In Situ Distance Tunneling Spectroscopy at Au(111)/0.02 M HClO[sub 4]

2004 ◽  
Vol 151 (3) ◽  
pp. E97 ◽  
Author(s):  
Martin Hugelmann ◽  
Werner Schindler
2005 ◽  
Vol 109 (13) ◽  
pp. 6262-6267 ◽  
Author(s):  
Philipp Hugelmann ◽  
Werner Schindler

2011 ◽  
Vol 11 (7) ◽  
pp. 6368-6370
Author(s):  
Hyun-Won Lee ◽  
Kyujoon Lee ◽  
Seongmin Choo ◽  
Nahyun Jo ◽  
Myung-Hwa Jung

2008 ◽  
Vol 8 (7) ◽  
pp. 3616-3620 ◽  
Author(s):  
K. Schouteden ◽  
D. A. Muzychenko ◽  
C. Van Haesendonck

Magnetic monolayer and bilayer Co islands of only a few nanometer in size were grown by atomic deposition on atomically flat Au(111) films. The islands were studied in situ by scanning tunneling microscopy (STM) and spectroscopy at low temperatures. Spin-resolved tunneling spectroscopy, using an STM tip with a magnetic coating, revealed that the Co islands exhibit a net magnetization perpendicular to the substrate surface due to the presence of spin-polarized d-states. A random distribution of islands with either upward or downward pointing magnetization was observed, without any specific correlation of magnetization orientation with island size or island height.


Langmuir ◽  
2006 ◽  
Vol 22 (6) ◽  
pp. 2426-2429 ◽  
Author(s):  
Emil Wierzbinski ◽  
Justin Arndt ◽  
William Hammond ◽  
Krzysztof Slowinski

1984 ◽  
Vol 75 ◽  
pp. 743-759 ◽  
Author(s):  
Kerry T. Nock

ABSTRACTA mission to rendezvous with the rings of Saturn is studied with regard to science rationale and instrumentation and engineering feasibility and design. Future detailedin situexploration of the rings of Saturn will require spacecraft systems with enormous propulsive capability. NASA is currently studying the critical technologies for just such a system, called Nuclear Electric Propulsion (NEP). Electric propulsion is the only technology which can effectively provide the required total impulse for this demanding mission. Furthermore, the power source must be nuclear because the solar energy reaching Saturn is only 1% of that at the Earth. An important aspect of this mission is the ability of the low thrust propulsion system to continuously boost the spacecraft above the ring plane as it spirals in toward Saturn, thus enabling scientific measurements of ring particles from only a few kilometers.


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