Saturday, July 2, 2016

Using Polarized Sun Glasses as a Viking Sunstone

This note is an annotated, illustrated version of a Chapter 8 section of the book Emergency Navigation, called Finding the Sun as a Viking Would. This note comes to be written now because we had made a (cryptic) Youtube video on this topic some years ago for the students of our online course in emergency navigation, and frankly it was not very clear what was going on in the video without the background of the course or that book.  But the video gained some attention and several commenters ask for clarification, so this is an attempt to do that. It is frankly a pretty neat technique, so I can appreciate the frustration of not knowing what was going on in the video.  Something seemed to be working (according to the narrator, me), but it was not obvious what!

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Leif Karlsen, in his book Secrets of the Viking Navigators, gives a good argument that the Vikings used crystals of Iceland spar to find the direction of the sun when just below the horizon or when obscured by fogbanks on the horizon, common at latitude 60° N where they did much of their ocean sailing. The technique he proposes works very well. We have done it many times using these Viking sunstones, which are readily available from gem shops online (you need a clear crystal, 1 to 2 inches on a side). This technique can pinpoint the direction to the sun to within a few degrees, and it was in fact used for many years in a more sophisticated arrangement as the basis of the Kollsman Sky Compass in the early days of polar exploration by air.  Leif’s original instrument is still on display and the Nordic Heritage Museum, just around the corner from Starpath HQ. I had the pleasure of working with Leif on the project for many years. His study is the definitive work on the most likely way the device was actually used in Viking times, but we had to publish a special peer-reviewed article to confirm his right to this claim.

You can simulate the sunstone method with about the same precision using any polarized film, such as the lenses of  polarized sunglasses or some polarized camera filters. Some older sextant models also have polarized filters on the sunshades.

In addition to that, you need a small piece of cellophane. Many clear packaging tapes, the transparent windows of a CD sleeve, or the protective packaging of many products are often cellophane. On the other hand, some clear plastic products that look like cellophane, are actually another type of plastic and will not work for this application.

To prepare the lens, attach a piece of cellophane diagonally across the lens as shown in the left inset in the graphic below. Look through the lens with the cellophane on the far side (sky side) of the lens. The lines with the arrowheads in the figure represent the edge of the cellophane, crossing the middle of the lens.  

Figure 8-4 from Emergency Navigation. The bottom left inset shows a cellophane tape on the glasses; the bottom right inset shows the direction to look. The top part shows 3 examples of applying this technique.  The middle one is what you see when looking in the right direction. The three images of that group would be on top of each other when actually yawing the orientation to the right and left of the true sun direction.   The groups on either side of that show what it looks like if you are not quite looking in the right direction when you yaw the device to the right and left.  You still find the direction to the sun, but it is not as easy to locate that on the horizon.   Start by looking in the direction that is opposite to your best guess of the sun’s bearing. You will not know exactly where to look, as that is what you are trying to discover. Once facing that best-guess direction away from the sun, angle your view up from the horizon by an amount that you estimate would put you about 90° from the line straight to the sun. Referring to the right inset, if you point to where you think the sun is, your thumb will point in the best direction to start looking for maximum polarization. If the sun is just on or below the horizon, you would look straight up. If the sun is about 30° above the horizon, you would look in the opposite direction at about 60° above the horizon.

In the video example, we used inexpensive polarized sunglasses that had no frame at all (Bartells in Ballard), it was just one piece of plastic formed into glasses. The we just cut them in half.  I think we used the clear packing tape we get from U-line, and taped a strip across the glass diagonally as shown.

Then you want to hold this up and look at the sky through the glasses and tape (tape on the opposite side you are looking at), but you do not look in the direction you think the sun is—even without seeing it (already set or obscured) you know very roughly the direction to the sun. Rather, you want to hold this up in the direction that is 90º from that direction. In other words, it the sun had just set (roughly the case in the video), then you would be holding this up, looking directly overhead. For cases when the sun is overcast or behind clouds but not near the horizon, then you would look in a direction opposite to the sun at an angle from the sun as illustrated in the picture.

An important requirement is that this direction you are looking, i.e. 90º from the estimated sun direction, has to have some clear sky. If you look 90º from the sun and it too is covered by clouds, this will not work.  Thee can be some level of overcast, but there must be some level of clear sky in that direction.  The closer you are to looking at 90º to the actual sun, and the clearer the sky is in that direction, the better it will work.


The three center group of drawings in the picture above show what you will see when you are facing the proper direction of maximum polarization, directly opposite the true bearing to the sun. When the cellophane edge is perpendicular to the horizon, the lens will be the same shade on both sides (cellophane side and no-cellophane side). When you rotate it slightly to the right and left (that is a yawing motion), the sides will change brightness, as shown in the two figures adjacent to the center one.  There are three groups of pictures here, we are talking now about the middle group, which is what you see when you are looking in the proper direction.

The two rotated views are shown to the right and left (in the center group), but they would actually be in the same position as the middle one, just rotated to the right or to the left. The video will illustrate what we actually see.

On the other hand, if you are not facing opposite the true direction to the sun, you will see what is shown on the right or left of the center figures. If you are facing to the right, the edge of the cellophane will lean right when the sides have the same brightness, as shown, and when facing to the left of the proper direction, you will see what is shown on the left.

In short you can find the direction to the sun even when pointed slightly wrong, but you will not get a good vertical line as shown in the middle group, which takes more judgement on locating the bearing on the horizon.

This is a subtle process that takes some practice… and patience. But once the procedure is grasped, it can then be repeated much more readily. The sequence is: Look in the approximate right direction and then in the approximate right elevation. Then, starting with the cellophane edge perpendicular to horizon, rotate the lens to find the orientation of that edge line when the two sides are about the same brightness. When you are in about the right direction, the two sides will switch in brightness quite prominently—providing you do indeed have a polarized filter and true.

I have always found when using the sunstone or these glasses in a hand held mode—as opposed to the device Leif invented for using a mirror—that it is easier and more accurate to hold a ruler along side the crystal or in this case the polarized glasses. The ruler enhances your perception of the yawing motion for better precision.  Also in the video I also used a mirror.  I just held the ruler and glasses up in one hand overhead and looked at it with a mirror in my lap. These modifications are (very crudely) sketched in the pictures below. (I will improve these when we can.) Also shown below is an illustration of the right direction to look.




You can try both methods to see what works best for you. Just looking up works fine and is likely best. We used the mirror just so someone could make the video.


Here is the video showing an actual measurement.  The screen caps preceding it below show what is meant by "right" and "wrong" heard in the video. 

Here is the explanation that is printed in the video description:

This is just after sunset, with a bright patch on the horizon to locate sun direction as a test. It is using a mirror facing straight up to view the glasses that have a piece of cellophane tape pasted diagonally across the glass. This can be done without the mirror by looking straight up to the taped glasses, but i could not take a video of it that way. The video was taken with an iPhone.

This is a modern version of using polarized film (cheap clip-on sunglasses, cut in half) as a Viking sun stone (Icelandic Spar). It is a way to find the direction to the sun after it has set or when it might be behind a cloud bank. Maximum polarization is in a direction 90º from the sun direction, which is straight up with the sun near the horizon.

I am holding a meter stick along the edge of the cellophane tape to enhance the rotation angle, which helps pinpoint the direction.
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When you watch the video, I am rotating the ruler and glasses to the right and left and noting which side is dark or light, and when the two sides are the same brightness, the the edge of the cellophane and in this case ruler are pointing to the sun... which was set below the horizon for some period of time as i was doing this.  I was using a mirror in this case only so i could make the video, which would he hard to to looking up. In this case a friend was taking the video over my shoulder looking down at the mirror. Doing this on your own there is no need for a mirror. It just gets in the way.  By the way, the obvious way to practice is do it (without a mirror as you can then see where you are pointed, and do it just at or after sunset so you know indeed what is the right answer.


Too far right. One side is darker than the other.

  
Just right, both sides same color. The Ruler is pointed to the sun, even though the sun is not viable at the moment. It could be set (as in this case) or obscured behind a fogbank or clouds.


Too far Left. One side is darker than the other.
 ----------------------------------------------- Here is the video -----------------------------------------------






A couple details  (my guess is, no one wants more details at this point!)
This technique works because scattered sunlight is polarized. If you imagine a line straight up to your zenith and another line straight toward the sun, then these two lines define a plane. The electromagnetic oscillations within sunlight that have been scattered by air molecules are perpendicular to that plane, whereas in direct sunlight these oscillations are randomly distributed in all directions. Sunlight that has been reflected from a surface (glare from the water, for example) is also polarized, which is the motivation for polarized sunglasses. This light is horizontally polarized parallel to the reflecting surface, which means that sunglasses designed to block this glare are vertically polarized. An easy way to test that a pair of glasses is polarized is simply to look at such a reflective glare and rotate the glasses (looking straight through the lenses to the glare, roll the lenses, without pitch or yaw), and you should see the intensity of the glare change quite noticeably. On land you can do the same with bright glare from a window or car hood or bumper. When the glasses are working properly, you can see though the glare-producing windshield into the car; without them, or with your head turned 90°, you see only glare.






If you are using a lens of a pair of sunglasses, chances are the polarization axis is parallel to the bottom of the glasses, which means you will find the brightest or darkest light transmission with the lens parallel or perpendicular to the horizon. If  this is not the case, find the best orientation and draw a line across the bottom of the lens when rotated into the darkest or brightest orientation—or mark the horizon with a piece of tape if you don’t have the right pen for the job.

When you attach the cellophane it should go diagonally across that axis.  Once you have this "polarization compass" assembled, look again to the correct direction and rotate the device. You will notice now that the right and left sides alternate in brightness; when the two sides have the same level of brightness, the edge of the cellophane is pointing to the sun. The trick is to hunt around for the best direction; rotate the compass, note the sharpness, turn left a bit, try again, turn right and try again. When the angle is optimum, look up a bit and then down, etc.

As shown in Figure 8-4, you are finding a great-circle arc that points to the sun, so when looking to the left of the proper vertical plane, the line will point right, and when looking to the right of it, the line will point left.

Once you find it with access to clear sky at 90º, the location of the brightness transition becomes very sharp. In short, this really works well.

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Final note.
After coming back to this video because of the several notifications we were getting here, I looked around at other videos online about the use of the sunstone itself.  There are quite a few. They vary from almost right, to totally bizarre.  I will try to get help and make a quick video of how to use an actual sunstone for this purpose.  It is easier than this.



Vic-Maui Race Day 1, 2, (3) Winds

The Vic-Maui race in 2016 has 4 starts, each at 930 am on July 9 to 12.  This note is about available wind data during the first few days of the race.  This would also, of course, apply to anyone sailing out the Strait, headed to Hawaii on any date.

We have gained fresh experience recently with regional wind models while working on the R2AK planning and analysis for our fast friends on MAD Dog. The best wind data available for the start are commercial products, and as such are only legal up to the starting gun. These winds are the main topic at hand, but once underway we must rely on free pubic data, which would include:

GFS (28 km),  available all the way to HI, but not too valuable till out in the ocean.

NAM (12 km), available from the Continental US run (CONUS) that goes about half way across and then again in HI region, but the NDFD would likely be better for that.


NAM CONUS coverage


NDFD (3 km). This is almost by definition the best free, public data, but it only goes out to Lon 133º W, and then is available again in HI, as shown below. It can be useful in the Strait as well. See The National Digital Forecast Database.  This is not strictly "model forecast," as any one of several models might have dominated its production on any given run, but rather it is the digitized forecast of the NWS using whatever model or input they chose to use.

NDFD HI coverage

All three of the above are available from saildocs underway.

For the start the free hi res data are the NDFD (above), but the best data is likely to be one of these:

HRRR (3 km).  This (High Resolution Rapid Refresh) model is updated hourly,  but only extends out 15 hours, and to get all 15h you must download 5 files. It is available from the Ocens WeatherNet app. Ocens offers short term accounts for this access as well as a 3-day free demo.  I am proud to have taken part in convincing our friends at Ocens to offer the grib format of this important data.  In the R2AK planning, there were several cases where this was hands down the best forecast. For leg one, it remained correct, despite all other models being wrong, as well as the NWS and CND text and VHF forecasts being wrong.

HRRR data. 15h of forecasts in 5 files. Goes north to Cambel River... ie perfect for the R2AK run to Seymour Narrows.

With that said, that is not the only data we used and benefited from.  We also used the

PredictWind PWC/G (1 km, 8 km). The smaller regions in the Strait are 1 km; the coastal regions are 8 km. See Predictwind.com


This product has several advantages. First it is super easy to access in Expedition or by email, and the 1 km hi-res models extend out 36 hours,  compared to 15h with HRRR.  They also have a convenient (Mac or PC) app called Predictwind Offshore that lets you either request and look at the data online, or what is often more convenient, it will prepare a template request that you just email to them when you need an update. The larger regions of 8 km are 390 kb each, the smaller regions of 1 km data are 250 kb each.  The 8 km (also hi res) goes out a 7 days—like the lower res GFS, more or less into the realm of the unknown. The navigator is of course going to say that in the ideal world you have both the hi res from PredictWind, and the HRRR from Ocens.  Maybe someday saildocs will offer the HRRR.

Predict Wind also has a weather routing/optimizing feature that seems to work pretty well. You can also use custom polars for the analysis.  For inland waters, however, it does not account for currents, which leaves Expedition at an advantage for that— but I should add here, if you do not have good current data, then you could be better off without using currents at all!  PW does offer and use ocean currents for the ocean routing.


UW WRF (1.3 km).  Unique to our local waters, we should always remember the UW WRF model, which is likely as good as any, but only available as a graphic format;  there is no grib format. The  model is run every 6h and data would typically be 8+ hr old when we get it, and indeed they might not be there when you want them. This is a public service of the UW Atmospheric Sciences Dept.,  with no guarantees.

UW WRF model, run every 6h extends out 60h.

 In fact, this model could be the best model for the region, but it is not updated often enough to compete with the HRRR, which is updated with all the latest actual wind observations every hour.  The HRRR model actually has wind forecasts every 15 minutes, but Ocens has not included that option.

Nevertheless, it is worth printing out the UW data before the start, and with a good connection offshore, perfectly legal underway.  You can figure out how to request the image forecast underway using saildocs—to be added in a future post.

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Looking ahead, two articles on the horizon are (1)  the use of a plugin for OpenCPN that *very neatly* lets you load weather maps into your navigation program. We have  been struggling on ways to do this, and simply did not know about that option.  Expedition can do this nicely. And (2) also still working with OpenCPN, which we use in our classes, there is another plug in for OpenCPN that does weather routing!  I have no idea how this works yet; we need to study that and report on it.


Monday, June 13, 2016

Can exceptional behavior be considered ordinary?

The answer is Yes, according to Justice Wilmer in the 1955 case of Velox vs Viking Monarch, wherein one anchored vessel dragged anchor and collided with another when both were sheltering from a severe storm, when there were maneuvers and procedures that might have avoided it if taken.

The nicely put conclusion was:


"I have been reminded, and quite properly reminded, that no seaman can be called upon to exercise more than ordinary care (see Rule 2a below); but I think it is necessary to observe that when a seaman is called upon to face wholly exceptional conditions, ordinary care of itself necessarily demands that exceptional precautions may have to be taken."
In other words, it is the ordinary practice of seaman to take exceptional precautions in exceptional conditions, just as it is to take normal precautions in normal conditions.

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RULE 2 Responsibility

(a) Nothing in these Rules shall exonerate any vessel, or the owner, master or crew thereof, from the consequences of any neglect to comply with these Rules or of the neglect of any precaution which may be required by the ordinary practice of seamen, or by the special circumstances of the case.


(b) In construing and complying with these Rules due regard shall be had to all dangers of navigation and collision and to any special circumstances, including the limitations of the vessels involved, which may make a departure from these Rules necessary to avoid immediate danger.


See also our very convenient (free) presentation of the Nav Rules and all related  documents we call Pocket Nav Rules Handbook.

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I recall a case when a hurricane passed over a fleet of anchored sailboats and the ones that survived spent all night at the helm with the engine on and in gear taking the strain off the anchor line—and periodically fending off those boats that failed to do so.  I think we also have some pictures of this, which I will look for. It was a student of ours.


Friday, June 3, 2016

Inside Passage and R2AK Weather

Here is a peek at an old page we had for our onboard training trips to Petersburg. We ran across it today by accident and realized this could be valuable to those doing the R2AK at the end of the month, or anyone headed north this summer.  So we checked and updated the links and added a couple new ones. You can see the page more clearly at the link below. This view is just to show what is there.  To view the links here you have to right click and choose back to return.