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JR West/West Japan Railway Co. 683-5000 Series 9-car 1,500V dc EMU No. T51 (クモハ 683-5511 leading)
Train TB1 07.09 Osaka (大阪)-Tsuruga (敦賀) Thunderbird limited express service
Shin-Osaka (新大阪), Osaka Prefecture, Japan
July 7th, 2013
1280 x 840
Almost all bacteria are so tiny they can only be seen through a microscope. Bacteria are made up of one cell, so they are a kind of unicellular organism
Courtesy of Mr. sathish -
Image Details
Instrument used: Tecnai
Magnification: 6000 x
Horizontal Field Width: 6.00 μm
Vacuum: 5 mbar
Voltage: 60 kv
Spot: 1.0
Working Distance: 5.8
Detector: SE
Multiply Festival (Sous-station Lebon).
Projet Diligence (http://www.projetdiligence.net/).
With Andrea Crews - Anker-Crew -Tristan de Bartolo - Donatella Bernardi - Marie Avril Berthet - Juliana Borinski - Carte Postale Records - Pierre Laurent Cassière Diego Castro - John Cejudo - Batiste César - Fréderic Chapon - Paul Chazal Code Magazine - Claudia Comte - Henry Deletra - Diligence - Antonin Demé - Elzo Durt - Barbara Fourneret - Gilles Furtwängler - Olivier Genoud - David Ghetto Ghostape - Sophie Graniou - Aloïs Godinat - Aurélie Henquin - Martin Hyde - Jesus Had A Sister Production - Klat -Laurent Kropf - Andréa Lapzeson - Le Bureau Des Consultations - Beat Lippert - R-Livraison - Ma-Asso - Fabrice Medina Mariana Melo - Adrien Missika - Optical Sound - Bianca Pedrina - Pictoplasma Pin-Up Badges - Emilie Pischedda - Plintub - Benoit Police - Pschiit - R-Livraison(SiC) - Sardine Animal - Scarlettjohanson - Louis Scoufaras - Serial Printer Valentin Souquet - Telegraphe Records - Maud Thomazeau - David de Tscharner - Benjamin Valenza - Nicolas Wagnières - Nicolas Welt - Dana Wyse & guests...
Clockwise from top: Adinkrahene (leadership), Ese Ne Tekrema (interdependence), Nysapo (wisdom), Dwennimen (strength), Akoma Ntoso (agreement), Osram Ne Nsoromma (love); center: Akoma (love)
(check these out for a laugh-he's a dancin' fool!!)
www.jibjab.com/starring_you/receipt/403653
www.jibjab.com/starring_you/receipt/403591
www.jibjab.com/starring_you/receipt/403393
Here's a couple more...these just crack me up!
The room was illuminated by both window lighting and florescent lighting of ~3500K. I WB'ed for the florescent lighting and the window lighting cast a blue tint on the front of her face. Funny how our eyes don't perceive this but the camera really picks up on it.
The display reads:
Multiple Launch Rocket System (MLRS)
M-270
The MLRS replaces the aging, "old reliable" 8 inch howitzer as the U.S. Army's primary General Support Artillery weapon system. The system's M-26 rocket is capable of engaging targets at a range of 30 KM while the Army Tactical Missile System (ATACMS) is able to engage a target at a range of 124 KM. It is capable of firing 12 rockets in less than one minute, delivering 7,728 submunitions. Each rocket delivers 644 submunitions, with a target area the size of a football field. This capacity earned MLRS the nickname "Steel Rain." MLRS units fired several thousand rockets and 32 ATACMS missiles during Operation Desert Shield / Storm. The MLRS has been successfully used in conducting Artillery raid operations., suppression / destruction of air defense operations, and as a reinforcing and general support weapon. Its unique capabilities make the MLRS a versatile and lethal weapons platform able to deliver various munitions, both close and deep, in the theater of operations. The responsiveness, survivability and lethality and range, and by expanding its suite of munitions. The MLRS is a Multi-National system developed by the United Kingdom, France, Germany, and Italy as well as the United States.
Caliber:
Rocket 226 mm (8.9 inch)
Missile 610 mm (24 inch)
Vehicle Weight:
Loaded 25,191 kg (55,420 lbs)
Empty 20,189 kg (44,416 lbs)
Vehicle Speed: 64 km/h (40 mph)
Vehicle Range: 483 km (300 miles)
Rocket Weight: 303 kg (667 lbs)
Missile Weight: 273 kg (600 lbs)
Traverse: 6,400 mils (360 degrees)
Detachment: 3
Museum # 94.59.1
Taken December 26th, 2010.
Experimental multiple exposure of the tulips during the Tulip Time Festival at Corbett Gardens in 2011.
Nikon F65. Fuji Pro 160S 35mm C41 film.
Corporal Audrey Enocq, a member of HMCS FREDERICTON's dive team, dives to inspect the hull of the ship during Operation REASSURANCE on 22 February 2023 in Souda Bay, Greece.
Please credit: Cpl Noé Marchon, Canadian Armed Forces Photo
La caporale Audrey Enocq, membre de l’équipe de plongée du NCSM FREDERICTON, effectue une plongée pour inspecter la coque du navire au cours de l’opération REASSURANCE, le 22 février 2023, dans la baie de Souda, en Grèce.
Photo : Cpl Noé Marchon, Forces armées canadiennes
From Sephora: The Multiple
Nars The Multiple is the original all-in-one, cream-to-powder, multi-purpose makeup stick. With fingertip application, The Multiple highlights, sculpts, and warms eyes, cheeks, lips, and body in an array of shades from sheer accents to mauve and bronze.
Sailors from HMCS FREDERICTON fold the Naval Jack while the ship leaves Souda Bay, Greece, during Operation REASSURANCE on 25 February 2023 in the Mediterranean Sea.
Please credit: Cpl Noé Marchon, Canadian Armed Forces Photo
Des marins du NCSM FREDERICTON plient le pavillon de beaupré au moment où le navire quitte la baie de Souda, en Grèce, au cours de l’opération REASSURANCE, le 25 février 2023, dans la Méditerranée.
Photo : Cpl Noé Marchon, Forces armées canadiennes
Commander Matthew Mitchell, Commanding Officer HMCS FREDERICTON, and Lieutenant-Commander Andrew Tunstall, Executive Officer, discuss on the jetty as the ship is berthed in Souda Bay, Greece, during Operation REASSURANCE on 22 February 2023.
Please credit: Cpl Noé Marchon, Canadian Armed Forces Photo
Le capitaine de frégate Matthew Mitchell, commandant du NCSM FREDERICTON, et le capitaine de corvette Andrew Tunstall, commandant en second, discutent sur la jetée alors que le navire est à quai dans la baie de Souda, en Grèce, au cours de l’opération REASSURANCE, le 22 février 2023.
Photo : Cpl Noé Marchon, Forces armées canadiennes
Members of the HMCS FREDERICTON diving team after a dive during Operation REASSURANCE on 22 February 2023 in Souda Harbour, Crete.
Please credit: Cpl Noé Marchon, Canadian Armed Forces Photo
Des membres de l’équipe de plongée du NCSM FREDERICTON après avoir effectué une plongée au cours de l’opération REASSURANCE, le 22 février 2023, dans la baie de Souda, en Grèce.
Photo : Cpl Noé Marchon, Forces armées canadiennes
This is a multiple exposure of two different photos of the same theme placed ontop of each other. I did this by getting two different negatives and placing them in the carrier together, that way when i exposed them and put them through the different chemicals they came out joined. I think the final effect is clever and i didn't expect it to look as good as it came out.
First try at the multiple exposure mode of the Lomo' Instant Automat by Lomography. EV -1 in the first shot kinda ruined it
Sigma Orionis (σ Ori) multiple star system
Credit: Giuseppe Donatiello
Sigma Orionis (σ Ori) is a multiple star system located in the constellation Orion, a short distance from Zeta Orionis (Alnitak).
It is a system composed of no fewer than five stars, all gravitationally bound.
The system is dominated by Sigma Orionis AB, a pair of blue stars of type O and B, respectively. The system includes other stars such as Sigma Orionis C, D, and E. The latter is the prototype of a rare type of helium-rich star. Except for AB, the other components form a Trapezium-type system, a small, young open cluster 3–5 million years old. The ensemble is cataloged as the multiple star STS 762. More accurate measurements provided by the Gaia satellite indicate a distance of 387.51 ± 1.32 pc, or approximately 1,264 light-years.
STS 761 is slightly further away from the STS 672 cluster. It is a fascinating triple star system. The three components are designated A, B, and C, where A and B form a close pair. The system is notable for being surrounded by a dust disk detected by the ALMA radio telescope. Its average distance is about 1,300 light-years.
Telescopic image
Maksutov 127/1500mm + Canon EOS 4000D
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σ Orionis is a multiple main-sequence star of spectral class O9 in the constellation of Orion with visual magnitude 3.81, also known as σ Orionis cluster. It is a visual double star which can be observed only with the help of very large telescopes.
The σ Orionis cluster is part of the Ori OB1b stellar association, commonly referred to as Orion's Belt. The cluster was not recognised until 1996 when a population of pre-main sequence stars was discovered around the star (J.A. Caballero, 2007).
Members of the embarked Air Detachment onboard HMCS FREDERICTON conduct visual inspection of the CH-148 Cyclone helicopter’s main rotor blades during Operation REASSURANCE on 21 February 2023 in Souda Bay, Greece.
Please credit: Cpl Noé Marchon, Canadian Armed Forces Photo
Des membres du détachement aérien embarqué à bord du NCSM FREDERICTON effectuent une inspection visuelle des pales du rotor principal de l’hélicoptère CH-148 Cyclone au cours de l’opération REASSURANCE, le 21 février 2023, dans la baie de Souda, en Grèce.
Photo : Cpl Noé Marchon, Forces armées canadiennes
Members of the embarked Air Detachment onboard HMCS FREDERICTON conduct maintenance on the CH-148 Cyclone helicopter’s main rotor head during Operation REASSURANCE on 21 February 2023 in Souda Bay, Greece.
Please credit: Cpl Noé Marchon, Canadian Armed Forces Photo
Des membres du détachement aérien embarqué à bord du NCSM FREDERICTON effectuent l’entretien de la tête de rotor principal de l’hélicoptère CH-148 Cyclone au cours de l’opération REASSURANCE, le 21 février 2023, dans la baie de Souda, en Grèce.
Photo : Cpl Noé Marchon, Forces armées canadiennes