1 / 21

RIM Russian Italian Missions

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.

neville-rocha
Download Presentation

RIM Russian Italian Missions

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript

  1. RIMRussian Italian Missions Piergiorgio Picozza INFN and University of “Rome Tor Vergata”

  2. Russia: Italy: CNR, Florence Bari Florence Frascati Naples Rome Trieste India: Mumbay Sweden: Germany: Siegen KTH, Stockholm RIM COLLABORATION Moscow St. Petersburg

  3. NINA-1 PAMELA NINA-2 ALTEINO: SILEYE-3 ALTEA: SILEYE-4 LAZIO SIRAD SILEYE-1 SILEYE-2 RIM PROGRAM NINA-1 NINA-2 PAMELA 1993 ·1994· 1995·1996· 1997·1998· 1999· 2000· 2001· 2002· 2003· 2004· 2005· 2006· 2007 ·2008 · 2009…… SILEYE-1 SILEYE-2 Alteino-SILEYE-3 Lazio ALTEA SI-RAD Si-Rad

  4. NINA-RESURS 97° 810 km NINA2-MITA 89° 440 km COSMOS rocket Plesetsk, Russia July 15 2000 ZENIT rocket Baikonur, Kazakhstan July 10 1998

  5. NINA Missions Nuclei P-Fe 10-200 MeV/n Cosmic Rays: Galactic Trapped Solar Flares NINA 1 NINA 2

  6. Cosmic ray abundances, with the odd-even effect, the peaks at C and O, and the relative depression of the light elements Li, Be and B Very good agreement among SIS, CRIS and NINA results Galactic Cosmic Rays

  7. S(E) = A exp(- )+ B(E) B(E) galactic background 3He : ( = 2.5 ± 0.6) 4He : ( = 3.7 ± 0.3) 3He/4He ratio increases with energy Solar Energetic Particles Particles *100 /(cm2 sr s) Time (day)

  8. Light Flashes

  9. The Detectors on board ISS

  10. SilEye projects University of Rome “Tor Vergata” SDS University of Genoa (Silicon Detector System, Composed by 6 SDU, Silicon Detector Units) VSU (Visual Stimulator Unit) ALTEA: July 4 2006 on board ISS SDU: 3 silicon planes with double detector, view X e Y: area: 2 x (8 x 8) cm2 pitch: 2.4 mm 32 strips per view thickness 380 µm threshold 0.21 MeV saturation 160 MeV planes distance : 3.75 cm maximum error of angular reconstruction: ±1.8° EEG

  11. ALTEA / Si-Rad Facility at Houston

  12. Pamela Flight Model ARKADY M. GALPER TALK

  13. June 15 2006

More Related