The Cycle of Daytime and Nighttime
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Starry Starry Night Part 1
Starry Starry Night Part 1 DO NOT WRITE ON THIS PORTION OF THE TEST 1. If a lunar eclipse occurs tonight, when is the soonest a solar eclipse can occur? A) Tomorrow B) In two weeks C) In six months D) In one year 2. The visible surface of the Sun is called its A) corona B) photosphere C) chromosphere D) atmosphere 3. Which moon in the Solar System has lakes and rivers on it: A) Triton B) Charon C) Titan D) Europa 4. The sixth planet from the Sun is: A) Mars B) Jupiter C) Saturn D) Uranus 5. The orbits of the planets and dwarf planets around the Sun are in the shape of: A) An eclipse B) A circle C) An ellipse D) None of the above 6. True or False: During the summer and winter solstices, nighttime and daytime are of equal length. 7. The diameter of the observable universe is estimated to be A) 93 billion miles B) 93 billion astronomical units C) 93 billion light years D) 93 trillion miles 8. Asteroids in the same orbit as Jupiter -- in front and behind it -- are called: A) Greeks B) Centaurs C) Trojans D) Kuiper Belt Objects 9. Saturn's rings are made mostly of: A) Methane ice B) Water ice C) Ammonia ice D) Ice cream 10. The highest volcano in the Solar System is on: A) Earth B) Venus C) Mars D) Io 11. The area in the Solar System just beyond the orbit of Neptune populated by icy bodies is called A) The asteroid belt B) The Oort cloud C) The Kuiper Belt D) None of the above 12. -
Conspicuity of High-Visibility Safety Apparel During Civil Twilight
UMTRI-2006-13 JUNE 2006 CONSPICUITY OF HIGH-VISIBILITY SAFETY APPAREL DURING CIVIL TWILIGHT JAMES R. SAYER MARY LYNN MEFFORD CONSPICUITY OF HIGH-VISIBILITY SAFETY APPAREL DURING CIVIL TWILIGHT James R. Sayer Mary Lynn Mefford The University of Michigan Transportation Research Institute Ann Arbor, MI 48109-2150 U.S.A. Report No. UMTRI-2006-13 June 2006 Technical Report Documentation Page 1. Report No. 2. Government Accession No. 3. Recipient’s Catalog No. UMTRI-2006-13 4. Title and Subtitle 5. Report Date Conspicuity of High-Visibility Safety Apparel During Civil June 2006 Twilight 6. Performing Organization Code 302753 7. Author(s) 8. Performing Organization Report No. Sayer, J.R. and Mefford, M.L. UMTRI-2006-13 9. Performing Organization Name and Address 10. Work Unit no. (TRAIS) The University of Michigan Transportation Research Institute 11. Contract or Grant No. 2901 Baxter Road Ann Arbor, Michigan 48109-2150 U.S.A. 12. Sponsoring Agency Name and Address 13. Type of Report and Period Covered The University of Michigan Industry Affiliation Program for 14. Sponsoring Agency Code Human Factors in Transportation Safety 15. Supplementary Notes The Affiliation Program currently includes Alps Automotive/Alpine Electronics, Autoliv, Avery Dennison, Bendix, BMW, Bosch, Com-Corp Industries, DaimlerChrysler, DBM Reflex, Decoma Autosystems, Denso, Federal-Mogul, Ford, GE, General Motors, Gentex, Grote Industries, Guide Corporation, Hella, Honda, Ichikoh Industries, Koito Manufacturing, Lang- Mekra North America, Magna Donnelly, Muth, Nissan, North American Lighting, Northrop Grumman, OSRAM Sylvania, Philips Lighting, Renault, Schefenacker International, Sisecam, SL Corporation, Stanley Electric, Toyota Technical Center, USA, Truck-Lite, Valeo, Visteon, 3M Personal Safety Products and 3M Traffic Safety Systems Information about the Affiliation Program is available at: http://www.umich.edu/~industry 16. -
Dark Model Adaptation: Semantic Image Segmentation from Daytime to Nighttime
Dark Model Adaptation: Semantic Image Segmentation from Daytime to Nighttime Dengxin Dai1 and Luc Van Gool1;2 Abstract— This work addresses the problem of semantic also under these adverse conditions. In this work, we focus image segmentation of nighttime scenes. Although considerable on semantic object recognition for nighttime driving scenes. progress has been made in semantic image segmentation, it Robust object recognition using visible light cameras is mainly related to daytime scenarios. This paper proposes a novel method to progressive adapt the semantic models trained remains a difficult problem. This is because the structural, on daytime scenes, along with large-scale annotations therein, textural and/or color features needed for object recognition to nighttime scenes via the bridge of twilight time — the time sometimes do not exist or highly disbursed by artificial lights, between dawn and sunrise, or between sunset and dusk. The to the point where it is difficult to recognize the objects goal of the method is to alleviate the cost of human annotation even for human. The problem is further compounded by for nighttime images by transferring knowledge from standard daytime conditions. In addition to the method, a new dataset camera noise [32] and motion blur. Due to this reason, of road scenes is compiled; it consists of 35,000 images ranging there are systems using far-infrared (FIR) cameras instead from daytime to twilight time and to nighttime. Also, a subset of the widely used visible light cameras for nighttime scene of the nighttime images are densely annotated for method understanding [31], [11]. Far-infrared (FIR) cameras can be evaluation. -
Midnight Sun and Northern Lights Name
volume 3 Midnight Sun and issue 5 Northern Lights It’s black, which absorbs the sun’s warmth. In fact, polar midnight, bears feel hot if the temperature rises above freezing. but the sun The polar nights are long and dark, but sometimes is shining there’s a light show in the sky. The northern lights, which brightly. Where are called the aurora, are often green or pink. They seem are you? You’re to wave and dance in the sky. Auroras are caused by gas in the Arctic, particles that were thrown off by the sun. These particles near the North collide in Earth’s atmosphere and make a beautiful show. Pole. During Few people live in the Arctic because it’s so cold, but the arctic Canada, Greenland, Norway, Iceland, and Russia are summer, the good places to see the midnight sun and the aurora. In ©2010 by Asbjørn Floden in Flickr. Some rights reserved http://creativecommons.org/licenses/by-nc/2.0/deed.en sun doesn’t fact, Norway is often called the Land of the Midnight set for months. Instead, it goes around the horizon. You Sun. could read outside at midnight. As you travel south The temperature stays warm, too, although not as from the North Pole, warm as where you live. The average temperature in there is less midnight sun the summer near the North Pole is about 32 degrees, and fewer northern lights. or freezing. That may sound cold to you, but it’s warm It gets warmer, too. Soon, in the Arctic. -
Daytime and Nighttime Polar Cloud and Snow Identification Using MODIS Data Qing Trepte SAIC, Hampton, VA USA Patrick Minnis Atmo
Daytime and Nighttime Polar Cloud and Snow Identification Using MODIS Data Qing Trepte SAIC, Hampton, VA USA Patrick Minnis Atmospheric Sciences, NASA Langley Research Center, Hampton, VA USA Robert F. Arduini SAIC, Hampton, VA USA Extended Abstract for SPIE 3rd International Asia-Pacific Environmental Remote Sensing Symposium 2002: Remote Sensing of the Atmosphere, Ocean, Environment, and Space Hangzhou, China October 23-27, 2002 Daytime and nighttime polar cloud and snow identification using MODIS data Qing Z. Trepte*a, Patrick Minnisb, Robert F. Arduinia aScience Applications International Corp.; bAtmospheric Sciences, NASA Langley Research Center ABSTRACT The Moderate Resolution Imaging Spectroradiometer (MODIS) on Terra, with its high horizontal resolution and frequent sampling over Arctic and Antarctic regions, provides unique data sets to study clouds and the surface energy balance over snow and ice surfaces. This paper describes a polar cloud mask using MODIS data. The daytime cloud and snow identification methods were developed using theoretical snow bi-directional reflectance models for the MODIS 1.6 and 3.75-µm channels. The model-based polar cloud mask minimizes the need for empirically adjusting the thresholds for a given set of conditions and reduces the error accrued from using single-value thresholds. During night, the MODIS brightness temperature differences (BTD) for 3.75 - 11, 3.75 - 12, 8.55 - 11, and 6.7 - 11 µm are used to detect clouds while snow and ice maps are used to determine snow and ice surfaces. At twilight, the combination of the 1.6-µm reflectance and the 3.75 - 11-µm BTD are used to detect clouds. -
Planit! User Guide
ALL-IN-ONE PLANNING APP FOR LANDSCAPE PHOTOGRAPHERS QUICK USER GUIDES The Sun and the Moon Rise and Set The Rise and Set page shows the 1 time of the sunrise, sunset, moonrise, and moonset on a day as A sunrise always happens before a The azimuth of the Sun or the well as their azimuth. Moon is shown as thick color sunset on the same day. However, on lines on the map . some days, the moonset could take place before the moonrise within the Confused about which line same day. On those days, we might 3 means what? Just look at the show either the next day’s moonset or colors of the icons and lines. the previous day’s moonrise Within the app, everything depending on the current time. In any related to the Sun is in orange. case, the left one is always moonrise Everything related to the Moon and the right one is always moonset. is in blue. Sunrise: a lighter orange Sunset: a darker orange Moonrise: a lighter blue 2 Moonset: a darker blue 4 You may see a little superscript “+1” or “1-” to some of the moonrise or moonset times. The “+1” or “1-” sign means the event happens on the next day or the previous day, respectively. Perpetual Day and Perpetual Night This is a very short day ( If further north, there is no Sometimes there is no sunrise only 2 hours) in Iceland. sunrise or sunset. or sunset for a given day. It is called the perpetual day when the Sun never sets, or perpetual night when the Sun never rises. -
Daytime and Nighttime Wetting
In partnership with Primary Children’s Hospital Daytime and nighttime wetting Some children have trouble staying dry at night. What are the signs of Others have trouble making it to the bathroom daytime wetting? during the daytime. But many children have a little The signs of daytime wetting include: trouble with both day and night issues. Learn more • Waiting until the last minute to use the bathroom about what causes daytime and nighttime wetting and how you can help your child. • Leaking What is daytime wetting? • Peeing more often Daytime wetting occurs when a child who is • Having stomach pain potty-trained has wetting accidents during the day. • Soiling or staining in your child’s underwear It is also called diurnal enuresis (en-you-REE-sis). One in 10 school-aged children have wetting accidents How can I help my child stop during the day. Girls are twice as likely as boys to daytime wetting? have daytime wetting problems. Your child can avoid daytime wetting by: What causes daytime wetting? • Taking their time when peeing Your child may have problems staying dry during • Peeing more often than they think they need to the day because: • Choosing rewards for trying to pee on a • They are too busy to get to the bathroom regular schedule • Their body doesn’t send a good signal to the brain • Drinking plenty of liquids, even at school that the bladder is full • Using the bathroom at least 6 times throughout • Their bladder may start to squeeze before they the whole day, especially when their bladder realize they need to go to the bathroom feels full • Following a routine (using the bathroom when they wake up, before going to school, after lunch, and after school) • Eating a healthy diet of fruits and vegetables to prevent constipation What is nighttime wetting? Nighttime wetting occurs when a child who is potty-trained wets their bed at night. -
Federal Communications Commission § 73.1730
Federal Communications Commission § 73.1730 writing, is signed by the licensees of ing daytime and until local sunset if the stations affected thereby and filed located west of the Class A station on in triplicate by each licensee with the the channel, or until local sunset at FCC in Washington, DC prior to the the Class A station if located east of time of the time of the proposed that station. Operation is also per- change. If time is of the essence, the mitted during nighttime hours not actual departure in operating schedule used by the Class A station or other may precede the actual filing of writ- stations on the channel. ten agreement, provided appropriate (b) No authorization will be granted notice is sent to the FCC. for: (d) If the license of an AM station au- (1) A new limited time station; thorized to share time does not specify (2) A limited time station operating the hours of operation, the station may on a changed frequency; be operated for the transmission of reg- (3) A limited time station with a new ular programs during the experimental transmitter site materially closer to period provided an agreement thereto the 0.1 mV/m contour of a co-channel is reached with the other stations with U.S. Class A station; or which the broadcast day is shared: And (4) Modification of the operating fa- further provided, Such operation is not cilities of a limited time station result- in conflict with § 73.72 (Operating dur- ing in increased radiation toward any ing the experimental period). -
The Effectiveness of Daytime Running Lights for Passenger Vehicles
DOT HS 811 029 September 2008 The Effectiveness of Daytime Running Lights For Passenger Vehicles This report is free of charge from the NHTSA Web site at www.nhtsa.dot.gov This publication is distributed by the U.S. Department of Transportation, National Highway Traffic Safety Administration, in the interest of information exchange. The opinions, findings and conclusions expressed in this publication are those of the author(s) and not necessarily those of the Department of Transportation or the National Highway Traffic Safety Administration. The United States Government assumes no liability for its content or use thereof. If trade or manufacturers’ names or products are mentioned, it is because they are considered essential to the object of the publication and should not be construed as an endorsement. The United States Government does not endorse products or manufacturers. Technical Report Documentation Page 1. Report No. 2. Government Accession No. 3. Recipient’s Catalog No. DOT HS 811 029 4. Title and Subtitle 5. Report Date The Effectiveness of Daytime Running Lights for Passenger Vehicles September 2008 6. Performing Organization Code 7. Author(s) 8. Performing Organization Report No. Jing-Shiarn Wang 9. Performing Organization Name and Address 10. Work Unit No. (TRAIS) Office of Regulatory Analysis and Evaluation 11. Contract or Grant No. National Center for Statistics and Analysis National Highway Traffic Safety Administration Washington, DC 20590 12. Sponsoring Agency Name and Address 13. Type of Report and Period Covered Department of Transportation National Highway Traffic Safety Administration NHTSA Technical Report 1200 New Jersey Avenue SE. 14. Sponsoring Agency Code Washington, DC 20590 15. -
Digital Daylight Observations of the Planets with Small Telescopes
EPSC Abstracts Vol. 8, EPSC2013-795, 2013 European Planetary Science Congress 2013 EEuropeaPn PlanetarSy Science CCongress c Author(s) 2013 Digital daylight observations of the planets with small telescopes Emmanouel (Manos) I. Kardasis (1) (1) Hellenic Amateur Astronomy Association , Athens-Greece [email protected] / Tel.00306945335808 ) Abstract the planetary imaging methodology with the sun above the horizon and some observational results. Planetary atmospheres are extremely dynamical, showing a variety of phenomena at different spatial 2. Methodology and temporal scales, therefore continuous monitoring is required. Amateur astronomers have The basic steps of digital planetary observations are provided a great amount of observations in the presented at [6]. Though, there are some special astronomical community. Some of which are difficulties in DDO, which will be presented along unique made under difficult observational with some solutions: conditions. When the planets are close to the sun, observations can only be made either in twilight or 1. Telescope base alignment. in broad daylight. The use of digital technology in recent years has made feasible daytime planetary 2. Filters observing programs. In this work we present the methodology and some results of digital daylight 3. Position of the planet in the sky observations (DDO) of planets obtained with a small telescope (11inches, 0.28 m). This work may 4. Finding the planet motivate more observers to digitally observe the planets during the day especially when this can be 5. Planetary viewing on the pc screen / important and unique. Focusing 1. Introduction 6. Camera settings Amateur astronomers worldwide continuously 7. Reflections & Thermal heating capturing many interesting hi-resolution images of the ever changing planetary atmospheres. -
On the Controls of Daytime Precipitation in the Amazonian Dry Season
BNL-113652-2017-JA On the Controls of Daytime Precipitation in the Amazonian Dry Season Virendra P. Ghate and Pavlos Kollias Accepted for publication in Journal of Hydrometeorology December 2016 Environmental & Climate Science Dept. Brookhaven National Laboratory U.S. Department of Energy USDOE Office of Science (SC), Biological and Environmental Research (BER) (SC-23) Notice: This manuscript has been authored by employees of Brookhaven Science Associates, LLC under Contract No. DE-SC0012704 with the U.S. Department of Energy. The publisher by accepting the manuscript for publication acknowledges that the United States Government retains a non-exclusive, paid-up, irrevocable, world-wide license to publish or reproduce the published form of this manuscript, or allow others to do so, for United States Government purposes. DISCLAIMER This report was prepared as an account of work sponsored by an agency of the United States Government. Neither the United States Government nor any agency thereof, nor any of their employees, nor any of their contractors, subcontractors, or their employees, makes any warranty, express or implied, or assumes any legal liability or responsibility for the accuracy, completeness, or any third party’s use or the results of such use of any information, apparatus, product, or process disclosed, or represents that its use would not infringe privately owned rights. Reference herein to any specific commercial product, process, or service by trade name, trademark, manufacturer, or otherwise, does not necessarily constitute or imply its endorsement, recommendation, or favoring by the United States Government or any agency thereof or its contractors or subcontractors. The views and opinions of authors expressed herein do not necessarily state or reflect those of the United States Government or any agency thereof. -
IJEST Template
Research & Reviews: Journal of Space Science & Technology ISSN: 2321-2837 (Online), ISSN: 2321-6506 V(Print) Volume 6, Issue 2 www.stmjournals.com Diurnal Variation of VLF Radio Wave Signal Strength at 19.8 and 24 kHz Received at Khatav India (16o46ʹN, 75o53ʹE) A.K. Sharma1, C.T. More2,* 1Department of Physics, Shivaji University, Kolhapur, Maharashtra, India 2Department of Physics, Miraj Mahavidyalaya, Miraj, Maharashtra, India Abstract The period from August 2009 to July 2010 was considered as a solar minimum period. In this period, solar activity like solar X-ray flares, solar wind, coronal mass ejections were at minimum level. In this research, it is focused on detailed study of diurnal behavior of VLF field strength of the waves transmitted by VLF station NWC Australia (19.8 kHz) and VLF station NAA, America (24 kHz). This research was carried out by using VLF Field strength Monitoring System located at Khatav India (16o46ʹN, 75o53ʹE) during the period August 2009 to July 2010. This study explores how the ionosphere and VLF radio waves react to the solar radiation. In case of NWC (19.8 kHz), the signal strength recording shows diurnal variation which depends on illumination of the propagation path by the sunlight. This also shows that the signal strength varies according to the solar zenith angle during daytime. In case of VLF signal transmitted by NAA at 24 kHz, the number of sunrises and sunsets are observed in VLF signal strength due to the variations of illumination of the D-region during daytime. In both the cases, the signal strength is more stable during daytime and fluctuating during nighttime due to the presence and absence of D-region during daytime and nighttime respectively.