In situ-XAS and catalytic study of acrolein hydrogenation over silver
... has been found in a pressure range from 20 bar down to 7.5 mbar, which is displayed in Fig. 1 for the silica supported silver catalyst. The values of Fig. 1 have been obtained from the three different set-ups. A more detailed investigation of the pressure dependence has revealed that, at least for t ...
... has been found in a pressure range from 20 bar down to 7.5 mbar, which is displayed in Fig. 1 for the silica supported silver catalyst. The values of Fig. 1 have been obtained from the three different set-ups. A more detailed investigation of the pressure dependence has revealed that, at least for t ...
Low-energy charged particle measurement by MAP-PACE onboard SELENE
... inside the mass analyzer and their positions are detected by one-dimensional circular resistive anode that is placed behind the MCP. These start electrons also generate start signals when they pass through a grid anode that is placed between the position-sensitive anode and the MCP. Most of the ions ...
... inside the mass analyzer and their positions are detected by one-dimensional circular resistive anode that is placed behind the MCP. These start electrons also generate start signals when they pass through a grid anode that is placed between the position-sensitive anode and the MCP. Most of the ions ...
L and T Dwarfs - Indiana University
... Better spatial resolution (seeing improvements, AO) IR and multi-color surveys (2MASS, DENIS, and Sloan) Breakthrough in understanding appearance of spectra ...
... Better spatial resolution (seeing improvements, AO) IR and multi-color surveys (2MASS, DENIS, and Sloan) Breakthrough in understanding appearance of spectra ...
The Sun The Sun is a very typical main sequence star. It contains 1000
... supplementary notes for more detail. Results from solar models are shown below. All energy genera9on through nuclear reac9ons occurs within the inner 20 % of the radius, where the temperature is high e ...
... supplementary notes for more detail. Results from solar models are shown below. All energy genera9on through nuclear reac9ons occurs within the inner 20 % of the radius, where the temperature is high e ...
Slide 1 - Experimental Elementary Particle Physics Group
... Nov. 2011 - successful “Lehman” review of the camera project; in preparation for requesting CD-1 approval Feb 2012 – CD-1 approval meeting held with Dr. Pat Dehmer. She plans to recommend that Dr. Brinkman sign the CD-1 approval after briefing him in next few weeks. Feb 2012 – FY13 President’s Reque ...
... Nov. 2011 - successful “Lehman” review of the camera project; in preparation for requesting CD-1 approval Feb 2012 – CD-1 approval meeting held with Dr. Pat Dehmer. She plans to recommend that Dr. Brinkman sign the CD-1 approval after briefing him in next few weeks. Feb 2012 – FY13 President’s Reque ...
Clathrates - An Exploration of the Chemistry of Caged Compounds
... Na gSi46, Nax Si 136 (X= 1-24) etc. are formed. Rb+ and Cs+ are too large to be incorporated into the cages of Si and Ge. Sn, however, forms clathrates with Rb + and Cs +yielding solids like RbzCS6 Sn46, Cs gSn46, K1.6CS6.4Sn44 and others. Figure 5 shows the inorganic clathrate structure. Inorganic ...
... Na gSi46, Nax Si 136 (X= 1-24) etc. are formed. Rb+ and Cs+ are too large to be incorporated into the cages of Si and Ge. Sn, however, forms clathrates with Rb + and Cs +yielding solids like RbzCS6 Sn46, Cs gSn46, K1.6CS6.4Sn44 and others. Figure 5 shows the inorganic clathrate structure. Inorganic ...
Chapter 5 Nuclear reactions in stars
... Chapter 11 of K&W. The main purpose of this chapter is to briefly analyse the differential equations of stellar evolution and their boundary conditions, and to see how the full set of equations can be simplified in some cases to allow simple or approximate solutions - so-called simple stellar models ...
... Chapter 11 of K&W. The main purpose of this chapter is to briefly analyse the differential equations of stellar evolution and their boundary conditions, and to see how the full set of equations can be simplified in some cases to allow simple or approximate solutions - so-called simple stellar models ...
The current status of ”Troitsk nu-mass”
... experiment are the Windowless Gaseous Tritium Source (WGTS) and the Electrostatic Spectrometer with Magnetic Adiabatic Collimation (ESMAC). Gaseous source, while being very complex to manufacture and maintain, is needed to avoid solid state effects such as source charging, neighbor excitation and ba ...
... experiment are the Windowless Gaseous Tritium Source (WGTS) and the Electrostatic Spectrometer with Magnetic Adiabatic Collimation (ESMAC). Gaseous source, while being very complex to manufacture and maintain, is needed to avoid solid state effects such as source charging, neighbor excitation and ba ...
The Energy of Electron Affinity to a Zirconium Atom
... S2. Then for the second set we carried out a calculation by the determinant PT method with the initial approximation corresponding to the set S1. This allowed us to determine the error of the PT for the set S2 (see Tables 1 and 2). The first basis set S1 for Zr included one-, two-, and three-particl ...
... S2. Then for the second set we carried out a calculation by the determinant PT method with the initial approximation corresponding to the set S1. This allowed us to determine the error of the PT for the set S2 (see Tables 1 and 2). The first basis set S1 for Zr included one-, two-, and three-particl ...
Microplasma
Microplasmas are plasmas of small dimensions, ranging from tens to thousands of micrometers. They can be generated at a variety of temperatures and pressures, existing as either thermal or non-thermal plasmas. Non-thermal microplasmas that can maintain their state at standard temperatures and pressures are readily available and accessible to scientists as they can be easily sustained and manipulated under standard conditions. Therefore, they can be employed for commercial, industrial, and medical applications, giving rise to the evolving field of microplasmas.