Sediment Grain-Size Analysis Methods
2026-03-12Application Note
Abstract: Grain size is a fundamental parameter for interpreting depositional processes, sediment transport, and environmental change in fluvial, coastal, and marine systems. This application note provides an overview of how sediment particle size distributions (PSDs) can be classified, measured, and reported using modern laboratory methods. It also presents practical strategies for integrating coarse and fine fractions and offers reporting guidelines to support clear, consistent, and comparable PSD datasets for sedimentary analysis.
Keywords: Sediment; grain size; particle size distribution; sieving; sedimentation; laser diffraction; image analysis
1. Introduction
Grain size distributions (PSDs) form the basis for reconstructing depositional environments, sediment transport dynamics, and post-depositional modification across rivers, deltas, coastal zones, continental shelves, and deep-water systems. Many surface processes—such as channel migration, delta growth, shoreline evolution, and shelf sedimentation—are controlled by how sediment of varying grain sizes is transported, sorted, and ultimately deposited. These relationships are illustrated in Figure 1. 
Figure 1. Schematic depiction of sediment transport modes in riverine or coastal settings.
In unconsolidated systems, sediments act as natural archives that record environmental conditions and depositional energy. A sample’s PSD reflects interactions among sediment supply, transport capacity, and local hydrodynamic conditions. For example, coarser and well-sorted sands typically form in higher-energy environments such as surf zones or channel bars, whereas finer, poorly sorted muds usually indicate low-energy settings like distal shelves, estuaries, or lacustrine environments.
Translating these conceptual relationships into laboratory PSD measurement can be challenging. Natural sediment samples commonly include:
- extremely broad size ranges, from sub-micron clay to centimeter-scale gravel and shell material.
- diverse mineralogy and grain shapes, including platy mica, elongate heavy minerals and angular lithic fragments.
- methodological inconsistencies stemming from a long history of traditional approaches (sieving, pipette, hydrometer) and modern optical techniques (laserdiffraction, imaging) which do not always produce numerically equivalent results.
This application note outlines how sediment grain size can be classified, measured, and integrated using modern laboratory workflows. The discussion is organized into three areas of focus:
- a. Grain size classification systems
- b. Measurement techniques
- c. Data integration and standardization
2. Grain Size Classification Systems
Grain size classification provides a common language for describing sediment and soil textures, enabling consistent interpretation across geology, soil science, engineering, and environmental studies.
2.1 Wentworth Scale
Sediments are most commonly categorized using the Wentworth scale, which divides particles into gravel, sand, silt, and clay based on their diameter [1]:
- Gravel: 2 mm to 64 mm
- Sand: 0.0625 mm (1/16 mm) to 2 mm
- Silt: 0.0039 mm (1/256 mm) to 0.0625 mm
- Clay: < 0.0039 mm (1/256 mm)
These categories form the foundation of sedimentological description and are widely used in depositional facies analysis, engineering applications and environmental assessments.
2.2 Phi Scale
For finer resolution within the Wentworth framework, sedimentologists frequently use the phi (φ) scale, a base-2 logarithmic transformation of grain diameter introduced by Krumbein [2]. Referenced to 1 mm, the phi scale expresses grain size in powers of two. The phi value is related to grain diameter (d, in mm) by the expression:
φ = −log2(d / D0)
where d is the grain diameter and D0 is 1 mm. This transformation converts the Wentworth scale into simple whole-number intervals, which makes grain-size data easier to handle in statistical and graphical analysis. Increasingly positive φ values correspond to progressively finer grain sizes than 1 mm, whereas increasingly negative φ values correspond to progressively coarser grain sizes.
The phi scale offers several advantages:
- Provides a uniform logarithmic axis for plotting PSDs.
- Supports widely used statistical descriptors such as the Folk and Ward mean, sorting, skewness, and kurtosis.[3]
- Facilitates comparison across historical and modern datasets.
3. Recommended Measurement Techniques
3.1 Overview of Common PSD techniques
Particle size analysis methods report an equivalent diameter, rather than the true three-dimensional geometry of each grain. For natural sediments—often mixtures of angular fragments, platy minerals, shell debris, and aggregates—this distinction is essential. Table 3.1 summarizes the commonly used PSD techniques and their operational characteristics. Because each technique defines particle size differently, PSDs measured by different instrument methods will not be numerically identical. In practice, laboratories select the method best suited to their size range, material type, and workflow.
3.2 Sieving
Working Principle
Figure 2. Typical sieving workflow for sediment analysis
Sieving mechanically separates grains according to their ability to pass through a stack of sieves arrange from coarse to fine (e.g. 8mm, 4 mm, 2 mm, 1 mm, 500 µm, 250 µm, 125 µm, 63 µm). After shaking, the mass retained on each sieve is recorded, and the percentage by mass in each size class is expressed as a percentage of the total sample
mass, from which a PSD can be calculated. The reported diameter corresponds to the minim grain dimension that passes through the sieve opening.
Table 3.1 Common techniques for particle size analysis of sediments
| Technique | Typical Size Range | Size Definition | Typical basis | Sample State | Typical Run Time |
| Sieving | 63 µm - 125 mm | Sieve-aperture passing size | Mass | Usually dry | 15-20 min |
| Sedimentation | 1 µm - 63 µm | Stokes equivalent sphere diameter | Mass | Suspension | tens of min to hours |
| Laser diffraction | 0.02 µm - 2000 um | Volume-equivalent sphere diameter | Volume | Wet or dry | 1 min |
| Optical microscopy | 30 µm - several mm | 2D projected size | Number | Usually dry | variable (count-based) |
Typical Applications
Sieving is most effective for the coarse fraction of sediment, including:
- beach and dune sands.
- channel and bar gravels.
- marine aggregates and shelly sediments.
- the sand- and gravel- portion of mixed samples.
In many coastal and marine workflows, sediment is dry-sieved down to a defined cut-off (for example, 1 mm), and finer material is analyzed with another technique, commonly laser diffraction. The coarse and fine datasets are later merged.
3.3 Sedimentation
Working Principle
Sedimentation methods determine grain size from the settling behavior of particles in a fluid column. Under laminar flow, small particles settle according to Stokes’ law, where settling velocity depends on diameter, density contrast, and fluid viscosity. By tracking mass or density over time, the cumulative proportion finer than a given Stokes-equivalent diameter can be derived.
In the pipette method, aliquots are withdrawn from a fixed depth at predetermined times, dried, and weighed to quantify the fine fraction remaining in suspension. In the hydrometer method, a hydrometer is used to measure changes in suspension density as particles settle, these readings are converted to a cumulative PSD.
Both methods and require careful control of dispersion, temperature, and fluid properties to ensure reliable results. 
Figure 3. Schematic comparison of pipette and hydrometer sedimentation methods.
Typical Applications
Sedimentation methods have a long history in the analysis of fine-grained sediments, particularly cohesive mud. Sedimentation methods remain widely used for:
- reproducing legacy datasets originally obtained by pipette or hydrometer.
- focused study of very fine silt and clay.
- laboratories optimized for traditional sedimentation workflows.
Although many modern marine and coastal laboratories have migrated to laser diffraction for the fine fraction due to higher throughput and continuous PSD output, sedimentation methods continue to serve as valuable reference techniques.
3.4 Laser Diffraction
Working Principle In sediment applications, laser diffraction is usually performed in wet dispersion. The sediment sample is suspended in a liquid and circulated through a measurement cell to maintain a representative population of particles. A laser beam passes through the flowing suspension, and the scattered light pattern, (where coarser particles scatter at small angles and finer particles at wider angles) is recorded.
Particle size distribution (PSD) is computed from this scattering pattern using an optical model (Fraunhofer or Mie). The technique provides rapid, repeatable measurements and is widely used in sediment transport, depositional analysis, and routine laboratory workflows.
Typical Applications

Figure 4. Working principle of a wet-dispersion laser diffraction system.
Laser diffraction is increasingly used to characterize:
- subtidal and intertidal sediments from muds to sands;
- estuarine, deltaic, and continental shelf deposits;
- suspended sediment collected from rivers, estuaries, and coastal waters.
Common laboratory workflow includes:
① Pre-treat sediment (e.g. desalination, removal of organics or carbonates per protocol).
② Optionally wet-sieve to remove coarse material (for example, 2 mm).
③ Disperse the fine fraction using chemical dispersants and/or ultrasonication.
④ Measure PSD by wet laser diffraction, typically with replicate runs.
Field applications include: In situ laser diffraction sensors deployed in rivers, estuaries, and coasts provide near-realtime particle size measurements to support studies of suspended sediment dynamics, resuspension events, and turbidity processes.[4]
3.5 Optical Microscopy
Working Principle
Optical microscopy and image-based particle analysis acquire two-dimensional images of sediment grains, either as static mounts or as particles passing through a flow cell, as shown in Figure 5. Image-processing algorithms identify individual grains and compute size and shape metrics such as:
- equivalent circular diameter based on projected area;
- maximum and minimum Feret diameters;
- aspect ratio, roundness, and related shape descriptors.
Typical Applications
Image-based methods are particularly valuable when:
- the coarse fractions (sand, gravel, shell fragments) are of primary interest.
- grain shape and angularity are required to interpret transport history or abrasion.
- visual confirmation of specific grain types or large particles is required.

Figure 5. Static and Dynamic imaging configurations for sediment grain analysis.
Image analysis is of ten combined with other PSD techniques (e.g. sieving or laser diffraction) to provide complementary grain-shape information and targeted verification of specific size classes.
4. Data Integration and Standardization
No single measurement technique effectively captures the full range of particle sizes found in natural sediments. As a result, laboratories routinely combine methods to obtain a complete PSD. A common workflow is to combine:
- dry sieving for the sand and gravel fraction above a chosen cut-off.
- wet laser diffraction for the finer fraction below that cut-off.
To merge these outputs into a single, coherent PSD, several steps are important
1. Define the cut-off size and splitting method.
The bulk sample must be divided in a reproducible way at the chosen boundary (e.g., 1 mm). The coarse fraction proceeds to sieving, and the fine fraction to laser diffraction. Clear documentation of the cut-of sieve and any wet-sieving procedures ensures consistency across samples.
2. Normalize datasets back to a common basis.
Because sieving repor ts mass fractions and laser diffraction typically reports volume-based PSDs, both datasets must be normalized back to a consistent reference – usually total sample mass. This step ensures that the merged PSD accurately reflects the true proportions of fine and coarse material.
3. Construct a unified PSD from complementary size domains.
The final cumulative PSD integrates:
- sieve-derived size classes for coarse grains, and
- laser-derived size classes for fine grains
This “split-and-merge” approach leverages the strength of each technique while minimizing the limitations associated with any single method.
Conclusion
Grain size is one of their most informative descriptors of sedimentary materials, offering insights into transport processes, depositional environments, and post-depositional modification. The reliability of PSD data, however, depends on how measurements are performed, interpreted, and reported. Sieving, sedimentation, laser diffraction, and image analysis can each deliver high-quality results when instruments are properly configured, and samples are appropriately pre-treated and dispersed. For meaningful comparison among datasets, or across laboratories, it is essential to clearly report:
- the diameter definition used.
- the reporting basis.
- and sample preparation and dispersion steps applied.
- any method-specific assumptions relevant to interpretation.
When wide particle size ranges are required, a split-and-merge workflow remains an efficient strategy—provided the cut-off, normalization, and potential sources of uncertainty are documented. With transparent methodology and consistent reporting, PSDs become a robust foundation for interpreting sediment dynamics, depositional processes and environmental change.
Reference
[1] Wentworth, C. K. (1922). A Scale of Grade and Class Terms for Clastic Sediments. The [2] Journal of Geology, 30(5), 377–392.
[2] Krumbein, W. C. (1934). Size frequency distributions of sediments. Journal of Sedimentary Petrology, 4(2), 65–77.
[3] Folk, R. L., & Ward, W. C. (1957). Brazos River Bar: A Study in the Significance of Grain Size Parameters. Journal of Sedimentary Petrology, 27(1), 3–26.
[4] DeepSizer 300 for Immediate Sediment Response in Extreme Hydrological Conditions.
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