Is the Term ‚Climate' Too Unspecific for a Fruitful Discussion?
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E-Region Auroral Ionosphere Model
atmosphere Article AIM-E: E-Region Auroral Ionosphere Model Vera Nikolaeva 1,* , Evgeny Gordeev 2 , Tima Sergienko 3, Ludmila Makarova 1 and Andrey Kotikov 4 1 Arctic and Antarctic Research Institute, 199397 Saint Petersburg, Russia; [email protected] 2 Earth’s Physics Department, Saint Petersburg State University, 199034 Saint Petersburg, Russia; [email protected] 3 Swedish Institute of Space Physics, 981 28 Kiruna, Sweden; [email protected] 4 Saint Petersburg Branch of Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation of Russian Academy of Sciences (IZMIRAN), 199034 Saint Petersburg, Russia; [email protected] * Correspondence: [email protected] Abstract: The auroral oval is the high-latitude region of the ionosphere characterized by strong vari- ability of its chemical composition due to precipitation of energetic particles from the magnetosphere. The complex nature of magnetospheric processes cause a wide range of dynamic variations in the auroral zone, which are difficult to forecast. Knowledge of electron concentrations in this highly turbulent region is of particular importance because it determines the propagation conditions for the radio waves. In this work we introduce the numerical model of the auroral E-region, which evaluates density variations of the 10 ionospheric species and 39 reactions initiated by both the solar extreme UV radiation and the magnetospheric electron precipitation. The chemical reaction rates differ in more than ten orders of magnitude, resulting in the high stiffness of the ordinary differential equations system considered, which was solved using the high-performance Gear method. The AIM-E model allowed us to calculate the concentration of the neutrals NO, N(4S), and N(2D), ions + + + + + 4 + 2 + 2 N ,N2 , NO ,O2 ,O ( S), O ( D), and O ( P), and electrons Ne, in the whole auroral zone in the Citation: Nikolaeva, V.; Gordeev, E.; 90-150 km altitude range in real time. -
Appendix I Glossary
Appendix I Glossary Editor: A.P.M. Baede A → indicates that the following term is also contained in this Glossary. Adjustment time centrimetric precision. Altimetry has the advantage of being a See: →Lifetime; see also: →Response time. measurement relative to a geocentric reference frame, rather than relative to land level as for a →tide gauge, and of affording quasi- Aerosols global coverage. A collection of airborne solid or liquid particles, with a typical size between 0.01 and 10 µm and residing in the atmosphere for Anthropogenic at least several hours. Aerosols may be of either natural or Resulting from or produced by human beings. anthropogenic origin. Aerosols may influence climate in two ways: directly through scattering and absorbing radiation, and Atmosphere indirectly through acting as condensation nuclei for cloud The gaseous envelope surrounding the Earth. The dry formation or modifying the optical properties and lifetime of atmosphere consists almost entirely of nitrogen (78.1% volume clouds. See: →Indirect aerosol effect. mixing ratio) and oxygen (20.9% volume mixing ratio), The term has also come to be associated, erroneously, with together with a number of trace gases, such as argon (0.93% the propellant used in “aerosol sprays”. volume mixing ratio), helium, and radiatively active →greenhouse gases such as →carbon dioxide (0.035% volume Afforestation mixing ratio), and ozone. In addition the atmosphere contains Planting of new forests on lands that historically have not water vapour, whose amount is highly variable but typically 1% contained forests. For a discussion of the term →forest and volume mixing ratio. The atmosphere also contains clouds and related terms such as afforestation, →reforestation, and →aerosols. -
The Observation of the Lightning Induced Variations in Atmospheric Ions
XV International Conference on Atmospheric Electricity, 15-20 June 2014, Norman, Oklahoma, U.S.A. The Observation of the Lightning Induced Variations in Atmospheric Ions Xuemeng Chen1,*, Hanna E. Manninen1,2, Pasi Aalto1, Petri Keronen1, Antti Mäkelä3, Jussi Paatero3, Tuukka Petäjä1 and Markku Kulmala1 1. Department of Physics, University of Helsinki, Helsinki, Finland 2. Institute of Physics, University of Tartu, Estonia 3. Finnish Meteorological Institute, Helsinki, Finland ABSTRACT: Variations in atmospheric ion concentration were studied in a boreal forest in Finland, with emphasis on the effect of lightning. In general, changes in ion concentrations have diurnal and seasonal patterns. Distinct features were found in ions of different size ranges, namely small ions (0.8 – 1.7 nm) and intermediate ions (1.7 – 7 nm). Preliminary results on two case studies of lightning effect are present, one with rain effect and the other not. Bursts in the concentrations of small ions and intermediate ions were observed in both cases. However, different trends in trace gases were observed for the two cases. Further investigation is needed to reveal the nature of lightning ions and the mechanism in their formation. The work is under progress. INTRODUCTION Atmospheric ions, or air ions, refer to electric charge carriers present in the atmosphere. Distinct features exist in their chemical composition, mass, size as well as number of carried charges. According to Tammet [1998], atmospheric ions can be classified into small or cluster ions, intermediate ions, and large ions based on their mobility (Z) in air, being Z > 0.5 cm2V-1s-1, 0.5 cm2V-1s-1 ≤ Z ≥ 0.03 cm2V-1s-1 and Z< 0.03 cm2V-1s-1, respectively. -
Aeronomy and Astrophysics
Aeronomy and astrophysics A southern high-latitude geomagnetic index: AES-80 C.G. MACLENNAN, Bell Laboratories, Lucent Technologies, Murray Hill, New Jersey 07974 P. B ALLATORE, Istito de Fisica della Spazio Interplanetario, Consiglio Nazionale della Ricerche, c.p. 27, 00044 Frascati, Rome, Italy M.J. ENGEBRETSON, Department of Physics, Augsburg College, Minneapolis, Minnesota 55454 L.J. LANZEROTTI, Bell Laboratories, Lucent Technologies, Murray Hill, New Jersey 07974 eomagnetic measurements obtained at McMurdo Sta- G tion (Arrival Heights) and at two of the U.S. automatic geophysical observatories (AGO-1; AGO-4) are being com- bined with measurements made at Casey and Dumont D'Urville to construct a Southern Hemisphere geomagnetic index for the geomagnetic latitude 80°S. The calculation of the index is modeled on the calculation of the Northern Hemi- sphere auroral electrojet index AE and is thus called the AES- 80 index. The AE index was developed to monitor geomagnetic activity at auroral zone latitudes in the Northern Hemisphere (Davis and Sugiura 1966) and indicates the level of auroral electrojet currents and in particular the occurrence of sub- storms (Baumjohann 1986). It is calculated as the difference between the upper (AU) and the lower (AL) envelope of mag- netograms from 12 observatories located at northern geomag- netic latitudes between 60° and 70° and rather uniformly distributed over all longitudes. Because of the land mass dis- tribution in Antarctica, it is impossible to have ground obser- vatories located uniformly at geomagnetic latitudes between 60° and 70°S (see figure 1). Unlike in the Northern Hemisphere, Figure 1. Map of Antarctica, with the stations used to calculate the however, it is possible in Antarctica to have reasonable ground AES-80 index shown as filled circles. -
UPPER ATMOSPHERE RESEARCH at INPE B.R. Clbmesha Department of Geophysics and Aeronomy Instituto De Pesquisas Espaciais
UPPER ATMOSPHERE RESEARCH AT INPE B.R. CLbMESHA Department of Geophysics and Aeronomy Instituto de Pesquisas Espaciais - INPE ABSTRACT Upper atmosphere research at INPE is mainly concerned with the chemistry and dynamics of the stratosphere, upper mesosphere and lower thermosphere, and the middle thermo- sphere. Experimental work includes lidar observations of the stratospheric aerosol, measurements of stratospheric ozone by Dobson spectrophotometers and by balloon and rocket-borne sondes, lidar measurements of atmospheric sodium, and photom- etric observations of 0, 02 , OH and Na emissions, including interferometric measurements of the 016300 emission for the purpose of determining thermospheric winds and temperature. The airglow observations also include measurements of a number of emissions produced by the precipitation of ener- getic neutral particles generated by charge exchange in the ring current. Some recent results of INPE's upper atmosphere program are presented.ii» this paper. ' ' n/ .71. 1- INTRODUCTION INPK maintains an active program of research into a number of aspects of upper atmosphere science, including both experimental and theoretical studies of the dynamics and chemistry of the stratosphere, mesosphere and lower thermosphere. Hxperimental work involves mainly ground-based optical techniques, although balloon and rocket-borne sondes are used for studies of stratospheric ozone, and a rocket-borne photometer payload is under development for measurements of a number of emissions from the thermosphere. Theoretical studies include numerical model- ling with special reference to a number of minor constituents related to the experimental measurements. In the following sec- tions we present a brief description of INPE's experimental fa- cilities in the area of upper atmosphere science, and outline some recent results. -
Status of NSF Space Physics
Status of NSF Space Physics Rich Behnke Therese Moretto, Bob Robinson, Anja Stromme, and Ray Walker National Academy – March 7,2013 • Status and Updates • NSF Response to the Academy’s “Solar and Space Physics: A Science for a Technological Society 2 The Five Geospace Programs • Solar Physics -- Paul Bellaire has retired, new PD has been selected – but not signed. • Magnetospheric Physics – Ray Walker • Aeronomy – Anja Stromme • Geospace Facilities – Bob Robinson • Space Weather and Instrumentation -- Therese Moretto Aeronomy (AER) • Typically around 95 proposals per year, about 1/3 funded. Budget is about $11M • Home of CEDAR • Program Director --Anja Stromme (SRII) 4 Magnetospheric Physics (MAG) • typically around 90 proposals per year, 1/3 funded. Budget is about $8.5M. • Home of GEM • Program Director – Ray Walker (UCLA) 5 Solar Physics Program (STR) •Typically around 80 proposals per year, 1/3 funded. Budget is about $8.5M •Home of SHINE •Program Director – Paul Bellaire/TBA 6 The Geospace Facilities Program (GS) Program Director – Bob Robinson • Six incoherent scatter radar sites (five awards:~$12M) • Lidar Consortium (six institutions: ~$1M) • Miscellaneous facility-related awards (facility supplements, CAREER, REU, Workshops, schools: ~1M) SuperDARN is being expanded • The Mid-latitude SuperDARN Array ( AGS’s first midscale project): New SuperDARN radars have been constructed and are operational at: Fort Hays, Kansas; Christmas Valley, Oregon; and Adak, Alaska • Negotiations are underway with Portuguese officials in the Azores -
Meteorology (MTEOR) 1
Meteorology (MTEOR) 1 MTEOR 140: Climate and Society METEOROLOGY (MTEOR) (Cross-listed with AGRON, ENV S, GEOL). Cr. 3. F.S. Any experimental courses offered by MTEOR can be found at: The climate system of our planet. How nature and our actions alter the registrar.iastate.edu/faculty-staff/courses/explistings/ (http:// existing energy balance leading to climate change. Past climates on www.registrar.iastate.edu/faculty-staff/courses/explistings/) our planet. The influence of climate on society and resource availability during the Holocene (~ 11,000 years ago to present) with focus on Courses primarily for undergraduates: changes post industrial revolution. Significant climate events that have altered our way of life in the past. Projected changes in future climate and MTEOR 107: Severe and Hazardous Weather potential impacts on society, environment and resources. Adaption to and (2-0) Cr. 1. F. mitigation of climate change. Understanding of atmospheric processes that play a role in creating severe and hazardous weather. Focus on thunderstorms, tornadoes, MTEOR 160: Water Resources of the World hurricanes, floods, blizzards, ice storms, and temperature extremes. (Cross-listed with AGRON, ENV S, GEOL). (3-0) Cr. 3. S. Impacts on lives and property. Study of the occurrence, history, development, and management of world water resources. Basic hydrologic principles including climate, surface MTEOR 111: Synoptic Applications water, groundwater, and water quality. Historical and current perspectives (1-0) Cr. 1. Repeatable. F. on water policy, use, and the role of water in society and the environment. Prereq: Credit or enrollment in MATH 165 Meets International Perspectives Requirement. Current weather discussions and introduction to synoptic-scale interpretation of meteorology. -
CEDAR an Aeronomy Initiative
Eos, Vol. 68, No. 2, January 13, 1987 Rep. 4, Bur. Gravimetrique Int., Toulouse, data, terrestrial gravity and other data, Rep. Bernard Moynot re France, 1982. 322, Dep. of Geodetic Sci. and Surveying, ceived his degree in mathe Balmino, G., C. Brossier, A. Cazenave, and F. Ohio State Univ., Columbus, 1982. matics from the Ecole Nor Nouel, Geoid of the Kerguelen Islands area Rapp, R. H., The determination of geoid un male Superieure of Paris determined from GEOS 3 Altimeter data, dulations and gravity anomalies from Sea in 1963. In 1956, he be /. Geophys. Res., 84, 3827, 1979. sat altimeter data,/ Geophys. Res., 88, 1552, gan working with the Cen Cazenave, A., B. Lago, and K. Dominh, 1983a. tre National d'Etudes Spa Thermal parameters of the oceanic litho- Rapp, R. H., The development of the Janu tiales, performing research sphere estimated from geoid height data, J. ary 1983 1° x 1° mean free-air anomaly in satellite geodesy and nu Geophys. Res., 88, 1105, 1983. data tape, internal report, Dept. of Geodet merical analysis. He is now Haxby, W. F., G. D. Karner, J. F. Labrecque, ic Sci. and Surveying, Ohio State Univ., Co with the Bureau Gravime and J. K. Weissel, Digital images of com lumbus, 1983ft. trique International in Toulouse. bined oceanic and continental data sets and Reigber, C, H. Muller, W. Bosch, G. Bal Michel Sarrailh gradu their use in tectonic studies, Eos Trans. mino, and B. Moynot, GRIM gravity model ated from the Institut de AGU, 64, 995, 1983. improvement using LAGEOS (GRIM 3- Physique du Globe in Lazarewicz, A. -
Atmospheric Physics I
Atmospheric Physics I PHYS 621, Fall 2016 Dates and Location: Tuesday & Thursday, 2:30PM- 3:45AM; Public Policy 367 INSTRUCTOR: Dr. Pengwang Zhai Email: [email protected] Ph.: 410-455-3682 (office) OFFICE HOURS: Anytime Through Email appointment TEXTS: Wallace, J.M. and P. V. Hobbs, Atmospheric Science: An Introductory Survey, 2nd ed., Elsevier, 2006 Salby, M. L., Fundamentals of Atmospheric Physics, Academic Press, 1996. REFERENCE TEXTS (Highly recommend): Holton, J. R. Introduction to Dynamic Meteorology, 4th ed., Academic Press, 2004. DESCRIPTION: Composition and structure of the earth's atmosphere, atmospheric radiation and thermodynamics, fundamentals of atmospheric dynamics, overview of climatology. GRADING: Homework (25%), Midterm (30%), Final (40%), Participation/Discussion(5%) Course Strategy: There will be no exam make-up except for University-policy accepted absence. To promote active learning, students are strongly encouraged to read the corresponding textbook chapters before each lecture. Pre-lecture homework and discussion assignments are given routinely before lectures. Reading the sections of the textbook corresponding to the assigned homework exercises is considered part of the homework assignment; you are responsible for material in the assigned reading whether or not it is discussed in the lecture. Homework will be due weekly in Thursday’s lecture. There will be a 30% penalty on late homework submissions. COURSE OUTLINE: Overview A. Earth's atmosphere System of units The Sun and the orbit and size of Earth Chemical constituents of Earth’s atmosphere Vertical structure of temperature and density Wind and precipitation Ozone layer, hydrological and carbon cycles Global Energy Budget B. Atmospheric Radiation Maxwell’s Equation & EM wave Blackbody radiation: Planck’s Law and Stefan-Boltzmann’s law Spectral characteristics of Solar and Thermal infrared radiation Atmospheric absorption & Greenhouse effect Atmospheric scattering, clouds and aerosols Radiative forcing and climate Spatial and Temporal distribution of solar radiation C. -
Twelve Lectures on Cloud Physics
Twelve Lectures on Cloud Physics Bjorn Stevens Winter Semester 2010-2011 Contents 1 Lecture 1: Clouds–An Overview3 1.1 Organization...........................................3 1.2 What is a cloud?.........................................3 1.3 Why are we interested in clouds?................................4 1.4 Cloud classification schemes..................................5 2 Lecture 2: Thermodynamic Basics6 2.1 Thermodynamics: A brief review................................6 2.2 Variables............................................8 2.3 Intensive, Extensive, and specific variables...........................8 2.3.1 Thermodynamic Coordinates..............................8 2.3.2 Composite Systems...................................8 2.3.3 The many variables of atmospheric thermodynamics.................8 2.4 Processes............................................ 10 2.5 Saturation............................................ 10 3 Lecture 3: Droplet Activation 11 3.1 Supersaturation over curved surfaces.............................. 12 3.2 Solute effects.......................................... 14 3.3 The Kohler¨ equation and its properties............................. 15 4 Lecture 4: Further Properties of an Isolated Drop 16 4.1 Diffusional growth....................................... 16 4.1.1 Temperature corrections................................ 18 4.1.2 Drop size effects on droplet growth.......................... 20 4.2 Terminal fall speeds of drops and droplets........................... 20 5 Lecture 5: Populations of Particles 22 5.1 -
4.3A Anticipating the Formation of Tornadoes Through Data Mining
4.3A Anticipating the formation of tornadoes through data mining Amy McGovern Derek H. Rosendahl School of Computer Science School of Meteorology University of Oklahoma University of Oklahoma Norman, OK Norman, OK [email protected] [email protected] Adrianna Kruger Meredith G. Beaton School of Computer Science School of Computer Science University of Oklahoma University of Oklahoma Norman, OK Norman, OK [email protected] [email protected] Rodger A. Brown Kelvin K. Droegemeier NOAA School of Meteorology National Severe Storms Laboratory University of Oklahoma Norman, OK Norman, OK [email protected] [email protected] 1. Introduction we develop new data mining techniques (computer science) to understand the data and analyze the re- sults (meteorology). This becomes a cycle where Severe weather phenomena such as tornados, thun- the results inform new techniques and new tech- derstorms, hail, and floods, annually cause signifi- niques produce new results. The results presented cant loss of life, property and crop destruction, and in this paper represent the beginning of this re- disruption of the transportation systems. The annual search. economic impact of these phenomena is estimated to be greater than 13 billion dollars (Pielke and Car- bone 2002). Any mitigation of the effects of these storms would be beneficial. 2. Meteorological Data We propose to enhance our understanding of the formation of severe weather events, specif- With our goal of improving the detection and antic- ically focusing on tornadoes, through data min- ipation of tornadoes, we are not taking the tradi- ing/knowledge discovery techniques. The process of tional route of examining radar reflectivity and ra- knowledge discovery is about making sense of data. -
On the Bernoulli Equation in the Free Atmosphere and Mechanism of Long-Lived Vortex Formation
Physical Science International Journal 11(4): 1-6, 2016, Article no.PSIJ.28055 ISSN: 2348-0130 SCIENCEDOMAIN international www.sciencedomain.org On the Bernoulli Equation in the Free Atmosphere and Mechanism of Long-lived Vortex Formation Andrei Nechayev 1* 1Department of Geographic, Lomonosov Moscow State University, 119991, Leninskiye Gori 1, Moscow, Russian Federation. Author’s contribution The sole author designed, analyzed and interpreted and prepared the manuscript. Article Information DOI: 10.9734/PSIJ/2016/28055 Editor(s): (1) Kazuharu Bamba, Division of Human Support System, Faculty of Symbiotic Systems Science, Fukushima University, Japan. (2) Christian Brosseau, Distinguished Professor, Department of Physics, Université de Bretagne Occidentale, France. Reviewers: (1) Isidro A. Pérez, University of Valladolid, Spain. (2) Anonymous, Russia. Complete Peer review History: http://www.sciencedomain.org/review-history/15874 Received 30 th June 2016 Accepted 11 th August 2016 Original Research Article th Published 20 August 2016 ABSTRACT A new universal mechanism of the formation of long-lived atmospheric vortex is proposed. It is based on the hydrodynamic pressure drop in the air stream, if air density decreases in the flow direction. The magnitude of this drop may increase with jet velocity increasing. It is assumed that jet, linking the atmospheric layers with different air density, may have a local area of low pressure which can generate the vortex. The possible conditions for the emergence and intensification of atmospheric vortices of various types are discussed. Keywords: Atmospheric vortex; hurricane; tornado; vortex formation mechanism. 1. INTRODUCTION amount of information about atmospheric vortices from the small and harmless dust devils Atmospheric vortex as a natural phenomenon to deadly tornado, destroying everything in its has long been known.