A Monte-Carlo Simulator package developed at CERN

if the magnetic field is not constant, you have 6 different options to define one component of the B vector using a MAG file.

The simplest and most often used magnetic field: you define a strength for a list of coordinates, and Synrad will interpolate between them.

MAG file format:

period dirX dirY dirZ N coordinate1 value1 coordinate2 value2 ... coordinateN valueN

The idea is that you have a machine (a dipole, for example) that begins at the **starting point** of the region, and is orientated in the (dirX,dirY,dirZ) direction, with a defined period. Then to calculate the magnetic field strength, the following is done:

1. The actual position is projected to the direction vector (scalar multiplication of the direction vector and the [actual_position-starting_point] vector

2. The projection is interpreted as the "ccordinate" (distance) and being looked up in the first column

3. It is interpolated between the N fixed coordinated (distances) written in the lines

**Example:** Your MAG file is the following for the Bx component:

100.0 0.0 0.0 1.0 2 0 2.0 100.0 3.0

It means the following: we have a machine oriented towards the Z axis (0,0,1). It has 2T field at the beginning (0cm) and 3T field at the end of the period (100cm).

Bx(0,0,50)=2.5Tesla (halfway between the two fixed coordinates)

Bx(0,0,120)=2.2Tesla (The period of 100cm is deducted from the 120cm distance)

The above two calculations assumed that the starting point is (0,0,0).

Use the same format as above. The dirX, dirY, dirZ numbers will be ignored. The coordinate will be the L value (distance along beam), with full periods subtracted.

You can define a periodic magnetic field. Format of the BXY file:

period dirX dirY dirZ N A1 B1 A2 B2 ... AN BN

Where period is the period of the sine and cosine function. DirX, dirY and dirZ are the same as before. N is the number of lines that follow.

A1, B1, A2, B2, ... are coefficients, to give the following magnetic field:

B(distance)=

A1*sin(distance*2PI/period) + B1*cos(distance*2PI/period) +

A2*sin^2(distance*2PI/period) + B2*cos^2(distance*2PI/period) +

...

AN*sin^N(distance*2PI/period) + BN*cos^N(distance*2PI/period)

If you choose this mode, one component's MAG file will set all the components of the magnetic vector. Load it as the X component's MAG file.

Format of the MAG file:

centerX centerY centerZ alfa beta rot K L

(centerX,centerY,centerZ) define where the center point *of the beginning* of the quadrupole is (ie. the starting point of its axis).

Alfa, beta and rot are 3 angles that define its orientation. The meaning of the angles, in radians, are:

alpha: angle with the XZ plane, positive towards Y

beta: angle with YZ plane, negative towards X

rot: quadrupole rotation around its centerline (that is defined by alpha, beta)

direction.X=-cos(alpha)*sin(beta)

direction.Y=sin(alpha)

direction.Z=cos(alpha)*cos(beta)

With the above parameters, you have the starting point and the direction of the axis.

K is the strength of the quadrupole (in Tesla*meters), and L is its length in cm (magnetic field is 0 outside the quadrupole).

You can see the snippet code calulcating the quarupole field here.

Allows to set up the Halbach wiggler field model.

This mode also sets the B vector's all components. Load the MAG file for the X component! MAG file format:

period dirX dirY dirZ N Kx K2

Here dirX,dirY, dirZ and N are not used (give any value).

The B vector is calculated the following way:

K=2PI/period

Ky=sqrt(K^2-Kx^2)

Bx(positionX,positionY,positionZ) = Kx/Ky*K2*sinh(Kx*positionX)*sinh(Ky*positionY)*cos(K*positionZ)

By(positionX,positionY,positionZ) = K2*sinh(Kx*positionX)*sinh(Ky*positionY)*cos(K*positionZ)

Bz(positionX,positionY,positionZ) = -K/Ky*K2*sinh(Kx*positionX)*sinh(Ky*positionY)*cos(K*positionZ)

A helix. MAG file format:

period phase dirX dirY dirZ N X1 Y1 X2 Y2 ... XN YN

The magnetic component is calculated the following way:

ratio = distance*2PI/period

B(ratio) = X1*sin(ratio)*cos(PI*phase/period) + Y1*cos(ratio)*sin(PI*phase/period)

+ X2*sin(**2***ratio)*cos(PI*phase/period) + Y2*cos(**2***ratio)*sin(PI*phase/period)

+ ...

+ XN*sin(**N***ratio)*cos(PI*phase/period) + YN*cos(**N***ratio)*sin(PI*phase/period)

Load it as X component, sets all 3 components of the B vector.

MAG file:

period dirX dirY dirZ N A X

where only *period *and *A *have meanings (give any value for others).

ratio = distance*2PI/period

Bx(ratio)=A*sin(ratio)

By(ratio)=A*cos(ratio)

Bz=0

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