Big Bear Solar Observatory

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Big Bear Solar Observatory
Old dome on the main BBSO building viewed from Big Bear Lake
Old dome on the main BBSO building
Organization New Jersey Institute of Technology
Location Big Bear Lake, California
Coordinates
Altitude 2,060 meters (6,760 ft)
Established 1969 (1969)
Website
www.bbso.njit.edu
Telescopes
New Solar Telescope 1.6 m reflector
FDHA telescope 10 cm refractor

The Big Bear Solar Observatory (BBSO) is a solar observatory located on the north side of Big Bear Lake in the San Bernardino Mountains of southwestern San Bernardino County, California (USA), approximately 120 kilometers (75 mi) east of downtown Los Angeles. The telescopes and instruments at the observatory are designed and employed specifically for studying the activities and phenomena of our solar system's star, the Sun.

General information[edit]

The observatory was built by the California Institute of Technology in 1969 under the direction of professor Harold Zirin.[1] Management of the observatory was transferred to the New Jersey Institute of Technology (NJIT) in 1997. Funding comes from NASA, the National Science Foundation, the United States Air Force, and other agencies.[2]

The location at Big Bear Lake is optimal due to the clarity of the sky and the presence of a body of water. The lake surface is about 2,055 meters (6,742 ft) above sea level, putting it above a significant portion of the atmosphere. The main observatory building is in the open waters of the lake, and was originally reached by boat, though a causeway was added later.[3] The water provides a cooling effect on the atmosphere surrounding the building and eliminates ground heat radiation waves that normally would cause optical aberrations.

Instruments[edit]

The observatory originally operated three solar telescopes: a 65 cm (26 in) vacuum reflector, a 24 cm (9.4 in) vacuum refractor, and a 20 cm (7.9 in) refractor. The 65 cm and 25 cm telescopes studied sunspots on the face of the Sun, while the 20 cm telescope tracked the full disk of the Sun from sunrise to sunset.

In 2006, the old main building dome was replaced with a larger, ventilated, 5/8 spherical dome in preparation for a new telescope.[4] It is a scaled-down version of the Southern Astrophysical Research Telescope (SOAR) dome, and incorporates several strategies to improve astronomical seeing.[5] Removal of the old 65 cm, and 25 cm telescopes took place in February 2007.[6]

In early 2007, DFM Engineering began building a new 1.6 m (63 in) clear aperture open frame, off-axis Gregorian telescope.[7] The New Solar Telescope (NST) saw first engineering light of the Sun at the Nasmyth focus in December 2008, and observations began in January 2009.[8] The telescope is set on an equatorial mount, which is attached to the existing pier. The mirror was figured from a 1.7 m blank by the University of Arizona Mirror Lab as a proof-of-concept for the mirrors of the Giant Magellan Telescope.[9] Until the Advanced Technology Solar Telescope is completed, the NST will be the largest clear aperture solar telescope in the world. It is able to resolve features on the Sun less than 50 km across. The project was a collaboration between BBSO/NJIT, the University of Hawaii Institute for Astronomy (UH IfA), and the Korea Astronomy and Space Science Institute (KASI).

In 2007, the 20 cm full-disk telescope was replaced by the 10 cm (3.9 in) Full Disk H-alpha (FDHA) Patrol Telescope, located in an additional small building called the Ash Dome.[10] It is co-mounted with another small telescope dedicated to observing earthshine.[11]

The observatory also hosts a station of the Global Oscillation Network Group, an experiment in helioseismology operated by the National Solar Observatory. It is located at the shore end of the causeway and began operating in 1995.[12]

Solar images[edit]

Top: Sun with Planet Mercury crossing its face. The small black dot at the top of the Sun is Mercury. Bottom photos: Shots of the Sun in hydrogen-alpha light through the 20 cm full-disc telescope. The left-hand image is a normal contrast image. The right-hand image, acquired on a different day, has its contrast enhanced by removing the limb darkening.

See also[edit]

References[edit]

  1. ^ Denker, C.; Naqvi, M.; Deng, N.; Tritschler, A.; Marquette, W. H. (2007). "Synoptic Observing at Big Bear Solar Observatory". The Physics of Chromospheric Plasmas ASP Conference Series 368: 515. Bibcode:2007ASPC..368..515D. 
  2. ^ "Big Bear Solar Observatory - FAQ". Big Bear Solar Observatory. Retrieved 2012-01-07. 
  3. ^ "Big Bear Solar Observatory - Causeway". Big Bear Solar Observatory. Retrieved 2012-01-15. 
  4. ^ "Big Bear Solar Observatory - Dome Blog". Big Bear Solar Observatory. Retrieved 2012-01-07. 
  5. ^ Verdoni, A. P.; Denker, C.; Varsik, J. R.; Shumko, S.; Nenow, J.; Coulter, R. (2007). "The thermal environment of the fiber glass dome for the new solar telescope at Big Bear Solar Observatory". Proceedings of SPIE 6689. pp. 66890Y. arXiv:0708.0622. doi:10.1117/12.734948. 
  6. ^ "Big Bear Solar Observatory - NST Blog Section 1". Big Bear Solar Observatory. Retrieved 2012-01-07. 
  7. ^ "Newsworthy Articles - Big Bear Solar Telescope". DFM Engineering, Inc. Retrieved 2012-01-07. 
  8. ^ "Big Bear Solar Observatory - NST Blog Section 5". Big Bear Solar Observatory. Retrieved 2012-01-07. 
  9. ^ Goode, Philip R.; Denker, Carsten J.; Didkovsky, Leonid I.; Kuhn, J. R.; Wang, Haimin (2003). "1.6 M Solar Telescope in Big Bear -- the NST". Journal of the Korean Astronomical Society 36: 125. Bibcode:2003JKAS...36S.125G. 
  10. ^ "Global High-Resolution H-alpha Network". Big Bear Solar Observatory. Retrieved 2012-01-07. 
  11. ^ "Project Earthshine". Big Bear Solar Observatory. Retrieved 2012-01-07. 
  12. ^ "NSO/GONG: Site - Big Bear". National Solar Observatory Global Oscillation Network Group. Retrieved 2012-01-07. 

External links[edit]