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Fog and Low Clouds As Troublemakers During Wildfi Res
When Our Heads Are in the Clouds Sometimes water droplets do not freeze in below- Detecting fog from space Up to 60,000 ft (18,000m) freezing temperatures. This happens if they do not have Weather satellites operated by the National Oceanic The fog comes a surface (like a dust particle or an ice crystal) upon and Atmospheric Administration (NOAA) collect data on on little cat feet. which to freeze. This below-freezing liquid water becomes clouds and storms. Cirrus Commercial Jetliner “supercooled.” Then when it touches a surface whose It sits looking (36,000 ft / 11,000m) temperature is below freezing, such as a road or sidewalk, NOAA operates two different types of satellites. over harbor and city Geostationary satellites orbit at about 22,236 miles Breitling Orbiter 3 the water will freeze instantly, making a super-slick icy on silent haunches (34,000 ft / 10,400m) Cirrocumulus coating on whatever it touches. This condition is called (35,786 kilometers) above sea level at the equator. At this and then moves on. Mount Everest (29,035 ft / 8,850m) freezing fog. altitude, the satellite makes one Earth orbit per day, just Carl Sandburg Cirrostratus as Earth rotates once per day. Thus, the satellite seems to 20,000 feet (6,000 m) Cumulonimbus hover over one spot below and keeps its “birds’-eye view” of nearly half the Earth at once. Altocumulus The other type of NOAA satellites are polar satellites. Their orbits pass over, or nearly over, the North and South Clear and cloudy regions over the U.S. -
On the Relationship Between Gravity Waves and Tropopause Height and Temperature Over the Globe Revealed by COSMIC Radio Occultation Measurements
atmosphere Article On the Relationship between Gravity Waves and Tropopause Height and Temperature over the Globe Revealed by COSMIC Radio Occultation Measurements Daocheng Yu 1, Xiaohua Xu 1,2,*, Jia Luo 1,3,* and Juan Li 1 1 School of Geodesy and Geomatics, Wuhan University, 129 Luoyu Road, Wuhan 430079, China; [email protected] (D.Y.); [email protected] (J.L.) 2 Collaborative Innovation Center for Geospatial Technology, 129 Luoyu Road, Wuhan 430079, China 3 Key Laboratory of Geospace Environment and Geodesy, Ministry of Education, 129 Luoyu Road, Wuhan 430079, China * Correspondence: [email protected] (X.X.); [email protected] (J.L.); Tel.: +86-27-68758520 (X.X.); +86-27-68778531 (J.L.) Received: 4 January 2019; Accepted: 6 February 2019; Published: 12 February 2019 Abstract: In this study, the relationship between gravity wave (GW) potential energy (Ep) and the tropopause height and temperature over the globe was investigated using COSMIC radio occultation (RO) dry temperature profiles during September 2006 to May 2013. The monthly means of GW Ep with a vertical resolution of 1 km and tropopause parameters were calculated for each 5◦ × 5◦ longitude-latitude grid. The correlation coefficients between Ep values at different altitudes and the tropopause height and temperature were calculated accordingly in each grid. It was found that at middle and high latitudes, GW Ep over the altitude range from lapse rate tropopause (LRT) to several km above had a significantly positive/negative correlation with LRT height (LRT-H)/ LRT temperature (LRT-T) and the peak correlation coefficients were determined over the altitudes of 10–14 km with distinct zonal distribution characteristics. -
Nighttime Secondary Ozone Layer During Major Stratospheric Sudden Warmings in Specified-Dynamics WACCM Olga V
JOURNAL OF GEOPHYSICAL RESEARCH: ATMOSPHERES, VOL. 118, 8346–8358, doi:10.1002/jgrd.50651, 2013 Nighttime secondary ozone layer during major stratospheric sudden warmings in specified-dynamics WACCM Olga V. Tweedy,1,2 Varavut Limpasuvan,1 Yvan J. Orsolini,3,4 Anne K. Smith,5 Rolando R. Garcia,5 Doug Kinnison,5 Cora E. Randall,6,7 Ole-Kristian Kvissel,8 Frode Stordal,8 V. Lynn Harvey,6,7 and Amal Chandran 9 Received 26 March 2013; revised 5 July 2013; accepted 15 July 2013; published 9 August 2013. [1] A major stratospheric sudden warming (SSW) strongly impacts the entire middle atmosphere up to the thermosphere. Currently, the role of atmospheric dynamics on polar ozone in the mesosphere-lower thermosphere (MLT) during SSWs is not well understood. Here we investigate the SSW-induced changes in the nighttime “secondary” (90–105 km) ozone maximum by examining the dynamics and distribution of key species (like H and O) important to ozone. We use output from the National Center for Atmospheric Research Whole Atmosphere Community Climate Model with “Specified Dynamics” (SD-WACCM), in which the simulation is constrained by meteorological reanalyses below 1 hPa. Composites are made based on six major SSW events with elevated stratopause episodes. Individual SSW cases of temperature and MLT nighttime ozone from the model are compared against the Sounding of the Atmosphere using Broadband Emission Radiometry observations aboard the NASA’s Thermosphere Ionosphere Mesosphere Energetics and Dynamics (TIMED) satellite. The evolution of ozone and major chemical trace species is associated with the anomalous vertical residual motion during SSWs and consistent with photochemical equilibrium governing the MLT nighttime ozone. -
Stratosphere-Troposphere Coupling: a Method to Diagnose Sources of Annular Mode Timescales
STRATOSPHERE-TROPOSPHERE COUPLING: A METHOD TO DIAGNOSE SOURCES OF ANNULAR MODE TIMESCALES Lawrence Mudryklevel, Paul Kushner p R ! ! SPARC DynVar level, Z(x,p,t)=− T (x,p,t)d ln p , (4) g !ps x,t p ( ) R ! ! Z(x,p,t)=− T (x,p,t)d ln p , (4) where p is the pressure at the surface, R is the specific gas constant and g is the gravitational acceleration s g !ps(x,t) where p is the pressure at theat surface, the surface.R is the specific gas constant and g is the gravitational acceleration Abstract s Geopotentiallevel, Height Decomposition Separation of AM Timescales p R ! ! at the surface. This time-varying geopotentialZ( canx,p,t be)= decomposed− T into(x,p a,t cli)dmatologyln p , and anomalies from the(4) climatology AM timescales track seasonal variations in the AM index’s decorrelation time6,7. For a hydrostatic fluid, geopotential height may be describedg !p sas(x ,ta) function of time, pressure level Timescales derived from Annular Mode (AM) variability provide dynamical and ashorizontalZ(x,p,t position)=Z (asx,p a )+temperatureδZ(x,p,t integral). Decomposing from the Earth’s the temperature surface to a andgiven surface pressure pressure fields inananalogous insight into stratosphere-troposphere coupling and are linked to the strengthThis of time-varying level, geopotentialwhere can beps is decomposed the pressure at into the a surface, climatologyR is the and specific anomalies gas constant from and theg is climatology the gravitational acceleration NCEP, 1958-2007 level: ^ a) o (yL ) d) o AM responses to climate forcings. -
Popular Summary of “Extratropical Stratosphere-Troposphere Mass Exchange”
Popular Summary of “Extratropical Stratosphere-Troposphere Mass Exchange” Mark Schoeberl Understanding the exchange of gases between the stratosphere and the troposphere is important for determining how pollutants enter the stratosphere and how they leave. This study does a global analysis of that the exchange of mass between the stratosphere and the troposphere. While the exchange of mass is not the same as the exchange of constituents, you can’t get the constituent exchange right if you have the mass exchange wrong. Thus this kind of calculation is an important test for models which also compute trace gas transport. In this study I computed the mass exchange for two assimilated data sets and a GCM. The models all agree that amount of mass descending from the stratosphere to the troposphere in the Northern Hemisphere extra tropics is -1 0” kg/s averaged over a year. The value for the Southern Hemisphere by about a factor of two. ( 10” kg of air is the amount of air in 100 km x 100 km area with a depth of 100 m - roughly the size of the D.C. metro area to a depth of 300 feet.) Most people have the idea that most of the mass enters the stratosphere through the tropics. But this study shows that almost 5 times more mass enters the stratosphere through the extra-tropics. This mass, however, is quickly recycled out again. Thus the lower most stratosphere is a mixture of upper stratospheric air and tropospheric air. This is an important result for understanding the chemistry of the lower stratosphere. -
Hohonu Volume 5 (PDF)
HOHONU 2007 VOLUME 5 A JOURNAL OF ACADEMIC WRITING This publication is available in alternate format upon request. TheUniversity of Hawai‘i is an Equal Opportunity Affirmative Action Institution. VOLUME 5 Hohonu 2 0 0 7 Academic Journal University of Hawai‘i at Hilo • Hawai‘i Community College Hohonu is publication funded by University of Hawai‘i at Hilo and Hawai‘i Community College student fees. All production and printing costs are administered by: University of Hawai‘i at Hilo/Hawai‘i Community College Board of Student Publications 200 W. Kawili Street Hilo, Hawai‘i 96720-4091 Phone: (808) 933-8823 Web: www.uhh.hawaii.edu/campuscenter/bosp All rights revert to the witers upon publication. All requests for reproduction and other propositions should be directed to writers. ii d d d d d d d d d d d d d d d d d d d d d d Table of Contents 1............................ A Fish in the Hand is Worth Two on the Net: Don’t Make me Think…different, by Piper Seldon 4..............................................................................................Abortion: Murder-Or Removal of Tissue?, by Dane Inouye 9...............................An Etymology of Four English Words, with Reference to both Grimm’s Law and Verner’s Law by Piper Seldon 11................................Artifacts and Native Burial Rights: Where do We Draw the Line?, by Jacqueline Van Blarcon 14..........................................................................................Ayahuasca: Earth’s Wisdom Revealed, by Jennifer Francisco 16......................................Beak of the Fish: What Cichlid Flocks Reveal About Speciation Processes, by Holly Jessop 26................................................................................. Climatic Effects of the 1815 Eruption of Tambora, by Jacob Smith 33...........................Columnar Joints: An Examination of Features, Formation and Cooling Models, by Mary Mathis 36.................... -
Aviation Glossary
AVIATION GLOSSARY 100-hour inspection – A complete inspection of an aircraft operated for hire required after every 100 hours of operation. It is identical to an annual inspection but may be performed by any certified Airframe and Powerplant mechanic. Absolute altitude – The vertical distance of an aircraft above the terrain. AD - See Airworthiness Directive. ADC – See Air Data Computer. ADF - See Automatic Direction Finder. Adverse yaw - A flight condition in which the nose of an aircraft tends to turn away from the intended direction of turn. Aeronautical Information Manual (AIM) – A primary FAA publication whose purpose is to instruct airmen about operating in the National Airspace System of the U.S. A/FD – See Airport/Facility Directory. AHRS – See Attitude Heading Reference System. Ailerons – A primary flight control surface mounted on the trailing edge of an airplane wing, near the tip. AIM – See Aeronautical Information Manual. Air data computer (ADC) – The system that receives and processes pitot pressure, static pressure, and temperature to present precise information in the cockpit such as altitude, indicated airspeed, true airspeed, vertical speed, wind direction and velocity, and air temperature. Airfoil – Any surface designed to obtain a useful reaction, or lift, from air passing over it. Airmen’s Meteorological Information (AIRMET) - Issued to advise pilots of significant weather, but describes conditions with lower intensities than SIGMETs. AIRMET – See Airmen’s Meteorological Information. Airport/Facility Directory (A/FD) – An FAA publication containing information on all airports, seaplane bases and heliports open to the public as well as communications data, navigational facilities and some procedures and special notices. -
Amplify Science Earth's Changing Climate
Lawrence Hall of Science has new instructional materials that address the Next Generation Science Standards! Check out these Middle School Units… As just one example, compare Middle School units from three different Hall programs. See for yourself how each program goes about addressing the Middle School NGSS Standards related to Human Impacts and Climate Change, and choose the approach that best meets the needs of your school district. MS NGSS Performance Expectations: Human Impacts and Climate Change • MS-ESS3-2. Analyze and interpret data on natural hazards to forecast future catastrophic events and inform the development of technologies to mitigate their effects. • MS-ESS3-3. Apply scientific principles to design a method for monitoring and minimizing a human impact on the Environment. • MS-ESS3-4. Construct an argument supported by evidence for how increases in human population and per-capita consumption of natural resources impact Earth’s systems. • MS-ESS3-5. Ask questions to clarify evidence of the factors that have caused the rise in global temperatures over the past century. Sample Units from Three Different Hall Programs • Amplify Science—Earth’s Changing Climate: Vanishing Ice Earth’s Changing Climate Engineering Internship • FOSS—Weather and Water • Ocean Sciences Sequence—The Ocean-Atmosphere Connection and Climate Change ©The Regents of the University of California ©The Regents of the University of California Description of two Middle School units from Amplify Science Earth’s Changing Climate: Vanishing Ice and Earth’s Changing Climate Engineering Internship Grade 6-8 Units — requiring at least 19 and 10 45-minute class sessions respectively (two of 27 Middle School Amplify Science units) The Problem: Why is the ice on Earth’s surface melting? Students’ Role: In the role of student climatologists, students investigate what is causing ice on Earth’s surface to melt in order to help the fictional World Climate Institute educate the public about the processes involved. -
Solar Energy Generation Model for High Altitude Long Endurance Platforms
Solar Energy Generation Model for High Altitude Long Endurance Platforms Mathilde Brizon∗ KTH - Royal Institute of Technology, Stockholm, Sweden For designing and evaluating new concepts for HALE platforms, the energy provided by solar cells is a key factor. The purpose of this thesis is to model the electrical power which can be harnessed by such a platform along any flight trajectory for different aircraft designs. At first, a model of the solar irradiance received at high altitude will be performed using the solar irradiance models already existing for ground level applications as a basis. A calculation of the efficiency of the energy generation will be performed taking into account each solar panel's position as well as shadows casted by the aircraft's structure. The evaluated set of trajectories allows a stationary positioning of a hale platform with varying wind conditions, time of day and latitude for an exemplary aircraft configuration. The qualitative effects of specific parameter changes on the harnessed solar energy is discussed as well as the fidelity of the energy generation model results. Nomenclature δ Solar declination ({) EQE Quantum efficiency (%) η Efficiency (%) hg Altitude of the aircraft (m) ◦ Γ Day angle ( ) hO3 Height of max ozone concentration(m) ◦ −2 −1 λg Longitude aircraft ( ) Id Direct irradiance (W:m .µm ) ◦ −2 −1 ! Hour angle ( ) Is Diffuse irradiance (W:m .µm ) ◦ −2 −1 φg Latitude of the aircraft ( ) Itot Total irradiance (W:m .µm ) ◦ −1 ◦ τ Rayleigh optical depth ({) kPmax;T Temperature Coefficient (%: C ) 2 A Solar cell -
Planets of the Solar System
Chapter Planets of the 27 Solar System Chapter OutlineOutline 1 ● Formation of the Solar System The Nebular Hypothesis Formation of the Planets Formation of Solid Earth Formation of Earth’s Atmosphere Formation of Earth’s Oceans 2 ● Models of the Solar System Early Models Kepler’s Laws Newton’s Explanation of Kepler’s Laws 3 ● The Inner Planets Mercury Venus Earth Mars 4 ● The Outer Planets Gas Giants Jupiter Saturn Uranus Neptune Objects Beyond Neptune Why It Matters Exoplanets UnderstandingU d t di theth formationf ti and the characteristics of our solar system and its planets can help scientists plan missions to study planets and solar systems around other stars in the universe. 746 Chapter 27 hhq10sena_psscho.inddq10sena_psscho.indd 774646 PDF 88/15/08/15/08 88:43:46:43:46 AAMM Inquiry Lab Planetary Distances 20 min Turn to Appendix E and find the table entitled Question to Get You Started “Solar System Data.” Use the data from the How would the distance of a planet from the sun “semimajor axis” row of planetary distances to affect the time it takes for the planet to complete devise an appropriate scale to model the distances one orbit? between planets. Then find an indoor or outdoor space that will accommodate the farthest distance. Mark some index cards with the name of each planet, use a measuring tape to measure the distances according to your scale, and place each index card at its correct location. 747 hhq10sena_psscho.inddq10sena_psscho.indd 774747 22/26/09/26/09 111:42:301:42:30 AAMM These reading tools will help you learn the material in this chapter. -
Global Warming Climate Records
ATM S 111: Global Warming Climate Records Jennifer Fletcher Day 24: July 26 2010 Reading For today: “Keeping Track” (Climate Records) pp. 171-192 For tomorrow/Wednesday: “The Long View” (Paleoclimate) pp. 193-226. The Instrumental Record from NASA Global temperature since 1880 Ten warmest years: 2001-2009 and 1998 (biggest El Niño ever) Separation into Northern/ Southern Hemispheres N. Hem. has warmed more (1o C vs 0.8o C globally) S. Hem. has warmed more steadily though Cooling in the record from 1940-1975 essentially only in the N. Hem. record (this is likely due to aerosol cooling) Temperature estimates from other groups CRUTEM3 (RG calls this UEA) NCDC (RG calls this NOAA) GISS (RG calls this NASA) yet another group Surface air temperature over land Thermometer between 1.25-2 m (4-6.5 ft) above ground White colored to reflect away direct sunlight Slats to ensure fresh air circulation “Stevenson screen”: invented by Robert Louis Stevenson’s dad Thomas Yearly average Central England temperature record (since 1659) Temperatures over Land Only NASA separates their analysis into land station data only (not including ship measurements) Warming in the station data record is larger than in the full record (1.1o C as opposed to 0.8o C) Sea surface temperature measurements Standard bucket Canvas bucket Insulated bucket (~1891) (pre WWII) (now) “Bucket” temperature: older style subject to evaporative cooling Starting around WWII: many temperature measurements taken from condenser intake pipe instead of from buckets. Typically 0.5 C warmer -
Atmospheric Thermal and Dynamic Vertical Structures of Summer Hourly Precipitation in Jiulong of the Tibetan Plateau
atmosphere Article Atmospheric Thermal and Dynamic Vertical Structures of Summer Hourly Precipitation in Jiulong of the Tibetan Plateau Yonglan Tang 1, Guirong Xu 1,*, Rong Wan 1, Xiaofang Wang 1, Junchao Wang 1 and Ping Li 2 1 Hubei Key Laboratory for Heavy Rain Monitoring and Warning Research, Institute of Heavy Rain, China Meteorological Administration, Wuhan 430205, China; [email protected] (Y.T.); [email protected] (R.W.); [email protected] (X.W.); [email protected] (J.W.) 2 Heavy Rain and Drought-Flood Disasters in Plateau and Basin Key Laboratory of Sichuan Province, Institute of Plateau Meteorology, China Meteorological Administration, Chengdu 610072, China; [email protected] * Correspondence: [email protected]; Tel.: +86-27-8180-4913 Abstract: It is an important to study atmospheric thermal and dynamic vertical structures over the Tibetan Plateau (TP) and their impact on precipitation by using long-term observation at represen- tative stations. This study exhibits the observational facts of summer precipitation variation on subdiurnal scale and its atmospheric thermal and dynamic vertical structures over the TP with hourly precipitation and intensive soundings in Jiulong during 2013–2020. It is found that precipitation amount and frequency are low in the daytime and high in the nighttime, and hourly precipitation greater than 1 mm mostly occurs at nighttime. Weak precipitation during the daytime may be caused by air advection, and strong precipitation at nighttime may be closely related with air convection. Both humidity and wind speed profiles show obvious fluctuation when precipitation occurs, and the greater the precipitation intensity, the larger the fluctuation. Moreover, the fluctuation of wind speed Citation: Tang, Y.; Xu, G.; Wan, R.; Wang, X.; Wang, J.; Li, P.