2011 International Summer Institute for Modeling in Astrophysics
Parent: International Summer Institute for Modeling in Astrophysics
eScholarship stats: History by Item for March through June, 2026
| Item | Title | Total requests | 2026-06 | 2026-05 | 2026-04 | 2026-03 |
|---|---|---|---|---|---|---|
| 0bx48606 | Planetary dynamics in collisional particle disks | 171 | 20 | 97 | 28 | 26 |
| 06k8s8bw | Destroying resonance between Neptune and its resonant Kuiper Belt Objects by stochastic planetesimal scatterings | 169 | 25 | 64 | 42 | 38 |
| 96m3847f | Analytical studies of fragmentation during gravitational collapse | 156 | 25 | 50 | 46 | 35 |
| 0xc2c5w6 | Multi-phase turbulent ISM: Theory Confronting Observations | 154 | 36 | 56 | 36 | 26 |
| 7f43z58p | Day-night cold traps for TiO in hot Jupiter atmospheres | 154 | 23 | 54 | 46 | 31 |
| 0r71s3v9 | Detecting the earliest stages of giant planet formation in scattered light | 147 | 21 | 59 | 37 | 30 |
| 1kt0k72g | Convectively generated zonal jets by thunderstorms on Jupiter | 144 | 20 | 58 | 35 | 31 |
| 4707m4sx | Ohmic dissipation in hot Jupiters | 143 | 22 | 44 | 34 | 43 |
| 7n09f14x | Improving the grain growth model in the outer part of circumstellar disks | 140 | 22 | 51 | 34 | 33 |
| 4v42t9t6 | Planetesimal formation: shear instabilities at the dust-rich mid-plane | 134 | 14 | 45 | 38 | 37 |
| 3p74t14x | A simple model for understanding the day-night temperature constrast on Hot Jupiters | 132 | 13 | 50 | 42 | 27 |
| 7m77v9sd | Charge exchange in the colliding winds of Hot Jupiters and their host stars | 129 | 22 | 39 | 40 | 28 |
| 35s753p6 | Disk Dynamos in Simulations of Collapsing Cores | 123 | 29 | 52 | 29 | 13 |
| 3813j8hb | Abundance and evolution of gas around Beta Pictoris | 118 | 17 | 49 | 32 | 20 |
| 4461g8gh | Gap formation in transitional and pre-transitional disks: dust filtration in the presence of coagulation and fragmentation. | 113 | 12 | 41 | 31 | 29 |
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