Interstellar Lattice Resonance: A Spectral Mask for  the Detection of 12.8 Hz Vacuum Drag in Voyager 1  S-Band Telemetry

Interstellar Lattice Resonance: A Spectral Mask for the Detection of 12.8 Hz Vacuum Drag in Voyager 1 S-Band Telemetry | Authorea try { document.documentElement.classList.add('js'); } catch (e) { } var _gaq = _gaq || []; _gaq.push(['_setAccount', 'G-8VDV14Y67G']); _gaq.push(['_trackPageview']); (function() { var ga = document.createElement('script'); ga.type = 'text/javascript'; ga.async = true; ga.src = ('https:' == document.location.protocol ? 'https://ssl' : 'http://www') + '.google-analytics.com/ga.js'; var s = document.getElementsByTagName('script')[0]; s.parentNode.insertBefore(ga, s); })(); Skip to main content Preprints Collections Wiley Open Research IET Open Research Ecological Society of Japan All Collections About About Authorea FAQs Contact Us Quick Search anywhere Search for preprint articles, keywords, etc. Search Search ADVANCED SEARCH SCROLL This is a preprint and has not been peer reviewed. Data may be preliminary. 19 February 2026 V1 Latest version Share on Interstellar Lattice Resonance: A Spectral Mask for the Detection of 12.8 Hz Vacuum Drag in Voyager 1 S-Band Telemetry Author : Heiko Grimberg 0009-0008-9039-4176 [email protected] Authors Info & Affiliations https://doi.org/10.22541/au.177153749.95402072/v1 166 views 75 downloads Contents Abstract Supplementary Material Information & Authors Metrics & Citations View Options References Figures Tables Media Share Abstract Since late 2025, the Voyager 1 spacecraft has primarily utilized its S-Band transmitter ($\approx 2.3$ GHz) due to technical constraints on the primary X-Band system. While this shift reduces data throughput, it inadvertently creates an ideal low-noise environment for detecting Ultra-Low Frequency (ULF) resonances in the Interstellar Medium (ISM). The Unified Chronofractal Field (UCF) theory, a zero-parameter ($k=0$) cosmological framework, predicts a specific geometric decoherence frequency at $12.84$ Hz, arising from the interaction between the spacecraft's baryon mass and the 14th iteration of the vacuum lattice ($\nu^{14}$). This paper defines the exact spectral mask, signal-to-noise ratio (SNR) requirements, and integration times ($t > 3600$s) necessary to isolate this signature from the Deep Space Network (DSN) raw telemetry. Detection of this resonance would constitute the first direct local evidence of discrete spacetime topology outside the heliopause. This is a caption Supplementary Material File (17_voyager1_sband_lattice14_protocol_v1.0.pdf) Download 3.76 MB Information & Authors Information Version history V1 Version 1 19 February 2026 Copyright This work is licensed under a Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License Keywords deep space network (dsn) lattice resonance (12.84 hz) mars time drift vacuum refresh rate voyager 1 telemetry Authors Affiliations Heiko Grimberg 0009-0008-9039-4176 [email protected] UCF Research Group View all articles by this author Metrics & Citations Metrics Article Usage 166 views 75 downloads .FvxKWukQNSOunydq8rnd { width: 100px; } Citations Download citation Heiko Grimberg. Interstellar Lattice Resonance: A Spectral Mask for the Detection of 12.8 Hz Vacuum Drag in Voyager 1 S-Band Telemetry. Authorea . 19 February 2026. 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