176 research outputs found
CONSUMO E DIGESTIBILIDADE APARENTE DO FENO DE Andropogon gayanus COLHIDO EM TRĂS IDADES DIFERENTES
Este experimento teve como objetivo avaliar o consumo e a digestibilidade aparente da matĂ©ria seca, proteĂna bruta, fraçÔes fibrosas, energia e balanço do nitrogĂȘnio do feno de Andropogon gayanus colhido em trĂȘs diferentes idades (56, 84 e 112 dias). O delineamento estatĂstico utilizado foi o inteiramente casualizado com trĂȘs tratamentos e seis repetiçÔes. As digestibilidades aparentes da matĂ©ria seca, das fraçÔes fibrosas e da energia bruta foram maiores para os fenos colhidos aos 56 e 84 dias (P0,05). Os valores de consumo e digestibilidade aparente apontam as idades de 56 e 84 dias como as melhores dentre as estudadas para o corte do capim A. gayanus para fenação.
Palavras-chave: forragem; ovino; valor nutritivo
GREEN FORAGE FIBROUS FRACTIONS AND THREE PEARL MILLET GENOTYPES SILAGE [Pennisetum glaucum (L). R. BR.] IN DIFFERENT FERMENTATION PERIODS
It was determined the fibrous fraction (NDF, ADF, cellulose, hemicellulose and lignin) in green forage and pearl millet silages (CMS-1, BRS-1501 and BN-2). The genotypes were planted at Embrapa Milho e Sorgo, ensiled in PVC laboratory silos and evaluated after one, three, five, seven, 14, 28 and 56 days. NDF values ranged from 46.96 to 62.43% and ADF from 27.86 to 34.56%. Hemicellulose contents in green forage were significantly lower than in silages after 56 days ensiling. The NDF, ADF, cellulose, hemicellulose and lignin mean values in green forages and silages after 56 days of fermentation were 60.76 and 51.8%, 33.58 and 31.54%, 29.25 and 27.66%, 27.18 and 20.26%; 4.33 and 3.89%, respectively. The NDF and ADF average values found in this work were lower than those reported in other studies. The hemicellulose fraction contributed as an additional subtract source to the fermentation process. BRS-1501 genotype showed the lower NDF and ADF contents
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
- âŠ