نتایج جستجو برای: umbra lagrangian

تعداد نتایج: 23332  

2013
Nicolás Buezas Esther Guerra Juan de Lara Javier Martín Miguel Monforte Fiorella Mori Eva Ogallar Oscar Pérez Jesús Sánchez Cuadrado

Almira Labs is a software company that develops valueadded services for the telecommunications industry. It is focused on innovative technologies that enable enterprise business and mobile and landline operators to offer next-generation voice-driven applications for all types of phones. Telephony services are built atop the proprietary Umbra framework, which is a Java API relying on the JAIN SL...

1999
M. Sobotka P. N. Brandt

The properties of penumbral grains (PGs) in a medium-size sunspot are studied from a 4.5 hour observation series acquired on 5 June 1993 at the Swedish Vacuum Solar Telescope, La Palma. The application of an image segmentation procedure and a feature tracking algorithm on a movie of 360 frames yields proper motions, intensities, and lifetimes for a set of 469 PGs. Almost 3/4 of the PGs move tow...

Journal: :Astronomy and Astrophysics 2021

Context. The sunspot umbra harbours the coolest plasma on solar surface due to presence of strong magnetic fields. atomic lines that are routinely used observe photosphere have weak signals in and often swamped by molecular lines. This makes it harder infer properties umbra, especially darkest regions.

Journal: :Anuário de Literatura 2022

Nesse artigo, o poema em prosa "Umbra”, de João da Cruz e Sousa (2008 [1891]), é tomado como epítome do espaço urbano derruído, reportando-o a Charles Baudelaire ao pós-simbolista “Sub-umbra”, Artur Sales (1987 [1950]), enunciação estranhamento saturnino (Giorgio Agamben) renúncia (Paul Valéry) justaposição conceito “fugacidade eterna” (BENJAMIN, 2006). Nessa dialética, imagem afloramento calcá...

2007
C. Emde B. Mayer

A solar eclipse is a rare but spectacular natural phenomenon and furthermore it is a challenge for radiative transfer modelling. Whereas a simple one-dimensional radiative transfer model with reduced solar irradiance at the top of the atmosphere can be used to calculate the brightness during partial eclipses a much more sophisticated model is required to calculate the brightness (i.e. the diffu...

Journal: :journal of sciences, islamic republic of iran 2011
n. elyasi

in this paper mathematical structure of time-dependent lagrangian systems and their symmetries are extended and the explicit relation between constants of motion and infinitesimal symmetries of time-dependent lagrangian systems are considered. starting point is time-independent lagrangian systems ,then we extend mathematical concepts of these systems such as equivalent lagrangian systems to the...

Journal: :Comput. Graph. Forum 2006
Xiao-Hua Cai Yun-Tao Jia Xi Wang Shi-Min Hu Ralph R. Martin

Generating soft shadows in real-time is difficult. Exact methods (such as ray tracing, and multiple light source simulation) are too slow, while approximate methods often over-estimate the umbra regions. In this paper, we introduce a new algorithm based on the shadow map method to quickly and accurately render soft shadows produced by a light source. Our method builds inner and outer translucen...

Journal: :Astronomy and Astrophysics 2021

Context. It is unclear why there a rather sharp boundary in sunspots between the umbra and penumbra. Both regions exhibit magnetoconvection, which manifests penumbral filaments penumbra umbral dots umbra. Aims. Here we compare physical properties of filaments. Our goal to understand how these convective features change across this related rapid increase brightness at umbra-penumbra boundary. Me...

1995
L. A. Gee M. A. Abidi

Image segmentation involves calculating the position of object boundaries. For scene analysis, the intent is to di erentiate objects from clutter by means of preprocessing. The objective of this paper is to examine and discuss two morphological techniques for preprocessing and segmenting range images. A MorphologicalWatershed Algorithm has been studied in detail for segmenting range images. Thi...

2008
H. Socas-Navarro

High-resolution imaging observations from the Hinode spacecraft in the Ca II H line are employed to study the dynamics of the chromosphere above a sunspot. We find that umbral flashes and other brightenings produced by the oscillation are extremely rich in fine structure, even beyond the resolving limit of our observations (0.22”). The umbra is tremendously dynamic, to the point that our time c...

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