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Big Bear Solar Observatory

Big Bear Solar Observatory (BBSO) is the premier university-based solar observatory in the United States. It is operated by New Jersey Institute of Technology (NJIT). BBSO features the most powerful solar telescope in the world - the 1.6 m clear aperture Goode Solar Telescope (GST), which has no obscuration in the optical train. Light corrected by adaptive optics is fed to either the visible (VIS) or near-infrared (NIRIS) spectro-polarimeter. Additionally, uncorrected light can be fed to a cryogenic spectrograph (CYRA) operating out to wavelengths of 5 microns. BBSO also operates full-disk patrol telescopes. 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. For details on BBSO instrumentation, including secondary telescopes, and science, see .

Big Bear Solar Observatory
GST dome.jpg
Dome on the main BBSO building viewed from Big Bear Lake
Organization New Jersey Institute of Technology
Observatory code G77
Location Big Bear Lake, California, US
Coordinates 34°15′30″N 116°55′16″W / 34.2583°N 116.921°W / 34.2583; -116.921Coordinates: 34°15′30″N 116°55′16″W / 34.2583°N 116.921°W / 34.2583; -116.921
Altitude 2,060 m (6,760 ft)
Established 1969
Telescopes Full Disk H-alpha (FDHA) Patrol Telescope
Goode Solar Telescope Edit this on Wikidata
Big Bear Solar Observatory is located in the US
Big Bear Solar Observatory
Location of Big Bear Solar Observatory
Commons page Related media on Wikimedia Commons


General informationEdit

BBSO is 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.

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 has more than a mile of water to the west, which is the direction from which the prevailing winds come. The cool lake provides a natural inversion that greatly reduces ground-layer turbulence and stabilizes images taken by the telescope. 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 with an approximate 200 meter causeway extending south from the north shore. Again, the water provides a cooling effect on the atmosphere surrounding the building and helps eliminate ground heat radiation waves that normally would cause optical aberrations.

GST During Installation into Dome Fall 2008

The observatory was built by the California Institute of Technology in 1969 under the direction of professor Harold Zirin. Management of the observatory was transferred to the New Jersey Institute of Technology (NJIT) in 1997, and the directorship of BBSO passed to NJIT professor Philip R. Goode. Now NJIT professor Wenda Cao is BBSO director. Funding comes from NASA, the National Science Foundation, the United States Air Force, and other agencies.


At the time of the transfer in 1997, the primary BBSO telescope was in the 0.5 m class, as were the world’s other high resolution solar telescopes. However, to resolve the fundamental scale in the Sun’s atmosphere (photon mean free path of 100 km at the Solar surface) an aperture of at least 1.5 m is required. Correction of distortion by the terrestrial atmospheric distortion by adaptive optics (AO, see is the enabling technology for the first facility class solar telescope built in the United States in a generation – the Goode Solar Telescope (GST). The GST is a 1.6 m clear aperture off-axis telescope, which feeds its unobstructed light to visible light and near-infrared (NIR) spectro-polarimeters. The GST benefits from three generations of AO, which now includes multi-conjugate AO (MCAO) in a demonstrator phase for wide-field correction. It is the only MCAO system in operation with three deformable mirrors.

Construction of the GST began in 2005 and the telescope saw first light in January 2009, with first AO corrected imaging in the Summer of 2010 in the NIR. Second generation AO corrected visible light in the Summer of 2012. In Summer 2016, first successful MCAO observations were made, which roughly trebled the corrected field of view – MCAO is essential for studies requiring wide field correction with high temporal cadence.

Until the Daniel K. Inouye Solar Telescope is completed, the GST will be the largest clear aperture solar telescope in the world - able to resolve features on the Sun less than 50 km across. The telescope was named the Goode Solar Telescope in July 2017.

Other telescopes in BBSO include the 10 cm (3.9 in) Full Disk H-alpha (FDHA) Patrol Telescope, located in an additional small building called the Ash Dome. It is co-mounted with another small telescope dedicated to observing earthshine. 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.

Solar imagesEdit

See alsoEdit

External linksEdit