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Source: paper_references, paper_reference_links, observed 2026-08-12T13:37:18.773587Z
Paper Citation Record · LEDGER
Dynamics and modulation of cosmic ray modified magnetosonic waves in a galactic gaseous rotating plasma
As of 13 August 2026, this Paper Citation Record lists 22 of 22 outbound references and 0 inbound Pith citation observations for arXiv:2411.16286.
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Pith citing papers itemized under the disclosed page cap.
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22 of 22 outbound references displayed
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- unresolved6
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Outbound references
Observation 3676fbd3-6e51-46d0-b376-3a20dc6b60ff · outbound
This paper cites The coefficients M and N are modified due to the inclusion of cosmic ray pressure, which affects the growth of the instability.
Dynamics and modulation of cosmic ray modified magnetosonic waves in a galactic gaseous rotating plasma The coefficients M and N are modified due to the inclusion of cosmic ray pressure, which affects the growth of the instability
Reference 2
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-12T13:37:18.908836Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.
Observation 333cd997-23c3-4a26-bc80-5f1192ec3de6 · outbound
This paper cites an unresolved cited work.
Dynamics and modulation of cosmic ray modified magnetosonic waves in a galactic gaseous rotating plasma Unresolved cited work
Reference 3
- Resolution
- unresolved
- raw_fallback, observed 2026-08-12T13:37:19.121520Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.
Observation e209a66b-85b1-4572-ade1-9b5cd058b14f · outbound
This paper cites Due to the effect of cosmic ray modified pressure, cosmic ray diffusivity, and magnetic resistivity, the dissipation term in Eq.
Dynamics and modulation of cosmic ray modified magnetosonic waves in a galactic gaseous rotating plasma Due to the effect of cosmic ray modified pressure, cosmic ray diffusivity, and magnetic resistivity, the dissipation term in Eq
Reference 4
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-12T13:37:19.027366Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.
Observation 1225babe-1c26-4745-8e1a-d5595be1d4b6 · outbound
This paper cites frozen-in-field.
Dynamics and modulation of cosmic ray modified magnetosonic waves in a galactic gaseous rotating plasma frozen-in-field
Reference 5
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-12T13:37:18.961646Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.
Observation f3104a14-4993-4c5f-afc1-5f1c32882846 · outbound
This paper cites Now, we move on to find various types of soliton and shock wave solutions from Eq.
Dynamics and modulation of cosmic ray modified magnetosonic waves in a galactic gaseous rotating plasma Now, we move on to find various types of soliton and shock wave solutions from Eq
Reference 6
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-12T13:37:19.072854Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.
Observation 17e66686-2a40-43ec-9a19-b77e29f66401 · outbound
This paper cites frozen-in-field.
Dynamics and modulation of cosmic ray modified magnetosonic waves in a galactic gaseous rotating plasma frozen-in-field
Reference 7
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-12T13:37:19.057805Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.
Observation 119f0963-0d82-46c1-88f2-5e14171d21fa · outbound
This paper cites an unresolved cited work.
Dynamics and modulation of cosmic ray modified magnetosonic waves in a galactic gaseous rotating plasma Unresolved cited work
Reference 8
- Resolution
- unresolved
- raw_fallback, observed 2026-08-12T13:37:18.842636Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.
Observation a7426af1-b212-4ea2-b323-c73f8aa465e1 · outbound
This paper cites Similar assumptions have been made previously in many experi- mental situations 43,44.
Dynamics and modulation of cosmic ray modified magnetosonic waves in a galactic gaseous rotating plasma Similar assumptions have been made previously in many experi- mental situations 43,44
Reference 10
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-12T13:37:19.105869Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.
Observation 2ddad8e0-bd8c-471d-bcef-5cf466a0ba67 · outbound
This paper cites Therefore, Fig.
Dynamics and modulation of cosmic ray modified magnetosonic waves in a galactic gaseous rotating plasma Therefore, Fig
Reference 11
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-12T13:37:19.010966Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.
Observation 9ee9ce07-933f-4980-b437-1250f70845cd · outbound
This paper cites an unresolved cited work.
Dynamics and modulation of cosmic ray modified magnetosonic waves in a galactic gaseous rotating plasma Unresolved cited work
Reference 12
- Resolution
- unresolved
- raw_fallback, observed 2026-08-12T13:37:18.994698Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.
Observation 5dfb7145-3a3b-4af6-b383-f738122bf5b6 · outbound
This paper cites (15) The dispersion ( 15) includes the effect of the Coriolis force due to the rotation of the plasma.
Dynamics and modulation of cosmic ray modified magnetosonic waves in a galactic gaseous rotating plasma (15) The dispersion ( 15) includes the effect of the Coriolis force due to the rotation of the plasma
Reference 13
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-12T13:37:19.153572Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.
Observation b52a177b-93f1-455a-9d6a-37b363ce9f58 · outbound
This paper cites an unresolved cited work.
Dynamics and modulation of cosmic ray modified magnetosonic waves in a galactic gaseous rotating plasma Unresolved cited work
Reference 14
- Resolution
- unresolved
- raw_fallback, observed 2026-08-12T13:37:18.977084Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.
Observation 49047cb5-cea0-4a39-ae77-aab64f299ae7 · outbound
This paper cites an unresolved cited work.
Dynamics and modulation of cosmic ray modified magnetosonic waves in a galactic gaseous rotating plasma Unresolved cited work
Reference 15
- Resolution
- unresolved
- raw_fallback, observed 2026-08-12T13:37:19.138397Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.
Observation e71122b7-3119-4e29-b394-c5554a053086 · outbound
This paper cites (53) The first-order rational rogue solution ( 53) reveals that a significant amount of magnetosonic wave energy is con- centrated in a relatively small area in space.
Dynamics and modulation of cosmic ray modified magnetosonic waves in a galactic gaseous rotating plasma (53) The first-order rational rogue solution ( 53) reveals that a significant amount of magnetosonic wave energy is con- centrated in a relatively small area in space
Reference 17
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- raw_fallback, observed 2026-08-12T13:37:18.889677Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.
Observation 28636e1d-5166-4830-9315-ddbe16538ee2 · outbound
This paper cites an unresolved cited work.
Dynamics and modulation of cosmic ray modified magnetosonic waves in a galactic gaseous rotating plasma Unresolved cited work
Reference 18
- Resolution
- unresolved
- raw_fallback, observed 2026-08-12T13:37:18.872144Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.
Observation 2dd8ed5b-3d7d-4848-8767-85a57028abbb · outbound
This paper cites In other words, the parameters κ0 and η0 in the present model yield the formation of shock structures.
Dynamics and modulation of cosmic ray modified magnetosonic waves in a galactic gaseous rotating plasma In other words, the parameters κ0 and η0 in the present model yield the formation of shock structures
Reference 21
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-12T13:37:19.091033Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.
Observation 5fcca186-4f8a-4174-80bb-a645d96eb5e4 · outbound
This paper cites It has been reported that the second-order rogue waves absorb more energy from the surrounding waves than the first-order rogue waves do, making them spikier than the first-order.
Dynamics and modulation of cosmic ray modified magnetosonic waves in a galactic gaseous rotating plasma It has been reported that the second-order rogue waves absorb more energy from the surrounding waves than the first-order rogue waves do, making them spikier than the first-order
Reference 22
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-12T13:37:18.828021Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.
Observation 5bb5dd16-14cf-4a83-9615-92d8210b0dee · outbound
This paper cites The waves become unstable due to the increase in the values of the parameters η and κ.
Dynamics and modulation of cosmic ray modified magnetosonic waves in a galactic gaseous rotating plasma The waves become unstable due to the increase in the values of the parameters η and κ
Reference 23
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-12T13:37:18.811996Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.
Observation a88093c7-c183-4d2a-8dde-086d0905bf69 · outbound
This paper cites The graphical representations of such profiles have been displayed in Fig.
Dynamics and modulation of cosmic ray modified magnetosonic waves in a galactic gaseous rotating plasma The graphical representations of such profiles have been displayed in Fig
Reference 38
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- verified fuzzy
- raw_fallback, observed 2026-08-12T13:37:19.042589Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.
Observation 54e17ab9-0d57-42c2-89a5-0aae4ea5b830 · outbound
This paper cites The study of such low-frequency waves and the modulation of sinusoidal waves, which describe various physical phenomena in plasma, is quite natural.
Dynamics and modulation of cosmic ray modified magnetosonic waves in a galactic gaseous rotating plasma The study of such low-frequency waves and the modulation of sinusoidal waves, which describe various physical phenomena in plasma, is quite natural
Reference 46
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-12T13:37:18.946174Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.
Observation 2fbad94b-588a-4d4a-8b7f-e9d1f0a4a14b · outbound
This paper cites However, in our case where M N > 0, the region carries bright (unstable) envelope solitons in the presence of small external perturbation.
Dynamics and modulation of cosmic ray modified magnetosonic waves in a galactic gaseous rotating plasma However, in our case where M N > 0, the region carries bright (unstable) envelope solitons in the presence of small external perturbation
Reference 51
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-12T13:37:18.930236Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.
Observation 5defb3ca-6187-4538-adf5-748725aff1f3 · outbound
This paper cites Initially, the typical first-order rogue wave profiles |B1| are plotted against X and T for two differ- ent values of Ω 0 in Fig.
Dynamics and modulation of cosmic ray modified magnetosonic waves in a galactic gaseous rotating plasma Initially, the typical first-order rogue wave profiles |B1| are plotted against X and T for two differ- ent values of Ω 0 in Fig
Reference 53
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-12T13:37:18.857489Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.
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