Mateorology

Meterology

Meteorology is the intrigrated scientific study of the atmosphere. Studies in the field draw out back millennia, though significant progress in meteorology did not take place until the 18th century. The 19th century saw humble evolution in the field after observing networks formation across several countries. It wasn't until after the development of the computer in the latter part of the 20th century that noteworthy breakthrough in weather forecasting was achieve

 materology phenominon 

Meteorological phenomenon are noticeable weather events that enlighten and are explained by the science of meteorology. Those measures are bound by the variables of Earth's atmosphere: warmth air heaviness, water vapor, and the gradients and interactions of each variable, and how they change over time. diverse spatial balance are intentional to establish how systems on confined, regional, and global levels impact weather conditions and climatology.

Meteorology, climatology, atmospheric physics, and atmospheric chemistry are sub-branches  of the atmospheric sciences. Meteorology and hydrology make up the interdisciplinary meadow of hydrometeorologyrelations between Earth's atmosphere and the ocean are part of coupled ocean-atmosphere studies. Meteorology has submission in many miscellaneous fields such as the military, energy sector production, transfer, agriculture and construction.

 origin of materology

The word "meteorology" is from Greek μετέωρος metéōros "lofty; high (in the sky)" (from μετα- meta- "beyond/above" and ἀείρω aeiro "I lift up") and -λογία -logia "-(o)logy", i.e. " which means the study of things in the air".

Ptolemy was written on the atmospheric refraction of light in the circumstance of astronomical explanation In 1021, Alhazen descrived  that atmospheric refraction is also accountable for twilight; he has  estimated that twilight begins when the sun is 19 degrees below the horizon and also worn a geometric determination on the basis of this to estimate the utmost possible height of the earth's atmosphere about 49 miles/ or 79 km

 

St. Albert the Great was the first to recommend that each drop of falling rain had the form of a small bubble, and that this form meant that the rainbow was created by light interacting with each raindrop. Roger Bacon was the first eho calculate the raw-boned size of the rainbow. He affirmed that the rainbow summit can not appear higher than 42 degrees above the horizon. In the late 13th century and early of 14th century, Kamāl al-Dīn al-Fārisī and Theodoric of Freiberg were the first who give the correct explanations for the prime rainbow phenomenon. Theoderic went further and also explained the minor rainbow. In 1716, Edmund Halley recommended that aurorae are caused by "magnetic effluvia" poignant along the Earth's magnetic field line