'1m sun' diaporamas de présentation

The origin of Cosmic Rays: New developments and old puzzles

445 views • 44 slides

High energy cosmic rays & neutrino astronomy

High energy cosmic rays & neutrino astronomy. Eli Waxman Weizmann Institute. X-Galactic/Ultra-high energy ( e >10 19 eV). Cosmic accelerators. log [dJ/dE]. E -2.7. Galactic. Protons. E -3. Source: Supernovae(?). X-Galactic. Heavy Nuclei. Source?. Light Nuclei?. Lighter. Source?. 1.

518 views • 39 slides

High energy neutrino astronomy: Challenges & Prospects

High energy neutrino astronomy: Challenges & Prospects. Eli Waxman Weizmann Institute, ISRAEL. High energy n ’ s: A new window. MeV n detectors: Solar & SN1987A n ’ s Stellar physics (Sun ’ s core, SNe core collapse) n physics >0.1 TeV n detectors:

414 views • 31 slides

337 views • 27 slides

Star and Planet Formation

Star and Planet Formation. Sommer term 2007 Henrik Beuther & Sebastian Wolf. 16.4 Introduction (H.B. & S.W.) 23.4 Physical processes, heating and cooling, radiation transfer (H.B.) 30.4 Gravitational collapse & early protostellar evolution I (H.B.)

330 views • 24 slides