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Midwest Vegetable Production Guide for Commercial Growers
Midwest Vegetable Production Guide for Commercial Growers 2019 Illinois University of Illinois Extension C1373-19 Indiana Purdue Extension ID-56 Iowa Iowa State University Extension and Outreach FG 0600 Kansas Kansas State University Research and Extension MF3279 Michigan Michigan State University Extension E0312 Minnesota University of Minnesota Extension BU-07094-S Missouri University of Missouri Extension MX384 Lincoln University of Missouri Cooperative Extension and Research LUCER 01-2019 Ohio Ohio State University Extension Bulletin 948 Stay Current For the most up-to-date version of this publication, visit: mwveguide.org Changes will be made throughout the year as they are received. Abbreviations Used in This Guide PHI pre-harvest interval — the minimum allowable time in days between the latest pesticide application and crop harvest AI active ingredient COC crop oil concentrate D dust formulation DF, DG dry flowable or water dispersible granule formulation E, EC emulsifiable concentrate F flowable formulation G granular formulation L, LC liquid concentrate formulation NIS nonionic surfactant REI re-entry interval RUP restricted use pesticide SC suspension concentrate W, WP wettable powder formulation Cover photo: Although a large proportion of broccoli Americans consume is produced in the western U.S, many Midwestern vegetable growers have been able to find local or regional markets for this crop. Health benefits include a high fiber content, vitamin C, vitamin K, iron and potassium. See the Cole Crops and Brassica Leafy Greens section, page 103. Insect, disease, and weed control recommendations in this publication are valid only for 2019. If registration for any of the chemicals suggested is changed during the year since the time of publication (December 2018), we will inform all area and county Extension staff. -
Snap Pea Salad Cream of Asparagus Soup
Snap Pea Salad Cream of Asparagus Soup Serves 4. Serves 4. Ingredients: Ingredients: Lemon vinaigrette (recipe follows) 2 pounds asparagus 1 pound sugar snap peas, trimmed and strings 1 Tablespoon butter removed 1 medium onion 3 ounces spring greens 4 cups reduced sodium chicken broth 2 Tablespoons low fat sour cream or yogurt Lemon Vinaigrette: Salt and pepper, to taste 3 Tablespoons olive oil 3 Tablespoons lemon Directions: juice, preferably fresh 1 teaspoon fresh or ½ 1. Wash asparagus. Remove tough ends. Cut teaspoon dried oregano in half. 1 garlic clove, minced 2. Melt butter in a large saucepan. Add onion and cook until soft, about 2 minutes. Directions: 3. Add asparagus and chicken stock to saucepan. Bring to a boil, cover and cook on 1. Lemon Vinaigrette: In a small jar or bowl, low for about 20 minutes or until tender. combine all ingredients. Cover and set Remove from heat. Using either a blender or aside. This can be made one day in immersion blender, puree until smooth. advance. Refrigerate until ready to use. 4. Top each serving with one teaspoon of sour 2. Wash and trim the peas. Slice in half on the cream or yogurt. diagonal. Set aside. Wash and dry greens. 3. Fill a 2-quart sauce pan half-full with water. Note: If using a blender, you will need to blend in Cover and bring to a boil. two batches. Since hot liquids expand, hold a 4. Add beans and blanch for 2 minutes. Drain. towel over the blender. Cover in cold water. Drain. 5. Stir together the vinaigrette. -
Tentative Lists Submitted by States Parties As of 15 April 2021, in Conformity with the Operational Guidelines
World Heritage 44 COM WHC/21/44.COM/8A Paris, 4 June 2021 Original: English UNITED NATIONS EDUCATIONAL, SCIENTIFIC AND CULTURAL ORGANIZATION CONVENTION CONCERNING THE PROTECTION OF THE WORLD CULTURAL AND NATURAL HERITAGE WORLD HERITAGE COMMITTEE Extended forty-fourth session Fuzhou (China) / Online meeting 16 – 31 July 2021 Item 8 of the Provisional Agenda: Establishment of the World Heritage List and of the List of World Heritage in Danger 8A. Tentative Lists submitted by States Parties as of 15 April 2021, in conformity with the Operational Guidelines SUMMARY This document presents the Tentative Lists of all States Parties submitted in conformity with the Operational Guidelines as of 15 April 2021. • Annex 1 presents a full list of States Parties indicating the date of the most recent Tentative List submission. • Annex 2 presents new Tentative Lists (or additions to Tentative Lists) submitted by States Parties since 16 April 2019. • Annex 3 presents a list of all sites included in the Tentative Lists of the States Parties to the Convention, in alphabetical order. Draft Decision: 44 COM 8A, see point II I. EXAMINATION OF TENTATIVE LISTS 1. The World Heritage Convention provides that each State Party to the Convention shall submit to the World Heritage Committee an inventory of the cultural and natural sites situated within its territory, which it considers suitable for inscription on the World Heritage List, and which it intends to nominate during the following five to ten years. Over the years, the Committee has repeatedly confirmed the importance of these Lists, also known as Tentative Lists, for planning purposes, comparative analyses of nominations and for facilitating the undertaking of global and thematic studies. -
IN-SITU RADIOMETRIC AGE DETERMINATION: a CRITICAL COMPONENT of MARS EXPLORATION. J. B. Plescia1 and T. D. Swindle2, 1Applied
Seventh International Conference on Mars 3278.pdf IN-SITU RADIOMETRIC AGE DETERMINATION: A CRITICAL COMPONENT OF MARS EXPLORATION. J. B. Plescia1 and T. D. Swindle2, 1Applied Physics Laboratory, Johns Hopkins University, 11100 Johns Hopkins Road, Laurel, MD 20723, [email protected]. 2Department of Planetary Sciences, Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ 85721, [email protected]. Introduction: In order to understand the geologic, Bombardment [12-18], although this remains a contro- climatic and possibly the biologic evolution of Mars, versial topic. It has also been suggested that the crater- the absolute timing of events must be established. ing rate over the last several billion years has not been Questions of climate change, glacial processes, avail- uniform, but rather has been punctuated by periodic ability of surface water, recent volcanism, and atmos- spikes in the rate [19-20]. pheric evolution all hinge on determining when those events occurred in absolute time. Resolving the abso- lute timing of events has become even more critical with the suggestions of currently active glacial and perhaps fluvial activity and very young volcanic activ- ity. Background: To date, only the relative chronology of events has been firmly established [1]. This has been accomplished through the use of impact crater counts in which the frequency of impact craters per unit area greater than or equal to some diameter is used as a reference for comparison among surfaces; the higher the frequency, the older the age [2-3]. This technique allows surfaces and events on different parts of a planet to be correlated in time. -
Martian Crater Morphology
ANALYSIS OF THE DEPTH-DIAMETER RELATIONSHIP OF MARTIAN CRATERS A Capstone Experience Thesis Presented by Jared Howenstine Completion Date: May 2006 Approved By: Professor M. Darby Dyar, Astronomy Professor Christopher Condit, Geology Professor Judith Young, Astronomy Abstract Title: Analysis of the Depth-Diameter Relationship of Martian Craters Author: Jared Howenstine, Astronomy Approved By: Judith Young, Astronomy Approved By: M. Darby Dyar, Astronomy Approved By: Christopher Condit, Geology CE Type: Departmental Honors Project Using a gridded version of maritan topography with the computer program Gridview, this project studied the depth-diameter relationship of martian impact craters. The work encompasses 361 profiles of impacts with diameters larger than 15 kilometers and is a continuation of work that was started at the Lunar and Planetary Institute in Houston, Texas under the guidance of Dr. Walter S. Keifer. Using the most ‘pristine,’ or deepest craters in the data a depth-diameter relationship was determined: d = 0.610D 0.327 , where d is the depth of the crater and D is the diameter of the crater, both in kilometers. This relationship can then be used to estimate the theoretical depth of any impact radius, and therefore can be used to estimate the pristine shape of the crater. With a depth-diameter ratio for a particular crater, the measured depth can then be compared to this theoretical value and an estimate of the amount of material within the crater, or fill, can then be calculated. The data includes 140 named impact craters, 3 basins, and 218 other impacts. The named data encompasses all named impact structures of greater than 100 kilometers in diameter. -
North Dakota Department of Agriculture $2605577.54 (Pdf)
FY15 Specialty Crop Block Grant Program- Farm Bill North Dakota Department of Agriculture Final Performance Report USDA Agreement # 15-SCBGP-ND-0026 CONTACT: Deanna Gierszewski, Specialty Crop Grant Administrator 600 E Boulevard Ave #602 Bismarck, ND 58505-0020 Phone: (701) 328-2191 Email: [email protected] Submitted: November 16, 2018 Resubmitted: January 29, 2019 Table of Contents: 1. Enhancing the Safe Use of Specialty Fruit and Vegetable Crops from Field to Table .......3 2. Development of improved fungicide application strategies for managing Sclerotinia head rot in confection sunflowers...............................................................................................10 3. Pea and Lentil Market Analysis .........................................................................................14 4. Optimizing agronomic practices for faba bean production in North Dakota.....................17 5. Optimizing fungicide application strategies for improved management of Sclerotinia in dry edible beans .................................................................................................................21 6. Enhancing Tree Selection and Evaluating Tree Species in Western North Dakota ..........26 7. State-wide screening of green foxtail for herbicide resistance ..........................................32 8. Identification of Pathogen, Soil and Plant Factors Important to Root Rot Development in Field Pea.............................................................................................................................35 -
11 Fall Unamagazine
FALL 2011 • VOLUME 19 • No. 3 FOR ALUMNI AND FRIENDS OF THE UNIVERSITY OF NORTH ALABAMA Cover Story 10 ..... Thanks a Million, Harvey Robbins Features 3 ..... The Transition 14 ..... From Zero to Infinity 16 ..... Something Special 20 ..... The Sounds of the Pride 28 ..... Southern Laughs 30 ..... Academic Affairs Awards 33 ..... Excellence in Teaching Award 34 ..... China 38 ..... Words on the Breeze Departments 2 ..... President’s Message 6 ..... Around the Campus 45 ..... Class Notes 47 ..... In Memory FALL 2011 • VOLUME 19 • No. 3 for alumni and friends of the University of North Alabama president’s message ADMINISTRATION William G. Cale, Jr. President William G. Cale, Jr. The annual everyone to attend one of these. You may Vice President for Academic Affairs/Provost Handy festival contact Dr. Alan Medders (Vice President John Thornell is drawing large for Advancement, [email protected]) Vice President for Business and Financial Affairs crowds to the many or Mr. Mark Linder (Director of Athletics, Steve Smith venues where music [email protected]) for information or to Vice President for Student Affairs is being played. At arrange a meeting for your group. David Shields this time of year Sometimes we measure success by Vice President for University Advancement William G. Cale, Jr. it is impossible the things we can see, like a new building. Alan Medders to go anywhere More often, though, success happens one Vice Provost for International Affairs in town and not hear music. The festival student at a time as we provide more and Chunsheng Zhang is also a reminder that we are less than better educational opportunities. -
Widespread Crater-Related Pitted Materials on Mars: Further Evidence for the Role of Target Volatiles During the Impact Process ⇑ Livio L
Icarus 220 (2012) 348–368 Contents lists available at SciVerse ScienceDirect Icarus journal homepage: www.elsevier.com/locate/icarus Widespread crater-related pitted materials on Mars: Further evidence for the role of target volatiles during the impact process ⇑ Livio L. Tornabene a, , Gordon R. Osinski a, Alfred S. McEwen b, Joseph M. Boyce c, Veronica J. Bray b, Christy M. Caudill b, John A. Grant d, Christopher W. Hamilton e, Sarah Mattson b, Peter J. Mouginis-Mark c a University of Western Ontario, Centre for Planetary Science and Exploration, Earth Sciences, London, ON, Canada N6A 5B7 b University of Arizona, Lunar and Planetary Lab, Tucson, AZ 85721-0092, USA c University of Hawai’i, Hawai’i Institute of Geophysics and Planetology, Ma¯noa, HI 96822, USA d Smithsonian Institution, Center for Earth and Planetary Studies, Washington, DC 20013-7012, USA e NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA article info abstract Article history: Recently acquired high-resolution images of martian impact craters provide further evidence for the Received 28 August 2011 interaction between subsurface volatiles and the impact cratering process. A densely pitted crater-related Revised 29 April 2012 unit has been identified in images of 204 craters from the Mars Reconnaissance Orbiter. This sample of Accepted 9 May 2012 craters are nearly equally distributed between the two hemispheres, spanning from 53°Sto62°N latitude. Available online 24 May 2012 They range in diameter from 1 to 150 km, and are found at elevations between À5.5 to +5.2 km relative to the martian datum. The pits are polygonal to quasi-circular depressions that often occur in dense clus- Keywords: ters and range in size from 10 m to as large as 3 km. -
Seed Catalog V3
Stillwater Valley Farm Seedlisting 2021 Hello and welcome to my third annual attempt at a descriptive catalog/formal seedlisting! In the past I have only used namelistings of seed, expecting that buyers do their own homework – but it is my hope that the descriptions on these pages will be of assistance, especially to those who may simply be curious. The purpose of this first page is to establish background and “ground rules”. I have always been a “farmer” ever since chewing down dirty carrots in my dad‟s garden, though I entered into seedkeeping after college. My beliefs and educational background established indigenous causes as something close to my heart, and beyond my basic self-sufficiency desires, the connection I feel to my seed is spiritual. It is something I take extremely seriously. I am not in this for profit; I am in this as “heart work” and a calling. I am a lone, economically challenged grower and I process and ship all of my seed by hand with no help. Therefore, I do not have a system for „buy it now‟ seeds and everything here is subject to my own whims and is only based on what I personally grow and provide. If you wish to obtain samples, these details will explain how. I understand they are long, but I ask you to read and respect them all. Informationals: – Varieties are offered in small quantities. I cannot provide poundage; please don‟t ask. A normal distribution of corn is approx. 200 seeds. A normal bean distribution is 20-30. -
The Quality of Leguminous Vegetables As Influenced by Preharvest Factors
Scientia Horticulturae 232 (2018) 191–205 Contents lists available at ScienceDirect Scientia Horticulturae journal homepage: www.elsevier.com/locate/scihorti The quality of leguminous vegetables as influenced by preharvest factors T Georgia Ntatsia, Marcos Egea Gutiérrez-Cortinesb, Ioannis Karapanosa, Ana Barrosc, Julia Weissb, ⁎ Astrit Balliud, Eduardo Augusto dos Santos Rosac, Dimitrios Savvasa, a Agricultural University of Athens, Faculty of Plant Sciences, Iera Odos 75, 11855 Athens, Greece b Universidad Politécnica de Cartagena, Instituto de Biotecnología Vegetal, 30202 Cartagena, Spain c Centre for the Research and Technology of Agro-Environmental and Biological Sciences, University of Trás-os-Montes e Alto Douro, (CITAB-UTAD), Quinta de Prados, 5000-801 Vila Real, Portugal d Agricultural University of Tirana, Department of Horticultural & Landscape Architecture, Koder Kamez 1029, Tirana, Albania ARTICLE INFO ABSTRACT Keywords: The cultivation of most legumes, aims to the production of either dry seeds consumed by humans, also known as Chemical composition pulses, or animal fodder. However, some legumes are cultivated for fresh consumption either as pods or as Human health immature seeds. The economically most important legumes consumed as vegetables are green pods of common Legume bean, cowpea, faba bean, snow pea (mangetout) and green pea seeds. As a rule, the legume vegetables are Morphological traits consumed after cooking and in many countries, they may be used to cover primary nutritional needs, because Nutritive value their protein content is high in comparison with most other vegetables. Furthermore, the legume vegetables, Quality Vegetable which have distinct organoleptic properties when compared to pulses, are also considered important sources of carbohydrates, essential minerals, vitamins, several other antioxidants and health promoting compounds, and dietary fiber. -
Martian Subsurface Properties and Crater Formation Processes Inferred from Fresh Impact Crater Geometries
Martian Subsurface Properties and Crater Formation Processes Inferred From Fresh Impact Crater Geometries The Harvard community has made this article openly available. Please share how this access benefits you. Your story matters Citation Stewart, Sarah T., and Gregory J. Valiant. 2006. Martian subsurface properties and crater formation processes inferred from fresh impact crater geometries. Meteoritics and Planetary Sciences 41: 1509-1537. Published Version http://meteoritics.org/ Citable link http://nrs.harvard.edu/urn-3:HUL.InstRepos:4727301 Terms of Use This article was downloaded from Harvard University’s DASH repository, and is made available under the terms and conditions applicable to Other Posted Material, as set forth at http:// nrs.harvard.edu/urn-3:HUL.InstRepos:dash.current.terms-of- use#LAA Meteoritics & Planetary Science 41, Nr 10, 1509–1537 (2006) Abstract available online at http://meteoritics.org Martian subsurface properties and crater formation processes inferred from fresh impact crater geometries Sarah T. STEWART* and Gregory J. VALIANT Department of Earth and Planetary Sciences, Harvard University, 20 Oxford Street, Cambridge, Massachusetts 02138, USA *Corresponding author. E-mail: [email protected] (Received 22 October 2005; revision accepted 30 June 2006) Abstract–The geometry of simple impact craters reflects the properties of the target materials, and the diverse range of fluidized morphologies observed in Martian ejecta blankets are controlled by the near-surface composition and the climate at the time of impact. Using the Mars Orbiter Laser Altimeter (MOLA) data set, quantitative information about the strength of the upper crust and the dynamics of Martian ejecta blankets may be derived from crater geometry measurements. -
Orbital Evidence for More Widespread Carbonate- 10.1002/2015JE004972 Bearing Rocks on Mars Key Point: James J
PUBLICATIONS Journal of Geophysical Research: Planets RESEARCH ARTICLE Orbital evidence for more widespread carbonate- 10.1002/2015JE004972 bearing rocks on Mars Key Point: James J. Wray1, Scott L. Murchie2, Janice L. Bishop3, Bethany L. Ehlmann4, Ralph E. Milliken5, • Carbonates coexist with phyllosili- 1 2 6 cates in exhumed Noachian rocks in Mary Beth Wilhelm , Kimberly D. Seelos , and Matthew Chojnacki several regions of Mars 1School of Earth and Atmospheric Sciences, Georgia Institute of Technology, Atlanta, Georgia, USA, 2The Johns Hopkins University/Applied Physics Laboratory, Laurel, Maryland, USA, 3SETI Institute, Mountain View, California, USA, 4Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, California, USA, 5Department of Geological Sciences, Brown Correspondence to: University, Providence, Rhode Island, USA, 6Lunar and Planetary Laboratory, University of Arizona, Tucson, Arizona, USA J. J. Wray, [email protected] Abstract Carbonates are key minerals for understanding ancient Martian environments because they Citation: are indicators of potentially habitable, neutral-to-alkaline water and may be an important reservoir for Wray, J. J., S. L. Murchie, J. L. Bishop, paleoatmospheric CO2. Previous remote sensing studies have identified mostly Mg-rich carbonates, both in B. L. Ehlmann, R. E. Milliken, M. B. Wilhelm, Martian dust and in a Late Noachian rock unit circumferential to the Isidis basin. Here we report evidence for older K. D. Seelos, and M. Chojnacki (2016), Orbital evidence for more widespread Fe- and/or Ca-rich carbonates exposed from the subsurface by impact craters and troughs. These carbonates carbonate-bearing rocks on Mars, are found in and around the Huygens basin northwest of Hellas, in western Noachis Terra between the Argyre – J.