rim russian italian missions
DESCRIPTION
RIM Russian Italian Missions. Piergiorgio Picozza INFN and University of “Rome Tor Vergata”. Russia:. Italy:. CNR, Florence. Bari. Florence. Frascati. Naples. Rome. Trieste. India:. Mumbay. Sweden:. Germany:. Siegen. KTH, Stockholm. RIM COLLABORATION. Moscow St. Petersburg. - PowerPoint PPT PresentationTRANSCRIPT
RIMRIM
Russian Italian MissionsRussian Italian Missions
Piergiorgio PicozzaPiergiorgio Picozza
INFN and University of “Rome Tor Vergata”INFN and University of “Rome Tor Vergata”
Bari Florence Frascati
Italy:TriesteNaples Rome CNR, Florence
Moscow St. Petersburg
Russia:
India:
Mumbay
Germany:Siegen
Sweden:KTH, Stockholm
RIM COLLABORATIONRIM COLLABORATION
1993 · 1994 · 1995 · 1996 · 1997 · 1998 · 1999 · 2000 · 2001 · 2002 · 2003 · 2004 · 2005 · 2006 · 2007 ·2008 · 2009……
PAMELA
NINA-2NINA-1
NINA-1 NINA-2
SILEYE-2 SILEYE-1 ALTEINO: SILEYE-3
SILEYE-1 SILEYE-2 Alteino-SILEYE-3 Lazio ALTEA SI-RAD
Si-Rad
RIM PROGRAMRIM PROGRAM
PAMELA
ALTEA: SILEYE-4
LAZIO SIRAD
ZENIT rocket Baikonur, Kazakhstan July 10 1998
COSMOS rocket
Plesetsk, Russia July 15 2000
NINA2-MITA
89° 440 km
NINA-RESURS
97° 810 km
NINA MissionsNuclei P-Fe
10-200 MeV/n
Cosmic Rays: Galactic
Trapped
Solar Flares
NINA 1
NINA 2
Galactic Cosmic RaysGalactic Cosmic Rays Cosmic ray abundances, with the Cosmic ray abundances, with the odd-evenodd-even effect, effect,
the peaks at C and O, and the relative depression the peaks at C and O, and the relative depression of the light elements Li, Be and B of the light elements Li, Be and B
Very good Very good agreementagreement among SIS, CRIS and NINA among SIS, CRIS and NINA resultsresults
Solar Energetic ParticlesSolar Energetic Particles
Time (day)
Par
ticl
es *
100
/(cm
2 sr
s)
S(E) = A exp(- S(E) = A exp(- )+ B(E) )+ B(E)
B(E) B(E) galactic backgroundgalactic background 33He : (He : ( = 2.5 ± 0.6) = 2.5 ± 0.6) 44He : (He : ( = 3.7 ± 0.3) = 3.7 ± 0.3) 33He/He/44He ratio increases with energyHe ratio increases with energy
Light FlashesLight Flashes
The Detectors on board ISS
ALTEA: July 4 2006on board ISS
SilEyeprojects
SDU:3 silicon planes with double detector, view X e Y:area: 2 x (8 x 8) cm2
pitch: 2.4 mm32 strips per viewthickness 380 µm
threshold 0.21 MeV saturation 160 MeVplanes distance : 3.75 cmmaximum error of angular reconstruction: ±1.8°
(Silicon Detector System,Composed by
6 SDU, Silicon Detector Units)
SDS
EEG
(Visual Stimulator Unit)
VSU
University of Genoa
University of Rome“Tor Vergata”
ALTEA / Si-Rad Facility at Houston
Pamela Flight ModelPamela Flight Model
ARKADY M. GALPER
TALK
June 15 2006