Vacuum collectors vacuTube

Collector vacuTube is a product, in which modern construction of heatpipe has been applied.

This solution enables heat exchange without direct contact with medium. The heat is received by evaporating alcohol mixture, flowing up and giving up the heat in heat exchanger. Then it is condensed and comes back down the collector.




Main advantages of vacuTube collector:

  • minimal heat losses due to application of vacuum as thermal insulation,
  • high efficiency at low external temperatures,
  • copper strip absorber, ultrasonic welded with highly selective layer,
  • pipes made of hardened borosilicate glass, vacuum closed with special metal alloy by thermocompression,
  • distributor boxes: made of extruded aluminum, furnace painted, distributor pipe made of copper,
  • warranty 5 years


Assembly:

  • angle of inclination 15 - 90º,
  • special designed assembly sets enabling quick and easy assembly of collectors on each type of roof and as a free standing structure on the ground.
If you are interested in solar collector sets that will enable you to limit heating costs in summer period up to 90% and annually up to 60%, please contact.

Within 24 hours we will send you results, selection suggestions and simulations of possible financial and ecological effects.


Technical specifications

 

vacuTube HP 65/20

vacuTube HP 65/30

Dimensions

1992x1450x165 mm

1992x2153x165 mm

Number of pipes

20

30

Gross surface

2,9 m2

4,29m2

Aperture surface

2,1 m2

3,21 m2

Absorber surface

2,0 m2

2,97 m2

Absorption coefficient

95%

Emission coefficient

5%

Linear loss coefficient

a1=1,16 W/m2K

Nonlinear loss coefficient

a2=0,0060 W/m2K2

Optical efficiency

n0=80,0%

Optical efficiency*

n0,05=67,00%

Maximum temperature in no-load state
collector

240oC

Maximum temperature in no-load state
pipe

290oC

Maximum working pressure

6 bar

Weight without medium

50 kg

87 kg

Liquid volume

0,9 l.

1,30 l.



*Efficiency calculated at insolation 1000 W/m2 (800 W/m2) and temperature differ
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