A solar storm observed from the Sun to Venus using the STEREO, Venus Express, and MESSENGER spacecraft

The suite of SECCHI optical imaging instruments on the STEREO-A spacecraft is used to track a solar storm, consisting of several coronal mass ejections (CMEs) and other coronal loops, as it propagates from the Sun into the heliosphere during May 2007. The 3-D propagation path of the largest interplanetary CME (ICME) is determined from the observations made by the SECCHI Heliospheric Imager (HI) on STEREO-A (HI-1/2A). Two parts of the CME are tracked through the SECCHI images, a bright loop and a V-shaped feature located at the rear of the event. We show that these two structures could be the result of line-of-sight integration of the light scattered by electrons located on a single flux rope. In addition to being imaged by HI, the CME is observed simultaneously by the plasma and magnetic field experiments on the Venus Express and MESSENGER spacecraft. The imaged loop and V-shaped structure bound, as expected, the flux rope observed in situ. The SECCHI images reveal that the leading loop-like structure propagated faster than the V-shaped structure, and a decrease in in situ CME speed occurred during the passage of the flux rope.We interpret this as the result of the continuous radial expansion of the flux rope as it progressed outward through the interplanetary medium. An expansion speed in the radial direction of ~30 km s-1 is obtained directly from the SECCHI-HI images and is in agreement with the difference in speed of the two structures observed in situ. This paper shows that the flux rope location can be determined from white light images, which could have important space weather applications.

Tracking the momentum flux of a CME and quantifying its influence on geomagnetically induced currents at Earth

We investigate a coronal mass ejection (CME) propagating toward Earth on 29 March 2011. This event is specifically chosen for its predominately northward directed magnetic field, so that the influence from the momentum flux onto Earth can be isolated. We focus our study on understanding how a small Earth-directed segment propagates. Mass images are created from the white-light cameras onboard STEREO which are also converted into mass height-time maps (mass J-maps). The mass tracks on these J-maps correspond to the sheath region between the CME and its associated shock front as detected by in situ measurements at L1. A time series of mass measurements from the STEREO COR-2A instrument is made along the Earth propagation direction. Qualitatively, this mass time series shows a remarkable resemblance to the L1 in situ density series. The in situ measurements are used as inputs into a three-dimensional (3-D) magnetospheric space weather simulation from the Community Coordinated Modeling Center. These simulations display a sudden compression of the magnetosphere from the large momentum flux at the leading edge of the CME, and predictions are made for the time derivative of the magnetic field (dB/dt) on the ground. The predicted dB/dt values were then compared with the observations from specific equatorially located ground stations and showed notable similarity. This study of the momentum of a CME from the Sun down to its influence on magnetic ground stations on Earth is presented as a preliminary proof of concept, such that future attempts may try to use remote sensing to create density and velocity time series as inputs to magnetospheric simulations.

Tests of sunspot number sequences: 1. Using ionosonde data

More than 70 years ago it was recognised that ionospheric F2-layer critical frequencies [foF2] had a strong relationship to sunspot number. Using historic datasets from the Slough and Washington ionosondes, we evaluate the best statistical fits of foF2 to sunspot numbers (at each Universal Time [UT] separately) in order to search for drifts and abrupt changes in the fit residuals over Solar Cycles 17-21. This test is carried out for the original composite of the Wolf/Zürich/International sunspot number [R], the new “backbone” group sunspot number [RBB] and the proposed “corrected sunspot number” [RC]. Polynomial fits are made both with and without allowance for the white-light facular area, which has been reported as being associated with cycle-to-cycle changes in the sunspot number - foF2 relationship. Over the interval studied here, R, RBB, and RC largely differ in their allowance for the “Waldmeier discontinuity” around 1945 (the correction factor for which for R, RBB and RC is, respectively, zero, effectively over 20 %, and explicitly 11.6 %). It is shown that for Solar Cycles 18-21, all three sunspot data sequences perform well, but that the fit residuals are lowest and most uniform for RBB. We here use foF2 for those UTs for which R, RBB, and RC all give correlations exceeding 0.99 for intervals both before and after the Waldmeier discontinuity. The error introduced by the Waldmeier discontinuity causes R to underestimate the fitted values based on the foF2 data for 1932-1945 but RBB overestimates them by almost the same factor, implying that the correction for the Waldmeier discontinuity inherent in RBB is too large by a factor of two. Fit residuals are smallest and most uniform for RC and the ionospheric data support the optimum discontinuity multiplicative correction factor derived from the independent Royal Greenwich Observatory (RGO) sunspot group data for the same interval.

A novel regeneration system for a wild passion fruit species (Passiflora cincinnata Mast.) based on somatic embryogenesis from mature zygotic embryos

The objective of the present work was to induce somatic embryogenesis from zygotic embryos of Passiflora cincinnata Masters. Zygotic embryos formed calli on media with different concentrations of 2,4-dichlorophenoxyacetic acid (2,4-D) and 4.5 mu M benzyladenine (BA) after 30 days of in vitro culture. A concentration of 18.1 mu M 2,4-D resulted in the largest number of somatic embryos. Embryogenic calli were yellowish and friable, forming whitish proembryogenic masses. Morphologically, embryogenic cells were small and had large nuclei and dense cytoplasm, whereas non-embryogenic cells were elongated, with small nuclei and less dense cytoplasm. Calli cultured under white light on basal Murashige and Skoog`s medium with activated charcoal produced embryos in all developmental stages. There were differences among the treatments, with some leading to the production of calli with embryos and some only to callus formation. Some abnormalities were associated with somatic embryos, including fused axes, fused cotyledons and polycotyledonary embryos. Production of secondary somatic embryos occurred in the first cycle of primary embryo development. Secondary embryos differentiated from the surface of the protodermal layer of primary embryos with intense cell proliferation, successive mitotic divisions in the initial phase of embryoid development, and a vascular system formed with no connection to the parental tissue. This secondary embryogenic system of P. cincinnata is characterized by intense proliferation and maintenance of embryogenic competence after successive subcultures. This reproducible protocol opens new prospects for massive propagation and is an alternative to the current organogenesis-based transformation protocol.

Menezesite, the first natural heteropolyniobate, from Cajati, Sao Paulo, Brazil: Description and crystal structure

Menezesite, ideally Ba2MgZr4(BaNb12O42)center dot 12H(2)O, occurs as a vug mineral in the contact zone between dolomite carbonatite and ""jacupirangite"" (=a pyroxenite) at the Jacupiranga mine, in Cajati county, Sao Paulo state, Brazil, associated with dolomite, calcite, magnetite, clinohumite, phlogopite, ancylite-(Ce), strontianite, pyrite, and tochilinite. This is also the type locality for quintinite-2H. The mineral forms rhombododecahedra up to I mm, isolated or in aggregates. Menezesite is transparent and displays a vitreous luster; it is reddish brown with a white streak. It is non-fluorescent. Mohs hardness is about 4. Calculated density derived from the empirical formula is 4.181 g/cm(3). It is isotropic, 1.93(1) (white light); n(calc) = 2.034. Menezesite exhibits weak anomalous birefringence. The empirical formula is (Ba1.47K0.53Ca0.3,Ce0.17Nd0.10Na0.06La0.02)(Sigma 2.66)(Mg0.94Mn0.23Fe0.23Al0.03)(Sigma 1.43)(Zr2.75Ti0.96Th0.29)(Sigma 4.00)[(Ba0.72Th0.26U0.02)(Sigma 1.00)(Nb9.23Ti2.29Ta0.36Si0.12)Sigma O-12.00(42)]center dot 12H(2)O. The mineral is cubic, space group 10 (204), a = 13.017(1) angstrom, V = 2206(1) angstrom(3), Z = 2. Menezesite is isostructural with the synthetic compound Mg-7[MgW12O42](OH)(4)center dot 8H(2)O. The mineral was named in honor of Luiz Alberto Dias Menezes Filho (born 1950), mining engineer, mineral collector and merchant. Both the description and the name were approved by the CNMMN-IMA (Nomenclature Proposal 2005-023). Menezesite is the first natural heteropolyniobate. Heteropolyanions have been employed in a range of applications that include virus-binding inorganic drugs (including the AIDs virus), homogeneous and heterogeneous catalysts, electro-optic and electrochromic materials, metal and protein binding, and as building blocks for nanostructuring of materials.

Footemineite, the Mn-analog of atencioite, from the Foote mine, Kings Mountain, Cleveland County, North Carolina, USA, and its relationship with other roscherite-group minerals

Footemineite, ideally Ca2Mn2+square Mn22+Be4(PO4)(6)(OH)(4)-6H(2)O, triclinic, is a new member of the roscherite group. It occurs on thin fractures crossing quartz-microcline-spodumene pegmatite at the Foote mine, Kings Mountain, Cleveland County, North Carolina, U.S.A. Associated minerals are albite, analcime, eosphorite, siderite/rhodochrosite, fairfieldite, fluorapatite, quartz, milarite, and pyrite. Footemineite forms prismatic to bladed generally rough to barrel-shaped crystals up to about 1.5 mm long and I mm in diameter. Its color is yellow, the streak is white, and the luster is vitreous to slightly pearly. Footemineite is transparent and non-fluorescent. Twinning is simple, by reflection, with twin boundaries across the length of the crystals. Cleavage is good on {0 (1) over bar1}) and {100}. Density (calc.) is 2.873 g/cm(3). Footemineite is biaxial (-), n(alpha) = 1.620(2), n(beta) = 1.627(2), n(gamma) = 1.634(2) (white light). 2V(obs) = 80 degrees, 2V(calc) = 89.6 degrees. Orientation: X boolean AND b similar to 12 degrees, Y boolean AND c similar to 15 degrees, Z boolean AND a similar to 15 degrees. Elongation direction is c, dispersion: r > v or r < v, weak. Pleochroism: beta (brownish yellow) > alpha = gamma (yellow). Mossbauer and IR spectra are given. The chemical composition is (EDS mode electron microprobe, Li and Be by ICP-OES, Fe3+:Fe2+ y Mossbauer, H2O by TG data, wt%): Li2O 0.23, BeO 9.54, CaO 9.43, SrO 0.23, BaO 0.24, MgO 0.18, MnO 26.16, FeO 2.77, Fe2O3 0.62, Al2O3 0.14, P2O5 36.58, SiO2 0.42, H2O 13.1, total 99.64. The empirical formula is (Ca1.89Sr0.03Ba0.02)Sigma(1.94)(Mn-0.90(2+)square(0.10))Sigma(1.00)(square 0.78Li0.17Mg0.05) Sigma(1.00)(Mn3.252+Fe0.432+ Fe0.093+Al0.03)Sigma(3.80) Be-4.30(P5.81Si0.08O24)[(OH)3.64(H2O)0.36]Sigma(4.00)center dot 6.00H(2)O . The strongest reflection peaks of the powder diffraction pattern [d, angstrom (1, %) (hkl)] are 9.575 (53) (010), 5.998 (100) (0 (1) over bar1), 4.848 (26) (021), 3.192 (44) (210), 3.003 (14) (0 (2) over bar2), 2.803 (38) ((1) over bar 03), 2.650 (29) ((2) over bar 02), 2.424 (14) (231). Single-crystal unit-cell parameters are a = 6.788(2), b = 9.972(3), c = 10.014(2) A, (x = 73.84(2), beta = 85.34(2), gamma = 87.44(2)degrees,V = 648.74 angstrom(3), Z = 1. The space group is P (1) over bar. Crystal structure was refined to R = 0.0347 with 1273 independent reflections (F > 2(5). Footemineite is dimorphous with roscherite, and isostructural with atencioite. It is identical with the mineral from Foote mine described as ""triclinic roscherite."" The name is for the Foote mine, type locality for this and several other minerals.

Theoretical and experimental optical holography

The intent of this paper is to present an analysis of optical holography. Both the physical theory behind holography and the experimental techniques used in making holograms will be presented. To accomplish this goal, the paper is divided into two independent sections: the theoretical section followed by the experimental section. Each section is intended to be a complete unit. The Theoretical Section is an exposure to the theory behind holography. This consists of a review of the concepts of interference and diffraction. followed by a brief review of partial coherence. The remaining part of the Theoretical Section is devoted to the mathematical analysis of optical holography. The Experimental Section begins with an introduction to the equipment and facilities currently available for optical holography at Colby College. Holographic procedures is dominated by the description of transmission holography (v.s. reflection. or white-light. holography). After these general holographic procedures a few variations on the basic transmission hologram are presented. The experimental section will end with an introduction to holographic interferometry, a major application of holographic techniques.

Control of Salmonella enterica serovar Enteritidis in laying hens by inactivated Salmonella Enteritidis vaccines

Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)

Efeito da temperatura e da luz na germinação de sementes de Acacia polyphylla DC.

Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)

Armazenamento e requerimento fotoblástico de sementes de Acacia polyphylla DC

Acacia polyphyla (Mimosaceae) é uma espécie arbórea nativa do Brasil, importante para a recuperação de áreas degradadas. Sementes dessa espécie foram armazenadas em condições naturais e artificiais, com os objetivos de avaliar a longevidade das sementes no solo, conservar a sua qualidade fisiológica pelo período correspondente a duas colheitas e verificar o requerimento fotoblástico das sementes armazenadas. em condições naturais, as sementes foram enterradas em clareira, sob dossel ralo e sob dossel denso. As sementes deterioraram rapidamente, revelando-se incapazes de compor o banco de sementes do solo. em condições artificiais, as sementes foram acondicionadas em diferentes embalagens e armazenadas por dois anos em ambiente não controlado e em câmara fria. Periodicamente, as sementes foram colocadas para germinar a 25ºC, na ausência de luz e sob fotoperíodo de oito horas sob luzes branca e de sombreamento. Durante todo o período de armazenamento, a germinação no escuro foi inferior à constatada sob luzes branca e de sombreamento. A qualidade fisiológica foi conservada por dois anos, quando as sementes foram acondicionadas em embalagem impermeável e armazenadas em câmara fria. O comportamento germinativo das sementes armazenadas por dois anos foi comparado com o de sementes recém-colhidas, em temperaturas constante e alternada, não sendo constatado efeito da idade e do regime de temperatura no requerimento fotoblástico das sementes.

Germinação de sementes de pau-ferro submetidas a diferentes condições de armazenamento, escarificação química, temperatura e luz

Caesalpinia leiostachya (Benth.) Ducke (pau-ferro) é uma planta arbórea nativa do Brasil, cujas sementes possuem dormência causada pela impermeabilidade do tegumento à água. Neste trabalho foram conduzidos dois experimentos, nos quais foram utilizados diferentes períodos de escarificação em ácido sulfúrico concentrado para superar a dormência das sementes. No primeiro experimento, sementes coletadas em agosto de 1997 foram armazenadas por oito meses em ambiente não controlado no interior do próprio fruto, e em câmara seca após serem extraídas dos frutos; a seguir, elas foram imersas em ácido sulfúrico por 0, 10, 20, 40, 60 e 80min e colocadas para germinar nas temperaturas constante de 25ºC e alternada de 20-30°C, sob fotoperíodo de 8h. No segundo experimento, sementes extraídas de frutos recém-coletados em agosto de 1998 foram imersas em ácido sulfúrico por 0, 10, 20, 30, 40 e 60min, seguido do teste de germinação conduzido nas mesmas temperaturas do experimento anterior, na ausência e presença de luz. Foram avaliados a porcentagem final e o índice de velocidade de germinação das sementes. Os resultados mostraram que (a) a manutenção das sementes no interior dos frutos é uma alternativa viável para o armazenamento durante o período adotado; (b) as sementes recém-coletadas são indiferentes à luz, nas duas temperaturas testadas; (c) as sementes recém-coletadas e as armazenadas germinam em maior velocidade a 25ºC; (d) em sementes armazenadas, a imersão em ácido sulfúrico por 10min é suficiente para superar a dormência; (e) em sementes recém-coletadas, a imersão em ácido sulfúrico por 20 a 30min favorece a porcentagem e a velocidade de germinação.

Crescimento in vitro e aclimatização de Cattleya loddigesii Lindley (Orchidaceae) com carvão ativado sob dois espectros luminosos

Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)

Utilização do teste de raios - x na avaliação dos efeitos da dessecação e infestação em diásporos de Canela-Batalha - Cryptocarya aschersoniana Mez (Lauraceae)

No presente trabalho, objetivou-se avaliar os efeitos da dessecação e identificar lesões por predação por insetos, em diásporos de canela-batalha (Cryptocarya aschersoniana Mez.), utilizando-se testes de raios X. Os danos provocados pela dessecação foram dimensionados nas imagens e associados à formação de plântulas. Diásporos recém-beneficiados (45 % de umidade e 37 % de germinação) foram colocados para secar em sala climatizada (20 ºC e 60 % UR), dentro de bandejas plásticas em camada única. Posteriormente, com o intuito de acelerar o processo de secagem, foram colocados em caixas de secagem com solução saturada de hidróxido de sódio (28 % UR) e amostrados com 45, 37, 35, 31 e 26 % de umidade. Para as radiografias, utilizou-se a intensidade de radiação de 40 kVp e tempo de exposição de 1,5 minutos. Posteriormente, as radiografias foram fotografadas e as imagens analisadas em computador, sendo medido o afastamento entre o endocarpo e a semente. As sementes foram classificadas em sementes intactas, sementes com afastamento parcial, sementes com afastamento total e sementes predadas. Os testes de germinação foram realizados sobre areia, em germinadores tipo Mangelsdorf a 25 ºC e luz branca constante. Pelos resultados, observa-se que a germinação é comprometida quando o teor de água das sementes fica abaixo de 26 %. Nesse ponto, o afastamento entre o endocarpo e a semente é de 0,65 mm. Houve uma correlação positiva entre a viabilidade das sementes, avaliada pelo teste de germinação, e o afastamento entre o endocarpo e a semente observado nas radiografias. A análise radiográfica possibilita identificar danos provocados por predação após infestação por insetos.

Uso de antibióticos para o controle de bactérias endógenas visando à micropropagação da figueira

A descontaminação dos explantes é um dos princípios básicos para o sucesso da cultura de tecidos. Um dos problemas diagnosticados na propagação in vitro da figueira, através de gemas apicais, é a contaminação endógena dos explantes por bactérias. Este trabalho teve como objetivo avaliar a eficiência de alguns antibióticos em meio de cultura para o controle de bactérias endógenas em gemas apicais de figueira. Foram avaliados os seguintes tratamentos: T1(sem adição de antibiótico); T2 (30 mg L-1 de cloranfenicol); T3 (250 mg L-1 de ampicilina sódica); T4 (500 mg L-1 de ácido nalidícico); T5 (150 mg L-1 de cefalotina sódica); T6 (500 mg L-1 de tetraciclina), e T7 (400 mg L-1 de norfloxacina). Após coletados em campo, os segmentos de ramos contendo as gemas foram colocados em recipiente com água corrente. Posteriormente, as gemas apicais foram imersas em álcool etílico a 70% e hipoclorito de sódio a 2,5%. Todo procedimento de desinfestação externa dos explantes foi realizado em câmara de fluxo laminar. Os explantes foram inoculados em tubos de ensaio contendo 15 mL de meio básico MS suplementado, após a autoclavagem, com as doses de antibióticos de acordo com os tratamentos estabelecidos. Após a inoculação, os explantes foram mantidos em sala de crescimento por quatro dias no escuro e, em seguida, sob fotoperíodo de 16 horas de luz branca fria e irradiância de 25 µmol m s-1, na temperatura de 22 ± 3ºC. A assepsia realizada externamente nos explantes foi suficiente para o controle de contaminação fúngica, e a adição de antibióticos ao meio, após autoclavagem, foi eficiente para o controle de bactérias endógenas, cujo antibiótico ampicilina sódica proporcionou mais de 90% de explantes sobreviventes.

Stability of cp-Ti and Ti-6Al-4V alloy for dental implants as a function of saliva pH - an electrochemical study

Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)