Antarctic Surface Reflectivity Calculations and Measurements from the ANITA-4 and HiCal-2 Experiments
arXiv:1801.08909 · doi:10.1103/PhysRevD.98.042004
Abstract
The balloon-borne HiCal radio-frequency (RF) transmitter, in concert with the ANITA radio-frequency receiver array, is designed to measure the Antarctic surface reflectivity in the RF wavelength regime. The amplitude of surface-reflected transmissions from HiCal, registered as triggered events by ANITA, can be compared with the direct transmissions preceding them by O(10) microseconds, to infer the surface power reflection coefficient . The first HiCal mission (HiCal-1, Jan. 2015) yielded a sample of 100 such pairs, resulting in estimates of at highly-glancing angles (i.e., zenith angles approaching ), with measured reflectivity for those events which exceeded extant calculations. The HiCal-2 experiment, flying from Dec., 2016-Jan., 2017, provided an improvement by nearly two orders of magnitude in our event statistics, allowing a considerably more precise mapping of the reflectivity over a wider range of incidence angles. We find general agreement between the HiCal-2 reflectivity results and those obtained with the earlier HiCal-1 mission, as well as estimates from Solar reflections in the radio-frequency regime. In parallel, our calculations of expected reflectivity have matured; herein, we use a plane-wave expansion to estimate the reflectivity R from both a flat, smooth surface (and, in so doing, recover the Fresnel reflectivity equations) and also a curved surface. Multiplying our flat-smooth reflectivity by improved Earth curvature and surface roughness corrections now provides significantly better agreement between theory and the HiCal 2a/2b measurements.
arXiv commentsubmitted to Astropart. Phys
References in corpus (9)
- Observational Constraints on the Ultra-high Energy Cosmic Neutrino Flux from the Second Flight of the ANITA Experiment
- Erratum: Observational Constraints on the Ultra-high Energy Cosmic Neutrino Flux from the Second Flight of the ANITA Experiment
- The Antarctic Impulsive Transient Antenna Ultra-high Energy Neutrino Detector Design, Performance, and Sensitivity for 2006-2007 Balloon Flight
- Observation of Ultra-high-energy Cosmic Rays with the ANITA Balloon-borne Radio Interferometer
- Characteristics of Four Upward-pointing Cosmic-ray-like Events Observed with ANITA
- Energy and Flux Measurements of Ultra-High Energy Cosmic Rays Observed During the First ANITA Flight
- A Passive Probe for Subsurface Oceans and Liquid Water in Jupiter's Icy Moons
- A scintillator based muon and KLong detector for the Belle II experiment
- Dynamic tunable notch filters for the Antarctic Impulsive Transient Antenna (ANITA)
Cited by in corpus (9)
- Constraints on the ultra-high energy cosmic neutrino flux from the fourth flight of ANITA
- The Payload for Ultrahigh Energy Observations (PUEO): A White Paper
- Addressing , , muon and ANITA anomalies in a minimal -parity violating supersymmetric framework
- Coherent transition radiation from the geomagnetically-induced current in cosmic-ray air showers: Implications for the anomalous events observed by ANITA
- A search for IceCube events in the direction of ANITA neutrino candidates
- Explaining the ANITA events by a gauge model
- Long-baseline horizontal radio-frequency transmission through polar ice
- Experimental tests of sub-surface reflectors as an explanation for the ANITA anomalous events
- General Treatment of Reflection of Spherical Electromagnetic Waves from a Spherical Surface and its Implications for the ANITA Anomalous Polarity Events