2011 International Summer Institute for Modeling in Astrophysics
Parent: International Summer Institute for Modeling in Astrophysics
eScholarship stats: Breakdown by Item for March through June, 2026
| Item | Title | Total requests | Download | View-only | %Dnld |
|---|---|---|---|---|---|
| 0bx48606 | Planetary dynamics in collisional particle disks | 171 | 47 | 124 | 27.5% |
| 06k8s8bw | Destroying resonance between Neptune and its resonant Kuiper Belt Objects by stochastic planetesimal scatterings | 169 | 48 | 121 | 28.4% |
| 96m3847f | Analytical studies of fragmentation during gravitational collapse | 156 | 57 | 99 | 36.5% |
| 0xc2c5w6 | Multi-phase turbulent ISM: Theory Confronting Observations | 154 | 60 | 94 | 39.0% |
| 7f43z58p | Day-night cold traps for TiO in hot Jupiter atmospheres | 154 | 68 | 86 | 44.2% |
| 0r71s3v9 | Detecting the earliest stages of giant planet formation in scattered light | 147 | 64 | 83 | 43.5% |
| 1kt0k72g | Convectively generated zonal jets by thunderstorms on Jupiter | 144 | 39 | 105 | 27.1% |
| 4707m4sx | Ohmic dissipation in hot Jupiters | 143 | 67 | 76 | 46.9% |
| 7n09f14x | Improving the grain growth model in the outer part of circumstellar disks | 140 | 51 | 89 | 36.4% |
| 4v42t9t6 | Planetesimal formation: shear instabilities at the dust-rich mid-plane | 134 | 36 | 98 | 26.9% |
| 3p74t14x | A simple model for understanding the day-night temperature constrast on Hot Jupiters | 132 | 48 | 84 | 36.4% |
| 7m77v9sd | Charge exchange in the colliding winds of Hot Jupiters and their host stars | 129 | 52 | 77 | 40.3% |
| 35s753p6 | Disk Dynamos in Simulations of Collapsing Cores | 123 | 49 | 74 | 39.8% |
| 3813j8hb | Abundance and evolution of gas around Beta Pictoris | 118 | 58 | 60 | 49.2% |
| 4461g8gh | Gap formation in transitional and pre-transitional disks: dust filtration in the presence of coagulation and fragmentation. | 113 | 33 | 80 | 29.2% |
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