The Mauna Loa Solar Observatory (MLSO) K-coronameter (Mk4), was decommissioned on August 2, 2013, to be replaced by the new COSMO K-coronagraph.
The MLSO K-coronameter was the longest operating white light coronal instrument in history. Originally known as the Mk3, it was designed in the late 1970s by NCAR High Altitude Observatory (HAO) engineers led by Bob Lee and HAO scientists led by Dick Fisher. Mk3 was built on the legacy of the Mk1 and Mk2 (Richard and Shirley Hansen, G. Wlerick, and J. Axtell). It was installed at the Mauna Loa Solar Observatory in 1979 and began providing science quality images of the low corona in January 1980. The Mk3 provided the first routine images of the white light corona from the ground and complemented space-based coronagraphs by observing in the very low corona, where most of the explosive events known as coronal mass ejections (CMEs) originate. The Mk3 nominal 18-month mission was to support the newly launched space-based Solar Maximum Mission Coronagraph by observing CMEs in their early formation and recording the variability of the corona over time scales of minutes to months. The Mk3 long out-lived its nominal mission and continued to provide coronal observations well into the 1990s.
With the approach of the SOlar Heliophysics Observatory (SOHO) Mission, HAO designed and implemented upgrades to the Mk3, known as Mk4, which included the installation of a CCD detector to replace the original diode array, a better polarizing beam splitter, and mechanically stable calibration tilt plate registration. Mk4 has continued to operate until the present. The Mk3/4 K-coronameter has provided 33 years of low coronal observations from the maximum of solar cycle 20 to the maximum of solar cycle 24 acquiring over a half a million images, recording over 1000 CMEs, and observing the brightness and morphological changes of the corona with solar cycle activity.
The K-coronameter will be replaced by the COSMO K-coronagraph (K-cor), an entirely new instrument which will produce images with 10 times better signal-to-noise and 12 times faster image cadence than the K-coronameter. K-cor will begin providing data in the fall of 2013.
All of the Mk3/Mk4 observations since 1980 are available from HAO’s Mauna Loa homepage
August 6th: The Mk4 Coronameter has been removed from the MLSO spar! Here is a time-lapse of the operation:
HAO recognizes the many scientists, engineers, observers and support staff who were responsible for the design, fabrication, testing, software, operation, repair, calibration, processing and dissemination of the Mk3/Mk4 instrument and observations:
Richard Fisher, and in reverse alphabetical order: Eric Yasukawa, Oran (Richard) White, Lisa Waters, F. Telang, Allen Stueben, Jack Streete, Kim Streander, Andrew Stanger, Ackley Smith, Leonard Sitongia, David Sime, Rick Sheffer, Paul Seagraves, Paula Rubin, Greg Rose, Steve Rogers, Kristine Rock, Art Poland, Gordon Newkirk, Richard Munro, Greg Muir, C. Muir, Robert MacQueen, Ed Lundin, Ron Lull, Robert Lee, Alice Lecinski, Terry Leach, Loren Laramore, Lee Lacey. Darryl Koon, Don Kolinski, Art Hundhausen, Howard Hull, Tom Holzer, E. Harper, Holly Gilbert, Charlie Garcia, Dennis Gallagher, John Firor, Frank Everts, David Elmore, Giuliana deToma, Tony Darnell, Duc Chu, Clarke Chambellan, Jay Chalmers, Greg Card, Joan Burkepile, Ben Berkey, Cheryl Baker and a host of others including many student assistants.