نتایج جستجو برای: Midplane

تعداد نتایج: 697  

A. Sharafi, A. Shirazi, Gh. Geraily, M. Allahverdi, M. Esfehani,

Background: Total Body Irradiation (TBI) is different from standard radiotherapy in many aspects, so it is not easy to predict the delivered dose to the patient under TBI treatment. Diode dosimetry procedures for surface dose reading can help to define variations of the actually delivered dose from the prescribed one. The aim of this study was to describe the measurements made to calib...

1993
Douglas N. Arnold

In this work-in-progress we report on a new approach to obtaining stable locking-free discretizations of the Reissner–Mindlin plate model. For a plate of thickness t with midplane section Ω ⊂ R the clamped Reissner–Mindlin plate model determines ω , the transverse displacement of the midplane, and φ , the rotation of fibers normal to the midplane, as the unique minimizer over H̊1(Ω)× H̊(Ω) of the...

Journal: :iranian journal of radiation research 0
m. allahverdi department of medical physics, tehran university of medical sciences, tehran, iran gh. geraily department of medical physics, tehran university of medical sciences, tehran, iran m. esfehani departments of radiology, iran university of medical sciences, tehran, iran a. sharafi department of radiotherapy and oncology, cancer institute, tehran university of medical sciences, tehran, iran a. shirazi department of medical physics, tehran university of medical sciences, tehran, iran

background: total body irradiation (tbi) is different from standard radiotherapy in many aspects, so it is not easy to predict the delivered dose to the patient under tbi treatment. diode dosimetry procedures for surface dose reading can help to define variations of the actually delivered dose from the prescribed one. the aim of this study was to describe the measurements made to calibrate diod...

2005
Cecilia Ceccarelli Carsten Dominik

Probing the gas and dust in proto-planetary disks is central for understanding the process of planet formation. In disks surrounding solar type protostars, the bulk of the disk mass resides in the outer midplane, which is cold (≤20 K), dense (≥ 107 cm−3) and depleted of CO. Observing the disk midplane has proved, therefore, to be a formidable challenge. Ceccarelli et al. (2004) detected H2D emi...

Journal: :IBM Journal of Research and Development 2005
James E. Hughes Pravin S. Patel Ivan R. Zapata Thomas D. Pahel Jack P. Wong Dhruv M. Desai Bradley D. Herrman

This paper describes the electrical architecture and design of the IBM eServere BladeCentert midplane and media interface card. The midplane provides the redundant interconnects among processor blades, switch modules, media interface card, and management modules. It also serves as the redundant power distribution medium from the power modules to all blades and other devices. A major attribute o...

2011
E. Chapillon S. Guilloteau F. Du

Context. The structure in density and temperature of protoplanetary disks surrounding low-mass stars is not well known yet. The protoplanetary disks’ midplane are expected to be very cold and thus depleted in molecules in gas phase, especially CO. Recent observations of molecules at very low apparent temperatures (∼6 K) challenge this current picture of the protoplanetary disk structures. Aims....

2017
Evelina Ametova Massimiliano Ferrucci Wim Dewulf

Abstract Cone-beam computed tomography (CT) with circular scanning trajectory is known to suffer from so called cone-beam artifacts. Cone-beam artifacts are errors in the reconstructed volume due to incomplete radon data. These artifacts increase with increasing distance of the reconstructed plane from the midplane, i.e. the plane containing the X-ray source. Theoretically, the midplane represe...

2008
Hiroshi Koyama Eve C. Ostriker

We use numerical simulations of turbulent, multiphase, self-gravitating gas orbiting in the disks of model galaxies to study the relationships among pressure, the vertical distribution of gas, and the relative proportions of dense and diffuse gas. A common assumption is that the interstellar medium (ISM) is in vertical hydrostatic equilibrium. We show that the disk height and mean midplane pres...

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