2020 Schedule of Events
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Midnight Sun, Part II by PA Lassiter
Midnight Sun, Part II by PA Lassiter . N.B. These chapters are based on characters created by Stephenie Meyer in Twilight, the novel. The title used here, Midnight Sun, some of the chapter titles, and all the non-interior dialogue between Edward and Bella are copyright Stephenie Meyer. The first half of Ms. Meyer’s rough-draft novel, of which this is a continuation, can be found at her website here: http://www.stepheniemeyer.com/pdf/midnightsun_partial_draft4.pdf 12. COMPLICATIONSPart B It was well after midnight when I found myself slipping through Bella’s window. This was becoming a habit that, in the light of day, I knew I should attempt to curb. But after nighttime fell and I had huntedfor though these visits might be irresponsible, I was determined they not be recklessall of my resolve quickly faded. There she lay, the sheet and blanket coiled around her restless body, her feet bound up outside the covers. I inhaled deeply through my nose, welcoming the searing pain that coursed down my throat. As always, Bella’s bedroom was warm and humid and saturated with her scent. Venom flowed into my mouth and my muscles tensed in readiness. But for what? Could I ever train my body to give up this devilish reaction to my beloved’s smell? I feared not. Cautiously, I held my breath and moved to her bedside. I untangled the bedclothes and spread them carefully over her again. She twitched suddenly, her legs scissoring as she rolled to her other side. I froze. “Edward,” she breathed. -
George Orwell in His Centenary Year a Catalan Perspective
THE ANNUAL JOAN GILI MEMORIAL LECTURE MIQUEL BERGA George Orwell in his Centenary Year A Catalan Perspective THE ANGLO-CATALAN SOCIETY 2003 © Miquel Berga i Bagué This edition: The Anglo-Catalan Society Produced and typeset by Hallamshire Publications Ltd, Porthmadog. This is the fifth in the regular series of lectures convened by The Anglo-Catalan Society, to be delivered at its annual conference, in commemoration of the figure of Joan Lluís Gili i Serra (1907-1998), founder member of the Society and Honorary Life President from 1979. The object of publication is to ensure wider diffusion, in English, for an address to the Society given by a distinguished figure of Catalan letters whose specialism coincides with an aspect of the multiple interests and achievements of Joan Gili, as scholar, bibliophile and translator. This lecture was given by Miquel Berga at Aberdare Hall, University of Wales (Cardiff), on 16 November 2002. Translation of the text of the lecture and general editing of the publication were the responsibility of Alan Yates, with the cooperation of Louise Johnson. We are grateful to Miquel Berga himself and to Iolanda Pelegrí of the Institució de les Lletres Catalanes for prompt and sympathetic collaboration. Thanks are also due to Pauline Climpson and Jenny Sayles for effective guidance throughout the editing and production stages. Grateful acknowledgement is made of regular sponsorship of The Annual Joan Gili Memorial Lectures provided by the Institució de les Lletres Catalanes, and of the grant towards publication costs received from the Fundació Congrés de Cultura Catalana. The author Miquel Berga was born in Salt (Girona) in 1952. -
Family Portrait Sessions Frequently Asked Questions Before Your Session
kiawahislandphoto.com Family Portrait Sessions Frequently Asked Questions before Your Session When you make an investment in photography, you want it to last a lifetime. Photographics has the expertise to capture the moment and the artistic style and resources to transform your images into works of art you’ll be proud to share and display. We want you to relax and enjoy the experience so all the joy and fun comes through in your portraits. If you have any concerns about your session, just give us a call or pull your photographer aside to discuss any special needs for your group. Relax, enjoy and smile. We’ve got this. Q: What should we wear? A: For outdoor photography on the beach, choose lighter tones and pastel colors for the most pleasing results. Family members don’t have to match exactly, but should stay coordinated with simple, comfortable clothing that blends with the beach environment. Avoid dark tops, busy patterns, graphics/logos, and primary colors that have a tendency to stand out and clash with the environment. Ladies, we’ll be kneeling and sitting in the sand so be wary of low necklines and short skirts. Overall…be comfortable. For great ideas visit our blog online. Q: When is the best time to take beach portraits? A: On the East Coast, the best time is the “golden hour” just before sunset when the light is softer and the temperature is more moderate. We don’t take portraits in the morning and early afternoon hours, because the sun on the beach is too intense which causes harsh shadows and squinting. -
Exploring Solar Cycle Influences on Polar Plasma Convection
Comparison of Terrestrial and Martian TEC at Dawn and Dusk during Solstices Angeline G. Burrell1 Beatriz Sanchez-Cano2, Mark Lester2, Russell Stoneback1, Olivier Witasse3, Marco Cartacci4 1Center for Space Sciences, University of Texas at Dallas 2Radio and Space Plasma Physics, University of Leicester 3European Space Agency, ESTEC – Scientific Support Office 4Istituto Nazionale di Astrofisica, Istituto di Astrofisica e Planetologia Spaziali 52nd ESLAB Symposium Outline • Motivation • Data and analysis – TEC sources – Data selection – Linear fitting • Results – Martian variations – Terrestrial variations – Similarities and differences • Conclusions Motivation • The Earth and Mars are arguably the most similar of the solar planets - They are both inner, rocky planets - They have similar axial tilts - They both have ionospheres that are formed primarily through EUV and X- ray radiation • Planetary differences can provide physical insights Total Electron Content (TEC) • The Global Positioning System • The Mars Advanced Radar for (GPS) measures TEC globally Subsurface and Ionosphere using a network of satellites and Sounding (MARSIS) measures ground receivers the TEC between the Martian • MIT Haystack provides calibrated surface and Mars Express TEC measurements • Mars Express has an inclination - Available from 1999 onward of 86.9˚ and a period of 7h, - Includes all open ground and allowing observations of all space-based sources locations and times - Specified with a 1˚ latitude by 1˚ • TEC is available for solar zenith longitude resolution with error estimates angles (SZA) greater than 75˚ Picardi and Sorge (2000), In: Proc. SPIE. Eighth International Rideout and Coster (2006) doi:10.1007/s10291-006-0029-5, 2006. Conference on Ground Penetrating Radar, vol. 4084, pp. 624–629. -
Solar Cycle, Seasonal, and Diurnal Variations of the Mars Upper
JournalofGeophysicalResearch: Planets RESEARCH ARTICLE Mars Global Ionosphere-Thermosphere Model: 10.1002/2014JE004715 Solar cycle, seasonal, and diurnal variations Key Points: of the Mars upper atmosphere • The Mars Global 1 2 3 4 5 6 Ionosphere-Thermosphere Model S. W. Bougher ,D.Pawlowski ,J.M.Bell , S. Nelli , T. McDunn , J. R. Murphy , (MGITM) is presented and validated M. Chizek6, and A. Ridley1 • MGITM captures solar cycle, seasonal, and diurnal trends observed above 1Atmospheric, Oceanic, and Space Sciences Department, University of Michigan, Ann Arbor, Michigan, USA, 2Physics 100 km 3 • MGITM variations will be compared Department, Eastern Michigan University, Ypsilanti, Michigan, USA, National Institute of Aerospace, Hampton, Virginia, 4 5 6 to key episodic variations in USA, Harris, ITS, Las Cruces, New Mexico, USA, Jet Propulsion Laboratory, Pasadena, California, USA, Astronomy future studies Department, New Mexico State University, Las Cruces, New Mexico, USA Correspondence to: S. W. Bougher, Abstract A new Mars Global Ionosphere-Thermosphere Model (M-GITM) is presented that combines [email protected] the terrestrial GITM framework with Mars fundamental physical parameters, ion-neutral chemistry, and key radiative processes in order to capture the basic observed features of the thermal, compositional, and Citation: dynamical structure of the Mars atmosphere from the ground to the exosphere (0–250 km). Lower, middle, Bougher, S. W., D. Pawlowski, and upper atmosphere processes are included, based in part upon formulations used in previous lower and J. M. Bell, S. Nelli, T. McDunn, upper atmosphere Mars GCMs. This enables the M-GITM code to be run for various seasonal, solar cycle, and J. R. -
Riverboat Twilight Paddlewheeler Cruise 4 Days / 3 Nights Departure Dates: Aug
Riverboat Twilight Paddlewheeler Cruise 4 Days / 3 Nights Departure Dates: Aug. 23-26; Oct. 18-21 Tour Code: RVTx91 DAY ONE — D Return with us to a simpler time when steamboats and paddle wheelers ruled the Mississippi River. We make our way through Wisconsin enroute to the small river town of Le Claire, IA. First we tour the Isabel Bloom Studio to see how this company maintains the legacy of artist Isabel Bloom. She has created thousands of delightful garden sculptures for retailers throughout the country and we have the opportunity for a behind-the- scenes tour. This evening we enjoy a welcome dinner at a local eatery before turning in for the night at the Holiday Inn Express. DAY TWO — B, L, D Board the Riverboat Twilight for our two day excursion up the Mississippi River. A continental breakfast awaits you upon boarding. Lunch and dinner meals will be served to you by the friendly crew at your reserved table. Beautiful scenery, activities and relaxation are all for you to enjoy as the boat winds its way upstream. From shallow marshes teaming with wildlife to palisades and high cliffs pass as we approach mining country. The Captain will point out sights of interest along the way and explain “locking through” procedures as we negotiate locks and dams. Showtime each afternoon features folk musicians, humorists and perhaps an appearance by Mark Twain himself! Browse the gift shop or enjoy your favorite cocktail at the bar. Ending day one of our cruise we check into the Grand Harbor Resort on the banks of the river in Dubuque, IA for a well deserved rest tonight. -
Daily Wind Changes in the Lower Levels of the Atmosphere
NOAA’s National Weather Service February 2014 Daily Wind Changes in the Lower Inside Levels of the Atmosphere General Aviation: Identify and Jeff Halblaub, Meteorologist, NWS Hastings, NE Communicate Hazardous Weather On most days, winds change substantially between the surface 3 and the lowest few thousand feet above ground level (AGL). These changes are part of the daily cycle driven by the sun. The atmosphere behaves like a fluid. The layer of fluid in contact with an underlying surface is called the boundary layer. The atmospheric boundary layer When’s the Next moves through a daily cycle based on heat from the sun. Front? This cycle of daytime heating and nighttime cooling explains why, under most circumstances, higher winds are confined above the surface Would you like an email at night. As low-level temperatures warm during the morning hours, when a new edition of those higher winds gradually drop down to the surface, resulting in The Front is online? Email daytime gustiness. [email protected]. A well-mixed boundary layer results in substantial turbulence. This Your subject line for the turbulence is magnified when cumulus clouds form posing challenges email should be “Subscribe to Visual Flight Rules (VFR) operation. When flying above the boundary to The Front.” layer, which is generally much smoother, there is an abrupt increase in turbulence during descent into the boundary layer. This turbulence continues down to the runway. Pilots frequently must deal with daytime gustiness during takeoffs and landings. These gusty surface winds usually begin in the late morning hours, peak in the afternoon, and end by early evening. -
Solar Wind Fluence to the Lunar Surface
44th Lunar and Planetary Science Conference (2013) 2015.pdf SOLAR WIND FLUENCE TO THE LUNAR SURFACE. D. M. Hurley1,3, W. M. Farrell2,3, 1JHU Applied Phys- ics Laboratory ([email protected]), 2NASA Goddard Space Flight Center, 3NASA Lunar Science Institute. Monolayers delivered in one lunation Introduction: The unperturbed solar wind bom- 90 bards the dayside of the Moon with electrons, protons, 60 and heavier ions throughout most of a lunation. Ex- cept when the Moon is in the Earth’s magnetotail for a 30 few days each lunation, the solar wind (shocked solar 0 N. Latitude wind in the magnetosheath, and unshocked solar wind -30 beyond Earth’s bow shock) has access to the dayside -60 surface of the Moon. Investigations of how the solar -90 wind could contribute to the composition and optical 0 90 180 270 360 properties of the lunar surface have a long history (e.g. E. Longitude [1-7]. Yet, it is instructive to revisit this issue and ex- Figure 2. The solar wind proton fluence as a function of amine the solar wind interaction piece by piece. selenographic position is shown in terms of fractions of Delivered Flux: The upper limit on the solar wind an equivalent monolayer of OH. The solid lines neglect thermal effects while the dashed lines include thermal as a potential source of OH can be established by as- effects. suming all of the incident solar wind protons are re- tained in the lunar regolith. The quiescent solar wind is implanted 3He as a resource guide. Fig. 2 shows the variable, but has density, n, of ~5 p+cm-3 and velocity, calculated fluence for one lunation assuming a spheri- v, of ~350 km s-1. -
Understanding Golden Hour, Blue Hour and Twilights
Understanding Golden Hour, Blue Hour and Twilights www.photopills.com Mark Gee proves everyone can take contagious images 1 Feel free to share this ebook © PhotoPills April 2017 Never Stop Learning The Definitive Guide to Shooting Hypnotic Star Trails How To Shoot Truly Contagious Milky Way Pictures A Guide to the Best Meteor Showers in 2017: When, Where and How to Shoot Them 7 Tips to Make the Next Supermoon Shine in Your Photos MORE TUTORIALS AT PHOTOPILLS.COM/ACADEMY Understanding How To Plan the Azimuth and Milky Way Using Elevation The Augmented Reality How to find How To Plan The moonrises and Next Full Moon moonsets PhotoPills Awards Get your photos featured and win $6,600 in cash prizes Learn more+ Join PhotoPillers from around the world for a 7 fun-filled days of learning and adventure in the island of light! Learn More We all know that light is the crucial element in photography. Understanding how it behaves and the factors that influence it is mandatory. For sunlight, we can distinguish the following light phases depending on the elevation of the sun: golden hour, blue hour, twilights, daytime and nighttime. Starting time and duration of these light phases depend on the location you are. This is why it is so important to thoughtfully plan for a right timing when your travel abroad. Predicting them is compulsory in travel photography. Also, by knowing when each phase occurs and its light conditions, you will be able to assess what type of photography will be most suitable for each moment. Understanding Golden Hour, Blue Hour and Twilights 6 “In almost all photography it’s the quality of light that makes or breaks the shot. -
Venus Cloud Morphology and Motions from Ground-Based Images at the Time of the Akatsuki Orbit Insertion
1 Venus cloud morphology and motions from ground-based images at the time of the Akatsuki orbit insertion A. Sánchez-Lavega1, J. Peralta2, J. M. Gomez-Forrellad3, R. Hueso1, S. Pérez-Hoyos1, I. Mendikoa1, J. F. Rojas1, T. Horinouchi4, Y. J. Lee2, S. Watanabe5 1Departamento de Física Aplicada I, Escuela de Ingeniería de Bilbao, Universidad del País Vasco UPV /EHU, Plaza Ingeniero Torres Quevedo, 48013 Bilbao, Spain. 2Institute of Space and Astronautical Science (ISAS/JAXA), Sagamihara, Kanagawa, Japan. 3Fundació Observatori Esteve Duran, Montseny 46, 08553 Seva, Barcelona, Spain. 4Faculty of Environment Earth Science, Hokkaido University, Hokkaido, Japan 5Department of Cosmoscience, Hokkaido University, Hokkaido, Japan *To whom correspondence should be addressed. E-mail: [email protected] † Partially based on observations obtained at Centro Astronómico Hispano Alemán, Observatorio de Calar Alto MPIA-CSIC, Almería, Spain. 2 Abstract We report Venus image observations around the two maximum elongations of the planet at June and October 2015. From these images we describe the global atmospheric dynamics and cloud morphology in the planet before the arrival of JAXA’s Akatsuki mission on December the 7th. The majority of the images were acquired at ultraviolet wavelengths (380-410 nm) using small telescopes. The Venus dayside was also observed with narrow band filters at other wavelengths (890 nm, 725-950 nm, 1.435 μm CO2 band) using the instrument PlanetCam-UPV/EHU at the 2.2m telescope in Calar Alto Observatory. In all cases, the lucky imaging methodology was used to improve the spatial resolution of the images over the atmospheric seeing. During the April-June period, the morphology of the upper cloud showed an irregular and chaotic texture with a well developed equatorial dark belt (afternoon hemisphere), whereas during October- December the dynamical regime was dominated by planetary-scale waves (Y- horizontal, C-reversed and ψ-horizontal features) formed by long streaks, and banding suggesting more stable conditions. -
Dawn-Dusk Asymmetries in Rotating Magnetospheres
Dawn-dusk Asymmetries in Rotating Magnetospheres: Lessons from Modeling Saturn Xianzhe Jia1,* and Margaret G. Kivelson1,2 (Email: [email protected]) 1. Department of Climate and Space Sciences and Engineering, University of Michigan, Ann Arbor, MI 48109 2. Department of Earth, Planetary, and Space Sciences, University of California, Los Angeles, CA 90095 This is the author manuscript accepted for publication and has undergone full peer review but has not been through the copyediting, typesetting, pagination and proofreading process, which may lead to differences between this version and the Version of Record. Please cite this article as doi: 10.1002/2015JA021950 1 This article is protected by copyright. All rights reserved. Manuscript submitted to Journal of Geophysical Research – Space Physics 2 This article is protected by copyright. All rights reserved. Abstract Spacecraft measurements reveal perplexing dawn-dusk asymmetries of field and plasma properties in the magnetospheres of Saturn and Jupiter. Here we describe a previously unrecognized source of dawn-dusk asymmetry in a rapidly rotating magnetosphere. We analyze two magnetohydrodynamic simulations, focusing on how flows along and across the field vary with local time in Saturn’s dayside magnetosphere. As plasma rotates from dawn to noon on a dipolarizing flux tube, it flows away from the equator along the flux tube at roughly half of the sound speed (Cs), the maximum speed at which a bulk plasma can flow along a flux tube into a lower pressure region. As plasma rotates from noon to dusk on a stretching flux tube, the field- aligned component of its centripetal acceleration decreases and it flows back towards the equator at speeds typically smaller than s. -
October '18 Newsletter
Upper Blue Mountains Camera Club Inc. Newsletter A camera is a tool for learning how to see without a camera. Dorthea Lange egardless of who you are as a time of day just after sunrise and again hour can make all the difference to your are ideal for capturing golden hour R photographer, or how long you’ve just before sunset, the sun is much lower landscape images. images; as the window for shooting will be been shooting – there’s a good chance in the sky, resulting in softer, more gentle With this in mind, we’ll take a look at a few longer than it would be during the shorter that you’ve heard the term “golden hour” lighting. This is a great time of day to aspects of the golden hour photography, days of winter. It’s also weather-dependent before – maybe you’ve even taken shots capture landscapes – ones that feature the and see how we can get the most from this – a clear day with just a few clouds is ideal, during this time of day. entire world awash in a beautiful glow. beautiful time of day. while overcast weather will block the light. In the photography world, the golden The right lighting can make a difference It’s worth noting that golden hour doesn’t In the continuing article, we’ll take a look at hour is considered to be one of the best between an everyday image, and one happen every day – it’s something that’s some of those aspects for making the most times of day to take photos – whether that’s truly spectacular, and timing your very much weather-dependent.