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pith:3CPOGD2K

pith:2026:3CPOGD2KWC3SSFF7VESVDYWJJ7
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Compact Dual-Polarization Schottky Barrier Diode Receivers for Submillimeter Wave Remote Sensing

Anders Emrich, Jan Stake, Olivier Auriacombe, Peter J. Sobis, Vladimir Drakinskiy

Co-optimized orthogonal E-field probes and subharmonic Schottky mixers deliver compact dual-polarization receivers with up to 34 dB isolation and 833 K noise temperature.

arxiv:2605.18330 v1 · 2026-05-18 · physics.ins-det · physics.app-ph

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\pithnumber{3CPOGD2KWC3SSFF7VESVDYWJJ7}

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Claims

C1strongest claim

the integrated dualpolarization receiver topology achieves excellent sensitivity in a highly compact package, offering an efficient and scalable solution for polarimetric applications in submillimeter-wave remote sensing

C2weakest assumption

The co-optimization and integration of the two orthogonal E-field probes with the subharmonic mixers does not introduce unaccounted losses, coupling, or fabrication variations that would degrade the reported isolation and noise performance in operational environments. (Abstract description of co-optimized integration and measured results)

C3one line summary

Compact dual-polarization Schottky barrier diode receivers at 315-650 GHz achieve up to 34 dB cross-polarization isolation, DSB noise temperatures down to 833 K, and Allan stability over 10 s in a single module with shared components.

References

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[1] P. Siegel, “Terahertz Technology,”IEEE Transactions on Microwave Theory and Techniques, vol. 50, no. 3, pp. 910–928, 2002, doi: 10.1109/22.989974 2002 · doi:10.1109/22.989974
[2] Matrix calculus and the Stokes parameters of polarized radiation, 1954 · doi:10.1119/1.1933670
[3] Fast radiative transfer approximating ice hydrometeor orientation and its implication on IWP retrievals, 2022 · doi:10.3390/rs14071594
[4] A general database of hydrometeor single scattering properties at microwave and sub-millimetre wavelengths, 2018 · doi:10.5194/essd-10-1301-
[5] Advanced terahertz frequency-domain ellipsometry instrumentation for in situ and ex situ applications, 2018 · doi:10.1109/tthz.2018.2814347

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Receipt and verification
First computed 2026-05-20T00:05:55.555410Z
Builder pith-number-builder-2026-05-17-v1
Signature Pith Ed25519 (pith-v1-2026-05) · public key
Schema pith-number/v1.0

Canonical hash

d89ee30f4ab0b72914bfa92551e2c94fe2003c2b37852771ec9cb64382b0ddf7

Aliases

arxiv: 2605.18330 · arxiv_version: 2605.18330v1 · doi: 10.48550/arxiv.2605.18330 · pith_short_12: 3CPOGD2KWC3S · pith_short_16: 3CPOGD2KWC3SSFF7 · pith_short_8: 3CPOGD2K
Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/3CPOGD2KWC3SSFF7VESVDYWJJ7 \
  | jq -c '.canonical_record' \
  | python3 -c "import sys,json,hashlib; b=json.dumps(json.loads(sys.stdin.read()), sort_keys=True, separators=(',',':'), ensure_ascii=False).encode(); print(hashlib.sha256(b).hexdigest())"
# expect: d89ee30f4ab0b72914bfa92551e2c94fe2003c2b37852771ec9cb64382b0ddf7
Canonical record JSON
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    "license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
    "primary_cat": "physics.ins-det",
    "submitted_at": "2026-05-18T12:47:50Z",
    "title_canon_sha256": "3e4bd960fb2bdc8af81877f1b110758bbd11e49576a0a80ae3752c122e06ef7c"
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