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PreprintarXiv licencearXiv

Synergy between laser linewidth and frequency chirp in mesospheric magnetometry based on the sodium laser guide star

Abstract

Mesospheric sodium magnetometry with a laser guide star measures the geomagnetic field near 90~km. Its sensitivity hinges on laser linewidth and chirp, yet prior work optimized these two parameters only separately. We use velocity-resolved density-matrix simulations of Larmor-synchronous pulsed Na D2 pumping to scan both parameters jointly. Linewidth and chirp exhibit a synergy: when chirping carries the recoil-mitigation role, the return flux stays within 1\% of its peak across linewidths of 2--10~MHz. The flux-optimal chirp is 0.19 MHz/upmu s, one fifth of the continuous-wave rate; this synergy guides high-sensitivity mesospheric magnetometer design.

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BibTeX
@misc{yang2026synergy,
  title = {{Synergy between laser linewidth and frequency chirp in mesospheric magnetometry based on the sodium laser guide star}},
  author = {Yucheng Yang and Chunyang Lei and Kai Guo and Shuai Wang},
  howpublished = {arXiv},
  year = {2026},
  month = oct,
  doi = {10.48550/arxiv.2608.28466},
  eprint = {2608.28466},
  archivePrefix = {arXiv},
  url = {https://arxiv.org/abs/2608.28466},
}
RIS
TY  - UNPB
TI  - Synergy between laser linewidth and frequency chirp in mesospheric magnetometry based on the sodium laser guide star
AU  - Yucheng Yang
AU  - Chunyang Lei
AU  - Kai Guo
AU  - Shuai Wang
PY  - 2026
DA  - 2026/10/13
PB  - arXiv
DO  - 10.48550/arxiv.2608.28466
UR  - https://arxiv.org/abs/2608.28466
AB  - Mesospheric sodium magnetometry with a laser guide star measures the geomagnetic field near 90~km. Its sensitivity hinges on laser linewidth and chirp, yet prior work optimized these two parameters only separately. We use velocity-resolved density-matrix simulations of Larmor-synchronous pulsed Na D_2 pumping to scan both parameters jointly. Linewidth and chirp exhibit a synergy: when chirping carries the recoil-mitigation role, the return flux stays within 1\% of its peak across linewidths of 2--10~MHz. The flux-optimal chirp is 0.19 MHz/upmu s, one fifth of the continuous-wave rate; this synergy guides high-sensitivity mesospheric magnetometer design.
ER  -