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Syncing to the Camera - Sync Speeds
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PostPosted: Mon Mar 12, 2007 2:29 pm 
Sync Connections

Firing a studio flash from the camera requires some form of instruction from the camera to tell the flash when to fire. This can be done with a sync cord, with a Radio Remote Control or, in some cases, by letting the camera fire its own built-in flash to set off the flash-sensitive slave trippers contained in most studio flash units.

But it is difficult or impossible to set the built-in flashes on many cameras so they fire at the right time. Most digital cameras use a “preflash” to set automatic exposure, for redeye reduction or to determine color balance and other settings. Unless the preflash can be disabled in the particular camera, it will trip the studio flash units prematurely and they will not expose the shot. Many cameras, including the popular Canon Digital Rebels, have no facility to disable the preflash and therefore cannot be used to trip studio flash from the camera flash.

These cameras and many others also lack a standard sync terminal to connect a studio flash, but most cameras do have a standard hot shoe. In order to connect a sync cord to such a camera, you may need a hot shoe adaptor. This adaptor provides a standard sync connection to which you can connect the sync cord provided with most studio flash units.

>> Click Here for more info on our HSA Hot Shoe Adaptor

However, the standard “PC style” photo sync cord connection is notoriously unreliable. They become loose, fall out and make poor connections regularly.

Radio Remote Controls

Because of this unavoidable unreliability with the PC sync connection, we highly recommend our CyberSync Radio Remote Control System for syncing our studio lights to the camera. The tiny transmitter slides right onto the camera hot shoe and runs typically for a year or more without changing batteries. A CyberSync receiver may be attached to one of the studio lights and when that light fires, any other studio flash units will also fire via their flash-sensitive slave trippers.

If you wish to make flashmeter tests from various positions in your shooting environment, it’s a simple matter to slip the CyberSync transmitter off of your hot shoe and carry it around with you to test-fire the lights. Or, you can invest in a second CyberSync transmitter expressly for this purpose as well as for backup.

If you are shooting in locations where other photographers are also shooting, you might want to use a separate CyberSync receiver for each of your lights and disable their slave trippers. Another way to accomplish this is to use an LG4X Four Channel Remote Control with a single CyberSync receiver plugged into it. This will fire all of your lights (up to four flash units) from a single receiver and will block slave tripping from other photographer’s lights. It will also, of course, give you complete remote control of your individual power levels right from your camera position.

>> Click Here for more info on our CyberSync Radio Remote Control System
>> Click Here for more info on our LG4X Four-Channel Wired Remote Control

Setting Correct Exposure Times with Studio Flash

First, successful studio flash use normally dictates that you turn off all automatic functions in the camera and shoot in full manual mode with a fixed ISO setting (preferably ISO100 for highest resolution and minimum noise). This will require you to set the aperture and exposure manually. A decent flashmeter is the easiest way to determining proper aperture settings.

>> Click Here for more info on Exposure, Histograms and Flashmeters

The Dreaded Black Band

Perhaps the most frequently asked question from studio flash users is “Why is there a black band across part of my picture?” The answer to this lies in the camera itself. Nearly all shooters are using cameras with focal plane shutters. This is the cause of the black band.

Focal Plane Shutter Explained

A focal plane shutter exposes the image by moving two light-blocking curtains across the front of the image sensor. The first curtain slides open to begin the exposure, then the second curtain slide closed to terminate the exposure. In order to expose the picture from a flash, both curtains must be open at the time the flash is fired.

As you shorten the camera’s exposure time a point is reached where the first curtain is not completely open before the second curtain begins to close. The effect becomes a “moving slit” that slides in front of the sensor at this critical exposure time setting. Thus the camera maker specifies a maximum sync speed that assures both curtains will be completely open when the flash is fired. If the flash is fired at shutter speeds faster than the maximum flash sync speed part of the sensor will be blocked by one of the curtains and part of the shot will be blacked out.

The maximum flash sync speed varies from camera to camera, with most modern digital SLR cameras being rated between 1/125 and 1/250 second. In order to avoid the black bars, you must not exceed these speeds. You must also consider any delay that might be introduced by radio remote controls since these can introduce a small delay between when the camera sends the fire command and when the flash unit actually receives it. It is therefore prudent to set the camera shutter speed somewhat below the published maximum flash sync speed. If your camera is rated at 1/200 second, shoot at 1/125 second to avoid problems.

What Sync Speed Should I Use in the Studio?

Many shooters don’t realize that in typical studio usage it is almost solely the flash duration of the flash unit that determines action stopping. This is because the brightness of the flash is typically hundreds of thousands brighter than the ambient studio lighting and modeling lamps. So, even if you shoot at 1/30 second shutter speed, the ambient light is generally so much weaker than the flash that it doesn’t contribute to the exposure. Setting the shutter speed at 1/60 to 1/125 will almost always result in proper flash exposures with no black bars or motion-blur.

Combining Flash with Sunlight or Other High Ambient Light

This situation changes when you are using flash outdoors or in areas with extreme amounts of ambient light. Here, the contribution of ambient light can approach or exceed the flash exposure and must be balanced and controlled.

If, for instance, the camera meter reads f8 at 1/60 second from the ambient light and you wish to use fill flash to bring the subject illumination up to f11, you would adjust the flashpower to achieve f8 from the flash unit. Then the subject will receive equal amounts of light from both the flash and ambient light – f11.

If you shoot a test picture under these conditions and see that you need more flash and less ambient, you can adjust the flashpower upward and shoot at a higher aperture to get the proper exposure. You can also move the shutter speed up to say 1/125 and leave the flashpower alone. The change in shutter speed will lower the amount of exposure from ambient light but will have no effect on the flash exposure. You cannot, however, set the shutter speed faster than the maximum flash sync speed or you will have dark bars on the flash exposure. If you cannot achieve sufficient flash by these methods you need to move the flash unit in closer to increase its illumination level.

This is tricky stuff. It is recommended the shooter endeavor to understand the relationships between ambient and flash and shutter speed and aperture, then do a lot of practicing. There are many good books on the subject.

Sports Shooting

These relationships are particularly important when shooting in sports arenas where the ratio of ambient to flash is considerable and where stopping action is paramount. Here, the power and flash duration of the flash are important. The flash must overpower the ambient light and the flash duration must be fast enough to stop action. This typically requires a T.5 flash duration of 1/1200 second or faster for good action stopping with as much flashpower as possible. Once again, shutter speeds faster than the camera’s maximum flash sync speed cannot be used to diminish the ambient light contribution or dark bars will result.


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