3D and Spatiotemporal Interpolation in Object and Surface Formation

2011 ◽  
pp. 183-207 ◽  
Author(s):  
Philip Kellman ◽  
Patrick Garrigan ◽  
Evan Palmer
Keyword(s):  
Surface Formation ◽  
Spatiotemporal Interpolation

Spatiotemporal Interpolation of High Frequency Irradiance Data for Inverter Testing

2021 ◽  
Author(s):  
Sophie Pelland ◽  
Alexandre Gagne ◽  
Mahmoud A. Allam ◽  
Dave Turcotte ◽  
Nayeem Ninad
Keyword(s):  
High Frequency ◽  
Spatiotemporal Interpolation ◽  
Irradiance Data

Thermodynamic Quantities of Surface Formation of Aqueous Electrolyte Solutions

1999 ◽  
Vol 209 (2) ◽  
pp. 403-407 ◽  
Author(s):  
Norihiro Matubayasi ◽  
Shin-ichiro Yamaguchi ◽  
Kazuo Yamamoto ◽  
Hideyuki Matsuo
Keyword(s):  
Aqueous Electrolyte ◽  
Electrolyte Solutions ◽  
Thermodynamic Quantities ◽  
Surface Formation ◽  
Aqueous Electrolyte Solutions

scholarly journals Subantarctic Mode Water Formation, Destruction, and Export in the Eddy-Permitting Southern Ocean State Estimate

2013 ◽  
Vol 43 (7) ◽  
pp. 1485-1511 ◽  
Author(s):  
Ivana Cerovečki ◽  
Lynne D. Talley ◽  
Matthew R. Mazloff ◽  
Guillaume Maze
Keyword(s):  
Southern Ocean ◽  
Buoyancy Flux ◽  
Differential Heat ◽  
Diapycnal Mixing ◽  
Mode Water ◽  
State Estimate ◽  
Surface Formation ◽  
Subantarctic Mode Water ◽  
The Pacific ◽  
The Difference

Abstract Subantarctic Mode Water (SAMW) is examined using the data-assimilating, eddy-permitting Southern Ocean State Estimate, for 2005 and 2006. Surface formation due to air–sea buoyancy flux is estimated using Walin analysis, and diapycnal mixing is diagnosed as the difference between surface formation and transport across 30°S, accounting for volume change with time. Water in the density range 26.5 < σθ < 27.1 kg m−3 that includes SAMW is exported northward in all three ocean sectors, with a net transport of (18.2, 17.1) Sv (1 Sv ≡ 106 m3 s−1; for years 2005, 2006); air–sea buoyancy fluxes form (13.2, 6.8) Sv, diapycnal mixing removes (−14.5, −12.6) Sv, and there is a volume loss of (−19.3, −22.9) Sv mostly occurring in the strongest SAMW formation locations. The most vigorous SAMW formation is in the Indian Ocean by air–sea buoyancy flux (9.4, 10.9) Sv, where it is partially destroyed by diapycnal mixing (−6.6, −3.1) Sv. There is strong export to the Pacific, where SAMW is destroyed both by air–sea buoyancy flux (−1.1, −4.6) Sv and diapycnal mixing (−5.6, −8.4) Sv. In the South Atlantic, SAMW is formed by air–sea buoyancy flux (5.0, 0.5) Sv and is destroyed by diapycnal mixing (−2.3, −1.1) Sv. Peaks in air–sea flux formation occur at the Southeast Indian and Southeast Pacific SAMWs (SEISAMWs, SEPSAMWs) densities. Formation over the broad SAMW circumpolar outcrop windows is largely from denser water, driven by differential freshwater gain, augmented or decreased by heating or cooling. In the SEISAMW and SEPSAMW source regions, however, formation is from lighter water, driven by differential heat loss.

Atomically flat diamond (100) surface formation by anisotropic etching of solid-solution reaction of carbon into nickel

2016 ◽  
Vol 68 ◽  
pp. 127-130 ◽  
Author(s):  
Kazuhiro Nakanishi ◽  
Hiroki Kuroshima ◽  
Tsubasa Matsumoto ◽  
Takao Inokuma ◽  
Norio Tokuda
Keyword(s):  
Solid Solution ◽  
Anisotropic Etching ◽  
Surface Formation ◽  
Solution Reaction ◽  
Atomically Flat

On-Surface Formation of Metal Nanowire Transparent Top Electrodes on CdSe Nanowire Array-Based Photoconductive Devices

2012 ◽  
Vol 4 (6) ◽  
pp. 3157-3162 ◽  
Author(s):  
Daniel Azulai ◽  
Uri Givan ◽  
Nava Shpaisman ◽  
Tatyana Levi Belenkova ◽  
Hagit Gilon ◽  
...  
Keyword(s):  
Nanowire Array ◽  
Surface Formation ◽  
Metal Nanowire
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