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Analysis of Convective Instability in Dusty Ferromagnetic Fluids with Magnetic Field-Dependent Viscosity Under Fluid-Permeable Magnetic Boundaries Cover

Analysis of Convective Instability in Dusty Ferromagnetic Fluids with Magnetic Field-Dependent Viscosity Under Fluid-Permeable Magnetic Boundaries

Open Access
|Jun 2025

Figures & Tables

Fig. 1.

Geometrical Configuration
Geometrical Configuration

Fig. 2.

Graph between Nc vs χ at δ = 0.05, h1 = 3 and Das = 1
Graph between Nc vs χ at δ = 0.05, h1 = 3 and Das = 1

Fig. 3.

Graph between Nc vs Das at h1 = 3, χ = 10 and M3 = 5
Graph between Nc vs Das at h1 = 3, χ = 10 and M3 = 5

Fig. 4.

Graph between Nc vs δ at χ = 10, Das = 1 and h1 = 3
Graph between Nc vs δ at χ = 10, Das = 1 and h1 = 3

Fig. 5.

Graph between Nc vs h1 at Das = 10, χ = 10 and M3 = 5
Graph between Nc vs h1 at Das = 10, χ = 10 and M3 = 5

Fig. 7.

Graph between Nc vs M3 at χ = 1, Das = 1 and h1 = 3
Graph between Nc vs M3 at χ = 1, Das = 1 and h1 = 3

Fig. 6.

Graph between Nc vs M3 at δ = 0.03, Das = 1 and h1 = 3
Graph between Nc vs M3 at δ = 0.03, Das = 1 and h1 = 3

Variation of critical magnetic Rayleigh numbers Nc with M3, χ and δ at fixed h1 = 3 and Das = 1

h1 = 3Critical Magnetic Rayleigh Number Nc(ac2) at
χM3δ = 0.01δ = 0.03δ = 0.05δ = 0.07δ = 0.09
11412.4400 (7.7909)420.6071 (7.7909)428.7742 (7.7909)436.9413 (7.7909)445.1085 (7.7909)
5333.0876 (7.0576)364.8102 (7.0576)396.5328 (7.0576)428.2554 (7.0576)459.9781 (7.0576)
10321.2218 (6.6092)379.6257 (6.6092)438.0297 (6.6092)496.4336 (6.6092)554.8376 (6.6092)
15323.9978 (6.3847)408.5190 (6.3847)493.0402 (6.3847)577.5614 (6.3847)662.0825 (6.3847)
20331.3287 (6.2498)441.7716 (6.2498)552.2144 (6.2498)662.6573 (6.2498)773.1002 (6.2498)
101494.4820 (8.9375)504.2737 (8.9375)514.0654 (8.9375)523.8572 (8.9375)533.6489 (8.9375)
5342.8150 (7.3292)375.4640 (7.3292)408.1130 (7.3292)440.7621 (7.3292)473.4111 (7.3292)
10324.5245 (6.7147)383.5290 (6.7147)442.5334 (6.7147)501.5379 (6.7147)560.5423 (6.7147)
15325.7133 (6.4415)410.6820 (6.4415)495.6507 (6.4415)580.6194 (6.4415)665.5881 (6.4415)
20332.4015 (6.2855)443.2020 (6.2855)554.0025 (6.2855)664.8030 (6.2855)775.6035 (6.2855)
1031525.1702 (9.3988)535.5696 (9.3988)545.9690 (9.3988)556.3685 (9.3988)566.7679 (9.3988)
5345.3312 (7.4019)378.2199 (7.4019)411.1086 (7.4019)443.9972 (7.4019)476.8859 (7.4019)
10325.3216 (6.7407)384.4710 (6.7407)443.6204 (6.7407)502.7697 (6.7407)561.9191 (6.7407)
15326.1164 (6.4551)411.1902 (6.4551)496.2641 (6.4551)581.3379 (6.4551)666.4118 (6.4551)
20332.6499 (6.2938)443.5332 (6.2938)554.4166 (6.2938)665.2999 (6.2938)776.1832 (6.2938)
1051525.5497 (9.4046)535.9567 (9.4046)546.3636 (9.4046)556.7705 (9.4046)567.1774 (9.4046)
5345.3597 (7.4027)378.2512 (7.4027)411.1426 (7.4027)444.0340 (7.4027)476.9254 (7.4027)
10325.3305 (6.7410)384.4815 (6.7410)443.6325 (6.7410)502.7835 (6.7410)561.9345 (6.7410)
15326.1209 (6.4552)411.1959 (6.4552)496.2709 (6.4552)581.3459 (6.4552)666.4209 (6.4552)
20332.6527 (6.2939)443.5369 (6.2939)554.4212 (6.2939)665.3054 (6.2939)776.1896 (6.2939)

Comparison of Values from the Present Study with Existing Studies

Free-FreeRigid-Rigid
Present StudyDhiman [10]Present StudyDhiman [10]
Rc(ac2) Rc(ac2) Rc(ac2) Rc(ac2)
M1 = 1360.0088 (5.4644)342.52 (5.174)913.1268 (10.2291)889.15 (9.921)
M1 = 5126.5677 (5.8260)116.49 (5.319)313.1211 (10.5816)299.56 (10.06)

Variation of critical magnetic Rayleigh numbers Nc with h1, M3 and Das at fixed χ = 10 and δ = 0_03

χ = 10Critical Magnetic Rayleigh Number Nc(ac2) at
M = 3h1Das = 0Das = 10Das = 102Das = 103Das = 105
311058.2 (7.1019)1713.5 (10.3132)2257.1 (11.8650)2371.8 (12.1002)2385.8 (12.1272)
3352.7195 (7.1019)571.1730 (10.3132)752.3706 (11.8650)790.5888 (12.1002)795.2814 (12.1272)
5211.6317 (7.1019)342.7038 (10.3132)451.4224 (11.8650)474.3533 (12.1002)477.1689 (12.1272)
7151.1655 (7.1019)244.7884 (10.3132)322.4445 (11.8650)338.8238 (12.1002)340.8349 (12.1272)
9117.5732 (7.1019)190.3910 (10.3132)250.7902 (11.8650)263.5296 (12.1002)265.0938 (12.1272)
51998.5998 (6.5835)1660.7 (9.6886)2210.0 (11.1916)2325.7 (11.4193)2339.9 (11.4454)
3332.8666 (6.5835)553.5690 (9.6886)736.6527 (11.1916)775.2371 (11.4193)779.9737 (11.4454)
5199.7200 (6.5835)332.1414 (9.6886)441.9916 (11.1916)465.1422 (11.4193)467.9842 (11.4454)
7142.6571 (6.5835)237.2439 (9.6886)315.7083 (11.1916)332.2445 (11.4193)334.2744 (11.4454)
9110.9555 (6.5835)184.5230 (9.6886)245.5509 (11.1916)258.4124 (11.4193)259.9912 (11.4454)
1011010.8 (5.9857)1734.0 (9.0216)2332.5 (10.4899)2458.4 (10.7120)2473.8 (10.7375)
3336.9392 (5.9857)578.0082 (9.0216)777.4880 (10.4899)819.4643 (10.7120)824.6157 (10.7375)
5202.1635 (5.9857)346.8049 (9.0216)466.4928 (10.4899)491.6786 (10.7120)494.7694 (10.7375)
7144.4025 (5.9857)247.7178 (9.0216)333.2092 (10.4899)351.1990 (10.7120)353.4067 (10.7375)
9112.3131 (5.9857)192.6694 (9.0216)259.1627 (10.4899)273.1548 (10.7120)274.8719 (10.7375)
1511077.7 (5.7151)1875.3 (8.7376)2534.0 (10.1969)2672.5 (10.4175)2689.5 (10.4428)
3359.2290 (5.7151)625.0951 (8.7376)844.6717 (10.1969)890.8388 (10.4175)896.5038 (10.4428)
5215.5374 (5.7151)375.0570 (8.7376)506.8030 (10.1969)534.5033 (10.4175)537.9023 (10.4428)
7153.9553 (5.7151)267.8979 (8.7376)362.0022 (10.1969)381.7881 (10.4175)384.2159 (10.4428)
9119.7430 (5.7151)208.3650 (8.7376)281.5572 (10.1969)296.9463 (10.4175)298.8346 (10.4428)

j_ama-2025-0040_utab_001

SymbolExplanation
dDepth of the ferromagnetic fluid layer (m)
tTime variable (s)
TTemperature (K)
T0, T1Reference temperatures at z = 0 and z = d respectively (K)
rRadius of a dust particle (m)
mMass of a dust particle (kg)
NdNumber density of dust particles (particles/3)
NDisturbance to number density of dust particles (particles/3)
CptHeat capacity of dust particles (kJ/m3K)
CH,VSpecific heat at constant magnetic field and volume (kJ/m3K)
K1Thermal conductivity (wmK)
K2Pyromagnetic coefficient = –∂M/∂T at (T0, H0) (A/mK)
KStokes drag coefficient (kg/s)
DasDarcy number accounting for velocity slip
pFluid pressure (psi)
pPressure perturbation (psi)
qVelocity of the ferrofluid (m/s)
q′ = (u′, v′, w′)Velocity perturbation of the fluid (m/s)
qdDust particle velocity (m/s)
qd′ = (l′, r′, s′),Dust velocity disturbance (m/s)
gGravitational acceleration, g = (0,0,–g) (m/s2)
D/DtConvective (material) derivative (s−1)
kx1, ky1Horizontal wave numbers in x and y directions (m−1)
kOverall wave number, k = ✓(kx12 + ky12) (m−1)
k^ Unit vector in the vertical (z) direction
HMagnetic field vector (A/m)
H, H0, HextMagnitude of field, reference field, and external magnetic field (A/m)
HMagnetic field perturbation (A/m)
BMagnetic flux density (T)
BMagnitude of magnetic induction (T)
MMagnetization (A/m)
MMagnetization disturbance (A/m)
M0Magnetization at (H0, T0) (A/m)
bSubscript indicating base (equilibrium) state
Greek Symbols
αThermal expansion coefficient (K−1)
βConstant thermal gradient |dT/dz| (K/m)
vKinematic viscosity (m2/s)
μDynamic viscosity (kg/m·s
μ1Dynamic viscosity under ambient magnetic field (kg/m·s
μ0Magnetic permeability of vacuum (H/m)
ρFluid density (kg/m3)
ρ0Reference density at T0 (kg/m3)
ρDensity perturbation (kg/m3)
θTemperature fluctuation (K)
ωRate of growth of disturbances (s−1)
χMagnetic susceptibility = ∂M/∂H at (T0, H0)
Gradient (del) operator (m−1)
ϕPerturbation in magnetic scalar potential (A)
DOI: https://doi.org/10.2478/ama-2025-0040 | Journal eISSN: 2300-5319 | Journal ISSN: 1898-4088
Language: English
Page range: 327 - 336
Submitted on: Dec 28, 2024
|
Accepted on: May 3, 2025
|
Published on: Jun 30, 2025
In partnership with: Paradigm Publishing Services
Publication frequency: 4 issues per year

© 2025 Awneesh KUMAR, Pankaj KUMAR, Abhishek THAKUR, Mandeep KAUR, published by Bialystok University of Technology
This work is licensed under the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 License.