Radiation mechanism of twin kilohertz quasi-periodic oscillations in neutron star low-mass X-ray binaries

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Table 1.

Comparison of the characteristic parameters.

	The corona loop of the Sun	The corona around the NS
r_c (cm)	10⁹ ∼ 10¹⁰^(a)	10⁶ ∼ 10⁷^(b)

n (cm⁻³)	10⁸ ∼ 10¹⁰^(a)	10¹⁸ ∼ 10²⁰^(c)

B(G)	10 ∼ 100 ^(a)	10⁸ ∼ 10⁹^(d)

ν (Hz)	0.001 ∼ 1 ^(a)	10² ∼ 10³^(d)

Notes. This table lists the characteristic parameters of the Corona loop of the Sun and the corona around the NS in a LMXB. The number density of electrons is considered as the indicative number density of the plasma in the corona around the NS in a LMXBs.

^(a)

Zimovets et al. (2021);

^(b)

Karpouzas et al. (2020);

^(c)

Zhang et al. (2017);

^(d)

Wijnands (2006).

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