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The late afternoon sun caught my eye on the city council building highlinghting the 7 flashes of yellow features.
This is SOOC and just a lift on the midtones for the shadows on the RHS.
Numerically Odd Theme
Parallel Lines Challenge
Interesting building in Florianópolis, during the sunset.
No amount of rotate/perspective will "fix" this image.
One of the world’s biggest Angular conference.
The beautiful city of Warsaw, amazing national stadium, 2 days, 15 talks, 5 workshops, Q&A session and much more!
Thank you to our wonderfull sponsors: Acaicoft, 7N, Twilio, SoftwareMill, SoftwarePlant, EDC Aviation Digital, Deloitte, CodiLime, Telerik, JetBrains, DataArt Poland. Thank you for the speakers, we are really appreciate that you came to Poland and share your knowledge! Thank you for communities from all over the world for your support. Thank you for ALL attendees!
Inktober 2018 ( 16 ) ANGULAR
I could not imagine anything more angular than the sinister face of The Shadow.
I have always liked this "pulp" hero, and it seemed like a very good opportunity to draw him.
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No he podido imaginar algo más angular que el siniestro rostro de La Sombra.
Siempre he sentido debilidad por este héroe "pulp", y me ha parecido una muy buena oportunidad para dibujarlo.
One of the world’s biggest Angular conference.
The beautiful city of Warsaw, amazing national stadium, 2 days, 15 talks, 5 workshops, Q&A session and much more!
Thank you to our wonderfull sponsors: Acaicoft, 7N, Twilio, SoftwareMill, SoftwarePlant, EDC Aviation Digital, Deloitte, CodiLime, Telerik, JetBrains, DataArt Poland. Thank you for the speakers, we are really appreciate that you came to Poland and share your knowledge! Thank you for communities from all over the world for your support. Thank you for ALL attendees!
One of the world’s biggest Angular conference.
The beautiful city of Warsaw, amazing national stadium, 2 days, 15 talks, 5 workshops, Q&A session and much more!
Thank you to our wonderfull sponsors: Acaicoft, 7N, Twilio, SoftwareMill, SoftwarePlant, EDC Aviation Digital, Deloitte, CodiLime, Telerik, JetBrains, DataArt Poland. Thank you for the speakers, we are really appreciate that you came to Poland and share your knowledge! Thank you for communities from all over the world for your support. Thank you for ALL attendees!
One of the world’s biggest Angular conference.
The beautiful city of Warsaw, amazing national stadium, 2 days, 15 talks, 5 workshops, Q&A session and much more!
Thank you to our wonderfull sponsors: Acaicoft, 7N, Twilio, SoftwareMill, SoftwarePlant, EDC Aviation Digital, Deloitte, CodiLime, Telerik, JetBrains, DataArt Poland. Thank you for the speakers, we are really appreciate that you came to Poland and share your knowledge! Thank you for communities from all over the world for your support. Thank you for ALL attendees!
One of the world’s biggest Angular conference.
The beautiful city of Warsaw, amazing national stadium, 2 days, 15 talks, 5 workshops, Q&A session and much more!
Thank you to our wonderfull sponsors: Acaicoft, 7N, Twilio, SoftwareMill, SoftwarePlant, EDC Aviation Digital, Deloitte, CodiLime, Telerik, JetBrains, DataArt Poland. Thank you for the speakers, we are really appreciate that you came to Poland and share your knowledge! Thank you for communities from all over the world for your support. Thank you for ALL attendees!
One of the world’s biggest Angular conference.
The beautiful city of Warsaw, amazing national stadium, 2 days, 15 talks, 5 workshops, Q&A session and much more!
Thank you to our wonderfull sponsors: Acaicoft, 7N, Twilio, SoftwareMill, SoftwarePlant, EDC Aviation Digital, Deloitte, CodiLime, Telerik, JetBrains, DataArt Poland. Thank you for the speakers, we are really appreciate that you came to Poland and share your knowledge! Thank you for communities from all over the world for your support. Thank you for ALL attendees!
Seen and shot on location as part of the architectural series in Markdorf, Germany. Post-processing done in Capture One 20.
Press 'L' fullscreen mode for optimum optical nerve stimulation.
Once the Shoshone River exits Rattlesnake Mountain into the Big Horn Basin at Cody the river remains in a canyon that has the Cody bench (river terrace) on both sides. An angular unconformity between the Quaternary Cody Terrace Gravels and the red Triassic Chugwater Formation is exposed in the bend of the river on the canyon wall in the center of the image. The Cody Rodeo Arena can be seen on the Cody Bench just behind the exposed unconformity.
Geologically, an unconformity is an erosional or non-depositional surface separating two rock masses or strata of different ages, indicating that sediment deposition was not continuous. In other words, an unconformity indicates that 1- the older rock layer was exposed to erosion for an interval of time before deposition of the younger; 2- there was a period of non-deposition between the time the 2 sediment layers were deposited at least at that location or 3- a combination of both. An angular unconformity is an unconformity where horizontally parallel strata of sedimentary rock are deposited on tilted and eroded layers, producing an angular discordance with the overlying layers. This indicates that the older beds were titled or deformed tectonically, then truncated by erosion, before the younger beds were deposited. The entire package can be subsequently deformed after deposition of the younger beds so they are no longer parallel but the discordance with the older beds still remains. Generally, development of an unconformity is accompanied by or preceded by uplift of the rock units or strata that will be eroded, and/or the fall of relative sea level, thus exposing rock units or strata to erosion. The presence of an unconformity indicates a gap or vacuity in the chronostratigraphic record.
The rocks visible in the foreground from front to back are shales; limestone and cherts on the Permian Park City Formation (also known as the Phosphoria Formation), and the tan sandstones of the Pennsylvanian Tensleep Formation. On top of the cliffs both to the left and the right in the foreground are topped with Quaternary Travertine Deposits that are part of the Colter's Hell (Also know as the Demaris or Cody) hydrothermal (hot springs) area.
for theme of the week "angularity".....taken at a family gathering to celebrate my brother and dad's birthdays, the inside of my brothers radiator !!
still getting to grips with the fuji....
Showroom
Crta. Santiago-Pontevedra a 9 Km. de Santiago de Compostela en dirección a Pontevedra. 15.866 Ameneiro-Teo (La Coruña) España.
Annotations
Geological Features
A - angular unconformity
B - fault
Stratigraphy
1 - Quaternary Travertine: hot springs deposits
2a - Quaternary Unconsolidated Recent Terrace Gravels (includes sand silt and cobbles)
2b - Cody Terrace (Bench) Deposits (gravel, sand; cobbles; silt and calcareous cement)
3 - Eocene Willwood Formation: seen in this image on the distant horizon.
4- Triassic Chugwater formation: red siltstone, shale and fine-grained sandstone
5- Triassic Dinwoody Formation: tan to dark red shale, gypsum and thin-bedded limestones and dolomites
6- Permian Park City Formation (also called Phosphoria): light gray to black shales, limestones, dolomites and chert nodules.
7-Pennsylvian Tensleep Sandstone with thin interbeds of limestone and dolomites at the base
Once the Shoshone River exits Rattlesnake Mountain into the Big Horn Basin at Cody the river remains in a canyon that has the Cody bench (river terrace) on both sides. An angular unconformity between the Quaternary Cody Terrace Gravels and the red Triassic Chugwater Formation is exposed in the bend of the river on the canyon wall in the center of the image. The Cody Rodeo Arena can be seen on the Cody Bench just behind the exposed unconformity.
Geologically, an unconformity is an erosional or non-depositional surface separating two rock masses or strata of different ages, indicating that sediment deposition was not continuous. In other words, an unconformity indicates that 1- the older rock layer was exposed to erosion for an interval of time before deposition of the younger; 2- there was a period of non-deposition between the time the 2 sediment layers were deposited at least at that location or 3- a combination of both. An angular unconformity is an unconformity where horizontally parallel strata of sedimentary rock are deposited on tilted and eroded layers, producing an angular discordance with the overlying layers. This indicates that the older beds were titled or deformed tectonically, then truncated by erosion, before the younger beds were deposited. The entire package can be subsequently deformed after deposition of the younger beds so they are no longer parallel but the discordance with the older beds still remains.
Generally, development of an unconformity is accompanied by or preceded by uplift of the rock units or strata that will be eroded, and/or the fall of relative sea level, thus exposing rock units or strata to erosion. The presence of an unconformity indicates a gap or vacuity in the chronostratigraphic record.
The rocks visible in the foreground from front to back are shales; limestone and cherts on the Permian Park City Formation (also known as the Phosphoria Formation), and the tan sandstones of the Pennsylvanian Tensleep Formation. On top of the cliffs both to the left and the right in the foreground are topped with Quaternary Travertine Deposits that are part of the Colter's Hell (Also know as the Demaris or Cody) hydrothermal (hot springs) area.
Showroom
Crta. Santiago-Pontevedra a 9 Km. de Santiago de Compostela en dirección a Pontevedra. 15.866 Ameneiro-Teo (La Coruña) España.
Showroom
Crta. Santiago-Pontevedra a 9 Km. de Santiago de Compostela en dirección a Pontevedra. 15.866 Ameneiro-Teo (La Coruña) España.
Showroom
Crta. Santiago-Pontevedra a 9 Km. de Santiago de Compostela en dirección a Pontevedra. 15.866 Ameneiro-Teo (La Coruña) España.
Showroom
Crta. Santiago-Pontevedra a 9 Km. de Santiago de Compostela en dirección a Pontevedra. 15.866 Ameneiro-Teo (La Coruña) España.
To see these in stereo, use the cross-eyed technique.
The highly inclined sedimentary rock units are part of the Twist Gulch Formation of Middle Jurassic age. They consist of fairly friable siltstones and fine grained sandstones. Laying unconformably on top of the Twist Gulch Formation are the lighter horizontal beds of the Mid-Paleocene Flagstaff Formation. These light colored beds are primarily sandstones.
Above the Flagstaff formation lie the Colton Formation, and the Green River Formation (upper Paleocene to Eocene).
GP-9 7554, in the service of the Penn Central Railroad, soaks up some sunshine in the New Haven engine yard, 1971.
24 exposiciones de 90 segundos con teleobjetivo 200 mm f/1.8, ISO 1.600, cámara Canon EOS 6D modificada. Centro, (AR): 18h 22m 21s, (Dec.): -04° 37' 40". Campo angular: 10.5º x 11.1º. Escala: 6.9 arcsec/pixel.
Grieta de Serpens-Aquila (también conocida como la Grieta Aquila). Es una región del cielo en las constelaciones del Águila, de la Cola de la Serpiente , y la occidental Ofiuco que contiene nubes oscuras interestelares. Esta región forma parte de la Gran Grieta, una banda oscura que pasa por el medio del plano de la Vía Láctea.
Las nubes que forman esta estructura son llamadas "nubes moleculares", constituyendo una fase del medio interestelar, el cual es frío y suficientemente denso como para formar, particularmente hidrógeno molecular (H2). Estas nubes son opacas a la luz en la parte visible del espectro debido a la presencia de polvo interestelar mezclado con los componentes gaseosos de las nubes. Por tal razón, las nubes en la grieta de la Serpiente - Águila bloquean la luz de las estrellas del fondo en el disco de la galaxia, formando la grieta oscura. Este complejo está ubicado en dirección hacia el centro de la galaxia, en donde estas nubes moleculares son comunes, así es posible que no todos los componentes de la grieta se encuentren a la misma distancia y físicamente asociados unos con otros.
Varias regiones formadoras de estrellas se proyectan hacia (o cerca) de la dirección de la grieta de la Serpiente- Águila, incluyendo Westerhout 40, la Serpens Main, el Serpens South, Serpiente NH3, y MWC297/SH2-62.
Sh2-60, RCW 173. Es una nebulosa de emisión visible en la constelación del Escudo.
Es una gran región H II situada en el brazo de Sagitario a una distancia de unos 7.200 años luz.
En su dirección se extiende la brillante fuente de ondas de radio W42, en cuya distancia hay cierto desacuerdo: algunas estimaciones sugieren 7.200 años luz, indicando de este modo una clara asociación con Sh2-60, mientras que otras estimaciones sugieren una distancia mucho más grande , hasta unos 43.000 años luz, colocando así a esta fuente cerca del centro galáctico.
En Sh2-60 estaría asociada con dos fuentes fuertes de la radiación infrarroja, RAFGL 5263 y IRAS 18335 y la nube molecular SYCSW 513, identificado a través de sus emisiones a la longitud de onda de CO.
Sh2-59, RCW 172. Es una nebulosa de emisión en la constelación del Escudo.
Se trata de una región H II que constituye la porción iluminada de una extensa burbuja en forma de nebulosidad compleja claramente visible en las imágenes tomadas en la longitud de onda Hα. Su distancia no es conocida con precisión: varía entre 10.000 y 18.000 años luz, con lo que podría situarse en el brazo exterior de Escudo-Centauro. En la misma dirección también se observa la estrella binaria de rayos X Scutum X-1, pero puede tratarse de una efecto de proyección. Según el catálogo Avedisova, Sh2-59 está asociada con la fuente de radiación infrarroja RAFGL 2203 y a una fuente de ondas de radio, que indican la actividad de formación de estrellas.
NGC 6664. Es un cúmulo estelar abierto de Trumpler tipo III2m en la constelación del Escudo. Tiene una magnitud aparente de +7.80 y un diámetro angular aparente de 16 '. Se encuentra a unos 6.200 años luz. Fue descubierto en 1784 por William Herschel.
Sh2-64, W40, RCW 174. Es una nebulosa de emisión en la constelación de la Serpens Cauda; y constituye una de las regiones más cercanas de formación estelar.
Forma parte de una importante región de formación de estrellas, combinado con la brillante W40 fuente de radio, en el que se originan las estrellas masivas; sin embargo, debido a su fuerte oscurecimiento por la nebulosidad oscura Grieta Serpens-Aquila, ha sido poco estudiada hasta hace poco. La nebulosa recibe la radiación ionizante de algunas estrellas jóvenes y masivas como OS1a W40, W40 y W40 OS2a OS3a, todo ello rodeado por un disco protoplanetario. Las estimaciones de su distancia son unos 1.300 años luz).
Los estudios realizados por el telescopio espacial de rayos X Chandra han identificado 194 fuentes de rayos X casi con toda seguridad asociados con W40, coincidente con el mayor número de objetos estelares jóvenes; las estrellas de la secuencia pre-principal identificadas en esta región son aproximadamente 600 y se agrupan en un grupo joven abierto por su forma esférica inmersos en la nube de gas y fuertemente oscurecida por los bancos de polvo interestelar de la región.
α Scuti (α Sct/HD 171443/HR 6973). Es la estrella más brillante de la constelación del Escudo. Recibe el nombre, de origen griego, Ionnina or Ioannina (Ιωάννινα), que literalmente significa «de Juan», aunque probablemente el nombre se refiere al diseño de «Escudo dentro de un escudo» del blasón de Sobieski, conocido como diseño «Janina».
Situada a 199 años luz, es una gigante naranja de tipo espectral K3III. Es 132 veces más luminosa que el Sol y su radio es 21 veces más grande que el radio solar.
Alfa Scuti es una estrella variable cuyo brillo varía entre magnitud 3,81 y 3,87. Se desconoce su período de oscilación —si es que tiene alguno— y la clase de variable que es.
B101. Es una nebulosa oscura en la constelación del Escudo, incluida en el catálogo de Barnard y descrita como “definida, irregular de 13’ x 4’ separada de la nebulosa B100 por un grupo disperso de estrellas”.
B100. Es una nebulosa oscura en la constelación del Escudo, incluida en el catálogo de Barnard y descrita como “definida, irregular, curvada de 16’ de largo. Más amplia en la zona final del sur.”
η Serpentis (58 Serpentis / HD 168723). Es una estrella en la constelación de Serpens de magnitud aparente +3,26. Situada en Serpens Cauda —la cola de la serpiente—, es la segunda estrella más brillante del conjunto de la constelación, solo superada por Unukalhai (α Serpentis). Si bien no tiene nombre propio habitual, ocasionalmente recibe el nombre de Tang, del mandarín 唐朝 "Táng Cháo", por la dinastía imperial Tang.
Situada a 60,5 años luz del sistema solar, Eta Serpentis es una gigante naranja. Su luminosidad bolométrica —en todas las longitudes de onda— es 19 veces mayor que la luminosidad solar y su diámetro unas seis veces más grande que el del Sol.
Eta Serpentis tiene un contenido metálico inferior al del Sol. Hace unos 150 millones de años terminó la fusión de su hidrógeno interno y probablemente esté aumentando en brillo con un núcleo inerte de helio; cuando en un futuro se convierta en una gigante roja, será 25 veces más luminosa que en la actualidad.
IC 1276, Palomar 7. Es un cúmulo globular situado a unos 17.600 años luz en la constelación de la Serpiente. Fue descubierto en 1889 por Lewis Swift. Independientemente en 1952, este cúmulo fue redescubierto por George Abell y catalogado en el Catálogo Palomar como Palomar 7.
NGC 6539, también GCL 85. Es un cúmulo globular en la constelación de Serpens. Fue descubierto por Theodor Brorsen en 1856. Dista unos 7.800 años luz.
24 exposures of 90 seconds with telephoto lens 200 mm f / 1.8, ISO 1,600, Canon EOS 6D camera modified. Center, (AR): 18h 22m 21s,
(Dec.): -04 ° 37 '40 ". Angular field: 10.5º x 11.1º.Scale: 6.9 arcsec / pixel.
Serpens-Aquila Rift (also known as Aquila Rift). It is a region of the sky in the constellations of the Eagle, the Tail of the Serpent, and the western Ophiuchus that contains dark interstellar clouds. This region is part of the Great Crack, a dark band that passes through the middle of the plane of the Milky Way.
The clouds that form this structure are called "molecular clouds", constituting a phase of the interstellar medium, which is cold and sufficiently dense to form, particularly molecular hydrogen (H2). These clouds are opaque to light in the visible part of the spectrum due to the presence of interstellar dust mixed with the gaseous components of the clouds. For this reason, the clouds in the crack of the Serpent - Eagle block the light of the bottom stars in the disk of the galaxy, forming the dark crack. This complex is located towards the center of the galaxy, where these molecular clouds are common, so it is possible that not all the components of the crack are at the same distance and physically associated with each other.
Several star-forming regions are projected toward (or near) the direction of the crack of the Serpent-Eagle, including Westerhout 40, Serpens Main, Serpens South, Serpent NH3, and MWC297 / SH2-62.
Sh2-60, RCW 173. It is a visible emission nebula in the Shield constellation.
It is a large H II region located in the arm of Sagittarius at a distance of about 7,200 light years.
In its direction extends the bright source of radio waves W42, at whose distance there is some disagreement: some estimates suggest 7,200 light years, indicating in this way a clear association with Sh2-60, while other estimates suggest a much larger distance , up to about 43,000 light years, placing this source near the galactic center.
In Sh2-60 it would be associated with two strong sources of infrared radiation, RAFGL 5263 and IRAS 18335 and the molecular cloud SYCSW 513, identified through its emissions at the CO wavelength.
Sh2-59, RCW 172. It is an emission nebula in the Shield constellation.
It is an H II region that constitutes the illuminated portion of an extensive bubble in the form of complex nebulosity clearly visible in the images taken at the Hα wavelength. Its distance is not known with precision: it varies between 10,000 and 18,000 light years, with what could be located in the outer arm of Escudo-Centauro. In the same direction, the binary X-ray star Scutum X-1 is also observed, but it may be a projection effect. According to the Avedisova catalog, Sh2-59 is associated with the source of infrared radiation RAFGL 2203 and a source of radio waves, which indicate the activity of star formation.
NGC 6664. It is an open stellar cluster of Trumpler type III2m in the Shield constellation. It has an apparent magnitude of +7.80 and an apparent angular diameter of 16 '. It is about 6,200 light years away. It was discovered in 1784 by William Herschel.
Sh2-64, W40, RCW 174. It is an emission nebula in the constellation of Serpens Cauda; and constitutes one of the closest regions of star formation.
It is part of an important star formation region, combined with the brilliant W40 radio source, in which massive stars originate; however, due to its strong obscuration by the dark nebulosity Serpens-Aquila Crack, it has been little studied until recently. The nebula receives the ionizing radiation of some young and massive stars like OS1a W40, W40 and W40 OS2a OS3a, all surrounded by a protoplanetary disk. The estimates of its distance are about 1,300 light years).
Studies conducted by the Chandra X-ray space telescope have identified 194 X-ray sources almost certainly associated with W40, coinciding with the largest number of young stellar objects; The stars of the pre-main sequence identified in this region are approximately 600 and are grouped in a young group opened by its spherical shape immersed in the gas cloud and strongly obscured by interstellar dust banks in the region.
Scuti α (α Sct / HD 171443 / HR 6973). It is the brightest star in the Shield constellation. It receives the name, of Greek origin, Ionnina or Ioannina (Ιωάννινα), which literally means «de Juan», although probably the name refers to the design of «Shield inside a shield» of the Sobieski coat of arms, known as «Janina» design .
Located at 199 light years, it is an orange giant of spectral type K3III. It is 132 times brighter than the Sun and its radius is 21 times larger than the solar radius.
Alpha Scuti is a variable star whose brightness varies between 3.81 and 3.87 magnitude. Its oscillation period is unknown -if it has any- and the kind of variable it is.
B101 It is a dark nebula in the constellation of the Shield, included in the Barnard catalog and described as "defined, irregular 13 'x 4' separated from the B100 nebula by a scattered group of stars."
B100 It is a dark nebula in the constellation of the Shield, included in the Barnard catalog and described as "defined, irregular, curved 16 'long. Wider in the southern end zone. "
η Serpentis (58 Serpentis / HD 168723). It is a star in the constellation of Serpens of apparent magnitude +3.26. Located in Serpens Cauda - the tail of the serpent -, it is the second brightest star in the constellation, only surpassed by Unukalhai (α Serpentis). Although it does not have its own proper name, it occasionally receives the name Tang, from the Mandarin 唐朝 "Táng Cháo", by the Tang imperial dynasty.
Located at 60.5 light years from the solar system, Eta Serpentis is an orange giant. Its bolometric luminosity -in all wavelengths- is 19 times greater than the solar luminosity and its diameter is six times larger than that of the Sun.
Eta Serpentis has a metallic content lower than that of the Sun. About 150 million years ago it finished the fusion of its internal hydrogen and is probably increasing in brightness with an inert nucleus of helium; when in the future it becomes a red giant, it will be 25 times more luminous than at present.
IC 1276, Palomar 7. It is a globular cluster located about 17,600 light years in the constellation of the Serpent. It was discovered in 1889 by Lewis Swift. Independently in 1952, this cluster was rediscovered by George Abell and cataloged in the Palomar Catalog as Palomar 7.
NGC 6539, also GCL 85. It is a globular cluster in the constellation of Serpens. It was discovered by Theodor Brorsen in 1856. It is about 7,800 light years away.
Click 'L' please. :)
From my last trip to Detroit. Have a few I may post over the next few weeks now that I know which ones will not be in the show. Friday Fave mosaic coming later!