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On our visit to Hong Kong Disneyland, we had the chance to experience Mystic Manor. Holy cow.
Words do not do justice to this attraction. It is pure magic, and integrates wonderful characters, an engaging story, great details, an excellent ride system, and beautiful music into an attraction that is the complete package. Mystic Manor takes the Disney dark ride experience to the next level, and shows just what the Imagineers can do when given the budget.
Check out my new Hong Kong Disneyland Guide, which contains reviews for every attraction at Hong Kong Disneyland.
Thanks for your views, comments, and faves!
Below are the various ways you can connect with me across the internet where I actively share my photos. The first one is my Disney-centric blog and the second is my travel-centric blog.
DisneyTouristBlog | TravelCaffeine | Facebook | Twitter | Instagram
Die Geschichte von Kreta ist sehr bewegt
-Minoische Zeit etwa 3000 v. Chr. bis 13.Jh v Chr
-archaische Zeitalter : 6. bis zum 4. Jahrhundert
-Byzantinisches Reich (395–1204)und Sarazenenherrschaft (826–961)
- Venezianische Herrschaft (1204–1669)
- Osmanische Herrschaft (1669–1897)
- De-facto-Unabhängigkeit (1898–1913)
- Vereinigung mit Griechenland (seit 1913)
- Minoan-Mycenaean Crete(3000-1300 BC)
- Classical, Hellenistic, Roman, Byzantine and Arab Crete(395-1204)
- Venetian Crete (1205–1669)
-Ottoman Crete (1669–1898)
- Independence(1898-1913)
-Crete was unified with mainland Greece(1913)
(Wikipedia)
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Im Straßenbild sieht man noch Minarette und Moscheen , aber die die meisten wurden einem anderen Zweck zugeführt. Geschichte kann man aber nicht ausradieren und ein friedlicher, harmonischer Mix aus Religionen, Architekturen, Kulturen kann doch nur bereichern.
There are still minarets and mosques in the street, but most of them have been brought to a different purpose. But you can not eradicate history and a peaceful, harmonious mix of religions, architecture, cultures can only enrich
...this is one of my oldest images...but i relly love it...i never seen a scene like this before and after in berlin...she was in the park with her husband and kids...they played basketball...suddlendy she went up and through a few balls...luck that i have my camera with me...
...i hope some more people view and like it...
@{-->-- ... thank you all very much my friends...:)))
Leica MP
Leica Elmarit 28mm f/2.8 III
Kodak T-Max 100
Ars Imago FD 1+39
6 min 20°C
Scan from negative film
Integration of the Orion spacecraft on top of the Space Launch System (SLS) rocket at NASA’s Kennedy Space Center in Florida.
The European Service Module that will power the first Orion uncrewed flight, ESM-1, was lifted up and mated with the rocket in preparation for launch, together with the crew module. Integration began on 20 October 2021, and the spacecraft was secured atop the powerful rocket six days later.
Artemis I is the first in a series of increasingly complex missions for human deep space exploration. The European Service Module will power Orion's crew module around the Moon and back with over 30 engines. The European Service Module provides electricity, water, oxygen and nitrogen as well as keeping the spacecraft at the right temperature and on course.
Credits: ESA - S. Corvaja
So here is my new look at the Great Nebula in Orion, this time made with narrowband filters and mapped color. Because the nebula is so bright a good image is possible with only seconds of integration - even in my bright skies here in Phoenix. But because it is so bright, it is also an opportunity to study the detailed structures of the nebula by making very long integrations. So this image was created from nearly 30 hours of integration time over several nights. That cluster of bright, young stars in the blue (oxygen emission) part of the nebula is the Trapezium cluster, the center of a stellar nursery where new stars are being born. These stars are lighting up the entire nebula which is roughly 25 light years in diameter - in angle, about the size of two Moons in Earth’s sky.
I feel so lucky that an infinitesimally small fraction of the photons created in this nebula travelled for such a long time (1500 years) through space and found their way into my tiny 6 inch telescope and onto my camera’s sensor. They subsequently produced an electronic signal that was recorded on a bit of silicon and finally rendered into an image viewable by our eyes and brains by even more silicon based devices. This all seems like a miracle to me.
And when we look at the image overall we see colors representing the different kinds of atoms in this amazing structure. These colors are not the colors we would see with our eyes if we were in a spaceship close enough to see colors with our unaided eyes. This image was made by assigning red, green, and blue colors to monochrome images made through filters that admit only a very specific color. Those filters are designed to pass photons coming from the atoms of sulfur, hydrogen, and oxygen. In the image here, yellow is a mixture of hydrogen and sulfur, red is mostly sulfur, and blue and shades of blue is oxygen. The molecular clouds and dust in the sky background are mostly a reddish brown.
IC 1396, 26 hours and 25 minutes of integration in SHO with Takahashi FSQ-106EDX4 106/382 telescope, f 3/6, QHY 600M Pro camera, are 317 shots of which in Ha 114x300 seconds, in OIII 101x300 seconds and in SII 102x300 seconds, processing with Pixinsight and Photoshop. All data and shots were captured with Telescope Live. IC 1396 is a very sparse open cluster associated with a large diffuse nebula, visible in the northern constellation Cepheus; it is located in a stretch of the Milky Way partially obscured by dense banks of dark nebulae, in a galactic region rich in neutral dust and gas with associated young and hot blue stars. The gases of the nebula complex of IC 1396 are excited by the stellar wind of the blue giant HD 206267, belonging to the Cepheus OB2 association. It seems that the expansion of this H II region created a large ring of molecular gas with a radius of about 12 parsecs, over a period of at least 3 million years. The ring structure extends for about 3° and is surrounded by a large number of dark blood cells, inside which the formation of new stars probably takes place due to compression by ionization, the shock wave front of stellar winds and radiation pressure; The largest blood cells are located on the northwestern side of the nebula region. In the eighties, 32 globules were identified, which received a numerical designation from 1 to 32 with the prefix GRS (Globules of Radial Systems); four radial systems of globules have been identified near IC 1396, while one of these is centered exactly on the nebula. Among the blood cells there is also the famous structure known as the Elephant trunk (see B 142). In the infrared, on the other hand, research has been conducted for the localization of young stellar objects associated with blood cells; It was thus discovered that only six sources associated with globules have a structure and luminosity such that they could have been caused by external heating, while most of these would not be related to star formation phenomena. In 2005, through a near-infrared study, 25 blood cells were identified, of which four had not been reported in the SIMBAD catalog; For all but four blood cells, it was possible to determine the mass, while it was not possible to measure the diameter for seven of them. Five globules contain a rich population of objects with reddened light, probably stars in formation; These five globules have the highest extinction rate, which would suggest a relationship between the intensity of star formation activity and the mass of the globules themselves. In blood cells with the smallest mass, star formation is often believed to be influenced by the radiation pressure of a bright star nearby; in a study conducted on one of these, illuminated by the bright blue giant HD 206267, a link with the distance of this star was highlighted, suggesting that evaporation due to photoionization affects the distribution of the mass of the blood cell around the blue giant. The influence of the star is given by the compression of the gases by the radiation pressure.
I am taking a different turn in photography.
I love incorporating art with photographs so now I play with my iPad and Laminar software.
Thus allows me to layer my bits and pieces hopefully into a more interesting landscape.
1200 sec each frame. 15 frames total. Integration 5h.
HEQ5 pro mount
80/480 deepsky superapo telescope
~387mm with focal reducer.
QHYCCD QHY163 mono astrocamera
PACIFIC OCEAN (May 18, 2021) A U.S. Marine Corps CH-53E Super Stallion assigned to Marine Medium Tiltrotor Squadron (VMM) 165 (Reinforced), 11th Marine Expeditionary Unit (MEU), takes off from amphibious transport dock USS Portland (LPD 27), May 18. Marines and Sailors of the 11th MEU and Essex Amphibious Ready Group (ARG) are underway conducting integrated training off the coast of southern California. (U.S. Marine Corps photo by Staff Sgt. Donald Holbert)
Detail of the undulator magnet installed in the Fermilab Integrable Optics Test Accelerator (IOTA) for experiment OSC on optical stochastic cooling
Acrylic and collage on illustration board. 2015
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