In situ radioglaciological measurements near Taylor Dome, Antarctica and implications for UHE neutrino astronomy

Radiowave detection of the Cherenkov radiation produced by neutrino-ice collisions requires an understanding of the radiofrequency (RF) response of cold polar ice. We herein report on a series of radioglaciological measurements performed approximately 10 km north of Taylor Dome Station, Antarctica f...

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Bibliographic Details
Main Authors: Besson, D., Jenkins, J., Matsuno, S., Nam, J., Smith, M., Barwick, S. W., Beatty, J. J., Binns, W. R., Chen, C., Chen, P., Clem, J. M., Connolly, A., Dowkontt, P. F., DuVernois, M. A., Field, R. C., Goldstein, D., Gorham, P. W., Goodhue, A., Hast, C., Hebert, C. L., Hoover, S., Israel, M. H., Kowalski, J., Learned, J. G., Liewer, K. M., Link, J. T., Lusczek, E., Mercurio, B., Miki, C., Miocinovic, P., Naudet, C. J., Ng, J., Nichol, R., Palladino, K., Reil, K., Romero-Wolf, A., Rosen, M., Ruckman, L., Saltzberg, D., Seckel, D., Varner, G. S., Walz, D., Wu, F.
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Published: arXiv 2007
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Online Access:https://dx.doi.org/10.48550/arxiv.astro-ph/0703413
https://arxiv.org/abs/astro-ph/0703413
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Summary:Radiowave detection of the Cherenkov radiation produced by neutrino-ice collisions requires an understanding of the radiofrequency (RF) response of cold polar ice. We herein report on a series of radioglaciological measurements performed approximately 10 km north of Taylor Dome Station, Antarctica from Dec. 6, 2006 - Dec. 16, 2006. Using RF signals broadcast from: a) an englacial discone, submerged to a depth of 100 meters and broadcasting to a surface dual polarization horn receiver, and b) a dual-polarization horn antenna on the surface transmitting signals which reflect off the underlying bed and back up to the surface receiver, we have made time-domain estimates of both the real (index-of-refraction) and imaginary (attenuation length) components of the complex ice dielectric constant. We have also measured the uniformity of ice response along two orthogonal axes in the horizontal plane. We observe a wavespeed asymmetry of order 0.1%, projected onto the vertical propagation axis, consistent with some previous measurements, but somewhat lower than others. : replacement of previous arXiv version with published version