2. Analizar si se advierten hábitos en las diversas oportunidades de aprendizaje que surgen en el ámbito escolar, como consecuencia del currículum prescripto y/o del currículum oculto. 3. Determinar la importancia de la adquisición de hábitos como objetivo educativo en la escuela. 4. Detectar si hay diferencias en la propuesta educativa ofrecida a los diversos grupos socio-económico-culturales.
Metodología: Exploratoria-descriptiva-correlacional-transeccional, que pretende especificar cómo se manifiestan las variables sometidas a análisis (tiempo-hábitos-oportunidades escolares de enseñanza-aprendizaje) y el grado de relación existente entre las mismas.
Técnicas: observación, análisis de contenido, cuestionario, entrevista.
Unidades de análisis: Presencia/ausencia de hábitos en el currículum escolar prescripto u oculto y en el comportamiento de maestros y alumnos; incidencia de los mismos sobre el aprovechamiento del tiempo escolar; existencia/inexistencia de diferencias en la propuesta educativa ofrecida a los diversos grupos socio-económicoculturales. Se realizará un muestreo estratificado proporcional, mediante una selección al azar, aleatoria simple; una distribución de frecuencias para encontrar la mediana, la razón y la tasa, a fin de implementar la prueba de hipótesis y realizar la estadística inferencial; se elaborará el informe de investigación.
Consideramos que el producto final favorecerá la toma de conciencia sobre la importancia de contemplar los hábitos en los maestros y en la formación integral de los alumnos, para optimizar el proceso de enseñanza -aprendizaje y ayudar a mejorar el funcionamiento institucional. Asimismo podrá proponerse como objeto de conocimiento científico para la formación docente y constituirse en un interesante insumo para la política educativa en lo que respecta a la formulación del currículum prescripto para los distintos niveles de educación formal obligatoria
Measurement of the cosmic ray spectrum above eV using inclined events detected with the Pierre Auger Observatory
A measurement of the cosmic-ray spectrum for energies exceeding
eV is presented, which is based on the analysis of showers
with zenith angles greater than detected with the Pierre Auger
Observatory between 1 January 2004 and 31 December 2013. The measured spectrum
confirms a flux suppression at the highest energies. Above
eV, the "ankle", the flux can be described by a power law with
index followed by
a smooth suppression region. For the energy () at which the
spectral flux has fallen to one-half of its extrapolated value in the absence
of suppression, we find
eV.Comment: Replaced with published version. Added journal reference and DO
Energy Estimation of Cosmic Rays with the Engineering Radio Array of the Pierre Auger Observatory
The Auger Engineering Radio Array (AERA) is part of the Pierre Auger
Observatory and is used to detect the radio emission of cosmic-ray air showers.
These observations are compared to the data of the surface detector stations of
the Observatory, which provide well-calibrated information on the cosmic-ray
energies and arrival directions. The response of the radio stations in the 30
to 80 MHz regime has been thoroughly calibrated to enable the reconstruction of
the incoming electric field. For the latter, the energy deposit per area is
determined from the radio pulses at each observer position and is interpolated
using a two-dimensional function that takes into account signal asymmetries due
to interference between the geomagnetic and charge-excess emission components.
The spatial integral over the signal distribution gives a direct measurement of
the energy transferred from the primary cosmic ray into radio emission in the
AERA frequency range. We measure 15.8 MeV of radiation energy for a 1 EeV air
shower arriving perpendicularly to the geomagnetic field. This radiation energy
-- corrected for geometrical effects -- is used as a cosmic-ray energy
estimator. Performing an absolute energy calibration against the
surface-detector information, we observe that this radio-energy estimator
scales quadratically with the cosmic-ray energy as expected for coherent
emission. We find an energy resolution of the radio reconstruction of 22% for
the data set and 17% for a high-quality subset containing only events with at
least five radio stations with signal.Comment: Replaced with published version. Added journal reference and DO
Measurement of the Radiation Energy in the Radio Signal of Extensive Air Showers as a Universal Estimator of Cosmic-Ray Energy
We measure the energy emitted by extensive air showers in the form of radio
emission in the frequency range from 30 to 80 MHz. Exploiting the accurate
energy scale of the Pierre Auger Observatory, we obtain a radiation energy of
15.8 \pm 0.7 (stat) \pm 6.7 (sys) MeV for cosmic rays with an energy of 1 EeV
arriving perpendicularly to a geomagnetic field of 0.24 G, scaling
quadratically with the cosmic-ray energy. A comparison with predictions from
state-of-the-art first-principle calculations shows agreement with our
measurement. The radiation energy provides direct access to the calorimetric
energy in the electromagnetic cascade of extensive air showers. Comparison with
our result thus allows the direct calibration of any cosmic-ray radio detector
against the well-established energy scale of the Pierre Auger Observatory.Comment: Replaced with published version. Added journal reference and DOI.
Supplemental material in the ancillary file
Multiple Scenario Generation of Subsurface Models:Consistent Integration of Information from Geophysical and Geological Data throuh Combination of Probabilistic Inverse Problem Theory and Geostatistics
Neutrinos with energies above 1017 eV are detectable with the Surface Detector Array of the Pierre Auger Observatory. The identification is efficiently performed for neutrinos of all flavors interacting in the atmosphere at large zenith angles, as well as for Earth-skimming \u3c4 neutrinos with nearly tangential trajectories relative to the Earth. No neutrino candidates were found in 3c 14.7 years of data taken up to 31 August 2018. This leads to restrictive upper bounds on their flux. The 90% C.L. single-flavor limit to the diffuse flux of ultra-high-energy neutrinos with an E\u3bd-2 spectrum in the energy range 1.0
7 1017 eV -2.5
7 1019 eV is E2 dN\u3bd/dE\u3bd < 4.4
7 10-9 GeV cm-2 s-1 sr-1, placing strong constraints on several models of neutrino production at EeV energies and on the properties of the sources of ultra-high-energy cosmic rays
Käytännön kosteikkosuunnittelu
Maatalouden vesiensuojelua edistetään monin tavoin. Ravinteita ja eroosioainesta sisältäviä valumavesiä pyritään puhdistamaan erilaisissa kosteikoissa. Tämä opas on kirjoitettu avuksi pienimuotoisten kosteikkojen perustamiseen. Oppaassa esitetään käytännönläheisesti kosteikon toteuttamisen eri vaiheet paikan valinnasta suunnitteluun ja rakentamiseen. Vuonna 2010 julkaistun painoksen tiedot on saatettu ajantasalle.
Julkaisu on toteutettu osana Tehoa maatalouden vesiensuojeluun (TEHO) -hanketta ja päivitetty TEHO Plus -hankkeen toimesta. Oppaan toivotaan lisäävän kiinnostusta kosteikkojen suunnitteluun ja edelleen niiden rakentamiseen
Search for patterns by combining cosmic-ray energy and arrival directions at the Pierre Auger Observatory
Searches for Anisotropies in the Arrival Directions of the Highest Energy Cosmic Rays Detected by the Pierre Auger Observatory
Interpretation of the depths of maximum of extensive air showers measured by the Pierre Auger Observatory
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