Abstract

MGMR3D is a code that calculates the complete radio footprint, i.e. intensity, polarization and pulse shapes, for a parametrized shower current density using a semianalytic approach. The non-Monte-Carlo code is fast (typically 10 seconds for a complete footprint) and thus can be used in a chi-square optimization calculation of atmospheric electric fields or to optimize antenna geometry.

Highlights

  • Since the code calculates the footprint from first principles once the currents are specified, the results include Cherenkov effects due to a finite refractivity of air

  • In response to request from the community we have build a code that is fast, predictive, and calculates the complete radio footprint from first principles using the 3-dimensional structure of an extensive air shower

  • As such it can be used in a chi-square optimization code to determine the current structure as function of height in the atmosphere as is needed for determining electric fields inclouds

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Summary

Introduction

Since the code calculates the footprint from first principles once the currents are specified, the results include Cherenkov effects due to a finite refractivity of air. In response to request from the community we have build a code that is fast, predictive, and calculates the complete radio footprint from first principles using the 3-dimensional structure of an extensive air shower. As such it can be used in a chi-square optimization code to determine the current structure as function of height in the atmosphere as is needed for determining electric fields in (thunder-)clouds.

Results
Conclusion

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