-
We observed that the total ice mass of a glacier is not preserved during SIA simulations without mass balance component. We further observe that the ice seems to move "uphill" and spread in regions wh…
-
Dear CASM developers,
I found that although the formation energies at 0K CE are zero for two end members (as they are set as references), the ones generated from finite-T MC are not.
I can under…
-
@jscuds @vsavram I didn't make this clear in #1, but there are 2 places in the LUNA algo where it will be useful to experiment with numerical methods: 1) The overall optimization algo, the focus of #…
-
I've been talking with @astrocaroline about an idea for augmenting the Sonora models with some cheap-and-useful ancillary information. Here is a sketch of the idea we have:
### An opportunity: fi…
-
I kinda hacked into this because I needed multiple countries included in the returns policy, but in my case the same policy applied to all, there were no differences. This would need further modificat…
-
Dear @mandli,
when I learn the **03 finite_differences** file, I could not understand the part of Error Analysis. Could you give me some help? thanks!!Please forgive me for asking some naive questio…
-
The DG method is implemented using matrix operators (Eigen library matrices) with double scalar type.
For the particle transport, we construct a matrix of the form $M=M' r + M^{''} r^2 + M^{'''} \Del…
-
`ProtocolDAGResult`s are pulled by users to evaluate free energy differences for `Transformation`s they are interested in. These can be rather large, and many can be pulled for a given `Transformation…
-
Right now, the jacobian of the full lightcurve doesn't match the finite differences at/around the points of contact. The lower level code works (ie. passes tests), which seems to indicate either 1) th…
-
In radio astronomy, we often are given a set of RA/Dec coordinates along with a VLSR (LSR usually being what Astropy calls LSRK) for each source. From this, we would like to compute the radial velocit…