2010 International Summer Institute for Modeling in Astrophysics
Parent: International Summer Institute for Modeling in Astrophysics
eScholarship stats: Breakdown by Item for October, 2024 through January, 2025
| Item | Title | Total requests | Download | View-only | %Dnld |
|---|---|---|---|---|---|
| 375312sn | Planet migration in self-gravitating disks | 21 | 1 | 20 | 4.8% |
| 54m812j0 | The orbital decay of a retrograde planet in a protoplanetary disk | 21 | 3 | 18 | 14.3% |
| 5ff523wv | Taming jets in magnetised fluids | 21 | 4 | 17 | 19.0% |
| 2jw7q6mj | MHD jet propagation in the case of DG Tau | 19 | 2 | 17 | 10.5% |
| 73q3t00z | Geostrophic turbulence with a magnetic field | 19 | 1 | 18 | 5.3% |
| 6t8022wn | Thermohaline mixing with the small Peclet number approximation | 18 | 3 | 15 | 16.7% |
| 66c9t3c5 | Production of Elephant Trunks in HII Regions by Radiation-Magnetohydrodynamic Instabilities | 15 | 1 | 14 | 6.7% |
| 6pp4m4hj | Searching for radiative instabilites in massive star envelopes | 15 | 0 | 15 | 0.0% |
| 80f7f71k | Fragmentation of metal-poor star-forming cores | 15 | 2 | 13 | 13.3% |
| 7d34p4sr | Radiative Rayleigh-Taylor instabilities | 14 | 3 | 11 | 21.4% |
| 1jx495sk | Singular tidal modes and the regularization of the tidal singularity | 13 | 0 | 13 | 0.0% |
| 4057c3wc | The role of radiation pressure in the dynamics of HII regions at z>1 | 11 | 1 | 10 | 9.1% |
| 8618016r | Spin-down of protostars through gravitational torques | 11 | 3 | 8 | 27.3% |
| 9kz418gf | Sweet-Parker Reconnection with Anomalous Resistivity — A Toy Model | 10 | 1 | 9 | 10.0% |
| 3rw147jx | Stoked Dynamos | 8 | 0 | 8 | 0.0% |
| 3bt2d4tq | The Sun's meridional circulation and interior magnetic field | 7 | 2 | 5 | 28.6% |
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