Photography may be the most important and most often used tool in the inspection and analysis of any accident reconstruction, product liability, or testing project. As professionals, our photographs need to be accurate, good quality, consistent, and useful. The key to all four is not usually new gear, but to improve the photographer. New gear won’t help much if you haven’t mastered the gear you already have.
This class is designed to help you consistently make good, accurate, and useful photos—every day in all kinds of light. We don’t always get to choose the locations, conditions, and light, but we must come back with usable photos in all conditions.
My next SAE C1729 Photography for Accident Reconstruction, Product Liability, and Testing class: https://www.sae.org/learn/content/c1729/ will be in Orlando, FL, from May 5 through 7, 2026. Here is the second of two posts showing some examples from the topics we’ll be discussing during the class.
Tire Marks at Wreck Site with and without Polarizer
Both 1/80 sec, ISO 200 made using Nikon D3s with Nikon 24-70 mm f/2.8 lens at 50 mm. Left without polarizer f/14, 1/80, ISO 200. Right with polarizer f/11, 1/80, ISO 200. [Click on image to enlarge, then click on back arrow to return to this post.]Polarizer plus Fill Flash Bring Out Details in Car
Left image without flash or polarizer. Right image with both. Both images were made with Nikon D810 with 24-70 mm lens at 40 mm with exposure 1/60 sec, ISO 160, and f/13 (w/o) and f/10 (w/). [Click on image to enlarge, then click on back arrow to return to this post.]Polarizer plus Fill Flash Reveals Critical Detail
Left image with no flash or polarizer. Right image with flash & polarizer. Note white scrapes on LR fender of right image that are obscured by glare on left image. Both made with ZEISS 50 mm f/2 macro lens on Nikon D850 at f/11, 1/25, ISO 64. [Click on image to enlarge, then click on back arrow to return to this post.]Side Lighting from Sun Illuminates Textures Hidden by Shade
Sun brought out texture and detail at White Sands, NM. Made with Nikon Z 8 and 24-70 mm f/2.8 lens at 33 mm with exposure f/11, 1/125/ ISO 64. [Click on image to enlarge, then click on back arrow to return to this post.]Scaling and Matching Photos Each Made Exactly Square to Camera
By ensuring scales were perpendicular when photographing both the car & the truck (three months later), allowed matching of lug nuts and scratch patterns. Both car & truck photos made with Nikon Z 7ii with Nikon Z 50 mm macro lens at f/13, 1/15 sec, ISO 64. [Click on image to enlarge, then click on back arrow to return to this post.]Faded Police Paint Marks Enhanced in Photoshop
Police paint marks that had faded & were coated in road salt were enhanced in Photoshop. Made with Nikon D3 and Nikon 24-70 mm f/2.8 lens at 50 mm with exposure f/9m 1/80 sec, ISO 200. [Click on image to enlarge, then click on back arrow to return to this post.]Effects of Image Size and Viewing Distance on Perspective
A photo made with a super wide and another one made with a telephoto lens viewed from the same position shows distortion in each. But viewed from the proper viewing distance, they can both look “normal”. Both made with a Nikon D810 with exposure f/10, 1/80 sec, ISO 64.
Setup for Ensuring Measuring Gauge is Perpendicular to Camera
Using Wimberley The Plamp II to hold Alcoa rim wear gauge in proper position & perpendicular to camera for photograph. Both made with Nikon D850 & ZEISS 50 mm f/2 macro lens with exposure f/14, 1/60 sec, ISO 64. [Click on image to enlarge, then click on back arrow to return to this post.]Setting Custom White Balance with Flash for Proper Color
Screen shots of menu of Nikon Z 8 with Godox TT685Nii flash with Flash WB on left, then with custom (Preset) WB—with flash!—on right. [Click on image to enlarge, then click on back arrow to return to this post.]In the class, we will explore all of these—and more!—including demonstrations and hands-on photo sessions so these techniques become useful tools for your investigations and analyses. Please make sure to check out Part One of this post for some of the other topics we’ll cover: https://vadnaisengineering.com/2025/08/28/examples-from-my-sae-automotive-forensic-photography-class-c1729/
Most importantly, we’ll build a good foundation of exposure, focusing, and composition. All along we’ll emphasize the importance of proper tripod, polarizer, and flash (including multiple flash) use. Additionally, we’ll learn about both kinds of night photography (documenting evidence at night vs accurately recording ambient light). We’ll also see how to properly size an image and to determine the proper viewing distance for the proper perspective.
This first class offering of 2026 is conveniently offered in Orlando, which is easy to get to from anywhere in the country. Please let me know if you have any questions. I hope to see you there.
During my SAE classes (https://www.sae.org/learn/content/c1729/) and various other classes and presentations, I demonstrate and recommend Godox flashes—specifically the TT685ii. They are powerful, robust, and intuitive to use.
They have the same technical specifications and features (including: guide number 197 ft/60 m at ISO 100; fully rotating and tilting head; and, built-in radio transmitters/receivers) as the equivalent camera manufacturer’s flashes, but at only $129, cost only 12% to 22% as much! [Click on image to enlarge, then click on left arrow to return to this post.]
Godox TT685iiN mounted on Nikon Z 8, with flash head tilted up and rotated right.
In other words, you can buy 4.5 to 8.5 Godox TT685ii flashes for the price of a single camera brand flash. This means you can buy two (or three) Godox TT685ii flashes and still have plenty of money for rechargeable batteries and a charger for them. (Of course, you’ll need the batteries and a charger regardless of which flash you buy.)
For off-camera use, I highly recommend getting at least two of these flashes. I always carry at least three TT685iiN flashes, along with an X3 N hot shoe trigger so I can use all flashes off-camera if necessary. (I also use the X3 N hot shoe trigger with my Godox MF-12 macro flashes. I’ll describe them in a future post.)
Important: To use TTL (through-the-lens) flash exposure, make sure you buy flashes designed for use with your camera brand.For example, I shoot Nikon, so I use the TT685iiN versions. Godox makes versions compatible with Nikon, Canon, Sony, FUJIFILM, and Olympus/Panasonic. This allows the flashes to be used in TTL mode. [Click on image to enlarge, then click on left arrow to return to this post.]
Godox TT685 Flash Hot Shoes for different camera brands. (Made with ZEISS Milvus 50 mm f/2 Macro lens on Nikon D850 at f/16, 1/200 sec, ISO 64. One Profoto B1x strobe to each side triggered by a Nikon SB-910 flash in the camera’s hot shoe.)
In the image above, the flash at the far left (“M”) is a full manual(non-camera specific, non-TTL) model. It has a single contact to allow the camera to fire the flash with fully manual settings (except with Sony cameras). The other flashes, from left to right, are Nikon, Canon, FUJIFILM, Olympus/Panasonic, and Sony.
Note that any flash may be used in full manual mode with any camera brand—except with Sony. The pin that fires the flash is offset on the Sony proprietary hot shoe (far right in photo above), so it doesn’t reliably fire a non-Sony flash—if fires it at all. Sony’s proprietary hot shoe means a Sony-compatible flash must be used on a Sony camera. It also means that Sony-specific flashes will not work in non-Sony camera hot shoes (although they will work as remote flashes).
I’ve been using TT685iiN flashes (I have six of them) almost daily since their release almost four years ago without a single problem or malfunction. I previously used the original TT685N flashes (I have three of them) without any issue. I also have bought another twenty or so TT685ii flashes for other camera brands for students to use in my classes. (Full disclosure: I am not affiliated with Godox. I just use and like their stuff!)
Note: The Godox V860iii is identical to the TT685ii, but it includes a proprietary rechargeable lithium-ion battery, and costs $100 more. The Godox V1 is identical to the V860iii, but has a round head and costs $30 more than the V860iii and $130 more than the TT685ii). All three flash models are fully interchangeable as on-or-off camera flashes with the Godox radio control system. A future post will illustrate and describe the differences between the Godox flash models.
Regardless of what flash brand you get, I strongly encourage you to get at least two flashes. Two flashes allow you to use the off-camera flash to fill in shadows and for side lighting to bring out textures, stampings, and raised lettering or elements. You’ll find they are something you’ll use almost daily in your forensic photography.
Takeaways:
-1- Godox TT685ii, V860iii, and V1 are well-made, robust, powerful, and intuitive flashes that cost much less than, but have the same performance specs as, flashes sold by camera manufacturers.
-2- This significantly lower cost makes it easy to buy two or more flashes, plus rechargeable batteries and a battery charger, for less money than a single camera manufacturer’s flash.
-3- Two flashes allow you to use the off-camera flash to fill in shadows and for side lighting to bring out textures, stampings, and raised lettering or elements.
-4- You need to make sure at least one of your flashes is compatible with your camera brand so you can use TTL (through-the-lens) flash exposure.
-5- If you don’t need or want light coming from a flash in your camera’s hot shoe, adding an X3 or X3 Pro hot shoe trigger will allow you to use all your flashes off camera, even in TTL.
My next SAE C1729 Photography for Accident Reconstruction, Product Liability, and Testing class: https://www.sae.org/learn/content/c1729/ will be in Orlando, FL, from May 5 through 7, 2026. Here is the first of two posts showing some examples from the topics we’ll be discussing during the class.
Tracking a Vehicle During Testing
Tracking by panning with Nikon D800E with 300 mm f/2.8 lens at f/6.3, 1/640 sec, ISO 400. [Click on image to enlarge, then click on back arrow to return to this post.]Using Fill Flash to Show Details in Shadows
Both with Nikon D850 and ZEISS Milvus 50 mm f/2 macro lens. Left side: No flash at f/10, 1/60 sec, ISO 64. Right side: Fill flash at f/11, 1/80 sec, ISO 64. [Click on image to enlarge, then click on back arrow to return to this post.]Showing Depths of Abrasions and Damage Using Two Flashes vs Ambient
Left side: Ambient only; Right side: One Profoto B1x strobe on either side of tread. Both with Nikon D850 with ZEISS Milvus 50 mm f/2 macro lens at f/16, ISO 100, 4.0 sec left & 1/200 sec right. [Click on image to enlarge, then click on back arrow to return to this post.]Controlling Background Brightness while Keeping Flash the Same
Both made with Nikon D850 and ZEISS Milvus 50 mm f/2 macro lens at f/14, ISO 64 with flash in hot shoe. Left side: 2.0 second exposure for bright background. Right side: 1/250 sec exposure for dark background. Background itself didn’t change. [Click on image to enlarge, then click on back arrow to return to this post.]Keeping Background Brightness the Same while Adding Fill Flash
Left side: Ambient light only. Right side: Same ambient light with added fill flash. Both with Nikon Z 8 with ZEISS Milvus 50 mm f/2 macro lens at f/16, 1/25 sec, ISO 64. [Click on image to enlarge, then click on back arrow to return to this post.]Using Macro Flashes vs On-Camera Flash for Recessed Subjects
Left side: flash in hot shoe (Godox TT685IIN) with head tilted -7°; Right side: one small macro flash (Godox MF-12) on either side of lens—no light from hot shoe flash. Both with Nikon D850 with ZEISS Distagon 25 mm f/2 lens at f/16, 1/200 sec, ISO 64. [Click on image to enlarge, then click on back arrow to return to this post.]Unintended Deception from Camera Position, Even with Same Lens
Both made with Nikon D850 with ZEISS Milvus 50 mm f/2 macro lens with fill flash. Left side: f/13, 1/40 sec, ISO 125. Right side: f/16, 1/30 sec, ISO 200. [Click on image to enlarge, then click on back arrow to return to this post.]Eliminating Glare Such As On Plastic Evidence Bag Using Two Flashes
Both made with Nikon D850 with ZEISS Milvus 50 mm f/2 macro lens. Left side: Ambient only (f/16, 1.0 sec, ISO 16). Right side: Ambient with one flash at right and one at left (f/16, 1/200 sec, ISO 64). [Click on image to enlarge, then click on back arrow to return to this post.]Using Tripod, Manual Exposure, & Manual Flash to Ensure Consistent Images for Demonstrating Function of Subject
Using a tripod, manual exposure, and manual flash ensure consistency between images. Both made with Nikon D850 and ZEISS Milvus 50 mm f/2 macro lens at f/16, 1/40 sec, ISO 64 plus flash. [Click on image to enlarge, then click on back arrow to return to this post.]Some of you may have noticed that—except for the Explorer testing, the Trailblazer, and the onboard tire inflation system images—each pair of images had the same exact composition. Only the lighting changed. This was only possible by using a tripod. Tripod use will be another area of concentration and practice in the class. Hopefully, you’ll learn to love using your tripod like I love using mine.
I’ll post another set of photograph pairs later to illustrate additional areas we’ll cover in the class.
In the meantime, please don’t hesitate to contact me by e-mail or phone if you have any questions or would like more information. I look forward to seeing you in Orlando, FL, in May. For more details or to register for the class, here is the link for the class: https://www.sae.org/learn/content/c1729/.
Both 1/80 sec, ISO 200 made using Nikon D3s with Nikon 24-70 mm f/2.8 lens at 50 mm. Left without polarizer f/14. Right with polarizer f/11.
[Click on image to enlarge, then click back arrow to return to this post.]
SAE will once again be hosting my class C1729 entitled Photography for Accident Reconstruction, Product Liability, and Testing from March 18-20, 2025. This time it will be in Peoria, AZ.
We will start with the basics of camera setup, menus, exposure, and gear (especially flashes, tripods, and polarizers). We will build on that with composition and focusing. There will be plenty of comparison images between bad and good images so we can see how and why images can be improved to show more detail and become more useful.
We will also discuss the special requirements and procedures for macro (close-up) and night photography, along with the importance of proper perspective. Finally, we will review file handling and post-processing.
We will have extended hands-on sessions to apply what we’ve learned to real world situations. As always, I will be bringing additional flashes, tripods, and polarizers for those who don’t have them, or who don’t have good ones, or who want to try new equipment.
There is still time to register for one or more of the forensic photography short courses being offered next week. Each will be from 8:00 am to 12:00 noon EST. They are:
Monday, January 20: Using Flash in Forensic Photographyby Tom Vadnais.
Tuesday, January 21: Close-Up and Macro Evidence Photography by Jerry Narowski.
Wednesday, January 22: Precision Lighting for Evidence Photography by Gale Spring.
Thursday, January 23: Photoshop Enhancement Techniques by George Reis.
Each four-hour course is only US$75, and each qualifies for continuing education credits after a short test and assignments are completed. Best of all, you’ll immediately be able to apply what you learn in each class in your daily work.
Here is a link for the descriptions and registrations for the four short courses—one per day next Monday through Thursday: https://www.ai2-3d.com/fps-courses
The Symposium will be held each of those days after the short courses. For the schedule and to register for the Symposium itself, please follow this link: https://www.ai2-3d.com/fps2025-schedule
You’ll need to register separately for each short course and for the Symposium itself. Since they’re all virtual, you don’t even have to travel!
While a tire expert can glean a bit of information from examining a tire that is still mounted on its rim, a tire analysis is rarely considered complete without a thorough inspection of its beads and its interior. Of course to do this, the tire has to be demounted from its rim.
It is common practice for the first tire expert who receives an assembled tire and wheel to photograph both sides of it. Next, that expert will mark the valve stem position on the outside sidewall with a tire crayon or silver ink pen (unless both beads are unseated and the tire freely rotates around its rim). Finally, the expert will have the tire demounted from its rim by an experienced tire tech. Most of the time, there is no need for other tire experts to be present during the tire demounting.
While this example is not from a case, this happened to me, and illustrates why it would have been essential to demount the tire to figure out why it failed.
I was driving my old Ford F-150 pickup to retrieve a truck tire and wheel for analysis when I heard a popping then a flopping noise from the rear. I wasn’t sure what it was, so I pulled over and saw the right rear tire had gone flat. [Click on image to enlarge, then click on back arrow to return to this post.]
Made with iPhone 11 Pro Max at f/1.8, 1/120 sec, ISO 32.
I saw this fairly long radial split or cut, but couldn’t tell what had caused it. Being a tire engineer, I regularly inspect my tires while keeping them properly inflated, but I hadn’t noticed any pending issue.
At the tire store, they demounted the tire and called me over to see. Somehow, this blade from a pair of shears cleanly penetrated the sidewall, carcass, and innerliner, and ended up inside the tire. [Click on image to enlarge, then click on back arrow to return to this post.]
Made with iPhone 11 Pro Max at f/1.8, 1/105 sec, ISO 125.
I would never have guessed that this long blade could have so cleanly and completely passed through the sidewall of a tire rotating at 45 mph. And without removing the tire from its rim, I would never have known what caused that radial cut.
Fortunately, in this case I knew the prior condition of the tire and about how suddenly the failure occurred.
In actual cases, it’s extremely rare to have such clean cut evidence (pun intended). In Part Two, I will show several examples of tire conditions that could only have been determined after the tire was demounted.
Takeaways:
-1- While a tire expert can gather information about a failed tire while it is still mounted, a thorough analysis cannot be completed until the tire is demounted from its rim.
-2- Demounting a tire from its rim is essential so the tire beads, the inside of the tire, and the condition of the wheel can all be analyzed. This includes examining for cracks, punctures, mounting/demounting damages, and repairs.
-3- On rare occasions like the one described, the actual cause of the failure is immediately obvious when the tire is demounted.
-4- It is common practice for the first tire expert to receive the tire and wheel assembly to photograph it as mounted, mark the valve position on the outside sidewall (if the beads are still seated), and have the tire professionally demounted. Typically, other tire experts do not need to be present for the demounting.
(Note: This post incorporates several important fundamentals along with the discussion of controlling sun stars. As always, it’s all summarized in the Takeaways at the end.)
A previous post illustrated how the number of aperture blades affected the number of rays produced in a sun star. As discussed, sun stars are created from bright spots of light in an image when the lens aperture is stopped down. While prominent sun stars might be desirable for landscape or creative photographs, they are usually unwanted in forensic photos. In fact, there have been instances where photographs with distinctive sun stars have been limited or disallowed. Here’s how to control—or even eliminate—their prominence.
There were three small, distinct bright light sources in the following night scene. A series of images was made at every whole aperture from f/16 through f/2. (As a reminder, there are six stops up from f/16: f/11, f/8, f/5.6, f/4, f/2.8, f/2.) Only four of the seven total images—each two stops apart—will be shown below. The other three intermittent images fit in the progression as you’d expect from what you’ll see below.
This first image was made with the aperture stopped down to f/16. As expected, the sun star rays were most distinct at this aperture. [Click on image to enlarge, then click on back arrow to return to this post.]
Sun Stars at f/16 made with Nikon Z 8 with Nikkor Z 50 mm f/1.2 S lens at f/16, 2.5 sec, ISO 64.
Opening up two stops to f/8 noticeably reduced the sun star effect. [Click on image to enlarge, then click on back arrow to return to this post.]
Sun Stars at f/8 made with Nikon Z 8 with Nikkor Z 50 mm f/1.2 S lens at f/8, 0.6 sec, ISO 64.
Opening up two more stops to f/4 almost completely eliminated the sun star effect. This should be acceptable for any foreseeable use. [Click on image to enlarge, then click on back arrow to return to this post.]
Sun Stars at f/4 made with Nikon Z 8 with Nikkor Z 50 mm f/1.2 S lens at f/4, 1/6 sec, ISO 64.
Finally, opening up yet two more stops to f/2 eliminated any trace of sun star rays. [Click on image to enlarge, then click on back arrow to return to this post.]
Sun Stars at f/2 made with Nikon Z 8 with Nikkor Z 50 mm f/1.2 S lens at f/2, 1/25 sec, ISO 64.
As you can see, the wider open the aperture (which means the lower the f-number), the less pronounced are the sun stars. But you can’t just adjust your aperture to either intensify or to eliminate sun stars. Whether it is daytime or nighttime photography, changing your aperture affects your image in two main ways: exposure and depth of field (DOF).
Recall that the smaller the f-number, the larger the lens opening. Just like 1/2 of a pie is twice as large as a 1/4 of a pie, a lens aperture of f/2 is twice the diameter of f/4. Here’s how changing aperture changes exposure and DOF:
Exposure: Opening the lens aperture lets in more light, which brightens the exposure. To keep the overall exposure the same, you must compensate by the same number of stops by using a faster shutter speed, lowering your ISO, or using a combination of both. Since all the above images were already at my Nikon Z 8’s lowest ISO of 64, my only option was to select a correspondingly faster shutter speed every time I opened up the aperture.
This means that for this series of four images, every time I opened up the lens aperture by two stops, I had to use a shutter speed that was two stops faster. As you can see from the captions under the images, at a constant ISO 64, the f/16 image required a 2.5 second exposure. Opening the aperture two stops to f/8 required a shutter speed of 0.6 seconds, which is two stops faster. Likewise, f/4 required 1/6 second and f/2 needed 1/25 second to keep the same overall exposure. Each were two stop increments of aperture and shutter speed.
As a side note, since the camera remained on a tripod throughout all the photographs, the shutter speed had no effect on the sharpness of the images. But changing shutter speeds will definitely affect the appearance of any moving elements in the image frame.
Depth of Field (DOF): DOF is how much of the scene—from near to far—is in acceptable focus for a given focus point. DOF is controlled by aperture. The more open the aperture, the less DOF. Conversely, stopping down the lens aperture increases DOF.
A deeper DOF is more critical in daytime photographs where almost everything is visible and, in most forensic photography, should be acceptably sharp. At night, a more shallow DOF can be perfectly acceptable, especially if the background and foreground are mostly black, as in the photos above.
As you can see on the enlargements by clicking on the photos above, f/4 would likely produce acceptable DOF. Depending on your case, even f/2 (or an aperture between f/2 and f/4) might give you all the DOF you need. As the photographer, you need to (and you get to!) decide on the tradeoff between DOF and sun star prominence.
Takeaways:
-1- You can control the prominence of sun stars from small, bright light sources (day or night) by your choice of aperture. The more stopped down your aperture, the longer and more prominent the rays. Opening up the aperture will shrink the rays until they essentially disappear at the most open apertures.
-2- Opening up or stopping down your aperture will also affect the DOF in your image. You must decide how much DOF you will need. That amount would likely be different for daylight versus night photos—even of the exact same scene.
-3- Just like with any other photography, opening up or stopping down the aperture will require that you correspondingly adjust your shutter speed, ISO, or a combination of both, to maintain the same overall exposure. Make sure your shutter speed is sufficient for your image, especially if there are moving objects in your frame. Also, setting your ISO as low as possible minimizes noise and maximizes dynamic range, both of which are even more important in night photography.
Many lenses have an odd number of aperture blades, but several have an even number. For most photography, there is little to no noticeable effect.
There is, however, a noticeable difference if you have a “sun star” in your image. A “sun star” is the name given to noticeable rays—day or night—emanating from the sun or from an artificial light source. A sun star is created when the lens is stopped down. The more the lens is stopped down, the larger the rays of the sun star.
An even number of aperture blades results in the same number of sun star rays. As the image below shows, a lens with ten blades (the TTArtisan 50 mm f/2 lens), stopped down to f/16, resulted in ten pronounced rays from a street light at night. [Click on image to enlarge, then click back arrow to return to this post.]
Made with Nikon Z 8 with TTArtisan 50 mm lens at f/16, 3.0 sec, ISO 64.
An odd number of blades results in twice the number of rays. Using the same camera as above, but switching to a lens with nine aperture blades (the Nikkor Z 50 mm f/1.2 S lens), also stopped down to f/16, resulted in eighteen sun star rays. [Click on image to enlarge, then click back arrow to return to this post.]
Made with Nikon Z 8 with Nikkor Z 50 mm f/1.2 S lens at f/16, 2.5 sec, ISO 64.
Takeaways:
-1- Day or night, “sun stars” are often created from small, bright light sources in a photograph when lenses are stopped down.
-2- An even number of lens aperture blades creates the same number of sun star rays. An odd number of blades results in double the number of rays.
-3- An even number of blades creates more pronounced rays than does an odd number of blades.
-4- Sun stars are usually undesirable in forensic photographs. A future post will describe how to control the prominence of those rays. But if you must stop down for depth of field, an odd number of lens aperture blades will create more rays, but they will be less obtrusive.
One kind of forensic night photography requires you to accurately capture the appearance of a scene as closely as possible under lighting conditions similar to what they were at the time of an incident. Of course that results in an overall image that appears dark since, after all, it is a night scene.
Using fully automatic exposure modes will result in the scene being significantly (and obviously) overexposed. This is because the camera is trying to record the scene as a mid-tone (frequently referred to as “middle gray” even when the subject isn’t gray). This automatic brightening of night scenes usually results in noisy, overexposed images that don’t resemble the actual scene at all.
Almost all consumer and prosumer cameras have a fully automatic exposure mode denoted by a green camera icon with or without the word “Auto”. The image below shows the full Auto mode icon on a Nikon D5600 and Canon T7i. (Professional cameras like my Nikon Z 8’s often do not have this mode.) [Click on the image to enlarge. Then click on back arrow to return to this post.]
Made with Nikon D850 and ZEISS Milvus 100 mm macro lens.
In Auto mode, the camera sets the aperture, shutter speed, and ISO, and you cannot change or override any of them! Because the photographer cannot affect exposure in any way in full Auto mode, when teaching I refer to it as the “Green Mode of Shame” to drive home the point that you as the photographer are left without any ability to control your exposure (or a number of other important settings). While this mode might work for ideal lighting during the day, it just doesn’t—and can’t—work for ambient light night photographs. (Note: Semi-automatic exposure modes Program, Aperture Priority, and Shutter Priority will be addressed in a future post.)
I made the following two images in a lighted parking lot that had a white, a black, and a silver vehicle in the scene. (Note: both images were captured in the camera’s raw NEF format.)
For this first image, I used a Nikon Z 5 in Auto mode (its Green Mode of Shame). As discussed above, the camera tried to create a mid-tone image, and I couldn’t do anything about it. [Click on the image to enlarge. Then click on back arrow to return to this post.]
Auto exposure mode with Auto ISO. Made with Nikon Z 5 with Nikkor Z 24-70 mm f/4 lens at 49 mm in raw mode. f/4, 1/50 sec, ISO 25,600.
Note the camera chose a wide open aperture to let in as much light as possible (f4 on that lens), and an ISO of 25,600(!), while setting the shutter speed to 1/50 of a second. (A shutter speed of 1/50 of a second is considered handholdable with a near 50 mm focal length. The thinking is that if someone is going to use a camera in Auto mode, the camera will most likely be handheld. Consequently, the camera will open the aperture and boost the ISO to keep the shutter speed handholdable. But as usual, I had this camera on a tripod, like I almost always do in any light. )
Even though the original image is quite noisy (the great reduction in size and the JPEG compression of this posted image reduced the appearance of noise from the original raw), that’s not the biggest issue with it. The real problem is the scene was nowhere near this bright; it didn’t look anything like this at the time I made this image.
For the image below, I switched to manual exposure mode (the only exposure mode I ever use). I kept the aperture at f/4, but then set the ISO to the camera’s minimum of 100 to minimize the image noise. Because the camera was on a tripod, I wasn’t too concerned about shutter speed as long as it stayed within reason. [Click on the image to enlarge. Then click on back arrow to return to this post.]
Manual exposure mode with ISO set at 100. Made with Nikon Z 5 with Nikkor Z 24-70 mm f/4 lens at 49 mm in raw mode. f/4, 1/3 sec, ISO 100.
With the aperture and ISO set, I adjusted the shutter speed until the image on the back of the LCD looked like what I was seeing with my naked eye. As it turns out, the Auto image was four stops lighter than this more accurate one.
Note 1: By default, I have the camera’s Picture Control set to Neutral with reduced contrast and saturation so the LCD closely matches my computer monitor.
Note 2: For an actual night photograph case, I start by tethering my camera to a laptop that is calibrated to match my desktop monitor. There’s much more to the actual process than I did for this demo, but it’s close enough to illustrate the point that you need to take manual control of the camera.
While this second image is close to showing the scene as I saw it, to view it properly, you would need to view it with a black surround in a darkened room with your monitor brightness set to 140 cd/m² to match what I see. Regardless of these technicalities, comparing the two images—in whatever light you’re in or computer you’re on—it is obvious that the upper Auto exposure image doesn’t look anything like the more accurate lower manual exposure mode image.
In a number of cases where I’ve done both the night photography and explained why photographs submitted by other experts or photographers were improper and misleading, all of those inaccurate photographs have been stricken and disallowed by the judge.
While it’s a little bit off-topic, being able to explain how and why photographs were made and why they accurately represent what they purport to show—and why other ones don’t—is critical in almost all ambient light night photography cases.
Takeaways:
-1- Fully automatic exposure modes (like Auto) are not designed to—and cannot—accurately capture ambient light night images.
-2- You need to shoot night photographs using manual exposure mode with a low ISO to minimize noise, with the appropriate aperture for the depth of field you need, and with the shutter speed set to match what the scene looks like to the naked eye. There’s much more to the whole process, but that’s the essence of it.
-3- While the lower photo looks much closer to what the parking lot looked like when I made the photographs, it was not made with the procedure I use for case work. It is close enough to make a quick demo comparison against a demonstrably incorrect Auto method that yielded a demonstrably incorrect image.
When inspecting a truck and downloading its HVEDR, it is important to document the actual tire parameters. This includes not only confirming tires sizes, but their load ranges. You must confirm that the tire sizes and load ranges match those on the safety certification label on the door jamb and in the values programmed into the HVEDR.
In its 2023 Truck Tire Data Book, Michelin summarizes the effects of different revs/mile in this Rule of Thumb: “When going from a lower Tire Revs./Mile [sic] to a higher Tire Revs./Mile, the actual vehicle speed is less than the speedometer reading. When going from a higher Tire Revs./Mile to a lower Tire Revs./Mile, the actual vehicle speed is greater than the speedometer reading.”
The revs/mile differences between load ranges in a given tire size might not be large, but they do exist—even in the same line of tires. For example, Michelin lists two 11R22.5 X Multi D tires: one load range G and the other load range H. For the load range G tire, Michelin lists the revs/mile as 496 while it lists 494 revs/mile for the load range H tire. Likewise, for the 11R22.5 Michelin X Line Energy Z tire line, the load range G revs/mile was 502 and the load range H was 503.
So just between two Michelin tire lines, there is a range of revs/mile from 494 to 503 for 11R22.5 tires. Not only that, but for one tire line, revs/mile were higher for the LRH tire than the LRG, while for the other tire line, the opposite was true.
At first it may seem that all tires of the same size would have the same revs/mile. But variations in tire construction, tread design, and tread depth can result in small variations in the actual revs/mile of a specific tire of the same size.
Tire companies determine the revs/mile from the test procedures set out in SAE Recommended Practice J1025. J1025 specifies speed (45 mph), load, inflation pressure, ambient temperature, configuration, break-in, warm up, surfaces, measurement devices, and test distances required for each test.
The four revs/mile values of the four 11R22.5 Michelin tires above weren’t far apart, but it is best to check and confirm. And even though a small difference in revs/mile may not end up being significant in your analysis, you want to confirm that the truck tires sizes and load ranges matched what was used when programming the HVEDR.
Many trucks have a variety of tire brands, sizes, load ranges, or a mixture of original and retreaded tires. In some cases, the truck may be gone or repaired, and all you have to work with is the HVEDR report itself. When you have tire variations or unknown tires, you might consider researching the ranges of any relevant tire property, like revs/mile, then running a sensitivity analysis to quantify the effect that range of values might have on any subsequent analysis involving data from the report.
Takeaways:
-1- During a truck inspection, don’t just document the tire manufacturer(s) and tire size(s), but be sure to include the tire load range(s). Compare their properties with the programmed values in the HVEDR report.
-2- If there are variations in the truck’s tires, check the various tire properties against the HVEDR programmed values.
-3- Using those tire property variations, it might be useful to perform a sensitivity analysis to quantify the effect of a range of revs/mile or other variable.
-4- To learn how to apply HVEDR data, I highly recommend SAE International class C1901 Advanced Applications of Heavy Vehicle EDR Data taught by Wes Grimes, Greg Wilcoxson, Dave Plant, and Brad Higgins: https://www.sae.org/learn/content/c1901/