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Somigliana Normal Gravity Calculator

Evaluate Somigliana normal gravity from an explicit ellipsoid and matching equatorial/polar normal-gravity constants in m/s^2; not observed gravity, altitude correction or a mixed-datum model.

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Description

Calculate Somigliana normal gravity from an explicit ellipsoid and compatible equatorial/polar constants.

Geodesy distinguishes a mathematical reference ellipsoid, a realized coordinate datum and the physical gravity field. Geodetic latitude follows the ellipsoid normal; geocentric latitude follows a radius from the center. Ellipsoidal height, orthometric height and geoid undulation are separate signed quantities. Keep the declared ellipsoid, coordinate axes, angular units and time scale with a result.

Calculate Somigliana normal gravity from an explicit ellipsoid and compatible equatorial/polar constants.

GRS80 provides a reference ellipsoid and a normal gravity model. Geometric flattening and model normal gravity are reference quantities; neither identifies a measured local gravity or a datum realization by itself.1

When to use this tool

Use this tool when you need to calculate Somigliana normal gravity from an explicit ellipsoid and compatible equatorial/polar constants.

How to use the tool and how it works

  1. Enter semiMajorMeters, flattening, latitudeDegrees, equatorialGravity, polarGravity using the definitions below.
  2. Run the operation. Resolve input-format errors before interpreting an output.
  3. Read result.gravityMetersPerSecondSquared, using the stated boundary, ordering, sign and absence conventions.

Let r=b/a=1−f and e²=f(2−f). Calculate [gammaEquator cos²(phi)+r gammaPole sin²(phi)]/sqrt(1−e²sin²(phi)), returning m/s².2

Input fieldMeaning and unitsAccepted input
semiMajorMetersEquatorial semiaxis a in meters, 1–10⁸. It is a radius, not a diameter.Finite numeric value satisfying the stated comparisons.
flatteningDimensionless ordinary flattening f=(a-b)/a, from zero through 0.02; supply f rather than inverse flattening.Finite numeric value satisfying the stated comparisons.
latitudeDegreesGeodetic latitude in degrees, north positive; the operation’s pole restrictions apply.Finite numeric value satisfying the stated comparisons.
equatorialGravityPositive normal gravity at the ellipsoid equator in m/s², at most 100.Finite numeric value satisfying the stated comparisons.
polarGravityPositive normal gravity at the ellipsoid pole in m/s², at most 100.Finite numeric value satisfying the stated comparisons.
Output fieldInterpretation
resultObject containing the fields below.
result.gravityMetersPerSecondSquaredModeled normal gravity in m/s², not an observed or height-corrected gravity.
json
{
  "input": {
    "semiMajorMeters": 10,
    "flattening": 0,
    "latitudeDegrees": 0,
    "equatorialGravity": 9.8,
    "polarGravity": 9.9
  },
  "output": {
    "result": {
      "gravityMetersPerSecondSquared": 9.8
    }
  }
}

Limitations and assumptions

  • Both caller-supplied normal gravities are in (0,100] m/s². This is normal gravity on the reference ellipsoid, not observed gravity at arbitrary elevation or a terrain/anomaly correction.
  • All quantities are finite and retain the units stated for this operation. Ellipsoid-parameter tools use semi-major axis 1–10⁸ m and dimensionless flattening 0–0.02; explicit-axis tools use 0.9a≤b≤a unless a tighter bound is stated. These tools do not fetch datums, geoid grids, satellite observations or Earth-orientation updates.
  • Every declared outer field is required and unknown outer fields are rejected. Strings and JSON text have size limits, lists are bounded to 128 entries, and JSON nesting/node counts are bounded. Tighter operation-specific bounds stated above take precedence.
  • Numeric results must be finite. Large physical magnitudes are allowed by the output evidence checks, while integer fields and source schemas retain their exactness rules. Source indexes are zero-based. Floating-point residues can remain even where an ideal formula gives an exact zero.

Alternative or Complementary methods

Use a coordinate transform for a change of representation and explicit datum parameters for a change of reference frame. Preserve model and convergence metadata, and use observation and datum information appropriate to a real survey before interpreting a computed tolerance as accuracy.

References

  1. Geodetic Reference System 1980 (corrected reference) — H. Moritz; International Association of Geodesy, hosted by MIT

  2. Tool behavior and example: Somigliana Normal Gravity Theoretical Formula Calculator — tool.io

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