Youtube comments of Solar Eclipse Timer (@solareclipsetimer).

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  141.  @emptiester  So, NASA is a public entity and our tax dollars pay for what they do. If they publish a picture, say from a Mars rover, you can use that image for your own work as long as you give NASA the due credit for the image. The same would be true if they published some esoteric data about a neutron star and you needed to use that NASA data: you can do it as long as it is properly referenced. Again, you paid for it with your tax dollars, their work is in the public domain. So, using it is "free," I guess if you want to look at it that way. And giving due credit is obvious. My NASA solar science friend uses my eclipse work and images in her talks and she always asks for my permission first and then gives me credit on the slide in her talk. However, NASA treats the "meatball' logo and the NASA "worm" graphic differently. They protect these as NASA branding and want their use to be limited to projects, events, work, etc. that are DIRECTLY affiliated with something that NASA is involved with and therefore approves of. I know this from working with NASA. You are on the honor system when you work with NASA on something. You are allowed to say you worked with NASA on something, but the wording, the context, and the need for a possible disclaimer are key. NASA NEVER wants those two things to be used to endorse a commercial product or service. So, you really have to be careful and honest. NASA doesn't have the time to police these guidelines everywhere. I hope that answers your question. Thanks for commenting.
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  509. Scott, the diamond ring and Baily's beads can have different goals for exposure depending on what you are trying to achieve with the image. Yes the diamond ring is brighter, because there is more photosphere visible, but it is also more diffuse, or spread out. Some people like the look of an over exposed diamond ring, where you can get that brilliant single sided "star burst" look. When I have taken my shots at 1/1000 or 1/2000 my diamond rings are very "tight". Especially when I am starting at about 20 seconds before C2. I tend not to get a really spread out diamond ring. To get a spread out ring, I think I should be at 1/500, maybe 1/250, because I would like to achieve a big over exposed diamond ring image. The other option would be to start my imaging at 30 or 35 seconds before C2 when there is even more photosphere. Both are ways to achieve a brilliant wide bursting diamond ring image. Remember the Moon is moving, so it is changing the light for you, so some image in the group of images you take is going to be perfect (depending on your tastes). Your first images maybe a "blowout" but the images a few second later maybe perfect. Remember, you are not taking a single diamond ring image. The diamond ring phase is a progression, just like beads are. You just have to take many images rapidly. But Baily's beads are a different issue, because their brightness area is small and becomes super-well defined bright points that get tighter and tighter. To get the final set of beads clearly defined to the limb of the Moon you do not want over exposure. So at this point the faster shutter speed is better. My goal is to make this exciting and rapidly progressing portion of the eclipse photography easy, so using a single shutter speed that is a "happy compromise" is what I teach.
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  766.  @imhusker Thanks for your reply. There are a lot of things in the original Specer document that ended up not being correct, for instance, a cycle life of 1,000 to 10,000 cycles. But that was the first shot at trying to figure out the engineering of carbon fiber hull for OceanGate, so there were a lot of unknowns. The safety factors in the Spencer document are just not relatable to the hull they built. As of this time, there is no comparable document in the public domain about safety factors for the V2 hull. You are correct, that the diagrams for the rings in the Spencer document were very rudimentary, and Tony Nissen testified that he worked with Spencer and another engineer that Tony hired to modify the rings. They came up with a new ring design for the forward and the aft rings as a matched set. They did a lot of engineering to match the moduli of the titanium to the carbon fiber hull. You are correct, I found documentation that the final C-channel width was 5 inches (I have edited the video to reflect that). However, when you watch videos of them gluing the rings on the V1 hull you can see where they milled down the outside diameter of the carbon fiber hull to get it down to 5 inches. (you can see the step-in). They used the same rings for the V2 hull and Phil Brooks testified how they cut the hull off the rings and then milled out the carbon fiber from the rings to reuse them. When you see close-up pictures of the V2 hull meeting the rings you can tell how much wider the hull was compared to the diameter of the rings; the hull steps down to the ring diameter. Thanks for adding to the discussion, I appreciate it.
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  1265. Thank you for your thoughtful comment. I appreciate you taking the time. The bridge analogy came from a certified mechanical engineer Bart Kemper. And, he talks about beam bending in simple mechanical engineering. The center of the Titan's hull did bend inward in the center. It pinched inward more in the center than the ends which were held by the rings. Tony Nissen testified about that regarding the first hull when he saw that the hull was deflecting in the center 37% more than predicted. So the cylinder did move downward, all around it the circumference in the center of the case. The next section of Mr. Kemper's testimony regarded a discussion of the Bailey's Bridge modular design (truss system) which boiled down to how you make it strong enough, and how much damage can occur, and where, before the load can no longer be distributed and things fail. So, if you keep cutting the top truss over the entire span of the bridge you are going to have issues. I thought his simplification was brilliant, especially if you are trying to teach non-engineers like the Coast Guard Board, and me, and the thousands of lay people interested in it. And Mr. Kemper is a smart guy with a lot of marine experience, and although it may have been simplified I don't believe he would have testified under oath on a concept that is flat-out wrong. So, the point I took away was that all of the surface grinding and not having cross-plies decreased the strength of the hull, causing more deflection which in turn loosened the co-bonding glue.
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  1474.  @onedollasnake  Great question about darkness!. It's complicated to explain with eclipses. In Texas this is a big umbra because its a long totality. The umbra is 120 miles in diameter, so at the centerline you are in the center of a big shadow. This is important because during an eclipse a lot of the ambient light at your position is from the sunlight at the horizon, so with this eclipse the horizon is far away. At an eclipse the sky is darkest right around the eclipse and then gets lighter and lighter towards the perimeter of the umbra and for 360° around you. So it's not like sunrise or sunset where the residual sunlight is only coming from a single direction. So the sky is not behaving like sunset, so it's hard to describe it using "minutes after sunset" but if I were to do that, yes, I would say overall it;s about 20 to 30 minutes after sunset. They other thing is, during an eclipse you go from very bright conditions at C2 to immediately dark conditions (at C2) when totality begins. So it seems much darker right at the start of totality until your eyes start to dark adapt. So for this long eclipse, over 4 minutes, it will seem to lighten later in totality because your eyes have time to dark adapt. Another way to judge the darkness of totality is by how much ambient light you have to use your equipment: how well can you see in your immediate area? I good way to understand this is to go outside on the night of a full Moon when the Moon is high in the sky. Look around you, your hands, the ground, bring a camera out and look at the controls, the ambient light directly around you is about the ambient light you will have during an eclipse to see your equipment. But you have to factor in eye dark adaptation. As I said before it seems much darker at the start of totality. You should watch my other videos on eclipse lighting; Over Exposed Eclipse., Eclipse Lighting 1, Eclipse Lighting 2, The Purkinje Effect, Eclipse Horizon.
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  1576. Jason, I just found your channel via this video and I liked this video a lot. The thing that kills me about electric vehicles and folks who are "green" and believe they are helping save the planet is: where does the power come to build your electric vehicle and then to re-cycle that big nasty battery when it has reached its end of life? Everyone has a "bromance" with Elon Musk, but did he excavate the land and build all of his factories with "clean" electric trucks and construction equipment? Are his huge factories completely off the grid regarding the power needed to assemble a "clean" vehicle? Are all of his subcontracted parts suppliers off the grid too? Do all of his thousands of employees who drive to work use "clean" vehicles to get there? Is fossil fuel used to install and maintain charging stations around the country? Is fossil fuel used ti maintain the server farms and the computer and internet capability to download updates to the cars? Is fossil fuel use to charge the car in your garage at night? And my biggest issue, how much power is going to be needed to eventually recycle all of those nasty 1,000-pound batteries? So in the "big picture" how much fossil fuel is used to produce, use and eventually mothball an electric vehicle? That is what needs to be studied, understood and published. Electric vehicles are not a "renewable energy manufacturing chain" from start to finish; meaning factory building, to vehicle end of life is not all done with windmills and solar panels. So I suspect that folks buying electric vehicles to be "green" would be alarmed about how much fossil fuel is used for them to be "green'. Can you do a video tho answer this question? Thanks!
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  2068. John, from what you described it seems like you did see shadow bands. Great! They are very low contrast shadows and generally are wavy or look like fluttering shadows. Then the entire group of the shadows will have a group motion, in some direction, so the entire visual experience is complex. They can vary in appearance all along the path or observing position. Some positions may not see them at all. Since they are so low contrast it is best to spread out a white sheet in front of you, or look at the ground area in your observing area that is light colored, like light colored concrete. You can see the white sheets spread out in my other "Eclipse Horizon" video that is a spinning camera. I have shadow bands video from 3 different observing positions in Tennessee that I am analyzing. I am working with some of my NASA solar scientist friends to come up with better theories of how they are caused. When we have some conclusions I will be posting a detailed video about shadow bands, so stay tuned to my channel. Regarding the overall experience of enjoying a total solar eclipse, it is very difficult to actually teach someone how to take it all in. There are just too many experiences to absorb. So you do the best you can and that is why Solar Eclipse Timer was so helpful to people, at least it provided a little direction. I have heard from many people that said they would not have seen shadow bands at all if the timer did not remind them when to look for them. This new YouTube channel I am creating will be a great resource now. I am going to work hard to make this channel the place to go to to learn about enjoying a total solar eclipse. Especially as I prepare people for 2024.
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  2137. Tommy, it's a bit more complicated than that because remember I STRESS that my procedure works only if you are using a GLASS solar filter because I know how much light they transmit. From the exposure numbers you gave me, I am guessing that you are using AstroSolar Baader film. That passes about 2 1/3 stops more light than glass. That is why you need to have such a fast shutter speed for your partial phases. (Although, if you went to ISO 200 you could be use 1/500s which could be close to glass. Especially the new Seymour glass) . Remember the relationship I teach is from your full solar disk setting (exposure) you will know where you will be for exposing the corona when your solar filter is off. Don't confuse the two things (because your solar filter material is different). One thing is with GLASS, it lets you know where you are with the inner/mid corona, to then know where you need to be with ring and beads. The second thing is for you, to forget that in your case, and just count stops to match what you see in my book. I generally work at F10, ISO 200, and ~1/200 for the partial phases, and shoot the ring and beads at 1/1000s (2 1/3 stop less light enters for beads Chapter 14). So now you have to count stops to match me. So, for partial phases, your ISO 400 is one stop more light than me and your shutter speed at 1/1000s is 2 1/3 stops less light than me (when I am at 1/200). So, your system is already letting in 1 1/3 stops less light than me when set up for the partial phases. So your shutter speed has to be 1 stop less light in shutter speed than your 1/1000s (to match me). So, if you use 1/2000 we should be equivalent. (For beads I am f10, ISO 200, 1/1000; that should equal f10, ISO 400, 1/2000s). Also, note that a 1/3 stop difference is not a big deal. Start imaging at 30 seconds before C2. In the Appendix chapter Simplifying Solar Eclipse Photography toward the back, there is a section called Solar Filters That Are Not Glass: read that. Exposure can be counted up and down and matched between the three variables. Did you download my Master Stop Chart? It makes it easy to count stops. The link is on the front page of my website, download it.
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