Rhythms During the Polar Night
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Polar Winds from VIIRS
Polar Winds from VIIRS Jeff Key*, Richard Dworak+, Dave Santek+, Wayne Bresky@, Steve Wanzong+ ! Jaime Daniels#, Andrew Bailey@, Chris Velden+, Hongming Qi^, Pete Keehn#, Walter Wolf#! ! *NOAA/National Environmental Satellite, Data, and Information Service, Madison, WI! + Cooperative Institute for Meteorological Satellite Studies, University of Wisconsin-Madison! #NOAA/National Environmental Satellite, Data, and Information Service, Camp Springs, MD! ^NOAA/National Environmental Satellite, Data, and Information Service, Camp Springs, MD! @I.M. Systems Group (IMSG), Rockville, MD USA! 11th International Winds Workshop, Auckland, 20-24 February 2012 The Polar Wind Product Suite MODIS Polar Winds LEO-GEO Polar Winds •" Aqua and Terra separately, bent pipe •" Combination of may geostationary data source Operational and polar-orbiting imagers •" Aqua and Terra combined, bent pipe •" Fills the 60-70 degree latitude gap •" Direct broadcast (DB) at EW –" McMurdo, Antarctica (Terra, Aqua) VIIRS Polar Winds –" Tromsø, Norway (Terra only) •" (Details on following slides) –" Sodankylä, Finland (Terra only) –" Fairbanks, Alaska (Terra, from UAF) EW AVHRR Polar Winds •" Global Area Coverage (GAC) for NOAA-15, -16, -17, -18, -19 Operational •" Metop Operational •" HRPT (High Resolution Picture Transmission = direct readout) at –" Barrow, Alaska, NOAA-16, -17, -18, -19 –" Rothera, Antarctica, NOAA-17, -18, -19 •" Historical GAC winds, 1982-2009. Two satellites throughout most of the time series. Polar Wind Product History Operational NWP Users of Polar Winds! 13 NWP centers in 9 countries: •" European Centre for Medium-Range Weather Forecasts (ECMWF) - since Jan 2003.! •" NASA Global Modeling and Assimilation Office (GMAO) - since early 2003.! •" Deutscher Wetterdienst (DWD) – MODIS since Nov 2003. DB and AVHRR.! •" Japan Meteorological Agency (JMA), Arctic only - since May 2004.! •" Canadian Meteorological Centre (CMC) – since Sep 2004. -
Water Ice Clouds in the Martian Atmosphere: General Circulation Model Experiments with a Simple Cloud Scheme Mark I
JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 107, NO. E9, 5064, doi:10.1029/2001JE001804, 2002 Water ice clouds in the Martian atmosphere: General circulation model experiments with a simple cloud scheme Mark I. Richardson Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, California, USA R. John Wilson Geophysical Fluid Dynamics Laboratory, National Oceanic and Atmospheric Administration, Princeton, New Jersey, USA Alexander V. Rodin Space Research Institute, Planetary Physics Division, Moscow, Russia Received 17 October 2001; revised 31 March 2002; accepted 5 June 2002; published 20 September 2002. [1] We present the first comprehensive general circulation model study of water ice condensation and cloud formation in the Martian atmosphere. We focus on the effects of condensation in limiting the vertical distribution and transport of water and on the importance of condensation for the generation of the observed Martian water cycle. We do not treat cloud ice radiative effects, ice sedimentation rates are prescribed, and we do not treat interactions between dust and cloud ice. The model generates cloud in a manner consistent with earlier one-dimensional (1-D) model results, typically evolving a uniform (constant mass mixing ratio) vertical distribution of vapor, which is capped by cloud at the level where the condensation point temperature is reached. Because of this vertical distribution of water, the Martian atmosphere is generally very far from fully saturated, in contrast to suggestions based upon interpretation of Viking data. This discrepancy results from inaccurate representation of the diurnal cycle of air temperatures in the Viking Infrared Thermal Mapper (IRTM) data. In fact, the model suggests that only the northern polar atmosphere in summer is consistently near its column-integrated holding capacity. -
June Solstice Activities (PDF)
Arctic Connection Linking Your Place to the MOSAiC Expedition June Solstice Edition Introduction As I write this, it is the June Solstice. The exact moment of solstice occurred a few hours ago, at 21:44 Universal Daylight Time. This was at 1:44 pm today here in Homer, Alaska. This moment marked when Earth’s north pole leaned most toward the sun, and the Earth’s south pole was tilted most away from the sun. On this day, the sun appears directly overhead at local noon for those living at 23.5 degrees north (the Tropic of Cancer), as far north as the sun ever gets. And during the December solstice, the sun appears directly overhead for those living at 23.5 degrees south (the Tropic of Capricorn). (In case you need a refresher, here’s the basic science from Earth & Sky.) In the northern hemisphere, the June Solstice is called the summer solstice and represents the day(s) with the most amount of daylight. I say days because in some parts of the northern hemisphere, the sun has stayed above the horizon for multiple days now and won’t rise again until the next month. This is often called the Midnight Sun, and the ice camp at the Polarstern has been bathed in light for many days. This is good news for the scientists of Leg 4, who are just now arriving to the floe. The extended daylight will help make all of the research tasks a little bit easier than those Leg 1 and Leg 2 researchers who had to work through the Polar Night. -
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. -
Shining a Light on Fish at Night: an Overview of Fish and Fisheries in the Dark of Night, and in Deep and Polar Seas Neil Hammerschlag University of Miami
Nova Southeastern University NSUWorks Marine & Environmental Sciences Faculty Articles Department of Marine and Environmental Sciences 1-1-2017 Shining a Light on Fish at Night: An Overview of Fish and Fisheries in the Dark of Night, and in Deep and Polar Seas Neil Hammerschlag University of Miami Carl G. Meyer University of Hawaii - Manoa Michael S. Grace Florida Institute of Technology - Melbourne Steven T. Kessel Michigan State University Tracey Sutton Nova Southeastern University, <<span class="elink">[email protected] See next page for additional authors Findollo outw thi mors aend infor addmitationional a boutworkNs oavta: hSouthettps://nastesruwn Uorknivse.rnositvyaa.ndedu/oc the Hc_faalmosca rCticleollesge of Natural Sciences and POacret aofno thegrapMhya.rine Biology Commons, and the Oceanography and Atmospheric Sciences and Meteorology Commons NSUWorks Citation Neil Hammerschlag, Carl G. Meyer, Michael S. Grace, Steven T. Kessel, Tracey Sutton, Euan S. Harvey, Claire B. Paris-Limouzy, David W. Kerstetter, and Steven J. Cooke. 2017. Shining a Light on Fish at Night: An Overview of Fish and Fisheries in the Dark of Night, and in Deep and Polar Seas .Bulletin of Marine Science : 1 -32. https://nsuworks.nova.edu/occ_facarticles/788. This Article is brought to you for free and open access by the Department of Marine and Environmental Sciences at NSUWorks. It has been accepted for inclusion in Marine & Environmental Sciences Faculty Articles by an authorized administrator of NSUWorks. For more information, please contact [email protected]. Authors Euan S. Harvey Curtin University - Perth, Australia Claire B. Paris-Limouzy University of Miami David W. Kerstetter Nova Southeastern University, [email protected] Steven J. -
Regions and Counties in Norway
Regions and counties in Norway REGIONS AND COUNTIES IN NORWAY Northern Norway Northern Norway is located in the north and is also the most eastern region. This region comprises the two counties Troms og Finnmark and Nordland. If you visit Northern Norway in December or January, you can experience the polar night. The polar night is when the sun is under the horizon the whole day. In Northern Norway, you can see the northern lights in winter. Norway is divided into five regions. Northern Norway is located in the north of Northern lights. Photo: Pxhere.com the country. Trøndelag is located in the middle of the country. Western Norway is During summer, you can see the midnight in the west, and Eastern Norway is in the sun in Northern Norway. The midnight sun east. The region located in the south is is when the sun does not set, and a part of called Southern Norway. the sun is visible above the horizon all night. Every part of the country is divided into counties. There are 11 counties in Norway. Troms and Finnmark Troms og Finnmark is located furthest north and east and borders Russia, Finland 1 The National Centre of Multicultural Education, Native languages, morsmal.no Regions and counties in Norway and Sweden. Tromsø is the largest city in Troms og Finnmark. Norway's northernmost point, Knivskjellodden, is located in Troms og Finnmark. The North Cape (Nordkapp) is better known and is located almost as far north as Knivskjellodden. The North Cape is a famous tourist destination in Norway. Skrei cod hanging to dry on a rack. -