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Working on a mass model

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2:09 am
July 21, 2010


Luke Maurits

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rpulkrabek said:

Another question; have we determined the Isp? If so, how?


 

The highest Isp you can achieve with PE and N2O is 247.0s, and this occurs with an O:F of 8:1.  I've found this same figure in multiple sources (including one textbook and at least one paper in which they determined it experimentally), so I trust it.

Main CLLARE workgroups: Mission Planning, Navigation and Guidance. I do maths, physics, C, Python and Java.

2:21 am
July 21, 2010


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rpulkrabek said:

I've completed the rest of the mass calculations. You can find all of the data from this OpenOffice spreadsheet. I tried to clean it up a bit and make it easier to read, also.

The next steps are to determine the correct values to use in OHKLA. How is the needed mass of the propellant determined? Once this is known, I understand how we then determine chamber and tank dimensions. I just don't see how propellant mass is determined. Does it come from USOFS? 


 

The Tsiolkovsky rocket equation relates dry rocket mass, wet rocket mass, specific impulse and delta-v (under ideal conditions).  If you give it any three of these, it will give you the fourth.  We know the Isp (see above).  We know the required delta-v – USOFS suggested an impulsive delta-v of 1500 m/s will result in an apogee of 100 km, and a Wikipedia article (though I now forget which one) gave precisely the same figure for suborbital flight.  Thanks to your work, we now know how to figure out dry mass as a function of propellant mass.

So, suppose we use x kg of propellant.  Using your mass models (plus some estimates for various things like the length of the recovery section, etc), we can figure out the dry mass of a rocket large enough to contain that x kg of propellant.  The wet mass is just the dry mass plus x kg, and the Isp is known.  So we can plug all of this into the Tsiolkovsky rocket equation and get out the resulting delta-v.  If it's higher than what we need, we make x a little bit smaller, and if it's lower than what we need, we make x a little bit bigger.  Rinse and repeat until we've zeroed in on a propellant mass which gives us the delta-v we want to whatever level of accuracy we desire.  This is exactly the process I used to get my mass estimate from last night.

My thought is that we should probably aim for a delta-v of 1600 m/s rather than 1500 m/s, just to be on the safe side, since USOFS is not exactly perfect.

Once we have decided on a quantity of propellant, we will know the rocket dimensions and so we can begin to model the thing in OpenRocket to get an independent confirmation that we're on the right track.  Of course, we don't have a thrust curve for our rocket, but we can "make up" some realistic ones since we know the Isp and the total propellant mass.  E.g. if we specify that the thrust is linearly decreasing over time and specify the total burn duration, then the thrust curve is uniquely specified.  I figure we can just do this for various thrust times in increments of 5s and see just how long a burn (or low a thrust) we can handle before we stop breaking the Karman line.  Unless the results of this tell us we need a really short burn time, we should be okay.

Main CLLARE workgroups: Mission Planning, Navigation and Guidance. I do maths, physics, C, Python and Java.

3:04 am
July 21, 2010


Luke Maurits

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Just realised I glossed over choosing the diameter.  Basically, the propellant mass required will vary with diameter, since the volume to surface area ratio of tanks and chambers will vary depending on whether they're tall and thin or short and wide.  At the same time, the rocket's fineness ratio (length to diameter) will vary.  We basically want to compromise between minimum propellant mass and a "good" fineness ratio.  Fineness ratio is not super important, but we may as well consider it.  Higher is basically better here, until you get beyond a certain point.  I have done a small survey of suborbital sounding rockets and seen fineness ratios as high as 30, but in general there seems to be two common "clusters" of ratios, one around about 7-8 and then another 15 on average.

Main CLLARE workgroups: Mission Planning, Navigation and Guidance. I do maths, physics, C, Python and Java.

4:16 am
July 21, 2010


rpulkrabek

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Post edited 4:50 am – July 21, 2010 by rpulkrabek


Luke Maurits said:

The highest Isp you can achieve with PE and N2O is 247.0s, and this occurs with an O:F of 8:1.  I've found this same figure in multiple sources (including one textbook and at least one paper in which they determined it experimentally), so I trust it.


 

Ok, maybe this is a good number to use a starting point for our calculations. Is there any way we can calculate it, or is this something that is better to measure experimentally.

Will we measure Isp from the scaled rockets we test and then use these values for the full scale OHKLA rocket?

If Isp=v_e/g, where v_e is the exhaust velocity, I think we can obtain this via a CFD analysis. Perhaps it's good to trust the number provided, but I would prefer to also validate it.

4:29 am
July 21, 2010


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Post edited 4:31 am – July 21, 2010 by rpulkrabek


Luke Maurits said:

The Tsiolkovsky rocket equation relates dry rocket mass, wet rocket mass, specific impulse and delta-v (under ideal conditions).  If you give it any three of these, it will give you the fourth.  We know the Isp (see above).  We know the required delta-v – USOFS suggested an impulsive delta-v of 1500 m/s will result in an apogee of 100 km, and a Wikipedia article (though I now forget which one) gave precisely the same figure for suborbital flight.  Thanks to your work, we now know how to figure out dry mass as a function of propellant mass.

So, suppose we use x kg of propellant.  Using your mass models (plus some estimates for various things like the length of the recovery section, etc), we can figure out the dry mass of a rocket large enough to contain that x kg of propellant.  The wet mass is just the dry mass plus x kg, and the Isp is known.  So we can plug all of this into the Tsiolkovsky rocket equation and get out the resulting delta-v.  If it's higher than what we need, we make x a little bit smaller, and if it's lower than what we need, we make x a little bit bigger.  Rinse and repeat until we've zeroed in on a propellant mass which gives us the delta-v we want to whatever level of accuracy we desire.  This is exactly the process I used to get my mass estimate from last night.


 

From the Tsiolkovsky rocket equation, I get that delta_v=Isp*g*ln((m_dryrocket+m_propellant)/m_dryrocket).

delta_v=1600

Isp=247

g=9.81

-> 1600=247*9.81*ln((m_dryrocket+m_propellant)/m_dryrocket)

As you said, we now have an equation to figure out m_dryrocket as a function of m_propellant; 2 equations, 2 variables.

Can't we solve this set of equations instead of using an iterative process?

4:49 am
July 21, 2010


Luke Maurits

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rpulkrabek said:

 

Ok, maybe this is a good number to use a starting point for our calculations. Is there any way we can calculate it, or is this something that is better to measure experimentally.

Will we measure Isp from the scaled rockets we test and then use these values for the full scale OHKLA rocket?

If Isp=v_e/g, where v_e is the exhaust velocity, I think we can obtain this via a CFD analysis. Perhaps it's good to trust the number provided, but I would prefer to also validate it.


 

Could we really get it out of a CFD analysis?  The exit velocity isn't simply determined by the engine geometry and the tank pressure, otherwise all propellants would have the same Isp.  It depends on how much energy is released by the combustion reaction, and on the masses of the molecules which are the products of that reaction.  In the case of a complex polymer like PE, I think there are in fact many different combustion reactions going on because the solid PE pyrolises into all kinds of gaseous and liquid compounds.  We would need to know the chemistry of all these reactions and also the relative proportions of those reactions going on in the combustion chamber.  I'm not saying it cannot be done, but I don't think it will be easy.

Main CLLARE workgroups: Mission Planning, Navigation and Guidance. I do maths, physics, C, Python and Java.

4:56 am
July 21, 2010


Luke Maurits

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rpulkrabek said:

As you said, we now have an equation to figure out m_dryrocket as a function of m_propellant; 2 equations, 2 variables.

Can't we solve this set of equations instead of using an iterative process?


 

We could, indeed.

Main CLLARE workgroups: Mission Planning, Navigation and Guidance. I do maths, physics, C, Python and Java.

5:12 am
July 21, 2010


rpulkrabek

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Luke Maurits said:

Could we really get it out of a CFD analysis?  The exit velocity isn't simply determined by the engine geometry and the tank pressure, otherwise all propellants would have the same Isp.  It depends on how much energy is released by the combustion reaction, and on the masses of the molecules which are the products of that reaction.  In the case of a complex polymer like PE, I think there are in fact many different combustion reactions going on because the solid PE pyrolises into all kinds of gaseous and liquid compounds.  We would need to know the chemistry of all these reactions and also the relative proportions of those reactions going on in the combustion chamber.  I'm not saying it cannot be done, but I don't think it will be easy.


 

Hmm, ok, that is a quite complex process. We could simply do the analysis with N20, but then it's not reliable, due to not having PE involved. We could determine a sort of hybrid material, where we would create our own material with the average combined properties (an average of the combusted materials) and plug those numbers in for the analysis. I haven't ever tried this before, and I'm not sure how it would work.

Perhaps it's best to take measured data from scaled rockets, and possibly compare those to scaled CFD results, to determine how reliable it could be. 

6:39 am
July 21, 2010


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Post edited 6:41 am – July 21, 2010 by rpulkrabek


 

I quickly made a plot comparing propellant mass to the chamber and tank mass for the three varying inside diameters we used. This isn't fully appropriate, since with the design we are planning on using, we can use different inside diameters for the chamber and tanks, for example, the ID of the chamber can be 20cm while the ID of the Tank can be 30cm. But still, I wanted to see what the relationship looked like.
Mass Plot 2010 7 21mouse
From what I can tell, it seems that the smaller the inside diameters, the smaller the total mass will be. It seems the relationship is not linear, though, as the 20cm and 10cm seem to be coming towards some sort of limit. It's difficult to tell, with only 3 sets of points. I'll see if I can come up with anything better still.

 

7:23 am
July 21, 2010


Luke Maurits

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Post edited 7:32 am – July 21, 2010 by Luke Maurits


Okay, I have now done a complete and proper version of the propellant investigation.

I did length and mass regressions for the 10, 20 and 30 cm chambers and tanks, and interpolate between these models to get estimates for arbitrary diameters – e.g., a 27.5 cm diameter chamber is modelled as having a dry mass which is 0.25 times the mass of a 20 cm diameter chamber plus 0.75 times the mass of a 30 cm chamber.  This is not perfectly accurate, of course, but it should be good enough for rough estimation purposes.  In addition to this, I also did a regression of the combustion chamber flange diameter against the combustion chamber diameter.  Then, when considering rockets, I would set the combustion chamber diameter, estimate the flange diameter using the regression, and then set the tank diameter to equal the flange diameter, so everything fits together just like it would in the actual rocket (modulo some wall thicknesses, but that's quite a small error).  I set the nosecone to be 5 times as long as it is in diameter.  The results are as follows:

+-----------------------+--------------------+-------------------+----------------+---------------+-----------------+
| Chamber diameter (cm) | Tank diameter (cm) | Rocket length (m) | Fineness ratio | Dry mass (kg) | Propellant (kg) |
+-----------------------+--------------------+-------------------+----------------+---------------+-----------------+
|           10          |      13.90333      |     13.156959     | 94.6317105327  | 103.019438461 |       96.5      |
|           11          |      14.94033      |    12.460042385   | 83.3987092989  | 103.182064337 |       96.7      |
|           12          |      15.97733      |    11.71429244    | 73.3182104895  | 102.862703985 |       96.4      |
|           13          |      17.01433      |    10.940101105   | 64.2993353544  | 102.118250364 |       95.7      |
|           14          |      18.05133      |    10.14712772    | 56.2126320886  | 100.970946884 |       94.6      |
|           15          |      19.08833      |     9.3517395     | 48.9919207181  | 99.4850038118 |       93.2      |
|           16          |      20.12533      |     8.58479267    | 42.6566554188  | 98.0448186538 |       91.9      |
|           17          |      21.16233      |    7.935636125    | 37.4988771321  |  98.721486819 |       92.5      |
|           18          |      22.19933      |     7.2725272     | 32.7601202379  | 99.2811430166 |       93.0      |
|           19          |      23.23633      |    6.601368825    | 28.4096878681  | 99.7554289662 |       93.5      |
|           20          |      24.27333      |     5.9167947     | 24.3757024685  | 100.084416952 |       93.8      |
|           21          |      25.31033      |    5.877518044    | 23.2218151403  | 101.825969364 |       95.4      |
|           22          |      26.34733      |     5.83347134    | 22.1406546318  | 103.496161153 |       97.0      |
|           23          |      27.38433      |    5.780182672    | 21.1076286037  |  105.03827619 |       98.4      |
|           24          |      28.42133      |    5.722720212    | 20.1353005366  | 106.507282134 |       99.8      |
|           25          |      29.45833      |     5.65914613    | 19.2106821059  | 107.875624438 |      101.1      |
+-----------------------+--------------------+-------------------+----------------+---------------+-----------------+

As you can see, required propellant mass is minimised at 91.9 kg with a chamber diameter of 16 cm and a tank diameter of 20 cm. However, this results in a very long rocket, 8.5 m long, with a fineness ratio of 42.  This is really rather impractical.  The difference in propellant between the best and worst cases is only about 10 kg, so we probably shouldn't worry about it too much.  Contrary to my expectations, it looks like the fineness ratio is going to be the main driver in sizing the rocket.  I think we should not consider any chamber diameters less than 20 cm, which corresponds to keeping the total rocket length under 6 m, which seems reasonable.  With a 20 cm chamber, we get a fineness ratio of 24, which matches the Atea 2 hybrid suborbital  rocket at Rocket Labs in NZ.  This is also roughly the same ratio as the Lambda LS-A, a Japanese solid suborbital rocket which has a fineness ratio of 21.  If we go all the way out to a 25 cm chamber (any larger and the flange diameter exceeds 30 cm, which means we can't accurately model the tank), we have a fineness ratio of 19.  I haven't seen that exact ratio before, but I've found several rockets with fineness ratios of 17, which is close.  So basically, anywhere within this range, the overall shape of the rocket is going to be quite close to other successful suborbital rockets, so we don't have to worry about much in that regard.

All of the above, of course, is based on rough estimates for the masses of everything (I'll fill out the table in an early post shortly to show the values I used for these calculations), so it's not exact – but it should be a pretty good ballpark.

So we now can say with some good confidence: we're looking at a rocket that's about 25-30 cm in outer diameter, 5-6 m long, with a dry mass of 100-110 kg and a propellant requirement of 90-100 kg.  Obviously we should do work to refine these ranges, but these are definitely the kind of ranges we're going to end up working in, unless some of our assumptions turn out to be very wrong.  It feels good to have this clear an idea of how things are going to look.  I'm really amazed at how close the dimensions are to the very first OHKLA design which was basically pulled out of our collective asses without any real engineering work!  We lucked out there.

One thing we should consider as we choose final dimensions is that we have to be able to actually find metal in the appropriate sizes.  Just because 26 cm turns out to be a great chamber diameter for us (to pick a number at random) doesn't mean that there are lots of people manufacturing and selling 26 cm diameter aluminium tubing with the wall thickness we want  – but it might be that 25 cm or 27 cm is the diameter of a very commonly used standard kind of tubing and so we have to settle for that because it will making finding materials easy.  In particular, if we're going to buy and build this rocket in the US, we might want to choose dimensions which are round numbers of inches to make this easier.  It's worth noting that 8 inches is 20.32 cm, so that metric and imperial almost overlap at that point, in terms of "nicenes".  Ideally, we want the design to be such that it's very easy for people all over the world to find materials in the appropriate dimensions.

EDIT: forgot to mention, the above data is also based on the assumption that the aerostructure is 2mm thick 6061 Al 6T.  I don't really know if that's appropriate – if we can make the walls thinner or need to make them thicker, propellant masses will go down or up, respectively.

Main CLLARE workgroups: Mission Planning, Navigation and Guidance. I do maths, physics, C, Python and Java.

12:04 am
July 23, 2010


Luke Maurits

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I have modelled the largest of the rockets in the table above – I rounded the tank diameter up to 30 cm and the propellant mass down to 100 kg to make things nice – in OpenRocket.  I put 6061 Al T6 into OR's materials database so it would accurately compute the mass of, e.g. fins and the aerostructure.  I also modelled the nosecone as being hollow fibreglass, since that is clearly how PSAS do things, so that makes the rocket a little lighter than the figures above.

The first thing I wanted to note in passing is that stability for this rocket isn't fantastic.  It is stable, but not by much – the centre of gravity is infront of the centre of pressure by 0.67 calibres (rocket diameters).  It's table as long as that number is above zero, but the higher the better.  For instance, PSAS set a stability margin of 3 calibres as a design requirement for their latest rocket.  I am not sure about the extent to which having canted fins makes this less of an issue – I definitely had to cant the fins 1 degree in OR for this thing to fly properly at all.  Without canting, and this low margin of stability, the 2m/s average windspeed that is OR's default setting was enough to tip the rocket over and send it into totally uncontrolled flight, which is bad.  With canting, though, this doesn't happen at all, so perhaps we're okay.  Anyway, I'm not sure how we could go about fixing this – to move the CM forward we'd need to either make the back of the rocket (with the engine) lighter, or the front of the rocket heavier (though that, of course, has drawbacks).  I'm not sure if we can move the CP back much, but will look into it.

Anyway, I'm not sure what to make of the OR simulations yet.  As it stands, no matter how quickly we dump the propellant (i.e. no matter how high the thrust), the apogee is only somewhere between 50 and 60 km, which is not really close to what we want.  If I turn the atmosphere off so there is no drag and make the burn time really really short to minimise gravity loss, then the maximum velocity is just under 1600 m/s, so our use of the Tsiolkovsky rocket equation is totally okay (as an aside, the apogee with no atmosphere is about 125 km).  We do have enough propellant to impart that sort of delta v.  So, at first appearance, the issue is that this isn't enough of a delta-v to get us suborbital, once we taken drag into account.

Now, if we'd just got the 1600 m/s figure from USOFS, I'd totally buy that, because USOFS is very rough.  However, the Wikipedia article on suborbital flight says "If one's goal is simply to "reach space", for example in competing for the Ansari X Prize,
horizontal motion is not needed. In this case the lowest required
delta-v is about 1.4 km/s, for a sub-orbital flight with a maximum
speed of about 1 km/s", which is even lower than the 1500 m/s figure we got from USOFS.  So 1600 m/s should definitely be enough to get past the Karman line.

Therefore, at this point, I'm starting to suspect that the problem is with the way OR calculates supersonic drag.  This is, of course, a known program: the program itself displays a warning once your rocket breaks Mach 1 that the body drag claculations may not be entirely correct, and Sampo himself has said that the supersonic drag modelling would need to be improved before OR was suitable for simulating something like OHKLA.  I need to do more reading, but I think perhaps OR is significantly overestimating drag, and this is why we're getting such a low apogee.  To test this I got it to plot the rocket's drag coefficient for the duration of a flight, and here is the result:

Openrocket ohkla simmouseThe drag coefficient is the yellow line, and as you can see, it's behaving quite oddly.  The initial peak shape around the 10s mark is, I think, normal.  Everything I've read about drag has suggested that as you approach Mach 1, drag starts to increase, peaking around Mach 1.2 or thereabouts and then slowly decreasing back down to subsonic levels past maybe Mach 2.  Those numbers could be quite wrong, but the qualitative behaviour I am sure is right.  However, notice that after engine burnout, the drag coefficient beings to climb, getting far higher than it was during the peak of the transonic drag.  It climbs for almost the entirety of the pre-apogee flight before steadying out at 1.45.  I could be wrong, but that behaviour doesn't feel right to me.  If the drag coefficient stayed down lower, around the subsonic levels, for most of the flight, it could buy us a lot of extra apogee altitude.

I'm going to do some more reading on how OR handles supersonic drag and perhaps also talk to Sampo about this.  I may also even play around with USOFS again, using OR's estimate of our rocket's subsonic drag coefficient to get better estimates out of it.  Although this may seem like a setback, I'm somewhat confident that this design is, in fact, good.  The work in OR with no atmosphere proves we have the right mass of propellant for a delta-v of about 1600 m/s, and that should definitely be enough. 

Main CLLARE workgroups: Mission Planning, Navigation and Guidance. I do maths, physics, C, Python and Java.

3:05 am
July 23, 2010


Luke Maurits

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Bad news. :(  While I still think something fishy is going on with the drag coefficients in OR, that doesn't actually explain the low altitude I was seeing.  It turns out that by the time that coefficient gets crazily high, the air density is low enough that there is minimal drag.  OR lets you plot the actual drag force in Newtons and I can see very clearly that there's no significant drag for most of the free-fall part of the flight.

The problem is the delta-v.

I found this really good article on suborbital delta-v requirements and all the different considerations which need to be taken into account.  Anyway, long story short, the 1.4 km/s figure on Wikipedia is actually ignoring all drag.  The fact that USOFS gave us almost the same figure when it was trying to take drag into account is obviously just due to USOFS being really, really poor.  Once you take drag and other losses into account, that article I linked to suggests a delta-v of 2,100 to 2,400 m/s to reach 100 km.

I reran the propellant mass calculations for a delta-v of 2400 m/s and that requires about 175 kg of propellant – an awful lot more than before!  The rocket is now 7.8 m long, for a fineness ratio of about 22.  I put an engine with this much propellant into OR (using a 30 second burn time with a constant thrust of 7000 N (really fairly small)) and now I'm getting an apogee of 113 km.  So it seems that we really do need a lot more propellant. :(  Perhaps not 175 kg, since that's getting us 13 km higher than required (although maybe we should shoot for 110 km, giving OR a 10% margin of error), but definitely a lot more than 90-100 kg.

The one positive of all this is that the longer rocket has much better stability margins, with 3.2 calibres of separation between the CG and CP.

As an alternative to adding propellant, we could drastically lower the dry mass somehow.  Replacing the aerostructure with fibreglass or carbon fibure could be one way to do this, although it would make construction a lot more problematic and perhaps more expensive to the point of cancelling out the cost of more propellant.  Another alternative would be to take advantage of the fact that hybrid engines can be throttled – rather than just opening the N2O valve up at launch and leaving it like that, we could throttle back somewhat during the thickest part of the atmosphere and then open it up again once we were higher up.  This would reduce drag losses somewhat.  It does complicate our valve-control and avionics requirements, though.

Main CLLARE workgroups: Mission Planning, Navigation and Guidance. I do maths, physics, C, Python and Java.

4:08 am
July 23, 2010


rpulkrabek

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Luke Maurits said:

+———————–+——————–+——————-+—————-+—————+—————–+

| Chamber diameter (cm) | Tank diameter (cm) | Rocket length (m) | Fineness ratio | Dry mass (kg) | Propellant (kg) |
+-----------------------+--------------------+-------------------+----------------+---------------+-----------------+
|           10          |      13.90333      |     13.156959     | 94.6317105327  | 103.019438461 |       96.5      |
|           11          |      14.94033      |    12.460042385   | 83.3987092989  | 103.182064337 |       96.7      |
|           12          |      15.97733      |    11.71429244    | 73.3182104895  | 102.862703985 |       96.4      |
|           13          |      17.01433      |    10.940101105   | 64.2993353544  | 102.118250364 |       95.7      |
|           14          |      18.05133      |    10.14712772    | 56.2126320886  | 100.970946884 |       94.6      |
|           15          |      19.08833      |     9.3517395     | 48.9919207181  | 99.4850038118 |       93.2      |
|           16          |      20.12533      |     8.58479267    | 42.6566554188  | 98.0448186538 |       91.9      |
|           17          |      21.16233      |    7.935636125    | 37.4988771321  |  98.721486819 |       92.5      |
|           18          |      22.19933      |     7.2725272     | 32.7601202379  | 99.2811430166 |       93.0      |
|           19          |      23.23633      |    6.601368825    | 28.4096878681  | 99.7554289662 |       93.5      |
|           20          |      24.27333      |     5.9167947     | 24.3757024685  | 100.084416952 |       93.8      |
|           21          |      25.31033      |    5.877518044    | 23.2218151403  | 101.825969364 |       95.4      |
|           22          |      26.34733      |     5.83347134    | 22.1406546318  | 103.496161153 |       97.0      |
|           23          |      27.38433      |    5.780182672    | 21.1076286037  |  105.03827619 |       98.4      |
|           24          |      28.42133      |    5.722720212    | 20.1353005366  | 106.507282134 |       99.8      |
|           25          |      29.45833      |     5.65914613    | 19.2106821059  | 107.875624438 |      101.1      |
+-----------------------+--------------------+-------------------+----------------+---------------+-----------------+

 

Sorry if I forgot to mention one thing. The flange diameter in the spreadsheet was meant to be a minimum flange diameter. This corresponds to the bolts used, so that the thread engagement of the bolts to the combustion chamber was 1.5*bolt_diameter. We can, of course, have larger flanges.

So now, the chamber diameter doesn't need to be linked to a specific tank diameter. We can adjust the lengths to ensure that the ratio is what we need. This is then more difficult to plot and achieve a relationship. I wonder if we can utilize linear algebra somehow for this. I was going to investigate at some point.

I suspect, though, that we would want to maximize the chamber diameter, so that we can now reduce the length of the rocket. One way to go about this is to have a combustion chamber that would then have skirts instead of flanges.

 

4:14 am
July 23, 2010


rpulkrabek

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Luke Maurits said:

Bad news. :(  While I still think something fishy is going on with the drag coefficients in OR, that doesn't actually explain the low altitude I was seeing.  It turns out that by the time that coefficient gets crazily high, the air density is low enough that there is minimal drag.  OR lets you plot the actual drag force in Newtons and I can see very clearly that there's no significant drag for most of the free-fall part of the flight.

The problem is the delta-v.


 

While this is a setback, it's not necessary bad news. It just means we have to reconfigure our rocket model. Going to space is a difficult task, it's up to us to find the most efficient way we can.

Our delta-v was wrong, but luckily we discovered why, and didn't have to spend any money it. We just have to understand the drag forces involved a bit better.

4:18 am
July 23, 2010


rpulkrabek

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Luke Maurits said:

As an alternative to adding propellant, we could drastically lower the dry mass somehow.  Replacing the aerostructure with fibreglass or carbon fibure could be one way to do this, although it would make construction a lot more problematic and perhaps more expensive to the point of cancelling out the cost of more propellant.  Another alternative would be to take advantage of the fact that hybrid engines can be throttled – rather than just opening the N2O valve up at launch and leaving it like that, we could throttle back somewhat during the thickest part of the atmosphere and then open it up again once we were higher up.  This would reduce drag losses somewhat.  It does complicate our valve-control and avionics requirements, though.


 

Is there a reason that some sort of plastic can't be used for the aerostructure?

5:05 am
July 23, 2010


Luke Maurits

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rpulkrabek said:

 

Is there a reason that some sort of plastic can't be used for the aerostructure?


 

No reason, as long as the plastic was strong enough not to bend due to wind-shear etc.  This is certainly something to consider, since it might be possible to find plastic tubing in the appropriate diameters of the shelf.  We may still need to use Al for the propulsion section, since that also has to deal with the weight of the engine plus the thrust (which is transferred to the aerostructure via the engine-mounting bolts).  There is also the possibility of some moderately high heat during the faster parts of the flight through the atmosphere.

Did you have any particular plastics in mind?

Main CLLARE workgroups: Mission Planning, Navigation and Guidance. I do maths, physics, C, Python and Java.

5:13 am
July 23, 2010


Luke Maurits

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Ohkla openrocket modelmouse
By the way, here's the OR diagram of the larger, Karman-line passing rocket.  You can see some basic stats around the place.  The big grey part is the engine – OR doesn't support an engine which isn't constant diameter, but it doesn't really matter for the sake of the simulation, since the CM is along the axis of symmetry anyway.

One thing to keep in mind is that, currently, OR is calculating the CM of the engine by assuming it is of uniform density, which in the case of a hybrid is quite wrong – the oxidiser tank is heavier than the fuel chamber.  This shouldn't affect the simulated apogee at all, but it does have ramifications for stability – in actual fact, the real CM of the rocket will be slightly forward of where it is shown, because of the heavier oxidiser tank.  This means that the stability margin is, in fact better than shown here.

Have to say, it looks pretty cool. sf smile

Main CLLARE workgroups: Mission Planning, Navigation and Guidance. I do maths, physics, C, Python and Java.

5:26 am
July 23, 2010


Luke Maurits

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rpulkrabek said:

Our delta-v was wrong, but luckily we discovered why, and didn't have to spend any money it. We just have to understand the drag forces involved a bit better.


 

It's true that we didn't have to spend any money to find this out, but the amount of money we'll need to spend per launch will now be almost twice what it was if we have to go from 100 kg to 175 kg, so it's still kind of a bummer.

Since the problem turned out to be entirely delta-v related, I don't think there's that much more understanding of drag to be done.  I checked Sampo's thesis and it turns out that OR does tend to overestimate drag at supersonic speeds – so, if OR says drag is not enough to keep us below 100 km, then that's probably correct.

Main CLLARE workgroups: Mission Planning, Navigation and Guidance. I do maths, physics, C, Python and Java.

7:33 am
July 23, 2010


Luke Maurits

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rpulkrabek said:

I suspect, though, that we would want to maximize the chamber diameter, so that we can now reduce the length of the rocket. One way to go about this is to have a combustion chamber that would then have skirts instead of flanges.


 

I think we definitely need to learn more about the requirements that efficient combustion place on the chamber dimensions before we can say too much about this with confidence – although I realise you weren't proposing this as something we definitely should do.

I think that, at the end of all this mass modelling, what we should come out with is a good set of requirements for the engine.  E.g. we should be able to say something very close to this:

  • The tank and chamber should be made of 6061 Al T6.
  • The engine should have a maximum outer diameter between 25 and 30 cm (anything narrower is going to have an absurdly high fineness ratio).
  • The total length of the engine should not exceed 5m (the 175 kg propellant engine I used to break the Karman line in OR is 4.3 m, so we know this is possible)
  • The total propellant mass should be 180 kg (this is more than enough with our current design (which can probably be made lighter) and has the nice property that a 8:1 O:F ratio results in 160 kg of N2O and 20 kg of PE, i.e. we have nice round numbers for both propellants).
  • The inner diameter of the chamber should be such that it is easy to buy PE rods of that diameter to use as grains.
  • The average thrust or maximum burn time should be SOMETHING WE STILL NEED TO FIGURE OUT

Then, one entirely self-contained subproject of OHKLA can be to build the best damn engine possible within these constraints.  Once that is done we can build everything else around the results of that.

I am slightly tempted to say that the maximum outer diameter of the engine should be 30 cm (which means the chamber can be basically anything less than that), since that way we know the inner diameter of the aerostructure and so people can work entirely independently on, e.g. the separation system that couples the different segments together.  On the one hand this feels kind of arbitrary and so I don't like making it a strong requirement.  But on the other hand, it's not really any bother to just fix the maxmium diameter since the oxidiser tank can have whatever L:D ratio we like and it won't make any difference – and it's a considerable advantage to be able to work on the segment couplers at the same time as the engine.

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9:07 am
July 23, 2010


Luke Maurits

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rpulkrabek said:

 

While this is a setback, it's not necessary bad news. It just means we have to reconfigure our rocket model. Going to space is a difficult task, it's up to us to find the most efficient way we can.

Our delta-v was wrong, but luckily we discovered why, and didn't have to spend any money it. We just have to understand the drag forces involved a bit better.


 

Actually, there's some silver lining to this cloud.

One thing I always wanted us to be able to do was to cluster a few OHKLA engines together to make a minimal TLI stage for very basic lunar and interplanetary probes.  To get from LEO to the moon takes a delta-v of about 3200 m/s.  Back when I thought OHKLA would need 1600 m/s, I thought we'd need to double the delta-v to send something to the moon, but if OHKLA needs 2100-2400 m/s then it's considerably less of an increase.

Main CLLARE workgroups: Mission Planning, Navigation and Guidance. I do maths, physics, C, Python and Java.

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