Level 2 Help for PHOTFIT2_BURATTI3

Weight of unisotropic and isotropic reflectance.

This parameter gives the absolut lower limit of the weight of unisotropic and 
isotropic reflectance.
If a sulution guess falls out-of-bonds then the attemp will be aborted and 
a new guess attempted.

This parameter gives the absolut upper limit of the weight of unisotropic and 
isotropic reflectance.
If a sulution guess falls out-of-bonds then the attemp will be aborted and 
a new guess attempted.

This parameter gives temperatur for the weight of unisotropic and isotropic 
reflectance.
This parameter gives the range over which random guesses can be expected to 
vary at first:
    ALBEDO_NEW = T_ALBEDO * tan( PI * ran_num + PI/2 ).
As the system cools the range will constrict gradually :
	T_ALBEDO_NEW_* = T_ALBEDO_OLD_* * scale, 
scale depends of NUMTEN.

Parameter of the Veverka and Mosher photometric functions.

This parameter gives the absolut lower limit of the parameter of the Veverka 
and Mosher photometric functions.
If a sulution guess falls out-of-bonds then the attemp will be aborted and 
a new guess attempted.

This parameter gives the absolut upper limit of the parameter of the Veverka 
and Mosher photometric functions.
If a sulution guess falls out-of-bonds then the attemp will be aborted and 
a new guess attempted.

This parameter gives temperatur for the parameter of the Veverka and Mosher 
photometric functions.
This parameter gives the range over which random guesses can be expected to 
vary at first:
    B_VEVERKA_NEW = T_B_VEVERKA * tan( PI * ran_num + PI/2 ).
As the system cools the range will constrict gradually :
	T_B_VEVERKA_NEW_* = T_B_VEVERKA_OLD_* * scale, 
scale depends of NUMTEN.

Parameter of the Veverka, Mosher and Buratti 
photometric functions.

This parameter gives the absolut lower limit of the parameter of the Veverka, 
Mosher and Buratti photometric functions.
If a sulution guess falls out-of-bonds then the attemp will be aborted and 
a new guess attempted.

This parameter gives the absolut upper limit of the parameter of the Veverka, 
Mosher and Buratti photometric functions.
If a sulution guess falls out-of-bonds then the attemp will be aborted and 
a new guess attempted.

This parameter gives temperatur for the parameter of the parameter of the 
Veverka, Mosher and Buratti photometric functions.
This parameter gives the range over which random guesses can be expected to 
vary at first:
    C_VEVERKA_NEW = T_C_VEVERKA * tan( PI * ran_num + PI/2 ).
As the system cools the range will constrict gradually :
	T_C_VEVERKA_NEW_* = T_C_VEVERKA_OLD_* * scale, 
scale depends of NUMTEN.

Parameter of the Veverka, Mosher and Buratti 
photometric functions.

This parameter gives the absolut lower limit of the parameter of the Veverka, 
Mosher and Buratti photometric functions.
If a sulution guess falls out-of-bonds then the attemp will be aborted and 
a new guess attempted.

This parameter gives the absolut upper limit of the parameter of the Veverka,
Mosher and Buratti photometric functions.
If a sulution guess falls out-of-bonds then the attemp will be aborted and 
a new guess attempted.

This parameter gives temperatur for the parameter of the Veverka, Mosher 
and Buratti photometric functions.
This parameter gives the range over which random guesses can be expected to 
vary at first:
    D_VEVERKA_NEW = T_D_VEVERKA * tan( PI * ran_num + PI/2 ).
As the system cools the range will constrict gradually :
	T_D_VEVERKA_NEW_* = T_D_VEVERKA_OLD_* * scale, 
scale depends of NUMTEN.

Buratti's parameter for modification of the Veverka photometric function.

This parameter gives the absolut lower limit of the Buratti's parameter for 
modification of the Veverka photometric function.
If a sulution guess falls out-of-bonds then the attemp will be aborted and 
a new guess attempted.

This parameter gives the absolut upper limit of the Buratti's parameter for 
modification of the Veverka photometric function.
If a sulution guess falls out-of-bonds then the attemp will be aborted and 
a new guess attempted.

This parameter gives temperatur for the Buratti's parameter for modification of 
the Veverka photometric function.
This parameter gives the range over which random guesses can be expected to 
vary at first:
    E_BURATTI_NEW = T_E_BURATTI * tan( PI * ran_num + PI/2 ).
As the system cools the range will constrict gradually :
	T_E_BURATTI_NEW_* = T_E_BURATTI_OLD_* * scale, 
scale depends of NUMTEN.