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Source: paper_references, paper_reference_links, observed 2026-08-14T14:28:38.257023Z
Paper Citation Record · LEDGER
Photophoresis in the circumjovian disk and its impact on the orbital configuration of the Galilean satellites
As of 16 August 2026, this Paper Citation Record lists 16 of 16 outbound references and 0 inbound Pith citation observations for arXiv:1908.03128.
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16 of 16 outbound references displayed
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Outbound references
Observation cbd67842-ec5d-4b41-ae82-55fbaafc1bba · outbound
This paper cites 1976, Progress of The oretical Physics, 56, 1756 Arakawa, S., Tanaka, H., Kataoka, A., & Nakamoto, T.
Photophoresis in the circumjovian disk and its impact on the orbital configuration of the Galilean satellites 1976, Progress of The oretical Physics, 56, 1756 Arakawa, S., Tanaka, H., Kataoka, A., & Nakamoto, T
Reference 1
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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 030a7dca-cd3e-4100-b1f8-86e50e3d851e · outbound
This paper cites 2013), Msat is the mass of the satellite, and Rsat is the radius of the satellite.
Photophoresis in the circumjovian disk and its impact on the orbital configuration of the Galilean satellites 2013), Msat is the mass of the satellite, and Rsat is the radius of the satellite
Reference 2
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- raw_fallback, observed 2026-08-14T14:28:39.078726Z
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No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation f4f59cdf-1039-426b-9240-d031f235a128 · outbound
This paper cites Here, we compare the photophoretic force FPh and the radiation force Frad.
Photophoresis in the circumjovian disk and its impact on the orbital configuration of the Galilean satellites Here, we compare the photophoretic force FPh and the radiation force Frad
Reference 3
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- raw_fallback, observed 2026-08-14T14:28:38.746354Z
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 f10bc67b-812f-4e8e-92db-7b51e66b606c · outbound
This paper cites Although the current magnetic field of Jupiter is 7.8 G, according to the observations from the Juno spacecraf t (Bolton et al.
Photophoresis in the circumjovian disk and its impact on the orbital configuration of the Galilean satellites Although the current magnetic field of Jupiter is 7.8 G, according to the observations from the Juno spacecraf t (Bolton et al
Reference 4
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No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation d7602c7b-412a-471f-93f9-8b828b8ac1a0 · outbound
This paper cites submitted).
Reference 5
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- raw_fallback, observed 2026-08-14T14:28:39.002627Z
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No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 686b17a3-77a2-417e-a0b7-443c3fce47a5 · outbound
This paper cites However, there is another requirement to make an inner cav- ity in a steady-state disk.
Photophoresis in the circumjovian disk and its impact on the orbital configuration of the Galilean satellites However, there is another requirement to make an inner cav- ity in a steady-state disk
Reference 6
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- raw_fallback, observed 2026-08-14T14:28:38.901354Z
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 32e7d2f6-a3d4-499d-bed6-cfd6f2e05099 · outbound
This paper cites an unresolved cited work.
Photophoresis in the circumjovian disk and its impact on the orbital configuration of the Galilean satellites Unresolved cited work
Reference 7
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- raw_fallback, observed 2026-08-14T14:28:38.885112Z
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 c18e293d-95d4-4a8f-a817-c212c23d631e · outbound
This paper cites (B.3) Then, the planetary radius of young Jupiter would be as large as twice that of current Jupiter if we assumed conservation o f spin angular momentum.
Photophoresis in the circumjovian disk and its impact on the orbital configuration of the Galilean satellites (B.3) Then, the planetary radius of young Jupiter would be as large as twice that of current Jupiter if we assumed conservation o f spin angular momentum
Reference 8
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- raw_fallback, observed 2026-08-14T14:28:38.841777Z
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 df5f6288-51fd-47f2-b57b-5fdd39c12394 · outbound
This paper cites Appendix C: Radiation pressure The radiation pressure is caused by the direct momentum tran s- fer of photons.
Photophoresis in the circumjovian disk and its impact on the orbital configuration of the Galilean satellites Appendix C: Radiation pressure The radiation pressure is caused by the direct momentum tran s- fer of photons
Reference 9
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- raw_fallback, observed 2026-08-14T14:28:38.759723Z
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 c6a6cbaf-3944-4345-8eb7-14619bf0f664 · outbound
This paper cites In contrast to FPh, the residual gravity caused by gas drag FD is independent of a/ lm (Weidenschilling 1977): FD = − 4πa3 3 ρp ρg dp dr.
Photophoresis in the circumjovian disk and its impact on the orbital configuration of the Galilean satellites In contrast to FPh, the residual gravity caused by gas drag FD is independent of a/ lm (Weidenschilling 1977): FD = − 4πa3 3 ρp ρg dp dr
Reference 10
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- raw_fallback, observed 2026-08-14T14:28:38.649330Z
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 a00ea9ac-1190-4232-b76f-9614d670c1b4 · outbound
This paper cites (E.1) The heat conduction timescale within a dust particle, τcond, is (Krauss & Wurm 2005; Loesche & Wurm.
Photophoresis in the circumjovian disk and its impact on the orbital configuration of the Galilean satellites (E.1) The heat conduction timescale within a dust particle, τcond, is (Krauss & Wurm 2005; Loesche & Wurm
Reference 11
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- raw_fallback, observed 2026-08-14T14:28:38.569171Z
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 897d02b8-5cb4-421e-b0f1-28a6df73cee7 · outbound
This paper cites an unresolved cited work.
Photophoresis in the circumjovian disk and its impact on the orbital configuration of the Galilean satellites Unresolved cited work
Reference 12
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No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 7ac529ea-cf4c-4540-a5c4-88adc370912d · outbound
This paper cites The contribution of gas to the Rosseland mean opacity of a disk with solar metallicity, κR, g, is given by Freedman et al.
Photophoresis in the circumjovian disk and its impact on the orbital configuration of the Galilean satellites The contribution of gas to the Rosseland mean opacity of a disk with solar metallicity, κR, g, is given by Freedman et al
Reference 13
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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 a4853fea-8513-4ad4-a385-811a67e1bea1 · outbound
This paper cites 8] −1 cm2 g−1.
Photophoresis in the circumjovian disk and its impact on the orbital configuration of the Galilean satellites 8] −1 cm2 g−1
Reference 14
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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 3635d6b6-61a4-4607-a456-5467aeb96ee0 · outbound
This paper cites Figure G.2 shows the surface density distribution of the dis k for various viscosity parameters.
Photophoresis in the circumjovian disk and its impact on the orbital configuration of the Galilean satellites Figure G.2 shows the surface density distribution of the dis k for various viscosity parameters
Reference 15
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- raw_fallback, observed 2026-08-14T14:28:38.311783Z
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 172ac995-392b-4d3c-b533-f814ea9100d6 · outbound
This paper cites The migration timescale τmig is given by (e.g., Paardekooper et al.
Photophoresis in the circumjovian disk and its impact on the orbital configuration of the Galilean satellites The migration timescale τmig is given by (e.g., Paardekooper et al
Reference 16
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- raw_fallback, observed 2026-08-14T14:28:38.293599Z
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.
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