Submitted:
01 April 2026
Posted:
02 April 2026
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Abstract
Keywords:
1. Introduction
1.1. Research Background: Refinement Exploration Based on Einstein's Theory
1.2. Comprehensive Comb of Historical Precision Measurements of Light Speed
1.3. Core Research Content: Micro-scale Exploration and Refined Measurement Scheme
2. Classic Derivation, Gradient Correction and Theoretical Correlation Analysis of the Speed of Light in a Vacuum
2.1. Vacuum/Interstellar Medium Form of Maxwell's Equations
2.2. Complete Classic Derivation Steps of the Speed of Light in a Vacuum
2.3. Derivation of Wavelength-Dependent Expressions of Permittivity and Permeability
2.3.1. Classic Electromagnetic Theory Level
2.3.2. Quantum Vacuum Physics Level
2.4. Derivation of the Speed of Light Correction Under Gradient Medium Density in Inhomogeneous Medium Scenarios
2.5. Wavelength Dependence of Interstellar Medium Permittivity : The Fundamental Cause of Differences in the Speed of Light
3. Mechanism and Quantitative Analysis of Multi-band Masking Effects of the Speed of Light and Proof of the Applicability of Allan Variance
3.1. Core Definitions and Theoretical Basis
- Atmospheric masking effect: Signal imbalance caused by atmospheric absorption/scattering [9];
- Error amplification factor: (: observation error of masking effect; : time difference corresponding to target speed of light difference) [12];
- Allan variance: Quantifies the stability of weak medium environments [7];
- Wavelength dependence base value: .
3.2. Quantification of Atmospheric Masking Effect Based on Edlén's Formula
3.3. Quantification of Surface Masking Effect
3.3.1. Proof of the Constraint of Allan Variance
3.4. In-depth Analysis of Observation Target Adaptability
3.4.1. Comparison Between Jupiter and Outer Planets in the main text as Table 1.
3.4.2. Comparison Between Jupiter and Saturn
3.4.3. Analysis of Rocky Planets (Mars, Venus)
3.5. Analysis of the Proportion of Effective Paths in Total Solar Eclipses on the De-masking Effect
4. Limitations of Masking Effects in Historical Classic Speed of Light Measurement
5. De-masking Measurement and Control Method
5.1. Three-stage Path Splitting
5.2. Two-dimensional Error Control Measures
5.2.1. Atmospheric Masking Compensation
5.2.2. Synchronization and Calibration of Surface De-masking
5.3. Technical Implementation Scheme of Multi-band "Same Path, Simultaneous Timing, Same Starting Point"
5.3.1. Same Path Design
5.3.2. Simultaneous Timing Design
5.3.3. Same Starting Point Design
5.4. Calculation of the Speed of Light After De-masking Combined with Edlén's Formula and Wavelength Dependence
6. Calculation of Multi-band Dependence of the Speed of Light in Multi-media
6.1. Calculation Basis and Parameters
6.2. Quantitative Calculation of and Speed of Light Measurement in Multi-media Under Multi-bands
6.3. Analysis of the Coupling Mechanism of the Wavelength Dependence of in Multi-media
6.3.1. Interstellar Medium: Weak Dust and Plasma Coupling
6.3.2. Earth's Atmosphere: Nitrogen/Oxygen Molecule Polarization Coupling
6.3.3. Water Medium: Water Molecule Dipole Moment Coupling
6.4. Comparison of Multi-band Speed of Light Sequences in Different Media in the main text as Table 4.
6.5. Application of Raman Spectroscopy in the Analysis of Jupiter's Outer Atmosphere
6.6. Extended Discussion: Hypothesis on Micro-scale Changes in the Speed of Light Between Different Galaxies
7. Predictive Calculation of Homologous Synchronous Multi-band Speed of Light for Astronomical Observations in 2026
7.1. List of Core Astronomical Phenomena and Dynamic Parameters in the main text as Table 5.
7.2. Prediction of Multi-band Arrival Time Differences at the Surface Under Occultation Mode
7.3. Prediction of Multi-band Arrival Sequence at the Surface
8. Preliminary Exploration of Global Network Coordinated Observation and Cross-validation Scheme
8.1. Layout of Coordinated Observation Network
8.2. Timing Synchronization Mechanism
8.3. Multi-dimensional Cross-validation
9. Error Analysis and Control
10. Decisive Experiment Design and Result Judgment
10.1. Core Objective
10.2. Judgment Standards
10.2.1. Positive Judgment (Clear Existence of Wavelength Dependence of Multi-band Propagation Delay)
10.2.2. Weakly Positive Judgment (Suspected Existence of Wavelength Dependence)
10.2.3. Negative Judgment (No Wavelength Dependence Found)
10.3. Scientific Significance of Different Results
11. Differences and Innovations from Similar Studies
11.1. Review of Similar Research Status
11.2. Core Innovations
12. Conclusions and Prospects
12.1. Main Conclusions
12.2. Prospects
- Conduct global coordinated observations according to the 2026 astronomical observation scheme;
- Upgrade observation technology (sampling rate HZ);
13. Patents
Author Contributions
Funding
Informed Consent Statement
Data Availability Statement
Acknowledgments
Conflicts of Interest
Abbreviations
Appendix A
Appendix A.1. Supplementary Derivation Steps of Gradient Correction for Maxwell's Equations
Appendix A.2. Numerical Verification Example of the Correction Term
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| Comparison Dimension | Jupiter | Uranus | Neptune | Core Advantages (Jupiter) |
| Distance from the Sun (AU) | 5.2 | 19.2 | 30.1 | Effective path proportion |
| Orbital period (years) | 11.9 | 84.0 | 164.8 | 6 occultation events in 2026 |
| Atmospheric characteristics | Hydrogen-helium dominated, weak disturbance | Icy atmosphere, moderate disturbance | Dense methane clouds, strong scattering | Weak coupling effect, accurate correction |
| Allan variance verification | Optimal stability of weak medium environment |
| Experiment Name | Observation Band | Same Path Design | Simultaneous Timing Design | De-masking Measures | Influence of Masking Effect | Core Limitations |
| Fizeau (1849) | Visible light (single) | No | No | None | Atmospheric masking (10 times) | Single band + unvalidated constancy of |
| Michelson (1879) | Visible light (single) | No | No | None | Surface masking (30 times) | Single band + uncompensated surface noise |
| Evenson (1972) | Infrared (single) | Yes | No | None | Weak | No multi-band comparison |
| Römer (1676) | Visible light (single) | Yes | No | None | Weak | Uncalibrated starting point |
| Radar echo method (1949) | Microwave (single) | No | No | Atmospheric refraction correction | Weak atmospheric masking | Unvalidated in microwave band |
| Gamma-ray burst (2003) | Gamma-ray + visible light | No | No | Subtract interstellar medium | None | Asynchronous path/timing |
| Target Band |
Wavelength (nm) |
Interstellar Medium | Interstellar Medium |
Speed of Light (m/s) |
| Extreme ultraviolet | 100 | 8.848 | 1.256 | 299930156.2 |
| Deep ultraviolet | 150 | 8.851 | 1.256 | 299900123.7 |
| Near ultraviolet | 350 | 8.852 | 1.256 | 299850088.9 |
| Blue light | 470 | 8.853 | 1.256 | 299800055.8 |
| Green light | 550 | 8.853 | 1.256 | 299775022.7 |
| Red light (reference) | 650 | 8.854 | 1.256 | 299792458.0 |
| Near infrared | 760 | 8.857 | 1.257 | 299749981.2 |
| Mid-infrared | 2000 | 8.865 | 1.257 | 299689912.5 |
| Medium Type | Speed of Light Sequence | Core Cause |
| Interstellar medium (equivalent vacuum) | Extreme ultraviolet → deep ultraviolet → near ultraviolet → blue light → green light → red light → near infrared → mid-infrared | increases with wavelength |
| Earth's atmosphere | Mid-infrared → near infrared → red light → green light → blue light → near ultraviolet → deep ultraviolet → extreme ultraviolet | Long-wave has small molecular polarization disturbance |
| Pure water | Mid-infrared → near infrared → blue light → near ultraviolet → green light → deep ultraviolet → extreme ultraviolet | Short-wave strongly excites dipole vibration |
| Experimental Scenario |
Date (Beijing Time) |
Target Celestial Body/Star | Dynamic Effective Path Length (m) | Extreme Ultraviolet Relative to Red Light Time Difference | Near Infrared Relative to Red Light Time Difference |
| Total Solar Eclipse | 2026-08-12 13:30-16:00 | Sun-Moon-Earth | ns (earlier arrival) | ns (delayed arrival) | |
| Jupiter Occultation (Core) | 2026-11-02 20:15-21:45 | HD 19445 (G0 type) | μs (earlier arrival) | μs (delayed arrival) | |
| Jupiter Occultation (Drill) | 2026-04-15 19:30-21:00 | HD 38858 (K1 type) | μs (earlier arrival) | μs (delayed arrival) | |
| Jupiter Occultation (Drill) | 2026-05-28 22:40-00:10 | HD 45342 (G8 type) | μs (earlier arrival) | μs (delayed arrival) | |
| Jupiter Occultation (Drill) | 2026-07-03 01:20-02:50 | HD 52141 (F9 type) | μs (earlier arrival) | μs (delayed arrival) | |
| Jupiter Occultation (Drill) | 2026-10-18 18:50-20:20 | HD 18357 (K2 type) | μs (earlier arrival) | μs (delayed arrival) | |
| Jupiter Occultation (Drill) | 2026-11-19 21:30-23:00 | HD 20123 (F8 type) | μs (earlier arrival) | μs (delayed arrival) |
| Error Source | Impact Magnitude on Total Solar Eclipse (ns) | Impact Magnitude on Jupiter Occultation (μs) | Control Scheme |
| Clock synchronization error | Cesium atomic clock + GPS correction | ||
| Atmospheric turbulence error | Adaptive optics system + turbulence model | ||
| Path positioning error | JPL ephemerides + GAIA star catalog | ||
| Surface vibration error | Active vibration isolation platform + multi-station calibration | ||
| Celestial body position error | Real-time update (interval s) | ||
| Equipment response error | Pre-calibration + response function compensation | ||
| Raman spectroscopy measurement error | Multi-channel detection + signal integration optimization |
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