View allAll Photos Tagged consistent
Satisfactoriamente avanzan las obras de infraestructura adelantadas por Prosperidad Social en los municipios de Villanueva y La Jagua del Pilar al Sur de La Guajira, consistentes en la construcción y renovación de tres parques y la pavimentación de más de mil metros viales en el barrio El Paraíso, respectivamente.
Así lo evidenció el director general de Prosperidad Social, Nemesio Roys Garzón, quien hizo un recorrido por las obras junto a la comunidad y autoridades locales de los dos municipios en donde se ejecutan estas obras con una inversión superior a los $8.300 millones.
"Estos proyectos de infraestructura llevan calidad de vida a la población de estos dos municipios del Sur de La Guajira, los terminaremos este año satisfactoriamente y están incluidos en las 65 obras que de manera histórica estamos ejecutando en el departamento con una inversión superior a los $128.000 millones durante el gobierno del presidente Santos", afirmó el director general de Prosperidad Social, Nemesio Roys Garzón.
El proyecto de construcción y remodelación de los parques 6 de Abril, La Fe y Román Ovalle en Villanueva registra un avance de cerca del 45%, beneficiará a más de 19 mil habitantes con una inversión superior a los $6.400 millones. Los espacios deportivos cuentan con cancha polideportiva, sintética y sistema de gimnasio biosaludable, brindando a la población
escenarios de encuentro, ampliando el potencial cultural y deportivo del municipio.
Por su parte, el proyecto de construcción de más de 1.000 metros de pavimento vial en el barrio El Paraíso en La Jagua del Pilar, registra un avance del 92% e incluye además la construcción de más de 1.000 metros de andenes, zonas verdes y señalización con una inversión de $1.905 millones.
La obra mejorará la calidad de vida de la comunidad que ya no padecerá afectaciones por el polvo o el encharcamiento en época de invierno. Se mejorará la conectividad del barrio con otros sectores, optimizando y reduciendo tiempos de desplazamiento. La obra, generó 35 empleos y beneficiará a unas 170 familias del barrio El Paraíso.
En La Jagua del Pilar también iniciará próximamente el mejoramiento de condiciones de vivienda de 100 hogares.
Villanueva Seguimiento Obra Parque 6 de Abril. / Abr. 27, 2018. (Fotografía Oficial Prosperidad Social / Joel González).
Esta fotografía oficial del Departamento Administrativo para la Prosperidad Social está disponible sólo para ser publicada por las organizaciones de noticias, medios nacionales e internacionales y/o para uso personal de impresión por el sujeto de la fotografía. La fotografía no puede ser alterada digitalmente o manipularse de ninguna manera, y tampoco puede usarse en materiales comerciales o políticos, anuncios, correos electrónicos, productos o promociones que de cualquier manera sugieran aprobación por parte del Departamento Administrativo para la Prosperidad Social.
Prosperidad Social Página Web / Twitter / Facebook / Youtube / Instagram
5 Jan 2025, 03:33 UT; Spotsylvania, Virginia USA. Bortle 4.5 zone.
Celestron C8 SCT at f/10.1. Orion Atlas AZ/EQ-G mount. Mallincam DS26cTEC camera, bin 1x1, exposure 16s, single frame, Optolong L'eNhance filter, no guiding, no calibration frames, sensor -5°C. Captured in Sharpcap Pro. Processed in PixInsight and Photoshop.
IDENTIFICATION OF Rigel BC
In the absence of a plate-solved location for Rigel BC the following information was considered:
1. Positive -- Published position angle (202° East of North) is consistent with labelled BC. Per ASTAP this image does not have standard orientation, e.g. it does not show North in the standard position -- up (0°). A corrected image would be rotated 7° and flipped on the horizontal axis for standard alignment with North, which puts the labelled star near the correct position.
2. Negative -- The brightest star in the field (besides Rigel A) is magnitude 6.35 and the nearby dimmer stars are approx. magnitude 10. The image of the labelled star BC (magnitude 7.5) is between them in size (brightness) but appears closer to magnitude 10 than 6.
3. Negative -- The separation of A from labelled BC in the image is roughly estimated from the image at 1 arcmin, not the expected 0.16 arcmin (9.5 arcsec).
4. Positive -- It is consistent with other posted amateur images of Rigel A & B.
BOTTOM LINE
I have 80% confidence that Rigel BC is correctly identified in this image, but another star could be obscured in the asymmetrical flare. An occulting bar may be used to verify dim Rigel BC against its brilliant companion in a subsequent image.
Appearance: Bright light blue star (Rigel A) and dim companions (Rigel B, C, and D), with adjacent variable star λ Eri (magnitude 6.35) at 3:00 position. The severe halo/flare around Rigel may be due to the filter, and may be asymmetrical due to moderate sensor tilt in the system.
Clouds: clear
Transparency: average
Seeing: below average
Apparent Magnitude (USNO): A 0.5-0.18, BC 7.5-7.6
Separation A-BC: 9.5 arcsec
Image scale:
Moon age, illuminated: xx, xx
Azimuth: xx°
Altitude: xx°
from Wikipedia
Rigel is a blue supergiant star in the constellation of Orion. It has the Bayer designation β Orionis, which is Latinized to Beta Orionis and abbreviated Beta Ori or β Ori. Rigel is the brightest and most massive component – and the eponym – of a star system of at least four stars that appear as a single blue-white point of light to the naked eye. This system is located at a distance of approximately 860 light-years (260 pc) from the Sun.
A star of spectral type B8Ia, Rigel is 120,000 times as luminous as the Sun, and is 18 to 24 times as massive, depending on the method and assumptions used. Its radius is more than seventy times that of the Sun, and its surface temperature is 12,100 K. Due to its stellar wind, Rigel's mass-loss is estimated to be ten million times that of the Sun. With an estimated age of seven to nine million years, Rigel has exhausted its core hydrogen fuel, expanded, and cooled to become a supergiant. It is expected to end its life as a type II supernova, leaving a neutron star or a black hole as a final remnant, depending on the initial mass of the star.
Rigel varies slightly in brightness, its apparent magnitude ranging from 0.05 to 0.18. It is classified as an Alpha Cygni variable due to the amplitude and periodicity of its brightness variation, as well as its spectral type. Its intrinsic variability is caused by pulsations in its unstable atmosphere. Rigel is generally the seventh-brightest star in the night sky and the brightest star in Orion, though it is occasionally outshone by Betelgeuse, which varies over a larger range.
A triple-star system is separated from Rigel by an angle of 9.5 arc seconds. It has an apparent magnitude of 6.7, making it 1/400th as bright as Rigel. Two stars in the system can be seen by large telescopes, and the brighter of the two is a spectroscopic binary. These three stars are all blue-white main-sequence stars, each three to four times as massive as the Sun. Rigel and the triple system orbit a common center of gravity with a period estimated to be 24,000 years. The inner stars of the triple system orbit each other every 10 days, and the outer star orbits the inner pair every 63 years. A much fainter star, separated from Rigel and the others by nearly an arc minute, may be part of the same star system.
In 2016, the International Astronomical Union (IAU) included the name "Rigel" in the IAU Catalog of Star Names. According to the IAU, this proper name applies only to the primary component A of the Rigel system. The system is listed variously in historical astronomical catalogs as H II 33, Σ 668, β 555, or ADS 3823. For simplicity, Rigel's companions are referred to as Rigel B, C, and D; the IAU describes such names as "useful nicknames" that are "unofficial". In modern comprehensive catalogs, the whole multiple star system is known as WDS 05145-0812 or CCDM 05145–0812.
The designation of Rigel as β Orionis (Latinized to beta Orionis) was made by Johann Bayer in 1603. The "beta" designation is usually given to the second-brightest star in each constellation, but Rigel is almost always brighter than α Orionis (Betelgeuse). Astronomer J.B. Kaler speculated that Bayer assigned letters during a rare period when variable star Betelgeuse temporarily outshone Rigel, resulting in Betelgeuse being designated "alpha" and Rigel designated "beta". However, closer examination of Bayer's method shows that he did not strictly order the stars by brightness, but instead grouped them first by magnitude, then by declination. Rigel and Betelgeuse were both classed as first magnitude, and in Orion the stars of each class appear to have been ordered north to south.
Rigel has many other stellar designations taken from various catalogs, including the Flamsteed 19 Orionis (19 Ori), the Bright Star Catalogue entry HR 1713, and the Henry Draper Catalogue number HD 34085. These designations frequently appear in the scientific literature,[ but rarely in popular writing. Rigel is listed in the General Catalogue of Variable Stars, but since its familiar Bayer designation is used instead of creating a separate variable star designation.
Rigel is an intrinsic variable star with an apparent magnitude ranging from 0.05 to 0.18. It is typically the seventh-brightest star in the celestial sphere, excluding the Sun, although occasionally fainter than Betelgeuse. Rigel appears slightly blue-white and has a B-V color index of −0.06. It contrasts strongly with reddish Betelgeuse.
Culminating every year at midnight on 12 December, and at 9:00 pm on 24 January, Rigel is visible on winter evenings in the Northern Hemisphere and on summer evenings in the Southern Hemisphere. In the Southern Hemisphere, Rigel is the first bright star of Orion visible as the constellation rises. Correspondingly, it is also the first star of Orion to set in most of the Northern Hemisphere. The star is a vertex of the "Winter Hexagon", an asterism that includes Aldebaran, Capella, Pollux, Procyon, and Sirius. Rigel is a prominent equatorial navigation star, being easily located and readily visible in all the world's oceans (the exception is the area north of the 82nd parallel north).
Rigel's spectral type is a defining point of the classification sequence for supergiants.[36][37] The overall spectrum is typical for a late B class star, with strong absorption lines of the hydrogen Balmer series as well as neutral helium lines and some of heavier elements such as oxygen, calcium, and magnesium.[38] The luminosity class for B8 stars is estimated from the strength and narrowness of the hydrogen spectral lines, and Rigel is assigned to the bright supergiant class Ia.[39] Variations in the spectrum have resulted in the assignment of different classes to Rigel, such as B8 Ia, B8 Iab, and B8 Iae.
As early as 1888, the heliocentric radial velocity of Rigel, as estimated from the Doppler shifts of its spectral lines, was seen to vary. This was confirmed and interpreted at the time as being due to a spectroscopic companion with a period of about 22 days. The radial velocity has since been measured to vary by about 10 km/s around a mean of 21.5 km/s.
In 1933, the Hα line in Rigel's spectrum was seen to be unusually weak and shifted 0.1 nm towards shorter wavelengths, while there was a narrow emission spike about 1.5 nm to the long wavelength side of the main absorption line. This is now known as a P Cygni profile after a star that shows this feature strongly in its spectrum. It is associated with mass loss where there is simultaneously emission from a dense wind close to the star and absorption from circumstellar material expanding away from the star.
The unusual Hα line profile is observed to vary unpredictably. It is a normal absorption line around a third of the time. About a quarter of the time, it is a double-peaked line, that is, an absorption line with an emission core or an emission line with an absorption core. About a quarter of the time it has a P Cygni profile; most of the rest of the time, the line has an inverse P Cygni profile, where the emission component is on the short wavelength side of the line. Rarely, there is a pure emission Hα line. The line profile changes are interpreted as variations in the quantity and velocity of material being expelled from the star. Occasional very high-velocity outflows have been inferred, and, more rarely, infalling material. The overall picture is one of large looping structures arising from the photosphere and driven by magnetic fields.
Rigel has been known to vary in brightness since at least 1930. The small amplitude of Rigel's brightness variation requires photoelectric or CCD photometry to be reliably detected. This brightness variation has no obvious period. Observations over 18 nights in 1984 showed variations at red, blue, and yellow wavelengths of up to 0.13 magnitudes on timescales of a few hours to several days, but again no clear period. Rigel's color index varies slightly, but this is not significantly correlated with its brightness variations.
From analysis of Hipparcos satellite photometry, Rigel is identified as belonging to the Alpha Cygni class of variable stars, defined as "non-radially pulsating supergiants of the Bep–AepIa spectral types". In those spectral types, the 'e' indicates that it displays emission lines in its spectrum, while the 'p' means it has an unspecified spectral peculiarity. Alpha Cygni type variables are generally considered to be irregular or have quasi-periods. Rigel was added to the General Catalogue of Variable Stars in the 74th name-list of variable stars on the basis of the Hipparcos photometry, which showed variations with a photographic amplitude of 0.039 magnitudes and a possible period of 2.075 days. Rigel was observed with the Canadian MOST satellite for nearly 28 days in 2009. Milli-magnitude variations were observed, and gradual changes in flux suggest the presence of long-period pulsation modes.
From observations of the variable Hα spectral line, Rigel's mass-loss rate due to stellar wind is estimated be (1.5±0.4)×10−7 solar masses per year (M☉/yr)—about ten million times more than the mass-loss rate from the Sun.[52] More detailed optical and K band infrared spectroscopic observations, together with VLTI interferometry, were taken from 2006 to 2010. Analysis of the Hα and Hγ line profiles, and measurement of the regions producing the lines, show that Rigel's stellar wind varies greatly in structure and strength. Loop and arm structures were also detected within the wind. Calculations of mass loss from the Hγ line give (9.4±0.9)×10−7 M☉/yr in 2006-7 and (7.6±1.1)×10−7 M☉/yr in 2009–10. Calculations using the Hα line give lower results, around 1.5×10−7 M☉/yr. The terminal wind velocity is 300 km/s. It is estimated that Rigel has lost about three solar masses (M☉) since beginning life as a star of 24±3 M☉ seven to nine million years ago.
Rigel's distance from the Sun is somewhat uncertain, different estimates being obtained by different methods. Old estimates placed it 166 parsecs (or 541 light years) away from the Sun. The 2007 Hipparcos new reduction of Rigel's parallax is 3.78±0.34 mas, giving a distance of 863 light-years (265 parsecs) with a margin of error of about 9%. Rigel B, usually considered to be physically associated with Rigel and at the same distance, has a Gaia Data Release 3 parallax of 3.2352±0.0553 mas, suggesting a distance around 1,000 light-years (310 parsecs). However, the measurements for this object may be unreliable.
Indirect distance estimation methods have also been employed. For example, Rigel is believed to be in a region of nebulosity, its radiation illuminating several nearby clouds. Most notable of these is the 5°-long IC 2118 (Witch Head Nebula), located at an angular separation of 2.5° from the star, or a projected distance of 39 light-years (12 parsecs) away. From measures of other nebula-embedded stars, IC 2118's distance is estimated to be 949 ± 7 light-years (291 ± 2 parsecs).
Rigel is an outlying member of the Orion OB1 association, which is located at a distance of up to 1,600 light-years (500 parsecs) from Earth. It is a member of the loosely defined Taurus-Orion R1 Association, somewhat closer at 1,200 light-years (360 parsecs). Rigel is thought to be considerably closer than most of the members of Orion OB1 and the Orion Nebula. Betelgeuse and Saiph lie at a similar distance to Rigel, although Betelgeuse is a runaway star with a complex history and might have originally formed in the main body of the association.
The star system of which Rigel is a part has at least four components. Rigel (sometimes called Rigel A to distinguish from the other components) has a visual companion, which is likely a close triple-star system. A fainter star at a wider separation might be a fifth component of the Rigel system.
William Herschel discovered Rigel to be a visual double star on 1 October 1781, cataloguing it as star 33 in the "second class of double stars" in his Catalogue of Double Stars, usually abbreviated to H II 33, or as H 2 33 in the Washington Double Star Catalogue.
Friedrich Georg Wilhelm von Struve first measured the relative position of the companion in 1822, cataloguing the visual pair as Σ 668. The secondary star is often referred to as Rigel B or β Orionis B. The angular separation of Rigel B from Rigel A is 9.5 arc seconds to its south along position angle 204°. Although not particularly faint at visual magnitude 6.7, the overall difference in brightness from Rigel A (about 6.6 magnitudes or 440 times fainter) makes it a challenging target for telescope apertures smaller than 15 cm (6 in).
At Rigel's estimated distance, Rigel B's projected separation from Rigel A is over 2,200 astronomical units (AU). Since its discovery, there has been no sign of orbital motion, although both stars share a similar common proper motion. The pair would have an estimated orbital period of 24,000 years. Gaia Data Release 2 (DR2) contains a somewhat unreliable parallax for Rigel B, placing it at about 1,100 light-years (340 parsecs), further away than the Hipparcos distance for Rigel, but similar to the Taurus-Orion R1 association. There is no parallax for Rigel in Gaia DR2. The Gaia DR2 proper motions for Rigel B and the Hipparcos proper motions for Rigel are both small, although not quite the same.
In 1871, Sherburne Wesley Burnham suspected Rigel B to be a binary system, and in 1878, he resolved it into two components. This visual companion is designated as component C (Rigel C), with a measured separation from component B that varies from less than 0.1″ to around 0.3″. In 2009, speckle interferometry showed the two almost identical components separated by 0.124″, with visual magnitudes of 7.5 and 7.6, respectively. Their estimated orbital period is 63 years. Burnham listed the Rigel multiple system as β 555 in his double star catalog or BU 555 in modern use.
Component B is a double-lined spectroscopic binary system, which shows two sets of spectral lines combined within its single stellar spectrum. Periodic changes observed in relative positions of these lines indicate an orbital period of 9.86 days. The two spectroscopic components Rigel Ba and Rigel Bb cannot be resolved in optical telescopes but are known to both be hot stars of spectral type around B9. This spectroscopic binary, together with the close visual component Rigel C, is likely a physical triple-star system, although Rigel C cannot be detected in the spectrum, which is inconsistent with its observed brightness.
In 1878, Burnham found another possibly associated star of approximately 13th magnitude. He listed it as component D of β 555, although it is unclear whether it is physically related or a coincidental alignment. Its 2017 separation from Rigel was 44.5″, almost due north at a position angle of 1°.[8] Gaia DR2 finds it to be a 12th magnitude sunlike star at approximately the same distance as Rigel. Likely a K-type main-sequence star, this star would have an orbital period of around 250,000 years, if it is part of the Rigel system.
A spectroscopic companion to Rigel was reported on the basis of radial velocity variations, and its orbit was even calculated, but subsequent work suggests the star does not exist and that observed pulsations are intrinsic to Rigel itself.
Rigel is a blue supergiant that has exhausted the hydrogen fuel in its core, expanded and cooled as it moved away from the main sequence across the upper part of the Hertzsprung–Russell diagram. When it was on the main sequence, its effective temperature would have been around 30,000 K. Rigel's complex variability at visual wavelengths is caused by stellar pulsations similar to those of Deneb. Further observations of radial velocity variations indicate that it simultaneously oscillates in at least 19 non-radial modes with periods ranging from about 1.2 to 74 days.
Estimation of many physical characteristics of blue supergiant stars, including Rigel, is challenging due to their rarity and uncertainty about how far they are from the Sun. As such, their characteristics are mainly estimated from theoretical stellar evolution models. Its effective temperature can be estimated from the spectral type and color to be around 12,100 K. A mass of 21±3 M☉ at an age of 8±1 million years has been estimated by comparing evolutionary tracks, while atmospheric modeling from the spectrum gives a mass of 24±8 M☉.
Although Rigel is often considered the most luminous star within 1,000 light-years of the Sun, its energy output is poorly known. Using the Hipparcos distance of 860 light-years (264 parsecs), the estimated relative luminosity for Rigel is about 120,000 times that of the Sun (L☉), but another recently published distance of 1,170 ± 130 light-years (360 ± 40 parsecs) suggests an even higher luminosity of 219,000 L☉. Other calculations based on theoretical stellar evolutionary models of Rigel's atmosphere give luminosities anywhere between 83,000 L☉ and 363,000 L☉, while summing the spectral energy distribution from historical photometry with the Hipparcos distance suggests a luminosity as low as 61,515±11,486 L☉.
A 2018 study using the Navy Precision Optical Interferometer measured the angular diameter as 2.526 mas. After correcting for limb darkening, the angular diameter is found to be 2.606±0.009 mas, yielding a radius of 74.1+6.1−7.3 R☉. An older measurement of the angular diameter gives 2.75±0.01 mas, equivalent to a radius of 78.9 R☉ at 264 pc. These radii are calculated assuming the Hipparcos distance of 264 pc; adopting a distance of 360 pc leads to a significantly larger size. Older distance estimates were mostly far lower than modern estimates, leading to lower radius estimates; a 1922 estimate by John Stanley Plaskett gave Rigel a diameter of 25 million miles, or approximately 28.9 R☉, smaller than its neighbor Aldebaran.
Due to their closeness to each other and ambiguity of the spectrum, little is known about the intrinsic properties of the members of the Rigel BC triple system. All three stars seem to be near equally hot B-type main-sequence stars that are three to four times as massive as the Sun.
Stellar evolution models suggest the pulsations of Rigel are powered by nuclear reactions in a hydrogen-burning shell that is at least partially non-convective. These pulsations are stronger and more numerous in stars that have evolved through a red supergiant phase and then increased in temperature to again become a blue supergiant. This is due to the decreased mass and increased levels of fusion products at the surface of the star.
Rigel is likely to be fusing helium in its core. Due to strong convection of helium produced in the core while Rigel was on the main sequence and in the hydrogen-burning shell since it became a supergiant, the fraction of helium at the surface has increased from 26.6% when the star formed to 32% now. The surface abundances of carbon, nitrogen, and oxygen seen in the spectrum are compatible with a post-red supergiant star only if its internal convection zones are modeled using non-homogeneous chemical conditions known as the Ledoux Criteria.
Rigel is expected to eventually end its stellar life as a type II supernova. It is one of the closest known potential supernova progenitors to Earth, and would be expected to have a maximum apparent magnitude of around −11 (about the same brightness as a quarter Moon or around 300 times brighter than Venus ever gets). The supernova would leave behind either a black hole or a neutron star.
El Gran Combo De Puerto Rico* – Sin Salsa No Hay Paraiso" 2010 CD MIX
VEAN/SEE VIDEO youtu.be/K8WMNTBkX4s
PARA CONTRATACIONES 787-799-4613
Genre: Latin
Style: Salsa, Son
Year: 2010
Tracklist
Sin Salsa No Hay Paraiso 3:47
El Problema Esta En El Coco 3:46
El Comejen 5:02
La Espuma Y La Ola 5:06
A Mi Me Gusta Mi Pueblo 4:48
Es La Mujer 4:14
Alguien Que Me Quite Tu Amor 4:41
Achilipu 4:42
Colombia Tierra Querida 4:39
La Receta De Amor 4:07
Review by Jason Birchmeier
A half-century into their recording career, El Gran Combo de Puerto Rico are still one of the leading salsa acts in Latin music, which is all the more remarkable when you consider that founder and bandleader Rafael Ithier was well into his eighties when he and his orchestra released Sin Salsa No Hay Paraíso. The third full-length studio album released since Gran Combo de Puerto Rico left Combo Records at the turn of the century, after a quarter-century of releasing a new studio album more or less every year on the label, Sin Salsa No Hay Paraíso is no less exciting than its predecessors, Aquí Estamos y...¡de Verdad! (2004) and Arroz con Habichuela (2006), the latter of which won the group a Latin Grammy award for Best Tropical Album. The title track of Sin Salsa No Hay Paraíso storms out of the gate as the album opener. One of El Gran Combo's best singles in recent years, "Sin Salsa No Hay Paraíso" is straight fire and sets the album aflame from the get-go. While none of the subsequent tracks on the ten-track album measure up to the stand-out title track, there are plenty of highlights, among them a new version of "Achilipú," which was originally released on the classic album De Punta a Punta (1971), and "Colombia Tierra Querida." Fans of El Gran Combo know what to expect on Sin Salsa No Hay Paraíso, as this group is nothing if not consistent, and the album doesn't disappoint, the title track in particular.
photograph by stacey lundeen. project #35 by Iris Taborsky-Tasa.
from the Consistent Variable Project - first attempt.
Audi consistently applies various efficiency measures. Audi A8 L is India dependable best performance model with latest features & long wheel-base luxury car at affordable price.
www.audidelhisouth.com/in_partner/p_30201/en/models/a8/a8...
15AUG2012:Imzadi is fit as a fiddle after consistent training for 6 1/2 months. Now I have to get back in shape after a foot injury (not caused by Imzadi).
Imzadi says: "Do you think this bridle makes my nose look long?". I'll have my first lesson in a year next week. There is a covered arena with special shock absorbing footing.
The barefoot trim for these conditions requires a pronounced mustang roll. It requires specialized knowledge to keep a barefoot draft in soft wet conditions like this but it is easy on her joints. I do miss being out west where all you needed to do was get a trim every 6 weeks. Picking was a bad word out there.
The 53rd annual Bon Odori Festival at Camp Zama was held Aug. 4. The festival is consistently the largest bilateral event of the year for U.S. Army Japan, this year attracting more than 30,000 visitors to the installation. The festival featured live entartainment, games for children, a variety of ethnic foods, bilateral sports, and a fireworks show.
About the United States Army Garrison Japan:
The United States Army Garrison Japan and its 16 supported installation sites are located in the island of Honshu and Okinawa in Japan. The USAG Japan mission is to support the Headquarters, U.S. Army Japan / I Corps (fwd) to ensure mission readiness and the quality of life of the Army community in a sustainable, transforming joint and combined environment.
The USAG-J area of responsibility spans 1,500 miles from north to south of Japan. Camp Zama, home for both HQ USARJ and USAG-J is located approximately 25 miles southwest of Tokyo in the cities of Zama and Sagamihara in Kanagawa Prefecture, Japan. The Camp Zama base cluster includes Sagamihara Housing Area and Sagami General Depot.
Akasaka Press Center is located in the center of Tokyo. The Akizuki/Kure area near Hiroshima is an ammunition depot. Yokohama North Dock is a port facility in the city of Yokohama, a major commerce port and a popular shopping area. USAG Torii Station is located 980 miles southwest of Camp Zama on the island of Okinawa.
We are the Army's home in Japan and the "Garrison of Choice" for Soldiers, Civilians and their Family members. We are committed in becoming the leader in the U.S. Army Installation Management Command by providing world-class installation services.
-----
To learn more about USAG Japan, please visit:
Official Website - www.usagj.jp.pac.army.mil
Facebook - www.facebook.com/usagj
Flickr - www.flickr.com/usagj
YouTube - www.youtube.com/usagjapan
Vimeo - www.vimeo.com/usagj
Twitter - www.twitter.com/usagjapan
Slideshare - www.slideshare.net/usagjapan
USARJ This Week on YouTube - www.youtube.com/usarjthisweek
Apparently, this is his "spot" - even the pose is almost identical to four days before.
Scanned from film.
A juzgar por las figuraciones heráldicas existentes en la catedral, consistentes en castillos y torres, se supone que las obras del claustro de la catedral de Tarragona se iniciaron bajo la prelatura de los obispos Ramón de Castellterçol y Ramón de Rocabertí, hacia 1194. Otras teorías, sin embargo, apuntan hacia el canónigo Berenguer de Castellet, y sitúan el inicio de las obras hacia 1214. En cualquier caso, el aludido Ramón de Rocabertí legó en su testamento la importante cantidad de 1000 sueldos para las obras del claustro.
El claustro se encuentra situado en la parte nordeste de la catedral, con planta rectangular de cuarenta y siete metros por cuarenta y seis, consta de cuatro galerías de seis tramos más los angulares comunes. Las divisiones quedan patentes por medio de pilares cuyos contrafuertes se asientan en el jardín del claustro. Parte de ellos incluyen canalones que vertían las aguas pluviales en dirección a la antigua cloaca romana, que se hallaba todavía en uso. Cubiertas con bóvedas de crucería siguiendo la tipología de los monasterios de Poblet y Vallbona de les Monges y con un gran patio central. Sus arcadas estas construidas por dos órdenes de soporte, en el superior hay grandes arcos ojivales ciegos con dos óculos de tracería calada colocados en el vértice central además de un friso con elementos polilobulados de ascendencia musulmana, que recorre toda la cornisa. En la parte inferior se distribuyen grupos de tres arcos de medio punto, decorados con puntas de diamante, sobre dobles columnas dentro de cada arco ojival ciego.
La decoración escultórica del claustro es extensa y se encuentra en los capiteles, impostas, en las bases, los frisos de los pilares angulares así como en los canecillos de la cornisa, en las ménsulas y en sus claves de bóveda.
Consistent: explosion (a) propels shrapnel into mouth 2, which triggers the explosion and closes the loop.
Inconsistent: explosion (b) paradoxically destroys both stages.
After Igor D. Novikov, 'Time Machine and Self-consistent Evolution in Problems with Self-interaction', Physical Review D, Vol. 45, No. 6, 1992: 1989-1994.
If it's consistently "bad," should I just keep knitting? I'm toying with the idea of finishing the back before I decide to abandon this completely. I'm trying to relax and go with it. I initially started knitting with circulars and the straights are yielding a slightly better results. I'm in love with the deep olive color.
Update: Washing and blocking helped somewhat; it also helped me to envision some possible solutions. I'm going to try a smaller needle and use the instructions for the medium rather than trying to knit the small.
Consistently ranked as the best Thai restaurant in North America. Here's one reason why. (via Foodspotting)
Royal Auto Spa strives to elevate our clients driving experience by Protecting/Maintaining their vehicles on a consistent basis. Serving Reno, Sparks and all of Washoe County Nevada.
Thomas Contreras
www.instagram.com/royal.autospa.sparks
www.facebook.com/Royal.Auto.Spa.Reno
Reno Ceramic coating
Reno paint correction
Reno boat detailing
Reno Car detailing service
Reno Car waxing service
Reno Clay bar treatment
Auto detailing Reno, Sparks, and Washoe Counties most professional mobile auto detailing company. We offer the most affordable and professional mobile car cleaning services in the area. We have detailing packages starting at $79.99 and go as far as meeting our customers expectations no matter the job.
Car waxing
Our Wash and Wax exterior package "Executive Exterior Detail" is our most popular package. Want to bring back that showroom shine? We apply a High Quality Carnuba Wax to all painted surfaces.
Clay bar treatment
Clay Bar Treatment is a task that is done before applying a wax. Clay Bars are a synthetic resin compound that can be flattened and used on exterior surfaces to "lift" any embedded contaminants that prevent any protection being applied such as a wax; properly.
Reno Exhaust tip polishing
Reno Full body wash
Reno Headlight polishing
Reno Interior scenting
Reno Interior vacuuming
Reno Seat shampooing
Reno Steam cleaning
Reno Wheel washing
Reno Ceramic Coating
Reno Paint Correction
Reno Auto Care Needs
Reno Basic Interior
Reno Boat Detailing
Reno Break Dust Removal
Reno Carnuba Wax
Reno Cars Paint
Reno Cleaned Door Jams
Reno Door Jams
Reno Door Panels Cleaned
Reno Dry Exterior
Reno Exterior Windows
Reno Floor Mats
Reno Interior Deep Clean
Reno Interior Windows Cleaned
Reno Iron Decon
Reno Quick Vacuum
Reno Rv Detailing
Reno Seat Belts
Reno Spot Treatment
Reno Tar Removal
Reno Tires Cleaned
Reno Ultimate Detail
Reno Vacuum Interior
photograph by stacey lundeen. project #34 by Julie Clark.
from the Consistent Variable Project - first attempt.
A whole bunch of PRs from this morning. I have doubts about the new 1 mile PR since the other two trackers I use (my Mi Band and Strava) aren’t consistent with this or each other… but if nothing else, I got my first 10K! Not a particularly fast time since I was walking and taking videos of frog sounds for a lot of the latter part 😂 but still! I never thought I would be running OR walking at all in the middle of July but I’ve been trying to improve my heat tolerance and pushing through the sweat. I have to be careful since I have polycythemia which makes temperature extremes more problematic (maybe part of why I’m so heat intolerant to begin with) but that’s why I’m now leaving the house at like 5am 😅 via Instagram instagr.am/p/Cfxa6IyOsbh/
First night 2019!
Consistent Quality Capture -- Always
It's YOUR Moment!
Follow on Instagram: www.instagram.com/http.www.DaveGill.Photography/
Full Un-Watermarked Gallery -- Proceeds to benefit SPCA of Wake County: davegillphotography.shootproof.com/gallery/8516390
The 53rd annual Bon Odori Festival at Camp Zama was held Aug. 4. The festival is consistently the largest bilateral event of the year for U.S. Army Japan, this year attracting more than 30,000 visitors to the installation. The festival featured live entartainment, games for children, a variety of ethnic foods, bilateral sports, and a fireworks show.
About the United States Army Garrison Japan:
The United States Army Garrison Japan and its 16 supported installation sites are located in the island of Honshu and Okinawa in Japan. The USAG Japan mission is to support the Headquarters, U.S. Army Japan / I Corps (fwd) to ensure mission readiness and the quality of life of the Army community in a sustainable, transforming joint and combined environment.
The USAG-J area of responsibility spans 1,500 miles from north to south of Japan. Camp Zama, home for both HQ USARJ and USAG-J is located approximately 25 miles southwest of Tokyo in the cities of Zama and Sagamihara in Kanagawa Prefecture, Japan. The Camp Zama base cluster includes Sagamihara Housing Area and Sagami General Depot.
Akasaka Press Center is located in the center of Tokyo. The Akizuki/Kure area near Hiroshima is an ammunition depot. Yokohama North Dock is a port facility in the city of Yokohama, a major commerce port and a popular shopping area. USAG Torii Station is located 980 miles southwest of Camp Zama on the island of Okinawa.
We are the Army's home in Japan and the "Garrison of Choice" for Soldiers, Civilians and their Family members. We are committed in becoming the leader in the U.S. Army Installation Management Command by providing world-class installation services.
-----
To learn more about USAG Japan, please visit:
Official Website - www.usagj.jp.pac.army.mil
Facebook - www.facebook.com/usagj
Flickr - www.flickr.com/usagj
YouTube - www.youtube.com/usagjapan
Vimeo - www.vimeo.com/usagj
Twitter - www.twitter.com/usagjapan
Slideshare - www.slideshare.net/usagjapan
USARJ This Week on YouTube - www.youtube.com/usarjthisweek
The 53rd annual Bon Odori Festival at Camp Zama was held Aug. 4. The festival is consistently the largest bilateral event of the year for U.S. Army Japan, this year attracting more than 30,000 visitors to the installation. The festival featured live entartainment, games for children, a variety of ethnic foods, bilateral sports, and a fireworks show.
About the United States Army Garrison Japan:
The United States Army Garrison Japan and its 16 supported installation sites are located in the island of Honshu and Okinawa in Japan. The USAG Japan mission is to support the Headquarters, U.S. Army Japan / I Corps (fwd) to ensure mission readiness and the quality of life of the Army community in a sustainable, transforming joint and combined environment.
The USAG-J area of responsibility spans 1,500 miles from north to south of Japan. Camp Zama, home for both HQ USARJ and USAG-J is located approximately 25 miles southwest of Tokyo in the cities of Zama and Sagamihara in Kanagawa Prefecture, Japan. The Camp Zama base cluster includes Sagamihara Housing Area and Sagami General Depot.
Akasaka Press Center is located in the center of Tokyo. The Akizuki/Kure area near Hiroshima is an ammunition depot. Yokohama North Dock is a port facility in the city of Yokohama, a major commerce port and a popular shopping area. USAG Torii Station is located 980 miles southwest of Camp Zama on the island of Okinawa.
We are the Army's home in Japan and the "Garrison of Choice" for Soldiers, Civilians and their Family members. We are committed in becoming the leader in the U.S. Army Installation Management Command by providing world-class installation services.
-----
To learn more about USAG Japan, please visit:
Official Website - www.usagj.jp.pac.army.mil
Facebook - www.facebook.com/usagj
Flickr - www.flickr.com/usagj
YouTube - www.youtube.com/usagjapan
Vimeo - www.vimeo.com/usagj
Twitter - www.twitter.com/usagjapan
Slideshare - www.slideshare.net/usagjapan
USARJ This Week on YouTube - www.youtube.com/usarjthisweek
Forex trading provides a chance to participate in a global economy with great potential. Because of its popularity among day traders, Forex has earned a reputation for producing rapid returns.
To not only succeed, but to succeed consistently, you must first comprehend the market and then fine-tune your trading technique.
1. Fundamental definitions: Forex day trading system and strategies
1.1. What is day trading?
Day trading is the practice of opening and closing positions on the same day. Day trading tactics are more action-packed and need traders being at their trading station throughout the session to follow the live price charts.
1.2. What is Forex Day Trading System and Forex Day Trading Strategy?
Forex day trading systems should not be confused with day trading strategies.
The primary distinction between a system and a strategy is that a system specifies a trading approach, but a strategy is more descriptive and gives more precise information, such as entry and exit locations, indicators, and time periods.
1.2.1. How many types of Forex Day Trading Systems?
Scalping: In this system, buying or selling occurs immediately after the deal becomes profitable. The goal of this trading style is to achieve profitability while you are just up a few pips. You might anticipate to trade a lot and create a lot of money. The profit per transaction is rather little.
Fading: Fading is a system in which equities, an index, or a currency pair are shorted shortly after an upward advance. You want to profit from market actions that attempt to recover an asset's previous price.
Daily Pivots: Profit is made in this technique by using the volatility of asset values on a daily basis. The purchasing or selling occurs at the low phase of the day, and the trade is closed during the high period of the day. The price objective here follows the same trend as described earlier.
Momentum: In this sort of Forex Day Trading Systems, trading is generally done on the basis of news releases or by detecting powerful moves that are trending and are supported by big volumes. In this approach, the price goal is reached when the volume begins to decline and bearish candles appear. You are normally seeking to buy an asset a few hours before news is out, and then sell it once the market has moved sufficiently in your favor.
1.2.2. How many types of Forex Day Trading Strategies?
The following are 5 of the most commonly used Forex Day Trading Strategies:
Trend trading: Trend traders try to earn money by examining the direction of asset prices and then purchasing or selling based on the direction of the trend. If the trend is upward, with prices reaching successive higher highs, traders would establish a long position and purchase the asset. If the trend is downward, with prices making successive lower lows, traders would sell to take a short position.
Swing trading: Swing trading is all about taking advantage of short-term price patterns, using the notion that prices in a trend never travel in one way. While trend traders strive to profit from long-term market trends, swing traders are more interested in minor price reversals in a market. They try to anticipate these reversals and trade to profit from minor market fluctuations.
Scalping: Scalping is a short-term trading method that focuses on having a high win rate by taking tiny but frequent profits. The notion is that you can create a large trading account just as readily by taking modest profits repeatedly as you can by executing fewer trades and seeking to lock in earnings in the long term.
Mean reversion: Mean reversion is the belief that prices, and other measures of value such as price-to-earnings (P/E) ratios, will always return to the historical mean. The method employs technical analysis techniques such as moving averages to identify assets whose recent performance has deviated significantly from their historical average. Mean reversion traders will then profit from the return to their usual trajectory.
Money flows: The money flow indicator indicates if an asset is oversold or overbought by combining volume and price rather than just the asset's price. It determines whether the money flow was positive or negative by comparing the number of deals from the previous day to the current day. A rating of 80 or higher indicates overbought circumstances and should be sold by the trader. A value of 20 or less implies oversold market conditions and is a buy signal.
2. How do I determine if I am a Forex day trader?
Be a forex day trader if you:
Enjoy starting and finishing a deal on the same day.
Have time to evaluate the markets in the morning and can follow them throughout the day.
want to know won or lost at the end of the day.
Not be a forex day trader if you:
Prefer long-term or short-term trading.
Don't have time to examine and watch the markets throughout the day.
Work during the day.
3. How to start day trading Forex?
To begin trading right now, open a genuine account or practice risk-free with virtual cash on our demo account.
Choose between spread betting and CFD trading as your product.
Investigate the forex market and consult our day trading guide for success ideas and methods.
Brush up on your technical analysis skills by studying price charts and technical indicators.
To preserve your capital, use risk-management instruments such as stop-loss orders.
4. How do Forex Day Traders make money?
Day traders use big amounts of cash to profit from slight price swings in highly liquid indices, equities, or currencies. In other words, these traders are not seeking for significant price falls and peaks. They are OK with little, moderate swings, but their transactions are greater and more frequent than those generated by traders who invest for longer periods of time. The primary goal of a day trader is to generate a large number of pips in a single day.
Day traders should ideally earn profits on both asset highs and lows in forex day trader strategies. The entry in the various systems employ comparable tools to those used in conventional trading; the only variation is in the time and approach.
5. What are the most profitable forex trading strategy for beginners?
After determining a time frame, the intended position size on a single trade, and the anticipated number of transactions you want to open during a specific time period, we'll go through three prominent Forex trading strategies for beginners that have shown to be profitable.
5.1 Scalping
Forex scalping is a popular trading method that focuses on minor market fluctuations. This approach entails opening a huge number of transactions in the hopes of making tiny returns on each one.
Hence, scalpers strive to maximize earnings by making a high number of minor gains. This method is diametrically opposed to remaining in a posture for hours, days, or even weeks.
Because of the liquidity and volatility of the Forex market, scalping is quite popular. Investors are seeking markets where the price movement is continually shifting in order to profit from modest variations.
5.2 Day Trading
The process of exchanging currencies in a single trading day is referred to as day trading. Day trading method, while applicable in all markets, is most commonly utilized in Forex. This trading strategy suggests that you open and close all deals in a single day.
To reduce risk, no position should be left open overnight. Unlike scalpers, who only want to stay in markets for a few minutes, day traders typically monitor and manage open deals throughout the day. Day traders produce trading ideas mostly using 30-minute and 1-hour time periods.
Many day traders base their trading methods on breaking news. Scheduled events, such as economic figures, interest rates, GDPs, elections, and so on, have a significant influence on the market.
5.3 Position Trading
Position trading is a long-term investment technique. This trading method, unlike scalping and day trading, is primarily concerned with basic variables.
Minor market swings are not taken into account in this technique since they have little impact on the overall market picture.
To detect cyclical patterns, position traders are likely to study central bank monetary policies, political developments, and other fundamental variables. Successful position traders may only open a few transactions every year. However, profit goals in these trades are likely to be in the hundreds of pips range.
6. To sump up: Key highlights about Forex Day Trading Systems and Strategies
The practice of starting and closing trades on the same day is known as day trading. Day trading strategies are more action-packed and need traders to stay at their trading station throughout the session in order to monitor the live price charts.
A system differs from a strategy in that it outlines a trading technique, but a strategy is more descriptive and provides more exact information.
The four most common Forex Day Trading Systems are: Scalping, Fading, Daily Pivots and Momentum.
The five most common Forex Day Trading Strategies are: Trend Trading, Day Trading, Scalping, Mean reversion, Money flows.
The most profitable Forex day trading strategies for beginners (can be changed in the future) are: Scalping, Day Trading, Position Trading.
Source: https://libraryoftrader.net/the-crucial-guide-to-forex-day-trading-systems-and-strategies
Samsung is consistent in producing user needful devices every time. Samsung Galaxy A13 is a trustworthy device with good performance. It possesses a minimalist style with striking design. With significantly faster wifi, a brighter and high resolution screen and NFC support which the phone has is not so common in the mid range phones. 50MP quad camera and healthy battery life are superior features in it. Get it online now.
www.xcite.com.sa/phones/mobile-phones/samsung/galaxy-a/a1...
#samsung_a13 #samsung_galaxy_a13, #samsung_galaxy_a13_price_in_saudiarabia, #samsung_a13_price_in_ksa, #galaxy_a13
Cruisers Yachts consistently delivers the most ergonomic and well laid out helms we’ve seen.
For more tests, reviews, captain's report go to Cruisers Yachts 540 Sports Coupe model page
La facciata, originariamente a coronamento orizzontale, si presenta attualmente a salienti con due ali curvilinee di raccordo, frutto del consistente ridimensionamento delle strutture interne con la trasformazione della chiesa, originariamente a tre navate, in un unico ambiente a sala. E’ divisa orizzontalmente da una cornice marcapiano scolpita a foglie d’acanto. Ben conservato è il portale trecentesco, forse opera dello stesso Nicola di Salvitto che realizzò la facciata della cattedrale di S. Panfilo: su un’alta zoccolatura si erge l’arcone a sesto acuto sostenuto esternamente da due colonne, alle quali si affiancano - lungo il profilo strombato - pilastri alternati a colonnine; la serie dei capitelli è decorata da foglie d’acanto. Nella lunetta è un affresco con la Madonna del latte tra angeli e devoti (fine sec. XIV). Le finestre ai lati del portale sono aggiunte posteriori; nella campata superiore del fronte rimane solo la cornice del rosone, a bassorilievo, mentre è andato perduto l’intero lavoro di traforo che ne decorava l’interno. Sul fianco sinistro della chiesa si osserva un ulteriore portale dalle linee tardo rinascimentali (oggi murato) nel quale, al centro di un timpano semicircolare spezzato, si innesta uno stemma mobile con l’emblema dell’Ordine francescano. Sulla sinistra vi è poi un portale minore, dalle linee più semplici, realizzato nel XIX secolo per permettere l’accesso ad un piccolo oratorio di proprietà della Confraternita di Santa Maria degli Angeli.
Tratto da:
www.visit-sulmona.it/poi/43/chiesa-di-san-francesco-della...
via WordPress ift.tt/2NikTot
Alix Perez has always been known as a legend in the game of drum and bass and bass music, est. 2005. Since then he’s consistently put out one of the most interesting and diverse bodies of work in D&B with both solid solo releases and collabs. Since the creation of his own 1985 label imprint in 2015 and his hooking up with Eprom to form the deep bass halftime juggernaut that is SHADES in 2017, the tapestry that is Perez has only become more rich and complex.
In 2018 Perez, 1985 and SHADES only got stronger, with multiple massive releases coming from all three entities. SHADES’s In Praise of Darkness LP hit the scene like a literal bass cannon and their sets were consistently ranked as some of the best of any festival during the season. Towards the end of the year Perez hooked up with Monty for the unexpected breakout EP Spatia and 1985 put out some of the most innovative releases of the year, full stop.
2019 is shaping up to be another massive one for Perez. 1985’s second compilation LP Edition 2 due out March 1 is filled with as much diversity as it is with sexy, deep bass and it will easily be one of the best compilation albums of the year. Another collab track with Monty called “Good to Me” has already been released as a teaser for that comp and has been praised heavily, so the portends is pretty good there.
Perez is also getting a jump on the festival season with a B2B set with Skeptical at the Rampage 10 year anniversary with which takes place March 29-31 in Belgium. If that weren’t enough, SHADES are also working on a follow-up EP to In Praise of Darkness, due out sometime in spring and Perez himself has already collabed with Red Eyes and Icicle on tracks.
Given all this, Your EDM thought it was high time to sit down with Alix Perez and see if he can help the bass scene at large get its bearings on all things Perez. His answers were like his beats: insightful, to the point and with lots of impact.
So we’re coming up 1985’s four-year anniversary and it seems like it’s really created a unique niche in bass music and D&B that needed to be there. How do you think the label has grown from its original concept in your eyes?
The label’s journey so far I think has been very organic and natural. We’re very focused on what we project sonically and visually. I’m especially particular in my choices and very selective about the music we put out but I think that’s a positive and results in a refined output. I’ve always had a clear vision for the imprint and we’re building a little family of artists that encapsulate what we do. It’s a collective effort.
Speaking to the point of your vision for 1985 and its collective nature, what was you impetus for putting together compilations like Edition 2 and its predecessor last year Edition 1?
With larger bodies of work like Edition 1 and 2 I feel it gives space for exploration and also time for a narrative. The way these VAs are compiled is like an artist album, with some progression and intensity throughout. It’s like slotting pieces together until they become one. Diversity is really important to me in general and I believe these LPs really give us the chance to pursue this.
Winding that out a bit, what kind of feel were you going for in the second Edition? How did you decide which artists to feature?
When I ask artists to put music forward for these LPs there’s no prerequisite. I’m just looking for experimentation in the music. It may sound cliché but I know something is right when I hear it.
Everyone is talking about the collab with Monty on “Good to Me”. How did that come about?
When I collaborate I much prefer being in the same room but that isn’t always possible, especially with Monty living in France and me in London. On this occasion he sent me an idea and I developed it. It came together really quite naturally.
Your solo track in the compilation is quite the blend of styles. I hear some SHADES in there and some old school Perez, but is almost sounds like a new style you’re creating. Is that somewhat representative of where you might be going in the future, or just a lot of fun tinkering?
It really is just having fun in the studio. I have to keep things varied to keep myself excited and fresh when writing. I think it’s really healthy to do so. Having other projects like SHADES allows me to disconnect and write from a new perspective. If I was to write the same vibes all the time it would probably drive me insane.
Speaking of SHADES, that new EP is upcoming as well. Can you give any info on the style or SHADES evolution that fans can expect without giving too much away?
We have a new EP on the way following on from our debut LP. It’s a continuation of our experimentation in sound. I’m really excited about this new one, I think it’s some of our best work to date, personally at least.
Another exciting thing upcoming for you is playing Rampage this March. How did that all come together?
As simple as being offered to play. When it comes to B2B sets, I love playing with Skeptical. We really connect on a level musically and having SP:MC on the set will be a heavy combo.
What are you most looking forward to about playing at Rampage?
Playing our sound to such a huge crowd. It’s pretty nerve racking to be honest. Nervous is good though, keeps you on your toes.
Any other releases coming up that you can discuss? Any other tours/festies?
I have a 140 record coming out in April on 1985. Pretty excited about that. Looking forward to playing Lightning in a Bottle as SHADES this year and a bunch of other festivals. The last Outlook in Pula will also be very special this year.
1985’s Edition 2 compilation LP featuring Alix Perez, Monty and tons more is out March 1 and can be purchased on Beatport. For more info on the Rampage festival this March in Belgium, click here.
www.facebook.com/plugins/video.php?href=https%3A%2F%2Fwww...
This article was first published on Your EDM. Source: Your EDM Interview: Alix Perez Drops by to Talk SHADES, Rampage, 1985 and All Things Perez
Your EDM Interview: Alix Perez Drops by to Talk SHADES, Rampage, 1985 and All Things Perez published first on soundwizreview.tumblr.com/
photograph by stacey lundeen. project #43 by complexgeometries.
from the Consistent Variable Project - first attempt.
The 53rd annual Bon Odori Festival at Camp Zama was held Aug. 4. The festival is consistently the largest bilateral event of the year for U.S. Army Japan, this year attracting more than 30,000 visitors to the installation. The festival featured live entartainment, games for children, a variety of ethnic foods, bilateral sports, and a fireworks show.
About the United States Army Garrison Japan:
The United States Army Garrison Japan and its 16 supported installation sites are located in the island of Honshu and Okinawa in Japan. The USAG Japan mission is to support the Headquarters, U.S. Army Japan / I Corps (fwd) to ensure mission readiness and the quality of life of the Army community in a sustainable, transforming joint and combined environment.
The USAG-J area of responsibility spans 1,500 miles from north to south of Japan. Camp Zama, home for both HQ USARJ and USAG-J is located approximately 25 miles southwest of Tokyo in the cities of Zama and Sagamihara in Kanagawa Prefecture, Japan. The Camp Zama base cluster includes Sagamihara Housing Area and Sagami General Depot.
Akasaka Press Center is located in the center of Tokyo. The Akizuki/Kure area near Hiroshima is an ammunition depot. Yokohama North Dock is a port facility in the city of Yokohama, a major commerce port and a popular shopping area. USAG Torii Station is located 980 miles southwest of Camp Zama on the island of Okinawa.
We are the Army's home in Japan and the "Garrison of Choice" for Soldiers, Civilians and their Family members. We are committed in becoming the leader in the U.S. Army Installation Management Command by providing world-class installation services.
-----
To learn more about USAG Japan, please visit:
Official Website - www.usagj.jp.pac.army.mil
Facebook - www.facebook.com/usagj
Flickr - www.flickr.com/usagj
YouTube - www.youtube.com/usagjapan
Vimeo - www.vimeo.com/usagj
Twitter - www.twitter.com/usagjapan
Slideshare - www.slideshare.net/usagjapan
USARJ This Week on YouTube - www.youtube.com/usarjthisweek
Consistent Performance Recognition, Cosgrove Realty, Boxborough: Robert Bostwick of CERO, Debbie Trumbull of Small Water Systems Services LLC, Beth Card
The 53rd annual Bon Odori Festival at Camp Zama was held Aug. 4. The festival is consistently the largest bilateral event of the year for U.S. Army Japan, this year attracting more than 30,000 visitors to the installation. The festival featured live entartainment, games for children, a variety of ethnic foods, bilateral sports, and a fireworks show.
About the United States Army Garrison Japan:
The United States Army Garrison Japan and its 16 supported installation sites are located in the island of Honshu and Okinawa in Japan. The USAG Japan mission is to support the Headquarters, U.S. Army Japan / I Corps (fwd) to ensure mission readiness and the quality of life of the Army community in a sustainable, transforming joint and combined environment.
The USAG-J area of responsibility spans 1,500 miles from north to south of Japan. Camp Zama, home for both HQ USARJ and USAG-J is located approximately 25 miles southwest of Tokyo in the cities of Zama and Sagamihara in Kanagawa Prefecture, Japan. The Camp Zama base cluster includes Sagamihara Housing Area and Sagami General Depot.
Akasaka Press Center is located in the center of Tokyo. The Akizuki/Kure area near Hiroshima is an ammunition depot. Yokohama North Dock is a port facility in the city of Yokohama, a major commerce port and a popular shopping area. USAG Torii Station is located 980 miles southwest of Camp Zama on the island of Okinawa.
We are the Army's home in Japan and the "Garrison of Choice" for Soldiers, Civilians and their Family members. We are committed in becoming the leader in the U.S. Army Installation Management Command by providing world-class installation services.
-----
To learn more about USAG Japan, please visit:
Official Website - www.usagj.jp.pac.army.mil
Facebook - www.facebook.com/usagj
Flickr - www.flickr.com/usagj
YouTube - www.youtube.com/usagjapan
Vimeo - www.vimeo.com/usagj
Twitter - www.twitter.com/usagjapan
Slideshare - www.slideshare.net/usagjapan
USARJ This Week on YouTube - www.youtube.com/usarjthisweek
photograph by stacey lundeen. project #48 by Hillary Brown.
from the Consistent Variable Project - first attempt.
to find out more about the 2nd Attempt watch www.WornJournal.com (they're good with the updates)
Bailey consistently goes above and beyond for our customers, making sure they have what they need, when they need it. She is quick to find solutions while clearly communicating with her team and customers. Thank you, Bailey, for your outstanding customer service and providing the best experience for our clients. You are an amazing team member and we so appreciate all that you do!
My Bride consistently complains that our children make weird faces when their picture is being taken. And yet....
Are you consistently hitting the treadmill but not seeing results? Or maybe you just want to maximize your gym time and get more out of your workout — totally reasonable! Here are six quick tips and tricks to mix and match that up your caloric burn and help you get the most out of your...
www.ourstyle.life/tips-to-burn-more-calories-on-the-tread...
The 53rd annual Bon Odori Festival at Camp Zama was held Aug. 4. The festival is consistently the largest bilateral event of the year for U.S. Army Japan, this year attracting more than 30,000 visitors to the installation. The festival featured live entartainment, games for children, a variety of ethnic foods, bilateral sports, and a fireworks show.
About the United States Army Garrison Japan:
The United States Army Garrison Japan and its 16 supported installation sites are located in the island of Honshu and Okinawa in Japan. The USAG Japan mission is to support the Headquarters, U.S. Army Japan / I Corps (fwd) to ensure mission readiness and the quality of life of the Army community in a sustainable, transforming joint and combined environment.
The USAG-J area of responsibility spans 1,500 miles from north to south of Japan. Camp Zama, home for both HQ USARJ and USAG-J is located approximately 25 miles southwest of Tokyo in the cities of Zama and Sagamihara in Kanagawa Prefecture, Japan. The Camp Zama base cluster includes Sagamihara Housing Area and Sagami General Depot.
Akasaka Press Center is located in the center of Tokyo. The Akizuki/Kure area near Hiroshima is an ammunition depot. Yokohama North Dock is a port facility in the city of Yokohama, a major commerce port and a popular shopping area. USAG Torii Station is located 980 miles southwest of Camp Zama on the island of Okinawa.
We are the Army's home in Japan and the "Garrison of Choice" for Soldiers, Civilians and their Family members. We are committed in becoming the leader in the U.S. Army Installation Management Command by providing world-class installation services.
-----
To learn more about USAG Japan, please visit:
Official Website - www.usagj.jp.pac.army.mil
Facebook - www.facebook.com/usagj
Flickr - www.flickr.com/usagj
YouTube - www.youtube.com/usagjapan
Vimeo - www.vimeo.com/usagj
Twitter - www.twitter.com/usagjapan
Slideshare - www.slideshare.net/usagjapan
USARJ This Week on YouTube - www.youtube.com/usarjthisweek
Our company specializes the offered products and designs with the latest fashion trends of embroidery. Machine Embroidery Design are very important assets of any textile industry which is recognized for its beautiful designs and features. Machines provide us consistent and flawless results within very less time. So, don't wait to get your customized designs digitized by our professional digitizers.
Machine Embroidery Design: www.digitemb.com/category/machine-embroidery-designs
Infinite Media works hard to promote and capture the essence of your company through exceptional design be it websites, graphic design, printed material, and technology with outstanding customer service to build long-term partnerships, while evolving with you and your business.
Ms. Ramen consistently demonstrates a high level of commitment and professionalism in the performance of her duties as an accounting technician. She set herself apart while managing Wilson Matches funding, conducting 99% of the research and working with 49 states to educate them on how to settle incorrect transactions which totaled over $1 million. She is active in her church and has served as a financial advisor within the church and has also served as the Secretary of the Filipino-American Society.
ImWEA has worked consistently for the implementation of wind energy.
To learn more visit our Knol at knol.google.com/k/wind-turbines/wind-energy-associations-... and our blogger at windturbinesllc.blogspot.com/2011/02/wind-energy-organiza...
Join our wind turbines community – www.windturbines.net
Satisfactoriamente avanzan las obras de infraestructura adelantadas por Prosperidad Social en los municipios de Villanueva y La Jagua del Pilar al Sur de La Guajira, consistentes en la construcción y renovación de tres parques y la pavimentación de más de mil metros viales en el barrio El Paraíso, respectivamente.
Así lo evidenció el director general de Prosperidad Social, Nemesio Roys Garzón, quien hizo un recorrido por las obras junto a la comunidad y autoridades locales de los dos municipios en donde se ejecutan estas obras con una inversión superior a los $8.300 millones.
"Estos proyectos de infraestructura llevan calidad de vida a la población de estos dos municipios del Sur de La Guajira, los terminaremos este año satisfactoriamente y están incluidos en las 65 obras que de manera histórica estamos ejecutando en el departamento con una inversión superior a los $128.000 millones durante el gobierno del presidente Santos", afirmó el director general de Prosperidad Social, Nemesio Roys Garzón.
El proyecto de construcción y remodelación de los parques 6 de Abril, La Fe y Román Ovalle en Villanueva registra un avance de cerca del 45%, beneficiará a más de 19 mil habitantes con una inversión superior a los $6.400 millones. Los espacios deportivos cuentan con cancha polideportiva, sintética y sistema de gimnasio biosaludable, brindando a la población
escenarios de encuentro, ampliando el potencial cultural y deportivo del municipio.
Por su parte, el proyecto de construcción de más de 1.000 metros de pavimento vial en el barrio El Paraíso en La Jagua del Pilar, registra un avance del 92% e incluye además la construcción de más de 1.000 metros de andenes, zonas verdes y señalización con una inversión de $1.905 millones.
La obra mejorará la calidad de vida de la comunidad que ya no padecerá afectaciones por el polvo o el encharcamiento en época de invierno. Se mejorará la conectividad del barrio con otros sectores, optimizando y reduciendo tiempos de desplazamiento. La obra, generó 35 empleos y beneficiará a unas 170 familias del barrio El Paraíso.
En La Jagua del Pilar también iniciará próximamente el mejoramiento de condiciones de vivienda de 100 hogares.
Villanueva Seguimiento Obra Parque 6 de Abril. / Abr. 27, 2018. (Fotografía Oficial Prosperidad Social / Joel González).
Esta fotografía oficial del Departamento Administrativo para la Prosperidad Social está disponible sólo para ser publicada por las organizaciones de noticias, medios nacionales e internacionales y/o para uso personal de impresión por el sujeto de la fotografía. La fotografía no puede ser alterada digitalmente o manipularse de ninguna manera, y tampoco puede usarse en materiales comerciales o políticos, anuncios, correos electrónicos, productos o promociones que de cualquier manera sugieran aprobación por parte del Departamento Administrativo para la Prosperidad Social.
Prosperidad Social Página Web / Twitter / Facebook / Youtube / Instagram
This guy is a consistent part of the scenery at Daley Plaza. Doesn't appear to have his "whistle" on this day.
Farhad Khoiee-Abbasi is a public protester who has become known in Chicago as "the FBI sign guy," and sometimes as simply "The Sign Guy". He even blows a whistle every now and then.
=======================================
You are welcome to pin, re-post, embed and share this image, but please do not reproduce for your personal gain or profit without my permission.
© All Rights Reserved