Meteor counts are added together into variable-sized bins before the flux is computed for each bin. The size of the bins can be defined using the settings below.
Note that the reported time of each bin is not the middle between begin and end, but the average time of all observations contributing to the bin. So it may deviate from (end/begin)/2 for each bin.
First, specify how much data you want in each bin, then the constraint on the time interval covered by each bin:

By default, all cameras are selected. You can manually select or deselect individual cameras. Alternatively you can select observers, countries or continents, and the corresponding cameras will be selected automatically.

Here you can specify further boundary conditions for the selection of the data set, like the stellar limiting magnitude and the radiant altitude.
For the lunar conditions you can decide, if they are combined by logical and or or. That is, and observation will only used if one, if the lunar altitude is not larger, and/or the lunar phase is not larger, and/or the distance from the center of fov is larger than the specified values.

 and   or 

 and   or 

Finally a few advanced settings for the generation of the activity profile: The population index, the zenith exponent, the perception coefficient correction, and the maximum value of the Y axis.
You can also define flux density threshols for outlier rejection, and if the flux or particle density is printed at the primary y-axis.