«ULTRAHEAVY»に関連する英語の本
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1
Opportunities in Cosmic-ray Physics and Astrophysics
Ultraheavy isotopes are particularly favorable from this point of view since the
rapid fall-off of abundances with increasing atomic number also means that there
are few parent nuclei from which spallation products can be made (see Figure
2.2) ...
2
Origin of Matter and Evolution of Galaxies 2000
[A] Spectrometer for Ultraheavy Nuclear Composition (SUNC) Telescope SUNC
is a large area Si-Cerenkov detector telescope (Fig. la) which measure the
elemental composition of heavy cosmic ray particles with relativistic velocity,
especially ...
3
Astronomy and Astrophysics:: Space Science in the ...
Examples include measurements of cosmic-ray positrons and antiprotons from
0.1 to approximately 4 GeV and measurements of the isotopic composition of
ultraheavy nuclei (Z > 30). The ultraheavy isotope measurements are considered
in ...
Space Science Board, Task Group on Astronomy and Astrophysics, National Research Council, 1988
4
Shim 89: Proceedings of the First International Symposium on ...
Reprints availahle directly from the puhlisher Photocopying permitted riy license
only Printed in Great Britain RANGE AND ENERGY LOSS OF ULTRAHEAVY
IONS IN SOLID STATE NUCLEAR TRACK DETECTORS C. DOMINGO, ...
5
Sulfur Oxides—Advances in Research and Application: 2013 ...
Furthermore, because the SO.sub.2 concentration in flue gas of such ultraheavy
oil is very high, there is a problem that a vanadium compound becomes
deposited on a surface of the NO.sub.x removal catalyst during an operation. “
Particularly ...
6
Gravitation, Cosmology, and Cosmic-Ray Physics
Ultraheavy Elements The quantitative study of ultraheavy (atomic number greater
than 30) nuclei has begun with the HEAO-3 satellite. Individual element
abundances have been measured for elements of even atomic number up to
about 60.
Panel on Gravitation, Cosmology, and Cosmic-Ray Physics, Physics Survey Committee, Board on Physics and Astronomy, 1986
7
Nuclear Tracks in Solids: Principles and Applications
As a by-product of their studies of ultraheavy cosmic rays, using plastic detectors,
Blanford et al. (1972) have detected low-energy heavy cosmic rays at a
geomagnetic latitude at which such particles in the primary radiation are
excluded by the ...
Robert Louis Fleischer, Paul Buford Price, Robert M. Walker, 1975
8
The Higgs Boson: Searching for the God Particle
Butitalso requires the existence of ultraheavy particles, called grand unified
particles, that have amass of about 10 16 GeV (1 GeV, roughly themass ofa
proton,isa billion electron volts). Among other interactions, these ultraheavy
particlesallow ...
Scientific American Editors, 2012
Theheart of Nakajima's proposed strategy relied on a high performance
ultraheavy bomber to be manufactured by his aircraftcompany, the 'Fugaku (
Mount Fuji)'. Prior to the disclosure ofthe projectstrategy, inearly1943, all of
Nakajima's ...
10
The Explorer Program for Astronomy and Astrophysics
This experiment will increase the total exposure for ultraheavy cosmic rays by
more than an order of magnitude, and will individually resolve elements as heavy
as uranium. It will be able to determine the relative contributions of r-process and
...
National Research Council (U.S.). Committee on Space Astronomy and Astrophysics, 1986
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Two Ultraheavy Elements Added to Periodic Table
A committee of international chemists and physicists has officially added two new elements to the periodic table: the ultraweighty elements 114 and 116. [partner ... «Wired News, 6月 11»
Acergy readies first Schilling UHD ROVs for deployment
Acergy has taken delivery of its first two ultraheavy-duty ROV systems from Schilling Robotics' Acergy Core Vehicle (ACV) line. Five additional ACV systems are ... «Offshore Shipping Online, 4月 07»
