2011 International Summer Institute for Modeling in Astrophysics
Parent: International Summer Institute for Modeling in Astrophysics
eScholarship stats: Breakdown by Item for December, 2024 through March, 2025
| Item | Title | Total requests | Download | View-only | %Dnld |
|---|---|---|---|---|---|
| 0r71s3v9 | Detecting the earliest stages of giant planet formation in scattered light | 42 | 6 | 36 | 14.3% |
| 4707m4sx | Ohmic dissipation in hot Jupiters | 26 | 4 | 22 | 15.4% |
| 3813j8hb | Abundance and evolution of gas around Beta Pictoris | 22 | 2 | 20 | 9.1% |
| 4461g8gh | Gap formation in transitional and pre-transitional disks: dust filtration in the presence of coagulation and fragmentation. | 21 | 1 | 20 | 4.8% |
| 7n09f14x | Improving the grain growth model in the outer part of circumstellar disks | 20 | 6 | 14 | 30.0% |
| 06k8s8bw | Destroying resonance between Neptune and its resonant Kuiper Belt Objects by stochastic planetesimal scatterings | 19 | 2 | 17 | 10.5% |
| 0bx48606 | Planetary dynamics in collisional particle disks | 19 | 1 | 18 | 5.3% |
| 96m3847f | Analytical studies of fragmentation during gravitational collapse | 19 | 4 | 15 | 21.1% |
| 1kt0k72g | Convectively generated zonal jets by thunderstorms on Jupiter | 17 | 1 | 16 | 5.9% |
| 0xc2c5w6 | Multi-phase turbulent ISM: Theory Confronting Observations | 16 | 5 | 11 | 31.3% |
| 35s753p6 | Disk Dynamos in Simulations of Collapsing Cores | 15 | 4 | 11 | 26.7% |
| 3p74t14x | A simple model for understanding the day-night temperature constrast on Hot Jupiters | 15 | 2 | 13 | 13.3% |
| 7f43z58p | Day-night cold traps for TiO in hot Jupiter atmospheres | 15 | 3 | 12 | 20.0% |
| 4v42t9t6 | Planetesimal formation: shear instabilities at the dust-rich mid-plane | 13 | 2 | 11 | 15.4% |
| 7m77v9sd | Charge exchange in the colliding winds of Hot Jupiters and their host stars | 11 | 2 | 9 | 18.2% |
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