raggi x
Recently Published Documents


TOTAL DOCUMENTS

99
(FIVE YEARS 0)

H-INDEX

5
(FIVE YEARS 0)

2020 ◽  
Vol 21 (3) ◽  
pp. 176-180
Author(s):  
Francesco Frigerio ◽  
Eleonora Poggiogalle ◽  
Lorenzo M. Donini
Keyword(s):  

2019 ◽  
Vol 4 (1) ◽  
pp. 12 ◽  
Author(s):  
Alessandro Puri ◽  
Giovanni Lepore ◽  
Francesco d’Acapito

LISA (Linea Italiana per la Spettroscopia di Assorbimento di raggi X) is the new Italian Collaborating Research Group (CRG) beamline at the European Synchrotron Radiation Facility (ESRF) dedicated to X-ray absorption spectroscopy (XAS). The beamline covers a wide energy range, 4 < E < 90 keV, which offers the possibility for probe the K and L edges of elements that are heavier than Ca. A liquid He/N2 cryostat and a compact furnace are available for measurements in a wide temperature range (10–1000 K), allowing for in situ chemical treatments and measurements under a controlled atmosphere. The sub-millimetric beam size, the high photon flux provided, and the X-ray fluorescence detectors available (HP-Ge, SDD) allow for the study of liquid and highly diluted samples. Trace elements in geological or environmental samples can be analyzed, even for very small sample areas, gaining information on oxidation states and host phases.


2011 ◽  
Vol 17 (1) ◽  
Author(s):  
G. RIGHINI
Keyword(s):  

.


1998 ◽  
Vol 188 ◽  
pp. 71-74
Author(s):  
A.N. Parmar ◽  
M. Bavdaz ◽  
F. Favata ◽  
T. Oosterbroek ◽  
A. Orr ◽  
...  

SAX, an acronym for “Satellite Italiano per Astronomia a raggi X”, now renamed “BeppoSAX” in honor of Giuseppe Occhialini, is the first X-ray mission sensitive in the very broad energy range between 0.1 and 300 keV (Boella et al. 1997a). The Narrow Field Instruments (NFI) have approximately 1° fields of view and consist of the imaging low- and medium-energy concentrator spectrometers (LECS, 0.1-10 keV, Parmar et al. 1997; and MECS, 1-10 keV, Boella et al. 1997b), and the non-imaging high pressure gas scintillation proportional counter (HPGSPC, 3-120 keV, Manzo et al. 1997) and Phoswich detector system (PDS, 15-300 keV, Frontera et al. 1997). All the NFI are coaligned and are normally operated simultaneously. In addition, the payload includes two wide field cameras (WFC, 2-30 keV; Jager et al. 1997) which observe in directions perpendicular to the NFI. These allow the detection of X-ray transient phenomena, as well as long-term variability studies.


1996 ◽  
Vol 7 (4) ◽  
pp. 251-264
Author(s):  
Annibale Mottana ◽  
Augusto Marcelli ◽  
Gabriele Giuli ◽  
Eleonora Paris ◽  
Fernando Scordari ◽  
...  
Keyword(s):  

Sign in / Sign up

Export Citation Format

Share Document