CosmicRayFlux

概要

パッケージ

クラス

階層ツリー

非推奨 API

索引

ヘルプ

前のクラス 次のクラス

フレームあり フレームなし

概要: 入れ子 | フィールド | コンストラクタ | メソッド

詳細: フィールド | コンストラクタ | メソッド

iceCube.uhe.muonModel
クラス CosmicRayFlux

java.lang.Object
  iceCube.uhe.muonModel.CosmicRayFlux

public class CosmicRayFlux
extends java.lang.Object
extends java.lang.Object

UHE Cosmic Ray Flux

コンストラクタの概要
`CosmicRayFlux()` Constructor: Calculate log(dJ/dE) @ E = energyBase

メソッドの概要
`boolean`	`doesCutOffExists()` Tell if the CR spectrum calculated in this object has a cutoff feature at the highest energy end
`double`	`getDFDLogE(double logEnergy)` calculate the log differential Flux dF/dLogE [/cm^2 sec sr] logEnergy [GeV]
`double`	`getDFDLogE(double logEnergy, double cosTheta)` calculate the log differential Flux dF/dLogE [/cm^2 sec sr] logEnergy [GeV] cos(zenith angle) This method is indentical to getDFDLogE(double logEnergy) because the cosmic ray flux is isotropic.
`double`	`getEFlux(double logEnergy)` calculate the differential Energy Flux [GeV /cm^2 sec sr] logEnergy [GeV]
`double`	`getEFlux(double logEnergy, double cosTheta)` calculate the differential Energy Flux [GeV /cm^2 sec sr] logEnergy [GeV] cos(zenith angle) This method is indentical to getEFlux(double logEnergy) because the cosmic ray flux is isotropic.
`boolean`	`isValidEnergy(double logEnergy)` Check if the energy is in the range where this power law model is valid.
`void`	`setCutOffFeature(boolean cutoffExists)` Sets on/off the cutoff feature at the highest energy end

クラス java.lang.Object から継承されたメソッド
`clone, equals, finalize, getClass, hashCode, notify, notifyAll, toString, wait, wait, wait`

コンストラクタの詳細

CosmicRayFlux

public CosmicRayFlux()

Constructor: Calculate log(dJ/dE) @ E = energyBase

メソッドの詳細

doesCutOffExists

public boolean doesCutOffExists()

Tell if the CR spectrum calculated in this object has a cutoff feature at the highest energy end

setCutOffFeature

public void setCutOffFeature(boolean cutoffExists)

Sets on/off the cutoff feature at the highest energy end

getEFlux

public double getEFlux(double logEnergy)

calculate the differential Energy Flux [GeV /cm^2 sec sr]

        logEnergy [GeV]

getEFlux

public double getEFlux(double logEnergy,
                       double cosTheta)

calculate the differential Energy Flux [GeV /cm^2 sec sr]

        logEnergy [GeV] cos(zenith angle)

This method is indentical to getEFlux(double logEnergy) because the cosmic ray flux is isotropic.

getDFDLogE

public double getDFDLogE(double logEnergy)

        calculate the log differential Flux dF/dLogE [/cm^2 sec sr] 

        logEnergy [GeV]

getDFDLogE

public double getDFDLogE(double logEnergy,
                         double cosTheta)

        calculate the log differential Flux dF/dLogE [/cm^2 sec sr] 

        logEnergy [GeV] cos(zenith angle)

This method is indentical to getDFDLogE(double logEnergy) because the cosmic ray flux is isotropic.

isValidEnergy

public boolean isValidEnergy(double logEnergy)

Check if the energy is in the range where this power law model is valid. It depends on whether the spectrum has a cutoff feature which you can set by calling the method void setCutOffFeature(boolean ).