International Atlas of Clouds and of States of the Sky
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Moons Phases and Tides
Moon’s Phases and Tides Moon Phases Half of the Moon is always lit up by the sun. As the Moon orbits the Earth, we see different parts of the lighted area. From Earth, the lit portion we see of the moon waxes (grows) and wanes (shrinks). The revolution of the Moon around the Earth makes the Moon look as if it is changing shape in the sky The Moon passes through four major shapes during a cycle that repeats itself every 29.5 days. The phases always follow one another in the same order: New moon Waxing Crescent First quarter Waxing Gibbous Full moon Waning Gibbous Third (last) Quarter Waning Crescent • IF LIT FROM THE RIGHT, IT IS WAXING OR GROWING • IF DARKENING FROM THE RIGHT, IT IS WANING (SHRINKING) Tides • The Moon's gravitational pull on the Earth cause the seas and oceans to rise and fall in an endless cycle of low and high tides. • Much of the Earth's shoreline life depends on the tides. – Crabs, starfish, mussels, barnacles, etc. – Tides caused by the Moon • The Earth's tides are caused by the gravitational pull of the Moon. • The Earth bulges slightly both toward and away from the Moon. -As the Earth rotates daily, the bulges move across the Earth. • The moon pulls strongly on the water on the side of Earth closest to the moon, causing the water to bulge. • It also pulls less strongly on Earth and on the water on the far side of Earth, which results in tides. What causes tides? • Tides are the rise and fall of ocean water. -
Contrail-Cirrus and Their Potential for Regional Climate Change
Contrail-Cirrus and Their Potential for Regional Climate Change Kenneth Sassen Department of Meteorology, University of Utah, Salt Lake City, Utah ABSTRACT After reviewing the indirect evidence for the regional climatic impact of contrail-generated cirrus clouds (contrail- cirrus), the author presents a variety of new measurements indicating the nature and scope of the problem. The assess- ment concentrates on polarization lidar and radiometric observations of persisting contrails from Salt Lake City, Utah, where an extended Project First ISCCP (International Satellite Cloud Climatology Program) Regional Experiment (FIRE) cirrus cloud dataset from the Facility for Atmospheric Remote Sensing has captured new information in a geographical area previously identified as being affected by relatively heavy air traffic. The following contrail properties are consid- ered: hourly and monthly frequency of occurrence; height, temperature, and relative humidity statistics; visible and in- frared radiative impacts; and microphysical content evaluated from in situ data and contrail optical phenomenon such as halos and coronas. Also presented are high-resolution lidar images of contrails from the recent SUCCESS experiment, and the results of an initial attempt to numerically simulate the radiative effects of an observed contrail. The evidence indicates that the direct radiative effects of contrails display the potential for regional climate change at many midlati- tude locations, even though the sign of the climatic impact may be uncertain. However, new information suggests that the unusually small particles typical of many persisting contrails may favor the albedo cooling over the greenhouse warming effect, depending on such factors as the geographic distribution and patterns in day versus night aircraft usage. -
Light, Color, and Atmospheric Optics
Light, Color, and Atmospheric Optics GEOL 1350: Introduction To Meteorology 1 2 • During the scattering process, no energy is gained or lost, and therefore, no temperature changes occur. • Scattering depends on the size of objects, in particular on the ratio of object’s diameter vs wavelength: 1. Rayleigh scattering (D/ < 0.03) 2. Mie scattering (0.03 ≤ D/ < 32) 3. Geometric scattering (D/ ≥ 32) 3 4 • Gas scattering: redirection of radiation by a gas molecule without a net transfer of energy of the molecules • Rayleigh scattering: absorption extinction 4 coefficient s depends on 1/ . • Molecules scatter short (blue) wavelengths preferentially over long (red) wavelengths. • The longer pathway of light through the atmosphere the more shorter wavelengths are scattered. 5 • As sunlight enters the atmosphere, the shorter visible wavelengths of violet, blue and green are scattered more by atmospheric gases than are the longer wavelengths of yellow, orange, and especially red. • The scattered waves of violet, blue, and green strike the eye from all directions. • Because our eyes are more sensitive to blue light, these waves, viewed together, produce the sensation of blue coming from all around us. 6 • Rayleigh Scattering • The selective scattering of blue light by air molecules and very small particles can make distant mountains appear blue. The blue ridge mountains in Virginia. 7 • When small particles, such as fine dust and salt, become suspended in the atmosphere, the color of the sky begins to change from blue to milky white. • These particles are large enough to scatter all wavelengths of visible light fairly evenly in all directions. -
Äikesega) Kaasnevad Ohtlikud Ilmanähtused
TALLINNA TEHNIKAÜLIKOOL Eesti Mereakadeemia Merenduskeskus Veeteede lektoraat Raldo Täll RÜNKSAJUPILVEDEGA KAASNEVAD OHTLIKUD ILMANÄHTUSED LÄÄNEMEREL Lõputöö Juhendajad: Jüri Kamenik Lia Pahapill Tallinn 2016 SISUKORD SISUKORD ................................................................................................................................ 2 SÕNASTIK ................................................................................................................................ 4 SISSEJUHATUS ........................................................................................................................ 6 1. RÜNKSAJUPILVED JA ÄIKE ............................................................................................. 8 1.1. Äikese tekkimine ja areng ............................................................................................. 10 1.1.1. Äikese arengustaadiumid ........................................................................................ 11 1.2. Äikeste klassifikatsioon ................................................................................................. 14 1.2.1. Sünoptilise olukorra põhine liigitus ........................................................................ 14 1.2.2. Äikese seos tsüklonitega ......................................................................................... 15 1.2.3. Organiseerumispõhine liigitus ................................................................................ 16 2. RÜNKSAJUPILVEDEGA (ÄIKESEGA) KAASNEVAD OHTLIKUD ILMANÄHTUSED -
ESSENTIALS of METEOROLOGY (7Th Ed.) GLOSSARY
ESSENTIALS OF METEOROLOGY (7th ed.) GLOSSARY Chapter 1 Aerosols Tiny suspended solid particles (dust, smoke, etc.) or liquid droplets that enter the atmosphere from either natural or human (anthropogenic) sources, such as the burning of fossil fuels. Sulfur-containing fossil fuels, such as coal, produce sulfate aerosols. Air density The ratio of the mass of a substance to the volume occupied by it. Air density is usually expressed as g/cm3 or kg/m3. Also See Density. Air pressure The pressure exerted by the mass of air above a given point, usually expressed in millibars (mb), inches of (atmospheric mercury (Hg) or in hectopascals (hPa). pressure) Atmosphere The envelope of gases that surround a planet and are held to it by the planet's gravitational attraction. The earth's atmosphere is mainly nitrogen and oxygen. Carbon dioxide (CO2) A colorless, odorless gas whose concentration is about 0.039 percent (390 ppm) in a volume of air near sea level. It is a selective absorber of infrared radiation and, consequently, it is important in the earth's atmospheric greenhouse effect. Solid CO2 is called dry ice. Climate The accumulation of daily and seasonal weather events over a long period of time. Front The transition zone between two distinct air masses. Hurricane A tropical cyclone having winds in excess of 64 knots (74 mi/hr). Ionosphere An electrified region of the upper atmosphere where fairly large concentrations of ions and free electrons exist. Lapse rate The rate at which an atmospheric variable (usually temperature) decreases with height. (See Environmental lapse rate.) Mesosphere The atmospheric layer between the stratosphere and the thermosphere. -
Atmospheric Optics Learning Module
Atmospheric Optics Learning Module Everything we see is the reflection of light and without light, everything would be dark. In this learning module, we will discuss the various wavelengths of light and how it is transmitted through Earth’s atmosphere to explain fascinating optical phenomena including why the sky is blue and how rainbows form! To get started, watch this video describing energy in the form of waves. A sundog and halo display in Greenland. Electromagnetic Spectrum (0 – 6:30) Source Electromagnetic Spectrum Electromagnetic (EM) radiation is light. Light you might see in a rainbow, or better yet, a double rainbow such as the one seen in Figure 1. But it is also radio waves, x-rays, and gamma rays. It is incredibly important because there are only two ways we can move energy from place to place. The first is using what is called a particle, or an object moving from place to place. The second way to move energy is through a wave. The interesting thing about EM radiation is that it is both a particle and a wave 1. Figure 1. Double rainbow Source 1 Created by Tyra Brown, Nicole Riemer, Eric Snodgrass and Anna Ortiz at the University of Illinois at Urbana- This work is licensed under a Creative Commons Attribution-ShareAlike 4.0 International License. Champaign. 2015-2016. Supported by the National Science Foundation CAREER Grant #1254428. There are many frequencies of EM radiation that we cannot see. So if we change the frequency, we might have radio waves, which we cannot see, but they are all around us! The same goes for x-rays you might get if you break a bone. -
Direccion De Personal Aeronautico Dpto. De
DIRECCION DE PERSONAL AERONAUTICO 26/09/2021 MTC DPTO. DE INSTRUCCION OGMS/DINF PREGUNTAS Y OPCIONES POR TEMA 14:03 Pag: 1 TEMA: 0626 ATP-RTC - Meteorology and Weather Services - Chap.8 COD_PREG: PREGUNTA: RPTA: PREG20098166 What is indicated on the Weather Depiction Chart by a continuous smooth C (9299) line enclosing a hatched geographic area? OPCION A: The entire area has ceilings less than 1,000 feet and/or visibility less than 3 miles OPCION B: More than 50 percent of the area enclosed by the smooth line is predicted to have IFR conditions OPCION C: Reporting stations within the enclosed area are all showing IFR conditions at the time of the report OPCION D: PREG20098167 The horizontal wind shear, critical for turbulence (moderate or greater) per B (9701) 150 miles is OPCION A: 18 knots or less OPCION B: greater than 18 knots OPCION C: not a factor, only vertical shear is a factor OPCION D: PREG20098168 A severe thunderstorm is one in which he surface wind is A (9706) OPCION A: 50 knots or greater and/or surface hail is 3/4 inch or more in diameter. OPCION B: 55 knots or greater and/or surface hail is 1/2 inch or more in diameter. OPCION C: 45 knots or greater and/or surface hail is 1 inch or more in diameter. OPCION D: PREG20098169 A squall is a sudden increase of at least 16 knots in average wind speed to a B (9708) sustained speed of OPCION A: 24 knots or more for at least 1 minute OPCION B: 22 knots or more for at least 1 minute OPCION C: 20 knots or more for at least 1 minute OPCION D: PREG20098170 A calm wind that is forecast, in the international Terminal Aerodrome B (9709) Forecast (TAF) is encoded as OPCION A: VRB00KT OPCION B: 00000KT OPCION C: 00003KT OPCION D: PREG20098171 In the International Terminal Aerodrome Forecast (TAF), a variable wind C (9710) direction is noted by "VRB" where the three digit direction usually appears. -
Atmospheric Optics
53 Atmospheric Optics Craig F. Bohren Pennsylvania State University, Department of Meteorology, University Park, Pennsylvania, USA Phone: (814) 466-6264; Fax: (814) 865-3663; e-mail: [email protected] Abstract Colors of the sky and colored displays in the sky are mostly a consequence of selective scattering by molecules or particles, absorption usually being irrelevant. Molecular scattering selective by wavelength – incident sunlight of some wavelengths being scattered more than others – but the same in any direction at all wavelengths gives rise to the blue of the sky and the red of sunsets and sunrises. Scattering by particles selective by direction – different in different directions at a given wavelength – gives rise to rainbows, coronas, iridescent clouds, the glory, sun dogs, halos, and other ice-crystal displays. The size distribution of these particles and their shapes determine what is observed, water droplets and ice crystals, for example, resulting in distinct displays. To understand the variation and color and brightness of the sky as well as the brightness of clouds requires coming to grips with multiple scattering: scatterers in an ensemble are illuminated by incident sunlight and by the scattered light from each other. The optical properties of an ensemble are not necessarily those of its individual members. Mirages are a consequence of the spatial variation of coherent scattering (refraction) by air molecules, whereas the green flash owes its existence to both coherent scattering by molecules and incoherent scattering -
A Physically-Based Night Sky Model Henrik Wann Jensen1 Fredo´ Durand2 Michael M
To appear in the SIGGRAPH conference proceedings A Physically-Based Night Sky Model Henrik Wann Jensen1 Fredo´ Durand2 Michael M. Stark3 Simon Premozeˇ 3 Julie Dorsey2 Peter Shirley3 1Stanford University 2Massachusetts Institute of Technology 3University of Utah Abstract 1 Introduction This paper presents a physically-based model of the night sky for In this paper, we present a physically-based model of the night sky realistic image synthesis. We model both the direct appearance for image synthesis, and demonstrate it in the context of a Monte of the night sky and the illumination coming from the Moon, the Carlo ray tracer. Our model includes the appearance and illumi- stars, the zodiacal light, and the atmosphere. To accurately predict nation of all significant sources of natural light in the night sky, the appearance of night scenes we use physically-based astronomi- except for rare or unpredictable phenomena such as aurora, comets, cal data, both for position and radiometry. The Moon is simulated and novas. as a geometric model illuminated by the Sun, using recently mea- The ability to render accurately the appearance of and illumi- sured elevation and albedo maps, as well as a specialized BRDF. nation from the night sky has a wide range of existing and poten- For visible stars, we include the position, magnitude, and temper- tial applications, including film, planetarium shows, drive and flight ature of the star, while for the Milky Way and other nebulae we simulators, and games. In addition, the night sky as a natural phe- use a processed photograph. Zodiacal light due to scattering in the nomenon of substantial visual interest is worthy of study simply for dust covering the solar system, galactic light, and airglow due to its intrinsic beauty. -
Moon Journals
Moon Journals Does the moon always look the same? How does it change over time? Use Chabot’s moon journal to track and observe our moon. Can you figure out how it changes? Instructions Print the pages below and assemble your moon journal by folding it in half from top to bottom, then again from left to right. Or make your own moon journal! Be sure to include space for multiple days and observations. Example DIY journals are featured below. SUGGESTED MATERIALS Moon Journal Paper Pencil Markers, colored pencils, or crayons Observe the moon and sketch what you see for a whole week. Try to observe the moon at the same time each night if you can. Extension Pick one of the moons you observed. Can you write a story about the moon, or make an artistic interpretation of what you saw? Can you make a model or sketch to show how the Earth moves around the sun, while the moon moves around the Earth? Check out some of the videos below to learn more about the moon! Storybots “Time to Shine” https://www.youtube.com/watch?v=i235Y2HRksA For Grown Ups – What’s Going On? Our moon is a natural satellite. It’s locked into orbit around Earth by Earth’s gravity. As the moon orbits the Earth, the surface of the moon reflects light from the sun. The light from the sun illuminates the moon, allowing us to see it in the night sky. Sometimes, the Earth casts a shadow on parts of the moon. When this happens, the light from the sun cannot illuminate the entire moon, instead it only lights up a portion. -
Convection Questions.Cdr
Name: _________________________ Sketch the four stages of thunderstorm development in the boxes below. This is not an art project, but give it a decent effort. For each cloud sketch, include the arrows showing the direction of the air movement going on - both in the cloud and near the ground (include both updrafts and downdrafts). Illustrate any processes going on inside the cloud. Cumulus mediocris Cumulus congestus (prior to ice formation) Cumulonimbus calvus Cumulonimbus incus Questions: 1. In the morning, you see some cumulus humilus. A few hours later (around noon), you still see cumulus humilus, with a few cumulus mediocris here and there. Later that afternoon, you look again and the sky is still littered with cumulus humilus and mediocris. Although the clouds are clearly moving around and changing shape, they really don't look any different than they did this morning. What can you conclude from this observation? A. The air is mostly Stable / Unstable (pick one) B. Thunderstorms are Likely / Unlikely (pick one) 2. In the morning, you see some cumulus humilus. A few hours later (around noon) you see a lot of cumulus congestus and some cumulus castellanus. What can you conclude from this observations? A. The air is mostly Stable / Unstable (pick one) B. Thunderstorms are Likely / Unlikely (pick one) 3. You are watching the local news and the weather reporter says that "Unstable air is moving into New Mexico for the next few days." What kind of weather do you expect in the next few days? A. Clear skies. B. Maybe some scattered cumulus but nothing else. -
Regional Codes and National Coding Practices, Volume II
Manual on Codes Regional Codes and National Coding Practices Volume II 2011 edition Updated in 2018 WEATHER CLIMATE WATER CLIMATE WEATHER WMO-No. 306 Manual on Codes Regional Codes and National Coding Practices Volume II 2011 edition Updated in 2018 WEATHER CLIMATE WATER CLIMATE WEATHER WMO-No. 306 WMO-No. 306 © World Meteorological Organization, 2011 The right of publication in print, electronic and any other form and in any language is reserved by WMO. Short extracts from WMO publications may be reproduced without authorization, provided that the complete source is clearly indicated. Editorial correspondence and requests to publish, reproduce or translate this publication in part or in whole should be addressed to: Chair, Publications Board World Meteorological Organization (WMO) 7 bis, avenue de la Paix Tel.: +41 (0) 22 730 84 03 P.O. Box 2300 Fax: +41 (0) 22 730 81 17 CH-1211 Geneva 2, Switzerland Email: [email protected] ISBN 978-92-63-10306-2 NOTE The designations employed in WMO publications and the presentation of material in this publication do not imply the expression of any opinion whatsoever on the part of the WMO concerning the legal status of any country, territory, city or area, or of its authorities, or concerning the delimitation of its frontiers or boundaries. The mention of specific companies or products does not imply that they are endorsed or recommended by WMO in preference to others of a similar nature which are not mentioned or advertised. PUBLICATION REVISION TRACK RECORD Purpose of Date Part/chapter/section