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Relevant bibliographies by topics / Top Arcade

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Journal articles

Academic literature on the topic 'Top Arcade'

Author: Grafiati

Published: 4 June 2021

Last updated: 15 February 2022

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Journal articles on the topic "Top Arcade"

1

Fang, X., C. Xia, and R. Keppens. "Modeling Prominence Formation in 2.5D." Proceedings of the International Astronomical Union 8, S300 (2013): 410–11. http://dx.doi.org/10.1017/s1743921313011319.

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AbstractWe use a 2.5-dimensional, fully thermodynamically and magnetohydrodynamically compatible model to imitate the formation process of normal polarity prominences on top of initially linear force-free arcades above photospheric neutral lines. In magnetic arcades hosting chromospheric, transition region, and coronal plasma, we perform a series of numerical simulations to do a parameter survey for multi-dimensional evaporation-condensation prominence models. The investigated parameters include the fixed angle of the magnetic arcade, the strength and spatial range of the localized chromospher

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2

Sherman, R. L. "Examination of Structural Differences in Gill Vasculature Among Some Batiod Elasmobranchs Using Corrosion Casting and SEM." Microscopy and Microanalysis 7, S2 (2001): 1208–9. http://dx.doi.org/10.1017/s1431927600032116.

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Classic studies of gill vasculature indicate the gross anatomy of elasmobranch gills is similar in most species, and in general, resembles those of teleosts. However, studies of fine gill structure examining arterio-arterial pathways in several species of batoid elasmobranchs (Order: Rajiiformes, Suborder: Myliobatoidei) have reported some structural differences. These differences include the presence, in urolophids (Urolophus jamaicensis, U. mucosus, U. paucimaculatus), of 1) a tip channel, possibly an extension of the afferent filament artery that runs along the top of the filament corpus ca

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3

Hosteaux, S., E. Chané, B. Decraemer, D. C. Talpeanu, and S. Poedts. "Ultrahigh-resolution model of a breakout CME embedded in the solar wind." Astronomy & Astrophysics 620 (November 30, 2018): A57. http://dx.doi.org/10.1051/0004-6361/201832976.

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Aims. We investigate the effect of a background solar wind on breakout coronal mass ejections, in particular, the effect on the different current sheets and the flux rope formation process. Methods. We obtained numerical simulation results by solving the magnetohydrodynamics equations on a 2.5D (axisymmetric) stretched grid. Ultrahigh spatial resolution is obtained by applying a solution adaptive mesh refinement scheme by increasing the grid resolution in regions of high electrical current, that is, by focussing on the maximum resolution of the current sheets that are forming. All simulations

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4

Tiyaworanan, Piyapong, Surut Jianmongkol, and Tala Thammaroj. "ANATOMICAL STUDY OF ARCADE OF STRUTHERS." Hand Surgery 15, no. 03 (2010): 157–59. http://dx.doi.org/10.1142/s0218810410004941.

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The incidence and the anatomical location of the arcade of Struthers as related to the arm length were studied in 62 arms of adult fresh-frozen cadavers. The distance between the greater tuberosity and the lateral epicondyle was designated as the arm length. The arcades of Struthers were identified in 85.4%. The mean arm length was 27.85 ± 1.3 cm. The mean of the distance between proximal border of the arcade of Struthers and the medial humeral epicondyle was 8.24 ± 2.06 cm. The mean ratio between the distance from the proximal border of the arcade to the tip of the medial epicondyle and arm l

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5

Schmit, Donald, and Sarah Gibson. "The Formation of a Cavity in a 3D Flux Rope." Proceedings of the International Astronomical Union 8, S300 (2013): 147–50. http://dx.doi.org/10.1017/s1743921313010880.

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AbstractThere are currently no three dimensional numerical models which describe the magnetic and energetic formation of prominences self-consistently. Consequently, there has not been significant progress made in understanding the connection between the dense prominence plasma and the coronal cavity. We have taken an ad-hoc approach to understanding the energetic implications of the magnetic models of prominence structure. We extract one dimensional magnetic field lines from a 3D MHD model of a flux rope and solve for hydrostatic balance along these field lines incorporating field-aligned the

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6

Sharma, Rohit, Durgesh Tripathi, Hiroaki Isobe, and Avyarthana Ghosh. "ON THE BRIGHT LOOP TOP EMISSION IN POST-ERUPTION ARCADES." Astrophysical Journal 823, no. 1 (2016): 47. http://dx.doi.org/10.3847/0004-637x/823/1/47.

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7

Pedersoli, Federico, Markus Zimmermann, Maximilian Schulze-Hagen, et al. "Retrograde Recanalization of the Celiac Artery via the Pancreaticoduodenal Arcade as a Safe and Valid Alternative to Antegrade Access." Vascular and Endovascular Surgery 54, no. 6 (2020): 477–81. http://dx.doi.org/10.1177/1538574420927132.

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Purpose: The antegrade recanalization of an occlusion or high-grade stenosis of the celiac artery via the aorta often represents a technical challenge. A retrograde approach via the superior mesenteric artery and the pancreaticoduodenal arcade may be an alternative approach. Based on our experience, we assess the technical success and the short- and mid-term outcomes of this bailout procedure. Methods: We performed a retrospective analysis of all consecutive patients who underwent recanalization and stent implantation in the celiac artery between January 2010 and December 2018. Data on vascula

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8

Cheng, C. Z., and G. S. Choe. "Formation of Thin Current Sheets in the Solar Atmosphere." International Astronomical Union Colloquium 167 (1998): 115–18. http://dx.doi.org/10.1017/s0252921100047400.

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AbstractIn a two-dimensional quadrupolar magnetic field geometry, it is demonstrated that various magnetohydrostatic equilibrium field configurations containing current sheets can be formed either by changes in thermal properties or by footpoint displacement. The shape of current sheets depends on the mass distribution in flux tubes. If the mass per flux tube is maximum at the center of the low-lying bipolar arcades, a current sheet is formed between these two arcades along the separatrix line as the plasma temperature (or the shearing footpoint displacement) is increased above a critical valu

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9

Bartholomew, Ryan, Joseph Zenga, Derrick Lin, Daniel Deschler, and Jeremy Richmon. "Tip-on-Tip Scapular (TOTS) Flap for Reconstruction of Combined Palatectomy and Rhinectomy Defects." Facial Plastic Surgery 34, no. 04 (2018): 389–93. http://dx.doi.org/10.1055/s-0038-1666784.

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AbstractCombination anterior palatectomy and rhinectomy defects result in complete loss of midface and nasal support and present a significant reconstructive challenge. A novel use of the scapular tip free flap—the tip-on-tip scapula flap—was developed to provide both palatal repair and restoration of intrinsic nasal support. The scapular tip bone is split into a large proximal segment for the anterior palate and a smaller distal bone segment for nasal framework reconstruction. Two patients undergoing reconstruction of both total palatectomy and partial rhinectomy defects at a single academic

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10

Tsuneta, Saku. "Solar Flares as an Ongoing Magnetic Reconnection Process." International Astronomical Union Colloquium 141 (1993): 239–48. http://dx.doi.org/10.1017/s025292110002916x.

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AbstractThe soft X-ray images taken by the Yohkoh Soft X-ray Telescope (SXT) provide a powerful new tool to solve the mechanism of solar flares. In particular, a limb flare that occurred on 1991, December 2 gives us convincing evidence that magnetic reconnection of a neutral sheet formed at the loop top participates in the flare energy release. The neutral sheet appears to be associated with a destabilized rising loop system (filament) sheared with respect to the flaring loop. Similar formations of X-ray arcades are seen in the quiet Sun associated with filament eruptions on much larger spatia

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