Datasets:
Update README.md
Browse files
README.md
CHANGED
@@ -12,6 +12,8 @@ task_ids:
|
|
12 |
- multivariate-time-series-forecasting
|
13 |
---
|
14 |
|
|
|
|
|
15 |
# How To Load from HuggingFace Hub
|
16 |
|
17 |
1. Be sure to have `the_well` installed (`pip install the_well`)
|
@@ -86,14 +88,14 @@ Table: VRMSE metrics on test sets (lower is better). Best results are shown in b
|
|
86 |
|
87 |
**Grid type:** spherical coordinates, uniform in \\((\log r, \theta,\phi)\\). Simulations are done for a portion of a sphere (not the whole sphere), so the simulation volume is like a spherical cake slice.
|
88 |
|
89 |
-
**Initial and boundary conditions:** The temperature at the inner boundary (IB) is first set to equal that of the appropriate radius coordinate in the MESA (1D) model (\\(400\~R_\odot\\) and \\(300\~R_\odot\\)) and the density selected to approximately recover the initial total mass of the star in the simulation (\\(15.4\~M_\odot\\) and \\(14\~M_\odot\\)).
|
90 |
Between \\(300\~R_\odot\\) and \\(400\~R_\odot\\), the initial profile is constructed with the radiative luminosity to be \\(10^5\~L_\odot\\), and this is kept fixed in the IB.
|
91 |
|
92 |
**Simulation time-step:** ~2 days.
|
93 |
|
94 |
-
**Data are stored separated by (\\(\Delta t\\)):** units here are sort of arbitrary, \\(\Delta t= 8\\).
|
95 |
|
96 |
-
**Total time range (\\(t_{min}\\) to \\(t_{max}\\)):** \\(t_{min} = 2\\), \\(t_{max} = 23402\\) (arbitrary).
|
97 |
|
98 |
**Spatial domain size:** \\(R\\) from \\(300-6700~{\rm R_\odot}\\), θ from \\(π/4−3π/4\\) and \\(\phi\\) from \\(0−π\\), with \\(δr/r ≈ 0.01\\).
|
99 |
|
|
|
12 |
- multivariate-time-series-forecasting
|
13 |
---
|
14 |
|
15 |
+
This Dataset is part of [The Well Collection](https://huggingface.co/papers/2412.00568).
|
16 |
+
|
17 |
# How To Load from HuggingFace Hub
|
18 |
|
19 |
1. Be sure to have `the_well` installed (`pip install the_well`)
|
|
|
88 |
|
89 |
**Grid type:** spherical coordinates, uniform in \\((\log r, \theta,\phi)\\). Simulations are done for a portion of a sphere (not the whole sphere), so the simulation volume is like a spherical cake slice.
|
90 |
|
91 |
+
**Initial and boundary conditions:** The temperature at the inner boundary (IB) is first set to equal that of the appropriate radius coordinate in the MESA (1D) model ( \\(400\~R_\odot\\) and \\(300\~R_\odot\\)) and the density selected to approximately recover the initial total mass of the star in the simulation ( \\(15.4\~M_\odot\\) and \\(14\~M_\odot\\)).
|
92 |
Between \\(300\~R_\odot\\) and \\(400\~R_\odot\\), the initial profile is constructed with the radiative luminosity to be \\(10^5\~L_\odot\\), and this is kept fixed in the IB.
|
93 |
|
94 |
**Simulation time-step:** ~2 days.
|
95 |
|
96 |
+
**Data are stored separated by ( \\(\Delta t\\)):** units here are sort of arbitrary, \\(\Delta t= 8\\).
|
97 |
|
98 |
+
**Total time range ( \\(t_{min}\\) to \\(t_{max}\\)):** \\(t_{min} = 2\\), \\(t_{max} = 23402\\) (arbitrary).
|
99 |
|
100 |
**Spatial domain size:** \\(R\\) from \\(300-6700~{\rm R_\odot}\\), θ from \\(π/4−3π/4\\) and \\(\phi\\) from \\(0−π\\), with \\(δr/r ≈ 0.01\\).
|
101 |
|