Triple
T2126381
| Position | Surface form | Disambiguated ID | Type / Status |
|---|---|---|---|
| Subject | Schwarzschild–Milne equations |
E46433
|
entity |
| Predicate | solutionMethods |
P8791
|
FINISHED |
| Object |
Feautrier method
The Feautrier method is a numerical technique used in radiative transfer to stably and accurately solve second-order differential equations for the radiation field in stellar atmospheres and similar media.
|
E236569
|
NE FINISHED |
Provenance (5 batches)
| Stage | Batch ID | Job type | Status |
|---|---|---|---|
| creating | batch_69a88a1626548190ae59a5028c3baa8e |
elicitation | completed |
| NER | batch_69abbdc3a12081908e95ae870207367f |
ner | completed |
| NED1 | batch_69ae51a0e8ac8190992588bf2bf496ab |
ned_source_triple | completed |
| NED2 | batch_69ae52e79c788190bbe6eb5baba08a71 |
ned_description | completed |
| NEDg | batch_69ae521c7810819086b88bb5f062597e |
nedg | completed |
Created at: March 4, 2026, 7:44 p.m.