Inferring physical parameters of solar filaments from simultaneous longitudinal and transverse oscillations

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Table 1.

Longitudinal oscillation parameters and inferred magnetic field.

Reference	P_l	B	B_u	B_G	B_γ
		(min)	(G)	(G)	(G)	(G)
	(1)	79.8	22.6	31.1 $_{- 9.0}^{+ 3.6}$ $Mathematical equation: $ ^{+3.6}_{-9.0} $$	29.7 $_{- 8.2}^{+ 3.9}$ $Mathematical equation: $ ^{+3.9}_{-8.2} $$	28.3 $_{- 9.1}^{+ 4.5}$ $Mathematical equation: $ ^{+4.5}_{-9.1} $$
(2)	18.31	5.1	6.8 $_{- 2.1}^{+ 1.2}$ $Mathematical equation: $ ^{+1.2}_{-2.1} $$	5.0 $_{- 0.5}^{+ 0.5}$ $Mathematical equation: $ ^{+0.5}_{-0.5} $$	5.1 $_{- 0.5}^{+ 0.5}$ $Mathematical equation: $ ^{+0.5}_{-0.5} $$

Notes. References, longitudinal oscillation period (P_l), reported magnetic field strengths (B), and most probable magnetic field inferred using uniform (B_u), Gaussian (B_G), and gamma (B_γ) priors, with uncertainties at the 68% credible interval. (1) Mazumder et al. (2020), (2) Pan et al. (2025).

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