Adaptive optics produces ultrasharp images of sunspot (Forwarded)

National Solar Observatory
Sunspot, New Mexico

For more information contact:
Dave Dooling, Outreach and Education Officer
505-434-7015

October 4, 2005

Adaptive optics produces ultrasharp images of sunspot

Advanced technologies now available at the National Science Foundation's
Dunn Solar Telescope at Sunspot, NM, are revealing striking details inside
sunspots and hint at features remaining to be discovered in solar
activity.

This image, spanning an area more than three times wider than Earth, was
made possible by the Dunn's recently completed AO76 advanced adaptive
optics image correction system and a new high-resolution CCD camera.

The Dunn is the nation's premier high-resolution solar telescope. The
Association of Universities for Research in Astronomy operates the Dunn as
part of the National Solar Observatory under a cooperative agreement with
the NSF.

This ultrasharp image of sunspot AR 10810 shows several objects of current
scientific interest. G-band bright points, which indicate the presence of
small-scale magnetic flux tubes, are seen near the sunspot and between
several granules (columns of hot gas circulating upward).

The dark cores of penumbral fibrils and bright penumbral grains are seen
as well in the sunspot penumbra (the fluted structures radiating outward
from the spot). These features hold the key to understanding the magnetic
structure of sunspots and can only be seen in ultra high-resolution images
such as this one. Magnetism in solar activity is the "dark energy problem"
being tackled in solar physics today.

Normally such features are beyond the grasp of ground-based solar
telescopes because of blurring by Earth's turbulent atmosphere. The Dunn's
AO76 system compensates for much of that blurring by reshaping a
deformable mirror 130 times a second to match changes in the atmosphere
and refocuses incoming light. This allows the Dunn to operate at its
diffraction limit (theoretical best) of 0.14 arc-second resolution, rather
than the 1.0 to 0.5 arc-second resolution normally allowed by Earth's
atmosphere.

The Dunn has two high-order adaptive optics benches, the only telescope in
the world with two systems, which enhances instrument setup and
operations.

This image was built from a series of 80 images, each 1/100th of a second
long (10 ms), taken over a period of 3 seconds by a high-resolution Dalsa
4M30 CCD camera in its first observing run after being added to the Dunn.
Speckle imaging reconstruction then compiles the 80 images and greatly
reduces residual seeing aberrations.

The camera is part of the equipment suite for the Dunn's
Diffraction-Limited Spectropolarimeter, which is designed to analyze
magnetic field strength and direction inside sunspots.

The Dunn and its new systems are available for the world solar physics
community to use.

The National Solar Observatory is operated by the Association of
Universities for Research in Astronomy, under a cooperative agreement with
the National Science Foundation.

Technical notes:

* Sunspot AR 10810, observed Sept. 23, 2005, 17:03:47 UTC
* The image was taken and processed by Friedrich Woeger, a graduate
student from the Kiepenheuer-Institut fur Sonnenphysik in Freiburg,
Germany, with the assistance of Chris Berst of NSO. Woeger is working as a
summer student with Thomas Rimmele at National Solar Observatory at
Sunspot, NM.
* The camera chip is 2,048 x 2,048 pixels in size. This image is 1,868
pixels square because of the speckle reconstruction technique and other
factors.
* The image was taken in G-band, a blue part of the spectrum (430.5 nm)
where magnetic features stand out in high contrast. The G-band contains
spectral lines formed by CH molecules.
* The finished image spans an angle of about 56 arc-seconds, equivalent to
about 3.2 times the diameter of Earth, or 40,630 km (~25,190 miles), at
the visible surface of the Sun.
* The companion image includes a NASA image of Earth to scale on the left
side and an unprocessed single frame on the right half.
* Dunn Solar Telescope: Aperture, 76 cm; diffraction limit, 0."14 @ 430.5
nm (G-band) or 0".17 @ 500 nm.
* Adaptive optics type: Shack-Hartmann wavefront correction system.

IMAGE CAPTIONS:

[Image 1:
Low-res: http://www.nso.edu/press/DALSA/DALSA_2K_M.jpg (216KB)
Hi-res: http://www.nso.edu/press/DALSA/DALSA_2K.jpg (1.4MB)]
High-resolution image of sunspot produced with the new camera attached to
the Dunn's adaptive optics system.

Mandatory credit: Friedrich Woeger, KIS, and Chris Berst and Mark Komsa,
NSO/AURA/NSF.

[Image 2:
Low-res: http://www.nso.edu/press/DALSA/DALSA_blur_M.jpg (188KB)
Hi-res: http://www.nso.edu/press/DALSA/DALSA_blur.jpg (1.1MB)]
In this version, a NASA image of Earth is added for scale, and both Earth
and sunspot are artificially blurred on the left half to simulate normal,
uncorrected seeing through Earth's atmosphere. (No "before" companion was
made for a "before-and-after" image set.)

Mandatory credit: Friedrich Woeger, KIS, and Chris Berst and Mark Komsa,
NSO/AURA/NSF.