Aptidão de solos da bacia hidrográfica do Rio do Peixe para aporte de fertilizantes orgânicos.

Condições climáticas, geologia e relevo; Solos; Potencial poluente da fertilização orgânica; Recomendações.bitstream/item/58414/1/CUsersPiazzonDocuments230.pd

Modeling the Radio Background from the First Black Holes at Cosmic Dawn: Implications for the 21 cm Absorption Amplitude

We estimate the 21 cm Radio Background from accretion onto the first intermediate-mass Black Holes between $z\approx 30$ and $z\approx 16$. Combining potentially optimistic, but plausible, scenarios for black hole formation and growth with empirical correlations between luminosity and radio-emission observed in low-redshift active galactic nuclei, we find that a model of black holes forming in molecular cooling halos is able to produce a 21 cm background that exceeds the Cosmic Microwave Background (CMB) at $z \approx 17$ though models involving larger halo masses are not entirely excluded. Such a background could explain the surprisingly large amplitude of the 21 cm absorption feature recently reported by the EDGES collaboration. Such black holes would also produce significant X-ray emission and contribute to the $0.5-2$ keV soft X-ray background at the level of $\approx 10^{-13}-10^{-12}$ erg sec$^{-1}$ cm$^{-2}$ deg$^{-2}$, consistent with existing constraints. In order to avoid heating the IGM over the EDGES trough, these black holes would need to be obscured by Hydrogen column depths of $N_\text{H} \sim 5 \times 10^{23} \text{cm}^{-2}$. Such black holes would avoid violating contraints on the CMB optical depth from Planck if their UV photon escape fractions were below $f_{\text{esc}} \lesssim 0.1$, which would be a natural result of $N_\text{H} \sim 5 \times 10^{23} \text{cm}^{-2}$ imposed by an unheated IGM.Comment: 10 pages, 7 figures, accepted to ApJ, replacement to match submitted versio

Recomendações para inoculação e peletizacao de sementes de leguminosas forrageiras tropicais.

Este trabalho teve por objetivo testar um produto adesivo de fácil obtenção e baixo preço, bem como verificar a adequação dos fosfatos de rocha regionais para formação de "pelets" e sua influência na sobrevivência do inoculante, aplicado a semente de diversas leguminosas forrageiras tropicais de interesse regional. Os resultados obtidos permitiram elaborar recomendações praticas (Tabela 2) que se encontram anexas.bitstream/item/138503/1/COT-17.pdfCNPG

A Low Noise Thermometer Readout for Ruthenium Oxide Resistors

The thermometer and thermal control system, for the Absolute Radiometer for Cosmology, Astrophysics, and Diffuse Emission (ARCADE) experiment, is described, including the design, testing, and results from the first flight of ARCADE. The noise is equivalent to about 1 Omega or 0.15 mK in a second for the RuO_2 resistive thermometers at 2.7 K. The average power dissipation in each thermometer is 1 nW. The control system can take full advantage of the thermometers to maintain stable temperatures. Systematic effects are still under investigation, but the measured precision and accuracy are sufficient to allow measurement of the cosmic background spectrum. Journal-ref: Review of Scientific Instruments Vol 73 #10 (Oct 2002)Comment: 5 pages text 7 figure

Inherent and learnt abilities for relative pitch in the vibrotactile domain using the fingertip

This paper reports experimental results concerning relative pitch discrimination. This is defined as the ability to distinguish one musical note as being higher or lower than another. Seventeen participants with normal hearing undertook a pitch discrimination experiment using the fingertip over a 16 session training period with a full baseline test before and after the training sessions. Two sinusoidal tones were presented, each of Is duration separated by a Is gap. A total of 24 tones were chosen to cover 12 intervals ranging from a semi-tone to an octave over the frequency range C3 to B4. The results show a high success rate for relative pitch discrimination with and without training. For intervals of 4 to 12 semitones, the success rates were >70% with or without the 16 training sessions. As a result of training, a significant improvement was found for individual intervals between 9 and 12 semitones when comparing the number of correct responses between pre-training and post-training tests. Comparison of pre- and post-training tests also showed an appreciable and significant improvement for the whole group of 12 intervals. In addition, reaction times to identify relative pitch tended to decrease over the training period

Consorciação de pastagem de Brachiaria decumbens Stapf v. Australiana, com leguminosas plantadas em faixas e sob condições de pastejo.

As pastagens de Brachiaria decumbens apos alguns anos de utilização podem apresentar um decréscimo na produção de matéria seca (MS) resultando em menor capacidade de suporte. Visando solucionar esse problema foi estabelecido um experimento com o objetivo de se manter ou elevar a produtividade de pastagens de B. decumbens pela introdução de leguminosas. As leguminosas foram estabelecidas em faixas onde estão sendo feitas avaliações de persistência das mesmas.bitstream/item/137377/1/PESQ-EM-ANDAMENTO-07.pd

The Temperature of the CMB at 10 GHz

We report the results of an effort to measure the low frequency portion of the spectrum of the Cosmic Microwave Background Radiation (CMB), using a balloon-borne instrument called ARCADE (Absolute Radiometer for Cosmology, Astrophysics, and Diffuse Emission). These measurements are to search for deviations from a thermal spectrum that are expected to exist in the CMB due to various processes in the early universe. The radiometric temperature was measured at 10 and 30 GHz using a cryogenic open-aperture instrument with no emissive windows. An external blackbody calibrator provides an in situ reference. A linear model is used to compare the radiometer output to a set of thermometers on the instrument. The unmodeled residuals are less than 50 mK peak-to-peak with a weighted RMS of 6 mK. Small corrections are made for the residual emission from the flight train, atmosphere, and foreground Galactic emission. The measured radiometric temperature of the CMB is 2.721 +/- 0.010 K at 10 GHz and 2.694 +/- 0.032 K at 30 GHz.Comment: 8 pages including 5 figures. Submitted to The Astrophysical Journa

Reciclagem de nitrogênio em pastagem consorciada de Calopogonium mucunoides com Brachiaria decumbens.

O trabalho estuda a reciclagem de nitrogênio (N) de Calopogonium mucunoides associado com Brachiaria decumbens, sob pastejo continuo, com lotação de 2,5 U.A/ha. As avaliações foram efetuadas através da medida de crescimento da matéria seca (MS) da gramínea e da leguminosa e da quantidade de N em Kg/ha, mobilizada pelo crescimento para a biomassa das plantas da pastagem. Efetuaram-se avaliações do N total e N assimilável (amônia + nitrato) no perfil do solo, a profundidade de 0 a 250 cm, bem como do desempenho do Rhizobium associado a leguminosa. Pode-se determinar que, a consorciação, o crescimento da gramínea, que mobilizou do solo para a vegetação 105,47 kg de N/ha, foi acrescido de mais 81,37 kg de N/ha por ano, mobilizado pelo crescimento da leguminosa.Na pastagem de gramínea pura, o N mobilizado do solo foi de 123,10 kg de N/ha. e uma diferença significativa (P<0,05) de 63,84 kg de N/ha por ano foi adicionada ao sistema da pastagem, sendo atribuída em sua maior parte a fixação simbiótica, realizada pelo Calopogonium mucunoides. O N reciclado resultou um aumento significativo (P<0,05) na oferta de N e proteína bruta na forragem disponível do pasto consociado, ao longo do ano. A leguminosa foi responsável também por um aumento significativo (P<0,05) da percentagem de N total na camada superficial do solo e aumentou significativamente (P<0,05) o conteúdo de N assimilável no perfil. Os estudos realizados em casa de vegetação, com Rhizobium isolado de plantas da pastagem, indicaram que a estirpe associada...bitstream/item/104558/1/Reciclagem-de-nitrogenio-em-pastagem.pd