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New full reprocess of this popular object after to be published by me on natural colors palette on January.
This images is a result of a 65 hours of integration time using rgb and narrow band filters.
The Jellyfish Nebula (IC 443) is a supernova remnant located in the constellation Gemini.
It is situated about 5,000 light-years away from Earth and spans across an area of about 50 light-years in diameter.
The nebula got its name because of its tentacle-like structures, which resemble those of a jellyfish.
These structures are formed from the shockwaves created by the explosion of a massive star, which occurred about 30,000 years ago.
The explosion produced a blast wave that is still expanding outward, colliding with the surrounding interstellar gas and dust and creating the striking filamentary structure we see today.
The Jellyfish Nebula emits light across a broad range of wavelengths, from radio waves to X-rays.
The filaments of gas and dust are primarily made up of hydrogen, but also contain other elements such as oxygen and sulfur.
The nebula also contains a pulsar, a highly magnetized, rotating neutron star that emits a beam of electromagnetic radiation.
Observations of the Jellyfish Nebula have provided important insights into the processes that shape and influence the interstellar medium. It is a popular target for astronomers studying supernova remnants and their interactions with the surrounding interstellar material.
Imaging Telescopes Or Lenses
Takahashi Epsilon-160ED
Imaging Cameras
QHYCCD QHY294 Pro M
Mounts
Sky-Watcher EQ6-R Pro ×
Filters
Baader Blue (CMOS-Optimized) 36 mm · Baader Green (CMOS-Optimized) 36 mm · Baader H-alpha 6.5nm (CMOS-Optimized) 36 mm · Baader O-III 6.5nm (CMOS-Optimized) 36 mm · Baader Red (CMOS-Optimized) 36 mm · Baader S-II 6.5nm (CMOS-Optimized) 36 mm
Accessories
Pegasus Astro FocusCube2 · Pegasus Astro Powerbox Advance Gen2 · QHYCCD QHYCFW3-M-US · TS-Optics Off-axis guider 9mm (TSOAG9G2) ×
Software
Starkeeper Voyager Custom Array
Guiding Cameras
ZWO ASI290MM Mini
Acquisition details
Dates:
Jan. 23, 2022 · Jan. 25, 2022 · Jan. 26, 2022 · Jan. 29, 2022 · Jan. 31, 2022
Frames:
Baader Blue (CMOS-Optimized) 36 mm: 115×60″(1h 55′) (gain: 0.00) bin 1×1
Baader Green (CMOS-Optimized) 36 mm: 115×60″(1h 55′) (gain: 0.00) -15°C bin 1×1
Baader H-alpha 6.5nm (CMOS-Optimized) 36 mm: 146×600″(24h 20′) (gain: 1600.00) -15°C bin 1×1
Baader O-III 6.5nm (CMOS-Optimized) 36 mm: 102×600″(17h) (gain: 1600.00) -15°C bin 1×1
Baader Red (CMOS-Optimized) 36 mm: 115×60″(1h 55′) (gain: 0.00) -15°C bin 1×1
Baader S-II 6.5nm (CMOS-Optimized) 36 mm: 112×600″(18h 40′) (gain: 1600.00) -15°C bin 1×1
Integration:
65h 45′
Avg. Moon age:
24.07 days
Avg. Moon phase:
34.69%
RA center: 06h18m11s.78
DEC center: +22°35′04″.9
Pixel scale: 3.557 arcsec/pixel
Orientation: 0.127 degrees
Field radius: 1.239 degrees
WCS transformation: thin plate spline
Find images in the same area
Resolution: 2082x1398
File size: 5.3 MB
Locations: AAS Montsec, Àger, Lleida, Spain
Data source: Own remote observatory
Remote source: Non-commercial independent facility
Gyaling and drum musicians at the Gustor festival, Spituk Gompa, Leh, Ladakh. The gyaling is a double reed oboe-like instrument used mainly in Tibetan monasteries (Ladakh is known as 'Little Tibet') that requires a technique called circular breathing in which the instrument will constantly be emitting a continuous tone, even while the musician inhales.
05/02/2019 www.allenfotowild.com
These were inspired by the Cantwell class Arrestor cruiser seen in Andor, the TIE Arrestor is an Imperial starfighter with two powerful tractor beam emitter dishes. It can be deployed to intercept, disable and tow Rebel starfighters suspected of stealing Imperial technology. It can also be used to capture Rebel personnel wanted for questioning.
This Imperial squadron has a purple accent colour, suggested by lamborghiniwafflesauce as the nemesis for Teal Squadron – the Imperial squadron leader’s TIE Arrestor is the one with more purple on it.
Thanks to Inthert for inspiration for the round cockpit design, who in turn was inspired TWP.
Access: Pervy pixelated musings (Particle emitter) by Birth *Get this item at the Kinky event!* www.flickr.com/photos/54911392@N03/ ; Felora single by LODE *This item was at the access event!* www.flickr.com/photos/chirzakavlodovic/
LM to Kinky event: maps.secondlife.com/secondlife/Liberty%20City/109/95/33
LM to birth: maps.secondlife.com/secondlife/Crocus%20Island/200/231/22
Hair: Jin delux hair by S-CLUB www.flickr.com/photos/194418943@N08/
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High energy photons are emitted in energy transitions of particles in the nucleus of atoms. The release of energy into photons and energetic particles is a defining feature of the thermonuclear furnaces streaking across this three hour composite image. That same release of energy from atomic nuclei fuzing or fracturing forms the basis for nuclear weapons, first realized in the weapons of war just beyond the horizon in this image. While the light pollution from Los Alamos makes for a poetic counterpoint to the star trails overhead, it really is the result of much more common (and benign) energy exchanges and scattering from smoke particulates. Maybe our uses of photons can aspire to be life giving and sustaining like ones overhead in this image.
As a star trail image, I was shooting for better, but as a nightscape scene, I appreciate it and enjoy the range of color and phenomena in the sky. I hope you enjoy the benign use of the photons I collected to compose this image for your enjoyment and appreciation of the beauty we still have.
Hopefully you do too!
Peace and cheers!
I have tried to include following maxwell material concept using a simple primitive
Bi directional scatter distribution function (BSDF), layered materials, ior, bump, anisotropy, scatter, transmittance, roughness, coating, clip map, normal map, dispersion, frost, displacement, self illumination and standard grey with hdri image based lighting
Most of materials come from Maxwell material Resource site, rest are preset.. some are my own. But all are my fave.
And of course, dedicated to the progress of a rising photographer Abdul Waris
To me, the best part of the holidays is seeing homes all lit up in Christmas lights. I've always had a weak spot for old-school colorful incandescent bulbs, but I can't help but appreciate the elaborate displays now made possible with energy-efficient LED light strings and sophisticated sequencing and synchronization systems.
Milkweed is a foul-smelling, wetland plant that emits a mild odour when left along but is especially pungent when damaged. Skunk open cabbage is one off the few plants that can produce heat through cellular respiration. Unfortunately almost destroyed !!!
Fagradalsfjall is a volcano on the Reykjanes Peninsula, around 40 kilometres (25 mi) from Reykjavík, Iceland. Its highest summit is Langhóll (385 m (1,263 ft)). A volcanic eruption began on 19 March 2021 in Geldingadalir to the south of Fagradalsfjall, which is still emitting fresh lava as of today.
Bangladesh used to be a global competitor alongside tea giants as Kenya, India and Sri Lanka. It produces about 56 million kg of tea per year of which 50 million kilograms account for domestic consumption. No wonder that tea stalls like these are found everywhere and Bangladeshis are known to be gluttonous tea drinkers.
This one is located at Saturia (near Baliati Jomidar Bari), near Dhaka
Esta imagen ha participado en el juego En un lugar de Flickr
Si no perteneces al grupo, no contestes, por favor.
Si quieres contestar, únete. :-)
Escondido entre dos valles se encuentra el municipio de Catí, donde la pujanza, que le otorgó el comercio de la lana y la ganadería durante la Edad Media, ha dejado buena muestra de la arquitectura de la época en su casco antiguo, declarado Conjunto Histórico Artístico , así como Bien de Interés Cultural. Una gran riqueza patrimonial y monumental sorprende al viajero en esta villa.
Los numerosos escudos y emblemas nobiliarios adornan los edificios religiosos y las casas señoriales del casco histórico.
Uno de los lugares enigmáticos de Catí, y que más visitas atrae, es la ermita de la Mare de Déu de l’Avellà o Emita de l’Avellà, un lugar conocido históricamente por la bondad de sus aguas. El Agua de l’Avellà se extrae del conocido manantial del mismo nombre, ya apreciado por los árabes. Hay constancia documental de la existencia de la fuente desde hace más 300 años. Fue declarada de utilidad pública en 1928.
En el interior de la Ermita de l’Avellà encontramos una exuberancia decorativa que, desde la misma entrada, está ornamentada con dorados y pinturas al fresco realizadas en 1737 obra del artista de Sant Mateu, Pasqual Mespletera, quien también decoró la Capilla de la Comunión de la iglesia de Catí.
The Multiverse light sculpture by Leo Villareal is on display at the moving walkway at the National Gallery of Art in Washington, DC. It is one of the coolest light shows that I have seen. The 40,000 light emitting diodes are constantly changing patterns as you move down the walkway between the East and West Gallery. Unfortunately, will only be there until November 2009. It would make a great permanent addition to the gallery.
Mount Etna emitting smoke, Catania, Sicily, Italy.
Mount Etna is Europe's highest and most active volcano. Towering above the city of Catania on the island of Sicily, it has been growing for about 500,000 years and is in the midst of a series of eruptions that began in 2001. It has experienced a variety of eruption styles, including violent explosions and voluminous lava flows. More than 25% of Sicily's population lives on Etna's slopes, and it is the main source of income for the island, both from agriculture (due to its rich volcanic soil) and tourism.
I've seen patches and bands of purple before. But over many years of aurora photography, I've only seen this once: a broad purple aurora. The purple wavelength is emitted by lighter gasses high up in the ionosphere, such as helium and hydrogen. The image was captured during a period of intense geomagnetic activity -- during a time when the Kp index hovered between about 5 and 8 for most of a week, resulting in what seem to have been the strongest and most sustained auroras of the last decade. This image is a panorama, made by stitching together six vertical frames captured in very quick succession with a 35mm f 1.4 lens (the extremely sharp, low coma, reasonably priced Sigma Art).
Not only the light-emitting organs, also the eyes show strong fluorescence. Notice that the pronotum ("hat") is transparent!
Refflection spectrum of pronotum
Objective: Mitutoyo 7.5 NA 0.21, tube lense 200mm (Nikon)
Illumination: UV (365nm) and oblique (white)
My heart fluttered and emitted a multicolored aura as I smiled agaisnt the cool breeze thinking of you. Along the white flowers, worn out bench, cold and almost old marble stone, I remembered and never forgot. Alone I sat, agaisnt the grass just inhaling all our memories, the nostalgia engulfing me until slumber has invaded my senses and stole my peace of mind.
There you was, in front of me. You had that usual killer smile, the one that made me blush and my heart stop.
"I am here." You said to me extending your hand, with a warm reassuring look. "I promise to never leave."
I smiled brightly, reaching to take your warmth. It was a beautiful autumn day, the smell of moist and then the smell of incoming rain.
It was the thunder that woke me up, but only in my memory. Of course, you were gone. Promises? Isn't there a saying they are meant to be broken?
The sun emitted three mid-level solar flares on July 22-23, 2016, the strongest peaking at 1:16 am EDT on July 23. The sun is currently in a period of low activity, moving toward what's called solar minimum when there are few to no solar eruptions – so these flares were the first large ones observed since April. They are categorized as mid-strength flares, substantially less intense than the most powerful solar flares.
These flares were classified as M-level flares. M-class flares are the category just below the most intense flares, X-class flares. The number provides more information about its strength. An M2 is twice as intense as an M1, an M3 is three times as intense, etc.
Of these three flares: The first was an M5.0, which peaked at 10:11 pm EDT on July 22, 2016. The second -- the strongest -- was an M7.6, which peaked at 1:16 am EDT on July 23. The final was an M5.5, which peaked 15 minutes later at 1:31 am EDT.
Credit: NASA/Goddard/SDO
Another night the Cudillero lighthouse emits its flashes to warn sailors about the distance from the coast. Considering myself a lighthouse lover, I really enjoyed watching this lighthouse shine in the Cantabrian Sea every night.
I wish you a happy weekend and much, much, much love and peace!
Press "L" to enlarge the picture.
_______________________________
El Faro de Cudillero brillando en la noche, Asturias, España
Otra noche más el faro de Cudillero emite sus destellos para avisar a navegantes sobre la distancia con la costa. Considerándome un amante de los faros, disfruté mucho viendo cada noche lucir este faro en el Mar Cantábrico.
Os deseo un feliz fin de semana y mucho, mucho, mucho amor y paz!
Pulsa "L" para ampliar la imagen.
The northern lights are elementary particle physics, superstition, mythology and folklore come to life. Throughout the ages they have filled people with wonder and fear. They have challenged and inspired scientists and artists. I can certainly add photographers! To see the aurora was an unforgettable experience. Auroras are caused by vast super-heated supersonic collections of smashed atoms, known as solar wind, that enter the earth’s upper atmosphere where they collide with oxygen and nitrogen atoms. These collisions usually take place between 60 & 300 km above ground, causing the oxygen and nitrogen atoms to become electrically excited and to emit light. The result is a dazzling dance of green, blue, white and red light.
La Tierra gira y forma estelas de estrellas que giran alrededor de la Estrella Polar.
Las antenas emiten ondas que viajan a través de nuestra atmósfera y escapan de ella viajando por el Universo, hasta unas distancias casi incomprensibles a nuestra mente humana.
Quizá algún día, algún ser extraterrestre escuche estas emisiones y sepa tirar del hilo para encontrar su origen, comunicarse con nosotros o incluso visitarnos...
5D III - Tokina 11-16 a 16mm - f/4 - 30s - ISO 400
91 tomas unidas con Startrails.
Lava emitted from the Pu'u O'o spatter cone part of Kilauea volcano on the island of Hawaii.
This type of lava is known by its Hawaiian name, pahoehoe lava, which means smooth, unbroken lava. It is basaltic lava that has a smooth, undulating or ropy surface. This is due to the movement of very fluid lava under a congealing surface crust. A pahoehoe flow typically advances as a series of small lobes and toes that continually break out from a cooled crust as can be seen here. Pahoehoe lavas typically have a temperature of 1100 to 1200 °C.
Recently erupted basalts lavas have low viscosity which means they usually flow easily and they release gases quickly so they are less likely to give rise to explosive eruptions. See: en.wikipedia.org/wiki/Lava
Puffballs are fungi, so named because clouds of brown dust-like spores are emitted when the mature fruitbody bursts or is impacted. Puffballs are in the division Basidiomycota and encompass several genera, including Calvatia, Calbovista and Lycoperdon.[1] True puffballs do not have a visible stalk or stem. The puffballs were previously treated as a taxonomic group called the Gasteromycetes or Gasteromycetidae, but they are now known to be a polyphyletic assemblage.
The Milwaukee Pierhead Light is an active lighthouse located in the Milwaukee harbor, just south of downtown. This aid to navigation is a 'sister' of the Kenosha North Pier Light. The station was established in 1872. It is west of the Milwaukee Breakwater Light, and is near the outflow of the Milwaukee River—not far east of where that river converged with the Kinnickinnic River—into the Milwaukee Harbor and Lake Michigan. This light has a round steel tower with a round gallery and a ten-sided lantern. In 1926, the original 4th Order Fresnel lens was transferred to the Milwaukee Breakwater Light, and that lens is now displayed at the Wisconsin Maritime Museum in Manitowoc, Wisconsin. The Fifth Order Fresnel lens—installed in 1926—was removed in 2005. The tower is newly painted circa 2007. The 5th Order lens is said to be on display also at the Wisconsin Maritime Museum. According to one source: "The original lantern room had helical bar windows and is believed to [be] the one presently on the Breakwater Light." This is corroborated by the report that the Breakwater Light has a "round cast iron lantern room [that] features helical astragal" in the lantern. A Submarine cable runs from this light to the Milwaukee Breakwater Light, upon which a lighted danger warning is displayed. The light was recently painted, circa 2007. From 1872 until 1926, the light had its own keepers. Thereafter, this light, like all of the lights in the harbor, was serviced by the resident Lighthouse keepers who were stationed at the neighboring North Point Light Station until it was automated. The light was listed on the National Register of Historic Places in September 2012.
Source: en.wikipedia.org/wiki/Milwaukee_Pierhead_Light
A lighthouse is a tower, building, or other type of structure designed to emit light from a system of lamps and lenses and to serve as a navigational aid for maritime pilots at sea or on inland waterways. Lighthouses mark dangerous coastlines, hazardous shoals, reefs, rocks and safe entries to harbors; they also assist in aerial navigation. Once widely used, the number of operational lighthouses has declined due to the expense of maintenance and use of electronic navigational systems.
The sun emitted a significant solar flare, peaking at 8:27 p.m. EDT on April 24, 2014. Images of the flare were captured by NASA's Solar Dynamics Observatory. Solar flares are powerful bursts of radiation. Harmful radiation from a flare cannot pass through Earth's atmosphere to physically affect humans on the ground, however -- when intense enough -- they can disturb the atmosphere in the layer where GPS and communications signals travel.
To see how this event may impact Earth, please visit NOAA's Space Weather Prediction Center at spaceweather.gov, the U.S. government's official source for space weather forecasts, alerts, watches and warnings.
This flare is classified as an X1.4 flare. X-class denotes the most intense flares, while the number provides more information about its strength. An X2 is twice as intense as an X1, an X3 is three times as intense, etc.
Credit: NASA/Goddard/SDO
Credit:
NASA/SDO
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This is another view of the impressive Multiverse light sculpture by Leo Villareal at the National Gallery of Art in Washington, DC. The 40,000 light emitting diodes are constantly changing patterns as you move down the walkway between the East and West Gallery.
This year, I had the idea of making an image of the “Île d’or” associated with the Milky Way andthe shooting stars of the “Perseids”. Mission not so obvious...
The Île d'Or is located in the Var, in the town of Saint-Raphaël, and faces the Dramont landing beach. It would have inspired Hergé to create the Black Island of the adventures of Tintin.
The Perseids are a swarm of shooting stars visible each year in August, when the Earth crosses its path. This year's peak was around August 10.
First difficulty… On this date the full moon took place. The Milky Way was therefore not visible, because of the strong luminosity emitted by the Moon.
So I made this image on August 2, when the Moon was setting early. The shooting stars were rather rare… Only one visible that evening… And luckily, it passed right above the lighthouse of the island, next to the Rho Ophuici region…
Another difficulty was to manage the heavy light pollution generated by the coastal towns (Sainte-Maxime, Saint-Raphaël and Saint-Tropez). This required reducing the "ISO" of the device and doing "stacking" consisting of stacking several (strictly identical) photos of the sky. The goal was to reduce noise and capture as much information as possible.
We can therefore distinguish the Milky Way, and its "bulb" (or "heart") inside which there are many nebulae, stars and globular clusters.
Here is the final image: panorama of 4 photos taken with the Sigma 28mm f/1.4 - Canon 6d Astrodon. 10 minutes of exposure.
I was accompanied that evening by my father. A good moment of sharing with the family!
Hope you like it, thanks in advance
Mount Etna is one of the most active volcanoes of the world, and that means that it changes frequently and rapidly. Eruptions make the mountain grow, not only at its summit (where there are four craters, one of which is currently building a huge new cone, the "New Southeast Crater"), but also on its flanks. Numerous larger and smaller cones dot the sides of the mountain, some rise up to 300 m above their surroundings, and each one is the product of a single eruption, because none of these flank cones erupts a second time.
The major eruptions in July-August 2001 and in October 2002 - January 2003 built two large new cones on the upper south flank of Etna. The cone of 2001 grew in a matter of a few days and reached a height of about 80 m, whereas the cone of the 2002-2003 eruption took about two months to grow to its final dimensions, and its highest point stands more than 200 m above the pre-eruption surface. Before the eruption, the place was a smooth slope descending from the Torre del Filosofo building at 2940 m elevation to the flat area of the "Piano del Lago" (the plain of the lake) at about 2550 m. When I returned to the area after the eruption, it was like discovering a new world. The smooth slope had become a huge mountain with two large craters, each of which contained multiple vents. Some of the vents still emitted vapor (and they continue to do so to the present day), and there were deposits of sulfur all over the place. Discovering this new volcanic world was a unique experience. Everything was BIG, highly irregular, and extremely colorful. Instantly, the new craters of 2002-2003 became the main attraction for visitors taking the guided tours with the cable-car (which was re-established in 2004 after having been partly destroyed during the 2001 and 2002-2003 eruption) and 4-wheel-drive buses. Some tourists can be seen on the far crest of the huge crater in this image, impressively rendering an idea of the scale. In the background, left of the center, the Southeast Crater rears its fractured cone, which itself had grown at breathtaking speed over the previous 5 years.
The view here is from the southern rim of the more southerly of the two large craters formed in 2002-2003, looking north.
The scene has changed little over the years since I took this photograph, on 26 June 2003. The sulfur deposits have faded somewhat, and parts of the crater walls have collapsed into the vents. Instead, since January 2011 we are assisting to the growth of yet another new volcanic mountain, the New Southeast Crater cone, which stands to the east (right) of the old Southeast Crater cone and has gained more than 200 m in height in one year. But that is another story, a story that is continuing at present, the latest variation on Etna's favorite theme: "How A Volcano Grows".
Photo taken with a Canon AE1 and scanned from original Ektachrome color slide
I often use this lamp to photograph small items. I like the reflections it shows from various lenses. I shot a bunch of reflections from the front surface, and deeper, elements from my Canon SX60 HS camera's lens. Somehow, I prefer this simple image of a readily available and easy to use photographic tool of proven value. It is a trusted part of my photography gear.
#MacroMondays #PhotographyGear
Not only the light-emitting organs, also the eyes show strong fluorescence. Notice that the pronotum ("hat") is transparent! It is rather thick (~ 5 microns), about 5-10 times the thickness of a typical fly wing.
Refflection spectrum of pronotum
Objective: Mitutoyo 7.5 NA 0.21, tube lense 200mm (Nikon)
Illumination: Oblique (white)
Sh2-112 is a visibly emitting nebula in the constellation of Cygnus.
It is located in the northern part of the constellation, about 1.5 ° to WNW of the brilliant star Deneb.
It is a circular H II region of apparent size of about 15', crossed by a dark band on its western side oriented in a north-south direction. It is believed that the star responsible for its excitation is BD+45 3216; estimates of the distance of this star provide a value of 1740 parsec (about 5670 light years), which would place so Sh2-112 in a region of the Orion Arm particularly rich and physically very close to the great nebulous system of Cygnus X.
Translated with www.DeepL.com/Translator
(credits Italina wiki: it.wikipedia.org/wiki/Sh2-112 )
Technical card
Imaging telescope or lens:Altair Astro RC250-TT 10" RC Truss Tube
Imaging camera:ZWO ASI1600MM-Cool
Mounts:Mesu 200 Mk2, Astro-Physics Mach-1 GTO CP4
Guiding telescope or lens:Celestron OAG Deluxe
Guiding camera:ZWO ASI174 Mini
Focal reducer:Riccardi Reducer/Flattener 0.75x
Software:Main Sequence Software Seqence Generator Pro, Pleiades Astrophoto PixInsight
Filters:Astrodon L Gen.2 E-series 36mm, Astrodon HA 36mm - 5nm, Astrodon B Gen.2 E-series 36mm, Astrodon G Gen.2 E-series 36mm, Astrodon R Gen.2 E-series 36mm, Astrodon S-II 36mm - 5nm, Astrodon O-III 36mm - 5nm
Accessories:ZWO EFW, MoonLite NiteCrawler WR30
Resolution: 2328x1760
Dates:July 7, 2019, July 21, 2019, Aug. 30, 2019, Aug. 31, 2019
Frames:
Astrodon B Gen.2 E-series 36mm: 35x30" (gain: 75.00) bin 1x1
Astrodon G Gen.2 E-series 36mm: 35x30" (gain: 75.00) -20C bin 1x1
Astrodon HA 36mm - 5nm: 148x600" (gain: 200.00) -20C bin 1x1
Astrodon O-III 36mm - 5nm: 30x600" (gain: 200.00) -20C bin 1x1
Astrodon R Gen.2 E-series 36mm: 35x30" (gain: 75.00) -20C bin 1x1
Astrodon S-II 36mm - 5nm: 42x600" (gain: 200.00) -20C bin 1x1
Integration: 37.5 hours
Avg. Moon age: 6.39 days
Avg. Moon phase: 27.92%
Astrometry.net job: 2916861
RA center: 308.507 degrees
DEC center: 45.642 degrees
Pixel scale: 1.007 arcsec/pixel
Orientation: 90.074 degrees
Field radius: 0.408 degrees
Locations: AAS Montsec, Àger, Lleida, Spain
Data source: Own remote observatory
Remote source: Non-commercial independent facility
Seen at Bushy Park, Wanganui
The hihi (stitchbird) was both rare and poorly known until the 1990s, as few people had an opportunity to visit the single remnant population on Little Barrier Island. However, thanks to successful conservation management and research, the hihi is now one of the better studied New Zealand bird species, and can be seen at several accessible translocation sites. Hihi are often curious, approaching people for close examination whilst emitting warning calls; yet the calls’ high pitch, and the bird’s rapid movements and colouration can make them hard to detect. Until 2006 the stitchbird was considered to be a honeyeater (Family Meliphagidae), which includes tūī and bellbird and c.100 other Australasian and Pacific species. However, genetic studies showed that the hihi belongs to a family of its own (Notiomystidae), closest to the New Zealand wattlebirds (Callaeidae, comprising huia, kōkako and saddlebacks). The hihi has a complex and unusual breeding system that includes pair and group nesting as well as promiscuity. They use a variety of mating positions and strategies that, when considered together, are unique in the bird world.
Curiosidades : Emite múltiples reclamos, algunos muy parecidos a los sonidos producidos por otros páridos, como el carbonero común. Sin embargo, los sonidos del herrerillo común son mucho menos potentes
Esa relajante tranquilidad y suavidad del sur....esa que hipnotiza como el fuego. El leve sonido del agua pasar por la rivera, la brisa del viento y las hojas moverse suavemente emitiendo un sonido delicado junto con leves crujidos de la madera, ahi parece que el tiempo se detiene, ideal para dejar colgada tu ropa y toalla secando, amarrar una hamaca y dormir.. zzzzzzzz...
Camino de la madera, Chile.
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