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Why this feature is necessary:
Enable the reV team and general public to run reV at scale in the cloud using OEDI datasets as inputs.
A possible solution is:
Current cloud readiness of reV's modules:
Gen: Cloud ready using HSDS and WTK/NSRDB data in OEDI
Econ: Cloud ready using HSDS and WTK/NSRDB data in OEDI
Aggregation: Needs exclusion files to be loaded into HSDS, plan is to load FY20 and FY21 final inclusion layers into OEDI before 10/29. Complex aggregation schemes would require all exclusion layers to be loaded into HSDS/OEDI.
Supply Curve: For internal runs we can use the xmission tables we've generated. For the public we need to determine:
a) If they can use our xmission tables or if we can "anonymize" our xmission tables for public use, otherwise
b) We need to create a lower fidelity open-source set of xmission tables
Potential performance issue:
HSDS currently has very limited throughput interms of number of concurrent requests. This will be an issue for generation. Fortunately we hope to ameliorate the issue by moving HSDS to lambda. This should be done by the end of FY21 Q1 and should enable nearly infinite scalability in terms of parallel requests. To properly take advantage of this, it could be useful to implement this feature in rex: parallel gets for list slices rex#111
Using gen/econ .h5 files in agg and supply curve. To solutions:
Move the files from S3 to local storage (not needed with LFS below)
In this lab, the cluster has 0 compute nodes when starting and maximum size set to 8 instances. AWS ParallelCluster will grow and shrink between the min and max limits based on the cluster utilization and job queue backlog.
A GP2 Amazon EBS volume will be attached to the head-node then shared through NFS to be mounted by the compute nodes on /shared. It is generally a good location to store applications or scripts. Keep in mind that the /home directory is shared on NFS as well.
Why this feature is necessary:
Enable the reV team and general public to run reV at scale in the cloud using OEDI datasets as inputs.
A possible solution is:
Current cloud readiness of reV's modules:
a) If they can use our xmission tables or if we can "anonymize" our xmission tables for public use, otherwise
b) We need to create a lower fidelity open-source set of xmission tables
Potential performance issue:
Cloud hardware / submission ideas:
Charge code
reV
Urgency / Timeframe
FY22 design Doc
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