Table 1 Waves diagnosed through multi-station methods
From: Planetary-scale MLT waves diagnosed through multi-station methods: a review
Implements | Configurations | Diagnosed waves [f,s] | Interpretations |
|---|---|---|---|
He et al. (2018a) | #2 | [\(\frac{1}{12.4h}\),1] | an LSB of a tide-RWNM interaction |
He et al. (2018) | #1 | [\(\frac{1}{12.4h}\),2],[\(\frac{1}{11.6h}\),3] | M2 and an USB of a tide-RWNM interaction |
He and Chau (2019) | #8 | [\(\frac{1}{12.4h}\),1],[\(\frac{1}{11.6h}\),3],[\(\frac{1}{12.4h}\),2],[2cpd,1],[2cpd,2],[2cpd,3] | LSB and USB of tide-RWNM interactions, M2, and three solar tides |
Forbes et al. (2020) | #9 | [\(\frac{1}{2-4d}\), –1] | UFKWs |
He et al. (2020a) | #3,#1 | [\(\frac{1}{10d}\),1],[\(\frac{1}{6d}\),1],[\(\frac{1}{12.6h}\),1],[\(\frac{1}{11.4h}\),3],[\(\frac{1}{12.4h}\),2] | RWNMs, M2, LSB and USB of tide-RWNM interactions |
#1,#7 | [1cpd,1],[2cpd,2],[3cpd,3],[4cpd,4],[5cpd,5],[6cpd,6] | migrating tides | |
He et al. (2020c) | #1,#2 | [\(\frac{1}{16d}\),1],[\(\frac{1}{16d}\),2],[\(\frac{1}{10d}\),1],[\(\frac{1}{5-6d}\),1] | RWNMs and their interaction USB |
He et al. (2021a) | #4,#5,#6 | [\(\frac{1}{50h}\),3], [\(\frac{1}{46h}\),2] | Q2DWs |
He et al. (2021b) | #1 | [\(\frac{1}{41h}\),4], [\(\frac{1}{57h}\),–3], [\(\frac{1}{50h}\),3], [\(\frac{1}{46h}\),-2], [\(\frac{1}{46h}\),–3], [\(\frac{1}{16h}\),4], [\(\frac{1}{16h}\),-1], \(\big [\frac{1}{10h},5\big ]\), [\(\frac{1}{10h}\),0], [\(\frac{1}{41h}\),4], [\(\frac{1}{57h}\),-3], [\(\frac{1}{10h}\),-1], [\(\frac{1}{9h}\),6], [\(\frac{1}{7h}\),0] | Q2DWs, four migrating tides, and SWs of Q2DW-tide interactions |
He and Forbes (2022) | #1 | [\(\frac{1}{16d}\),1], [\(\frac{1}{4d}\),2], [\(\frac{1}{2d}\),2], [\(\frac{1}{7d}\),2], [\(\frac{1}{8d}\),2, [\(\frac{1}{6d}\),] | RWNMs, Q2DW, and RWNM secondary harmonic generation |
Forbes et al. (2021) | #5 | [\(\frac{1}{16h}\),4] | USB of a Q2DW-tide interaction |