Biomes by Keneisha Boozer
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Fossil Fuels
Gonzaga Debate Institute 1 Warming Core Warming Bad Gonzaga Debate Institute 2 Warming Core ***Science Debate*** Gonzaga Debate Institute 3 Warming Core Warming Real – Generic Warming real - consensus Brooks 12 - Staff writer, KQED news (Jon, staff writer, KQED news, citing Craig Miller, environmental scientist, 5/3/12, "Is Climate Change Real? For the Thousandth Time, Yes," KQED News, http://blogs.kqed.org/newsfix/2012/05/03/is- climate-change-real-for-the-thousandth-time-yes/) BROOKS: So what are the organizations that say climate change is real? MILLER: Virtually ever major, credible scientific organization in the world. It’s not just the UN’s Intergovernmental Panel on Climate Change. Organizations like the National Academy of Sciences, the American Geophysical Union, the American Association for the Advancement of Science. And that's echoed in most countries around the world. All of the most credible, most prestigious scientific organizations accept the fundamental findings of the IPCC. The last comprehensive report from the IPCC, based on research, came out in 2007. And at that time, they said in this report, which is known as AR-4, that there is "very high confidence" that the net effect of human activities since 1750 has been one of warming. Scientists are very careful, unusually careful, about how they put things. But then they say "very likely," or "very high confidence," they’re talking 90%. BROOKS: So it’s not 100%? MILLER: In the realm of science; there’s virtually never 100% certainty about anything. You know, as someone once pointed out, gravity is a theory. BROOKS: Gravity is testable, though.. -
Zonal Harmonics of Solar Magnetic Field for Solar Cycle Forecast
Zonal harmonics of solar magnetic field for solar cycle forecast VN Obridkoa,e, DD Sokoloffa,c,d, VV Pipinb, AS Shibalovaa,c,d, IM Livshitsa aIzmiran, Kaluzhskoe Sh., 4, Troitsk, Moscow, 108840, Russia bInstitute of Solar-Terrestrial Physics, Russian Academy of Sciences, Irkutsk, 664033, Russia cDepartment of Physics, Moscow State University, 19991, Russia dMoscow Center of Fundamental and Applied Mathematics, Moscow, 119991, Russia eCentral Astronomical Observatory of the Russian Academy of Sciences at Pulkovo, St. Petersburg Abstract According to the scheme of action of the solar dynamo, the poloidal magnetic field can be considered a source of production of the toroidal magnetic field by the solar differential rotation. From the polar magnetic field proxies, it is natural to expect that solar Cycle 25 will be weak as recorded in sunspot data. We suggest that there are parameters of the zonal harmonics of the solar surface magnetic field, such as the magnitude of the l = 3 harmonic or the effective multipole index, that can be used as a reasonable addition to the polar magnetic field proxies. We discuss also some specific features of solar activity indices in Cycles 23 and 24. Keywords: Sun: magnetic fields, Sun: oscillations, sunspots 1. Introduction The problem of forecasting solar activity is a long-lasting one. Actually, this problem occurred as soon as the solar cycle was discovered, but we are still far from its definite solution. Before each sunspot maximum, forecasts of the cycle amplitude appear, but the predicted values are in quite a wide range (Obridko, 1995; Lantos and Richard, 1998). The past two Cycles, 23 and 24, were no exception. -
Trophobiosis Between Formicidae and Hemiptera (Sternorrhyncha and Auchenorrhyncha): an Overview
December, 2001 Neotropical Entomology 30(4) 501 FORUM Trophobiosis Between Formicidae and Hemiptera (Sternorrhyncha and Auchenorrhyncha): an Overview JACQUES H.C. DELABIE 1Lab. Mirmecologia, UPA Convênio CEPLAC/UESC, Centro de Pesquisas do Cacau, CEPLAC, C. postal 7, 45600-000, Itabuna, BA and Depto. Ciências Agrárias e Ambientais, Univ. Estadual de Santa Cruz, 45660-000, Ilhéus, BA, [email protected] Neotropical Entomology 30(4): 501-516 (2001) Trofobiose Entre Formicidae e Hemiptera (Sternorrhyncha e Auchenorrhyncha): Uma Visão Geral RESUMO – Fêz-se uma revisão sobre a relação conhecida como trofobiose e que ocorre de forma convergente entre formigas e diferentes grupos de Hemiptera Sternorrhyncha e Auchenorrhyncha (até então conhecidos como ‘Homoptera’). As principais características dos ‘Homoptera’ e dos Formicidae que favorecem as interações trofobióticas, tais como a excreção de honeydew por insetos sugadores, atendimento por formigas e necessidades fisiológicas dos dois grupos de insetos, são discutidas. Aspectos da sua evolução convergente são apresenta- dos. O sistema mais arcaico não é exatamente trofobiótico, as forrageadoras coletam o honeydew despejado ao acaso na folhagem por indivíduos ou grupos de ‘Homoptera’ não associados. As relações trofobióticas mais comuns são facultativas, no entanto, esta forma de mutualismo é extremamente diversificada e é responsável por numerosas adaptações fisiológicas, morfológicas ou comportamentais entre os ‘Homoptera’, em particular Sternorrhyncha. As trofobioses mais diferenciadas são verdadeiras simbioses onde as adaptações mais extremas são observadas do lado dos ‘Homoptera’. Ao mesmo tempo, as formigas mostram adaptações comportamentais que resultam de um longo período de coevolução. Considerando-se os inse- tos sugadores como principais pragas dos cultivos em nível mundial, as implicações das rela- ções trofobióticas são discutidas no contexto das comunidades de insetos em geral, focalizan- do os problemas que geram em Manejo Integrado de Pragas (MIP), em particular. -
Co-Adaptations Between Ceratocystidaceae Ambrosia Fungi and the Mycangia of Their Associated Ambrosia Beetles
Iowa State University Capstones, Theses and Graduate Theses and Dissertations Dissertations 2018 Co-adaptations between Ceratocystidaceae ambrosia fungi and the mycangia of their associated ambrosia beetles Chase Gabriel Mayers Iowa State University Follow this and additional works at: https://lib.dr.iastate.edu/etd Part of the Biodiversity Commons, Biology Commons, Developmental Biology Commons, and the Evolution Commons Recommended Citation Mayers, Chase Gabriel, "Co-adaptations between Ceratocystidaceae ambrosia fungi and the mycangia of their associated ambrosia beetles" (2018). Graduate Theses and Dissertations. 16731. https://lib.dr.iastate.edu/etd/16731 This Dissertation is brought to you for free and open access by the Iowa State University Capstones, Theses and Dissertations at Iowa State University Digital Repository. It has been accepted for inclusion in Graduate Theses and Dissertations by an authorized administrator of Iowa State University Digital Repository. For more information, please contact [email protected]. Co-adaptations between Ceratocystidaceae ambrosia fungi and the mycangia of their associated ambrosia beetles by Chase Gabriel Mayers A dissertation submitted to the graduate faculty in partial fulfillment of the requirements for the degree of DOCTOR OF PHILOSOPHY Major: Microbiology Program of Study Committee: Thomas C. Harrington, Major Professor Mark L. Gleason Larry J. Halverson Dennis V. Lavrov John D. Nason The student author, whose presentation of the scholarship herein was approved by the program of study committee, is solely responsible for the content of this dissertation. The Graduate College will ensure this dissertation is globally accessible and will not permit alterations after a degree is conferred. Iowa State University Ames, Iowa 2018 Copyright © Chase Gabriel Mayers, 2018. -
Statistical Study of Solar Activity Parameters of Solar Cycle 24
Volume 65, Issue 1, 2021 Journal of Scientific Research Institute of Science, Banaras Hindu University, Varanasi, India. Statistical Study of Solar Activity Parameters of Solar Cycle 24 Abha Singh1 and Kalpana Patel*2 1Department of Physics, T.D.P.G. College, Jaunpur-222002, U.P., India. [email protected] 2Department of Physics, SRM Institute of Science and Technology, Delhi-NCR Campus, Delhi-Meerut Road, Modinagar-201204, U.P. India. [email protected]* Abstract: The solar atmosphere is one of the most dynamic smoothed sunspot numbers that was brought into existence with environments studied in modern astrophysics. The term solar its classification (Kunzel, 1961). The number predicts short term activity refers to physical phenomena occurring within the periodic high and low activity of the Sun. The part of the cycle magnetically heated outer atmosphere of the Sun at various time with low sunspot activity is referred to as "solar minimum" scales. S un spots, high-speed solar wind, solar flares and coronal while region with maximum solar activity is called as "solar mass ejections are the basic parameters that govern maximum”. Hathaway et al. (2002) examined the ‘group’ solar activity. All solar activity is driven by the solar magnetic field. The present paper studies the relation between various solar sunspot number which shows it use in featuring the Sun’s features during solar cycle 24. The study reveals that there exists a performance during the solar year (Hoyt & Schatten, 1998a). good correlation between various parameters. This indicates that they all belong to same origin i.e., the variability of Sun’s magnetic Coronal mass ejections (CMEs) are the explosions in the solar 42field. -
Effects of Version 2 of the International Sunspot Number on Naïve
https://ntrs.nasa.gov/search.jsp?R=20190001636 2019-08-30T11:15:09+00:00Z View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by NASA Technical Reports Server Space Weather RESEARCH ARTICLE Effects of Version 2 of the International Sunspot Number on 10.1029/2018SW002080 Naïve Predictions of Solar Cycle 25 Key Points: • A new calibration of sunspot W. Dean Pesnell1 number must be used in solar cycle predictions 1Solar Physics Laboratory, NASA/Goddard Space Flight Center, Greenbelt, MD, USA • The climatological average is used to assess other predictions • Other simple predictions are not very accurate or useful Abstract The recalibration of the International Sunspot Number brings new challenges to predictions of Solar Cycle 25. One is that the list of extrema for the original series is no longer usable because the values of all maxima and minima are different for the new version of the sunspot number. Timings of extrema are Correspondence to: W. D. Pesnell, less sensitive to the recalibration but are a natural result of the calculation. Predictions of Solar Cycle 25 [email protected] published before 2016 must be converted to the new version of the sunspot number. Any prediction method that looks across the entire time span will have to be reconsidered because values in the nineteenth Citation: century were corrected by a larger factor than those in the twentieth century. We report a list of solar Pesnell, W. D. (2018). Effects of maxima and minima values and timings based on the recalibrated sunspot number. -
Homologies of the Head of Membracoidea Based on Nymphal Morphology with Notes on Other Groups of Auchenorrhyncha (Hemiptera)
Eur. J. Entomol. 107: 597–613, 2010 http://www.eje.cz/scripts/viewabstract.php?abstract=1571 ISSN 1210-5759 (print), 1802-8829 (online) Homologies of the head of Membracoidea based on nymphal morphology with notes on other groups of Auchenorrhyncha (Hemiptera) DMITRY A. DMITRIEV Illinois Natural History Survey, Institute of Natural Resource Sustainability at the University of Illinois at Urbana-Champaign, Champaign, Illinois, USA; e-mail: [email protected] Key words. Hemiptera, Membracoidea, Cicadellidae, Cicadoidea, Cercopoidea, Fulgoroidea, head, morphology, ground plan Abstract. The ground plan and comparative morphology of the nymphal head of Membracoidea are presented with particular emphasis on the position of the clypeus, frons, epistomal suture, and ecdysial line. Differences in interpretation of the head structures in Auchenorrhyncha are discussed. Membracoidea head may vary more extensively than heads in any other group of insects. It is often modified by the development of an anterior carina, which apparently was gained and lost multiple times within Membracoidea. The main modifications of the head of Membracoidea and comparison of those changes with the head of other superfamilies of Auchenorrhyncha are described. INTRODUCTION MATERIAL AND METHODS The general morphology of the insect head is relatively Dried and pinned specimens were studied under an Olympus well studied (Ferris, 1942, 1943, 1944; Cook, 1944; SZX12 microscope with SZX-DA drawing tube attachment. DuPorte, 1946; Snodgrass, 1947; Matsuda, 1965; Detailed study of internal structures and boundaries of sclerites Kukalová-Peck, 1985, 1987, 1991, 1992, 2008). There is based on examination of exuviae and specimens cleared in are also a few papers in which the hemipteran head is 5% KOH. -
Relations Between Wood-Inhabiting Insects and Fungi
RELATIONS BETWEEN WOOD-INHABITING INSECTS AND FUNGI NINA P. KRIVOSHEINA AN. Severtzov Institute of Evolutionary Animal Morphology and Ecology U.S.S.R. Academy of Sciences Moscow 117071 U.S.S.R. INTRODUCTION It is widely known that xylophagous insects do not usually attack healthy, resistant trees. In order to overcome these defenses, inner-bark feeding insects have developed symbiotic interrelationships with various organisms, fungi in particular. In this paper, using our own data together with that available in the literature, we analyze the forms of relationships between insects and fungi and the role of these interactions at various stages of wood decomposition. In doing so, we distinguish between the following fungal-insect relationships: 1) ambrosia mycetophagous insects, symbiotically associated with primary ambrosia fungi 2) ambrosia xylomycetophagous (phloeomycetophagous) insects, symbiotically associated with wood-coloring fungi (auxiliary ambrosia fungi according to Batra 1985) 3) xylophagous insects, symbiotically associated with fungi causing vascular mycoses 4) destructive xylo-, mycetophagous insects, associated with wooddestroying fungi. The representatives of the first three groups develop in living wood or fresh timber. Representatives of the last group develop in dead wood, though in the earliest stages they can colonize living, but irreversibly weakened wood. REVIEW Ambrosia Mycetophagous Insects This group includes insects which have necessary ectosymbiotic connections with a specific group of fungi imperfecti, the ambrosia fungi, and several characteristic features. The ambrosia fungi are highly sensitive to drought and develop only in moist wood. They are host specific, associated with certain species of insects, and are located only in colonized galleries or on the body of xylobionts. -
Arxiv:2005.12166V1 [Astro-Ph.SR] 25 May 2020
Draft version May 26, 2020 Typeset using LATEX modern style in AASTeX63 A model-free, data-based forecast for sunspot cycle 25 Aleix Espua-Fontcuberta,1 Saikat Chatterjee,2 Dhrubaditya Mitra,1 and Dibyendu Nandy3 1NORDITA, Royal Institute of Technology and Stockholm University, Roslagstullsbacken 23, SE-10691 Stockholm, Sweden 2School of Electrical Engg and Computer Science, KTH Royal Institute of Technology, Sweden 3Center of Excellence in Space Sciences India and Department of Physical Sciences, Indian Insitute of Science Education and Research Kolkata, Mohanpur 741246, India ABSTRACT The dynamic activity of the Sun, governed by its cycle of sunspots { strongly mag- netized regions that are observed on its surface { modulate our solar system space environment creating space weather. Severe space weather leads to disruptions in satellite operations, telecommunications, electric power grids and air-traffic on po- lar routes. Forecasting the cycle of sunspots, however, has remained a challenging problem. We use reservoir computing { a model-free, neural{network based machine- learning technique { to forecast the upcoming solar cycle, sunspot cycle 25. The standard algorithm forecasts that solar cycle 25 is going to last about ten years, the maxima is going to appear in the year 2024 and the maximum number of sunspots is going to be 113 (±15). We also develop a novel variation of the standard algorithm whose forecasts for duration and peak timing matches that of the standard algorithm, but whose peak amplitude forecast is 124 (±2) { within the upper bound of the stan- dard reservoir computing algorithm. We conclude that sunspot cycle 25 is likely to be a weak, lower than average solar cycle, somewhat similar in strength to sunspot cycle 24. -
Irina N. Kitiashvili (NASA Ames Research Center)
Global Evolution of Solar Magnetic Fields and Prediction of Solar Activity Cycles Irina N. Kitiashvili (NASA Ames Research Center) Prediction of solar activity cycles is challenging because the physical processes inside the Sun involve a broad range of multiscale dynamics that no model can reproduce, and the available observations are highly limited and cover mostly surface layers. Helioseismology makes it possible to probe solar dynamics in the convective zone, but variations in the differential rotation and meridional circulation are currently available for only two solar activity cycles. It has been demonstrated that sunspot observations, which cover over 400 years, can be used to calibrate the Parker-Kleeorin-Ruzmaikin model and that the Ensemble Kalman Filter (EnKF) method can be used to link the model magnetic fields to sunspot observations to make reliable predictions of a following cycle. However, for more accurate predictions, it is necessary to use actual observations of the solar magnetic fields, which are available for only four solar cycles. This raises the question of how limitations in observational data and model uncertainties affect predictive capabilities and implies the need for the development of new forecast methodologies and validation criteria. In this presentation, I will discuss the influence of the limited number of available observations on the accuracy of EnKF estimates of solar cycle parameters. Data Assimilation Methodology Comparison of hemispheric sunspot numbers, Test ‘Prediction’ of Solar Cycles 23 and -
Systematics and Biogeography of Leafhoppers in Madagascar
SYSTEMATICS AND BIOGEOGRAPHY OF LEAFHOPPERS IN MADAGASCAR BY SINDHU MANUBHAI KRISHNANKUTTY DISSERTATION Submitted in partial fulfillment of the requirements for the degree of Doctor of Philosophy in Entomology in the Graduate College of the University of Illinois at Urbana-Champaign, 2012 Urbana, Illinois Doctoral Committee: Dr. Christopher H. Dietrich, Illinois Natural History Survey, Chair, Director of Research Professor May Berenbaum Professor James Whitfield Dr. Steve Taylor, Illinois Natural History Survey ABSTRACT The biodiversity of Madagascar is well appreciated due to its high level of species richness and endemism. With more natural habitat being destroyed due to colonization and fulfilling essential needs of humans, presently it is considered as one of the priority hotspots for biodiversity conservation. Despite being the most diverse invertebrates in Madagascar, several insect families remain poorly known. Cicadellidae, one of the largest insect families distributed worldwide is one among them. Prior knowledge of leafhopper fauna of Madagascar is based on only five previously published taxonomic studies and very limited sampling. No attempt using phylogenetic methods has been made to understand relationships among the leafhopper genera and to test the monophyly of previously recognized endemic Malagasy taxa. Owing to their Mesozoic origin, moderate dispersal abilities, and spectacular radiation in both New and Old World tropics, leafhoppers are excellent models for biogeographic and evolutionary studies related to the origins of the Malagasy fauna. A recent terrestrial arthropod inventory project in Madagascar conducted by the California Academy of Sciences yielded >60,000 ethanol-preserved leafhopper specimens, including representatives of most previously recorded species as well as many new species. This new material provided an opportunity to examine the phylogeny and biogeography of Malagasy leafhoppers in much greater detail than ever before possible. -
The Leafhoppers and Froghoppers of Australia and New Zealand (Homoptera: Cicadelloidea and Cercopoidea)
AUSTRALIAN MUSEUM SCIENTIFIC PUBLICATIONS Evans, J. W., 1966. The leafhoppers and froghoppers of Australia and New Zealand (Homoptera: Cicadelloidea and Cercopoidea). Australian Museum Memoir 12: 1–347. [31 December 1966]. doi:10.3853/j.0067-1967.12.1966.425 ISSN 0067-1967 Published by the Australian Museum, Sydney naturenature cultureculture discover discover AustralianAustralian Museum Museum science science is is freely freely accessible accessible online online at at www.australianmuseum.net.au/publications/www.australianmuseum.net.au/publications/ 66 CollegeCollege Street,Street, SydneySydney NSWNSW 2010,2010, AustraliaAustralia THE AUSTRALIAN MUSEUM, SYDNEY MEMOIR X I I The Leafhoppers and Froghoppers of Australia and New Zealand (Hornoptera: Cicadelloidea and Cercopoidea) BY J. W. EVANS* Published by order of the Trustees Sydney, 1966 * 47 Bundarra Road, Bellevue Hill, Sydney, N.S.W., Australia G 2690-1 Registered in Australia for transmission by post as a book SYDNEY: V. C. N. BLIGHT, GOVERNMENT PRINTER, 1966 Contents Part I BIOLOGY. DISTRIBUTION AND EVOLUTION Page Introduction . 5 General characteristics . .. 7 Relationships with other Hornoptera . .. 8 Biology . .. 8 Plant associations . .. 8 The Australian fauna . 9 The New Zealand fauna . 10 The Faunas of New Guinea and New Caledonia Zoogeography . Distribution . Evolution . Abundance . Economic si-gnificance . Some research suggestions . Collecting methods and collections . Part I1 SYSTEMI~TICS Morphology . Characters distinguishing the Cicadelloidea and Cercopoidea The Families of the Cicadelloidea . Classification . Eurymelidae . Cicadellidae . Membracidae . The Families of the Cercopoidea . Cercopoidae . Aphrophoridae . Machaerotidae . Acknowledgements . List or new names . References . List of New Zealand Cicadelloidea and Cercopoidea . Index . PART I BIOLOGY, DISTRIBUTION AND EVOLUTION Introduction Although the insect faunas of Australia and New Zealand are of remarkable interest, there are very few works which deal in a comprehensive fashion with particular groups.