I'm new to Apache Cassandra. While reading about it, I found in following paragraph that node and partition do not mean the same.
One suggested measure of whether a secondary index is warranted is whether the number of partitions is approximately equal to number of nodes in cluster. Mathematically this seem to offer a balance of speeding up the reads rather than slowing them down.
Can anyone clarify?
The number of partitions is the number of buckets you can split your data into by unique values of your indexed columns. So, for example, if you index on sex, you'll get two partitions: male and female. If you index on US states, you'll get 50. If you index on email, you may get the # of partitions comparable to the number of rows in the table. The guideline specifies that the performance is best when the number of unique values in the indexed column is the same as the number of nodes.
Related
I would like to know if there is an efficient strategy to write my Spark dataframe in a delta Table in Datalake.
As a rule of thumb I am splitting the dataframe into some column that has between 70 and 300 different values.
The 'trick' I use to see which column is the candidate to use in the "partitionBy" is the following.
I transform my dataframe into a temporary table and look at the cardinality.
df.createOrReplaceTempView("my_table")
%sql
select
count(distinct(column1)) as column1,
count(distinct(column2)) as column2,
...
from my_table
Then I pick the column with a cardinality between 70 - 300, depending on the size of the table
mentally calculating table_size / 128 MB -->is this correct ?
df.write.partitionBy("column_candidate")
.format("delta")
.mode("overwrite")
.option("overwriteSchema", "true")
.save(outputpaht)
This method I use does not seem very scientific, and I would like to know if there is a better way to estimate it.I have also seen that there is something called "repartition" but I don't know how to use it or if it is interesting.
How can I calculate the partitions in a more scientific way?
The number of partitions in spark should be decided thoughtfully based on the cluster configuration and requirements of the application. Increasing the number of partitions will make each partition have less data or no data at all. Apache Spark can run a single concurrent task for every partition of an RDD, up to the total number of cores in the cluster. If a cluster has 30 cores then programmers want their RDDs to have 30 cores at the very least or maybe 2 or 3 times of that.
Some acclaimed guidelines for the number of partitions in Spark are as follows-
When the number of partitions is between 100 and 10K partitions based on the size of the cluster and data, the lower and upper bound should be determined.
o The lower bound for spark partitions is determined by 2 X number of cores in the cluster available to application.
o Determining the upper bound for partitions in Spark, the task should take 100+ ms time to execute. If it takes less time, then the partitioned data might be too small or the application might be spending extra time in scheduling tasks.
For more information Refer this article
I am new to the timescale database. I was learning about chunks and how to create chunks based on time.
But there is another time/space chunking which is confusing me a lot. Please help me with below queries.
What is a dimension in a timescale DB?
What is space chunking and how it works?
Thanks in advance.
A dimension in TimescaleDB is associated with a column. Each hypertable requires to define at least a time dimension, which is a time column for the time series. Then a hypertable is divided into chunks, where each chunk contains data for a time interval of the time dimension. As result all new data usually arrives into the latets chunk, while other chunks contain older data.
Then, it is possible to define space dimensions on other columns, for example device column or/and location column. No interval is defined for space dimensions, instead a number of partitions is defined. So for the same time interval, several chunks will be created, which is equivalent to the number of partitions. Data are distributed by a hashing function on the values of the space dimension. For example, if 3 partitions are defined for a space dimension on device column and 12 different device values were present in the data, each space chunk will contain 4 different values with a hash function uniformly distributing the values.
Space dimensions are specifically useful for parallel I/O, when data are stored on several disks. Another scenario is multinode, i.e., distributed version of hypertable (beta feature, which coming to release in 2.0).
There are some complex usage cases when space partitioning will be also helpful.
You can read more in add_dimension docs, cloud KB about space partitioning
A note in the doc:
Supporting more than one additional dimension is currently experimental.
AFAIK, in case of Relational Database on MPP hardware, the key to performance is a correct data distribution. While Dimensional Modeling is about query flexibility, you don't even know how the data will be queried (shuffled) in future.
For example, you have MPP Data Warehouse (Greenplum, Redshift, Synapse Analytics). For example, in 1-2 years, you expect your fact table will grow up to 10 billion of rows and you'll have 15-30 dimension tables of 10s millions of rows. How the data should be distributed accross DW nodes? Is there any common techniques? Like shard fact table and replicate dimension tables. Or should I minimize node amount in MPP DW?
I can bring specific use case, but I believe that the question arise from my misunderstanding of how Dimensional Modeling could be paired with scaling out.
One technique I’ve seen applied with success in the past is: segment the fact table (e.g., by mod’ing the date key), and distribute all dimensions across all nodes. That way all joins can be done locally.
Note that even with large dimensions, their total size on disk should be a small fraction of the total needed for the fact table.
Stackoverflow!
I wonder if there is a fancy way in Spark 2.0 to solve the situation below.
The situation is like this.
Dataset1 (TargetData) has this schema and has about 20 milion records.
id (String)
vector of embedding result (Array, 300 dim)
Dataset2 (DictionaryData) has this schema and has about 9,000 records.
dict key (String)
vector of embedding result (Array, 300 dim)
For each vector of records in dataset 1, I want to find the dict key that will be the maximum when I compute cosine similarity it with dataset 2.
Initially, I tried cross-join dataset1 and dataset2 and calculate cosine simliarity of all records, but the amount of data is too large to be available in my environment.
I have not tried it yet, but I thought of collecting dataset2 as a list and then applying udf.
Are there any other method in this situation?
Thanks,
There might be two options the one is to broadcast Dataset2 since you need to scan it for each row of Dataset1 thus avoid the network delays by accessing it from a different node. Of course in this case you need to consider first if your cluster can handle the memory cost which 9000rows x 300cols(not too big in my opinion). Also you still need your join although with broadcasting should be faster. The other option is to populate a RowMatrix from your existing vectors and leave spark do the calculations for you
So, I understand that in general one should use coalesce() when:
the number of partitions decreases due to a filter or some other operation that may result in reducing the original dataset (RDD, DF). coalesce() is useful for running operations more efficiently after filtering down a large dataset.
I also understand that it is less expensive than repartition as it reduces shuffling by moving data only if necessary. My problem is how to define the parameter that coalesce takes (idealPartionionNo). I am working on a project which was passed to me from another engineer and he was using the below calculation to compute the value of that parameter.
// DEFINE OPTIMAL PARTITION NUMBER
implicit val NO_OF_EXECUTOR_INSTANCES = sc.getConf.getInt("spark.executor.instances", 5)
implicit val NO_OF_EXECUTOR_CORES = sc.getConf.getInt("spark.executor.cores", 2)
val idealPartionionNo = NO_OF_EXECUTOR_INSTANCES * NO_OF_EXECUTOR_CORES * REPARTITION_FACTOR
This is then used with a partitioner object:
val partitioner = new HashPartitioner(idealPartionionNo)
but also used with:
RDD.filter(x=>x._3<30).coalesce(idealPartionionNo)
Is this the right approach? What is the main idea behind the idealPartionionNo value computation? What is the REPARTITION_FACTOR? How do I generally work to define that?
Also, since YARN is responsible for identifying the available executors on the fly is there a way of getting that number (AVAILABLE_EXECUTOR_INSTANCES) on the fly and use that for computing idealPartionionNo (i.e. replace NO_OF_EXECUTOR_INSTANCES with AVAILABLE_EXECUTOR_INSTANCES)?
Ideally, some actual examples of the form:
Here 's a dataset (size);
Here's a number of transformations and possible reuses of an RDD/DF.
Here is where you should repartition/coalesce.
Assume you have n executors with m cores and a partition factor equal to k
then:
The ideal number of partitions would be ==> ???
Also, if you can refer me to a nice blog that explains these I would really appreciate it.
In practice optimal number of partitions depends more on the data you have, transformations you use and overall configuration than the available resources.
If the number of partitions is too low you'll experience long GC pauses, different types of memory issues, and lastly suboptimal resource utilization.
If the number of partitions is too high then maintenance cost can easily exceed processing cost. Moreover, if you use non-distributed reducing operations (like reduce in contrast to treeReduce), a large number of partitions results in a higher load on the driver.
You can find a number of rules which suggest oversubscribing partitions compared to the number of cores (factor 2 or 3 seems to be common) or keeping partitions at a certain size but this doesn't take into account your own code:
If you allocate a lot you can expect long GC pauses and it is probably better to go with smaller partitions.
If a certain piece of code is expensive then your shuffle cost can be amortized by a higher concurrency.
If you have a filter you can adjust the number of partitions based on a discriminative power of the predicate (you make different decisions if you expect to retain 5% of the data and 99% of the data).
In my opinion:
With one-off jobs keep higher number partitions to stay on the safe side (slower is better than failing).
With reusable jobs start with conservative configuration then execute - monitor - adjust configuration - repeat.
Don't try to use fixed number of partitions based on the number of executors or cores. First understand your data and code, then adjust configuration to reflect your understanding.
Usually, it is relatively easy to determine the amount of raw data per partition for which your cluster exhibits stable behavior (in my experience it is somewhere in the range of few hundred megabytes, depending on the format, data structure you use to load data, and configuration). This is the "magic number" you're looking for.
Some things you have to remember in general:
Number of partitions doesn't necessarily reflect
data distribution. Any operation that requires shuffle (*byKey, join, RDD.partitionBy, Dataset.repartition) can result in non-uniform data distribution. Always monitor your jobs for symptoms of a significant data skew.
Number of partitions in general is not constant. Any operation with multiple dependencies (union, coGroup, join) can affect the number of partitions.
Your question is a valid one, but Spark partitioning optimization depends entirely on the computation you're running. You need to have a good reason to repartition/coalesce; if you're just counting an RDD (even if it has a huge number of sparsely populated partitions), then any repartition/coalesce step is just going to slow you down.
Repartition vs coalesce
The difference between repartition(n) (which is the same as coalesce(n, shuffle = true) and coalesce(n, shuffle = false) has to do with execution model. The shuffle model takes each partition in the original RDD, randomly sends its data around to all executors, and results in an RDD with the new (smaller or greater) number of partitions. The no-shuffle model creates a new RDD which loads multiple partitions as one task.
Let's consider this computation:
sc.textFile("massive_file.txt")
.filter(sparseFilterFunction) // leaves only 0.1% of the lines
.coalesce(numPartitions, shuffle = shuffle)
If shuffle is true, then the text file / filter computations happen in a number of tasks given by the defaults in textFile, and the tiny filtered results are shuffled. If shuffle is false, then the number of total tasks is at most numPartitions.
If numPartitions is 1, then the difference is quite stark. The shuffle model will process and filter the data in parallel, then send the 0.1% of filtered results to one executor for downstream DAG operations. The no-shuffle model will process and filter the data all on one core from the beginning.
Steps to take
Consider your downstream operations. If you're just using this dataset once, then you probably don't need to repartition at all. If you are saving the filtered RDD for later use (to disk, for example), then consider the tradeoffs above. It takes experience to become familiar with these models and when one performs better, so try both out and see how they perform!
As others have answered, there is no formula which calculates what you ask for. That said, You can make an educated guess on the first part and then fine tune it over time.
The first step is to make sure you have enough partitions. If you have NO_OF_EXECUTOR_INSTANCES executors and NO_OF_EXECUTOR_CORES cores per executor then you can process NO_OF_EXECUTOR_INSTANCES*NO_OF_EXECUTOR_CORES partitions at the same time (each would go to a specific core of a specific instance).
That said this assumes everything is divided equally between the cores and everything takes exactly the same time to process. This is rarely the case. There is a good chance that some of them would be finished before others either because of locallity (e.g. the data needs to come from a different node) or simply because they are not balanced (e.g. if you have data partitioned by root domain then partitions including google would probably be quite big). This is where the REPARTITION_FACTOR comes into play. The idea is that we "overbook" each core and therefore if one finishes very quickly and one finishes slowly we have the option of dividing the tasks between them. A factor of 2-3 is generally a good idea.
Now lets take a look at the size of a single partition. Lets say your entire data is X MB in size and you have N partitions. Each partition would be on average X/N MBs. If N is large relative to X then you might have very small average partition size (e.g. a few KB). In this case it is usually a good idea to lower N because the overhead of managing each partition becomes too high. On the other hand if the size is very large (e.g. a few GB) then you need to hold a lot of data at the same time which would cause issues such as garbage collection, high memory usage etc.
The optimal size is a good question but generally people seem to prefer partitions of 100-1000MB but in truth tens of MB probably would also be good.
Another thing you should note is when you do the calculation how your partitions change. For example, lets say you start with 1000 partitions of 100MB each but then filter the data so each partition becomes 1K then you should probably coalesce. Similar issues can happen when you do a groupby or join. In such cases both the size of the partition and the number of partitions change and might reach an undesirable size.