Puneet Varma (Editor)

Sunrise (telescope)

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Website
  
Official Page

Mission type
  
Balloon-borne telescope

Operator
  
Max Planck Institute for Solar System Research (MPS)

Mission duration
  
6 days (2009), 5 days (2013)

Manufacturer
  
Max Planck Institute for Solar System Research Kiepenheuer Institute for Solar Physics High Altitude Observatory Lockheed Martin Solar and Astrophysics Laboratory Instituto de Astrofísica de Canarias Instituto Nacional de Técnica Aeroespacial Instituto de Astrofísica de Andalucía Grupo de Astronomía y Ciencias del Espacio

Launch mass
  
2 t (2.0 long tons; 2.2 short tons)

The Sunrise balloon-borne solar observatory consists of a 1m aperture Gregory telescope, a UV filter imager, an imaging vector polarimeter, an image stabilization system and further infrastructure. The first science flight of Sunrise yielded high-quality data that reveal the structure, dynamics and evolution of solar convection, oscillations and magnetic fields at a resolution of around 100 km in the quiet Sun.

Contents

The strong absorption of UV radiation by the Earth's atmosphere makes it challenging to carry out ground-based observations at these wavelengths. A balloon mission reaching altitudes of above 30 km benefits from a reduction of UV absorption by 99%, making engineering solutions for the telescope easier. The launch site was in the arctic region to make uninterrupted observation of the Sun over several days possible. The telescope has a 1 metre primary mirror that directs the 1 kW of solar radiation to the first focal point where 99% of the radiation is reflected out of the telescope, the remaining light is transferred into several instruments.

The one metre diameter primary mirror is made from a glass ceramic zerodur, it is the central part of the gondola of nearly 2 tons. Solar panels of 1.5 kW output power are used to power the onboard equipment and a hard disk array of 2 x 2.4 Terabyte is used to store the data during flight.

Instruments

  • CWS, Correlating Wavefront Sensor is a CCD camera with 1 kHz read-outs responsible generate the images necessary for image stabilization and proper alignment.
  • SUFI, Sunrise Filter Imager observes the sun in five distinct wavelengths 214, 300, 312, 388 and 397 nm, on a 2048 x 2048 pixel CCD, through a filter wheele.
  • IMaX, Imaging Magnetograph eXperiment observes the Zeeman splitting of the iron line (FeI) around 525 nm. The observed field of view is 50 x 50 arcseconds.
  • Flights

    1. Sunrise's first flight was launched at 8:05 8 June 2009 local time from Esrange, near Kiruna, Sweden and it landed 1:45 14 June 2009 local time on Somerset Island, Nunavut, northern Canada after a flight duration nearly six days.
    2. Sunrise's second flight was launched at 7:38 (5:38 UTC) on 12 June 2013 from Esrange, near Kiruna, Sweden, and it landed afternoon 17 June 2013 on Boothia peninsula, Nunavut, northern Canada after a flight duration of over 5 days.

    References

    Sunrise (telescope) Wikipedia