atacama large millimeter/submillimeter array karl g. jansky very large array robert c. byrd green...

26
Atacama Large Millimeter/submillimeter Array Karl G. Jansky Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array Radio Telescopes and Radiometers 2015 Single Dish School Jim Condon NRAO, Charlottesville

Upload: kerry-wilkins

Post on 13-Dec-2015

224 views

Category:

Documents


0 download

TRANSCRIPT

Atacama Large Millimeter/submillimeter Array

Karl G. Jansky Very Large ArrayRobert C. Byrd Green Bank Telescope

Very Long Baseline Array

Radio Telescopes and Radiometers2015 Single Dish School

Jim CondonNRAO, Charlottesville

Radio Telescopes and Antennas• An antenna is any device that

converts electromagnetic radiation traveling through space to electrical currents flowing in a wire (receiving antenna) or vice-versa (transmitting antenna).

• Radio telescopes, and only radio telescopes, contain antennas.

• Most of a typical radio telescope is not an antenna − the big dish just redirects electromagnetic radiation to the antenna part.

Single Dish School 2015 July 6

Electromagnetic radiation is produced by accelerating charged particles

Single Dish School 2015 July 6

Dipole antenna Power pattern

Single Dish School 2015 July 6

Reciprocity theorem

Single Dish School 2015 July 6

The receiving and transmitting patterns of an antenna are identical.

Ground-plane Waveguide horn vertical = ½ of a half-wave dipole

Single Dish School 2015 July 6

The waveguide horn used to discover λ = 21 cm HI emission from our Galaxy

Single Dish School 2015 July 6

Parabolic reflector:directivity and collecting area

Single Dish School 2015 July 6

Prime focus

Aperture

Single Dish School 2015 July 6

Illumination, field, and power patterns

Single Dish School 2015 July 6

Cassegrain subreflector

Single Dish School 2015 July 6

140-foot (43 m)Cassegrain

Single Dish School 2015 July 6

Reflector surface errors

Single Dish School 2015 July 6

100 m homology telescope in Effelsberg

Single Dish School 2015 July 6

GBT: homology plus active surface

Single Dish School 2015 July 6

GBT Offset Gregorian + Prime Focusfor unblocked aperture

Single Dish School 2015 July 6

Single Dish School 2015 July 6

GBT feeds andradiometers

Single Dish School 2015 July 6

Antenna output noise: voltage and power

Single Dish School 2015 July 6

TA = “antenna temperature”Ae = effective area

S = flux densityPν = power per unit frequencyk = Boltzmann’s constant ≈ 1.38 × 10−23 Joules per Kelvin

The simplest radiometer

Single Dish School 2015 July 6

Square-law detector: output noise voltage is proportional to input power

Single Dish School 2015 July 6

Integrator output noise for: N = 50 samples N = 200 samples

Single Dish School 2015 July 6

Differential radiometer

Single Dish School 2015 July 6

Superheterodyne receiver

Single Dish School 2015 July 6

Spectrometers and software-defined digital back ends

Single Dish School 2015 July 6

The National Radio Astronomy Observatory is a facility of the National Science Foundation

operated under cooperative agreement by Associated Universities, Inc.

To learn more about radio astronomy, Google Essential Radio Astronomy http://www.cv.nrao.edu/course/astr534/ERA.shtml or see the printed book (4 copies are on reserve)

Single Dish School 2015 July 6