scholarly journals Postural Analysis: Description of a Dedicated System. An Upgrade

Author(s):  
Sergio Palandri

Abstract BackgroundIn June 2021 an aericle was published describing a possible ssystem to perform postural analysis. In six months use, the ssystem has more clarely showed its lights and shadoes. So the author tought some improvements of the sustem that are now ready to be applyed. This article will show them in details.Materials and MethodsUpgrade interested both aspects close connected to the analysis and both connected to its management .ResultsFirst results obtained are interesting and encourage the use of the upgrades introduced. However a more long period of use is necessary to confirm first resultas.ConclusionsUpgrading is a natural step in every life project. And it is made up not only by a single step. So also this system may be further improved with other upgrades in the future.

2004 ◽  
Vol 193 ◽  
pp. 133-137 ◽  
Author(s):  
M. Monelli ◽  
A.R. Walker ◽  
G. Bono ◽  
R. Buonanno ◽  
F. Caputo ◽  
...  

AbstractWe present first results concerning the detection of variable stars in the Carina dwarf Spheroidal from B, V images collected with the 4-m CTIO telescope. We show a sample of candidate variables spanning from the tip of the Red Giant Branch down to the Main Sequence turn off. Finally, we discuss the future photometric and spectroscopic developments of this project.


2002 ◽  
Vol 09 (02) ◽  
pp. 883-888 ◽  
Author(s):  
G. H. FECHER ◽  
J. BRAUN ◽  
A. OELSNER ◽  
CH. OSTERTAG ◽  
G. SCHÖNHENSE

The angular dependence of the circular dichroism in photoemission from Pt(111) was investigated for excitation with VUV and soft X-ray radiation. VUV excitation was used to probe band structure and the circular dichroism for valence band emission. The measurements are compared to full relativistic single step photoemission calculations. XPS was used to investigate the circular dichroism in emission from the 4f core level. In this case, the dichroism is induced by photoelectron diffraction. First results from single step core level calculations are compared to the experimental observations.


2019 ◽  
Vol 111 ◽  
pp. 06011
Author(s):  
Joachim Seifert ◽  
Paul Seidel ◽  
Jens Werner ◽  
Andrea Meinzenbach

Due to the energy system transformation initiated by the German government, the energy supply structures will be much more decentralized in the future. In the following publication the methodology of a Regional Virtual Power Plant will be described and first results from a field test will be presented.


2008 ◽  
Vol 7 ◽  
pp. S72
Author(s):  
M. Vreys ◽  
M. Moens ◽  
F. Vermeulen ◽  
K. De Boeck ◽  
M. Proesmans

1998 ◽  
Vol 164 ◽  
pp. 141-142 ◽  
Author(s):  
V. Altunin ◽  
A. Beasley ◽  
E. Lűdke ◽  
V. Alekseev ◽  
B. Lipatov ◽  
...  

AbstractIn this paper we report the first results of the 327 MHz VLBI survey which has been carried out in the last two years to select potential candidate sources for the future SVLBI missions and to search for directions of small scattering-“holes” in the interstellar scattering medium. During the three VLBI sessions conducted so far, we observed about 80 sources. Preliminary data analyzed from the first part of the survey shows that at least 17 out of 50 sources have compact components with a size smaller than 30 mas.


1999 ◽  
Vol 172 ◽  
pp. 349-358
Author(s):  
P.J. Message

AbstractThis paper begins with a brief review of a form of the Lie series transformation, and then reports some new results in the study, using Lie series methods, of the orbit of Saturn’s satellite Hyperion. In particular, improved expressions are given for the long-period perturbations of the orbital elements which describe the motion in the orbit plane, and also first results for expressions for the short-period perturbations in the apse longitude, derived from the Lie series generating function.


2020 ◽  
Author(s):  
Oliver Kirner ◽  
Jöckel Patrick ◽  
Sören Johansson ◽  
Gerald Wetzel ◽  
Franziska Winterstein

<p>The increasing future methane (CH<sub>4</sub>) leads to changes in the lifetime of CH<sub>4</sub> and in the Hydroxyl radical (OH) and (O<sub>3</sub>) mixing ratios and distribution in the lower atmosphere. With increasing CH<sub>4</sub> the lifetime of CH<sub>4</sub> and the O<sub>3</sub> mixing ratios in the troposphere will increase, the tropospheric OH mixing ratios will decrease (Winterstein et al., 2019; Zhao et al., 2019). The CH<sub>4</sub> changes, together with the future Nitrous oxide (N<sub>2</sub>O) and temperature increase, will lead to a different tropospheric chemistry. For example, substances as acetone (CH<sub>3</sub>COCH<sub>3</sub>), ethane (C<sub>2</sub>H<sub>6</sub>), formic acid (HCOOH) or peroxy acetyl nitrate (PAN) will change their distribution and mixing ratios.</p><p>In different studies we could show that EMAC (ECHAM/MESSy Atmospheric Chemistry, Jöckel et al., 2010) has the ability to simulate some of the mentioned tropospheric substances in comparison to results of the GLORIA (Gimballed Limb Observer for Radiance Imaging of the Atmosphere) instrument, used on board of the research aircrafts Geophysica and HALO during the STRATOCLIM (July/August 2017) and WISE (August to October 2017) campaigns (Johansson et al., 2020; Wetzel et al., 2020).   </p><p>In this study, we will additional show the first results of the simulated future changes of tropospheric chemistry (especially with focus on CH<sub>3</sub>COCH<sub>3</sub>, C<sub>2</sub>H<sub>6</sub>, HCOOH and PAN and the upper troposphere) related to the future increase of CH<sub>4</sub>, N<sub>2</sub>O and temperature change as a result of climate change. For these we use different EMAC simulations from the project ESCiMo (Earth System Chemistry Integrated Modelling, Jöckel et al., 2016).</p><p>We will present some results of the comparison of EMAC to GLORIA and results with regard to the future development of the (upper) tropospheric chemistry in EMAC.    </p>


2002 ◽  
Vol 17 (22) ◽  
pp. 3026-3035
Author(s):  
◽  
FABIO BOSSI

Since April 1999, the KLOE experiment at DAΦNE has collected about 200 pb-1 of data, produced in e+ - e- collision at the c.m. energy of 1020 MeV, the mass of the ϕ(1020) meson. This data has been used for detailed studies on the ϕ radiative decays, as well as on rare [Formula: see text] decays. The first results, based on the ~ 20 pb-1 collected in year 2000 are presented here. Perspectives for the future data taking are also discussed.


Author(s):  
Ulrich Quade ◽  
Thomas Kluth

Since more than 20 years the company Siempelkamp is deeply involved in the field of melting and recycling of radioactively contaminated metals from operation and decommissioning of nuclear installations across Europe. The experience of this long period shows clearly that only a combination of recycling inside the nuclear industry and release for reuse outside the nuclear market will generate the optimum results for the minimisation of radioactive waste volume. Final disposal volume is becoming more and more the status of an own resource within our nuclear business and should be handled very carefully in the future. The paper gives a compact overview about the impressive results of melting treatment, the current potential of the melting plant CARLA and about further developments.


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