Our changing Sun

Stellar astronomy tells us much about the long-term evolution of our Sun while forensic evidence (for example, cosmic-ray products in ice cores) gives us indications of its fluctuations over the last millennium. However, such studies do not give us a sufficiently detailed understanding of solar change over the last century to allow us to detect and quantify any role that the Sun might have played in the observed rise in average surface temperatures on Earth. This paper describes recent research that has filled this gap by applying advances in our understanding of the effects and structure of the solar wind to historical data on the Earth's magnetic field.

A doubling of the sun's coronal magnetic field during the last 100 years

The solar wind is an extended ionized gas of very high electrical conductivity, and therefore drags some magnetic flux out of the Sun to fill the heliosphere with a weak interplanetary magnetic field(1,2). Magnetic reconnection-the merging of oppositely directed magnetic fields-between the interplanetary field and the Earth's magnetic field allows energy from the solar wind to enter the near-Earth environment. The Sun's properties, such as its luminosity, are related to its magnetic field, although the connections are still not well understood(3,4). Moreover, changes in the heliospheric magnetic field have been linked with changes in total cloud cover over the Earth, which may influence global climate(5), Here we show that measurements of the near-Earth interplanetary magnetic field reveal that the total magnetic flux leaving the Sun has risen by a factor of 1.4 since 1964: surrogate measurements of the interplanetary magnetic field indicate that the increase since 1901 has been by a factor of 2,3, This increase may be related to chaotic changes in the dynamo that generates the solar magnetic field. We do not yet know quantitatively how such changes will influence the global environment.

The interconnection of the magnetic fields of the Earth and the sun

Magnetic reconnection facilitates the transfer of mass, energy, and momentum from the solar wind, through the Earth's magnetosphere and into the upper atmosphere. Recently, combined observations using both ground-based and satellite instruments have revealed much about how reconnection takes place. This new understanding has great signficance for systems which exploit, or operate within, the Earth's plasma environment, as well as for a wide variety of scientific studies.

Observation in the MINOS far detector of the shadowing of cosmic rays by the sun and moon

The shadowing of cosmic ray primaries by the moon and sun was observed by the MINOS far detector at a depth of 2070 mwe using 83.54 million cosmic ray muons accumulated over 1857.91 live-days. The shadow of the moon was detected at the 5.6 sigma level and the shadow of the sun at the 3.8 sigma level using a log-likelihood search in celestial coordinates. The moon shadow was used to quantify the absolute astrophysical pointing of the detector to be 0.17 +/- 0.12 degrees. Hints of interplanetary magnetic field effects were observed in both the sun and moon shadow. Published by Elsevier B.V.

Universal Experimental Measurement System «Sun-Walker» : Automotive measurement system for the evaluation of the solar irradiation distribution for the tests of the solar concentrated systems.

This Thesis project is a part of the research conducted in Solar industry. ABSOLICON Solar Concentrator AB has invented and started production of the prospective solar concentrated system Absolicon X10. The aims of this Thesis project are designing, assembling, calibrating and putting in operation the automatic measurement system intended to evaluate distribution of density of solar radiation in the focal line of the concentrated parabolic reflectors and to measure radiation from the artificial source of light being a calibration-testing tool.On the basis of the requirements of the company’s administration and needs of designing the concentrated reflectors the operation conditions for the Sun-Walker were formulated. As the first step, the complex design of the whole system was made and division on the parts was specified. After the preliminary conducted simulation of the functions and operation conditions of the all parts were formulated.As the next steps, the detailed design of all the parts was made. Most components were ordered from respective companies. Some of the mechanical components were made in the workshop of the company. All parts of the Sun-Walker were assembled and tested. The software part, which controls the Sun-Walker work and conducts measurements of solar irradiation, was created on the LabVIEW basis. To tune and test the software part, the special simulator was designed and assembled.When all parts were assembled in the complete system, the Sun-Walker was tested, calibrated and tuned.

Han, hon, höna? : En kvantitativ studie om attityder till det könsneutrala personliga pronomenet hen

Språk både reflekterar och påverkar vår världssyn. Hur mottas då försök från gräsrotsnivå att introducera ett könsneutralt pronomen i ett språk som speglar den i samhället rådande könsdikotomin? Syftet med denna uppsats är att utifrån Hirdmans och Butlers respektive genusteorier undersöka vilken inställning användare på ett stort svenskt internetforum har till det könsneutrala personliga pronomenet hen. Undersökningen genomfördes med hjälp av en internetbaserad enkät som besvarades av cirka 150 personer. För att analysera svaren till de slutna frågorna tog vi hjälp av statistikprogrammet SPSS och för att bearbeta de öppna frågorna har vi använt oss av en tematisk analys. Resultatet visar på starkt polariserade åsikter runt hen, där ungefär lika många personer är för som emot ordet. Bland dem som är emot användandet av hen uppfattar de flesta att syftet med ordet är att skapa ett könslöst samhälle, medan hen-förespråkarna ser det som ett komplement till hon och han. Vi har även kunnat se att det finns ett visst samband mellan individens attityd till hen och dennes syn på kön och genus, vilket bekräftar vår hypotes om att det finns en sådan korrelation.

Interview with Louise "Lou" Trucks

In her December 2014 interview with Michelle Dubert-Bellrichard, Louise “Lou” Trucks detailed her thoughts and memories of her time at Winthrop. Trucks spoke of the time period from 1960-1964 as a music and music education double major. Trucks shared the benefits of being a music major, her involvement in campus traditions and organizations, and the rigor of her studies. Trucks concludes her interview detailing her life after Winthrop in Bloomington, IN and Rochester, NY. This interview was conducted for inclusion into the Louise Pettus Archives and Special Collections Oral History Program.

Extração com CO2 supercrítico de óleos essenciais de Hon-sho e Ho-sho : experimentos e modelagem

Uma das tecnologias que mais avançou nas últimas décadas, como uma alternativa para as tradicionais técnicas de extração de produtos naturais, é a técnica de Extração com Fluidos Supercríticos. A extração com fluidos supercríticos destacase entre os processos industriais de extração pela qualidade dos produtos obtidos e por não causar danos ambientais quando usa dióxido de carbono (CO2) no estado supercrítico como solvente. Este trabalho teve como objetivo a realização de experimentos de extração de óleos essenciais com dióxido de carbono no estado supercrítico de folhas de duas variedades da árvore Canforeira (Cinnamomum camphor Ness & Eberm.) conhecidas como Hon-sho e Ho-sho, a fim de determinar as melhores condições operacionais de processo. Os óleos essenciais obtidos destas plantas têm importância econômica devido aos seus principais componentes: linalol e cânfora. Os melhores parâmetros de extração obtidos, quando se consideram os rendimentos de óleo essencial, foram os seguintes: vazão de CO2 = 2 mL/min, temperatura = 50°C, pressão = 90 bar e diâmetro de partícula = 0,1 mm. Outro objetivo foi a obtenção das curvas de extração: Rendimento de óleo essencial versus Tempo de extração, adequando, a partir dos dados experimentais, alguns modelos matemáticos encontrados na literatura para descrever o comportamento destas extrações. Dos modelos estudados o que melhor se adequou à extração de óleos essenciais de folhas foi o modelo proposto por Reverchon (1996), o qual proporcionou uma boa reprodutibilidade dos dados experimentais, mostrandose eficiente na representação de extração com fluidos supercríticos de óleos essenciais de Hon-sho e Ho-sho a partir de suas folhas.

Beyond sea, sun and fun in Rio de Janeiro: understanding exchange students motivations and interests

O objetivo deste estudo é compreender o que leva estudantes de intercâmbio ao Rio de Janeiro, quais são suas motivações e interesses que influenciam na escolha dessa cidade, um destino pouco tradicional para intercâmbios, que recebe um crescente número de intercambistas de países desenvolvidos. Também apresentamos uma discussão mais ampla sobre a educação internacional do século 21, posicionando programas de intercâmbio como uma das possíveis iniciativas para a internacionalização de instituições de ensino superior. Para responder essa questão, 20 estudantes de 11 países foram entrevistados. Os resultados indicam que existe muito mais no Rio de Janeiro além do sol e das belas praias. Há uma grande variedade de interesses que explicam porque estudantes de intercâmbio escolhem esse destino. O clichê sobre sol, praia e carnaval se manifestou em diversas respostas, no entanto, nunca como principal fator. Intercambistas se interessam pela cidade por diversos motivos além das atrações turísticas, como aprender português, melhorar o currículo e estar em uma economia emergente. Recomendações para a internacionalização de instituições de educação e uma agenda de pesquisa para o desenvolvimento desse tópico são apresentadas na parte final.

Automated system of seedling image analysis (SVIS) and electrical conductivity to assess sun hemp seed vigor

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

Nonsphericity of the Moon and Near Sun-Synchronous Polar Lunar Orbits

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