Search

This is proposal to encode the Gunjala Gondi script in the international character encoding standard Unicode. The script was published in Unicode version 11.0 in 2018. The script is used to write Adilabad Gondi (or Southern Gondi) in the Maharashtra and Telangana states of India.

We report the first GNO solar neutrino results for the measuring period GNOI, solar exposure time May 20, 1998 till January 12, 2000. In the present analysis, counting results for solar runs SR1 - SR19 were used till April 4, 2000. With counting completed for all but the last 3 runs (SR17 - SR19), the GNO I result is [65.8 +10.2 -9.6 (stat.) +3.4 -3.6 (syst.)]SNU (1sigma) or [65.8 + 10.7 -10.2 (incl. syst.)]SNU (1sigma) with errors combined. This may be compared to the result for Gallex(I-IV), which is [77.5 +7.6 -7.8 (incl. syst.)] SNU (1sigma). A combined result from both GNOI and Gallex(I-IV) together is [74.1 + 6.7 -6.8 (incl. syst.)] SNU (1sigma)., submitted to Physics Letters B, June 2000. PACS: 26.65. +t ; 14.60 Pq. Corresponding author: till.kirsten@mpi-hd.mpg.de ; bellotti@mi.infn.it

La simulación ha ganado espacio en el mundo tecnológico como herramienta cientifica y técnico profesional, especialmente en el ámbito de las redes de comunicaciones. En el presente trabajo se tratará sobre una nueva herramienta de limulación bajo código libre y licencia GNU, desarrollada para los estudiantes y profesionales, recurso interactivo de investigación y análisis, simulado sobre las redes de datos y su evolución a redes como la GPON en el cual se pueden obtenenr y entregar información, uqe permita indagar, planificar y dimensionar recursos de una red GPON con la revisión y análisis de los resultados e información optimizando y comprobando las distintas deficiencias o limitantes sobre...

Estimation of magnitude and frequency of extreme rainfall has immense importance to make decisions about hydraulic structures like spillways, dikes and dams etc. This research involves the estimation of regional rainfall quantiles of 23 sites using L-moment based index flood regional frequency analysis. Initially, different tests are applied to check the assumptions of independence, stationarity and identical distribution. An L-moment based discordancy measure is used to detect discordant sites. Since in Pakistan, highly elevated area receive more rainfall. On the basis of this characteristic, the study region is divided into three regions which satisfy the L-moment based heterogeneity statistics using Monte Carlo simulations from Kappa distribution. The regional quantile estimates are obtained from GEV, GNO and GLO distributions which are found to be best choices for all three regions based on L-moment ratio diagram, Z-Statistics and average weighted difference values. For robust regional estimates, some accuracy measures are calculated using a simulation study of regional L-moment algorithm. On the basis of relative bias, relative absolute bias and relative RMSE, GNO is found be best robust for regional quantile estimation at lager return periods of 50, 100, 500 and 1000 and GEV at return periods of 1, 2, 5, 10 and 20 for all three regions.

Die radiochemischen Gallium-Experimente GALLEX/GNO und SAGE haben zur Lösung des solaren Neutrinoproblems und der Entdeckung von Neutrino-Oszillationen wesentlich beigetragen. Mit dem Einsatz eines neuen hocheffizienten Detektorkonzepts, das auf Tieftemperaturdetektoren beruht, kann das Potential der Experimente weiter erheblich verbessert werden. Im Rahmen dieser Arbeit wurden die Daten dieser Experimente weiter analysiert und mit dem neuen Detektorkonzept Messungen durchgeführt, u.a. eine Langzeitmessung des 71Ge-Zerfalls. Die neue, hocheffiziente Nachweistechnik für niederenergetische Röntgen-Strahlung kann auch in einer Vielzahl weiterer Aktivitätsanalysen Anwendung finden. The radiochemical Gallium experiments GALLEX/GNO and SAGE have contributed considerably to the solution of the solar neutrino problem and the discovery of neutrino oscillations. Using a new, highly efficient detector concept based on low temperature detectors, the potential of the experiments can be improved substantially. In this work, the data analysis of the experiments was continued and measurements using the new detector concept were performed, e.g. a long-term measurement of the decay of 71Ge. The new, highly efficient detection method for low-energy X-rays is applicable in a variety of different activity analyses.

We report the complete GNO solar neutrino results for the measuring periods GNO III, GNO II, and GNO I. The result for GNO III (last 15 solar runs) is [54.3 + 9.9 - 9.3 (stat.)+- 2.3 (syst.)] SNU (1 sigma) or [54.3 + 10.2 - 9.6 (incl. syst.)] SNU (1 sigma) with errors combined. The GNO experiment is now terminated after altogether 58 solar exposure runs that were performed between May 20, 1998 and April 9, 2003. The combined result for GNO (I+II+III) is [62.9 + 5.5 - 5.3 (stat.) +- 2.5 (syst.)] SNU (1 sigma) or [62.9 + 6.0 - 5.9] SNU (1 sigma) with errors combined in quadrature. Overall, gallium based solar observations at LNGS (first in GALLEX, later in GNO) lasted from May 14, 1991 through April 9, 2003. The joint result from 123 runs in GNO and GALLEX is [69.3 +- 5.5 (incl. syst.)] SNU (1 sigma). The distribution of the individual run results is consistent with the hypothesis of a neutrino flux that is constant in time. Implications from the data in particle- and astrophysics are reiterated., Comment: 22 pages incl. 9 Figures and 8 Tables. to appear in: Physics Letters B (accepted April 13, 2005) PACS: 26.65.+t ; 14.60.Pq