lobate
lobed

Lava flows often have a lobate appearance at the edges.

Lobate scarps are the most common structural landforms in the Bach region.

The ultimate segments (pinnules) of the fronds are mostly lobate or digitate.

On the floor is a lobate scarp that was formed as a result of contraction of the lava.

In materials that were deformed under very high temperatures, lobate grain boundaries may be taken as evidence for diffusion creep.

These glaciers are termed lobate debris aprons when surrounding mounds and mesas.

Murray and others (1974) described them as having a sinuous outline, a slightly lobate front, and a length of more than 500 km.

Schistochila have lobate lips.

Where sediment is abundant and wave and current action limited, deltas tend to be lobate, the classic example being the Nile.

These materials are called lobate debris aprons (LDA's).

Despite a lack of unequivocally volcanic characteristics, the localisation and rounded, lobate shape of these plains strongly support volcanic origins.

The flanks of Ascraeus Mons are covered with narrow, lobate lava flows and lava channels.

Broader and lobate leaves of some Alyogyne cultivars may have been hybridized with Alyogyne huegelii.

The last three segments of the trunk form a "tail" built by three pairs of thin, lobate blades directed upward and outward (see figure 3.20).

The inner region of the ejecta is characterized by a lobate appearance indicative of the flow of a liquid (or slushy) substance over the surface.

The latest episode of tectonic activity led to the formation of the lobate scarp, which actually runs tangentially to the ring of wrinkle ridges.

Some of these channels may be influenced by lahars, as indicated by their surface textures and ridged, lobate deposits at their margins and termini.

About 80% of the Venusian surface is covered by smooth, volcanic plains, consisting of 70% plains with wrinkle ridges and 10% smooth or lobate plains.

Lobate scarps are widely distributed over Mercury and consist of sinuous to arcuate scarps that transect preexisting plains and craters.

These lobate ridges appear to be of compressive tectonic origin and, although global in distribution, may be deflected locally by the presence of preexisting, basin-related structure.

Lobate scarps, seen extensively on planet Mercury, are in the form of undulating to arcuate scarps; wrinkle ridges are observed in the smooth plains materials.

The lobate scarps typically transect smooth plains materials (early Calorian age) on the floors of craters, but post-Caloris craters are superposed on them.

They are lobate with long spines protruding centrally; these spines are in some cases (e.g. Zhijinites) pillar-like, constituted of a bundle rods (originally aragonite?)

The complex comprises a lobate hectagonal colonnade portico enclosing a garden and the deconsacrated church of San Michele ai Sepolcri ("Saint Michael by the Sepulchers").

There is usually only one style with a lobed stigma.

The lobed leaves are generally found only at the base of the plant.

The lobed leaves are shiny dark green and maintain their small size.

The lobed oval leaves are 1 to 4 centimeters long.

Each is made up of 20 to 30 narrow leaflets with lobed edges.

The name of the species was derived from its distinctive lobed diaphragm.

Another piece from the same time is a lobed bowl of opaque turquoise glass.

The leaves are green and shiny with deep triangular lobed margins.

Each is white to cream in color with purple spotting on the lobed lips.

Leaves more deeply lobed than 'Ardis' with waist in middle.

The lobed leaves are located in a rosette around the base of the stem.

Some thought the red and yellow lobed types were beautiful, but we all agreed they had a rather bland taste.

The lobed leaves are up to 5 centimeters long and generally triangular in shape.

Lobed oval leaves under 2 centimeters long occur at the base of the plant.

A cliff face fell away before her, marked here and there by the lobed flow of landslides.

They have a distinctive three lobed lip and long spurs, similar to Aquilegia.

The cap is sticky when wet and has an irregularly lobed margin.

It has a diamond shaped blade at the end of a lobed, narrow claw.

The five petals are joined into a lobed, open corolla which is white with a red ring near the center.

There is a lobed tail at the hindwing tomus in some species.

Each leaf is divided into a few lobed or toothed leaflets.

The lobed leaves usually are 10-15 cm across.

Each funnel-shaped flower is about half a centimeter long and wide with a lobed face.

The leaves have rounded lobed blades borne on long petioles.

The three lobed leaves are purple and sticky when young and become bright green with age.