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In 1977 almost two thirds of the Presbyterian Churches in Australia voted to join with Methodists and Congregationalists to form the new Uniting Church in Australia.
en.wikipedia.org/wiki/Uniting_Church_in_Australia
This rationalisation process was partly a result of commitment to ecumenism and liberal theology, but also had serious economic and practical reasons as well. It was considered that a pooling of resources would strengthen the church, especially in their social work.
Whilst their commitment to social issues continues, it also cannot be denied that this has had very little impact on slowing the decline in church numbers as a whole. Pockets of growth continue, but only in the conservative evangelical or charismatic wings of the church. This is simply a fact.
Those denominations that chose to remain Presbyterian have also generally maintained membership levels. It appears the problem liberal Christians have is convincing people that their values are any different from the secular values that abound in everyday society. In which case, why not go to the beach instead?
But I'm pleased to say that St Andrew's continues in Evandale, and this wonderful building is a monument to the dedication of the early Scottish settlers in the region.
www.facebook.com/pages/category/Church/St-Andrews-Uniting...
The Himalayas, or Himalaya, form a mountain range in Asia separating the plains of the Indian subcontinent from the Tibetan Plateau.
The Himalayan range has many of the Earth's highest peaks, including the highest, Mount Everest. The Himalayas include over fifty mountains exceeding 7,200 metres (23,600 ft) in elevation, including ten of the fourteen 8000m peaks. By contrast, the highest peak outside Asia – Aconcagua, in the Andes – is 6,961 metres (22,838 ft) tall.
The Himalayan range is bordered on the northwest by the Karakoram and Hindu Kush ranges, on the north by the Tibetan Plateau, and on the south by the Indo-Gangetic Plain. The Himalayas are distinct from the other great ranges of central Asia, although sometimes the term Himalaya is loosely used to include the Karakoram and some of the other ranges. The Himalayas – inhabited by 52.7 million people – are spread across five countries: India, Nepal, Bhutan, China and Pakistan, with the first three countries having sovereignty over most of the range. Some of the world's major rivers, the Indus, the Ganges, and the Tsangpo-Brahmaputra, rise in the Himalayas, and their combined drainage basin is home to roughly 600 million people. The Himalayas have profoundly shaped the cultures of the Indian subcontinent; many Himalayan peaks are sacred in Hinduism and Buddhism.
Lifted by the subduction of the Indian tectonic plate under the Eurasian Plate, the Himalayan mountain range runs, west-northwest to east-southeast, in an arc 2,400 kilometres (1,500 mi) long.
For the Pimp my Pixels group.
The original image is not mine and can be seen here: www.flickr.com/photos/artistdom/2926368805/
© Jerry T Patterson - All Rights Reserved Worldwide In Perpetuity - No Unauthorized Use. Absolutely no permission is granted in any form, fashion or way, digital or otherwise, to use my Flickr images on blogs, personal or professional websites or any other media form without my direct written permission.
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Equipment: Canon 5D Mark III, Canon 16-35mm f2.8L II USM lens
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In September 2015, I was scouting out and photographing numerous sites around Lake Tahoe, California and many sites in the Eastern Sierras for a short 5 days.
One the night of September 17, I took the Bonsai Rock Milky Way shot with the moon just above the distant mountain peaks.
The next day we moved down into the Eastern Sierras where I had been planning to photograph the iconic bristlecone pine tree with the Milky Way. Little did I know on the way down how well the moon would come into play with my night sky photography work there.
I used a long established technique to get the moon rays in this shoot while I light painted the bristlecone pine tree with my special light.
In 2017, I will have two 5 day Milky Way photography workshop in Arches National Park in Moab, Utah, one over the 3rd week in March and one over the 3rd week in April.
During each of the two workshops, I will conduct 3 4+ hour Milky Way Photoshop post processing session where I teach all the techniques I used to create this final photo but this time it will be more of what is called a "Deep Dive" PS post processing session and workshop participants will need a laptop with Photoshop CS 2017. Lightroom will work but lacks some functionality used in what I will teach.
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My Milky Way night sky photography workshops
In 2017, I will be leading two 4 day photography workshops in Jackson Hole. During both workshops, I will take my group out for 3 nights of my Milky Way night sky workshop.
My 2017 4-5 day photography workshop schedule:
ANP, Canyonlands & Monument Valley - March 24-29
Icons of the Southwest w/Ryan Smith - April 23-28
Jackson Hole, Wyoming spring - June 21-25
Jackson Hole, Wyoming fall - September 19-23
The great part is that in 2017 I will return to Jackson Hole for the incredible wildflowers throughout the valley and the surrounding mountains.
Do you shoot the Milky Way but need a little help in getting the Milky Way to jump out of your photos ? If so, take a look at my ebook A Photographer's Milky Way Processing Guide - A Photoshop HowTo
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You may also find me at: .. Amazon || Smashwords || 500px || 72dpi || Google+ || facebook || Instagram
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Time to chill out to Adele's song ... Hello.
Thanks for stopping by.
James -
Here are photos of the tornado forming, along with a description of each.
My friend, Nick Lee, is a storm spotter. He and I were out taking these
photos that day. He is the copyright owner and has given me permission to
share them with you.
Dirk
P.S.: Please use the descriptions somehow in your description of the photos.
Description of photos:
Tornado-1: shows the storm coming around the corner into view.
Tornado-2: Inflow notch seen - this is where the air feeding the updraft was
located at.
Tornado-3 & 4: Tornado on ground getting closer to City of Cullman. At this
point it was passing Good Hope and going through Cullman County.
Tornado-5: Here you can see another vortex forming. What we were witnessing
was a rapid intensification of this storm from an EF2 to a multi-vortex EF4.
Tornado-6: Even though the funnel is hard to see, the tornado was still on
the ground. Here you can see the multiple vortexes spinning around the one
in the middle that looks like it is invisible.
Tulips (Tulipa) form a genus of spring-blooming perennial herbaceous bulbiferous geophytes (having bulbs as storage organs). The flowers are usually large, showy and brightly coloured, generally red, pink, yellow, or white (usually in warm colours). They often have a different coloured blotch at the base of the tepals (petals and sepals, collectively), internally. Because of a degree of variability within the populations, and a long history of cultivation, classification has been complex and controversial. The tulip is a member of the Liliaceae (lily) family, along with 14 other genera, where it is most closely related to Amana, Erythronium and Gagea in the tribe Lilieae. There are about 75 species, and these are divided among four subgenera. The name "tulip" is thought to be derived from a Persian word for turban, which it may have been thought to resemble.
Tulips originally were found in a band stretching from Southern Europe to Central Asia, but since the seventeenth century have become widely naturalised and cultivated (see map). In their natural state they are adapted to steppes and mountainous areas with temperate climates. Flowering in the spring, they become dormant in the summer once the flowers and leaves die back, emerging above ground as a shoot from the underground bulb in early spring.
First experiments with a new form in the ever-evolving world of Pano-Sabotage photography that's been dubbed "MonitorPano". It's both a new turn for me and a return to a very old tactic I used in 2012 where I achieved coarse but provoking layers by photographing, with my Canon Rebel XS, my computers screen saver as it faded in and out between images in my photo files. The great thing was that the images didn't just click from one to the next like a slide show, they faded in and out over top of each other. There was always a "crossover" point where the two images would occupy the same amount of "presence" on the screen thereby becoming "fused" or "blended" ... in effect ... layered. A cruder version of Brian Enos Installation piece, "77 Million Paintings", perhaps, but using the same idea.
www.youtube.com/watch?v=h0_4rCfpNzw
By the time Apple brought out the next Operating System, they'd taken out that scrolling slide show feature from what was then "iPhoto" and re-dubbed it "Photos". It always amazes me how the Silicon Valley geeks always "improve" things by taking out unique and wonderful features. Gotta mow it all down to sameness and uniformity, I guess. Unique features are seen as "mistakes".
Liz Mack has asked, "How long will it take for Apple to 'correct' the algorithms that allow for Pano-Sabotage photography ?"
MonitorPano, even though being hotly used right now and to great effect has actually been around quietly for a few years now. Don of the PANO-vision group was actually one of the first Pano-Sabotage artists to start "pano-ing" his desktop screen, and has often produced some very unique work with this method. Recently, Bill Smith, Paul Ewing and Liz Mack have taken it up with a vengeance with striking results.
"Graph ET 1" is the first finished piece that I created using the same technique the Paul, Bill, Liz and Don use. All of us in "PANO-Vision" learn a lot from each other and each of us makes invaluable contributions to the groups knowledge and technique base by that sharing. In PANO, as well call it for short, it's not about competition. We thrive by sharing. Each of us grows by contributing to an ongoing and easy exchange.
"MonitorPano" is achieved by setting one's cell phone camera on "Pano", clicking it on, while focusing on the desktop monitor and using the other hand to tap the arrow right ( or left ) key to quickly jump from photo to photo while the cell phone hand is pano-sabotaging the whole "pass". Tricky, and it takes some co-ordination, but it can be quite surprising what results.
This image was created for the PANO-Vision Groups Summer Contest, "PANO to the Metal".
www.flickr.com/groups/2892788@N23/discuss/72157667684597037/
Image culled from SLR shots done in 2011 and
"MonitorPanoed" and processed June 6, 2018.
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© Richard S Warner ( Visionheart ) - 2018. All Rights Reserved. This image is not for use in any form without explicit, express, written permission.
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I am VERY proud to announce that I was chosen to be the feature artist of the "Kreative People" Group's Spring Gallery - Running until the end of June. I really must thank both abstractartangel77 and Xandram for bestowing me with this great honour. The link to the gallery appears below:
Please visit my Kreative People Highlight Gallery HERE
POURSUIVRE LA BEAUTÉ EN AUVERGNE.
BrÖk et Plume.
Parce que à cette OEUVRE grandiose qui ose, il s'est passé une chose (...).
PASSAAAAAAAGE
ÉNERGIE
Et tout l'environnement a suivi.
MIRACLE ET NON MIRAGE.
Qui sait, peut-être le tout début d'une sacralité en germe dans le coeur et le labeur, en duo.
Mère et fils.
A Dieu vaille et le fasse.
CHEMIN vraiment.
Dans le cadre des oeuvres HORIZONS SANCY.
A la prochaine image, précisions.
Forma parte de las figuras del paso de Nuestro Padre Jesús de Nazaret, de la Hdad. de Pino Montano, Sevilla.
Realizado por el escultor Fernando Castejón López en 2007.
Tekergős járatával érkezik Rákoskeresztúr és Madárdomb határán található egyik megállójába a BKV egyik Ikarus 412-es autóbusza (Ikarus 412.10A, BPI-020, később AA CV-201). Budapestre az ezredforduló környékén érkezett a típus, ezáltal a BKV első alacsonypadlós buszai lettek ezek. Ezek Magyarországon az Ikarus 400-as széria utolsó képviselői, melyek már csak a fővárosban közlekednek, néhány alacsonypadlós autó- és trolibusz formájában.
Imagen creativa. Photosoph. Gracias de antemano por vuestros comentarios, awards, favoritos, invitaciones a grupo y la elección para galerías; perdonad que quizás no pueda responder individualmente . Todos los derechos reservados
Fujinon 50/1.4
Sand of Plum Island contains deep purple and dark grey patches. It is due to high abundance of almandine-pyrope garnet, pyroxene augite, and magnetic minerals such as ilmenite and hematite. Epidote adds some greenish hue. The source of the minerals is a terminal moraine that contains huge boulders of igneous and metamorphic rocks and products of their decomposition.
Named after the distinctive white band at the base of bill. Medium size, grayish-brown goose, with irregular black barring on underparts; orange feet and legs. Bill distinctive orange in Greenland form with whitish tip. Most young birds acquire white front and bill during first Winter; acquire black belly markings by second Fall. Color and size vary in adults: small, pale arctic tundra birds have heavy barring; taiga breeding birds are larger, darker with less barrings. Greenland form has heaviest barrings. Casual and increasing Winter visitor on East coast from Quebec to Georgia, although the goose is very uncommon east of the Mississippi River.
This lone goose was among hundreds of Canadian Geese near an icy campus lake, Mt. Holyoke College. Was a very cold, overcast day here today. The sun just peeked out for a few minutes and I caught this shot. The bird is rare for this month and in this region of US.
Nikon VR 500 mm f/4e lens, f/5.6, 1/3200s, ISO 640.
Thanks to all of you who 'fave' and comment on the photograph.
Dungeness is a headland on the coast of Kent, England, formed largely of a shingle beach in the form of a cuspate foreland. It shelters a large area of low-lying land, Romney Marsh. Dungeness is also the name of the power station and a few other nearby buildings near the beach, and of an important ecological site at the same location.
Dungeness is one of the largest expanses of shingle in the world. It is of international conservation importance for its geomorphology, plant and invertebrate communities and birdlife. This is recognised and protected mostly through its conservation designations as a National Nature Reserve (NNR), a Special Protection Area (SPA), a Special Area of Conservation (SAC) and part of the Site of Special Scientific Interest (SSSI) of Dungeness, Romney Marsh and Rye Bay.
There is a remarkable variety of wildlife living at Dungeness, with over 600 different types of plant: a third of all those found in Britain. It is one of the best places in Britain to find insects such as moths, bees and beetles, and spiders; many of these are very rare, some found nowhere else in Britain.
The short-haired bumblebee, Bombus subterraneus, was last found in the UK in 1988, but has survived in New Zealand after being shipped there more than 100 years ago. It is to be reintroduced at Dungeness. It is planned that the first bees will be introduced in the spring of 2010.
The flooded gravel pits on Denge Beach, both brackish and fresh water, provide an important refuge for many migratory and coastal bird species. The RSPB has a bird sanctuary there and every year thousands of bird watchers descend on the peninsula to catch a glimpse of a rare bird from the bird observatory.
One of the most remarkable features of the site is an area known as 'the patch' or, by anglers, as 'the boil'. The waste hot water and sewage from the Dungeness nuclear power stations are pumped into the sea through two outfall pipes, enriching the biological productivity of the sea bed and attracting seabirds from miles around.
Beach fishing is popular at Dungeness, with the area being a nationally recognised cod fishing venue in the winter.
The name Dungeness derives from Old Norse nes: "headland", with the first part probably connected with the nearby Denge Marsh. Popular etymology ascribes a French origin to the toponym, giving an interpretation as "dangerous nose".
Reims (Marne) - Palais du Tau - Salle du Tau (ou salle du Festin).
.
Cette salle avait initialement une forme de T, d'où son nom. Cette vaste salle maintenant rectangulaire depuis les travaux de Robert de Cotte au XVIIe siècle, fut auparavant remaniée à la fin du XVe siècle pour l'archevêque Guillaume Briçonnet. Ses armoiries, mêlées avec celles de l'héraldique ecclésiastique, sont sculptées sur la cheminée. La charpente en bois de la salle a la forme d'une carène de navire inversé et présente neuf poutres horizontales. La salle, fortement endommagée lors de l'incendie de 1914 qui détruisit ce plafond mais épargna la cheminée, fut restaurée suivant d'anciennes gravures. Deux grandes tentures murales illustrant l'histoire du Fort Roy Clovis, datant du XVe siècle, sont exposées. Cette salle est appelée également salle du Festin car le banquet suivant le sacre royal s'y déroulait..
I just popped up to the local village churchyard, hoping to see some of these. This one is the only individual where I managed some half-decent shots.
Sminthurinus aureus has several colour forms. There is an all yellow form and some dark forms. The dark forms like this, often retain the yellow legs and antennae. This individual was 0.6mm in length. They can be quite difficult to find (I use a 5x hand-lens) until you "get your eye in". This one was under a fallen laurel leaf. Whenever I see see fallen laurel leaves, I always check underneath for springtails!
Chorsu is always chaos, smoke, and constant movement. But sometimes you manage to catch a moment when all this bazaar noise fades into the background. The light falls in such a way that it carves out one specific scene from the hustle, and the dead black eats up everything else.
(EN) Bath's coralblenny - (FR) Blennie de Bath
Ecsenius bathi black stripes form, Pura Island, Indonesia
Seasonally dimorphic, the fall form of this species with strong lavender edging and predominantly orange coloration on the dorsal hind wings will overwinter as an adult. It will be one of the earliest butterflies to fly in spring and may even be encountered on warm winter days in early February. This butterfly does not rely on floral nectar, but prefers to sip flowing tree sap, carrion and dung. Male butterflies love to puddle and are notoriously territorial meeting any intruder that enters their territory.
This long-distance traveler has wandered east from its normal home in the Rocky Mountains and areas west. This color phase was once called the Oregon junco and has a black head and brown back.
Shes very cold in this form and she has a limit if she stays too long her heart will stop and she will die
Photographed in NYC 1/5/2015
Best viewed large size
PLEASE,NO GRAPHICS WITH YOUR COMMENTS!!!!!!!!!!!!!!!!!!!!
No Group Invites with Graphics Please!
Please contact me before using this photography or art concept
© All rights reserved
A new image from the NASA/ESA/CSA James Webb Space Telescope reveals a remarkable cosmic sight: at least 17 concentric dust rings emanating from a pair of stars. Located just over 5000 light-years from Earth, the duo is collectively known as Wolf-Rayet 140. Each ring was created when the two stars came close together and their stellar winds (streams of gas they blow into space) met, compressing the gas and forming dust. The stars’ orbits bring them together about once every eight years; like the rings of a tree’s trunk, the dust loops mark the passage of time.
In addition to Webb’s overall sensitivity, its Mid-Infrared Instrument (MIRI) is uniquely qualified to study the dust rings. These rings are also called shells by astronomers because they are thicker and wider than they appear in the image. Webb’s science instruments detect infrared light, a range of wavelengths invisible to the human eye.
Contributed under both ESA and NASA leadership, Webb’s MIRI instrument detects the longest infrared wavelengths. This means that it can often see cooler objects – including the dust rings – than Webb’s other instruments can. MIRI’s spectrometer also revealed the composition of the dust, formed mostly from material ejected by a type of star known as a Wolf-Rayet star. A Wolf-Rayet star is born with at least 25 times more mass than our Sun and is nearing the end of its life, when it will likely explode as a supernova and then collapse into a black hole. Burning hotter than in its youth, a Wolf-Rayet star generates powerful winds that push huge amounts of gas into space. The Wolf-Rayet star in this particular pair may have shed more than half its original mass via this process.
Transforming gas into dust is somewhat like turning flour into bread. It requires specific conditions and ingredients. Hydrogen, the most common element found in stars, can’t form dust on its own. But because Wolf-Rayet stars shed so much mass, they also eject more complex elements typically found deep in a star’s interior, including carbon. The heavy elements in the wind cool as they travel into space and are then compressed where the winds from both stars meet, like when two hands knead dough.
Some other Wolf-Rayet systems form dust, but none is known to make rings like Wolf-Rayet 140 does. The unique ring pattern forms because the orbit of the Wolf-Rayet star in WR 140 is elongated, not circular. Only when the stars come close together – about the same distance between Earth and the Sun – and their winds collide is the gas under sufficient pressure to form dust. With circular orbits, Wolf-Rayet binaries can produce dust continuously.
The science team thinks WR 140’s winds also swept the surrounding area clear of residual material they might otherwise collide with, which may be why the rings remain so pristine rather than smeared or dispersed. There are likely even more rings that have become so faint and dispersed, not even Webb can see them in the data.
Wolf-Rayet stars may seem exotic compared to our Sun, but they may have played a role in star and planet formation. When a Wolf-Rayet star clears an area, the swept-up material can pile up at the outskirts and become dense enough for new stars to form. There is some evidence the Sun formed in such a scenario.
Using data from MIRI’s Medium Resolution Spectroscopy mode, the new study provides the best evidence yet that Wolf-Rayet stars produce carbon-rich dust molecules. What’s more, the preservation of the dust shells indicates that this dust can survive in the hostile environment between stars, going on to supply material for future stars and planets. The catch is that while astronomers estimate that there should be at least a few thousand Wolf-Rayet stars in our galaxy, only about 600 have been found to date.
These results have been published today in Nature Astronomy.
MIRI was contributed by ESA and NASA, with the instrument designed and built by a consortium of nationally funded European Institutes (the MIRI European Consortium) in partnership with JPL and the University of Arizona.
[Image Description: The background of this Webb image of star Wolf-Rayet 140 is black. A pair of bright stars dominates the centre of the image, with at least 17 pink-orange concentric dust rings emanating from them. Throughout the scene are a range of distant galaxies, the majority of which are very tiny and red, appearing as splotches.]
Credits: NASA/ESA/CSA/STScI/JPL-Caltech; CC BY 4.0
"The Canadian National Railways was formed in 1923 to rescue several financially troubled rail lines. At the time of the merger new motive power was badly needed and the CNR's first order for new locomotives was given to the Canadian Locomotive Company to build sixteen "Mountain" type locomotives.
This batch of sixteen 4-8-2s were delivered in 1923 and was designated as Class U-1-a and assigned road numbers 6000 through 6015. These locomotives had 26 x 30 cylinders, 73" drivers, a 210 psi boiler pressure and exerted 49,588 lbs of tractive effort. They weighed 354,110 lbs and were used on express passenger trains between Montreal and Toronto.
Twenty-one more "Mountains" were delivered from the Canadian Locomotive Company during 1924 and 1925. These locomotives were designated as Class U-1-b and given road numbers 6016 through 6036. They were similar to the Class U-1-a "Mountains" and were added to the passenger motive power roster.
Five more 4-8-2s (Class U-1-d, road numbers 6042 through 6046) from the Canadian Locomotive Company and twelve more 4-8-2s (Class U-1-e, road numbers 6047 through 6058) from the Montreal Locomotive Works were delivered in 1929 and 1930. These last two groups had minor improvements but were essentially the same as the sixteen delivered in 1923.
A final batch of twenty “Mountains” was delivered by the Montreal Locomotive Works in 1944. This group was designated as Class U-1-f and assigned road numbers 6060 through 6079. These very heavy (416,500 lbs) locomotives were semi-streamlined and intended to be used primarily for fast passenger service. Some were also used in a dual freight and passenger capacity. They were capable of reaching speeds up to 100 miles per hour.
The U-1-f class locomotives had a distinguishing conical nose that housed the headlight and the number lamps. The stack was flared after the British style. They were normally painted in CNR's passenger colours of black with green board skirts, cab and tender. Some of them were eventually converted to burn oil.
There are five surviving CNR "Mountains":
"6015 at station yard in Jasper, AB
6043 at Assiniboine Park in Winnipeg, MB
6060 at the Rocky Mountain Railway Society in Calgary, AB
6069 at Bayview Park in Sarnia, ON
6077 at Prescott Park in Capreol, ON "