Maps Utilisateurs d'un lecteur d'écran : cliquez ici pour accéder à la version HTML brut Nouveauté ! Faites glisser et déposez les icônes pour réorganiser vos applications. Connectez-vous pour essayer. PlusAutres résultats Google Connexion 100 m 500 pieds Satellite Trafic Photos Météo ferropolis Quitter Modifier dans Google Map MakerSignaler un problème Données cartographiques ©2014 GeoBasis-DE/BKG (©2009), Google - Ferropolis Ferropolisstraße 1, 06773 Gräfenhainichen, Allemagne · ferropolis.de 9 avis · ItinéraireRechercher à proximitéplus Google Maps - ©2014 Google - Conditions d'utilisation - Confidentialité Pour restituer le niveau de détail visible à l'écran, cliquez sur le lien "Imprimer" à côté de la carte. Pistes cyclables Voies réservées Routes empruntables à vélo
Qualquer objeto se torna sensível ao toque com Touché Interfaces “touch” estão em vários lugares: smartphones, caixas eletrônicos, tablets, totens interativos. Mas se depender da Disney Research e da nova tecnologia apresentada por eles há alguns dias, qualquer objeto pode se tornar sensível ao toque. Inclusive líquidos. (!) Confira no vídeo abaixo como funciona a tecnologia: la place du feu dans la mecanique quantique Git So, what is Git in a nutshell? This is an important section to absorb, because if you understand what Git is and the fundamentals of how it works, then using Git effectively will probably be much easier for you. As you learn Git, try to clear your mind of the things you may know about other VCSs, such as Subversion and Perforce; doing so will help you avoid subtle confusion when using the tool. Snapshots, Not Differences The major difference between Git and any other VCS (Subversion and friends included) is the way Git thinks about its data. Figure 1-4. Git doesn’t think of or store its data this way. Figure 1-5. This is an important distinction between Git and nearly all other VCSs. Nearly Every Operation Is Local Most operations in Git only need local files and resources to operate — generally no information is needed from another computer on your network. This also means that there is very little you can’t do if you’re offline or off VPN. Git Has Integrity Git Generally Only Adds Data
alive video (1) Facebook Écoles & universités De nous jours, les médias numériques sont omniprésents dans les études et la vie professionnelle. MAGIX soutient activement les écoles et les universités depuis de nombreuses années en mettant à disposition de manière optimale des compétences multimédias diversifiées. Les solutions complètes réalisées exclusivement pour les enseignants et les étudiants recouvrent tous les grands domaines d'application de la production de médias numériques : vidéo, musique, graphisme et webdesign. Profitez de : Solutions logicielles simples d'utilisation pour obtenir d'excellents résultats en un temps recordLicences multiples attrayantesQualité Made in GermanyFormations avancées compétentes dans tous les domaines du multimédia Venez visiter le portail d'éducation MAGIX
Phaistos Disc The Phaistos Disc (also spelled Phaistos Disk, Phaestos Disc) is a disk of fired clay from the Minoan palace of Phaistos on the Greek island of Crete, possibly dating to the middle or late Minoan Bronze Age (2nd millennium BC). It is about 15 cm (5.9 in) in diameter and covered on both sides with a spiral of stamped symbols. Its purpose and meaning, and even its original geographical place of manufacture, remain disputed, making it one of the most famous mysteries of archaeology. This unique object is now on display at the archaeological museum of Heraklion. The disc was discovered in 1908 by the Italian archaeologist Luigi Pernier in the Minoan palace-site of Phaistos, and features 241 tokens, comprising 45 unique signs, which were apparently made by pressing hieroglyphic "seals" into a disc of soft clay, in a clockwise sequence spiraling toward the disc's center. Discovery Tablet PH-1 It was found in the main cell of an underground "temple depository". Authenticity Dating Typography Signs
Mirrors - JDSU (Photonics Handbook | Optical Materials & Coatings) A mirror is an important element in many optical systems. Its basic function is to redirect light, often with the purpose of making an optical system more compact. This article discusses the kinds of thin-film coatings that can be used for mirrors. The choice of coating depends on the application, including the spectral range of interest, the optical wavefront quality desired and the cost limitations. The basic difference between the household mirror and the optical mirror is that one is coated on the back surface and the other is coated on the front. A mirror’s substrate surface should be flat and smooth. For some applications, a mirror’s ability to conduct heat is important. Metal mirror coatings The simplest and most common mirror coating is a thin layer of metal. TABLE 1.n AND k FOR SELECTED METALS *Aluminum has a reflectance dip at 0.8 µm: for λ = 0.8 µm, n = 2.80 and k = 8.45 for λ = 0.9 µm, n = 2.06 and k = 8.30 SOURCE: Handbook of Optical Constants of Solids Figure 1. Figure 2. 1.
animations An experiental 3D-animation from my image of NGC 6752 I have tested a new method to publish my 3D-images as a form of Lenticular prints. For this technique to work, I need series of images from different angles, in this case 24 images are needed. Lenticular printing is actually an old technique but in past few years it has become much more sophisticated. The results can be stunning visually, image plane disappears and object floats in and outside of the frame. Since astronomical objects are too far away, no real parallax can be imaged. NOTE! A globular cluster, NGC 6752, as an animated 3D-study Please, let the image load, the size is ~6.5MB 24-frames, images are meant for a lenticular 3D-print. NOTE. Original 2D image of the object Image of the NGC 6752 from the year 2010 Original blog post, with technical info, can be seen here: What are globular clusters? First of all, they are very beautiful, visually and imaged! A screenshot from the 3D-modeling software
Hourglass Nebula The Engraved Hourglass Nebula (also known as MyCn 18) is a young planetary nebula situated in the southern constellation Musca about 8,000 light-years away from Earth. It was discovered by Annie Jump Cannon and Margaret W. Mayall during their work on an extended Henry Draper Catalogue (the catalogue was built between 1918 and 1924). At the time, it was designated simply as a small faint planetary nebula. Much improved telescopes and imaging techniques allowed the hourglass shape of the nebula to be discovered by Raghvendra Sahai and John Trauger of the Jet Propulsion Laboratory on January 18, 1996. The Hourglass Nebula was photographed by the Wide Field and Planetary Camera 2 of the Hubble Space Telescope. A less-famous "Hourglass Nebula" is located inside the Lagoon Nebula. Hourglass Nebula in popular culture[edit] See also[edit] Hourglass Nebula in fiction. References[edit] Coordinates:
Aerial Cam - Specialist archaeological photography, on site and aerial photography Cité de Cinéma,la réalisation des reportages, des documentaires, des courts métrages, des spots publicitaires, et des téléfilms La diversité des paysages, la diversité ethnique, la lumière exceptionnelle, une main d’œuvre locale abondante, tous ces éléments font de Ouarzazate l’un des lieux les plus désirés du Maroc par les cinéastes. L’Industrie cinématographique est très prometteuse dans la vie de cette province. En effet, les plus célèbres cinéastes ont tourné sur ses terres, on peut citer à titre d’exemple : Martin Scorcesse avec « Kundun »,Ridley Scott avec « Gladiator » et «Kingdom of Heaven», Alain Chabbat avec « Astérix et Obélix» , Stefan Sommers avec « La Momille", « Le Diamant du Nil » de Lewis Teague, « Un thé au Sahara» de Bernardo Bertolucci , le pionnier Jacques Becker avec « Ali Baba et les 40 Voleurs » tourné en 1954 et la liste est longue. A côté des longs métrages, Ouarzazate a connu aussi la réalisation des reportages, des documentaires, des courts métrages, des spots publicitaires, et des téléfilms. Studios Atlas Studios Kanzaman CLA Studios
Sound Made Visible The generic term for the patterns of vibration that occur on the surface of an object when excited by an incident sound is ‘modal phenomena,’ a field of study that covers everything from vibrations in suspension bridges, to vibrations in body parts of cars, to the effects of sound on the human skeleton and internal organs. In the 1970’s this branch of science was named ‘cymatics’ by Swiss doctor Hans Jenny, a word that derives from the Greek ‘kyma,’ meaning ‘wave’ and the inspiration for the name of our CymaScope instrument. The classical view of modal phenomena is that modal patterns form as a consequence of the natural resonant frequencies, or modes, of the object or membrane; current mathematical techniques used to describe this class of phenomena say nothing about the quality of the exciting sound. Musical sounds contain many harmonics so when a circular membrane is excited by a complex musical sound the resulting modal pattern(s) are, naturally, also complex. Applications