Spectral model used in the simulations of Mars halo and disc, adapted from Dennerl et al. (2006). We note the emission process involved, the original incoming solar wind ion species, or the participating molecular species involved, the emission energy, the atomic transition involved, and the photon fluxes used for scaling the model. Note, we take the fluxes (Dennerl et al. 2006), without considering the upper and lower energy bounds in that work.
| Index . | Label . | Emission . | Solar wind . | Energy . | Transition . | Fluxes . | |
|---|---|---|---|---|---|---|---|
| . | . | process . | ion . | (eV) . | . | Disc . | Halo . |
| . | . | . | . | . | . | (|$\rm 10^{-6}\, cm^{-2}\, s^{-1}$|) . | |
| 1 | C52 | CX | |$\rm C^{6+}$| | 367.6 | 2p |$\rightarrow$| 1s | 11.0 | 9.1 |
| 2 | C45 | CX | |$\rm C^{5+}$| | 378.5 | 5p |$\rightarrow$| 1s | 2.8 | 8.4 |
| 3 | N22 | F | |$\rm N_{2}$| | 394.0 | |$3\, \sigma _{g}\, \rightarrow$| 1s | 5.8 | 1.4 |
| 4 | C53 | CX | |$\rm C^{6+}$| | 435.6 | 3p |$\rightarrow$| 1s | 1.9 | 7.9 |
| 5 | C54 | CX | |$\rm C^{6+}$| | 459.4 | 4p |$\rightarrow$| 1s | 5.7 | 5.3 |
| 6 | C55 | CX | |$\rm C^{6+}$| | 470.4 | 5p |$\rightarrow$| 1s | 2.7 | 5.5 |
| 7 | N62 | CX | |$\rm N^{7+}$| | 500.3 | 2p |$\rightarrow$| 1s | 4.5 | 7.1 |
| 8 | CO2b | F | |$\rm CO_{2}$| | 523.5 | |$3\, \sigma _{u}\rightarrow$| 1s | 21.7 | 3.6 |
| 9 | CO2a | F | |$\rm CO_{2}$| | 527.7 | |$1\, \pi _{g}\rightarrow$| 1s | 23.2 | 3.5 |
| 10 | O6f | CX | |$\rm O^{7+}$| | 560.9 | 2|$\rm ^{1}P_{1}$||$\, \rightarrow \, 1\rm ^{1}S_{0}$| | 4.2 | 5.3 |
| 11 | O6i | CX | |$\rm O^{7+}$| | 568.5 | 2|$\rm ^{3}P_{1}$||$\, \rightarrow \, 1\rm ^{1}S_{0}$| | 1.2 | 2.2 |
| 12 | O6r | CX | |$\rm O^{7+}$| | 574.0 | 2|$\rm ^{3}S_{1}$||$\, \rightarrow \, 1\rm ^{1}S_{0}$| | 7.0 | 1.4 |
| 13 | N63 | CX | |$\rm N^{7+}$| | 593.0 | 3p |$\rightarrow$| 1s | 2.4 | 22.0 |
| 14 | O72 | CX | |$\rm O^{8+}$| | 653.6 | 2p |$\rightarrow$| 1s | 4.3 | 7.4 |
| 15 | O65 | CX | |$\rm O^{7+}$| | 712.5 | 5p |$\rightarrow$| 1s | 0.4 | 6.2 |
| 16 | O74 | CX | |$\rm O^{8+}$| | 817.0 | 4p |$\rightarrow$| 1s | 0.4 | 1.6 |
| 17 | Ne72 | F, CX|$^a$| | |$\rm Ne^{8+}$| | 872.5 | 2p |$\rightarrow$| 1s | 0.5 | 3.8 |
| Index . | Label . | Emission . | Solar wind . | Energy . | Transition . | Fluxes . | |
|---|---|---|---|---|---|---|---|
| . | . | process . | ion . | (eV) . | . | Disc . | Halo . |
| . | . | . | . | . | . | (|$\rm 10^{-6}\, cm^{-2}\, s^{-1}$|) . | |
| 1 | C52 | CX | |$\rm C^{6+}$| | 367.6 | 2p |$\rightarrow$| 1s | 11.0 | 9.1 |
| 2 | C45 | CX | |$\rm C^{5+}$| | 378.5 | 5p |$\rightarrow$| 1s | 2.8 | 8.4 |
| 3 | N22 | F | |$\rm N_{2}$| | 394.0 | |$3\, \sigma _{g}\, \rightarrow$| 1s | 5.8 | 1.4 |
| 4 | C53 | CX | |$\rm C^{6+}$| | 435.6 | 3p |$\rightarrow$| 1s | 1.9 | 7.9 |
| 5 | C54 | CX | |$\rm C^{6+}$| | 459.4 | 4p |$\rightarrow$| 1s | 5.7 | 5.3 |
| 6 | C55 | CX | |$\rm C^{6+}$| | 470.4 | 5p |$\rightarrow$| 1s | 2.7 | 5.5 |
| 7 | N62 | CX | |$\rm N^{7+}$| | 500.3 | 2p |$\rightarrow$| 1s | 4.5 | 7.1 |
| 8 | CO2b | F | |$\rm CO_{2}$| | 523.5 | |$3\, \sigma _{u}\rightarrow$| 1s | 21.7 | 3.6 |
| 9 | CO2a | F | |$\rm CO_{2}$| | 527.7 | |$1\, \pi _{g}\rightarrow$| 1s | 23.2 | 3.5 |
| 10 | O6f | CX | |$\rm O^{7+}$| | 560.9 | 2|$\rm ^{1}P_{1}$||$\, \rightarrow \, 1\rm ^{1}S_{0}$| | 4.2 | 5.3 |
| 11 | O6i | CX | |$\rm O^{7+}$| | 568.5 | 2|$\rm ^{3}P_{1}$||$\, \rightarrow \, 1\rm ^{1}S_{0}$| | 1.2 | 2.2 |
| 12 | O6r | CX | |$\rm O^{7+}$| | 574.0 | 2|$\rm ^{3}S_{1}$||$\, \rightarrow \, 1\rm ^{1}S_{0}$| | 7.0 | 1.4 |
| 13 | N63 | CX | |$\rm N^{7+}$| | 593.0 | 3p |$\rightarrow$| 1s | 2.4 | 22.0 |
| 14 | O72 | CX | |$\rm O^{8+}$| | 653.6 | 2p |$\rightarrow$| 1s | 4.3 | 7.4 |
| 15 | O65 | CX | |$\rm O^{7+}$| | 712.5 | 5p |$\rightarrow$| 1s | 0.4 | 6.2 |
| 16 | O74 | CX | |$\rm O^{8+}$| | 817.0 | 4p |$\rightarrow$| 1s | 0.4 | 1.6 |
| 17 | Ne72 | F, CX|$^a$| | |$\rm Ne^{8+}$| | 872.5 | 2p |$\rightarrow$| 1s | 0.5 | 3.8 |
a This line is debatably from charge exchange, see the comment in table 2 of Koutroumpa et al. (2012), but here we keep the F assignment to align with the original publication.
Spectral model used in the simulations of Mars halo and disc, adapted from Dennerl et al. (2006). We note the emission process involved, the original incoming solar wind ion species, or the participating molecular species involved, the emission energy, the atomic transition involved, and the photon fluxes used for scaling the model. Note, we take the fluxes (Dennerl et al. 2006), without considering the upper and lower energy bounds in that work.
| Index . | Label . | Emission . | Solar wind . | Energy . | Transition . | Fluxes . | |
|---|---|---|---|---|---|---|---|
| . | . | process . | ion . | (eV) . | . | Disc . | Halo . |
| . | . | . | . | . | . | (|$\rm 10^{-6}\, cm^{-2}\, s^{-1}$|) . | |
| 1 | C52 | CX | |$\rm C^{6+}$| | 367.6 | 2p |$\rightarrow$| 1s | 11.0 | 9.1 |
| 2 | C45 | CX | |$\rm C^{5+}$| | 378.5 | 5p |$\rightarrow$| 1s | 2.8 | 8.4 |
| 3 | N22 | F | |$\rm N_{2}$| | 394.0 | |$3\, \sigma _{g}\, \rightarrow$| 1s | 5.8 | 1.4 |
| 4 | C53 | CX | |$\rm C^{6+}$| | 435.6 | 3p |$\rightarrow$| 1s | 1.9 | 7.9 |
| 5 | C54 | CX | |$\rm C^{6+}$| | 459.4 | 4p |$\rightarrow$| 1s | 5.7 | 5.3 |
| 6 | C55 | CX | |$\rm C^{6+}$| | 470.4 | 5p |$\rightarrow$| 1s | 2.7 | 5.5 |
| 7 | N62 | CX | |$\rm N^{7+}$| | 500.3 | 2p |$\rightarrow$| 1s | 4.5 | 7.1 |
| 8 | CO2b | F | |$\rm CO_{2}$| | 523.5 | |$3\, \sigma _{u}\rightarrow$| 1s | 21.7 | 3.6 |
| 9 | CO2a | F | |$\rm CO_{2}$| | 527.7 | |$1\, \pi _{g}\rightarrow$| 1s | 23.2 | 3.5 |
| 10 | O6f | CX | |$\rm O^{7+}$| | 560.9 | 2|$\rm ^{1}P_{1}$||$\, \rightarrow \, 1\rm ^{1}S_{0}$| | 4.2 | 5.3 |
| 11 | O6i | CX | |$\rm O^{7+}$| | 568.5 | 2|$\rm ^{3}P_{1}$||$\, \rightarrow \, 1\rm ^{1}S_{0}$| | 1.2 | 2.2 |
| 12 | O6r | CX | |$\rm O^{7+}$| | 574.0 | 2|$\rm ^{3}S_{1}$||$\, \rightarrow \, 1\rm ^{1}S_{0}$| | 7.0 | 1.4 |
| 13 | N63 | CX | |$\rm N^{7+}$| | 593.0 | 3p |$\rightarrow$| 1s | 2.4 | 22.0 |
| 14 | O72 | CX | |$\rm O^{8+}$| | 653.6 | 2p |$\rightarrow$| 1s | 4.3 | 7.4 |
| 15 | O65 | CX | |$\rm O^{7+}$| | 712.5 | 5p |$\rightarrow$| 1s | 0.4 | 6.2 |
| 16 | O74 | CX | |$\rm O^{8+}$| | 817.0 | 4p |$\rightarrow$| 1s | 0.4 | 1.6 |
| 17 | Ne72 | F, CX|$^a$| | |$\rm Ne^{8+}$| | 872.5 | 2p |$\rightarrow$| 1s | 0.5 | 3.8 |
| Index . | Label . | Emission . | Solar wind . | Energy . | Transition . | Fluxes . | |
|---|---|---|---|---|---|---|---|
| . | . | process . | ion . | (eV) . | . | Disc . | Halo . |
| . | . | . | . | . | . | (|$\rm 10^{-6}\, cm^{-2}\, s^{-1}$|) . | |
| 1 | C52 | CX | |$\rm C^{6+}$| | 367.6 | 2p |$\rightarrow$| 1s | 11.0 | 9.1 |
| 2 | C45 | CX | |$\rm C^{5+}$| | 378.5 | 5p |$\rightarrow$| 1s | 2.8 | 8.4 |
| 3 | N22 | F | |$\rm N_{2}$| | 394.0 | |$3\, \sigma _{g}\, \rightarrow$| 1s | 5.8 | 1.4 |
| 4 | C53 | CX | |$\rm C^{6+}$| | 435.6 | 3p |$\rightarrow$| 1s | 1.9 | 7.9 |
| 5 | C54 | CX | |$\rm C^{6+}$| | 459.4 | 4p |$\rightarrow$| 1s | 5.7 | 5.3 |
| 6 | C55 | CX | |$\rm C^{6+}$| | 470.4 | 5p |$\rightarrow$| 1s | 2.7 | 5.5 |
| 7 | N62 | CX | |$\rm N^{7+}$| | 500.3 | 2p |$\rightarrow$| 1s | 4.5 | 7.1 |
| 8 | CO2b | F | |$\rm CO_{2}$| | 523.5 | |$3\, \sigma _{u}\rightarrow$| 1s | 21.7 | 3.6 |
| 9 | CO2a | F | |$\rm CO_{2}$| | 527.7 | |$1\, \pi _{g}\rightarrow$| 1s | 23.2 | 3.5 |
| 10 | O6f | CX | |$\rm O^{7+}$| | 560.9 | 2|$\rm ^{1}P_{1}$||$\, \rightarrow \, 1\rm ^{1}S_{0}$| | 4.2 | 5.3 |
| 11 | O6i | CX | |$\rm O^{7+}$| | 568.5 | 2|$\rm ^{3}P_{1}$||$\, \rightarrow \, 1\rm ^{1}S_{0}$| | 1.2 | 2.2 |
| 12 | O6r | CX | |$\rm O^{7+}$| | 574.0 | 2|$\rm ^{3}S_{1}$||$\, \rightarrow \, 1\rm ^{1}S_{0}$| | 7.0 | 1.4 |
| 13 | N63 | CX | |$\rm N^{7+}$| | 593.0 | 3p |$\rightarrow$| 1s | 2.4 | 22.0 |
| 14 | O72 | CX | |$\rm O^{8+}$| | 653.6 | 2p |$\rightarrow$| 1s | 4.3 | 7.4 |
| 15 | O65 | CX | |$\rm O^{7+}$| | 712.5 | 5p |$\rightarrow$| 1s | 0.4 | 6.2 |
| 16 | O74 | CX | |$\rm O^{8+}$| | 817.0 | 4p |$\rightarrow$| 1s | 0.4 | 1.6 |
| 17 | Ne72 | F, CX|$^a$| | |$\rm Ne^{8+}$| | 872.5 | 2p |$\rightarrow$| 1s | 0.5 | 3.8 |
a This line is debatably from charge exchange, see the comment in table 2 of Koutroumpa et al. (2012), but here we keep the F assignment to align with the original publication.
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