Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical | Paper Citation Record

Observation 9bf6a150-746b-4ca4-817b-8505111ef6ab · outbound

This paper cites , Ferriz-Mas , A.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical , Ferriz-Mas , A

Reference 1

Resolution: verified exact; doi, observed 2026-08-10T22:18:21.804887Z

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Observation 9b277296-28c9-4fca-b3cf-72dd143227bb · outbound

This paper cites , Brun , A.S.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical , Brun , A.S

Reference 2

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Observation f36c1d97-7865-49ed-b534-283e2c5f0489 · outbound

This paper cites : 1961 , The Topology of the Sun's Magnetic Field and the 22-YEAR Cycle.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical : 1961 , The Topology of the Sun's Magnetic Field and the 22-YEAR Cycle

Reference 3

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Observation 68717365-4cab-4132-b903-d21983a37a1c · outbound

This paper cites , Nandy , D.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical , Nandy , D

Reference 4

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Observation 782d2503-d507-428b-ad5b-1f0528e8b13a · outbound

This paper cites , Karak , B.B.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical , Karak , B.B

Reference 5

Resolution: verified exact; doi, observed 2026-08-10T22:18:21.769217Z

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Observation f37aa57f-eac3-4bc6-b050-1fa31cd6b4ab · outbound

This paper cites , Karak , B.B.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical , Karak , B.B

Reference 6

Resolution: unresolved; no resolver link, observed 2026-08-10T22:18:20.663694Z

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Observation bafe6ba0-c013-4f4c-a054-7effc5bbfda8 · outbound

This paper cites , Browning , M.K.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical , Browning , M.K

Reference 7

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Observation 1ed7b545-2dda-4a7d-a353-e5148bc03453 · outbound

This paper cites , Miesch , M.S.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical , Miesch , M.S

Reference 8

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Observation 741d8506-7ff5-40c3-9a3f-9fbcfbc7cbd0 · outbound

This paper cites , Strugarek , A.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical , Strugarek , A

Reference 9

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Observation 622958e9-27cf-4e21-a278-a32ddf191857 · outbound

This paper cites , Strugarek , A.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical , Strugarek , A

Reference 10

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Observation 06469552-f5c4-4434-9324-4041a8a58ab0 · outbound

This paper cites , Sch \"u ssler , M.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical , Sch \"u ssler , M

Reference 11

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Observation 135d0ca2-30a7-415d-906f-c20f99b54da0 · outbound

This paper cites , Sch \"u ssler , M.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical , Sch \"u ssler , M

Reference 12

Resolution: unresolved; no resolver link, observed 2026-08-10T22:18:20.689472Z

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Observation 491471c1-cde4-40aa-b90d-3ef05444147e · outbound

This paper cites , Sch \"u ssler , M.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical , Sch \"u ssler , M

Reference 13

Resolution: verified exact; doi, observed 2026-08-10T22:18:21.698195Z

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Observation 1419b243-7f85-4164-ba5c-d428eed92244 · outbound

This paper cites , Sch \"u ssler , M.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical , Sch \"u ssler , M

Reference 14

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Observation 9ec9286e-9a46-451f-bc1d-83c2702ebe4f · outbound

This paper cites : 2020 , Dynamo models of the solar cycle.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical : 2020 , Dynamo models of the solar cycle

Reference 15

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Observation 40f3ea73-75a6-411a-987e-f17d935a9f0e · outbound

This paper cites , Barlet , G.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical , Barlet , G

Reference 16

Resolution: verified exact; doi, observed 2026-08-10T22:18:21.668465Z

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Observation 5176d462-b931-4c1b-be03-0390782e3323 · outbound

This paper cites , Dikpati , M.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical , Dikpati , M

Reference 17

Resolution: verified exact; doi, observed 2026-08-10T22:18:21.656464Z

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Observation 32348654-3ce2-4e92-9d9a-d41e9c960c4c · outbound

This paper cites , Blais-Laurier , G.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical , Blais-Laurier , G

Reference 18

Resolution: verified exact; doi, observed 2026-08-10T22:18:21.643918Z

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No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation dab17951-eb7c-42b2-b74a-62ed7e26cf1e · outbound

This paper cites , St-Jean , C.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical , St-Jean , C

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-10T22:18:20.719462Z

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Observation 915e2b4d-5faa-43cc-9126-78142fa3b8ae · outbound

This paper cites , Nandy , D.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical , Nandy , D

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-10T22:18:20.724347Z

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Observation a54fe661-a796-4adb-9a11-dc8558416390 · outbound

This paper cites , Hazra , G.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical , Hazra , G

Reference 21

Resolution: verified exact; doi, observed 2026-08-10T22:18:21.615929Z

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Observation 9b929c77-8edc-4ea9-8e06-6764978d3079 · outbound

This paper cites , Karak , B.B.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical , Karak , B.B

Reference 22

Resolution: verified exact; doi, observed 2026-08-10T22:18:21.603751Z

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Observation 5e4419fa-d971-48bf-ac1f-a8a5e3d1d0a0 · outbound

This paper cites , Karak , B.B.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical , Karak , B.B

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-10T22:18:20.736594Z

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Observation 875a4858-8db7-4f0d-838f-2be97eb779a3 · outbound

This paper cites , Chatterjee , P.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical , Chatterjee , P

Reference 24

Resolution: unresolved; no resolver link, observed 2026-08-10T22:18:20.740573Z

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Observation 4fc82ca5-01e4-44fb-a337-966da4657c80 · outbound

This paper cites , Nandy , D.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical , Nandy , D

Reference 25

Resolution: verified exact; doi, observed 2026-08-10T22:18:21.583631Z

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No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 4038fe5a-435c-4ffd-a5ef-3d0adb96f188 · outbound

This paper cites , Sch\"ussler , M.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical , Sch\"ussler , M

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-10T22:18:20.748526Z

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Observation 4c64abac-882e-4334-bfde-93b18a8dd71e · outbound

This paper cites , Solanki , S.K.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical , Solanki , S.K

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-10T22:18:20.752086Z

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Observation 513bd675-0d45-4426-a8b1-4a41cd8b0407 · outbound

This paper cites , Charbonneau , P.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical , Charbonneau , P

Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-10T22:18:20.756060Z

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Observation dea64815-ba44-4b02-bccc-23c1156f9550 · outbound

This paper cites : 1976 , The Maunder Minimum.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical : 1976 , The Maunder Minimum

Reference 29

Resolution: unresolved; no resolver link, observed 2026-08-10T22:18:20.760213Z

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Observation 4d8da046-9843-498e-9c2b-fd805e7480a6 · outbound

This paper cites , Fang , F.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical , Fang , F

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-10T22:18:20.763751Z

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Observation 97385516-e5c8-4c38-8399-64e57222e760 · outbound

This paper cites Waldmeier Effect in Stellar Cycles.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical Waldmeier Effect in Stellar Cycles

Reference 31

Resolution: verified exact; local_arxiv, observed 2026-08-10T22:18:21.821936Z

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Observation 7ffc0432-0ec6-4f1d-911c-7331240186cc · outbound

This paper cites , Kumar , P.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical , Kumar , P

Reference 32

Resolution: verified exact; doi, observed 2026-08-10T22:18:21.550972Z

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Observation 4c599e81-a972-4b70-a0e9-bcb9b6da99cf · outbound

This paper cites : 2015 , The Solar Cycle.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical : 2015 , The Solar Cycle

Reference 33

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Observation 45397fdc-8d65-4327-b146-cf64af6c6b61 · outbound

This paper cites , Choudhuri , A.R.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical , Choudhuri , A.R

Reference 34

Resolution: verified exact; doi, observed 2026-08-10T22:18:21.531676Z

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No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 1f8f9f7e-e6a1-4247-843a-c69fb78b0399 · outbound

This paper cites , Nandy , D.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical , Nandy , D

Reference 35

Resolution: unresolved; no resolver link, observed 2026-08-10T22:18:20.784535Z

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Observation 56cfa1ea-fe90-4c68-b4e1-cd852e60a99b · outbound

This paper cites , Passos , D.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical , Passos , D

Reference 36

Resolution: verified exact; doi, observed 2026-08-10T22:18:21.509613Z

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No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation a0900cfa-bd47-4b16-87f6-ef0fb6e5d01f · outbound

This paper cites , Kusano , K.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical , Kusano , K

Reference 37

Resolution: unresolved; no resolver link, observed 2026-08-10T22:18:20.793267Z

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Observation e109b245-8caa-49cf-ba59-43163cdb2941 · outbound

This paper cites , Karak , B.B.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical , Karak , B.B

Reference 38

Resolution: verified exact; doi, observed 2026-08-10T22:18:21.489160Z

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No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 8d452972-63dd-45e7-be69-f3614e4aad2a · outbound

This paper cites , Cameron , R.H.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical , Cameron , R.H

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-10T22:18:20.801850Z

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Observation 1508affa-31b1-43af-9f60-80c790b91c7a · outbound

This paper cites a pyl \"a , M.J. , K \.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical a pyl \"a , M.J. , K \

Reference 40

Resolution: verified exact; doi, observed 2026-08-10T22:18:21.468981Z

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No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 4301be1c-f4f4-4886-a59b-00146a95f073 · outbound

This paper cites , Browning , M.K.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical , Browning , M.K

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-10T22:18:20.810158Z

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Observation f38269c1-ae54-4572-a777-8312e5ef912d · outbound

This paper cites : 2010 , Importance of Meridional Circulation in Flux Transport Dynamo: The Possibility of a Maunder-like Grand Minimum.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical : 2010 , Importance of Meridional Circulation in Flux Transport Dynamo: The Possibility of a Maunder-like Grand Minimum

Reference 42

Resolution: unresolved; no resolver link, observed 2026-08-10T22:18:20.813917Z

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Observation dde8b90e-0ed5-4879-94d2-ef5185fd4d40 · outbound

This paper cites : 2023 , Models for the long-term variations of solar activity.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical : 2023 , Models for the long-term variations of solar activity

Reference 43

Resolution: unresolved; no resolver link, observed 2026-08-10T22:18:20.817743Z

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Observation f71d8439-38a1-4def-9cdb-a33f3d56d41e · outbound

This paper cites , Choudhuri , A.R.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical , Choudhuri , A.R

Reference 44

Resolution: verified exact; doi, observed 2026-08-10T22:18:21.431586Z

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No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 2a8dc1c8-6765-452f-b0b8-fd4828f8332d · outbound

This paper cites , Miesch , M.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical , Miesch , M

Reference 45

Resolution: verified exact; doi, observed 2026-08-10T22:18:21.417929Z

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No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation b3126901-f375-4aba-ac8e-63f61f54e38e · outbound

This paper cites , Miesch , M.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical , Miesch , M

Reference 46

Resolution: verified exact; doi, observed 2026-08-10T22:18:21.403955Z

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No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation a7c6fbc5-1dc7-4d11-8785-e9a1d146f506 · outbound

This paper cites , Kitchatinov , L.L.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical , Kitchatinov , L.L

Reference 47

Resolution: verified exact; doi, observed 2026-08-10T22:18:21.389450Z

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No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation a8679a90-2f31-441a-8be8-e455510b683a · outbound

This paper cites , Mandal , S.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical , Mandal , S

Reference 48

Resolution: verified exact; doi, observed 2026-08-10T22:18:21.375300Z

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Observation 4509e2f7-9e99-47ef-9edd-ff7da6bbad15 · outbound

This paper cites , Miesch , M.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical , Miesch , M

Reference 49

Resolution: unresolved; no resolver link, observed 2026-08-10T22:18:20.844804Z

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Observation af67a16a-fb02-412e-ab4b-2a4f0d057dc3 · outbound

This paper cites , Jiang , J.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical , Jiang , J

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-10T22:18:20.848543Z

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Observation 353725d8-ebe4-490a-96db-23e051547c0c · outbound

This paper cites a pyl \"a , P.J. , K \.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical a pyl \"a , P.J. , K \

Reference 51

Resolution: unresolved; no resolver link, observed 2026-08-10T22:18:20.852409Z

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Observation 0ed0e4dc-d5d5-47b6-b727-4077289ddabb · outbound

This paper cites , Nepomnyashchikh , A.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical , Nepomnyashchikh , A

Reference 52

Resolution: verified exact; doi, observed 2026-08-10T22:18:21.340380Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 3b32e18e-62ed-41ef-9013-f5fc36803653 · outbound

This paper cites , Olemskoy , S.V.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical , Olemskoy , S.V

Reference 53

Resolution: unresolved; no resolver link, observed 2026-08-10T22:18:20.860335Z

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Observation 03021e8e-2bbb-4fab-bf16-0ec16d2e68d8 · outbound

This paper cites , Olemskoy , S.V.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical , Olemskoy , S.V

Reference 54

Resolution: unresolved; no resolver link, observed 2026-08-10T22:18:20.864109Z

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Observation 73faea62-bdf1-4dc7-8f1f-fcb2e08bd5ec · outbound

This paper cites , R \"a dler , K.H.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical , R \"a dler , K.H

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-10T22:18:20.868265Z

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Observation b63eb834-b95a-4ec3-bd42-40e6ccb90bdd · outbound

This paper cites , Biswas , A.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical , Biswas , A

Reference 56

Resolution: unresolved; no resolver link, observed 2026-08-10T22:18:20.872246Z

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Observation 72b7efdb-ed61-43c0-b44c-f154672a1326 · outbound

This paper cites , Karak , B.B.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical , Karak , B.B

Reference 57

Resolution: verified exact; doi, observed 2026-08-10T22:18:21.312222Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 9dfe6ddd-efa9-4a3d-8619-37fb413cfd94 · outbound

This paper cites , Karak , B.B.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical , Karak , B.B

Reference 58

Resolution: verified exact; doi, observed 2026-08-10T22:18:21.300379Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 5818940f-fbae-403a-b79f-e13bda5d239f · outbound

This paper cites , Nagy , M.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical , Nagy , M

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-10T22:18:20.885143Z

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Unavailable: canonical work link unavailable.

Observation b8d234a2-4fe5-4125-a9d5-2af770058e35 · outbound

This paper cites : 1969 , A Magneto-Kinematic Model of the Solar Cycle.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical : 1969 , A Magneto-Kinematic Model of the Solar Cycle

Reference 60

Resolution: unresolved; no resolver link, observed 2026-08-10T22:18:20.889280Z

Source-reported events for the cited work

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Observation e0b0cda8-3a86-46a4-86f5-03058312a474 · outbound

This paper cites , Egeland , R.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical , Egeland , R

Reference 61

Resolution: unresolved; no resolver link, observed 2026-08-10T22:18:20.893688Z

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Observation e86afe78-b767-498f-9e73-04529a761db5 · outbound

This paper cites : 1978 , Magnetic field generation in electrically conducting fluids.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical : 1978 , Magnetic field generation in electrically conducting fluids

Reference 62

Resolution: unresolved; no resolver link, observed 2026-08-10T22:18:20.898428Z

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Observation 13a5e0cc-5d9f-4b57-847f-06bf1945a822 · outbound

This paper cites , Karak , B.B.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical , Karak , B.B

Reference 63

Resolution: unresolved; no resolver link, observed 2026-08-10T22:18:20.903417Z

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Observation 53a1cae6-baa9-4f0d-9448-2230714bb315 · outbound

This paper cites , Dasi-Espuig , M.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical , Dasi-Espuig , M

Reference 64

Resolution: unresolved; no resolver link, observed 2026-08-10T22:18:20.908166Z

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Observation b240f45a-6962-4a14-ad15-8aba21783f25 · outbound

This paper cites , Hartmann , L.W.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical , Hartmann , L.W

Reference 65

Resolution: unresolved; no resolver link, observed 2026-08-10T22:18:20.912084Z

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Observation 7a054db8-8217-416a-8947-b4cb4839505a · outbound

This paper cites , Kitchatinov , L.L.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical , Kitchatinov , L.L

Reference 66

Resolution: unresolved; no resolver link, observed 2026-08-10T22:18:20.916518Z

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Observation 30f7c20a-a645-4eaa-840b-527b7400f5f8 · outbound

This paper cites , Choudhuri , A.R.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical , Choudhuri , A.R

Reference 67

Resolution: verified exact; doi, observed 2026-08-10T22:18:21.234519Z

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No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 1c7dc166-a153-4fe3-935c-b4b4062fe6ce · outbound

This paper cites : 1955 , Hydromagnetic Dynamo Models.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical : 1955 , Hydromagnetic Dynamo Models

Reference 68

Resolution: unresolved; no resolver link, observed 2026-08-10T22:18:20.925575Z

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Observation 0469e193-50fd-4b78-821c-fbcf09188b56 · outbound

This paper cites , Nandy , D.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical , Nandy , D

Reference 69

Resolution: verified exact; doi, observed 2026-08-10T22:18:21.214640Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 6c739ce6-2710-4caf-94e0-bc2de9d9d0e2 · outbound

This paper cites , Charbonneau , P.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical , Charbonneau , P

Reference 70

Resolution: unresolved; no resolver link, observed 2026-08-10T22:18:20.956946Z

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Observation 64a7dfac-3d3b-4364-98b1-47da9f294f48 · outbound

This paper cites : 1984 , Age-rotation relationship for late-type main-sequence stars.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical : 1984 , Age-rotation relationship for late-type main-sequence stars

Reference 71

Resolution: unresolved; no resolver link, observed 2026-08-10T22:18:20.970349Z

Source-reported events for the cited work

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Observation 009fa843-3788-40db-841c-338ad61c2b33 · outbound

This paper cites , Nesme-Ribes , E.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical , Nesme-Ribes , E

Reference 72

Resolution: verified fuzzy; raw_fallback, observed 2026-08-10T22:18:21.957802Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation cf6c862a-d069-4239-a65c-988cf2a3042e · outbound

This paper cites , Scherrer , P.H.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical , Scherrer , P.H

Reference 73

Resolution: unresolved; no resolver link, observed 2026-08-10T22:18:20.978249Z

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Observation 52e3b543-8e6d-4684-8f1e-8a57c813de50 · outbound

This paper cites , Wright , J.T.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical , Wright , J.T

Reference 74

Resolution: unresolved; no resolver link, observed 2026-08-10T22:18:20.982440Z

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Observation d364ccdf-ffd0-4ef8-b3fb-1220dd681d13 · outbound

This paper cites : 1972 , Time Scales for CA II Emission Decay, Rotational Braking, and Lithium Depletion.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical : 1972 , Time Scales for CA II Emission Decay, Rotational Braking, and Lithium Depletion

Reference 75

Resolution: unresolved; no resolver link, observed 2026-08-10T22:18:20.986969Z

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Observation 7f4c74e4-af99-495d-9418-384dcad3c75a · outbound

This paper cites , Jha , B.K.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical , Jha , B.K

Reference 76

Resolution: unresolved; no resolver link, observed 2026-08-10T22:18:20.991748Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7b7d2c92-484b-4ded-9fb8-c90dffd95f09 · outbound

This paper cites , Beaudoin , P.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical , Beaudoin , P

Reference 77

Resolution: unresolved; no resolver link, observed 2026-08-10T22:18:20.996025Z

Source-reported events for the cited work

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Observation c3ef8f07-1f9c-4750-8ec6-8c55b9ea8987 · outbound

This paper cites , Nandy , D.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical , Nandy , D

Reference 78

Resolution: unresolved; no resolver link, observed 2026-08-10T22:18:21.000159Z

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Observation dd9b98b9-58d7-4fd2-9c52-07c8fdf414bc · outbound

This paper cites : 2023 , A history of solar activity over millennia.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical : 2023 , A history of solar activity over millennia

Reference 79

Resolution: unresolved; no resolver link, observed 2026-08-10T22:18:21.004327Z

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Observation e42f49d2-d1d5-4ad8-949d-83ed4075aa2a · outbound

This paper cites , Solanki , S.K.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical , Solanki , S.K

Reference 80

Resolution: verified fuzzy; raw_fallback, observed 2026-08-10T22:18:21.944504Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation de4f232b-28ea-4cae-977d-ee6455b50128 · outbound

This paper cites , Solanki , S.K.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical , Solanki , S.K

Reference 81

Resolution: unresolved; no resolver link, observed 2026-08-10T22:18:21.012859Z

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Observation 08be9f21-4aba-456e-921f-2f3ba1ef8d81 · outbound

This paper cites , Solanki , S.K.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical , Solanki , S.K

Reference 82

Resolution: verified exact; doi, observed 2026-08-10T22:18:21.125057Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 0245eacf-bdb6-4211-8dff-bbb9334aa893 · outbound

This paper cites , Karak , B.B.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical , Karak , B.B

Reference 83

Resolution: verified exact; doi, observed 2026-08-10T22:18:21.109416Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation abca3594-2fb6-4308-8913-d9d76691245f · outbound

This paper cites , Karak , B.B.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical , Karak , B.B

Reference 84

Resolution: unresolved; no resolver link, observed 2026-08-10T22:18:21.027094Z

Source-reported events for the cited work

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Observation b9d135bc-3efa-43a0-b048-fc93616cdc57 · outbound

This paper cites , Gregory , S.G.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical , Gregory , S.G

Reference 85

Resolution: unresolved; no resolver link, observed 2026-08-10T22:18:21.031962Z

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Observation 231203f1-3a30-42bb-8757-b1a7af4b2e70 · outbound

This paper cites , Nandy , D.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical , Nandy , D

Reference 86

Resolution: unresolved; no resolver link, observed 2026-08-10T22:18:21.036595Z

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Observation 2c5041a1-71aa-4e6a-bc4c-c8847e1bc8a1 · outbound

This paper cites : 2016, Stellar Magnetic Activity Cycles, and Hunting for Maunder Minimum-like Events among Sun-like Stars.

Analyses of features of magnetic cycles at different amounts of dynamo supercriticality: Solar dynamo is about two times critical : 2016, Stellar Magnetic Activity Cycles, and Hunting for Maunder Minimum-like Events among Sun-like Stars

Reference 87

Resolution: verified fuzzy; raw_fallback, observed 2026-08-10T22:18:21.930313Z

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No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

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