Summary of "Lec- 3: Distributed Systems and Distributed Computing"

Summary: Distributed Systems and Distributed Computing

Definitions and core idea

Distributed system: a collection of independent computers that appears to users as a single coherent system. Components cooperate (via message passing) to achieve a common goal.

Distributed computing: using a distributed system to solve computational problems by dividing a problem into tasks that are solved by one or more computers communicating with one another.

Primary purposes and benefits

High-level architecture (layers / components)

How distributed computing solves problems (workflow)

  1. Form a team (cluster) of independent machines and present them as a single system to users.
  2. Partition the large problem or data set into smaller tasks or chunks.
  3. Assign tasks to different machines (nodes); each node works on its assigned portion.
  4. Nodes communicate and coordinate via message passing (IPC) to exchange data, control signals, or intermediate results.
  5. Aggregate results from nodes to produce the final output visible to the user (single input → single output despite internal distribution).
  6. Use replication, redundancy, and middleware features so services remain available when individual nodes fail.

Distinction: distributed computing vs. parallel computing

Historical and practical context / examples

Noted takeaways

Methodology / step-by-step instructions

Speakers / sources

Category ?

Educational


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