Paper Citation Record · LEDGER

Driving solar coronal MHD simulations on high-performance computers

As of 16 August 2026, this Paper Citation Record lists 38 of 38 outbound references and 0 inbound Pith citation observations for arXiv:1908.08557.

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

pith.paper-citation-record.v1
1908.08557 v1

Coverage vector

measured 38 of 38 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-14T11:41:16.576835Z

measured 38 of 38 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-16T06:30:59.297886+00:00

measured 0 of 0 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links

measured 0 of 1 external citation measurements

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

Source: cited_works

Reference resolution

38 of 38 outbound references displayed

verified exact11
verified fuzzy5
unresolved22
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External citation measurements

No source-named external measurement is stored.

Outbound references

Observation 2bfd62a5-773f-4ebd-b403-a352d84ca82f · outbound

This paper cites and Gudiksen, B., On the nature of coronal loops above the quiet sun network.

Driving solar coronal MHD simulations on high-performance computers and Gudiksen, B., On the nature of coronal loops above the quiet sun network

Reference 1

Resolution: verified exact; doi, observed 2026-08-14T11:41:17.011137Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation 81ee1312-d0b0-4388-bf5d-2b59adc2e1bd · outbound

This paper cites urlcolor=magenta Contr.

Driving solar coronal MHD simulations on high-performance computers urlcolor=magenta Contr

Reference 2

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T11:41:17.131695Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation e79344ad-d9cb-4c51-965a-d2b0daae3308 · outbound

This paper cites an unresolved cited work.

Driving solar coronal MHD simulations on high-performance computers Unresolved cited work

Reference 3

Resolution: unresolved; raw_fallback, observed 2026-08-14T11:41:17.112198Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation 11895988-df9a-47bf-9d2d-5d2a982703df · outbound

This paper cites urlcolor=magenta Cent.

Driving solar coronal MHD simulations on high-performance computers urlcolor=magenta Cent

Reference 4

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T11:41:17.090900Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation 5dd3a2ec-0bd8-4339-8af1-a00799d1cc0d · outbound

This paper cites urlcolor=magenta ApJL http://adsabs.harvard.edu/abs/2017ApJ...850L..29B , 2017, 850, L29 (5pp), DOI: urlcolor=blue 10.3847/2041-8213/aa9988 https://doi.org/10.3847/2041-8213/aa9988.

Driving solar coronal MHD simulations on high-performance computers urlcolor=magenta ApJL http://adsabs.harvard.edu/abs/2017ApJ...850L..29B , 2017, 850, L29 (5pp), DOI: urlcolor=blue 10.3847/2041-8213/aa9988 https://doi.org/10.3847/2041-8213/aa9988

Reference 5

Resolution: unresolved; no resolver link, observed 2026-08-14T11:41:16.375501Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6f874c09-76cd-4b23-a9d7-18aa6644fefd · outbound

This paper cites and Peter, H., Observationally driven 3D MHD model of the solar corona above an active region.

Driving solar coronal MHD simulations on high-performance computers and Peter, H., Observationally driven 3D MHD model of the solar corona above an active region

Reference 6

Resolution: unresolved; no resolver link, observed 2026-08-14T11:41:16.380227Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6d984f71-8643-497b-90f8-77246aa5326c · outbound

This paper cites and Peter, H., Coronal loops above an Active Region: Observation versus model.

Driving solar coronal MHD simulations on high-performance computers and Peter, H., Coronal loops above an Active Region: Observation versus model

Reference 7

Resolution: verified exact; doi, observed 2026-08-14T11:41:16.953573Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation 57d53885-69f1-4358-bc15-de12dc988139 · outbound

This paper cites and Peter, H., Coronal energy input and dissipation in a solar Active Region 3D MHD model.

Driving solar coronal MHD simulations on high-performance computers and Peter, H., Coronal energy input and dissipation in a solar Active Region 3D MHD model

Reference 8

Resolution: verified exact; doi, observed 2026-08-14T11:41:16.940230Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation 80e44ce9-4563-41fa-a28a-bc4f88a6b5ed · outbound

This paper cites and Peter, H., Scaling laws of coronal loops compared to a 3D MHD model of an active region.

Driving solar coronal MHD simulations on high-performance computers and Peter, H., Scaling laws of coronal loops compared to a 3D MHD model of an active region

Reference 9

Resolution: verified exact; doi, observed 2026-08-14T11:41:16.922500Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation aea972a9-c700-48e6-bc17-16e2e4603fe3 · outbound

This paper cites and Brandenburg , A., Magnetic Helicity Reversal in the Corona at Small Plasma Beta.

Driving solar coronal MHD simulations on high-performance computers and Brandenburg , A., Magnetic Helicity Reversal in the Corona at Small Plasma Beta

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-14T11:41:16.401060Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 55d7e1a1-dc88-4673-88c0-235b195252e3 · outbound

This paper cites and Cheung , M.C.M., A model for the formation of the active region corona driven by magnetic flux emergence.

Driving solar coronal MHD simulations on high-performance computers and Cheung , M.C.M., A model for the formation of the active region corona driven by magnetic flux emergence

Reference 11

Resolution: verified exact; doi, observed 2026-08-14T11:41:16.895614Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation cf28a85c-9d49-4f86-8973-bc6cfbda9cca · outbound

This paper cites and Antiochos , S.K., Effect of coronal elemental abundances on the radiative loss function.

Driving solar coronal MHD simulations on high-performance computers and Antiochos , S.K., Effect of coronal elemental abundances on the radiative loss function

Reference 12

Resolution: unresolved; no resolver link, observed 2026-08-14T11:41:16.422020Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 781cdea8-85f9-41dc-980f-5202079bc243 · outbound

This paper cites and Nordlund, ., Bulk heating and slender magnetic loops in the solar corona.

Driving solar coronal MHD simulations on high-performance computers and Nordlund, ., Bulk heating and slender magnetic loops in the solar corona

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-14T11:41:16.427145Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c0405390-5eda-44bc-812f-1135b92be174 · outbound

This paper cites and Nordlund, ., An ab initio approach to the solar coronal heating problem.

Driving solar coronal MHD simulations on high-performance computers and Nordlund, ., An ab initio approach to the solar coronal heating problem

Reference 14

Resolution: unresolved; no resolver link, observed 2026-08-14T11:41:16.434447Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 292708fb-0788-44c4-9c70-0185b25248dc · outbound

This paper cites and Carlsson, M., On Redshifts and Blueshifts in the Transition Region and Corona.

Driving solar coronal MHD simulations on high-performance computers and Carlsson, M., On Redshifts and Blueshifts in the Transition Region and Corona

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-14T11:41:16.440098Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1e08d39e-ef1b-4beb-b2a2-4bb769c7dc83 · outbound

This paper cites urlcolor=magenta Sol.

Driving solar coronal MHD simulations on high-performance computers urlcolor=magenta Sol

Reference 16

Resolution: unresolved; no resolver link, observed 2026-08-14T11:41:16.446576Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 84492f0c-448c-40d2-bea0-e77e8471e9b4 · outbound

This paper cites and Golub , L., The Hinode (Solar-B) Mission: An Overview.

Driving solar coronal MHD simulations on high-performance computers and Golub , L., The Hinode (Solar-B) Mission: An Overview

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-14T11:41:16.451174Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2f885ff0-4579-432f-a2ef-74e7f004a2b6 · outbound

This paper cites and Tsuneta , S., The Hinode Spectro-Polarimeter.

Driving solar coronal MHD simulations on high-performance computers and Tsuneta , S., The Hinode Spectro-Polarimeter

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-14T11:41:16.455995Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 222d465c-49a2-42f1-a81c-95bb8b6538b4 · outbound

This paper cites and Moreno-Insertis, F., On the Origin of the Type II Spicules: Dynamic Three-dimensional MHD Simulations.

Driving solar coronal MHD simulations on high-performance computers and Moreno-Insertis, F., On the Origin of the Type II Spicules: Dynamic Three-dimensional MHD Simulations

Reference 19

Resolution: verified exact; doi, observed 2026-08-14T11:41:16.810630Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation 8aab8c8c-240b-45e1-aafc-586062f8a411 · outbound

This paper cites urlcolor=magenta ApJ http://adsabs.harvard.edu/abs/1972ApJ...174..499P , 1972, 174, 499--510, DOI: urlcolor=blue 10.1086/151512 https://doi.org/10.1086/151512.

Driving solar coronal MHD simulations on high-performance computers urlcolor=magenta ApJ http://adsabs.harvard.edu/abs/1972ApJ...174..499P , 1972, 174, 499--510, DOI: urlcolor=blue 10.1086/151512 https://doi.org/10.1086/151512

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-14T11:41:16.466139Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 458ee83e-a9cc-436a-ab3b-eda376a7a352 · outbound

This paper cites urlcolor=magenta ApJ http://adsabs.harvard.edu/abs/1988ApJ...330..474P , 1988, 330, 474--479, DOI: urlcolor=blue 10.1086/166485 https://doi.org/10.1086/166485.

Driving solar coronal MHD simulations on high-performance computers urlcolor=magenta ApJ http://adsabs.harvard.edu/abs/1988ApJ...330..474P , 1988, 330, 474--479, DOI: urlcolor=blue 10.1086/166485 https://doi.org/10.1086/166485

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-14T11:41:16.473354Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation cf63b867-4048-4825-b6c9-ffb5a685530a · outbound

This paper cites and Bingert, S., Constant cross section of loops in the solar corona.

Driving solar coronal MHD simulations on high-performance computers and Bingert, S., Constant cross section of loops in the solar corona

Reference 22

Resolution: verified exact; doi, observed 2026-08-14T11:41:16.772545Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation 8bdf2308-c479-447c-a724-04b8e3f2c233 · outbound

This paper cites and Korreck , K.E., Structure of solar coronal loops: from miniature to large-scale.

Driving solar coronal MHD simulations on high-performance computers and Korreck , K.E., Structure of solar coronal loops: from miniature to large-scale

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-14T11:41:16.489106Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8c1742a1-b9ff-4290-befb-c4f9dc4a92e3 · outbound

This paper cites and Cameron , R.H., Limitations of force-free magnetic field extrapolations: Revisiting basic assumptions.

Driving solar coronal MHD simulations on high-performance computers and Cameron , R.H., Limitations of force-free magnetic field extrapolations: Revisiting basic assumptions

Reference 24

Resolution: verified exact; doi, observed 2026-08-14T11:41:16.746588Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation 8c37b8dc-3753-4ab0-970d-7252dbf9ae73 · outbound

This paper cites and Dahlburg , R.B., Coronal Heating, Weak MHD Turbulence, and Scaling Laws.

Driving solar coronal MHD simulations on high-performance computers and Dahlburg , R.B., Coronal Heating, Weak MHD Turbulence, and Scaling Laws

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-14T11:41:16.499629Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8ebbd1ad-0eb1-46c5-8bc4-329c254465ef · outbound

This paper cites and Dahlburg , R.B., Nonlinear Dynamics of the Parker Scenario for Coronal Heating.

Driving solar coronal MHD simulations on high-performance computers and Dahlburg , R.B., Nonlinear Dynamics of the Parker Scenario for Coronal Heating

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-14T11:41:16.509141Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0a7d7ed5-8985-4d4e-9816-428d9fb94647 · outbound

This paper cites urlcolor=magenta ApJ http://adsabs.harvard.edu/abs/2012ApJ...750...62R , 2012, 750, 62, DOI: urlcolor=blue 10.1088/0004-637X/750/1/62 https://doi.org/10.1088/0004-637X/750/1/62.

Driving solar coronal MHD simulations on high-performance computers urlcolor=magenta ApJ http://adsabs.harvard.edu/abs/2012ApJ...750...62R , 2012, 750, 62, DOI: urlcolor=blue 10.1088/0004-637X/750/1/62 https://doi.org/10.1088/0004-637X/750/1/62

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-14T11:41:16.514666Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 06568acb-16fe-4dff-b2fe-bd4c5fe9902b · outbound

This paper cites urlcolor=magenta ApJ http://esoads.eso.org/abs/2017ApJ...834...10R , 2017, 834, 10, DOI: urlcolor=blue 10.3847/1538-4357/834/1/10 https://doi.org/10.3847/1538-4357/834/1/10.

Driving solar coronal MHD simulations on high-performance computers urlcolor=magenta ApJ http://esoads.eso.org/abs/2017ApJ...834...10R , 2017, 834, 10, DOI: urlcolor=blue 10.3847/1538-4357/834/1/10 https://doi.org/10.3847/1538-4357/834/1/10

Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-14T11:41:16.519941Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5fe5aa92-ac9b-470c-8b93-5fe7a0aefbcc · outbound

This paper cites and Sanchez Almeida , J., Empirical model of an average solar granule ; in Cool Stars, Stellar Systems, and the Sun , edited by R.

Driving solar coronal MHD simulations on high-performance computers and Sanchez Almeida , J., Empirical model of an average solar granule ; in Cool Stars, Stellar Systems, and the Sun , edited by R

Reference 29

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T11:41:17.068113Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation da150b2b-dac2-4973-bd70-ac8e571500a2 · outbound

This paper cites and Title, A.M., On the patterns of the solar granulation and supergranulation.

Driving solar coronal MHD simulations on high-performance computers and Title, A.M., On the patterns of the solar granulation and supergranulation

Reference 30

Resolution: verified exact; doi, observed 2026-08-14T11:41:16.686105Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation 99df11a4-dff9-4d75-90b7-ebaab155d493 · outbound

This paper cites urlcolor=magenta ApJ http://adsabs.harvard.edu/abs/1957ApJ...126..202S , 1957, 126, 202, DOI: urlcolor=blue 10.1086/146386 https://doi.org/10.1086/146386.

Driving solar coronal MHD simulations on high-performance computers urlcolor=magenta ApJ http://adsabs.harvard.edu/abs/1957ApJ...126..202S , 1957, 126, 202, DOI: urlcolor=blue 10.1086/146386 https://doi.org/10.1086/146386

Reference 31

Resolution: verified exact; doi, observed 2026-08-14T11:41:16.671424Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation 67cefafa-7103-4c59-b406-438badbbb470 · outbound

This paper cites and H \"a rm, R., Transport phenomena in a completely ionized gas.

Driving solar coronal MHD simulations on high-performance computers and H \"a rm, R., Transport phenomena in a completely ionized gas

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-14T11:41:16.542462Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 834142c5-166d-49e1-8d5f-be32b3f66f60 · outbound

This paper cites and Owens , J.K., The Solar Optical Telescope for the Hinode Mission: An Overview.

Driving solar coronal MHD simulations on high-performance computers and Owens , J.K., The Solar Optical Telescope for the Hinode Mission: An Overview

Reference 33

Resolution: unresolved; no resolver link, observed 2026-08-14T11:41:16.546824Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 95bbaaed-2135-448c-ba8e-b2ddb55fcc21 · outbound

This paper cites and Berger , M.A., On the Relationship Between Photospheric Footpoint Motions and Coronal Heating in Solar Active Regions.

Driving solar coronal MHD simulations on high-performance computers and Berger , M.A., On the Relationship Between Photospheric Footpoint Motions and Coronal Heating in Solar Active Regions

Reference 34

Resolution: verified exact; doi, observed 2026-08-14T11:41:16.646828Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation fa85d71a-462f-42dc-9082-3cc0643514b1 · outbound

This paper cites and DeLuca , E.E., Heating of the Solar Chromosphere and Corona by Alfv \'e n Wave Turbulence.

Driving solar coronal MHD simulations on high-performance computers and DeLuca , E.E., Heating of the Solar Chromosphere and Corona by Alfv \'e n Wave Turbulence

Reference 35

Resolution: unresolved; no resolver link, observed 2026-08-14T11:41:16.555770Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a510de01-8563-4dee-ac1c-72638fd12f16 · outbound

This paper cites and Erd \'e lyi , R., Magnetic tornadoes as energy channels into the solar corona.

Driving solar coronal MHD simulations on high-performance computers and Erd \'e lyi , R., Magnetic tornadoes as energy channels into the solar corona

Reference 36

Resolution: unresolved; no resolver link, observed 2026-08-14T11:41:16.561882Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 37ae0449-fac6-42cd-8a3a-220f6c84c86e · outbound

This paper cites , " * write output.state after.block = add.period write newline.

Driving solar coronal MHD simulations on high-performance computers , " * write output.state after.block = add.period write newline

Reference 37

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T11:41:17.042368Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation 7dc093fa-512f-4280-9893-209ca97f52b8 · outbound

This paper cites write newline.

Driving solar coronal MHD simulations on high-performance computers write newline

Reference 38

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T11:41:17.027066Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Pith citing papers

No inbound Pith citation observations are available.