Metrology for gold absorber/silicon membrane x-ray reticles

1990 ◽  
Author(s):  
Bernard J. Dardzinski ◽  
Robert A. Grant ◽  
Daniel D. Ball
Keyword(s):  
X Ray ◽  
1991 ◽  
Author(s):  
Diane K. Stewart ◽  
Jacob Fuchs ◽  
Robert A. Grant ◽  
Irving Plotnik

1992 ◽  
Vol 17 (1-4) ◽  
pp. 189-192 ◽  
Author(s):  
R.E. Acosta ◽  
W.A. Johnson ◽  
B.S. Berry ◽  
W.C. Pritchet

1994 ◽  
Vol 23 (1-4) ◽  
pp. 235-238 ◽  
Author(s):  
W.J. Dauksher ◽  
D.J. Resnick ◽  
W.A. Johnson ◽  
A.W. Yanof
Keyword(s):  
X Ray ◽  

Author(s):  
Kwang-Cheol Lee ◽  
Seung S. Lee

We present a noval method of 3D microfabrication with LIGA process that utilizes a deep X-ray mask in which a microactuator is integrated. The integrated micro-actuator oscillates the X-ray absorber, which is formed on the shuttle mass of the micro-actuator, during X-ray exposures to modify that absorbed dose profile in X-ray resist, typically PMMA. 3D PMMA microstructures according to the modulated dose controur are revealed after GG development. An X-ray mask with integrated comb drive actuator is fabricated using deep reactive ion etching, absorber electroplating, and bulk micromachining with silicon-on-insulator wafer. 1 mm × 1 mm, 20 μm thick silicon shuttle mass as a mask blank is supported by four 1 mm long suspesnsion beams and is driven by the comb electrodes. A 10 μm thick, 50 μm line and spaced gold absorber pattern is electroplated on the shuttle mass before the release step. The fundamental frequency and arnplitured are around 3.6 kHz and 20 μm, respectively, for a dc bias of 100 V and an ac bias of 20 VP-P (peak-peak). Fabricated PMMA microstructure shows 15.4 μm deep, S-shaped cross section in the case of 1.6 kJ cm−3 surface dose and GG development at 35°C for 40 minutes.


1990 ◽  
Vol 29 (Part 1, No. 11) ◽  
pp. 2605-2609 ◽  
Author(s):  
B. Löchel ◽  
J. Chlebek ◽  
J. Grimm ◽  
H.-L. Huber ◽  
A. Macioßek

2021 ◽  
Vol 11 ◽  
pp. 184798042110561
Author(s):  
Cuong Tu Ho ◽  
Thuong Thuong Lam ◽  
Hanh Thi Nguyen ◽  
Canh Xuan Nguyen ◽  
Quang Le Dang ◽  
...  

The synthesis of CdS nanoparticles was developed based on the unconventional design of bioelectrochemical system (BES) inoculated with Shewanella sp. HN-41. The BES configuration included two bottle chambers separated by silicon membrane but directly connected by a graphite electrode perforating through silicon membrane, namely, non-external circuit bioelectrochemical system (nec_BES). Shewanella sp. HN-41 in the anode of nec_BES consumed lactate and transferred electrons to the graphite electrode end in the anode and, in its turn, the graphite electrode end in the cathode reduced directly thiosulfate to sulphide, forming CdS nanoparticles after 21 days. CdS nanoparticles with the average size of approximately 17 nm were synthesized in the cathode solution. The hollow, spherical, and void structure of particles was observed by transmission electron microscopy (TEM) and scanning electron microscopy (SEM) images. The energy dispersive X-ray spectroscopy (EDS) study confirmed the nanoparticles contained Cd and S elements, and X-ray diffraction (XRD) data showed a strong crystalline phase and mixed crystallites of CdS nanoparticles. The UV-Vis absorption spectra of CdS nanoparticles revealed the blue shift in excitonic transition with respect to CdS bulk material, suggesting its potential application in optical studies. The bioelectrochemical system can be applied for the removal and preparation of other sulphide heavy metals.


1994 ◽  
Vol 144 ◽  
pp. 275-277
Author(s):  
M. Karlický ◽  
J. C. Hénoux

AbstractUsing a new ID hybrid model of the electron bombardment in flare loops, we study not only the evolution of densities, plasma velocities and temperatures in the loop, but also the temporal and spatial evolution of hard X-ray emission. In the present paper a continuous bombardment by electrons isotropically accelerated at the top of flare loop with a power-law injection distribution function is considered. The computations include the effects of the return-current that reduces significantly the depth of the chromospheric layer which is evaporated. The present modelling is made with superthermal electron parameters corresponding to the classical resistivity regime for an input energy flux of superthermal electrons of 109erg cm−2s−1. It was found that due to the electron bombardment the two chromospheric evaporation waves are generated at both feet of the loop and they propagate up to the top, where they collide and cause temporary density and hard X-ray enhancements.


1994 ◽  
Vol 144 ◽  
pp. 1-9
Author(s):  
A. H. Gabriel

The development of the physics of the solar atmosphere during the last 50 years has been greatly influenced by the increasing capability of observations made from space. Access to images and spectra of the hotter plasma in the UV, XUV and X-ray regions provided a major advance over the few coronal forbidden lines seen in the visible and enabled the cooler chromospheric and photospheric plasma to be seen in its proper perspective, as part of a total system. In this way space observations have stimulated new and important advances, not only in space but also in ground-based observations and theoretical modelling, so that today we find a well-balanced harmony between the three techniques.


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