Comparisons of observed and forward modeled Balmer-α intensities from WACCM-X and MSIS-00
From 2000 to 2001, ground-based geocoronal hydrogen Balmer-α (Hα) observations were obtained from Pine Bluff Observatory (PBO) in Wisconsin (43.07°N, 270.33°E) using a high spectral resolution (R ≈ 80,000) Fabry-Perot interferometer (FPI). In previous work, the PBO March 2000 observations have been...
| الحاوية / القاعدة: | Frontiers in Astronomy and Space Sciences |
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| المؤلفون الرئيسيون: | , , , , , , , |
| التنسيق: | مقال |
| اللغة: | الإنجليزية |
| منشور في: |
Frontiers Media S.A.
2026-04-01
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| الموضوعات: | |
| الوصول للمادة أونلاين: | https://www.frontiersin.org/articles/10.3389/fspas.2026.1643505/full |
