cos(zenith angle) of the primary particle.
Dot line represents events whose hit DOM number above 80.
(high energy events)
|
cos(zenith angle) of the primary particle weighted by hte CR flux.
Dot line represents events whose hit DOM number above 80.
(high energy events)
|
azimuth angle of the primary particle.
|
cos(zenith angle) of the primary particle Vs the energy.
larger dots represents events whose hit DOM number above 80.
(high energy events)
|
Multiplicity of muons
Dot line: without cut
normal line: with DOM#>80
|
Multiplicity Vs primary energy
|
cos(Zenith angle) Vs Multiplicity of muons
|
Energy distribution at IceCube detector (in ice)
Dot line: without cut
normal line: with DOM#>80
|
Energy distribution at IceCube detector (in ice) weighted by the CR flux
Dot line: without cut
normal line: with DOM#>80
|
Energy in ice Vs primary energy
|
Energy in ice Vs primary energy
Iron leands to ~factor 2 more muon bundle energy
|
cos(zenith angle) Vs energy in ice
|
Energy distribution at surface
Dot line: without cut
normal line: with DOM#>80
|
Energy distribution at surface weighted by the CR flux
Dot line: without cut
normal line: with DOM#>80
|
Energy at surface Vs primary energy
|
Energy at surface Vs primary energy
Iron leands to ~factor 2 more muon bundle energy
|
cos(zenith angle) Vs energy at surface
|
Energy at surface Vs energy in ice
There is a constant energy loss during the propagation
from surface to the detector (~log10(0.2)~30%)
|
Npe distribution at IceCube detector (in ice)
ECUTS thres 1 TeV
Dot line: without cut
normal line: with DOM#>80
|
Npe distribution at IceCube detector (in ice)
ECUTS thres 1 TeV
Dot line: without cut
normal line: with DOM#>80
|
Npe Vs in-ice bundle energy
|
Cos(zenith angle) Vs Npe in ice
|