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Paper Citation Record · LEDGER

Constraining the radial decay timescale of solar surface magnetic field through a comparative study of data-assimilative 2D surface flux transport and 3D dynamo models

As of 10 August 2026, this Paper Citation Record lists 100 of 296 outbound references and 0 inbound Pith citation observations for arXiv:2607.16939.

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pith.paper-citation-record.v1
2607.16939 v1

Coverage vector

measured 100 of 296 reference resolution

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Pith citing papers itemized under the disclosed page cap.

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Source: cited_works

Reference resolution

100 of 296 outbound references displayed

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External citation measurements

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Outbound references

Observation 8b5f33d7-ff5b-4c10-8590-f8397c09e1b0 · outbound

This paper cites The Astropy Project: Sustaining and Growing a Community-oriented Open-source Project and the Latest Major Release (v5.0) of the Core Package.

Constraining the radial decay timescale of solar surface magnetic field through a comparative study of data-assimilative 2D surface flux transport and 3D dynamo models The Astropy Project: Sustaining and Growing a Community-oriented Open-source Project and the Latest Major Release (v5.0) of the Core Package

Reference 1

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Observation abb2a9a6-222b-4230-9173-6df73487fb4a · outbound

This paper cites The Astropy Project: Building an inclusive, open-science project and status of the v2.0 core package.

Constraining the radial decay timescale of solar surface magnetic field through a comparative study of data-assimilative 2D surface flux transport and 3D dynamo models The Astropy Project: Building an inclusive, open-science project and status of the v2.0 core package

Reference 2

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Observation 67e697a8-1af8-49b9-a14c-466e01f1ff18 · outbound

This paper cites Quantifying the Observational Effort Required for the Radial Velocity Characterization of TESS Planets.

Constraining the radial decay timescale of solar surface magnetic field through a comparative study of data-assimilative 2D surface flux transport and 3D dynamo models Quantifying the Observational Effort Required for the Radial Velocity Characterization of TESS Planets

Reference 5

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Observation 1411fb9a-8eda-4736-8eac-1ea6df217a8c · outbound

This paper cites X-ray Scattering Echoes and Ghost Halos from the Intergalactic Medium: Relation to the nature of AGN variability.

Constraining the radial decay timescale of solar surface magnetic field through a comparative study of data-assimilative 2D surface flux transport and 3D dynamo models X-ray Scattering Echoes and Ghost Halos from the Intergalactic Medium: Relation to the nature of AGN variability

Reference 6

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Constraining the radial decay timescale of solar surface magnetic field through a comparative study of data-assimilative 2D surface flux transport and 3D dynamo models 1989", month =

Reference 8

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Constraining the radial decay timescale of solar surface magnetic field through a comparative study of data-assimilative 2D surface flux transport and 3D dynamo models Unresolved cited work

Reference 9

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Observation b2c4540b-dea8-4b06-97ef-805c0a2a028b · outbound

This paper cites Quasi-periodic Fast Propagating Magnetoacoustic Waves during the Magnetic Reconnection Between Solar Coronal Loops.

Constraining the radial decay timescale of solar surface magnetic field through a comparative study of data-assimilative 2D surface flux transport and 3D dynamo models Quasi-periodic Fast Propagating Magnetoacoustic Waves during the Magnetic Reconnection Between Solar Coronal Loops

Reference 10

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Observation 317622db-1b08-4feb-a5da-9d21eaeee023 · outbound

This paper cites Nominal values for selected solar and planetary quantities: IAU 2015 Resolution B3.

Constraining the radial decay timescale of solar surface magnetic field through a comparative study of data-assimilative 2D surface flux transport and 3D dynamo models Nominal values for selected solar and planetary quantities: IAU 2015 Resolution B3

Reference 11

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This paper cites Swift X-Ray Observations of Classical Novae. II. The Super Soft Source sample.

Constraining the radial decay timescale of solar surface magnetic field through a comparative study of data-assimilative 2D surface flux transport and 3D dynamo models Swift X-Ray Observations of Classical Novae. II. The Super Soft Source sample

Reference 12

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Constraining the radial decay timescale of solar surface magnetic field through a comparative study of data-assimilative 2D surface flux transport and 3D dynamo models Solar Physics , keywords =

Reference 14

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Constraining the radial decay timescale of solar surface magnetic field through a comparative study of data-assimilative 2D surface flux transport and 3D dynamo models Observables Processing for the Helioseismic and Magnetic Imager Instrument on the Solar Dynamics Observatory

Reference 15

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This paper cites Solar Active Region Magnetogram Image Dataset for Studies of Space Weather.

Constraining the radial decay timescale of solar surface magnetic field through a comparative study of data-assimilative 2D surface flux transport and 3D dynamo models Solar Active Region Magnetogram Image Dataset for Studies of Space Weather

Reference 16

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Observation 6ea6b336-33d6-44fb-94c7-f00ed958014c · outbound

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Constraining the radial decay timescale of solar surface magnetic field through a comparative study of data-assimilative 2D surface flux transport and 3D dynamo models and Stulajter, Miko M

Reference 17

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Constraining the radial decay timescale of solar surface magnetic field through a comparative study of data-assimilative 2D surface flux transport and 3D dynamo models Unresolved cited work

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Constraining the radial decay timescale of solar surface magnetic field through a comparative study of data-assimilative 2D surface flux transport and 3D dynamo models 2016 , note =

Reference 20

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Constraining the radial decay timescale of solar surface magnetic field through a comparative study of data-assimilative 2D surface flux transport and 3D dynamo models Clune and J.R

Reference 21

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This paper cites Full--Sphere Simulations of a Circulation--Dominated Solar Dynamo: Exploring the Parity Issue.

Constraining the radial decay timescale of solar surface magnetic field through a comparative study of data-assimilative 2D surface flux transport and 3D dynamo models Full--Sphere Simulations of a Circulation--Dominated Solar Dynamo: Exploring the Parity Issue

Reference 23

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Constraining the radial decay timescale of solar surface magnetic field through a comparative study of data-assimilative 2D surface flux transport and 3D dynamo models and Hathaway, D

Reference 25

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Constraining the radial decay timescale of solar surface magnetic field through a comparative study of data-assimilative 2D surface flux transport and 3D dynamo models and Cameron, R

Reference 27

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Constraining the radial decay timescale of solar surface magnetic field through a comparative study of data-assimilative 2D surface flux transport and 3D dynamo models Unresolved cited work

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Constraining the radial decay timescale of solar surface magnetic field through a comparative study of data-assimilative 2D surface flux transport and 3D dynamo models How well does surface magnetism represent deep Sun-like star dynamo action?

Reference 30

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Constraining the radial decay timescale of solar surface magnetic field through a comparative study of data-assimilative 2D surface flux transport and 3D dynamo models and Kosovichev, Alexander G

Reference 31

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This paper cites Babcock-Leighton solar dynamo: the role of downward pumping and the equatorward propagation of activity.

Constraining the radial decay timescale of solar surface magnetic field through a comparative study of data-assimilative 2D surface flux transport and 3D dynamo models Babcock-Leighton solar dynamo: the role of downward pumping and the equatorward propagation of activity

Reference 32

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Constraining the radial decay timescale of solar surface magnetic field through a comparative study of data-assimilative 2D surface flux transport and 3D dynamo models , year = 1919, month = apr, volume =

Reference 34

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Constraining the radial decay timescale of solar surface magnetic field through a comparative study of data-assimilative 2D surface flux transport and 3D dynamo models , year = 1969, month = apr, volume =

Reference 39

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Constraining the radial decay timescale of solar surface magnetic field through a comparative study of data-assimilative 2D surface flux transport and 3D dynamo models Observationally guided models for the solar dynamo and the role of the surface field

Reference 40

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Constraining the radial decay timescale of solar surface magnetic field through a comparative study of data-assimilative 2D surface flux transport and 3D dynamo models The Meridional Circulation of the Sun: Observations, Theory and Connections with the Solar Dynamo

Reference 41

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Constraining the radial decay timescale of solar surface magnetic field through a comparative study of data-assimilative 2D surface flux transport and 3D dynamo models Science , keywords =

Reference 42

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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=arxiv_source observed=2026-08-01T19:35:40.254352Z digest=sha256:4e151cbad68e0cf846e373a481f5f23b18464792148d3c37a74470788fba7bfb

Observation 386b0de4-48fc-49f5-b020-8b7be21b8c6c · outbound

This paper cites Predicting the Sun's Polar Magnetic Fields with a Surface Flux Transport Model.

Constraining the radial decay timescale of solar surface magnetic field through a comparative study of data-assimilative 2D surface flux transport and 3D dynamo models Predicting the Sun's Polar Magnetic Fields with a Surface Flux Transport Model

Reference 43

Resolution
unresolved
no resolver link, observed 2026-08-01T19:35:40.349809Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:35:40.349809Z digest=sha256:4bbff69a18abc0bb24b554a7c20da10ab34e55117cd1b16d074d4a2a0b07d88d

Reference 44

Resolution
unresolved
no resolver link, observed 2026-08-01T19:35:40.441223Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:35:40.441223Z digest=sha256:e5d17a58d6e66125fbe50b51ef0b39b76f142025ed55b6a0bce53ba026f42820

Observation e3fee9a8-ffd3-4096-bd67-95b558472cc4 · outbound

This paper cites Effects of the scatter in sunspot group tilt angles on the large-scale magnetic field at the solar surface.

Constraining the radial decay timescale of solar surface magnetic field through a comparative study of data-assimilative 2D surface flux transport and 3D dynamo models Effects of the scatter in sunspot group tilt angles on the large-scale magnetic field at the solar surface

Reference 45

Resolution
unresolved
no resolver link, observed 2026-08-01T19:35:40.558327Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:35:40.558327Z digest=sha256:e8484d2e1e018f828dee70b38f541b35c5fcb33dde30b71a88407c4bd45d99f4

Reference 46

Resolution
unresolved
no resolver link, observed 2026-08-01T19:35:40.689880Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:35:40.689880Z digest=sha256:5079fb74973a040af49ef7e0705f510e05ce6ca2608b94e9f0c03cfda71bde01

Observation ea3840cc-fa92-4166-b9ca-e01c1627b795 · outbound

This paper cites Prediction of the strength and timing of sunspot cycle 25 reveal decadal-scale space environmental conditions.

Constraining the radial decay timescale of solar surface magnetic field through a comparative study of data-assimilative 2D surface flux transport and 3D dynamo models Prediction of the strength and timing of sunspot cycle 25 reveal decadal-scale space environmental conditions

Reference 47

Resolution
unresolved
no resolver link, observed 2026-08-01T19:35:40.838057Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:35:40.838057Z digest=sha256:e99925e7d1e0ce96ca0818f747645d05712b836bb81820af0e0a73acd4127a39

Observation c84741e8-6dc4-4f00-9719-39eedaa9c27d · outbound

This paper cites A coupled 2$\times$2D Babcock-Leighton solar dynamo model. I. Surface magnetic flux evolution.

Constraining the radial decay timescale of solar surface magnetic field through a comparative study of data-assimilative 2D surface flux transport and 3D dynamo models A coupled 2$\times$2D Babcock-Leighton solar dynamo model. I. Surface magnetic flux evolution

Reference 48

Resolution
unresolved
no resolver link, observed 2026-08-01T19:35:41.003491Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:35:41.003491Z digest=sha256:97bdee291b87462d838ec25313a9c97fce5470bcbd6b2c9c65ac42022326d94d

Observation c0a5321d-0ca4-4ca6-b48e-a2d4c32de452 · outbound

This paper cites A coupled $2\times2$D Babcock-Leighton solar dynamo model. II. Reference dynamo solutions.

Constraining the radial decay timescale of solar surface magnetic field through a comparative study of data-assimilative 2D surface flux transport and 3D dynamo models A coupled $2\times2$D Babcock-Leighton solar dynamo model. II. Reference dynamo solutions

Reference 49

Resolution
unresolved
no resolver link, observed 2026-08-01T19:35:41.193025Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:35:41.193025Z digest=sha256:0605947cb3582c321cb1c83e6d93dd2d777960acca0671976da82b84c124f1b7

Observation 4eef63b6-4d52-4143-88b7-4fbb44d7486f · outbound

This paper cites an unresolved cited work.

Constraining the radial decay timescale of solar surface magnetic field through a comparative study of data-assimilative 2D surface flux transport and 3D dynamo models Unresolved cited work

Reference 50

Resolution
verified exact
doi, observed 2026-08-01T19:38:38.322954Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=arxiv_source observed=2026-08-01T19:35:41.386440Z digest=sha256:c5e4545e01c7d9eaca505cafe49b96cac2bd4a084a15da33790006e7d395e2db

Observation 84afa375-c08a-4fd8-9492-0ed183eb87bb · outbound

This paper cites A Double-Ring Algorithm for Modeling Solar Active Regions: Unifying Kinematic Dynamo Models and Surface Flux-Transport Simulations.

Constraining the radial decay timescale of solar surface magnetic field through a comparative study of data-assimilative 2D surface flux transport and 3D dynamo models A Double-Ring Algorithm for Modeling Solar Active Regions: Unifying Kinematic Dynamo Models and Surface Flux-Transport Simulations

Reference 51

Resolution
unresolved
no resolver link, observed 2026-08-01T19:35:41.509230Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:35:41.509230Z digest=sha256:ab886460dfe8a11d103eb128bb7d10181f63863724c6aa0808f9b528c2dece59

Observation af5a0590-9ef6-4b06-bb06-152c392ec619 · outbound

This paper cites Kodai School on Solar Physics , year = 2007, editor =.

Constraining the radial decay timescale of solar surface magnetic field through a comparative study of data-assimilative 2D surface flux transport and 3D dynamo models Kodai School on Solar Physics , year = 2007, editor =

Reference 52

Resolution
unresolved
no resolver link, observed 2026-08-01T19:35:41.642793Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:35:41.642793Z digest=sha256:106ad3ef473d34e835936797e8e61a3eee8650f986e0cb1392777fc95dabed97

Observation cb031df4-6c5c-4969-a1be-f3835d24de8c · outbound

This paper cites Science , keywords =.

Constraining the radial decay timescale of solar surface magnetic field through a comparative study of data-assimilative 2D surface flux transport and 3D dynamo models Science , keywords =

Reference 53

Resolution
unresolved
no resolver link, observed 2026-08-01T19:35:41.772359Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:35:41.772359Z digest=sha256:51d3b4ab69dcb87fc939300f2625e682a5163b3afffa203991a1141e9e912c8f

Reference 54

Resolution
unresolved
no resolver link, observed 2026-08-01T19:35:41.858861Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:35:41.858861Z digest=sha256:3a25c145b1a3ca062649d7b05146df3bbef12d805ae68b7c1b0fabd2d50e5cb1

Observation 509c2604-548f-4db3-9620-9d1d047b71a7 · outbound

This paper cites an unresolved cited work.

Constraining the radial decay timescale of solar surface magnetic field through a comparative study of data-assimilative 2D surface flux transport and 3D dynamo models Unresolved cited work

Reference 55

Resolution
parse uncertain
no resolver link, observed 2026-08-01T19:35:41.926598Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:35:41.926598Z digest=sha256:7a1d4e8339aad6856f59ce0d06f8937178b11e449ebd3bd395d0628b34963ea1

Observation e450ce3d-1365-4076-97ad-4ac86d2cb11f · outbound

This paper cites Surface flux transport modeling for solar cycles 15--21: effects of cycle-dependent tilt angles of sunspot groups.

Constraining the radial decay timescale of solar surface magnetic field through a comparative study of data-assimilative 2D surface flux transport and 3D dynamo models Surface flux transport modeling for solar cycles 15--21: effects of cycle-dependent tilt angles of sunspot groups

Reference 56

Resolution
unresolved
no resolver link, observed 2026-08-01T19:35:42.048537Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:35:42.048537Z digest=sha256:d005d0034305ba408899e74ff65ce6f17f962643d79be8baea3d5d9ec67bb3bc

Reference 57

Resolution
verified exact
doi, observed 2026-08-01T19:38:38.159376Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=arxiv_source observed=2026-08-01T19:35:42.100293Z digest=sha256:a793246a3f996728e5718ed55b4569558b9ec43169623bd70d26d9ceb4e936fc

Observation b3027169-6a65-4c5a-9825-41a9d4d67e07 · outbound

This paper cites Ensemble Kalman Filter Data Assimilation Into Surface Flux Transport Model To Infer Surface Flows: An Observing System Simulation Experiment.

Constraining the radial decay timescale of solar surface magnetic field through a comparative study of data-assimilative 2D surface flux transport and 3D dynamo models Ensemble Kalman Filter Data Assimilation Into Surface Flux Transport Model To Infer Surface Flows: An Observing System Simulation Experiment

Reference 58

Resolution
unresolved
no resolver link, observed 2026-08-01T19:35:42.165485Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:35:42.165485Z digest=sha256:88666bb8dccb345975aa3ddd950b3d38afb5bd74582011d1335c6e598cfabc80

Reference 59

Resolution
unresolved
no resolver link, observed 2026-08-01T19:35:42.303605Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:35:42.303605Z digest=sha256:6e434accd236aa900401372776272b2bca4a01ac319699a64c78b0381de76b7d

Reference 60

Resolution
unresolved
no resolver link, observed 2026-08-01T19:35:42.427052Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:35:42.427052Z digest=sha256:44988e7ce10e5f308577f1a14ce54c60202800413dec84acde2c91a161743ef8

Observation 3d294be1-bf2f-4e06-b667-67e5cd57d77e · outbound

This paper cites The Advective Flux Transport Model: Improving the Far-Side with Active Regions observed by STEREO 304\r{A}.

Constraining the radial decay timescale of solar surface magnetic field through a comparative study of data-assimilative 2D surface flux transport and 3D dynamo models The Advective Flux Transport Model: Improving the Far-Side with Active Regions observed by STEREO 304\r{A}

Reference 61

Resolution
unresolved
no resolver link, observed 2026-08-01T19:35:42.497988Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:35:42.497988Z digest=sha256:7ec8f2a88ffdb2ff57c513e646cb38e6a3d7838b12a4a0ebbab0d50d5b3ab065

Reference 62

Resolution
unresolved
no resolver link, observed 2026-08-01T19:35:42.579315Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:35:42.579315Z digest=sha256:ba56e410e53f5df3e1361675e51e84a2e0c7a495f9e7589b251d3def0e0e879e

Observation 5a10ca77-7f76-4b66-a4d6-0756995b4762 · outbound

This paper cites Solar Wind 13 , year = 2013, editor =.

Constraining the radial decay timescale of solar surface magnetic field through a comparative study of data-assimilative 2D surface flux transport and 3D dynamo models Solar Wind 13 , year = 2013, editor =

Reference 63

Resolution
unresolved
no resolver link, observed 2026-08-01T19:35:42.621492Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:35:42.621492Z digest=sha256:1ab5c862d0c6f7de23a38388532749ced3b5a64a931a8da0213c07a83e5910bc

Reference 64

Resolution
unresolved
no resolver link, observed 2026-08-01T19:35:42.706869Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:35:42.706869Z digest=sha256:768e1ddc8c566fead629676288a12bb5fd89759ecdc29939fbe6f03a2175988a

Reference 65

Resolution
unresolved
no resolver link, observed 2026-08-01T19:35:42.770478Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:35:42.770478Z digest=sha256:6fe4755cd1323f69151269c68f78fc10c9efe3fb87f808bd4d420706160932ce

Reference 66

Resolution
unresolved
no resolver link, observed 2026-08-01T19:35:42.949404Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:35:42.949404Z digest=sha256:67e4e88db556e6cca778eaa4c8adf5da310036ae687cec20360495b3843f5639

Observation 0de1a7b6-9199-419c-b9c2-78932e564997 · outbound

This paper cites Astronomy & Astrophysics , keywords =.

Constraining the radial decay timescale of solar surface magnetic field through a comparative study of data-assimilative 2D surface flux transport and 3D dynamo models Astronomy & Astrophysics , keywords =

Reference 67

Resolution
verified exact
doi, observed 2026-08-01T19:38:38.026152Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=arxiv_source observed=2026-08-01T19:35:43.031930Z digest=sha256:53658d9935355a9e6af7c72badc8870a61de7120188825086a473527bea5a278

Reference 68

Resolution
verified exact
doi, observed 2026-08-01T19:38:37.938648Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=arxiv_source observed=2026-08-01T19:35:43.111067Z digest=sha256:1ecf976c8454dba0aa046fd2f2468dba4edf0f9aed4eab288eb84dfc72e0ee72

Observation 08bd80c4-a00f-4429-acd4-4e2433ff6310 · outbound

This paper cites Forecasting the solar cycle using variational data assimilation: validation on cycles 22 to 25.

Constraining the radial decay timescale of solar surface magnetic field through a comparative study of data-assimilative 2D surface flux transport and 3D dynamo models Forecasting the solar cycle using variational data assimilation: validation on cycles 22 to 25

Reference 69

Resolution
unresolved
no resolver link, observed 2026-08-01T19:35:43.173147Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:35:43.173147Z digest=sha256:e3f872777fd8da398a6383d5c501a4ce488432f5beb46cb1935d98c1ab0e7928

Reference 70

Resolution
unresolved
no resolver link, observed 2026-08-01T19:35:43.232595Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:35:43.232595Z digest=sha256:58b9d7be3bef62b2cfb0cd23c3a6941d05d6cbbfbd03fa960cb446e3216fdd63

Observation e63431a9-5f0b-4529-b843-e92792c78768 · outbound

This paper cites Journal of Atmospheric and Solar-Terrestrial Physics , keywords =.

Constraining the radial decay timescale of solar surface magnetic field through a comparative study of data-assimilative 2D surface flux transport and 3D dynamo models Journal of Atmospheric and Solar-Terrestrial Physics , keywords =

Reference 71

Resolution
unresolved
no resolver link, observed 2026-08-01T19:35:43.293483Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:35:43.293483Z digest=sha256:32506ee3e2dc3aef49f76c32d78e3ee899485d2ddbf6aa44bb83464bada11703

Reference 72

Resolution
unresolved
no resolver link, observed 2026-08-01T19:35:43.350693Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:35:43.350693Z digest=sha256:f311504c08dc7e31b28b5c9ecb7ac4c1377a87d3c861d5a04a9a3699a147e399

Reference 73

Resolution
unresolved
no resolver link, observed 2026-08-01T19:35:43.463187Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:35:43.463187Z digest=sha256:e6268b923a207158eb59cfc31e4219bd2dfc3c31a18e4c904d020ff6d91a96fe

Reference 74

Resolution
unresolved
no resolver link, observed 2026-08-01T19:35:43.519252Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:35:43.519252Z digest=sha256:ee98b56a48735b61d8597a5d8c9ac6fe9a81556d541ab65bd9d3f5f19f71c80b

Observation b9daac12-fcd0-47b7-adfa-8390af2f741c · outbound

This paper cites Living Reviews in Solar Physics , keywords =.

Constraining the radial decay timescale of solar surface magnetic field through a comparative study of data-assimilative 2D surface flux transport and 3D dynamo models Living Reviews in Solar Physics , keywords =

Reference 75

Resolution
unresolved
no resolver link, observed 2026-08-01T19:35:43.597152Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:35:43.597152Z digest=sha256:83f6f804301bc5f2f7d864c92942b5336a715735e23a38c7d5ab3c0b9d182f99

Observation 528f0e96-7b74-45dd-9729-543f17f8ea46 · outbound

This paper cites Local Helioseismology of Sunspots: Current Status and Perspectives (Invited Review).

Constraining the radial decay timescale of solar surface magnetic field through a comparative study of data-assimilative 2D surface flux transport and 3D dynamo models Local Helioseismology of Sunspots: Current Status and Perspectives (Invited Review)

Reference 76

Resolution
unresolved
no resolver link, observed 2026-08-01T19:35:43.678036Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:35:43.678036Z digest=sha256:341d799980bdb1bc5b3012e369633d6ad8e370e747c8de3f909aaf8ef9df363b

Reference 77

Resolution
unresolved
no resolver link, observed 2026-08-01T19:35:43.765854Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:35:43.765854Z digest=sha256:367c8fdb73e782c5f42676c3a3111027636de82986632419f95e099454e359d1

Observation 68baca47-2ae8-42aa-baa2-f05d21e9661b · outbound

This paper cites The Sun's Global Photospheric and Coronal Magnetic Fields: Observations and Models.

Constraining the radial decay timescale of solar surface magnetic field through a comparative study of data-assimilative 2D surface flux transport and 3D dynamo models The Sun's Global Photospheric and Coronal Magnetic Fields: Observations and Models

Reference 78

Resolution
unresolved
no resolver link, observed 2026-08-01T19:35:43.856157Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:35:43.856157Z digest=sha256:fb1ddddaf319a1cbabf6dba3b961828f4ae969d80ab74187db21925564df8513

Observation 86cdc599-04e1-42ba-874e-9addd9907658 · outbound

This paper cites , year = 1964, month = nov, volume =.

Constraining the radial decay timescale of solar surface magnetic field through a comparative study of data-assimilative 2D surface flux transport and 3D dynamo models , year = 1964, month = nov, volume =

Reference 79

Resolution
unresolved
no resolver link, observed 2026-08-01T19:35:43.939353Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:35:43.939353Z digest=sha256:729fb53fed7c3690aa75c65751f003baff712723c89e2557de96df0d4f08b8a1

Observation 7ff9b787-9b9a-407a-8671-24121f6190f8 · outbound

This paper cites Living Reviews in Solar Physics , keywords =.

Constraining the radial decay timescale of solar surface magnetic field through a comparative study of data-assimilative 2D surface flux transport and 3D dynamo models Living Reviews in Solar Physics , keywords =

Reference 80

Resolution
verified exact
doi, observed 2026-08-01T19:38:37.815433Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=arxiv_source observed=2026-08-01T19:35:44.030231Z digest=sha256:409f05650c919c38d6375d94a2f94762912799619a22cc169cd92597ef7f0c1b

Reference 81

Resolution
verified exact
doi, observed 2026-08-01T19:38:37.619380Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=arxiv_source observed=2026-08-01T19:35:44.124292Z digest=sha256:9337efa729257f139b333ea21618445ff38b5076d146b78bcc0326bb129697d2

Reference 82

Resolution
unresolved
no resolver link, observed 2026-08-01T19:35:44.283288Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:35:44.283288Z digest=sha256:e08068b63db10cd63bc2a3ec188fece253f5700cb76c8f7033799dcd621560e3

Reference 83

Resolution
unresolved
no resolver link, observed 2026-08-01T19:35:44.462355Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:35:44.462355Z digest=sha256:8913887efa95beca4c378e8d5bc703b85352a3a35fe7a830449f224a41d25560

Observation bfafdb48-34ee-4843-907f-15d0b5092e93 · outbound

This paper cites The solar magnetic field since 1700: II. Physical reconstruction of total, polar and open flux.

Constraining the radial decay timescale of solar surface magnetic field through a comparative study of data-assimilative 2D surface flux transport and 3D dynamo models The solar magnetic field since 1700: II. Physical reconstruction of total, polar and open flux

Reference 84

Resolution
unresolved
no resolver link, observed 2026-08-01T19:35:44.649206Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:35:44.649206Z digest=sha256:2dc1b3eed78cc045c8504f2924d95761ae3b3f11d26df09d1f06b3ea64e7001e

Reference 85

Resolution
unresolved
no resolver link, observed 2026-08-01T19:35:44.826240Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:35:44.826240Z digest=sha256:a476613ea34cbb9acef21eec514f4303c8f3fedf0153d0446930ba6267fc22d3

Observation 15491131-dc58-433e-96d9-86c4689df1a2 · outbound

This paper cites an unresolved cited work.

Constraining the radial decay timescale of solar surface magnetic field through a comparative study of data-assimilative 2D surface flux transport and 3D dynamo models Unresolved cited work

Reference 86

Resolution
unresolved
no resolver link, observed 2026-08-01T19:35:44.940671Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:35:44.940671Z digest=sha256:adb64664970596f6b5aa8b98bb94fbee16265728b4fa9c64194df613eccc5bf6

Observation c2526289-12a5-4380-8dce-47458d62b799 · outbound

This paper cites Algebraic quantification of an active region's contribution to the solar cycle.

Constraining the radial decay timescale of solar surface magnetic field through a comparative study of data-assimilative 2D surface flux transport and 3D dynamo models Algebraic quantification of an active region's contribution to the solar cycle

Reference 87

Resolution
unresolved
no resolver link, observed 2026-08-01T19:35:45.004198Z

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Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:35:45.004198Z digest=sha256:67e2f3a4d1fd075593e657453e63c423ce3fa56f06fd73c679bde8ced9c40b4c

Reference 88

Resolution
unresolved
no resolver link, observed 2026-08-01T19:35:45.060710Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:35:45.060710Z digest=sha256:010aa24cfba0087d6ce20da52d8c8f58d65b14ce35786b0017ccd32a3ae03cdd

Reference 89

Resolution
unresolved
no resolver link, observed 2026-08-01T19:35:45.121849Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:35:45.121849Z digest=sha256:6da52068ffadf231b8209458ed9b517665612c1277b9ea58f3da5f697abd2a05

Reference 90

Resolution
unresolved
no resolver link, observed 2026-08-01T19:35:45.228683Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:35:45.228683Z digest=sha256:b61a011dc73549de51131b43af131aa1eb0446438bd2ad6e1f56e8534bfafc99

Reference 91

Resolution
unresolved
no resolver link, observed 2026-08-01T19:35:45.351360Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:35:45.351360Z digest=sha256:9499ce37c17886b85984d6455c0007804042ff29e06af9ad9da037d9dd61d664

Reference 92

Resolution
verified exact
doi, observed 2026-08-01T19:38:37.483692Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=arxiv_source observed=2026-08-01T19:35:45.418056Z digest=sha256:843691fd1d111b4158858ff6831ae472b3f02e7aadb5d4f88076b8063db9da52

Observation 64492082-13de-404c-b192-f9dff70b0047 · outbound

This paper cites Optimization of surface flux transport models for the solar polar magnetic field.

Constraining the radial decay timescale of solar surface magnetic field through a comparative study of data-assimilative 2D surface flux transport and 3D dynamo models Optimization of surface flux transport models for the solar polar magnetic field

Reference 93

Resolution
unresolved
no resolver link, observed 2026-08-01T19:35:45.479764Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:35:45.479764Z digest=sha256:7e3f731e0f62d0ef8fcb36bcae29190738909f35f86da3cbdbfb954e409e304e

Reference 94

Resolution
unresolved
no resolver link, observed 2026-08-01T19:35:45.540535Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:35:45.540535Z digest=sha256:eaddd02a40642162726776f594157ebee3624745246d4d14bb0c777a7b6cf3d2

Reference 95

Resolution
verified exact
doi, observed 2026-08-01T19:38:37.352373Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=arxiv_source observed=2026-08-01T19:35:45.630348Z digest=sha256:af44257bf9d074ec9d3000618dce88e07198d9b392866c59525d122f6f7f8cbd

Observation 5032d51d-b52a-4864-9768-0b0b20a79f74 · outbound

This paper cites an unresolved cited work.

Constraining the radial decay timescale of solar surface magnetic field through a comparative study of data-assimilative 2D surface flux transport and 3D dynamo models Unresolved cited work

Reference 96

Resolution
verified exact
doi, observed 2026-08-01T19:38:37.204663Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=arxiv_source observed=2026-08-01T19:35:45.720608Z digest=sha256:8e09324217883a1dc0d4a0e227b74a089957e002468cdb5abaf8198b1b208a6d

Reference 97

Resolution
unresolved
no resolver link, observed 2026-08-01T19:35:45.829953Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:35:45.829953Z digest=sha256:92d61c55d8270850807dea4abb7f41ad413a70c03ec762f178125ed1c9183001

Reference 98

Resolution
unresolved
no resolver link, observed 2026-08-01T19:35:45.938926Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:35:45.938926Z digest=sha256:1c58ad7fad2b35ab220661e3864d6a1ada04d872de6790fd7416e6691f789986

Reference 99

Resolution
unresolved
no resolver link, observed 2026-08-01T19:35:46.023334Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:35:46.023334Z digest=sha256:f47e539c95237516bdad8ca97a845ef04a6f7e33694073c87fffb4115fb68497

Reference 100

Resolution
verified exact
doi, observed 2026-08-01T19:38:37.072727Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=arxiv_source observed=2026-08-01T19:35:46.128207Z digest=sha256:54d0f50404252de470b4c2ce14644bccd9c60bb3869605019ad21eefebfee226

Reference 101

Resolution
unresolved
no resolver link, observed 2026-08-01T19:35:46.238189Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:35:46.238189Z digest=sha256:bda84f39ae2c57665825ce44521af46cb9323abff69bda7d0290df9a7f9c9473

Reference 102

Resolution
verified exact
doi, observed 2026-08-01T19:38:36.913428Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=arxiv_source observed=2026-08-01T19:35:46.346750Z digest=sha256:62e8ebf6d241863888be79c72add70b6923a5ac0002bc872e7a1ad4d3fc3a3f5

Observation 549da7da-add2-4789-bdd0-fce89762f6a1 · outbound

This paper cites Living Reviews in Solar Physics , keywords =.

Constraining the radial decay timescale of solar surface magnetic field through a comparative study of data-assimilative 2D surface flux transport and 3D dynamo models Living Reviews in Solar Physics , keywords =

Reference 103

Resolution
verified exact
doi, observed 2026-08-01T19:38:36.745736Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=arxiv_source observed=2026-08-01T19:35:46.457740Z digest=sha256:fe110ecfcd1147e3551f0869e77b84e01238a40ecaa7c3251e61c0bd58078e15

Pith citing papers

No inbound Pith citation observations are available.