ASKiIMAN™ ARCHIVE / PHYSICAL GEOGRAPHY
--:--:-- · -- --- ----
AEOLIAN DEPOSITIONAL DUNES (NCERT FIG 7.16) WIND DIRECTION →
1. BARCHAN
→
HORNS POINT
DOWNWIND →
2. PARABOLIC
→
REVERSE BARCHAN
← HORNS UPWIND
3. SEIF / LONG.
1-WINGED SEIF &
PARALLEL RIDGES
TRANSVERSE (⊥ WIND · RICH SAND) LOESS SILT & THAR DHRIAN
WORLD G TO K · GEOMORPHIC AGENTS & LANDFORMS · NODE 52 OF 106

Aeolian Depositional Landforms

Stoss vs. Slip-Face Physics · Barchans, Parabolic & Seif Dunes · Longitudinal vs. Transverse · Loess & Thar Dhrian (28 Micro-Realms)

The Five NCERT Sand Dune Geometries & Loess Blankets (NCERT Chapter 7)

Wind is a supreme sorting agent. While fine dust travels high in suspension to blanket distant regions as Loess, saltating sand grains accumulate behind obstacles to form Sand Dunes with a gentle windward slope and a $34^\circ$ leeward slip-face. Depending on wind constancy, sand supply, and vegetation, NCERT Figure 7.16 classifies five primary dune forms: 1) crescentic Barchans (wings point downwind), 2) vegetation-pinned Parabolic Dunes (reversed barchans), 3) one-winged Seifs, 4) parallel Longitudinal Dunes (poor sand supply), and 5) perpendicular Transverse Dunes (abundant sand supply).

1. BARCHAN (HORNS DOWNWIND →) ↔ 2. PARABOLIC (← HORNS UPWIND · VEGETATION) → 3. SEIF (SINGLE WING) & 4. LONGITUDINAL (POOR SAND) → 5. TRANSVERSE (⊥ WIND · RICH SAND) → 6. LOESS & THAR DHRIAN

I. Dune Aerodynamics, Stoss vs. Slip-Face Physics & Migration (NCERT)

MICRO-REALM 01

Obstacle Prerequisite

  • Dry hot deserts are good for sand dunes
  • Obstacles to initiate dune formation
  • Are equally important (NCERT first rule)
MICRO-REALM 02

Stoss vs. Leeward Slip-Face

  • Windward (Stoss) slope: Gentle ($10^\circ\text{–}15^\circ$)
  • Sand saltates up windward ramp to crest
  • Leeward (Slip-face): Steep ($32^\circ\text{–}34^\circ$)
MICRO-REALM 03

34° Angle of Repose

34° MAX
AVALANCHE
  • Maximum stable slope of dry loose sand
  • When crest oversteepens beyond $34^\circ$
  • Sand avalanches down the slip-face
MICRO-REALM 04

Dune Migration & Cross-Beds

  • Erosion on stoss + deposition on lee
  • Dune marches downwind (up to 30 m/yr)
  • Preserves inclined Foreset Cross-bedding
MICRO-REALM 05

Aeolian Sand Ripples

  • Smallest aeolian bedform (cm-scale)
  • Wavelength matches mean saltation hop
  • Coarsest grains concentrate at ripple crests
MICRO-REALM 06

Nebkhas (Coppice Dunes)

  • Embryonic sand mound trapped around
  • Desert scrub bushes (Calligonum/Capparis)
  • Streamlined wind-shadow sand tongue
MICRO-REALM 07

Draa (Mega-Dunes) & Gassi

GASSI
  • Draa: Colossal compound erg ridges (100–400 m)
  • Gassi: Rocky sand-free interdune corridor
  • Used as caravan highways across Sahara

II. Barchans, Parabolic Dunes & Seifs (NCERT Fig 7.16 Core)

MICRO-REALM 08

1. Barchans (Crescentic)

WIND →
  • Crescent-shaped dunes (NCERT Fig 7.16a)
  • Points or wings directed AWAY from wind
  • i.e., Horns point DOWNWIND!
MICRO-REALM 09

Barchan Conditions (NCERT)

1. CONSTANT WIND DIRECTION2. MODERATE SAND + UNIFORM FLOOR
  • Form where wind direction is constant
  • And moderate throughout the year
  • Over uniform surfaces with limited sand
MICRO-REALM 10

Barchanoid Ridges

  • As sand supply increases, barchans crowd
  • Lateral horns fuse into wavy scalloped rows
  • Transitional stage to Transverse dunes
MICRO-REALM 11

2. Parabolic Dunes (NCERT)

WIND →
  • Form when sandy surfaces are partially
  • Covered with vegetation (NCERT Fig 7.16b)
  • Parabolic dunes are REVERSED BARCHANS!
MICRO-REALM 12

Barchan vs. Parabolic

BAR
vs
PAR
  • Both have the SAME wind direction
  • Barchan: Center lags, horns race downwind
  • Parabolic: Vegetation pins horns upwind!
MICRO-REALM 13

Hairpin Blowout Dunes

  • Central blowout nose advances far downwind
  • Leaves long parallel vegetated arms
  • Characteristic of semi-arid Thar margins
MICRO-REALM 14

3. Seif Dunes (One-Winged)

  • Arabic "Saif" = Curved Sword
  • Similar to barchan with a small difference:
  • Seif has ONLY ONE WING or point (NCERT)!

III. Longitudinal, Transverse & Star Dunes (NCERT Fig 7.16 Core)

MICRO-REALM 15

Seif Scale & Wind Shift

SHIFT IN WIND CONDITIONS →100 M HIGH × 100 KM LONG
  • Occurs when there is a shift in wind
  • Lone wing of seif grows very long & high
  • Reaches 100 m height & 100 km length
MICRO-REALM 16

4. Longitudinal Dunes

  • Long ridges of considerable length
  • But low in height; PARALLEL to wind
  • Supply of sand is POOR & wind is constant!
MICRO-REALM 17

5. Transverse Dunes

  • Aligned PERPENDICULAR ($90^\circ$) to wind
  • Form when wind direction is constant
  • And source of sand is ABUNDANT (NCERT)!
MICRO-REALM 18

Longitudinal vs. Transverse

LONGITUDINAL:
∥ · POOR SAND
TRANSVERSE:
⊥ · RICH SAND
  • #1 UPSC Prelims comparative trap
  • Longitudinal: Parallel + Poor sand supply
  • Transverse: Perpendicular + Abundant sand
MICRO-REALM 19

Star Dunes (Rhourds)

  • Multi-directional seasonal wind regime
  • 3 or more radiating arms from central peak
  • Remain stationary & grow 300+ m tall
MICRO-REALM 20

Sand Sheets & Whalebacks

  • Flat to gently undulating sand plains
  • Zibar: Coarse bimodal sand without slip-faces
  • Selima Sand Sheet (Eastern Sahara)
MICRO-REALM 21

Echo, Climbing & Falling Dunes

  • Topographically anchored obstacle dunes
  • Echo/Climbing dune on windward cliff face
  • Falling dune cascades down leeward scarp

IV. Loess Silt Blankets & Indian Thar Desert Depositional Landforms

MICRO-REALM 22

Loess (Wind-Blown Silt)

UNSTRATIFIED · POROUSCALCAREOUS YELLOW SILT
  • Fine dust ($0.02\text{–}0.05\text{ mm}$) carried in suspension
  • Deposited outside desert margins
  • Homogeneous, unstratified, friable & fertile
MICRO-REALM 23

Desert vs. Glacial Loess

DESERT LOESS:
GOBI → CHINA
GLACIAL LOESS:
OUTWASH SILT
  • 1) Desert source: Gobi deflation $\to$ N. China
  • 2) Glacial source: Outwash rock-flour silt
  • Blown across North America & Europe
MICRO-REALM 24

Global Loess Provinces

  • Loess Plateau (China): 100–300 m thick; Yellow River (Hwang Ho)
  • Vertical cleavage enables Yaodong cave homes
  • Ukraine Chernozem & Argentine Pampas
MICRO-REALM 25

Thar "Dhrian" & "Dhoros"

DHRIAN (SHIFTING DUNES)
& DHORO DEPRESSIONS
  • Dhrian: Shifting sand dunes in Marusthali
  • Dhoro: Long trough between longitudinal dunes
  • Sam, Khuri (Jaisalmer) & Churu barchans
MICRO-REALM 26

Thar Parabolic Dominance

PARABOLIC DUNES = #1MOST WIDESPREAD IN THAR
  • Because Thar is a vegetated semi-arid desert
  • Anchored Parabolic & coalesced raked dunes
  • Cover the largest area in Western Rajasthan!
MICRO-REALM 27

Bhur, Karewa Loess & Miliolite

BHURKAREWAMILIOLITE
  • Bhur: Wind-blown sand ridges in Upper Ganga-Ramganga plain
  • Kashmir Karewas & Son-Belan loess caps
  • Saurashtra Miliolite: Aeolianite limestone
MICRO-REALM 28

Master NCERT Fig 7.16 Key

BARCHANPARABOLICSEIFLONGITUD.TRANSV.LOESS
  • Completes Aeolian Landforms triad (50–52)
  • All 5 NCERT Fig 7.16 dune types mastered
  • Transitions to Realm 53 (Glaciers)

Core Distinctions

1. Barchan vs. Parabolic vs. Seif Dunes (NCERT Figure 7.16 Exact Rules)

• Barchans: Crescent-shaped dunes with two wings/horns directed downwind (away from wind); form on bare uniform surfaces with constant wind.
• Parabolic Dunes: Form when sandy surfaces are partially covered with vegetation; they are reversed barchans (horns anchored upwind, convex nose pointing downwind) with the same wind direction.
• Seif Dunes: Similar to barchans except a Seif has only ONE wing or point, created when there is a shift in wind conditions.

2. Longitudinal vs. Transverse Dunes (Sand Supply Contrast — NCERT)

• Longitudinal Dunes: Long ridges of low height aligned parallel to wind; form when wind is constant and supply of sand is POOR.
• Transverse Dunes: Long wavy ridges aligned perpendicular to wind; form when wind is constant and the source of sand is ABUNDANT.

3. Sand Dunes (Saltation) vs. Loess (Suspension)

Sand Dunes are stratified, cross-bedded mounds of medium quartz sand ($0.1\text{–}0.5\text{ mm}$) moved locally by saltation. Loess is an unstratified, porous, calcareous blanket of fine yellow silt ($<0.05\text{ mm}$) carried hundreds of kilometres in suspension.

NCERT Fig 7.16 Dune Matrix

Orientation, Wings & Sand Supply Key

1. BARCHAN2 Wings Downwind (→) · Bare
2. PARABOLIC2 Wings Upwind (←) · Flora
3. SEIF DUNE1 Wing Only · Wind Shift
4. LONGITUDINALParallel (∥) · POOR Sand
5. TRANSVERSEPerpendicular (⊥) · RICH Sand