https://dx.doi.org/10.5194/egusphere-egu24-7996">
 

Creative Commons License

Creative Commons Attribution 4.0 International License
This work is licensed under a Creative Commons Attribution 4.0 International License.

Abstract

The LOFAR radio telescope works on a principle of radio interferometric imaging. It coherently sums the signal of hundreds of antennas in northern Netherlands, covering the 30-80 MHz window of the very high frequency (VHF) band of 30-300 MHz. We are using the TRI-D algorithm to extract 3-D polarization data of a lightning flash observed by LOFAR. TRI-D functions by coherently summing recorded voltages, accounting for the antenna function, polarization, and geometric time delay for each voxel. The result is split into time slices. A coherent intensity is calculated for each time slice, and the maximum of this value is set as a source location. The outcome is a reconstructed source location and polarization as seen by the LOFAR antennas. We are now exploring the accuracy of TRI-D in response to realistic parameters. In this work, we perform a Monte Carlo error analysis which simulates the voltages on each antenna from an assumed dipole emitter, adds normally distributed noise, and then reconstructs the source properties with TRI-D. The difference between the simulated input and the reconstruction gives us an estimate of the resulting error bars. We will show a detailed account of the interferometry technique that produces our data, the Monte Carlo simulation that tests the accuracy of our model and finally, our polarization results.

Department

Physics

Publication Date

11-27-2024

Journal Title

EGU General Assembly 2024

Publisher

Copernicus GmbH

Digital Object Identifier (DOI)

https://dx.doi.org/10.5194/egusphere-egu24-7996

Document Type

Conference Proceeding

Rights

© Author(s) 2024.

Comments

This is an open access article published by Copernicus GmbH in EGU General Assembly 2024 in 2024, available online: https://dx.doi.org/10.5194/egusphere-egu24-7996

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