How to deal with runtime changes to tenant-location in a clustered, multitenant web application with app-managed datasources?
I have a Java web application that supports multi-tenancy to keep customer data
separate.
Algorithm to Find the Aggregate Mass of “Granola Bar”-Like Structures?
I’m a planetary science researcher and one project I’m working on is N-body simulations of Saturn’s rings. The goal of this particular study is to watch as particles clump together under their own self-gravity and measure the aggregate mass of the clumps versus the mean velocity of all particles in the cell. We’re trying to figure out if this can explain some observations made by the Cassini spacecraft during the Saturnian summer solstice when large structures were seen casting shadows on the nearly edge-on rings. Below is a screenshot of what any given timestep looks like. (Each particle is 2 m in diameter and the simulation cell itself is around 700 m across.)
Algorithm to Find the Aggregate Mass of “Granola Bar”-Like Structures?
I’m a planetary science researcher and one project I’m working on is N-body simulations of Saturn’s rings. The goal of this particular study is to watch as particles clump together under their own self-gravity and measure the aggregate mass of the clumps versus the mean velocity of all particles in the cell. We’re trying to figure out if this can explain some observations made by the Cassini spacecraft during the Saturnian summer solstice when large structures were seen casting shadows on the nearly edge-on rings. Below is a screenshot of what any given timestep looks like. (Each particle is 2 m in diameter and the simulation cell itself is around 700 m across.)
Algorithm to Find the Aggregate Mass of “Granola Bar”-Like Structures?
I’m a planetary science researcher and one project I’m working on is N-body simulations of Saturn’s rings. The goal of this particular study is to watch as particles clump together under their own self-gravity and measure the aggregate mass of the clumps versus the mean velocity of all particles in the cell. We’re trying to figure out if this can explain some observations made by the Cassini spacecraft during the Saturnian summer solstice when large structures were seen casting shadows on the nearly edge-on rings. Below is a screenshot of what any given timestep looks like. (Each particle is 2 m in diameter and the simulation cell itself is around 700 m across.)
Algorithm to Find the Aggregate Mass of “Granola Bar”-Like Structures?
I’m a planetary science researcher and one project I’m working on is N-body simulations of Saturn’s rings. The goal of this particular study is to watch as particles clump together under their own self-gravity and measure the aggregate mass of the clumps versus the mean velocity of all particles in the cell. We’re trying to figure out if this can explain some observations made by the Cassini spacecraft during the Saturnian summer solstice when large structures were seen casting shadows on the nearly edge-on rings. Below is a screenshot of what any given timestep looks like. (Each particle is 2 m in diameter and the simulation cell itself is around 700 m across.)
Algorithm to Find the Aggregate Mass of “Granola Bar”-Like Structures?
I’m a planetary science researcher and one project I’m working on is N-body simulations of Saturn’s rings. The goal of this particular study is to watch as particles clump together under their own self-gravity and measure the aggregate mass of the clumps versus the mean velocity of all particles in the cell. We’re trying to figure out if this can explain some observations made by the Cassini spacecraft during the Saturnian summer solstice when large structures were seen casting shadows on the nearly edge-on rings. Below is a screenshot of what any given timestep looks like. (Each particle is 2 m in diameter and the simulation cell itself is around 700 m across.)
Is there any Layer approach for multicluster communication instead of service mesh approach?
We are investigating on communication between our clusters (AWS and GCP mostly) and we investigating solutions like Istio and linkerd. but the things is all of them connects each cluster to another one (like star network).
How to test issues in a local development environment that can only be introduced by clustering in production?
We recently clustered an application, and it came to light that because of how we’re doing SSL offloading via the load balancer in production it didn’t work right. I had to mimic this functionality on my local machine by SSL offloading Apache with a proxy, but it still isn’t a 1-to-1 comparison. Similar issues can arise when dealing with stateful applications and sticky sessions. What would be the industry standard for testing this kind of production “black box” scenario in a local environment, especially as it relates to clustering?
Why does storm not supply a mechanism for supplying topology necessary dependent jars other than the fat jar?
Following is a question that I had posted at the incubator-storm-user mailing list (verbatim). I had decided to open up the question here as well, because it also contains a conceptual side to it, which might be answered by non-storm users.
Why does storm not supply a mechanism for supplying topology necessary dependent jars other than the fat jar?
Following is a question that I had posted at the incubator-storm-user mailing list (verbatim). I had decided to open up the question here as well, because it also contains a conceptual side to it, which might be answered by non-storm users.