Cosmic Rays and Astroparticle Physics

foundationsresultsequations+8 morephenomena+9 moreoweddepends_on (declared)depends_on (declared)depends_on (declared)depends_on (declared)depends_on (declared)depends_on (declared)depends_on (declared)depends_on (declared)depends_on (declared)depends_on (declared)depends_on (declared)depends_on (declared)depends_on (declared)depends_on (declared)depends_on (declared)depends_on (declared)depends_on (declared)depends_on (declared)depends_on (declared)depends_on (declared)notation 115.1: Rigidity and atmospheric depth115.1 Rigidity and atm…theorem 115.19: Heitler's cascade115.19 Heitler's cascadetheorem 115.21: Muon number and its scaling115.21 Muon number and…corollary 115.22: Superposition: more muons, shallower maximum115.22 Superposition: m…proposition 115.26: A steep spectrum converts an energy error into a flux error115.26 A steep spectrum…theorem 115.31: Second-order Fermi acceleration115.31 Second-order Fer…theorem 115.33: The spectrum from a strong shock115.33 The spectrum fro…proposition 115.34: Propagation steepens the source spectrum115.34 Propagation stee…theorem 115.36: The Hillas criterion115.36 The Hillas crite…proposition 115.52: The natural beam exceeds the collider by a factor of thirty115.52 The natural beam…equation 115.1: eq:cosmicray-rigidityeq. (115.1)equation 115.2: eq:cosmicray-deptheq. (115.2)equation 115.3: eq:cosmicray-atmospheric-deptheq. (115.3)equation 115.8: eq:cosmicray-larmoreq. (115.8)equation 115.11: eq:cosmicray-stormer-azimutheq. (115.11)equation 115.14: eq:cosmicray-curvatureeq. (115.14)equation 115.15: eq:cosmicray-ionisationeq. (115.15)equation 115.16: eq:cosmicray-radlosseq. (115.16)equation 115.19: eq:cosmicray-pdg-fluxeq. (115.19)equation 115.20: eq:cosmicray-powerlaweq. (115.20)equation 115.21: eq:cosmicray-integral-fluxeq. (115.21)equation 115.24: eq:cosmicray-grammageeq. (115.24)equation 115.25: eq:cosmicray-bc-indexeq. (115.25)phenomenon 115.2: Ionisation increases with altitude115.2 Ionisation incre…phenomenon 115.4: The primary intensity depends on geomagnetic latitude115.4 The primary inte…phenomenon 115.5: The primaries arrive preferentially from the west115.5 The primaries ar…phenomenon 115.8: A positive particle of electronic mass115.8 A positive parti…phenomenon 115.9: A constant secondary range means a two-body decay115.9 A constant secon…phenomenon 115.10: Copious production, slow decay115.10 Copious producti…phenomenon 115.11: A power-law spectrum over eleven decades115.11 A power-law spec…phenomenon 115.13: The knee115.13 The kneephenomenon 115.15: The highest-energy primaries are not confined by the Galaxy115.15 The highest-ener…phenomenon 115.16: Light secondary nuclei are enormously overabundant115.16 Light secondary…phenomenon 115.18: A single primary makes a wide particle front115.18 A single primary…phenomenon 115.25: Composition inferred from the depth of maximum115.25 Composition infe…phenomenon 115.29: Supernovae can supply the Galactic cosmic-ray power115.29 Supernovae can s…pending : ch:17-cosmic-rays-astroparticle@pending-1pendingpending : ch:17-cosmic-rays-astroparticle@pending-2pendingpending : ch:17-cosmic-rays-astroparticle@pending-3pendingpending : ch:17-cosmic-rays-astroparticle@pending-4pendingpending : ch:17-cosmic-rays-astroparticle@pending-5pending
The chain of Cosmic Rays and Astroparticle Physics: 41 of 58 objects, read left to right from what the chapter assumes to what tests it. Solid lines are declared logical edges, dashed ones were inferred from the structure of the source. Click any node to open its own chain.

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