30 An example: Secondaries Hümmer et al, Astropart. Phys. 34 (2010) 205 =2, B=10 3 G, R=10 9.6 km Cooling: charged,, K Secondary spectra (,, K) become
{"Image DocumentName": "An example: Secondaries", "Image ImageDescription": "a=2, B=103 G, R=109.6 km. Secondary spectra (m, p, K) become loss-steepend above a critical energy. Ec depends on particle physics only (m, t0), and B. Leads to characteristic flavor composition. Any additional cooling processes mainly affecting the primaries will not affect the flavor composition. Flavor ratios most robust predicition for sources? The only way to directly measure B? Cooling: charged m, p, K. Spectral split. Pile-up effect \uf0f0 Flavor ratio! Ec. Ec. Ec. H\u00fcmmer et al, Astropart. Phys. 34 (2010) 205.", "Image XResolution": "37", "Image YResolution": "37", "Image ResolutionUnit": "Pixels/Centimeter", "Image Software": "SlidePlayer", "Image YCbCrPositioning": "Centered"}