Table 2.
Evaluation of the different terms of the ponderomotive force and the induced Karpman–Washimi magnetic field B2.
Environments | ωpe/|Ωe| | βe | κ |
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Mκ/MMB − 1 | References |
---|---|---|---|---|---|---|---|
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|||||||
CL | 1.0 − 1.6 | 4 − 20 (−4) | 1.8 − 4.0 | 0.002%−0.072% | 0.003%−0.117% | 0.005%−0.205% | 1, 2 |
SW (0.25 AU) | 40 − 90 | 0.07 − 0.7 | 2 − 6 | 0.2%−18% | 0.3%−23% | 0.5%−38% | 3, 4, 5, 6 |
SW (1 AU) | 100 − 140 | 0.6 − 2.0 | 2 − 6 | 1%−18% | 2%−23% | 4%−38% | 3, 4, 5, 6 |
MSh | 20 − 60 | 0.3 − 0.7 | 2.5 − 4.0 | 1%−8% | 2%−11% | 3%−19% | 7, 8 |
MPa | 9 − 12 | 0.08 − 0.10 | 6 − 9 | 0.1%−0.2% | 0.2%−0.4% | 0.3%−0.7% | 7, 9 |
MTaLb | 2 − 7 | 2 − 5 (−3) | 5 − 7 | 0.004%−0.015% | 0.006%−0.025% | 0.011%−0.044% | 10, 11 |
(40 Re − 100 Re) | |||||||
MTaLb | 10 − 17 | 0.02 − 0.05 | 5 − 7 | 0.04%−0.15% | 0.06%−0.25% | 0.11%−0.44% | 10, 11 |
(160 Re − 200 Re) | |||||||
PSh | 10 − 40 | 0.4 − 1.0 | 3 − 5 | 1%−5% | 2%−8% | 3%−13% | 11, 12 |
(60 Re − 100 Re) | |||||||
PSh | 30 − 60 | 0.6 − 1.5 | 3 − 5 | 2%−5% | 3%−8% | 5%−13% | 11, 12 |
(160 Re − 200 Re) | |||||||
PCu | 10 − 50 | 0.4 − 10 | 2.0 − 3.5 | 2%−18% | 3%−23% | 6%−38% | 13 |
IH | 200 − 1000 | 30 − 350 | 1.6 − 1.9 | – | – | – | 14, 15 |
Ring current | 9 − 70 | 2 − 200 | 5.5 − 6.5 | – | – | – | 16 |
Near MTa | 14 − 48 | 1.7 − 5.4 | 2.4 − 4.5 | – | – | – | 17 |
(7 Re − 20 Re) |
Notes. The relative difference of the ponderomotive force terms for the Kappa and Maxwellian case is expressed as a percentage for a range of typical values of the parameters ωpe/|Ωe|, βe, and κ, with ω/|Ωe| = 0.1 for a variety of spatial conditions indicated by their abbreviations, which are as follows: coronal loops(CL); solar wind (SW); magnetosheath (MSh); magnetopause (Mpa); magnetotail lobes (MTaLb); plasma sheet (PSh); polar cusps (PCu); inner heliosheath (IH). The numbers in parentheses represent the magnitude order. The ponderomotive temporal factor and the induced Karpman–Washimi magnetization share the same column.
References. (1) Brooks et al. (2021); (2) Vocks et al. (2008); (3) Matteini et al. (2012); (4) Wilson et al. (2018); (5) Livadiotis (2015); (6) Bale et al. (2016); (7) Phan et al. (1994); (8) Ogasawara et al. (2013); (9) Kirpichev et al. (2021); (10) Lui & Krimigis (1983); (11) Slavin et al. (1985); (12) Kletzing (2003); (13) Ren et al. (2023); (14) Livadiotis et al. (2022); (15) Burlaga et al. (2006); (16) Pisarenko et al. (2002); (17) Runov et al. (2015).
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