HO CHI MINH’S WORKING STYLE, SCIENTIFIC, OBJECTIVE AND HONEST

2020 ◽  
Vol 9 (6) ◽  
Author(s):  
Tho Le Duc
Keyword(s):  
2018 ◽  
Vol 44 ◽  
pp. 00061
Author(s):  
Anna Jurga ◽  
Joanna Kuźma ◽  
Paweł Płuszka ◽  
Piotr Chmielewski ◽  
Edyta Bobrowska ◽  
...  

The article presents the concept of experimental research system to investigate aeroponic cultivation in microgravity condition. The main scientific objective is to define the forces acting in droplet-root system exposed to microgravity conditions especially the adhesion and cohesion phenomena. The concept of a research platform is presented in this paper and includes electrical, hydraulic and optical system.


2020 ◽  
pp. 189-212
Author(s):  
Jennifer Hsieh

As part of democratic liberalization in the late 1970s and 1980s, noise abatement signified the Kuomintang (KMT) regime’s attention to the quality of life of local Taiwanese residents. However, the use of scientific, objective indicators for noise, such as decibels, also had the effect of subjecting individual, human experience to the standardizing techniques of quantification and measurement. This chapter examines the application of Western technologies of audiometry and noise abatement in the context of Taiwan’s transition to a postauthoritarian state. Through an analysis of audiometric testing of hearing health among schoolchildren and neighborhood-wide socioacoustic surveys that assessed noise tolerance levels, this chapter asks how hearing and noise became interests of the state—as both a source of state authority and a symbol of liberal governance.


2020 ◽  
pp. 29-50
Author(s):  
Robert H. Riffenburgh ◽  
Daniel L. Gillen
Keyword(s):  

1984 ◽  
Vol 86 ◽  
pp. 32-35
Author(s):  
J.W. Cook ◽  
G.E. Brueckner ◽  
J.-D.F. Bartoe ◽  
D.G. Socker

The HRTS (High Resolution Telescope and Spectrograph) instrument is a high spectral (0.05 Å) and spatial (<1 arc sec) resolution spectrograph with a slit length of 900 arc sec on the solar disk (see Bartoe and Brueckner 1975, 1978). HRTS contains in addition a double grating, zero dispersion broadband spectroheliograph which images the spectrograph slit jaw plate (see Cook et al. 1983). The central wavelength is tunable by changing the grating geometry. Hα images are also photographed from the slit jaw plate image. HRTS has been flown four times as a rocket payload, and will fly in April 1985 as one of the solar experiments aboard Spacelab 2. The four rocket flights of the HRTS program have each been customized for a particular scientific objective. For the fourth flight, because the original hardware was utilized as the basis of the Spacelab HRTS, the opportunity was used to design and build a new rocket HRTS instrument specialized for observations at the solar limb. In this configuration the photographic speed was increased, a new curved slit was fabricated, and the spectroheliograph was modified for limb observations. The scientific observing program was a study of structure and short term temporal evolution at the limb, with a comparison of quiet and coronal hole areas.


1987 ◽  
Vol 7 (2) ◽  
pp. 197-204 ◽  
Author(s):  
J. Lim ◽  
G. J. Nelson ◽  
A. E. Vaughan

AbstractThe design and scientific applications of a 96-channel filter spectrograph of 1 MHz resolution are presented. The spectrograph is currently under construction and will be installed on the Parkes telescope in 1987-1988. Its main scientific objective is dynamic spectral studies of decimetre- and metre-wavelength bursts from flare stars. However, it will also be used for performing large-scale pulsar surveys, and dynamic spectral observations of interplanetary scintillation of compact sources, interstellar scintillation of compact extragalactic sources, and interesting radio sources in general.We show that plasma emission generated in the coronae of flare stars should be detectable at metre- and decimetre-wavelengths. We plan to search for fundamental and second-harmonic plasma radiation by observing in two harmonically related bands, 200 to 250 MHz and 400 to 500 MHz. With noise-adding to stabilize receiver gain, the sensitivity (3σ) of each channel of the spectrograph is ∼ 1.5 Jy for a 1-s integration. Previous studies have reported peak flux densities of up to ∼ 35 Jy and ∼ 12 Jy at 240 MHz and 410 MHz respectively for radio bursts from flare stars.


Servis plus ◽  
10.12737/2791 ◽  
2014 ◽  
Vol 8 (1) ◽  
pp. 23-28
Author(s):  
Галина Камнева ◽  
Galina Kamneva ◽  
Сергей Сотников ◽  
Sergey Sotnikov

The article deals with the evolution of the vision that the Russia-descendant community based out of Russia communicated through scientific literature, mass media, and Russian public opinion at different stages of democratic reforms. The author draws conclusions concerning the establishment of scientific objective vision of the Russia-descendant non-Russia-based community at the turn of the 21s´century and the development of a comprehensive informational and social/cultural dialogue between Russia and emigrants from Russia.


1965 ◽  
Vol 161 (984) ◽  
pp. 363-375 ◽  

For the meteorologist the elucidation of the reasons for past climatic fluctuations or changes must be a major scientific objective in order that he may be better placed with regard to the future. But before he can attempt a satisfactory explanation of past climatic events, great or small, he must be provided with quantitative data. He must know the magnitude, the extent and the time of incidence of the phenomena. We are acutely in need of more accurate dating of the events whose effects are brought to our notice by botanical evidence. We need to know their spatial extent because we can readily think of events affecting the sun which would be likely to produce immediate reactions over the whole earth. But we can equally readily think of others, such as the freezing of the Norwegian Sea that would very rapidly affect the climate and the vegetation of the coast of Norway but would, at best, make but a slight impression on that of a distant area such as the plain of north China. Accordingly, the meteorologist finds himself immediately interested in the quite notable changes represented by the recurrence-surfaces in the bogs of north-west Europe. Twenty years have passed since van Post (1944) described the results of the many pollen-analytical investigations up to that time as ‘a kaleidoscopic synthesis of larger and smaller climatic waves’. He was disposed to think that period lengths of approximately 1700 years, 800 to 900 years and about 400 or 200 years might be deduced for the undulations of climate. But he went on to say that ‘if the facts appear to agree approximately, then the theory becomes positively dangerous for it may tempt us to wishful thinking that obscures our vision of the empirical realities’. It is with some of these realities that I propose to deal.


2007 ◽  
Vol 3 (S244) ◽  
pp. 289-294 ◽  
Author(s):  
N. R. Napolitano ◽  
A. J. Romanowsky ◽  
L. Coccato ◽  
M. Capaccioli ◽  
N. G. Douglas ◽  
...  

AbstractWe examine the dark matter properties of nearby early-type galaxies using planetary nebulae (PNe) as mass probes. We have designed a specialised instrument, the Planetary Nebula Spectrograph (PN.S) operating at the William Herschel telescope, with the purpose of measuring PN velocities with best efficiency. The primary scientific objective of this custom-built instrument is the study of the PN kinematics in 12 ordinary round galaxies. Preliminary results showing a dearth of dark matter in ordinary galaxies (Romanowskyet al. 2003) are now confirmed by the first complete PN.S datasets. On the other hand early-type galaxies with a “regular” dark matter content are starting to be observed among the brighter PN.S target sample, thus confirming a correlation between the global dark-to-luminous mass virial ratio (fDM=MDMM*) and the galaxy luminosity and mass.


2014 ◽  
Vol 926-930 ◽  
pp. 3220-3223
Author(s):  
Qing Cong Zhao

When a security attribute of the assets assignment is valuated, the commonly used method is based on the analysis of the corporate business strategy, combined with the data value given directly by the experience and intuition of the evaluators. This assessment process is lack of scientific basis. Grey Statistical evaluation can composite the views of related personnel in different department and give confidence interval. The scientific, objective and impartial assignment process is ensured by the statistical results. For example of asset integrity assignment, the process can be completed by the method used of grey statistical evaluation.


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