If you want us to put it in the simplest words possible, the Zone System is a helps us get the right exposure in all our photos, every time, without fail, even in the strangest light settings, and without a trusty matrix meter. It is a magical system conceived of by none other than Ansel Adams himself, along with photographer Fred Archer in the late 1930s. As the father of landscape describes himself, the Zone System is “not an invention of mine; it is a codification of the principles of sensitometry, worked out by Fred Archer and myself at the Art Center School in Los Angeles, around 1939-40.” These masters of photography created the Zone System to help us expose in tricky lighting situations where the dynamic range is out of whack, or the lighting is fooling your light meter into creating exposures that are too bright or too dark.
The Zone System was originally developed for black and white sheet film, which was the only type used in those days. Sheet film was individually developed on standard exposure papers, but today we have color roll film that can be mass developed on papers with varying exposures. The Zone system is as much applicable to these “modern” methods as they were to the film it was created for, and can even help digital photographers get perfect exposures. And guess what? Digital photographers, the Zone System can work for you too!
Technically you probably don’t. However, for those of you who are exposure perfectionists, the Zone System is extremely effective in measuring different tones and the dynamic range of a frame that you are about to shoot. It helps you make the perfect exposure with just a spot meter to work with. This gives you immense control over what you’re shooting. You don’t just make guesses at what the right exposure might be, or waste film bracketing “just in case”. Thus, you can easily figure out when you require extra lighting, and what kind and amount of lighting that might be, or whether there is need for a fill flash to get the right brightness. It can also help you figure out if you need graduated neutral density filters.
The zone system is highly beneficial in capturing accurate images when the camera is unable to set the exposure to an accurate reading, so that you get to decide what your image will turn out like, and you know exactly how it will look before you make the exposure.
A camera’s metering system measures accurate exposure readings by focusing on the middle grey tones, which is 18% grey. This grey is the average of black and white. So, when you are shooting in a bright area, your camera will try to dim the light by bringing it down to the average and making the image underexposed in the process. Similarly, when you are shooting in a dark area, your camera will try to increase the brightness of the image, making it over-exposed. Understanding this mechanism is crucial to understanding how the zone system can be used.
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Sean Goebel - Mauna Kea Heavens 2 | gif by FD
Will Jupiter’s Great Red Spot turn into a wee red dot? by BOB KING
Watch out! One day it may just go away. Jupiter’s most celebrated atmospheric beauty mark, the Great Red Spot (GRS), has been shrinking for years. When I was a kid in the ’60s peering through my Edmund 6-inch reflector, not only was the Spot decidedly red, but it was extremely easy to see. Back then it really did span three Earths. Not anymore.
In the 1880s the GRS resembled a huge blimp gliding high above white crystalline clouds of ammonia and spanned 40,000 km (25, 000 miles) across. You couldn’t miss it even in those small brass refractors that were the standard amateur observing gear back in the day. Nearly one hundred years later in 1979, the Spot’s north-south extent has remained virtually unchanged, but it’s girth had shrunk to 25,000 km (15,535 miles) or just shy of two Earth diameters. Recent work done by expert astrophotographer Damian Peach using the WINJUPOS program to precisely measure the GRS in high resolution photos over the past 10 years indicates a continued steady shrinkage:
2003 Feb – 18,420km (11,445 miles)
2005 Apr – 18,000km (11,184)
2010 Sep – 17,624km (10,951)
2013 Jan – 16,954km (10,534)
2013 Sep – 15,894km (9,876)
2013 Dec – 15,302km (9,508) = 1.2 Earth diameters
If these figures stand up to professional scrutiny, it make one wonder how long the spot will continue to be a planetary highlight. It also helps explain why it’s become rather difficult to see in smaller telescopes in recent years. Yes, it’s been paler than normal and that’s played a big part, but combine pallor with a hundred-plus years of downsizing and it’s no wonder beginning amateur astronomers often struggle to locate the Spot in smaller telescopes. This observing season the Spot has developed a more pronounced red color, but unless you know what to look for, you may miss it entirely unless the local atmospheric seeing is excellent.
Not only has the Spot been shrinking, its rotation period has been speeding up. Older references give the period of one rotation at 6 days. John Rogers (British Astronomical Assn.) published a 2012 paper on the evolution of the GRS and discovered that between 2006 to 2012 – the same time as the Spot has been steadily shrinking – its rotation period has spun up to 4 days. As it shrinks, the storm appears to be conserving angular momentum by spinning faster the same way an ice skater spins up when she pulls in her arms.
Rogers also estimated a max wind speed of 300 mph, up from about 250 mph in 2006. Despite its smaller girth, this Jovian hurricane’s winds pack more punch than ever. Even more fascinating, the Great Red Spot may have even disappeared altogether from 1713 to 1830 before reappearing in 1831 as a long, pale “hollow”. According to Rogers, no observations or sketches of that era mention it. Surely something so prominent wouldn’t be missed. This begs the question of what happened in 1831. Was the “hollow” the genesis of a brand new Red Spot unrelated to the one first seen by astronomer Giovanni Cassini in 1665? Or was it the resurgence of Cassini’s Spot?
Clearly, the GRS waxes and wanes but exactly what makes it persist? By all accounts, it should have dissipated after just a few decades in Jupiter’s turbulent environment, but a new model developed by Pedram Hassanzadeh, a postdoctoral fellow at Harvard University, and Philip Marcus, a professor of fluid dynamics at the University of California-Berkeley, may help to explain its longevity. At least three factors appear to be at play:
* Jupiter has no land masses. Once a large storm forms, it can sustain itself for much longer than a hurricane on Earth, which plays itself out soon after making landfall.
* Eat or be eaten: A large vortex or whirlpool like the GRS can merge with and absorb energy from numerous smaller vortices carried along by the jet streams.
* In the Hassanzadeh and Marcus model, as the storm loses energy, it’s rejuvenated by vertical winds that transport hot and cold gases in and out of the Spot, restoring its energy. Their model also predicts radial or converging winds within the Spot that suck air from neighboring jet streams toward its center. The energy gained sustains the GRS.
If the shrinkage continues, “Great” may soon have to be dropped from the Red Spot’s title. In the meantime, Oval BA (nicknamed Red Spot Jr.) and about half the size of the GRS, waits in the wings. Located along the edge of the South Temperate Belt on the opposite side of the planet from the GRS, Oval BA formed from the merger of three smaller white ovals between 1998 and 2000. Will it give the hallowed storm a run for its money? We’ll be watching.
At left, photo of Jupiter’s enormous Great Red Spot in 1879 from Agnes Clerk’s Book ” A History of Astronomy in the 19th Century”. At right, Jupiter on Jan. 10, 2014. Credit: Damian Peach
Ham Radio, 1940s
Space Station View of the Full Moon
Credit: NASA & ISS
Comet 67P/C-G is framed by one of Rosetta’s solar wings, which is 46 feet long. A stream of gas and dust extends from an active area of the comet’s neck, about 10 miles away. (via NY Times)
As the daughter of our town’s E.S.D.A. Coordinator, I have always been intrigued by ham radio. My father (and elmer) has been a ham for about 40 years. He actually received his license when he was in high school!
After studying for three weeks, I went to take the ham test. I was very discouraged to see that I was the only girl in the room. However, I was treated like a queen by the group that was hosting the test. They seemed excited to have a female in their midst.
Upon receiving my Technician license, I eagerly awaited the Tuesday night ARES net (which my dad happens to be the Net Control of). Again, I was saddened to hear but a few female voices. Over time, I noticed that the female hams rarely checked in to the net. I wondered why these women who worked so hard to achieve their licenses would not want to take advantage of all that ham radio has to offer.
I hope that women are being encouraged to be active hams. Whether they join a club or simply make contacts, females are providing a fresh voice and perspective to the hobby. So, ladies, do not be shy! Proudly check in with your call sign. You have earned it!
Found a couple old photos of my mom practicing her ham radio skillz back in the day. Ham radio was actually the catalyst through which she met my father. Take that, Internet Dating.
My grandma made that dress she’s wearing with their call letters appliquéd along the hem.
http://player.vimeo.com/video/62255585
Comet Panstarrs captured in gorgeous time-lapse above the skies of Boulder, CO by Patrick Cullis. Lovely stuff.
Comets are mysterious frozen chunks of stellar and planetary debris, these dirty snowballs that wander in darkness until their tails are blown bright and wide by solar winds. Some follow paths so random and eccentric that they may pass a star only once, or perhaps not at all, instead floating through interstellar space, never to be known. But for those fleeting moments, like Panstarrs’ current passage, they are like icy candles lit for our enjoyment by the breath of the sun.
A song of ice and fire, indeed.