Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria | Paper Citation Record

Observation 6f93ac43-acc6-4e9d-9e8c-6e43ef5e56e5 · outbound

This paper cites F ′ = G′ = 0, it is clear that Q > 0 implies δ2HC > 0.

Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria F ′ = G′ = 0, it is clear that Q > 0 implies δ2HC > 0

Reference 1

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Observation bd76a2d8-17cc-47e1-aa98-200f5e2f8617 · outbound

This paper cites Here the set of dynamical variables, say u, are the mass density ρ the ﬂuid velocity v and the generalized magnetic ﬁeld B∗ suggested in [ 38], given by B∗ = B +d2 e∇ × (∇ × B ρ ).

Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria Here the set of dynamical variables, say u, are the mass density ρ the ﬂuid velocity v and the generalized magnetic ﬁeld B∗ suggested in [ 38], given by B∗ = B +d2 e∇ × (∇ × B ρ )

Reference 2

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Observation 9e55a35e-45e4-4cce-b185-d977104a1cfb · outbound

This paper cites Terry, Rev.

Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria Terry, Rev

Reference 3

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T11:36:59.294643Z

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Observation 2b774a32-0149-44b2-ae8f-c1e5c2792acc · outbound

This paper cites In this case, the ﬂow is purely toroidal, but there is poloidal current created by the electrons.

Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria In this case, the ﬂow is purely toroidal, but there is poloidal current created by the electrons

Reference 4

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T11:36:59.626576Z

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Observation 0964e7d6-a356-47f5-bfad-c661fbb54ff7 · outbound

This paper cites Wahlberg, and A.

Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria Wahlberg, and A

Reference 5

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Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria Unresolved cited work

Reference 6

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Observation ee4c2935-d410-472c-8573-c1a4f805d7a4 · outbound

This paper cites Hence, a simple way to get rid of the indeﬁniteness is to assume δρ =δBφ = ∇ ×δv⊥ = 0.

Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria Hence, a simple way to get rid of the indeﬁniteness is to assume δρ =δBφ = ∇ ×δv⊥ = 0

Reference 7

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Observation f6866567-d10a-4782-9fc0-beb8e646e6b5 · outbound

This paper cites and then try to eliminate the explicit appearance of δBφ and δv⊥ into δ2HC by other means.

Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria and then try to eliminate the explicit appearance of δBφ and δv⊥ into δ2HC by other means

Reference 8

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Observation 3c1cc117-8b44-4023-94a7-4d956df27a78 · outbound

This paper cites This is a standard procedure to ob- tain simpliﬁed forms of the Lyapunov functional and im- proved stability criteria (e.g.

Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria This is a standard procedure to ob- tain simpliﬁed forms of the Lyapunov functional and im- proved stability criteria (e.g

Reference 9

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T11:36:59.554395Z

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Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria Unresolved cited work

Reference 10

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Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria Unresolved cited work

Reference 11

Resolution: unresolved; raw_fallback, observed 2026-08-14T11:36:59.173184Z

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Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria Unresolved cited work

Reference 12

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Observation 124ab53a-9c54-465d-bf17-d404d325eda2 · outbound

This paper cites Ishida, H.

Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria Ishida, H

Reference 13

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Observation f32dfbf1-895b-41ca-bb0f-fc9efa11c435 · outbound

This paper cites The most important advantage of our formulation can be seen though, after employing the Lagrange-Euler map: ﬁrst because (.

Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria The most important advantage of our formulation can be seen though, after employing the Lagrange-Euler map: ﬁrst because (

Reference 14

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T11:36:59.481978Z

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Observation 3d499e0c-2a21-4332-b249-18d30283b92e · outbound

This paper cites problem- atic.

Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria problem- atic

Reference 15

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Observation cd5acd5d-def7-4192-a136-2e3d09aa1068 · outbound

This paper cites Eule- rianize.

Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria Eule- rianize

Reference 16

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Observation 65e00300-1980-4762-8e14-f7aa5f2a3f5f · outbound

This paper cites The impact of the Hall term on tokamak plasmas.

Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria The impact of the Hall term on tokamak plasmas

Reference 17

Resolution: verified exact; local_arxiv, observed 2026-08-14T11:36:58.502865Z

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Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria Unresolved cited work

Reference 18

Resolution: unresolved; raw_fallback, observed 2026-08-14T11:36:59.090530Z

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Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria Unresolved cited work

Reference 19

Resolution: unresolved; raw_fallback, observed 2026-08-14T11:36:59.410006Z

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Observation 9f119aa8-6852-4ce3-9231-7889bbb2a173 · outbound

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Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria Unresolved cited work

Reference 20

Resolution: unresolved; raw_fallback, observed 2026-08-14T11:36:59.062488Z

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Observation a061c353-8bed-439b-8610-f8f95b2e6f94 · outbound

This paper cites Holm, Phys.

Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria Holm, Phys

Reference 21

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T11:36:59.048538Z

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Observation f135b305-716d-4225-aa38-3e6b844e0319 · outbound

This paper cites Hirota, Z.

Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria Hirota, Z

Reference 22

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T11:36:59.034619Z

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Observation 673732dd-9c3e-479d-ba4d-ac971763b7e0 · outbound

This paper cites Torasso and E.

Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria Torasso and E

Reference 23

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T11:36:59.019892Z

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Observation 51ea1844-9c19-48cd-a7d6-38cfb643f761 · outbound

This paper cites The same holds also for terms of the form bi · (cj × ck), since (cj × ck) is normal to the characteristic surfaces at each point, if not zero.

Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria The same holds also for terms of the form bi · (cj × ck), since (cj × ck) is normal to the characteristic surfaces at each point, if not zero

Reference 24

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T11:36:59.337873Z

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Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria Unresolved cited work

Reference 25

Resolution: unresolved; raw_fallback, observed 2026-08-14T11:36:59.322456Z

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Observation 2abf425f-f780-4c18-a226-075e903edd6e · outbound

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Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria Unresolved cited work

Reference 26

Resolution: unresolved; raw_fallback, observed 2026-08-14T11:36:59.308005Z

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Observation c425e46e-e073-4696-9b59-8e9d3f468102 · outbound

This paper cites Lüst, Fortschr.

Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria Lüst, Fortschr

Reference 27

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T11:36:58.963719Z

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Observation f3bbbeb3-5247-45bb-a7f9-c430898907be · outbound

This paper cites Wagner, Plasma Phys.

Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria Wagner, Plasma Phys

Reference 28

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Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria Unresolved cited work

Reference 29

Resolution: unresolved; raw_fallback, observed 2026-08-14T11:36:58.935081Z

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Observation 23d01716-79fa-4a04-adda-8f4029be15a3 · outbound

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Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria Unresolved cited work

Reference 30

Resolution: unresolved; raw_fallback, observed 2026-08-14T11:36:59.598798Z

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Observation 2fe21898-b83b-4ffb-af77-3688d24e1b0a · outbound

This paper cites It is not diﬃcult to adjust the free parameters in ( 35) to make conditions ( 28)–( 29) to be satisﬁed everywhere in the plasma.

Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria It is not diﬃcult to adjust the free parameters in ( 35) to make conditions ( 28)–( 29) to be satisﬁed everywhere in the plasma

Reference 31

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T11:36:59.613080Z

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Observation 9ae851b3-5bf9-482a-a032-43e16da9ff87 · outbound

This paper cites Lazzaro, and E.

Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria Lazzaro, and E

Reference 32

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T11:36:59.234611Z

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Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria Unresolved cited work

Reference 33

Resolution: unresolved; raw_fallback, observed 2026-08-14T11:36:59.218848Z

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Observation 3c7ee7d6-c322-41a1-9ba4-3fcee3281671 · outbound

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Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria Unresolved cited work

Reference 34

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Observation 8e27582e-56d9-4890-9058-fcc6da8aa0d4 · outbound

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Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria Unresolved cited work

Reference 35

Resolution: unresolved; raw_fallback, observed 2026-08-14T11:36:58.849206Z

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Observation a192b62d-8b0e-4f08-8d89-32c6b8532f32 · outbound

This paper cites Andreussi, P.

Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria Andreussi, P

Reference 36

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T11:36:58.835481Z

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Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria Unresolved cited work

Reference 37

Resolution: unresolved; raw_fallback, observed 2026-08-14T11:36:58.821644Z

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Observation beb74d64-e32f-4d7b-ab35-314ae22d37f2 · outbound

This paper cites Barnes, Physics of Plasmas 9, 560 (2002).

Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria Barnes, Physics of Plasmas 9, 560 (2002)

Reference 38

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Observation 8dc92883-66c8-432f-801e-ebe6759b7a00 · outbound

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Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria Unresolved cited work

Reference 39

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Observation a17417f2-f553-458b-9c32-ff7d1b9f8c5d · outbound

This paper cites Andrés P.

Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria Andrés P

Reference 40

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T11:36:59.105624Z

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Observation eaed0d56-a89e-4dda-8018-4be1ffe253ec · outbound

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Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria Unresolved cited work

Reference 41

Resolution: unresolved; raw_fallback, observed 2026-08-14T11:36:58.764562Z

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Observation d8c3115f-dbc9-40ca-9d73-0effd8feadb0 · outbound

This paper cites Andreussi, P.

Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria Andreussi, P

Reference 42

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T11:36:58.750486Z

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Observation 2ed1cebf-a40f-408f-8549-5e3a880d2ce2 · outbound

This paper cites Hameiri and R.

Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria Hameiri and R

Reference 43

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T11:36:59.076782Z

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Observation 5ab98027-ccc6-4559-b51a-91a1116b078b · outbound

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Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria Unresolved cited work

Reference 44

Resolution: unresolved; raw_fallback, observed 2026-08-14T11:36:59.539826Z

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Observation 44215563-e2a0-4d16-9d9f-c3925236e269 · outbound

This paper cites Tassi, P.

Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria Tassi, P

Reference 45

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T11:36:58.710260Z

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Observation 8c069209-2bd2-44d2-a83a-e08f771eedec · outbound

This paper cites Tassi, T.

Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria Tassi, T

Reference 46

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T11:36:58.696371Z

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Observation ad099f80-53e6-4a5a-b6b8-c570141dc1a7 · outbound

This paper cites As a ﬁnal point we stress that this stability criterion is genera l enough to capture a large variety of modes as long as k+’s are large enough.

Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria As a ﬁnal point we stress that this stability criterion is genera l enough to capture a large variety of modes as long as k+’s are large enough

Reference 47

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T11:36:59.525745Z

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Observation cf98d27d-4e19-44f3-bb73-16d261b01ee8 · outbound

This paper cites Ilgisonis, Fusion Technology, 35:1T, 170-174 (1999).

Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria Ilgisonis, Fusion Technology, 35:1T, 170-174 (1999)

Reference 48

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T11:36:59.005886Z

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Observation 63bb1fc7-2cef-4717-a2a4-088799a44c92 · outbound

This paper cites Elsasser and P.

Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria Elsasser and P

Reference 49

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T11:36:58.992134Z

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Observation 351623c5-d824-45cf-a783-e724503cdfd4 · outbound

This paper cites Spiess and K.

Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria Spiess and K

Reference 50

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T11:36:58.978002Z

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Observation 23b48f08-492a-4cfb-9e78-6b9609064b4d · outbound

This paper cites Hameiri, Phys.

Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria Hameiri, Phys

Reference 51

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T11:36:58.622149Z

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Observation 71c25226-319d-4782-b983-036387bc8f6b · outbound

This paper cites Kimura and P.

Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria Kimura and P

Reference 52

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T11:36:58.949695Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 4c85fd7f-fcfc-4a64-af97-12219f34f8e5 · outbound

This paper cites an unresolved cited work.

Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria Unresolved cited work

Reference 53

Resolution: unresolved; raw_fallback, observed 2026-08-14T11:36:58.594041Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation b6394525-7bba-4dfe-adb0-6680ddd45520 · outbound

This paper cites Lingam, P.

Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria Lingam, P

Reference 54

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T11:36:58.921139Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation b3ee2910-826e-4b93-aa9f-e65431e0a9cc · outbound

This paper cites an unresolved cited work.

Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria Unresolved cited work

Reference 55

Resolution: unresolved; raw_fallback, observed 2026-08-14T11:36:58.906548Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 5db617c4-ba58-4d07-ac44-edf9710ebae7 · outbound

This paper cites Lingam, G.

Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria Lingam, G

Reference 56

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T11:36:58.891801Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 1c449002-14b6-4f3e-b21b-18f3bb88f164 · outbound

This paper cites an unresolved cited work.

Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria Unresolved cited work

Reference 57

Resolution: unresolved; raw_fallback, observed 2026-08-14T11:36:58.877584Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 17ee1452-70a1-4b81-80d1-427cbc35fd6b · outbound

This paper cites an unresolved cited work.

Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria Unresolved cited work

Reference 58

Resolution: unresolved; raw_fallback, observed 2026-08-14T11:36:58.863530Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 518aa7d9-12a2-42b4-bb12-6e73cad0e634 · outbound

This paper cites Lingam, P.

Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria Lingam, P

Reference 62

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T11:36:58.807602Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 57023173-baab-4360-96b1-9dab1a7966a6 · outbound

This paper cites an unresolved cited work.

Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria Unresolved cited work

Reference 63

Resolution: unresolved; raw_fallback, observed 2026-08-14T11:36:58.792799Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 1ba38018-8561-4fbb-a321-4a2f5351fb8d · outbound

This paper cites an unresolved cited work.

Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria Unresolved cited work

Reference 64

Resolution: unresolved; raw_fallback, observed 2026-08-14T11:36:58.778628Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 46e5c709-62f3-42c5-8122-7b0942555016 · outbound

This paper cites an unresolved cited work.

Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria Unresolved cited work

Reference 67

Resolution: unresolved; raw_fallback, observed 2026-08-14T11:36:58.736757Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 6d9e6901-3d65-4750-a586-4f2e0a7695d2 · outbound

This paper cites Andreussi, P.

Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria Andreussi, P

Reference 68

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T11:36:58.723629Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 873c52bf-4f5e-47c8-aac7-5b9013521306 · outbound

This paper cites Hameiri, Phys.

Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria Hameiri, Phys

Reference 71

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T11:36:58.681090Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 402640cc-30ea-43d8-806d-357d816130e5 · outbound

This paper cites an unresolved cited work.

Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria Unresolved cited work

Reference 72

Resolution: unresolved; raw_fallback, observed 2026-08-14T11:36:58.666418Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 6802743b-78f3-45a1-8656-5e0720b2f0a5 · outbound

This paper cites an unresolved cited work.

Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria Unresolved cited work

Reference 73

Resolution: unresolved; raw_fallback, observed 2026-08-14T11:36:58.652154Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation bd560253-a234-4e8a-bed9-835896125801 · outbound

This paper cites Yoshida and E.

Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria Yoshida and E

Reference 74

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T11:36:58.637172Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation bb2ae16f-9005-48c6-b0f9-156a920a8407 · outbound

This paper cites an unresolved cited work.

Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria Unresolved cited work

Reference 76

Resolution: unresolved; raw_fallback, observed 2026-08-14T11:36:58.608039Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 87b4ad23-93d6-41e8-bfda-53c65e4ce141 · outbound

This paper cites Newcomb, Ann.

Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria Newcomb, Ann

Reference 78

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T11:36:58.578881Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 15271645-d28f-45a6-a1ef-d6ae6b3f6927 · outbound

This paper cites Hameiri, Phys.

Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria Hameiri, Phys

Reference 79

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T11:36:58.563718Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation dabdf25c-7a30-4a0d-ab5b-e5963ff9876d · outbound

This paper cites Newcomb, Nucl.

Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria Newcomb, Nucl

Reference 80

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T11:36:58.549798Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 3a4209f4-f50a-48d0-a15a-1188e661178a · outbound

This paper cites This is equivalent to imposing x′ = x, after performing a single ﬂuid Lagrange-Euler map (which involves the unperturbed trajectories, e.g.

Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria This is equivalent to imposing x′ = x, after performing a single ﬂuid Lagrange-Euler map (which involves the unperturbed trajectories, e.g

Reference 81

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T11:36:59.496409Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 39a2d51b-cead-4809-b93d-e6315efc8a8f · outbound

This paper cites an unresolved cited work.

Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria Unresolved cited work

Reference 82

Resolution: unresolved; raw_fallback, observed 2026-08-14T11:36:59.424672Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation b0380de3-351c-4a22-a3eb-cda90c54d7c6 · outbound

This paper cites Lagrangian Formalism for a System Composed of Sev- eral Fluids Interacting through Electromagnetic Forces.

Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria Lagrangian Formalism for a System Composed of Sev- eral Fluids Interacting through Electromagnetic Forces

Reference 83

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T11:36:58.534553Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 3aaeaa8d-ca1f-4c40-ab25-217fb9f4ba66 · outbound

This paper cites an unresolved cited work.

Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria Unresolved cited work

Reference 84

Resolution: unresolved; raw_fallback, observed 2026-08-14T11:36:59.438454Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation caf407b3-9c6a-48c7-a14c-0ebd3ceda128 · outbound

This paper cites an unresolved cited work.

Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria Unresolved cited work

Reference 85

Resolution: unresolved; raw_fallback, observed 2026-08-14T11:36:58.519030Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 1aced50d-31af-47c6-8dd9-b2e65d4584ed · outbound

This paper cites In view of this condition, the term that contains Φ 1 in W can be eliminated upon 13 integrating by parts.

Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria In view of this condition, the term that contains Φ 1 in W can be eliminated upon 13 integrating by parts

Reference 87

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T11:36:59.453037Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation b5b57ed3-8017-4f26-aacf-3eb831fd9d4d · outbound

This paper cites Note that the term containing ∇Φ 1 can be neglected in view of ∇ · (ρη ) = 0 and η · ˆ n ⏐ ⏐ ∂D = 0.

Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria Note that the term containing ∇Φ 1 can be neglected in view of ∇ · (ρη ) = 0 and η · ˆ n ⏐ ⏐ ∂D = 0

Reference 104

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T11:36:59.381515Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 2a6e09df-cf27-4e8b-8157-77140e10cf75 · outbound

This paper cites an unresolved cited work.

Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria Unresolved cited work

Reference 105

Resolution: unresolved; raw_fallback, observed 2026-08-14T11:36:59.395761Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation c00ecbbb-8d31-4ec9-967d-56dc92124aba · outbound

This paper cites an unresolved cited work.

Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria Unresolved cited work

Reference 115

Resolution: unresolved; raw_fallback, observed 2026-08-14T11:36:59.510829Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation b9231ac9-c897-4fa8-a23c-e8dc08addfb0 · outbound

This paper cites ( 117) along ∇φ we ﬁnd ∇(rBφ) · (∇ψ∗ × ∇φ) = 0 , ⇔rBφ =F (ψ∗).

Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria ( 117) along ∇φ we ﬁnd ∇(rBφ) · (∇ψ∗ × ∇φ) = 0 , ⇔rBφ =F (ψ∗)

Reference 116

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T11:36:59.366964Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 29e87552-f0dc-4294-b1a8-72964e3d2571 · outbound

This paper cites an unresolved cited work.

Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria Unresolved cited work

Reference 118

Resolution: unresolved; raw_fallback, observed 2026-08-14T11:36:59.352495Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

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