'Low energy gamma' presentation slideshows

Radiation Interaction - Detection

688 views • 35 slides

Radiation Detectors / Particle Detectors

642 views • 27 slides

Gus Sinnis Los Alamos National Laboratory for the HAWC Collaboration

H igh A ltitude W ater C herenkov Telescope. g. Gus Sinnis Los Alamos National Laboratory for the HAWC Collaboration. Scientific Goals of HAWC. What are the origins of Galactic cosmic rays? Detailed map of the Galactic diffuse emission Extended sources - Morphology & Energy Spectra

462 views • 22 slides

Gamma and X ray interactions

Gamma and X ray interactions. NUCP 2371 Rad Pro III. EM Energy. Energy of the EM radiation is determined by its frequency E= hf h= planks constant =6.6 x 10 -34 J sec Or 4.1 x 10 -15 eV sec F= frequency of the EM radiation Frequency is the inverse of wavelength. Photon Interactions.

442 views • 20 slides

Spectrum if all energy is captured in detector. Allows identification of gamma energy.

296 views • 20 slides

Gamma and X ray interactions

Gamma and X ray interactions. NUCP 2371 Rad Pro III. EM Energy. Energy of the EM radiation is determined by its frequency E= hf h= planks constant =6.6 x 10 -34 J sec Or 4.1 x 10 -15 eV sec F= frequency of the EM radiation Frequency is the inverse of wavelength. Photon Interactions.

214 views • 20 slides