Corrigendum: Relativistically upshifted higher harmonic generation via relativistic flying mirrors (Plasma Physics and Controlled Fusion (2018) 60 (074007) DOI: 10.1088/1361-6587/aac068)
| Autor: | Koga, JK, Bulanov, SV, Esirkepov, TZ, Kando, M, Bulanov, SS, Pirozhkov, AS |
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| Jazyk: | angličtina |
| Rok vydání: | 2018 |
| Předmět: | |
| Zdroj: | Koga, JK; Bulanov, SV; Esirkepov, TZ; Kando, M; Bulanov, SS; & Pirozhkov, AS. (2018). Corrigendum: Relativistically upshifted higher harmonic generation via relativistic flying mirrors (Plasma Physics and Controlled Fusion (2018) 60 (074007) DOI: 10.1088/1361-6587/aac068). Plasma Physics and Controlled Fusion, 60(9), 099501-099501. doi: 10.1088/1361-6587/aad012. Lawrence Berkeley National Laboratory: Retrieved from: http://www.escholarship.org/uc/item/1mz2w24m Plasma Physics and Controlled Fusion, vol 60, iss 9 |
| DOI: | 10.1088/1361-6587/aac068). |
| Popis: | © 2018 IOP Publishing Ltd. In the calculation of the reflection coefficient for the partial reflection of an electromagnetic wave from a breaking plasma wave in section 2.1 Low Intensity regime (as ≤ 1), an incorrect value for γph was used. The two sentences after equation (3) should be corrected to Taking θ = 0 and using equation (2) giving γph ≈ 2.1 for Np = 1 and ωs/ωpe = 1.57 we get that Rδ ≈ 9.47 × 10-2. This can be seen to be in rough agreement with the ratio of the reflected spectrum broad peak around 15≲kx/ks ≲ 24 (blue solid line) to that of the original pulse kx/ks ≈1 (thick solid line) in figure 4. In addition, upon closer examination of figure 6, the last sentence in section 2.2. Near-relativistic Intensity regime (as ≈ 1) should be corrected to It can be seen that the ratio of the reflected spectrum region aound kx/ks ≈10 (blue solid line) to that of the original pulse kx/ks ≈1 (thick solid line) in figure 6 is roughly 10 times lower than that of the low intensity case. These modifications do not change our conclusions. |
| Databáze: | OpenAIRE |
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