Skip to content
DraconiticResearch
Search Sources API
203,234 studies31 sourcesUpdated 26 min ago
PreprintCC BY-NC-SA 4.0arXiv

Exact spherical-wave forward model for radio reflection from stratified media and implications for the anomalous-polarity events observed by ANITA

Abstract

Radio detection of ultra-high energy particles relies on the propagation and reflection of broadband radio pulses at boundaries between natural media. In the Sommerfeld--Weyl treatment, a spherical wave is decomposed into plane-wave components and their reflection from a single homogeneous interface is calculated exactly. We extend that treatment to an arbitrary number of laterally uniform spherical layers. Both the spherical-wave decomposition of the source and the spherical geometry of the boundary are retained, while the reflection and transmission coefficients of the plane-wave components are replaced by the exact characteristic-matrix coefficients of the layered medium, evaluated at the local incidence angle on the spherical boundary. When the layer contrast is removed, the formalism recovers the single-boundary result to machine precision, and it reproduces the published spherical-surface reflectivity calculation to better than 1.1% at ten HiCal-2 elevation angles, with a mean deviation of 0.6%. We reproduce the measured HiCal-1 reflected pulses from their measured direct partners, with a best signed correlation of $0.83$ and a median of $0.70$ across $106$ pairs, of which $101$ show the expected polarity inversion. Applied to the six reported ANITA anomalous-polarity event geometries, the buried-layer refractive index required for a sign change of the reflection coefficient ranges from $1.68$ at the steepest event to $3.8−−5.4$ at the four near-horizon events. The full waveform calculation gives no non-inverted reflected pulse at any of these angles, showing that shallow, laterally uniform firn layering does not account for the polarity of the anomalous ANITA events. Because the formalism depends only on the complex refractive index of the medium, it applies more generally to isotropic, nonmagnetic stratified media, including ice, lunar regolith, and conducting layers.

Related

  1. Relativistic Spherical Accretion in Nonrotating Black Hole Spacetimes: Astrophysical Implications
    David Barrero-González, Alejandro Cruz-Osorio
    arXivPreprintCC BY 4.0Full textHigh-energy astrophysicsGravitation & general relativityarXiv
  2. Coherent radio bursts, polarity reversal, and quiescent emission from the M4V dwarf WW PsA
    Jackson Mitchell-Bolton, Laura Driessen, Tara Murphy +6
    arXivPreprintarXiv licenceFull textHigh-energy astrophysicsSolar & stellar physicsarXiv
  3. Cause of chromospheric opposite polarity intrusions discovered in Sunrise III/SCIP data: MURaM-ChE simulations point to twisted flux ropes
    Patrick A. Ondratschek, Damien F. Przybylski, Robert H. Cameron +33
    arXivPreprintCC BY-SA 4.0Full textSolar & stellar physicsarXiv
  4. The diversity of planetary climates in the Solar System as a basis for reflection and work on the study of exoplanet climates
    Olivier Planchon
    HALPreprintCC BY 4.0Full textPlanetary science & exoplanetsGeneral earth scienceHAL
  5. Anomalous Electric Fields in Earth's Turbulent Magnetosheath: Insights From 3D Hybrid Simulations
    Jeffersson A. Agudelo Rueda, Julia E. Stawarz, Luca Franci +3
    HALPreprintCC BY 4.0Full textPlanetary science & exoplanetsPlasma physicsHAL
BibTeX
@misc{dasgupta2026exact,
  title = {{Exact spherical-wave forward model for radio reflection from stratified media and implications for the anomalous-polarity events observed by ANITA}},
  author = {Paramita Dasgupta},
  howpublished = {arXiv},
  year = {2026},
  month = aug,
  doi = {10.48550/arxiv.2608.15989},
  eprint = {2608.15989},
  archivePrefix = {arXiv},
  url = {https://arxiv.org/abs/2608.15989},
  note = {CC BY-NC-SA 4.0},
}
RIS
TY  - UNPB
TI  - Exact spherical-wave forward model for radio reflection from stratified media and implications for the anomalous-polarity events observed by ANITA
AU  - Paramita Dasgupta
PY  - 2026
DA  - 2026/08/27
PB  - arXiv
DO  - 10.48550/arxiv.2608.15989
UR  - https://arxiv.org/abs/2608.15989
AB  - Radio detection of ultra-high energy particles relies on the propagation and reflection of broadband radio pulses at boundaries between natural media. In the Sommerfeld--Weyl treatment, a spherical wave is decomposed into plane-wave components and their reflection from a single homogeneous interface is calculated exactly. We extend that treatment to an arbitrary number of laterally uniform spherical layers. Both the spherical-wave decomposition of the source and the spherical geometry of the boundary are retained, while the reflection and transmission coefficients of the plane-wave components are replaced by the exact characteristic-matrix coefficients of the layered medium, evaluated at the local incidence angle on the spherical boundary. When the layer contrast is removed, the formalism recovers the single-boundary result to machine precision, and it reproduces the published spherical-surface reflectivity calculation to better than 1.1% at ten HiCal-2 elevation angles, with a mean deviation of 0.6%. We reproduce the measured HiCal-1 reflected pulses from their measured direct partners, with a best signed correlation of $0.83$ and a median of $0.70$ across $106$ pairs, of which $101$ show the expected polarity inversion. Applied to the six reported ANITA anomalous-polarity event geometries, the buried-layer refractive index required for a sign change of the reflection coefficient ranges from $1.68$ at the steepest event to $3.8−−5.4$ at the four near-horizon events. The full waveform calculation gives no non-inverted reflected pulse at any of these angles, showing that shallow, laterally uniform firn layering does not account for the polarity of the anomalous ANITA events. Because the formalism depends only on the complex refractive index of the medium, it applies more generally to isotropic, nonmagnetic stratified media, including ice, lunar regolith, and conducting layers.
ER  -