International Summer Institute for Modeling in Astrophysics
Parent: UCSC Department of Astronomy and Astrophysics
eScholarship stats: Breakdown by Item for October, 2024 through January, 2025
| Item | Title | Total requests | Download | View-only | %Dnld |
|---|---|---|---|---|---|
| 0r71s3v9 | Detecting the earliest stages of giant planet formation in scattered light | 31 | 5 | 26 | 16.1% |
| 375312sn | Planet migration in self-gravitating disks | 21 | 1 | 20 | 4.8% |
| 3813j8hb | Abundance and evolution of gas around Beta Pictoris | 21 | 4 | 17 | 19.0% |
| 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% |
| 7f43z58p | Day-night cold traps for TiO in hot Jupiter atmospheres | 19 | 3 | 16 | 15.8% |
| 4461g8gh | Gap formation in transitional and pre-transitional disks: dust filtration in the presence of coagulation and fragmentation. | 18 | 1 | 17 | 5.6% |
| 6t8022wn | Thermohaline mixing with the small Peclet number approximation | 18 | 3 | 15 | 16.7% |
| 06k8s8bw | Destroying resonance between Neptune and its resonant Kuiper Belt Objects by stochastic planetesimal scatterings | 17 | 1 | 16 | 5.9% |
| 0xc2c5w6 | Multi-phase turbulent ISM: Theory Confronting Observations | 17 | 2 | 15 | 11.8% |
| 1kt0k72g | Convectively generated zonal jets by thunderstorms on Jupiter | 17 | 1 | 16 | 5.9% |
| 4707m4sx | Ohmic dissipation in hot Jupiters | 16 | 2 | 14 | 12.5% |
| 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% |
| 7d34p4sr | Radiative Rayleigh-Taylor instabilities | 15 | 3 | 12 | 20.0% |
| 80f7f71k | Fragmentation of metal-poor star-forming cores | 15 | 2 | 13 | 13.3% |
| 7n09f14x | Improving the grain growth model in the outer part of circumstellar disks | 14 | 1 | 13 | 7.1% |
| 1jx495sk | Singular tidal modes and the regularization of the tidal singularity | 13 | 0 | 13 | 0.0% |
| 35s753p6 | Disk Dynamos in Simulations of Collapsing Cores | 13 | 2 | 11 | 15.4% |
| 7m77v9sd | Charge exchange in the colliding winds of Hot Jupiters and their host stars | 13 | 1 | 12 | 7.7% |
| 3p74t14x | A simple model for understanding the day-night temperature constrast on Hot Jupiters | 12 | 1 | 11 | 8.3% |
| 4v42t9t6 | Planetesimal formation: shear instabilities at the dust-rich mid-plane | 12 | 1 | 11 | 8.3% |
| 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% |
| 0bx48606 | Planetary dynamics in collisional particle disks | 9 | 0 | 9 | 0.0% |
| 3rw147jx | Stoked Dynamos | 8 | 0 | 8 | 0.0% |
| 96m3847f | Analytical studies of fragmentation during gravitational collapse | 8 | 2 | 6 | 25.0% |
| 3bt2d4tq | The Sun's meridional circulation and interior magnetic field | 7 | 2 | 5 | 28.6% |
Note: Due to the evolving nature of web traffic, the data presented here should be considered approximate and subject to revision. Learn more.