Paper Citation Record · LEDGER

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT

As of 5 August 2026, this Paper Citation Record lists 75 of 75 outbound references and 1 inbound Pith citation observation for arXiv:2601.10675.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
2601.10675 v2

Coverage vector

measured 75 of 75 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-05-16T13:51:43.084134Z

measured 76 of 76 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-05T06:32:48.257954+00:00

measured 1 of 1 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-05-07T14:13:51.680688Z

measured 0 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: pith, observed 2026-05-12T10:41:31.975027Z

Reference resolution

75 of 75 outbound references displayed

verified exact1
verified fuzzy57
unresolved17
parse uncertain0
malformed identifier0
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External citation measurements

No source-named external measurement is stored.

Outbound references

Observation 21f4ebbe-752d-458b-b903-9c9477c613ea · outbound

This paper cites an unresolved cited work.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT Unresolved cited work

Reference 1

Resolution: unresolved; raw_fallback, observed 2026-05-16T13:52:57.283352Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 796f89e2-290f-4d31-bd89-903a763f3f0e · outbound

This paper cites N., Leisner, A., Antiochos, S.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT N., Leisner, A., Antiochos, S

Reference 2

Resolution: verified fuzzy; raw_fallback, observed 2026-05-16T13:52:57.291500Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation bc7fd97f-82a9-4ffc-afac-88e00de03a41 · outbound

This paper cites I., Scott, R.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT I., Scott, R

Reference 3

Resolution: verified fuzzy; raw_fallback, observed 2026-05-16T13:52:57.299091Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 155abc58-347e-458e-8336-c446c6d96358 · outbound

This paper cites M., et al.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT M., et al

Reference 4

Resolution: verified fuzzy; raw_fallback, observed 2026-05-16T13:52:57.318930Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 83b8d7d2-6959-4f1f-8614-a12ec75d0ef3 · outbound

This paper cites 2021, A & A, 650, A18.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT 2021, A & A, 650, A18

Reference 5

Resolution: verified fuzzy; raw_fallback, observed 2026-05-16T13:52:57.293837Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 0fdc5ad9-180a-4fd8-961a-7b94303b432e · outbound

This paper cites D., Goetz, K., Harvey, P.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT D., Goetz, K., Harvey, P

Reference 6

Resolution: verified fuzzy; raw_fallback, observed 2026-05-16T13:52:57.332235Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation b5e3ed1c-5c52-4ab9-a4da-7b53c45e02d2 · outbound

This paper cites J., Forsyth, R.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT J., Forsyth, R

Reference 7

Resolution: verified fuzzy; raw_fallback, observed 2026-05-16T13:52:57.325773Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 7a1a25f5-a866-461c-83bc-4975bba60575 · outbound

This paper cites 2024, A & A.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT 2024, A & A

Reference 8

Resolution: verified fuzzy; raw_fallback, observed 2026-05-16T13:52:57.316542Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation f7536cf0-09b9-46b3-8501-6d36da1be354 · outbound

This paper cites P ., Sorokina, D., Lani, A., & Poedts, S.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT P ., Sorokina, D., Lani, A., & Poedts, S

Reference 9

Resolution: verified fuzzy; raw_fallback, observed 2026-05-16T13:52:57.270865Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 78d8d9a0-75fd-4142-8b0e-9ad919ddce9d · outbound

This paper cites an unresolved cited work.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT Unresolved cited work

Reference 10

Resolution: unresolved; raw_fallback, observed 2026-05-16T13:52:57.285949Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 8dd4c069-0465-4ed5-a3ad-ef946734a7cb · outbound

This paper cites an unresolved cited work.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT Unresolved cited work

Reference 11

Resolution: unresolved; raw_fallback, observed 2026-05-16T13:52:57.296478Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 602a852b-bf49-4378-b6e0-e3e6028afcb7 · outbound

This paper cites an unresolved cited work.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT Unresolved cited work

Reference 12

Resolution: unresolved; raw_fallback, observed 2026-05-16T13:52:57.280977Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation c51d2c9a-b2a1-4efa-8b00-77084aeacaa2 · outbound

This paper cites M., Downs, C., Linker, J.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT M., Downs, C., Linker, J

Reference 13

Resolution: verified fuzzy; raw_fallback, observed 2026-05-16T13:52:57.328008Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 28ac3f6a-5d6b-42b2-a795-0881a01f1910 · outbound

This paper cites an unresolved cited work.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT Unresolved cited work

Reference 14

Resolution: unresolved; raw_fallback, observed 2026-05-16T13:52:57.275571Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 613a07e1-cb36-494b-b17c-c5f125e539b5 · outbound

This paper cites A., Caplan, R.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT A., Caplan, R

Reference 15

Resolution: verified fuzzy; raw_fallback, observed 2026-05-16T13:52:57.309633Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 94c4bb27-c584-4ffc-96ef-b3da505143bd · outbound

This paper cites I., van der Holst, B., et al.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT I., van der Holst, B., et al

Reference 16

Resolution: verified fuzzy; raw_fallback, observed 2026-05-16T13:52:57.301775Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 35c69212-54a1-42d8-8c6d-8437c037e6e8 · outbound

This paper cites S., Li, C.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT S., Li, C

Reference 17

Resolution: verified fuzzy; raw_fallback, observed 2026-05-16T13:52:57.307328Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation d283176c-78df-4486-a0f1-d0c0aa28940e · outbound

This paper cites S., Liu, X.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT S., Liu, X

Reference 18

Resolution: verified fuzzy; raw_fallback, observed 2026-05-16T13:52:57.321278Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 205829dc-f2e1-4dcd-ae06-676b5698bd9c · outbound

This paper cites S., Lv, J.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT S., Lv, J

Reference 19

Resolution: verified fuzzy; raw_fallback, observed 2026-05-16T13:52:57.304200Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 2e48e424-fc09-4ac1-a15f-c989aa353a85 · outbound

This paper cites S., Ma, X.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT S., Ma, X

Reference 20

Resolution: verified fuzzy; raw_fallback, observed 2026-05-16T13:52:57.278099Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation a0209855-7d1e-41df-9e03-e3d68e64da94 · outbound

This paper cites S., Wang, H.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT S., Wang, H

Reference 21

Resolution: verified fuzzy; raw_fallback, observed 2026-05-16T13:52:57.311936Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 86b52f64-1887-450e-bcf7-9e033d87f1d3 · outbound

This paper cites S., Xiang, C.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT S., Xiang, C

Reference 22

Resolution: verified fuzzy; raw_fallback, observed 2026-05-16T13:52:57.273132Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation e6e9de97-0008-47a7-beb9-e427686a42dc · outbound

This paper cites S., Y ang, L.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT S., Y ang, L

Reference 23

Resolution: verified fuzzy; raw_fallback, observed 2026-05-16T13:52:57.314239Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 1160516a-723c-4d95-81d9-296e6e20eb6e · outbound

This paper cites an unresolved cited work.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT Unresolved cited work

Reference 24

Resolution: unresolved; raw_fallback, observed 2026-05-16T13:52:57.330209Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 056419d9-9b9d-471d-9e56-59915a515c6c · outbound

This paper cites J., V elli, M.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT J., V elli, M

Reference 25

Resolution: verified fuzzy; raw_fallback, observed 2026-05-16T13:52:57.215012Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 8f7c1994-05de-43a0-b7cc-78d33c07c38a · outbound

This paper cites M., Owens, M., Macneil, A., & Lockwood, M.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT M., Owens, M., Macneil, A., & Lockwood, M

Reference 26

Resolution: verified fuzzy; raw_fallback, observed 2026-05-16T13:52:57.323274Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation ce29d000-5e6c-475c-83f5-88b5c2b031da · outbound

This paper cites V ., Carlsson, M., Hansteen, V.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT V ., Carlsson, M., Hansteen, V

Reference 27

Resolution: verified fuzzy; raw_fallback, observed 2026-05-16T13:52:57.288506Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation a6e964b0-164f-4c95-a2f9-bf2f8dc2dab7 · outbound

This paper cites P ., Cheung, M.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT P ., Cheung, M

Reference 28

Resolution: verified fuzzy; raw_fallback, observed 2026-05-16T13:52:57.219561Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 7574f8cb-ab1d-41d0-93e6-9d5a2cb0cb78 · outbound

This paper cites T., Abbett, W.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT T., Abbett, W

Reference 29

Resolution: verified fuzzy; raw_fallback, observed 2026-05-16T13:52:57.217167Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 04ec6828-e460-4658-bbbc-2e74b8804db3 · outbound

This paper cites 2025, ApJ, 993, 130.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT 2025, ApJ, 993, 130

Reference 30

Resolution: verified fuzzy; raw_fallback, observed 2026-05-16T13:52:57.194680Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation f4ed721f-f526-410b-9811-b461e1e67158 · outbound

This paper cites 2010, Proc.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT 2010, Proc

Reference 31

Resolution: verified fuzzy; raw_fallback, observed 2026-05-16T13:52:57.184400Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 0bc2a256-5a18-4697-9ea0-77404ba788b7 · outbound

This paper cites an unresolved cited work.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT Unresolved cited work

Reference 32

Resolution: unresolved; raw_fallback, observed 2026-05-16T13:52:57.186509Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 57eeab5e-80a2-48c5-95b7-556149ca5163 · outbound

This paper cites 2005, in Proc.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT 2005, in Proc

Reference 33

Resolution: verified fuzzy; raw_fallback, observed 2026-05-16T13:52:57.221751Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation d08ef60c-cb36-4521-a26f-0a557f3da27e · outbound

This paper cites an unresolved cited work.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT Unresolved cited work

Reference 34

Resolution: unresolved; raw_fallback, observed 2026-05-16T13:52:57.212558Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 3eaed6db-de8f-4fa5-bd1a-2a85ece1fb8a · outbound

This paper cites 2005, in LNCS 3514, V ol.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT 2005, in LNCS 3514, V ol

Reference 35

Resolution: verified fuzzy; raw_fallback, observed 2026-05-16T13:52:57.210379Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation ec937faf-5819-4ecf-870e-a338a4ce64ba · outbound

This paper cites 2013, in AIAA 2013-2589, 21th AIAA CFD Conference, San Diego (CA).

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT 2013, in AIAA 2013-2589, 21th AIAA CFD Conference, San Diego (CA)

Reference 36

Resolution: verified fuzzy; raw_fallback, observed 2026-05-16T13:52:57.192648Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 76a45229-e524-4fea-a913-3d034d01d31f · outbound

This paper cites C., Wang, H.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT C., Wang, H

Reference 37

Resolution: verified fuzzy; raw_fallback, observed 2026-05-16T13:52:57.190310Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 27d0d799-a5b5-4748-a127-586821960479 · outbound

This paper cites 2023, A & A, 675, A10 1.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT 2023, A & A, 675, A10 1

Reference 38

Resolution: verified fuzzy; raw_fallback, observed 2026-05-16T13:52:57.260543Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation a312baa9-d9bf-4520-8d69-b4322f1f024f · outbound

This paper cites A., Caplan, R.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT A., Caplan, R

Reference 39

Resolution: verified fuzzy; raw_fallback, observed 2026-05-16T13:52:57.205614Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation b1a1a9f3-1dfc-4075-8333-33ef96d20772 · outbound

This paper cites A., Heinemann, S.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT A., Heinemann, S

Reference 40

Resolution: verified fuzzy; raw_fallback, observed 2026-05-16T13:52:57.174469Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 31b94ba0-b3f3-4002-8106-27e573b28320 · outbound

This paper cites A., Miki ´c, Z., Biesecker, D.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT A., Miki ´c, Z., Biesecker, D

Reference 41

Resolution: verified fuzzy; raw_fallback, observed 2026-05-16T13:52:57.203518Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 269e0bb7-f977-42b4-92fb-7ee78069c5b4 · outbound

This paper cites I., et al.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT I., et al

Reference 42

Resolution: verified fuzzy; raw_fallback, observed 2026-05-16T13:52:57.208053Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 42270c00-4659-4973-a06a-69f3703795df · outbound

This paper cites J., Feng, X.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT J., Feng, X

Reference 43

Resolution: verified fuzzy; raw_fallback, observed 2026-05-16T13:52:57.201311Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation bed3b15e-7311-4302-a35f-b1eef19e298d · outbound

This paper cites an unresolved cited work.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT Unresolved cited work

Reference 44

Resolution: unresolved; raw_fallback, observed 2026-05-16T13:52:57.223907Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation ff576f5f-0d83-4172-b1b0-e8371c761163 · outbound

This paper cites an unresolved cited work.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT Unresolved cited work

Reference 45

Resolution: unresolved; raw_fallback, observed 2026-05-16T13:52:57.228429Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 7df41a6b-8d8c-416e-8c50-1fce0ab632cf · outbound

This paper cites an unresolved cited work.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT Unresolved cited work

Reference 46

Resolution: unresolved; raw_fallback, observed 2026-05-16T13:52:57.226249Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 9bc200e4-c519-469b-8328-267b99a84d88 · outbound

This paper cites I., Lionello, R., Downs, C., et al.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT I., Lionello, R., Downs, C., et al

Reference 47

Resolution: verified fuzzy; raw_fallback, observed 2026-05-16T13:52:57.196839Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 245d0245-133e-4ac4-897f-56f186eaf90c · outbound

This paper cites an unresolved cited work.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT Unresolved cited work

Reference 48

Resolution: unresolved; raw_fallback, observed 2026-05-16T13:52:57.188465Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation ecd2a6ee-405a-4ea0-9788-61e8597f7ed0 · outbound

This paper cites J., Bame, S.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT J., Bame, S

Reference 49

Resolution: verified fuzzy; raw_fallback, observed 2026-05-16T13:52:57.243755Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 0fe28f96-b367-4084-af45-070536b884dd · outbound

This paper cites an unresolved cited work.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT Unresolved cited work

Reference 50

Resolution: unresolved; raw_fallback, observed 2026-05-16T13:52:57.180252Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 22f17716-74c9-4033-b37d-f8044c52e2b9 · outbound

This paper cites 2025, RA S Tech.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT 2025, RA S Tech

Reference 51

Resolution: verified fuzzy; raw_fallback, observed 2026-05-16T13:52:57.182396Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 8f8c79ab-0a9c-4e85-9d98-a8eea3ea526f · outbound

This paper cites an unresolved cited work.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT Unresolved cited work

Reference 52

Resolution: unresolved; raw_fallback, observed 2026-05-16T13:52:57.176446Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 0ba0ea5c-850d-4f99-b230-dd434ba56901 · outbound

This paper cites 2026, Astronomy & Ast rophysics, 705, A86.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT 2026, Astronomy & Ast rophysics, 705, A86

Reference 53

Resolution: verified fuzzy; raw_fallback, observed 2026-05-16T13:52:57.236269Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 838cffb3-74c6-4ebc-8bef-bb5ffb232557 · outbound

This paper cites J., Arge, C.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT J., Arge, C

Reference 54

Resolution: verified fuzzy; raw_fallback, observed 2026-05-16T13:52:57.199050Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 6234fe0d-2065-407b-b5f2-a91175441da3 · outbound

This paper cites J., Lockwood, M., Riley, P ., & Linker, J.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT J., Lockwood, M., Riley, P ., & Linker, J

Reference 55

Resolution: verified fuzzy; raw_fallback, observed 2026-05-16T13:52:57.170651Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 874f516d-d2b6-44d8-a218-5f53d4472779 · outbound

This paper cites S., et al.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT S., et al

Reference 56

Resolution: verified fuzzy; raw_fallback, observed 2026-05-16T13:52:57.168735Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 6c5ef86a-1237-43e2-9fc0-65aaacce681f · outbound

This paper cites S., Réville, V ., & Strugarek, A.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT S., Réville, V ., & Strugarek, A

Reference 57

Resolution: verified fuzzy; raw_fallback, observed 2026-05-16T13:52:57.241559Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 65edc782-6163-4f20-b311-fd0b837e0b14 · outbound

This paper cites 2023, ApJ, 943, 124.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT 2023, ApJ, 943, 124

Reference 58

Resolution: verified fuzzy; raw_fallback, observed 2026-05-16T13:52:57.248375Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 64092a9a-a8c6-496a-9096-00daed8c63b3 · outbound

This paper cites 2022, ApJ, 936 , 19 Réville, V.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT 2022, ApJ, 936 , 19 Réville, V

Reference 59

Resolution: verified fuzzy; raw_fallback, observed 2026-05-16T13:52:57.246213Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 45860ea4-c5a9-4c54-a4f8-bda5e39f4a1a · outbound

This paper cites 2019, ApJ, 884, 18.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT 2019, ApJ, 884, 18

Reference 60

Resolution: verified fuzzy; raw_fallback, observed 2026-05-16T13:52:57.268712Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation f48ba1d2-1275-46e5-af60-12057c0cbbdd · outbound

This paper cites M., et al.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT M., et al

Reference 61

Resolution: verified fuzzy; raw_fallback, observed 2026-05-16T13:52:57.230822Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 6e8bc5fb-355e-4361-ace0-11e3c94df5cf · outbound

This paper cites an unresolved cited work.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT Unresolved cited work

Reference 62

Resolution: unresolved; raw_fallback, observed 2026-05-16T13:52:57.263043Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation b2a46463-afc7-45d0-8d03-a9dd4f6504e9 · outbound

This paper cites K., Hirzberger, J., Riethmüller, T.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT K., Hirzberger, J., Riethmüller, T

Reference 63

Resolution: verified fuzzy; raw_fallback, observed 2026-05-16T13:52:57.250804Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 3c1ef441-bb1c-450e-a03a-29997d0c0ea7 · outbound

This paper cites K., Hirzberger, J., Riethmüller, T.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT K., Hirzberger, J., Riethmüller, T

Reference 64

Resolution: verified fuzzy; raw_fallback, observed 2026-05-16T13:52:57.255692Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 9095a090-fa62-4a0d-bf4a-e11819bda8bc · outbound

This paper cites 1998, Space Sci.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT 1998, Space Sci

Reference 65

Resolution: verified fuzzy; raw_fallback, observed 2026-05-16T13:52:57.164671Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation e7254c98-5d30-457c-a69c-b2f30fa80b40 · outbound

This paper cites an unresolved cited work.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT Unresolved cited work

Reference 66

Resolution: unresolved; raw_fallback, observed 2026-05-16T13:52:57.257925Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation aeccaf5c-4de1-47f3-b349-2fc1a0736f4f · outbound

This paper cites an unresolved cited work.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT Unresolved cited work

Reference 67

Resolution: unresolved; raw_fallback, observed 2026-05-16T13:52:57.166611Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation f7b4b1f9-7f21-423c-9c23-dc37788dfa1e · outbound

This paper cites K., Bertello, L., Boyden, J.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT K., Bertello, L., Boyden, J

Reference 68

Resolution: verified fuzzy; raw_fallback, observed 2026-05-16T13:52:57.238802Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 6658683f-1984-41f6-b573-6594fa31bff8 · outbound

This paper cites & Hathaway, D.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT & Hathaway, D

Reference 69

Resolution: verified fuzzy; raw_fallback, observed 2026-05-16T13:52:57.162751Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 0083b085-1d79-423d-8bef-1d0aa4c60d67 · outbound

This paper cites N., Pattichis, M., Hock-Mysliwiec, R.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT N., Pattichis, M., Hock-Mysliwiec, R

Reference 70

Resolution: verified fuzzy; raw_fallback, observed 2026-05-16T13:52:57.253294Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation aba295f1-4c65-4bd3-be83-0947941273c0 · outbound

This paper cites P ., Poedts, S., Lani, A., et al.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT P ., Poedts, S., Lani, A., et al

Reference 71

Resolution: verified exact; arxiv_id, observed 2026-05-16T13:52:56.912694Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 39fb6876-829e-41cc-9d3a-8f5b45ba0e4b · outbound

This paper cites S., & Xiang, C.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT S., & Xiang, C

Reference 72

Resolution: verified fuzzy; raw_fallback, observed 2026-05-16T13:52:57.233309Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation f095af1d-295b-4be4-8f18-8d6510de7e53 · outbound

This paper cites & Sheeley, Jr., N.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT & Sheeley, Jr., N

Reference 73

Resolution: verified fuzzy; raw_fallback, observed 2026-05-16T13:52:57.172559Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation d823b7df-5e12-458a-8a75-3e2a19a446da · outbound

This paper cites M., Ulrich, R.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT M., Ulrich, R

Reference 74

Resolution: verified fuzzy; raw_fallback, observed 2026-05-16T13:52:57.178390Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation ece80d6b-2913-4f0b-b2b6-f11191a02400 · outbound

This paper cites G., Page, D.

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT G., Page, D

Reference 75

Resolution: verified fuzzy; raw_fallback, observed 2026-05-16T13:52:57.266115Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Pith citing papers

Observation d1b086b1-e549-484d-a7df-0a7ce9468d79 · inbound

COCONUT: Toward practical time-evolving Sun-to-Earth magnetohydrodynamic modeling cites this paper.

COCONUT: Toward practical time-evolving Sun-to-Earth magnetohydrodynamic modeling MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT

Reference 71

Resolution: metadata mismatch; local_arxiv, observed 2026-05-12T10:41:31.979332Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.