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NaturalOccurences
Morning Glory Cloudsrare meteorological
phenomenon observed in Northern Australia's Gulf of Carpentaria
can be up to 1,000 kilometres long, 1 to 2 kilometres high
When Do These Morning Clouds Form?Morning Glory is likely to occur when the humidity in the area is high, which provides moisture for the cloud to form, and when strong sea breezes have blown the preceding day.
1942No rainfall
Roll Clouds
Gravity HillLocated in Leh, Ladakh
The layout of the area and surrounding slopes create an optical illusion that the downhill road is actually an uphill road. Objects and cars on the hill may appear to roll "uphill" in defiance of gravity when they are, in fact, rolling downhill.
Tianzi Mountains
Located in the Hunan Province of China
named after the farmer Xiang Dakun
led a successful local farmers' revolt and called himself "tianzi"
This means "son of Heaven"
deemed sacred by many Sulamitos who used to inhabit the outer regions of Hunan
The Tianzi Mountains were formed from quartz sandstone of 400 million years ago through the intermittent rising of the crust for 2 million years.
Largest Salt Flat
Natural Formation
Located in Potosi, Bolivia
Formation42000 years ago-Lake Minchin
Lake Tauca
Lake CoipasaPoopo Lake and Uru Uru Lake
Salt Deserts- Salar de Coipasa & Salar de Uyuni
Salar de Uyuni viewed from space, with Salar de Coipasa in the top left corner
During the wet season, Titicaca overflows and discharges into Poopó, which, in turn, floods Salar De Coipasa and Salar de Uyuni.
Green Lake
Styria, Austria
Surrounded by Hochschwab Mountains
So this looks like a normal park……..
Going…..
Going……
SPRING TIME
Gone
During WINTER:
1m-2m(3ft-7ft) deep.
Surrounding area used as a county park.
During SPRING-SUMMER:
12m(39ft) deep
Begins to recede in July
So What Causes This Transformation?
Auroras
natural light display in the sky
Arctic and Antartic regions
Polar LightsRoman goddess of dawn
Aurora Borealis
Aurora Australis
Aurora BorealisNORTH POLE
SOUTH POLE Aurora Australis
What Causes Auroras?Auroras are produced when the
magnetosphere is sufficiently disturbed by the solar wind that the trajectories of
charged particles in both solar wind and magnetospheric plasma, mainly in the form of electrons and protons, precipitate them into the upper atmosphere (thermosphere/exosphere), where their energy is lost. The
resulting ionization and excitation of atmospheric constituents emits light of
varying colour and complexity.
RedGreenBlueUltraviolet
InfraredYellow
Pink