The solar-neutrino problem, 1995Il Nuovo Cimento C - Tập 18 - Trang 671-684 - 1995
V. Berezinsky
The status of the Solar-Neutrino Problem (SNP), as is seen in 1995, is reviewed.
Basically, there are two principal solutions to the SNP: i) withstandard
neutrino (neutrino of SM of electroweak interactions) and ii) withnon-standard
neutrino (neutrino beyond the SM). Actually, one can distinguish three
solar-neutrino problems: the deficit of8B neutrinos, the deficit of7Be neutrinos
and the HOMESTA... hiện toàn bộ
On the relationship between the gradient and the bulk Richardson number for the atmospheric surface layerIl Nuovo Cimento C - Tập 15 - Trang 111-114 - 1992
N. M. Zoumakis
Semi-empirical formulations which have been proposed to describe the wind and
potential temperature profiles are used to derive relationships between the
gradient Richardson number, Ri, the finite-difference layer Richardson number,
Rib, the surface layer Richardson number, Ris, and the bulk Richardson number,B,
through the atmospheric surface layer. The theoretical analysis for stable
conditions ... hiện toàn bộ
An application of neural nets to the Rome precipitation series (1782–1989)Il Nuovo Cimento C - Tập 18 - Trang 547-561 - 1995
D. Anfossi, C. Cappa, S. Alessio
In a recent paper Elsner and Tsonis (1992) have demonstrated the feasibility of
short-term prediction of climatic data by means of neural nets. In this paper,
the same technique has been applied to the rather long (208 years) Rome
precipitation series. At first, some examples of artificially generated time
series, ranging from analytical functions to a mathematical model, have been
used to test th... hiện toàn bộ
Helios 1+helios 2: a summary of IMF observations performed in the inner solar system during 1975–1981Il Nuovo Cimento C - Tập 5 - Trang 497-506 - 1982
U. Villante, F. Mariani, R. Cirone
The experimental observations performed by Helios 1 and Helios 2 spacecraft
allow one to monitor the IMF conditions in the inner solars ystem
(0.3≦r≦0.6A.U.) over many years. The field orientation closely corresponds to
the theoretical predictions and the histograms of the distributions of the
angular elements are possibly more peaked around the expected values than those
ones obtained at greater ... hiện toàn bộ
Proposal to build a neutrino observatory in Sudbury, CanadaIl Nuovo Cimento C - Tập 9 - Trang 308-317 - 1986
D. Sinclair, A. L. Carter, D. Kessler, E. D. Earle, P. Jagam, J. J. Simpson, R. C. Allen, H. H. Chen, P. J. Doe, E. D. Hallman, W. F. Davidson, R. S. Storey, A. B. McDonald, G. T. Ewan, H. -B. Mak, B. C. Robertson
The proposal to build a heavy-water Čerenkov detector deep underground is
discussed. The main physics objectives are to measure the8B solar neutrino flux,
to identify neutrino oscillations and to watch for gravitational collapse. The
measurements of the sources of background and the optical properties of heavy
water, which are necessary to prove the feasibility of the detector, are
reported. The p... hiện toàn bộ
Weiner filters for gravitational-wave antennas: Characteristics and applicationsIl Nuovo Cimento C - Tập 17 - Trang 713-744 - 1994
P. Astone, P. Bonifazi, G. V. Pallottino, G. Pizzella
We report on the application of Wiener filters to the data of Weber-type
gravitational-wave antennas, with particular reference to data processed by
means of lock-in amplifiers driven at the frequencies of the modes of the
detector. After a review of some basic results concerning the filtering of the
data, we briefly examine the relationship between Wiener filters and matched
filters. The discussi... hiện toàn bộ