2011 International Summer Institute for Modeling in Astrophysics
Parent: International Summer Institute for Modeling in Astrophysics
eScholarship stats: Breakdown by Item for June through September, 2024
Item | Title | Total requests | Download | View-only | %Dnld |
---|---|---|---|---|---|
0r71s3v9 | Detecting the earliest stages of giant planet formation in scattered light | 49 | 31 | 18 | 63.3% |
4v42t9t6 | Planetesimal formation: shear instabilities at the dust-rich mid-plane | 37 | 24 | 13 | 64.9% |
7f43z58p | Day-night cold traps for TiO in hot Jupiter atmospheres | 35 | 20 | 15 | 57.1% |
4707m4sx | Ohmic dissipation in hot Jupiters | 26 | 8 | 18 | 30.8% |
0xc2c5w6 | Multi-phase turbulent ISM: Theory Confronting Observations | 25 | 13 | 12 | 52.0% |
7n09f14x | Improving the grain growth model in the outer part of circumstellar disks | 23 | 6 | 17 | 26.1% |
1kt0k72g | Convectively generated zonal jets by thunderstorms on Jupiter | 22 | 4 | 18 | 18.2% |
4461g8gh | Gap formation in transitional and pre-transitional disks: dust filtration in the presence of coagulation and fragmentation. | 20 | 3 | 17 | 15.0% |
0bx48606 | Planetary dynamics in collisional particle disks | 19 | 3 | 16 | 15.8% |
35s753p6 | Disk Dynamos in Simulations of Collapsing Cores | 19 | 5 | 14 | 26.3% |
96m3847f | Analytical studies of fragmentation during gravitational collapse | 17 | 1 | 16 | 5.9% |
06k8s8bw | Destroying resonance between Neptune and its resonant Kuiper Belt Objects by stochastic planetesimal scatterings | 16 | 3 | 13 | 18.8% |
3p74t14x | A simple model for understanding the day-night temperature constrast on Hot Jupiters | 16 | 3 | 13 | 18.8% |
7m77v9sd | Charge exchange in the colliding winds of Hot Jupiters and their host stars | 16 | 3 | 13 | 18.8% |
3813j8hb | Abundance and evolution of gas around Beta Pictoris | 14 | 1 | 13 | 7.1% |
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