Plateau de Bure Interferometer

Former astronomical observatory

The Plateau de Bure Interferometer (PdBI) was a six-antenna interferometer on the Pic de Bure (2550 m) in the French Alps, operated by the Institut de radioastronomie millimétrique. In 2014, it has been replaced by the Northern Extended Millimeter Array.

Nº Q6151482 ★★★

Rara · Lugares

Plateau de Bure Interferometer

Former astronomical observatory

Texto en inglés

The Plateau de Bure Interferometer (PdBI) was a six-antenna interferometer on the Pic de Bure (2550 m) in the French Alps, operated by the Institut de radioastronomie millimétrique. In 2014, it has been replaced by the Northern Extended Millimeter Array.

En el mapa

Ver en OpenStreetMap · © los colaboradores de OpenStreetMap

Último precio

—

Precio mínimo

—

Mediana 7 d

—

Ventas 30 d

0

Rango 30 d

—

En circulación

0

Cotización

Ver tabla
Fechamediana MínMáxventas

Historial de ventas

Última venta
—
Media 30 d
—
Mínimo 30 d
—
Máximo 30 d
—
Ventas 7 d
0
Ventas 30 d
0

Aún no hay ventas.

Ventas anónimas: sin comprador ni vendedor. Las cifras solo cuentan ventas entre jugadores.

№ Ediciones numeradas · 0 acuñadas Próximo n.º 1 · Puntos ×3
En Wikipedia

Texto en inglés Aún no hay artículo en tu idioma: extracto en inglés.

The Plateau de Bure Interferometer (PdBI) was a six-antenna interferometer on the Pic de Bure (2550 m) in the French Alps, operated by the Institut de radioastronomie millimétrique. In 2014, it has been replaced by the Northern Extended Millimeter Array. It was specifically designed for millimetre-wave observations and specialises in studies of line emission from molecular gas and radio continuum of cold dust. The interferometer consisted of six antennas with a diameter of 15 m each. These antennas could be placed in a T-shaped pattern, with north–south track of 368 m and an east–west track of 768 m. There were 32 stations along these tracks where the antennas can be positioned. Observing bands are at 3, 2, 1.8 and 0.8 mm. At an observing wavelength of 3 mm (100 GHz frequency) each of these telescopes could resolve two objects 45 arcseconds apart from each other on the sky. In an interferometer, these 45″ are actually the size of the field of view. So an interferometer like this one images, at very high resolution (better than 1″), structures smaller than 45″.

Texto: Wikipedia en inglés, CC BY-SA 4.0. · Imagen: Douchet Quentin (CC BY-SA 3.0) ·

Cartas cercanas

Ver la ficha

Confirmación