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The result is a fluid Eulerian perturbation generated by translating the entire equilibrium phase-space distribution function through ${\xi }_x$:Here $\Delta$ follows the displaced flux tube. Magnetic flux freezing carries the tube and its particles across the equilibrium pressure gradient. To leading order the tube changes neither its field strength nor its length by enough to alter the particle phase-space distribution function: these changes are smaller by plasma beta or $L_p/R$. Parallel streaming remains within the same displaced tube, on which the original equilibrium phase-space distribution function was uniform. It therefore cannot erase the displacement-generated contrast between adjacent tubes. This is why the term $v_{\parallel }\delta b_x{\partial }_x{f}_{0\alpha }$ in c exactly cancels the apparent parallel relaxation of $-{\xi }_x{\partial }_x{f}_{0\alpha }$. No collisional restoration of a Maxwell-Boltzmann distribution is needed.

Both mechanisms can extract free energy from an equilibrium pressure gradient in unfavorable magnetic field-line curvature, but the dynamics retained here is the macroscopic electromagnetic displacement of a flux tube. It depends on the total pressure gradient, including electron and ion contributions, and it does not require an ion temperature gradient specifically. Its stable branch has $\omega \sim k_{\parallel }{v}_A$; with low plasma beta, this is much faster than ion parallel streaming at the same $k_{\parallel }$.

The familiar ion-temperature-gradient instability is a slower drift-scale instability. In its usual electrostatic ordering the Boltzmann electron response is established by rapid electron parallel motion, while ion magnetic drifts, ion temperature evolution and polarization drift provide the instability dynamics. A representative ordering isThe last two expressions specify scales rather than exact geometric factors; $L_{T_i}^{-1}=-d\ln T_{0i}/dx$. The present leading kinetic magnetohydrodynamics system drops these relative species drifts and their finite-gyroradius corrections. It also retains the perturbed field direction, which enforces the advected-distribution cancellation in c; a rapid electron streaming rate alone cannot turn that cancellation into a Boltzmann electron response on an unperturbed field.

To recover ion-temperature-gradient instability physics, take the slow, nearly electrostatic limit $|\omega |/(k_{\parallel }{v}_A)\ll 1$, retain magnetic curvature drift, gradient-B drift and polarization drift in low-flow drift kinetics or gyrokinetics, and allow a sufficiently strong destabilizing ion temperature gradient. At long perpendicular wavelengths one may still have $k_{\perp }{\rho }_i\ll 1$, provided the leading nonzero ion polarization is kept; at $k_{\perp }{\rho }_i=O(1)$ full finite Larmor radius effects are needed. There is no contradiction between a drift-scale ion-temperature-gradient instability and the macroscopic interchange instability derived here: they use different asymptotic balances.