3D characterization of the magnetic response of the Aimorés Intrusive Complex (Brazil) aiming to identify similarities with impact craters

Author(s):  
Maria Oliveira ◽  
Aline Melo ◽  
Marcos Vasconcelos ◽  
Mariana Bandeira
Polymer ◽  
2017 ◽  
Vol 118 ◽  
pp. 68-74 ◽  
Author(s):  
Muhammad Nisar ◽  
Carlos Pérez Bergmann ◽  
Julian Geshev ◽  
Raúl Quijada ◽  
Griselda Barrera Galland

2012 ◽  
Vol 117 (E12) ◽  
pp. n/a-n/a ◽  
Author(s):  
Matthieu J. Talpe ◽  
Maria T. Zuber ◽  
Di Yang ◽  
Gregory A. Neumann ◽  
Sean C. Solomon ◽  
...  

1997 ◽  
Author(s):  
Michael J. Mazur ◽  
Robert R. Stewart ◽  
Hans‐Henrik Westbroek

2018 ◽  
Vol 47 (7) ◽  
pp. 3421-3429 ◽  
Author(s):  
X. A. Velásquez Moya ◽  
R. Cardona ◽  
J. I. Villa Hernández ◽  
D. A. Landínez Téllez ◽  
J. Roa-Rojas

Author(s):  
John R. Devaney ◽  
Kenneth Evans

There exists on the visible surface of the moon, a continuous range of impact craters from the very large to those below the resolution limits of terrestrial telescopes. The RANGER, SURVEYOR and LUNAR ORBITER programs extended the knowledge of existent craters down to those several centimeters in diameter. Prior to the actual examination of lunar material returned by the Apollo 11 mission, a debate was being carried on as to whether craters from hyper-velocity particles existed in the microscopic realm. Soon after the first samples were examined via Scanning Electron Microscopy, the point in question was settled with a definite affirmative.The initial effort in conjunction with Caltech scientist G. J. Wasserberg had as its goal the solution of two problems: (1) Can impact craters be differentiated from bubble bursts?(2) What are the characteristics of impact craters?To pursue the first problem initial efforts were designed to study samples with low possibility of bubbles or voids. This resulted in the examination of a chip of lunar feldspar with a large pit on its exposed surface.


1991 ◽  
Vol 69 (9) ◽  
pp. 6738-6740 ◽  
Author(s):  
A. Shaulov ◽  
R. Bhargava ◽  
S. Shatz
Keyword(s):  

2016 ◽  
Vol 42 (10) ◽  
pp. 11889-11900 ◽  
Author(s):  
D. Alonso-Domínguez ◽  
I. Álvarez-Serrano ◽  
M.L. López ◽  
Gabriel J. Cuello ◽  
Eloy Asensio ◽  
...  

2009 ◽  
Vol 4 (2) ◽  
pp. 79-83
Author(s):  
R. Zandonay ◽  
R. G. Delatorre ◽  
A. A. Pasa

Schottky diodes were prepared by photoinduced electrodeposition of Co on p-Si, probing the influence of different concentrations of CoSO4 (26 and 104 mM) in the electrolyte on the electrical properties of the metal-semiconductor interface. Current density versus voltage (JxV) and capacitance versus voltage (CxV) measurements were performed in diodes with different Co thicknesses to obtain the barrier heights and ideality factors. Atomic force microscopy (AFM) and vibrating sample magnetometry (VSM) were additional techniques used to determine the surface morphology and the magnetic response. Devices with improved electrical properties were observed by increasing the thickness of the metal, i. e., saturation currents with values of about 0.1 mA.cm-2, ideality factors close to 1.19 and barrier heights of about 0.65 eV were determined.


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