Thunderstorms, Hurricanes, and Winter Storms — Covered in This and Related Guides — Can Cause Property Damage, Bodily Injury Or Even Death
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3. Electrical Structure of Thunderstorm Clouds
3. Electrical Structure of Thunderstorm Clouds 1 Cloud Charge Structure and Mechanisms of Cloud Electrification An isolated thundercloud in the central New Mexico, with rudimentary indication of how electric charge is thought to be distributed and around the thundercloud, as inferred from the remote and in situ observations. Adapted from Krehbiel (1986). 2 2 Cloud Charge Structure and Mechanisms of Cloud Electrification A vertical tripole representing the idealized gross charge structure of a thundercloud. The negative screening layer charges at the cloud top and the positive corona space charge produced at ground are ignored here. 3 3 Cloud Charge Structure and Mechanisms of Cloud Electrification E = 2 E (−)cos( 90o−α) Q H = 2 2 3/2 2πεo()H + r sinα = k Q = const R2 ( ) Method of images for finding the electric field due to a negative point charge above a perfectly conducting ground at a field point located at the ground surface. 4 4 Cloud Charge Structure and Mechanisms of Cloud Electrification The electric field at ground due to the vertical tripole, labeled “Total”, as a function of the distance from the axis of the tripole. Also shown are the contributions to the total electric field from the three individual charges of the tripole. An upward directed electric field is defined as positive (according to the physics sign convention). 5 5 Cloud Charge Structure and Mechanisms of Cloud Electrification Electric Field Change Due to Negative Cloud-to-Ground Discharge Electric Field Change Due to a Cloud Discharge Electric Field Change, kV/m Change, Electric Field Electric Field Change, kV/m Change, Electric Field Distance, km Distance, km Electric field change at ground, due to the Electric field change at ground, due to the total removal of the negative charge of the total removal of the negative and upper vertical tripole via a cloud-to-ground positive charges of the vertical tripole via a discharge, as a function of distance from cloud discharge, as a function of distance from the axis of the tripole. -
Sirocco Manual
SIROCCO INSTALLATION PROPER INSTALLATION IS IMPORTANT. IF YOU NEED ASSISTANCE, CONSULT A CONTRACTOR ELECTRICIAN OR TELEVISION ANTENNA INSTALLER (CHECK WITH YOUR LOCAL BUILDING SUPPLY, OR HARDWARE STORE FOR REFERRALS). TO PROMOTE CONFIDENCE, PERFORM A TRIAL WIRING BEFORE INSTALLATION. Determine where you are going to locate both the 1 rooftop sensor and the read-out. Feed the terminal lug end of the 2-conductor cable through 2 2-CONDUCTOR WIND SPEED the rubber boot and connect the lugs to the terminals on the bottom CABLE SENSOR of the wind speed sensor. (Do NOT adjust the nuts that are already BOOT on the sensor). The polarity does not matter. COTTER PIN 3 Slide the stub mast through the rubber boot and insert the stub mast into the bottom of the wind speed sensor. Secure with the cotter pin. Coat all conections with silicone sealant and slip the boot over the sensor. STRAIGHT STUB MAST Secure the sensor and the stub mast to your antenna 2-CONDUCTOR mast (not supplied) with the two hose clamps. Radio CABLE 4 Shack and similar stores have a selection of antenna HOSE CLAMPS masts and roof mounting brackets. Choose a mount that best suits your location and provides at least eight feet of vertical clearance above objects on the roof. TALL MAST EVE 8 FEET 5 Follow the instructions supplied with the antenna MOUNT VENT-PIPE mount and secure the mast to the mount. MOUNT CABLE WALL CHIMNEY Secure the wire to the building using CLIPS TRIPOD MOUNT MOUNT MOUNT 6 CAULK cable clips (do not use regular staples). -
PROTECT YOUR PROPERTY from STORM SURGE Owning a House Is One of the Most Important Investments Most People Make
PROTECT YOUR PROPERTY FROM STORM SURGE Owning a house is one of the most important investments most people make. Rent is a large expense for many households. We work hard to provide a home and a future for ourselves and our loved ones. If you live near the coast, where storm surge is possible, take the time to protect yourself, your family and your belongings. Storm surge is the most dangerous and destructive part of coastal flooding. It can turn a peaceful waterfront into a rushing wall of water that floods homes, erodes beaches and damages roadways. While you can’t prevent a storm surge, you can minimize damage to keep your home and those who live there safe. First, determine the Base Flood Elevation (BFE) for your home. The BFE is how high floodwater is likely to rise during a 1%-annual-chance event. BFEs are used to manage floodplains in your community. The regulations about BFEs could affect your home. To find your BFE, you can look up your address on the National Flood Hazard Layer. If you need help accessing or understanding your BFE, contact FEMA’s Flood Mapping and Insurance eXchange. You can send an email to FEMA-FMIX@ fema.dhs.gov or call 877 FEMA MAP (877-336-2627). Your local floodplain manager can help you find this information. Here’s how you can help protect your home from a storm surge. OUTSIDE YOUR HOME ELEVATE While it is an investment, elevating your SECURE Do you have a manufactured home and want flood insurance YOUR HOME home is one of the most effective ways MANUFACTURED from the National Flood Insurance Program? If so, your home to mitigate storm surge effects. -
February 2021 Historical Winter Storm Event South-Central Texas
Austin/San Antonio Weather Forecast Office WEATHER EVENT SUMMARY February 2021 Historical Winter Storm Event South-Central Texas 10-18 February 2021 A Snow-Covered Texas. GeoColor satellite image from the morning of 15 February, 2021. February 2021 South Central Texas Historical Winter Storm Event South-Central Texas Winter Storm Event February 10-18, 2021 Event Summary Overview An unprecedented and historical eight-day period of winter weather occurred between 10 February and 18 February across South-Central Texas. The first push of arctic air arrived in the area on 10 February, with the cold air dropping temperatures into the 20s and 30s across most of the area. The first of several frozen precipitation events occurred on the morning of 11 February where up to 0.75 inches of freezing rain accumulated on surfaces in Llano and Burnet Counties and 0.25-0.50 inches of freezing rain accumulated across the Austin metropolitan area with lesser amounts in portions of the Hill Country and New Braunfels area. For several days, the cold air mass remained in place across South-Central Texas, but a much colder air mass remained stationary across the Northern Plains. This record-breaking arctic air was able to finally move south into the region late on 14 February and into 15 February as a strong upper level low-pressure system moved through the Southern Plains. As this system moved through the region, snow began to fall and temperatures quickly fell into the single digits and teens. Most areas of South-Central Texas picked up at least an inch of snow with the highest amounts seen from Del Rio and Eagle Pass extending to the northeast into the Austin and San Antonio areas. -
Climatic Information of Western Sahel F
Discussion Paper | Discussion Paper | Discussion Paper | Discussion Paper | Clim. Past Discuss., 10, 3877–3900, 2014 www.clim-past-discuss.net/10/3877/2014/ doi:10.5194/cpd-10-3877-2014 CPD © Author(s) 2014. CC Attribution 3.0 License. 10, 3877–3900, 2014 This discussion paper is/has been under review for the journal Climate of the Past (CP). Climatic information Please refer to the corresponding final paper in CP if available. of Western Sahel V. Millán and Climatic information of Western Sahel F. S. Rodrigo (1535–1793 AD) in original documentary sources Title Page Abstract Introduction V. Millán and F. S. Rodrigo Conclusions References Department of Applied Physics, University of Almería, Carretera de San Urbano, s/n, 04120, Almería, Spain Tables Figures Received: 11 September 2014 – Accepted: 12 September 2014 – Published: 26 September J I 2014 Correspondence to: F. S. Rodrigo ([email protected]) J I Published by Copernicus Publications on behalf of the European Geosciences Union. Back Close Full Screen / Esc Printer-friendly Version Interactive Discussion 3877 Discussion Paper | Discussion Paper | Discussion Paper | Discussion Paper | Abstract CPD The Sahel is the semi-arid transition zone between arid Sahara and humid tropical Africa, extending approximately 10–20◦ N from Mauritania in the West to Sudan in the 10, 3877–3900, 2014 East. The African continent, one of the most vulnerable regions to climate change, 5 is subject to frequent droughts and famine. One climate challenge research is to iso- Climatic information late those aspects of climate variability that are natural from those that are related of Western Sahel to human influences. -
North American Notes
268 NORTH AMERICAN NOTES NORTH AMERICAN NOTES BY KENNETH A. HENDERSON HE year I 967 marked the Centennial celebration of the purchase of Alaska from Russia by the United States and the Centenary of the Articles of Confederation which formed the Canadian provinces into the Dominion of Canada. Thus both Alaska and Canada were in a mood to celebrate, and a part of this celebration was expressed · in an extremely active climbing season both in Alaska and the Yukon, where some of the highest mountains on the continent are located. While much of the officially sponsored mountaineering activity was concentrated in the border mountains between Alaska and the Yukon, there was intense activity all over Alaska as well. More information is now available on the first winter ascent of Mount McKinley mentioned in A.J. 72. 329. The team of eight was inter national in scope, a Frenchman, Swiss, German, Japanese, and New Zealander, the rest Americans. The successful group of three reached the summit on February 28 in typical Alaskan weather, -62° F. and winds of 35-40 knots. On their return they were stormbound at Denali Pass camp, I7,3oo ft. for seven days. For the forty days they were on the mountain temperatures averaged -35° to -40° F. (A.A.J. I6. 2I.) One of the most important attacks on McKinley in the summer of I967 was probably the three-pronged assault on the South face by the three parties under the general direction of Boyd Everett (A.A.J. I6. IO). The fourteen men flew in to the South east fork of the Kahiltna glacier on June 22 and split into three groups for the climbs. -
Understanding Storm Surge
The Education Program at the New Jersey Sea Grant Consortium 22 Magruder Road, Fort Hancock, NJ 07732 (732) 872-1300 www.njseagrant.org UNDERSTANDING STORM SURGE OVERVIEW In this climate education module, students will gain an understanding of the term “storm surge” by exploring the meteorological principles that create storms and generate storm surges. Many basics of weather are discussed, including air pressure, air circulation, and the influence of the Coriolis effect on weather. TABLE OF Background……………………………………….......................1-4 CONTENTS Activity #1- Oceans of Pressure …......................................... 5-10 Activity #2- Windy Balloon ……………………….................... 11-13 Activity #3- Density Driven Currents ………………................ 14-18 Activity #4- Coriolis Effect……………………………………. 19-22 Activity #5- Pressure Driven Storms and Surge…………..... 23-25 Activity #6- Surge of the Storm ………................................. 26-34 How Meteorologists’ Measure and Predict Storm Surge…… 35-37 Why should you care about understanding storm surge? ...... 38-39 Storm Surge Watches and Warnings ………………….……. 40-42 NOAA’s Top 10 Tips for Being Ready for a Storm Surge…...... 43 References …............................................................................ 44 OBJECTIVES Following completion of this module, students will be able to: Define storm surge and the factors that influence it Learn how temperature affects air density and the formation of high and low pressure systems in the atmosphere Explore the effect of gravity on air in the atmosphere Discover the role of Earth’s rotation on global and localized wind patterns Examine the effects that air pressure has on storm surge levels Determine how storm surge affects coastal communities Explore the impact of shoreline shape and beach slope on storm surge GRADE LEVEL 5 – 12 The New Jersey Sea Grant Consortium (NJSGC) is an affiliation of colleges, universities and other groups dedicated to advancing knowledge and stewardship of New Jersey’s marine and coastal environment. -
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. -
Cloud and Precipitation Radars
Sponsored by the U.S. Department of Energy Office of Science, the Atmospheric Radiation Measurement (ARM) Climate Research Facility maintains heavily ARM Radar Data instrumented fixed and mobile field sites that measure clouds, aerosols, Radar data is inherently complex. ARM radars are developed, operated, and overseen by engineers, scientists, radiation, and precipitation. data analysts, and technicians to ensure common goals of quality, characterization, calibration, data Data from these sites are used by availability, and utility of radars. scientists to improve the computer models that simulate Earth’s climate system. Storage Process Data Post- Data Cloud and Management processing Products Precipitation Radars Mentors Mentors Cloud systems vary with climatic regimes, and observational DQO Translators Data capabilities must account for these differences. Radars are DMF Developers archive Site scientist DMF the only means to obtain both quantitative and qualitative observations of clouds over a large area. At each ARM fixed and mobile site, millimeter and centimeter wavelength radars are used to obtain observations Calibration Configuration of the horizontal and vertical distributions of clouds, as well Scan strategy as the retrieval of geophysical variables to characterize cloud Site operations properties. This unprecedented assortment of 32 radars Radar End provides a unique capability for high-resolution delineation Mentors science users of cloud evolution, morphology, and characteristics. One-of-a-Kind Radar Network Advanced Data Products and Tools All ARM radars, with the exception of three, are equipped with dual- Reectivity (dBz) • Active Remotely Sensed Cloud Locations (ARSCL) – combines data from active remote sensors with polarization technology. Combined -60 -40 -20 0 20 40 50 60 radar observations to produce an objective determination of hydrometeor height distributions and retrieval with multiple frequencies, this 1 μm 10 μm 100 μm 1 mm 1 cm 10 cm 10-3 10-2 10-1 100 101 102 of cloud properties. -
Hail Size and Melting Considerations in Thunderstorms
Hail Size and Melting Considerations in Thunderstorms NWS Louisville, KY Hail Size and Melting Considerations Two primary factors associated with surface hail size: • Hail generation and initial size in storm • How much melting occurs as hail falls to ground Factors Contributing to Hail Generation and Size in Storm • Storm type: supercells produce larger hail than quasi-linear convective systems (QLCSs) and pulse storms; incipient cells (intense updraft) produce larger hail than after cells congeal into a mesoscale convective system (MCS) • Storm tilt: updraft/downdraft separation promotes hail growth • Updraft strength: increases hail generation and residence time in storm • Dry air aloft (~800-500): leads to evaporative cooling which promotes hail growth and size • Steep mid-level lapse rates: suggests presence of mid-level cool/dry air; promotes strong updraft • Echo tops: taller storms can tap colder air aloft (high refl above -20° C levels) and increase hail residence time in cloud • Cell/boundary mergers: promotes stronger updraft and better chance for hail formation • Values of WBZ height: hail is most favorable with height of 7-12 kft; less favorable if < 6 kft (air mass too cool, although small hail/graupel likely from low-top storms) and if >> 12 kft (melting) The size of hail at surface can’t be determined from looking at reflectivity values in a storm alone Factors Contributing to Hail Size at Surface • Large stones: better chance to reach ground than small stones which melt faster on their descent • Stones melt faster in wet environment than in dry (RH has strong effect); dry air in ~800-500 mb layer is very important to produce evaporative cooling and limit hail melting during descent (why stones are smaller or non-existent during MCSs due to saturated environment – and weaker updraft) • Hail falling within rain melts at a much greater rate than hail falling separate from rain (especially for small hail) • Vertical wind shear is critical in surface hail size to separate the updraft and downdraft and limit duration hail falls in heavy rain. -
Our Atmosphere Greece Sicily Athens
National Aeronautics and Space Administration Sardinia Italy Turkey Our Atmosphere Greece Sicily Athens he atmosphere is a life-giving blanket of air that surrounds our Crete T Tunisia Earth; it is composed of gases that protect us from the Sun’s intense ultraviolet Gulf of Gables radiation, allowing life to flourish. Greenhouse gases like carbon dioxide, Mediterranean Sea ozone, and methane are steadily increasing from year to year. These gases trap infrared radiation (heat) emitted from Earth’s surface and atmosphere, Gulf of causing the atmosphere to warm. Conversely, clouds as well as many tiny Sidra suspended liquid or solid particles in the air such as dust, smoke, and Egypt Libya pollution—called aerosols—reflect the Sun’s radiative energy, which leads N to cooling. This delicate balance of incoming and reflected solar radiation 200 km and emitted infrared energy is critical in maintaining the Earth’s climate Turkey Greece and sustaining life. Research using computer models and satellite data from NASA’s Earth Sicily Observing System enhances our understanding of the physical processes Athens affecting trends in temperature, humidity, clouds, and aerosols and helps us assess the impact of a changing atmosphere on the global climate. Crete Tunisia Gulf of Gables Mediterranean Sea September 17, 1979 Gulf of Sidra October 6, 1986 September 20, 1993 Egypt Libya September 10, 2000 Aerosol Index low high September 24, 2006 On August 26, 2007, wildfires in southern Greece stretched along the southwest coast of the Peloponnese producing Total Ozone (Dobson Units) plumes of smoke that drifted across the Mediterranean Sea as far as Libya along Africa’s north coast. -
Severe Weather Forecasting Tip Sheet: WFO Louisville
Severe Weather Forecasting Tip Sheet: WFO Louisville Vertical Wind Shear & SRH Tornadic Supercells 0-6 km bulk shear > 40 kts – supercells Unstable warm sector air mass, with well-defined warm and cold fronts (i.e., strong extratropical cyclone) 0-6 km bulk shear 20-35 kts – organized multicells Strong mid and upper-level jet observed to dive southward into upper-level shortwave trough, then 0-6 km bulk shear < 10-20 kts – disorganized multicells rapidly exit the trough and cross into the warm sector air mass. 0-8 km bulk shear > 52 kts – long-lived supercells Pronounced upper-level divergence occurs on the nose and exit region of the jet. 0-3 km bulk shear > 30-40 kts – bowing thunderstorms A low-level jet forms in response to upper-level jet, which increases northward flux of moisture. SRH Intense northwest-southwest upper-level flow/strong southerly low-level flow creates a wind profile which 0-3 km SRH > 150 m2 s-2 = updraft rotation becomes more likely 2 -2 is very conducive for supercell development. Storms often exhibit rapid development along cold front, 0-3 km SRH > 300-400 m s = rotating updrafts and supercell development likely dryline, or pre-frontal convergence axis, and then move east into warm sector. BOTH 2 -2 Most intense tornadic supercells often occur in close proximity to where upper-level jet intersects low- 0-6 km shear < 35 kts with 0-3 km SRH > 150 m s – brief rotation but not persistent level jet, although tornadic supercells can occur north and south of upper jet as well.