Air Masses and Frontal Zones
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Link Between the Double-Intertropical Convergence Zone Problem and Cloud Biases Over the Southern Ocean
Link between the double-Intertropical Convergence Zone problem and cloud biases over the Southern Ocean Yen-Ting Hwang1 and Dargan M. W. Frierson Department of Atmospheric Sciences, University of Washington, Seattle, WA 98195-1640 Edited by Mark H. Thiemens, University of California at San Diego, La Jolla, CA, and approved February 15, 2013 (received for review August 2, 2012) The double-Intertropical Convergence Zone (ITCZ) problem, in which climate models show that the bias can be reduced by changing excessive precipitation is produced in the Southern Hemisphere aspects of the convection scheme (e.g., refs. 7–9) or changing the tropics, which resembles a Southern Hemisphere counterpart to the surface wind stress formulation (e.g., ref. 10). Given the complex strong Northern Hemisphere ITCZ, is perhaps the most significant feedback processes in the tropics, it is challenging to understand and most persistent bias of global climate models. In this study, we the mechanisms by which the sensitivity experiments listed above look to the extratropics for possible causes of the double-ITCZ improve tropical precipitation. problem by performing a global energetic analysis with historical Recent work in general circulation theory has suggested that simulations from a suite of global climate models and comparing one should not only look within the tropics for features that affect with satellite observations of the Earth’s energy budget. Our results tropical precipitation. A set of idealized experiments showed that show that models with more energy flux into the Southern heating a global climate model exclusively in the extratropics can Hemisphere atmosphere (at the top of the atmosphere and at the lead to tropical rainfall shifts from one side of the tropics to the surface) tend to have a stronger double-ITCZ bias, consistent with other (11). -
Tropical Weather Discussion
TROPICAL WEATHER DISCUSSION • Purpose The Tropical Weather Discussion describes major synoptic weather features and significant areas of disturbed weather in the tropics. The product is intended to provide current weather information for those who need to know the current state of the atmosphere and expected trends to assist them in their decision making. The product gives significant weather features, areas of disturbed weather, expected trends, the meteorological reasoning behind the forecast, model performance, and in some cases a degree of confidence. • Content The Tropical Weather Discussion is a narrative explaining the current weather conditions across the tropics and the expected short-term changes. The product is divided into four different sections as outline below: 1. SPECIAL FEATURES (event-driven) The special features section includes descriptions of hurricanes, tropical storms, tropical depressions, subtropical cyclones, and any other feature of significance that may develop into a tropical or subtropical cyclone. For active tropical cyclones, this section provides the latest advisory data on the system. Associated middle and upper level interactions as well as significant clouds and convection are discussed with each system. This section is omitted if none of these features is present. 2. TROPICAL WAVES (event-driven) This section provides a description of the strength, position, and movement of all tropical waves analyzed on the surface analysis, from east to west. A brief reason for a wave’s position is usually given, citing surface observations, upper air time sections, satellite imagery, etc. The associated convection is discussed with each tropical wave as well as any potential impacts to landmasses or marine interests. -
The Effects of the Atmosphere and Weather on Radio Astronomy Observations
The Effects of the Atmosphere and Weather on Radio Astronomy Observations Ronald J Maddalena July 2011 The Influence of the Atmosphere and Weather at cm- and mm-wavelengths Opacity Cloud Cover Calibration Continuum performance System performance – Tsys Calibration Observing techniques Winds Hardware design Pointing Refraction Safety Pointing Telescope Scheduling Air Mass Proportion of proposals Calibration that should be accepted Interferometer & VLB phase Telescope productivity errors Aperture phase errors Structure of the Lower Atmosphere Refraction Refraction Index of Refraction is weather dependent: .3 73×105 ⋅ P (mBar) 6 77 6. ⋅ PTotal (mBar) H 2O (n0 − )1 ⋅10 ≈ + +... T(C) + 273.15 ()T(C) + 273.15 2 P (mBar) ≈ 6.112⋅ea H 2O .7 62⋅TDewPt (C) where a ≈ 243.12 +TDewPt (C) Froome & Essen, 1969 http://cires.colorado.edu/~voemel/vp.html Guide to Meteorological Instruments and Methods of Observation (CIMO Guide) (WMO, 2008) Refraction For plane-parallel approximation: n0 • Cos(Elev Obs )=Cos(Elev True ) R = Elev Obs – Elev True = (n 0-1) • Cot(Elev Obs ) Good to above 30 ° only For spherical Earth: n 0 dn() h Elev− Elev = a ⋅ n ⋅cos( Elev ) ⋅ Obs True0 Obs 2 2 2 2 2 ∫1 nh()(⋅ ah + )() ⋅ nh − an ⋅0 ⋅ cos( Elev Obs ) a = Earth radius; h = distance above sea level of atmospheric layer, n(h) = index of refraction at height h; n 0 = ground-level index of refraction See, for example, Smart, “Spherical Astronomy” Refraction Important for good pointing when combining: large aperture telescopes at high frequencies at low elevations (i.e., the GBT) Every observatory handles refraction differently. Offset pointing helps eliminates refraction errors Since n(h) isn’t usually known, most (all?) observatories use some simplifying model. -
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. -
Air Mass Effect on the Performance of Organic Solar Cells
Available online at www.sciencedirect.com ScienceDirect Energy Procedia 36 ( 2013 ) 714 – 721 TerraGreen 13 International Conference 2013 - Advancements in Renewable Energy and Clean Environment Air mass effect on the performance of organic solar cells A. Guechi1*, M. Chegaar2 and M. Aillerie3,4, # 1Institute of Optics and Precision Mechanics, Ferhat Abbas University, 19000, Setif, Algeria 2L.O.C, Department of Physics, Faculty of Sciences, Ferhat Abbas University, 19000, Setif, Algeria Email : [email protected], [email protected] 3Lorraine University, LMOPS-EA 4423, 57070 Metz, France 4Supelec, LMOPS, 57070 Metz, France #Email: [email protected] Abstract The objective of this study is to evaluate the effect of variations in global and diffuse solar spectral distribution due to the variation of air mass on the performance of two types of solar cells, DPB (etraphenyl–dibenzo–periflanthene) and CuPc (Copper-Phthalocyanine) using the spectral irradiance model for clear skies, SMARTS2, over typical rural environment in Setif. Air mass can reduce the sunlight reaching a solar cell and thereby cause a reduction in the electrical current, fill factor, open circuit voltage and efficiency. The results indicate that this atmospheric parameter causes different effects on the electrical current produced by DPB and CuPc solar cells. In addition, air mass reduces the current of the DPB and CuPc cells by 82.34% and 83.07 % respectively under global radiation. However these reductions are 37.85 % and 38.06%, for DPB and CuPc cells respectively under diffuse solar radiation. The efficiency decreases with increasing air mass for both DPB and CuPc solar cells. © 20132013 The The Authors. -
Nighttime Photochemical Model and Night Airglow on Venus
Planetary and Space Science 85 (2013) 78–88 Contents lists available at ScienceDirect Planetary and Space Science journal homepage: www.elsevier.com/locate/pss Nighttime photochemical model and night airglow on Venus Vladimir A. Krasnopolsky n a Department of Physics, Catholic University of America, Washington, DC 20064, USA b Moscow Institute of Physics and Technology, Dolgoprudnyy 141700 Russia article info abstract Article history: The photochemical model for the Venus nighttime atmosphere and night airglow (Krasnopolsky, 2010, Received 23 December 2012 Icarus 207, 17–27) has been revised to account for the SPICAV detection of the nighttime ozone layer and Received in revised form more detailed spectroscopy and morphology of the OH nightglow. Nighttime chemistry on Venus is 28 April 2013 induced by fluxes of O, N, H, and Cl with mean hemispheric values of 3 Â 1012,1.2Â 109,1010, and Accepted 31 May 2013 − − 1010 cm 2 s 1, respectively. These fluxes are proportional to column abundances of these species in the Available online 18 June 2013 daytime atmosphere above 90 km, and this favors their validity. The model includes 86 reactions of 29 Keywords: species. The calculated abundances of Cl2, ClO, and ClNO3 exceed a ppb level at 80–90 km, and Venus perspectives of their detection are briefly discussed. Properties of the ozone layer in the model agree Photochemistry with those observed by SPICAV. An alternative model without the flux of Cl agrees with the observed O Night airglow 3 peak altitude and density but predicts an increase of ozone to 4 Â 108 cm−3 at 80 km. -
ESCI 344 – Tropical Meteorology Lesson 3 – General Circulation of the Tropics
ESCI 344 – Tropical Meteorology Lesson 3 – General Circulation of the Tropics References: Forecaster’s Guide to Tropical Meteorology (updated), Ramage Climate Dynamics of the Tropics, Hastenrath Tropical Climatology (2nd ed), McGregor and Nieuwolt Tropical Meteorology, Tarakanov Climate and Weather in the Tropics, Riehl General Circulation of the Tropical Atmosphere, Vol II, Newell et al. “The South Pacific Convergence Zone (SPCZ): A Review”, Vincent, Mon.Wea. Rev., 122, 1949-1970, 1994 “The Central Pacific Near-Equatorial Convergence Zone”, Ramage, J. Geophys. Res., 86, 6580-6598 Reading: Introduction to the Meteorology and Climate of the Tropics, Chapter 3 Vincent, “The SPCZ: A Review” Lau and Yang, “Walker Circulation” James, “Hadley Circulation” Waliser, “Intertropical Convergence Zones” Hastenrath, “Tropical Climates” Madden, “Intraseasonal Oscillation (MJO)” TERMINOLOGY Boreal refers to the Northern Hemisphere Austral refers to the Southern Hemisphere LATITUDINAL HEAT IMBALANCE Net radiation flux is defined as the difference in incoming radiation flux and outgoing radiation flux. A positive net radiation flux indicates a surplus of energy, while a negative net radiation flux indicates a deficit. This figure shows the longitudinally-averaged, annual-mean radiation fluxes at the top of the atmosphere. Outgoing shortwave is due to scattering and reflection. Net shortwave is the difference between the incoming and outgoing shortwave radiation. When the earth-atmosphere system is considered as a whole, there is a positive net radiation flux between about 40N and 40S, while there is a negative net radiation flux poleward of 40 in both hemispheres. In order for a steady-state temperature to be achieved, there must be transport of heat from the earth’s surface to the atmosphere, and from the tropics to the polar regions. -
Synoptic Meteorology
Lecture Notes on Synoptic Meteorology For Integrated Meteorological Training Course By Dr. Prakash Khare Scientist E India Meteorological Department Meteorological Training Institute Pashan,Pune-8 186 IMTC SYLLABUS OF SYNOPTIC METEOROLOGY (FOR DIRECT RECRUITED S.A’S OF IMD) Theory (25 Periods) ❖ Scales of weather systems; Network of Observatories; Surface, upper air; special observations (satellite, radar, aircraft etc.); analysis of fields of meteorological elements on synoptic charts; Vertical time / cross sections and their analysis. ❖ Wind and pressure analysis: Isobars on level surface and contours on constant pressure surface. Isotherms, thickness field; examples of geostrophic, gradient and thermal winds: slope of pressure system, streamline and Isotachs analysis. ❖ Western disturbance and its structure and associated weather, Waves in mid-latitude westerlies. ❖ Thunderstorm and severe local storm, synoptic conditions favourable for thunderstorm, concepts of triggering mechanism, conditional instability; Norwesters, dust storm, hail storm. Squall, tornado, microburst/cloudburst, landslide. ❖ Indian summer monsoon; S.W. Monsoon onset: semi permanent systems, Active and break monsoon, Monsoon depressions: MTC; Offshore troughs/vortices. Influence of extra tropical troughs and typhoons in northwest Pacific; withdrawal of S.W. Monsoon, Northeast monsoon, ❖ Tropical Cyclone: Life cycle, vertical and horizontal structure of TC, Its movement and intensification. Weather associated with TC. Easterly wave and its structure and associated weather. ❖ Jet Streams – WMO definition of Jet stream, different jet streams around the globe, Jet streams and weather ❖ Meso-scale meteorology, sea and land breezes, mountain/valley winds, mountain wave. ❖ Short range weather forecasting (Elementary ideas only); persistence, climatology and steering methods, movement and development of synoptic scale systems; Analogue techniques- prediction of individual weather elements, visibility, surface and upper level winds, convective phenomena. -
BASIC WEATHER CONCEPTS CHAPTER TWO WIND, PRESSURE • Be Familiar with Global Wind Patterns
LLI BASIC WEATHER CONCEPTS CHAPTER TWO WIND, PRESSURE • Be familiar with global wind patterns. • Understand barometric pressure. • Know the factors that affect the wind. • Predict the circulation of winds around highs and lows. • Determine the direction to a low. • Understand winds aloft and how they differ from surface winds. 1 EquatorPole Air Flow warm equatorial air rises, then moves to cooler mid-latitude regions then sinks 2 Mid-latitude High note each higher latitude region is colder until Pole is reached 3 What is a Hadley Cell? The Hadley cell, named after George Hadley, is a global scale tropical atmospheric circulation that features air rising near the equator, flowing poleward at 10–15 kilometers above the surface, descending in the subtropics, and then returning equatorward near the surface. This process maintains the Global Energy Balance preventing the equator from becoming hotter and polar regions becoming colder. 4 Global Highs and Lows 5 Global Winds 6 Video of Atmospheric Circulation • Global Atmospheric Circulation 1:54 mins. • https://www.youtube.com/watch?v=DHrapzH PCSA 7 European Explorers used Tradewinds St. Augustine >30˚ N > 30˚ S 9 Land Masses Modify Global Pattern 10 Key Points to Remember about Heat and Pressure • Heat: energy (heat) is always transferred from WARM to COLD • Pressure: pressure always flows from HIGH to LOW 11 Pressure Differences – HIGH pressure areas – like Hills – LOW pressure areas – like valleys Earth’s rotation causes winds to turn rather than travel straight from high to low 12 Winds around Highs and Lows highs-clockwise, lows counterclockwise 13 Movement of Air in Low Pressure and High Pressure Regions • Air molecules* move counterclockwise (in the Northern Hemisphere) and rise in a low pressure area. -
The Intertropical Convergence Zone of the Eastern Pacific Region (I)*
The Intertropical Convergence Zone of the Eastern Pacific Region (I)* MAJOR LEO ALPERT, A.C. Hq. AAF Weather Service, Asheville, N. C. INTRODUCTION Recently a large number of weather ob- servations have become available from air- ITTLE INFORMATION concerning the craft patrols in the Eastern Pacific Ocean structure and position of the inter- L between 90°W to 95°W Longitude, and 7°S tropical convergence zone in the East- to 14°N Latitude. From December 1941 to ern Pacific Ocean was available prior to the late 1944, hourly weather observations were war. As daily weather reports from ships made daily by patrol aircraft, flying between have never been numerous from this area, the Republic of Guatemala in Central Amer- all attempts to show the position of the ica, the Galapagos Archipelago and the main- intertropical convergence zone based upon land of Ecuador in South America. Data an interpretation of summarized ship re- for the period February 1942 to January ports are open to question. The charts pub- 1944 have been plotted on daily charts and lished in the " Atlas of Climatic Charts of analyzed by the author. the Oceans'n are probably the best of these The grand total of observations available for this region. They are based upon fre- from the aircraft patrols in the area from quencies of true-wind directions determined 10°N to 5°S for the period February 1942 by observing the effect of wind on the sea to January 1944, inclusive, is two to four surface from a moving ship at Greenwich times as great as the grand total of observa- Noon during the period 1885-1933. -
Two Phases of the Holocene East African Humid Period: Inferred From
Earth and Planetary Science Letters 460 (2017) 123–134 Contents lists available at ScienceDirect Earth and Planetary Science Letters www.elsevier.com/locate/epsl Two phases of the Holocene East African Humid Period: Inferred from a high-resolution geochemical record off Tanzania ∗ Xiting Liu a,b, , Rebecca Rendle-Bühring b, Holger Kuhlmann b, Anchun Li a a Key Laboratory of Marine Geology and Environment, Institute of Oceanology, Chinese Academy of Sciences, Qingdao 266071, China b MARUM – Center for Marine Environmental Sciences and Faculty of Geosciences, University of Bremen, D-28359 Bremen, Germany a r t i c l e i n f o a b s t r a c t Article history: During the Holocene, the most notably climatic change across the African continent is the African Received 10 August 2016 Humid Period (AHP), however the pace and primary forcing for this pluvial condition is still ambiguous, Received in revised form 2 December 2016 particularly in East Africa. We present a high-resolution marine sediment record off Tanzania to provide Accepted 11 December 2016 insights into the climatic conditions of inland East Africa during the Holocene. Major element ratios Available online xxxx (i.e., log-ratios of Fe/Ca and Ti/Ca), derived from X-Ray Fluorescence scanning, have been employed to Editor: M. Frank document variations in humidity in East Africa. Our results show that the AHP is represented by two Keywords: humid phases: an intense humid period from the beginning of the Holocene to 8ka (AHP I); and a African Humid Period moderate humid period spanning from 8 to 5.5 ka (AHP II). -
How Does Intertropical Convergence Zone Variation Impact on Tropical Cyclone in the Northern Hemisphere?
Geophysical Research Abstracts Vol. 19, EGU2017-16196, 2017 EGU General Assembly 2017 © Author(s) 2017. CC Attribution 3.0 License. How Does Intertropical Convergence Zone Variation Impact on Tropical Cyclone in the Northern Hemisphere? Liping Ma (1,2) and Richard Williams (2) (1) Chinese Academy of Meteorological Sciences, Beijing, China, (2) University of Liverpool, Department of Earth, Ocean & Ecological Sciences, School of Environmental Sciences, Liverpool, UK Enhanced sea surface temperature is expected to be favourable for more tropical cyclone formation. However, a surprising result emerges from the analysis of the frequency of tropical cyclones in the global tropical oceans in the northern hemisphere. The frequency of tropical cyclones positively correlates with a strengthening and northward movement of the Intertropical Convergence Zone (ITCZ hereafter). There is a different regional character for the tropical cyclones activity: in the Western North Pacific, the number of tropical cyclones has been decreasing since 1960s, whereas in the Eastern North Pacific and North Atlantic, the number of tropical cyclones has been increasing since 1949 and 1984 respectively. Most of the tropical cyclones in the tropical oceans are generated within the ITCZ (called the monsoon trough in the Western North Pacific, and the easterly wave in the Eastern North Pacific and North Atlantic). At the same time, there are changes in the strength and position of the ITCZ. In the Western North Pacific, ITCZ strength has been weakening and its position has been moving equatorward since the 1960s when the tropical cyclones frequency decreased. In the Eastern North Pacific, the ITCZ has been strengthening and moving northward where the tropical cyclone frequency has been increasing since 1949.