Cool - the process I'm using is to get the density at a series of points above the plane....
I hope this makes sense...
I think so! I should be back in a few days, when I will ask for a location to start at ...
Cool - the process I'm using is to get the density at a series of points above the plane....
I hope this makes sense...
Readings from different parts of the galaxy would be very useful. So far the results seem to be consistent everywhere, but it would be nice to be sure!
Hmm... I think I see what you mean, Taen. It would be quite a broad-brush approach, so perhaps not suited to finding the overall density given the rapid rate of change of density as we move from the plane, but we could perhaps measure the density as it applies to mass code A systems (...) maybe up to mass code D.
(Also - as a general method of finding the density, I think that's an excellent idea and ought to have applications elsewhere - if we get the way the scale height changes narrowed down, we could work out some formulae to get the overall density of a sector just by looking at system counts on the plane!)
That would be interesting to see!One slight oddity I've noticed is Eol Prou is extremely lopsided. FG-Y G, and DL-Y G number in the thousands, whereas the others are in the low hundreds, some with under 100. (I very recently completed a data run to get a minimum of 10 complete system scans from all of the G's and a minimum of 3 of each of the F's. Also known as 320 million in post 2.3 dollars. Was gathering data to find patterns on the inter-relationships between the boxels.)
I've no special preference as to direction - if you're doing a series of surveys, perhaps head along one of the spiral arms?BaldEagle said:Any preference where I should head to Jackie?
The line I've got on the graph is a fit line I've been trying based on combining two scale heights (for the thin and thick disk) - the formula is upthread somewhere. But I think we will need to add a third component for the galactic bulge based on the set of results from nearer to Sadge.
(This) is my current spreadsheet of results. I got about half way through my second survey in HEGUA (using a simple version of the Taen method) but it was proving troublesome due to overlapping survey areas - I will try another with a modified approach. Promising, though.
I'm heading back to the Bubble to take care of some urgent business there now... can't make my mind up...
Incidentally, I'm not 100% confident about my boxel calculations. I haven't worked out how to accurately determine the... mass code modifier?... the number immediately to the right of the mass code. (eg. f1, f2, e6, d13, etc). I'm a little surprised that I can obtain the rest subsector codes without that, which makes me think that I've either made a mistake, or that I don't fully comprehend what that modifier does.
It's a counter - each time the first three letters go round a full cycle of the alphabet from AA-A to ZZ-Z, that number increments by one, which is why it generally increases as you go "north" in a sector.
The "yourboat" program here might be useful to you?
Readings from different parts of the galaxy would be very useful. So far the results seem to be consistent everywhere, but it would be nice to be sure!
I'm planning to reach Beagle's Point with a soon-to-depart expedition, fancy some readings along the way?
Right now I'm heading towards Colonia, I'm planning to navigate (ehm..."astrogate"?) on top of the galactic plane, but when I'll join the expedition I'll follow the route near the plane. Not sure to have understood the "Taen approach", since I've not yet grasped the cartographics system, but I can surely give some N and R data in respect to the distance from the plane.