Titan U glossary

Hail Core

A hail core is the concentrated region of a thunderstorm where hail is either falling to the surface or being held aloft by the updraft. On radar it shows as a very high-reflectivity center, and in the field it appears as a bright, often whitish shaft below the storm.

A hail core is the concentrated region of a thunderstorm where hail is either falling to the surface or being held aloft by the updraft. On radar it shows as a very high-reflectivity center, and in the field it appears as a bright, often whitish shaft below the storm.

How it forms

Hail grows when a strong updraft suspends embryos in the mixed-phase layer of the storm, where supercooled water is available for accretion. The stones circulate through repeated passes of freezing and collection, adding layers of clear and cloudy ice. A stone stays aloft until the updraft can no longer support it, then falls out on the downshear or downdraft side of the storm.

The heaviest hail typically ends up along the outer edge of the strongest updraft, on the boundary between updraft and downdraft. That geometry is why radar often shows the strongest hail signature just adjacent to the storm's updraft core rather than at its exact center.

How forecasters and spotters read it

Environmental clues to a strong hail core start with CAPE and shear. Higher CAPE supports stronger updrafts that can suspend larger stones, and shear separates the updraft from the downdraft so precipitation does not fall back through the updraft and choke it. A lower freezing level and dry midlevel air also help, because stones melt less before reaching the ground and dry air enhances evaporative cooling around the downdraft.

In the field, a bright, luminous, almost white core beneath a strong supercell is a common hail signature. Spotters typically report hail size relative to common objects, since size drives damage far more than count does.

Where it misleads

A tall, intense hail core aloft does not mean giant hail is reaching the surface. Melting through a deep warm layer can shrink hail substantially before it lands, and pulse storms may hold their largest stones aloft and never drop them at severe size.

The visual brightness of a hail shaft can also come from very heavy rain lit by the sun. Definitive confirmation usually needs a dual-polarization radar signature or a ground report.

Keep going

How Hail Core connects

Builds on 2

  • Updraft

    A hail core builds on a strong updraft, which holds growing stones aloft where supercooled water lets them gain layers of ice.

  • Freezing Level

    How much hail from a hail core reaches the ground at size builds partly on the freezing level, since a lower one usually means less melting on the way down.

Contrasts with 1

  • Precipitation Core

    A hail core and a heavy rain core can look alike on reflectivity, so telling them apart usually takes dual-polarization data or a ground report.

Measured by 1

  • Maximum Estimated Size of Hail

    The likely size of the largest hail in a hail core is estimated on radar by MESH, which uses reflectivity from the sub-freezing part of the storm.

Seen in 3

  • Composite Reflectivity

    Composite reflectivity is a first-glance product for hail-supporting cores held aloft, which a low tilt may not show.

  • Differential Reflectivity

    Differential reflectivity helps flag a hail core, since high reflectivity with ZDR near zero suggests tumbling hailstones rather than only rain.

  • Radar Reflectivity

    A hail core shows on radar as a very high reflectivity center, though high reflectivity alone does not confirm hail.

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