[ATM] Fan locations & function for a 32
Dr. Wm. D. Hanagan, Jr.
hanaganl at comcast.net
Wed Jan 31 05:48:39 JST 2007
Bob Drew wrote:
> I accept the concept of sweeping away the boundary layer from the
> primary mirror surface. And I’ll use some fans under the mirror back.
......
> 1. Should the flow be across the mirror front be from one side to the
> other side? Or should it be vertically? (From the lower side of mirror
> box, exiting on the top? or vice versa? ) The scope will have a full
> shroud as a minimum or possibly a rigid tube later.
>
> 2. Since its operating in conjunction with the above (and without
> starting a debate) should the fans (imbedded in the cell underneath
> the mirror) suck or draw the air down and vent out the back of the
> box, or blow on the back of the mirror.
>
> 3.Are there 3” diameter fans that would be able to maintain flow
> across a box about 40” wide, or would a 4” be nec.? Brand names and
> models also appreciated
>
> The mirror is a 32” f4, 3” thick weighing about 200 lbs.
.......
Bob,
Here are a few recommendations.
Crossflow Fans
If you use a rectangular rather than a tube shaped mirror box, or you
can otherwise accommodate them, I would strongly recommend using one or
more "crossflow" fans. Crossflow fans are designed to produce an airflow
pattern that's almost exactly what we need to sweep the thermal boundary
layer from in front of a telescope mirror. Here's a link to a ball
bearing crossflow fan that is relatively inexpensive when you consider
the width of the air stream it produces. The speed of this fan is
controlled by the DC voltage applied (between 6V and 12V).
http://www.coolermaster.com/index.php?LT=english&Language_s=2&url_place=product&p_serial=STF-B01-E1
Much longer models are available from other manufacturers that produce a
wider swath of air flow. A Google search on "Crossflow Fans" will turn
up a large number of other options to consider, many of which are
available in 12 Volt models.
Square Fans
If you must use a tube, especially a smaller diameter tube, the
straight-line crossflow fan can be difficult to integrate into your
design. The more common square fans can be used in that situation to
sweep the surface of the mirror. Here's a link to an 80mm ball-bearing
fan (Sanyo Denki San-Ace 80 X 15 mm) which is only 15 mm deep from front
to back, so it will fit into tight spaces.
http://www.sidewindercomputers.com/sandenpetace.html
The 15 mm depth allows these fans to be mounted on the INSIDE of a 10"
I.D. tube which houses an 8" diameter mirror without blocking the
incoming light path for objects near the center of the field of view. As
the primary diameter increases, the space constraints on an inside
mounted square fan ease up as you go to larger tube and mirror
diameters, provided the typical 1" clear space exists between the mirror
and the inside of the tube wall. Even with inside mounted fans, the tube
itself will still need vent holes in the tube wall for each fan. Those
vent holes need to be at least as large as the inside opening of the fan
cage in order not to seriously diminish the volume of air moved by the fan.
An inside mounted fan can be useful to avoid a variety of mechanical
conflicts and space constraints, and it makes it more convenient to
mount a filter on the outside of the tube. However, I would consider the
use of a filter as experimental.
I wouldn't expect square fans to sweep a path much wider than roughly
1.5 times the diameter of the fan blade. Of course, the factor you use
depends greatly on how low a minimum airflow you can tolerate over the
surface of the mirror. You might want as many as 6 inlet and 6 outlet
fans for your 32" mirror. At $18.95, using 12 of these to ventilate a
32" mirror would be a little expensive compared to using crossflow fans.
Of course, the cost for the fans would be nothing compared to the
overall cost of a 32" telescope.
The Airflow Pattern Across the Face of the Mirror
You raised the question of whether the air coming out of a square fan
will travel the full distance across the face of a large mirror. The
airflow pattern of square fans is cone shaped and the air speed
diminishes fairly quickly as you move away from the fan. The airflow
pattern of crossflow fans is more linear and holds together over a much
greater distance out away from the fan. However, airflow takes the path
of least resistance. The combination of inflow and outflow fans that you
mentioned will put the path of least resistance directly across the face
of the mirror. If you keep that arrangement, I think you can expect most
of the air coming in to flow past the face of the mirror to the outflow
fans, even if you use square fans.
Direction of Airflow and the Dust Problem
Using fans introduces so much airflow through the telescope tube that
natural convection is likely to make a trivial contribution to cooling
the mirror and destroying the boundary layer, if indeed it contributes
at all. One concern introduced by using fans is the increased amount of
dust that passes through the telescope. A lot of dust can get kicked up
near ground level on a dry day. To draw as little of that dust into the
telescope as possible, I would recommend arranging for the air to flow
from top to bottom. I would duct the airflow from the vent fans out the
back of the box only if a minimum duct cross section of 1.5-2" X D can
be accommodated. Otherwise I'd run the air directly out the bottom side
of the mirror box.
Filtration
The airflow that you get with most crossflow and square fans drops
precipitously if you use a filter having the same area as the fan
intake. However, a box housing a filter with a vastly larger surface
area, or even a serpentine air inlet, might be usable for filtering dust
out of the incoming air stream. I'm still experimenting with approaches
for filtering the air and I can't give you any specific instructions on
this except to say that if you use a filter, the intake area must be
very large to have any hope of maintaining a high airflow across the
primary mirror.
I hope all of that helps.
Clear Skies,
Bill Hanagan
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