May 01, 2012 Volume 08 Issue 17
 

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Maximum precision provides a new view of the universe

ALMA does not use one single antenna for observation purposes but rather 66 receivers, precisely controlled and interconnected to form a giant telescope. Exact positioning of the antennas at the Chilean site, ensured by angle encoders from HEIDENHAIN, is of paramount importance. [Photo credit: ESO/José Francisco Salgado (josefrancisco.org)]

 

 

 

 

The international ALMA project is a source of prestige for all those involved. Although the observatory is to be completed in 2013, it began supplying breathtaking images from the depths of the universe on October 3, 2011, after 12 of the 100-ton antennas went online. Twenty-four of the 66 total antennas have been brought online to date.

The ALMA observatory in the Atacama Desert in northern Chile sits on a desert plateau 5,000 m above sea level. It is the most powerful radio telescope in the world, and the world's most complex terrestrial observatory. With ALMA, short for "Atacama Large Millimeter/Submillimeter Array," astronomers aim to investigate remote galaxies and search for the building blocks of solar systems and inhabitable planets. Construction of the observatory is not complete, but the unexpectedly high level of precision evident as antennas have come online has caused intense excitement throughout the world.

ALMA does not use one single antenna to observe the cosmos but many receivers positioned precisely and interconnected to become a single telescope. Alma Correlator, one of the most rapid specialized supercomputers in the world, calculates the image data of the antennas to produce a general overall view.

Pinpoint accuracy, light years away
The coupling of the antennas to produce a giant telescope enables ALMA to capture images of celestial bodies at a distance of many millions of light years. Exact positioning of the antennas is of elementary importance, because the slightest imprecision can distort the results and lead to blurred images.

The ERA 7480C angle encoder consists of a scanning unit and a one-piece steel scale tape as graduation carrier. The steel scale tape is supplied by HEIDENHAIN as standard to a length of 30 m and significantly longer on request. Circle segments are available in applications with no full circle or if measurement is not required over 360°. The ERA 4282C modular encoder consists of a scale drum and a highly compact scanning head.

 

 

 

 

A decision was made by those responsible for the 25 European radio antennas to order angle encoders from HEIDENHAIN. The company, from Traunreut in Upper Bavaria, Germany, has been developing angle encoders for almost 60 years and is considered a pioneer in this sector. With outstanding measurement precision and a high level of long-term stability, these devices ensure the required accuracy for aligning the ALMA antennas.

A special strength of the HEIDENHAIN angle encoders used in the project is outstanding precision within one signal period. They function without contact, so they are especially suitable for use in precision devices.

Precise measurement of horizontal and vertical angles
To align the horizontal angle (azimuth) with precision, the European ALMA antennas use the new incremental ERA 7480C angle encoder with 247,800 scale lines and a diameter of 3,155 mm (124.21 in. or 10.3 ft). The ERA 7480C was specifically developed for use with the ALMA, and the tape length was adapted precisely according to the required diameter. Achievable precision was simulated beforehand as a part of project development. The ERA 7000 angle encoders consist of a scanning unit and a one-piece steel scale tape as graduation carrier.

The vertical angle (elevation) is set by the researchers in Chile with the aid of the ERA 4282C angle encoder from HEIDENHAIN. The especially precise angle encoder of the ERA 4000 series, featuring a steel scale drum, has 32,786 scale lines and a diameter of 209 mm (8.23 in.).

The interface electronics from HEIDENHAIN adapt the encoder signals to the interface of the subsequent electronics. The new external EIB 749 interface box interpolates and compensates the output signals from the scanning head, and position values are output via Ethernet to the antenna's control computer.

Schematic representation of a circular graduation with distance-coded reference marks (ERA 4480 with 20,000 lines as example).

 

 

Angle encoders
The term "angle encoder" is typically used to describe encoders that have an accuracy of greater than ±5 angular seconds and a line count above 10,000. These angle encoders are found in applications that require the highly accurate measurement of angles in the range of a few angular seconds, e.g. in rotary tables and swivel heads on machine tools, C axes on lathes, and also in measuring equipment and telescopes.

Measuring principle
HEIDENHAIN encoders incorporate measuring standards of periodic structures known as graduations. These graduations are applied to a carrier substrate of glass or steel. With the incremental measuring method used, for example, for the ALMA space telescope, the graduation consists of a periodic grating structure. The position information is gained by counting the individual increments (measuring steps) from a datum set to any location. Since an absolute reference is required to ascertain positions, the measuring standard has an additional track that bears distance-coded reference marks. The absolute position on the scale, established by the reference mark, is gated with exactly one measuring step.

Improving productivity overall
Products from HEIDENHAIN ensure that machines and plants work productively and efficiently. DR. JOHANNES HEIDENHAIN GmbH develops and manufactures linear and angle encoders, rotary encoders, digital readouts, and numerical controls for demanding positioning tasks. HEIDENHAIN products are used primarily in high-precision machine tools as well as in plants for the production and processing of electronic components.

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HEIDENHAIN

Source: DR. JOHANNES HEIDENHAIN GmbH, Traunreut, Germany

Published May 2012

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