Table A.3
Comparison with previous studies regarding source locations and resonant electron energy.
| Reference | Type of events (number) | Source locationa (°) | Energy (keV) |
|---|---|---|---|
| This work | Io-A (5) | 160–170 | 2–6 |
| Io-B (5) | 177–192 | 3–7 | |
| Io-C (12) | 273–328 | 2–9 | |
| Io-D (48) | 50–122 | 7–16 | |
| non-Io-A (3) | 161–186 | 15–22 | |
| non-Io-C (5) | 251–339 | 5–13 | |
| non-Io-D (1) | 25–35 | 8–14 | |
| Lamy et al. (2022b)b | Io-A (2) | 172–182 (1) | 5–13 |
| Io-B(3) | 2–6 | ||
| Io-C(2) | 5–13 | ||
| Io-D(4) | 4–16 | ||
| Martos et al. (2020)c | Io-A (1) | 177–180 | 10–15 |
| Io-B (1) | 180–192 | 1.6–4.4 | |
| Io-C (1) | 295 | 11 | |
| Imai et al. (2017b) | A source (2) | 163–183 | 0.5–11 |
b One Io-A emission is represented by the main UV spot, and other events represented by Io’s longitude are not listed here.
c The Io-D case in this paper is dubious and not listed here. We note that it has a more reasonable result in Lamy et al. (2022b).
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