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10 June 2010 • NCAR’s Coronal Multichannel Polarimeter (CoMP) found a new home early this year on Hawaii’s Mauna Loa, a high-elevation paradise for astronomical observers. Developed in 2004 by the center’s High Altitude Observatory, the NSF-funded instrument had been gathering detailed data on coronal magnetism at the National Solar Observatory in Sunspot, New Mexico.
Peter Nelson (NCAR High Altitude Observatory) adjusts the alignment of NCAR’s Coronal Multichannel Polarimeter shortly after its arrival at Hawaii’s Mauna Loa Solar Observatory. The instrument was moved to Hawaii in February after six years at the National Solar Observatory in New Mexico. CoMP’s diffusing lens (the small black ring at top) sits atop the instrument’s telescope. (Photo by Andy Watt.)
Magnetic fields are difficult to assess within the thin, superheated coronal environment, but CoMP’s highly sensitive infrared sensors have done the job well. The instrument’s 20-centimeter (8-inch) telescope tracks magnetic activity around the entire edge of the Sun, covering much more area than previous instruments and gathering data as often as every 15 seconds.
Among other landmarks, CoMP collected the first-ever coronal observations of Alfvén waves, fast-moving perturbations that emanate from the Sun along magnetic field lines. Previously detected only in the heliosphere, the waves were found to be far more prevalent than expected within the corona, where their influence is subtle. “Alfvén waves can provide us with a window into processes that are fundamental to the workings of the Sun and its impacts on Earth,” noted NCAR principal investigator Steven Tomczyk in 2007, when the findings were published in Science.
In February, NCAR technicians installed CoMP at the center’s Mauna Loa Solar Observatory (MLSO), which monitors solar activity on a year-round basis. Placing CoMP at Mauna Loa will greatly expand the observing opportunities for the instrument, which requires pristine skies. Observers will be able to operate CoMP on more than 300 clear days each year in Hawaii, compared to about 30 in New Mexico. “It is a huge improvement,” says Tomczyk.
To make room for CoMP, the observatory replaced its former Prominence and Inner Coronal Studies instrument with a more compact sensor that detects the same emission line of hydrogen, known as h-alpha, but at a fraction of the cost and with higher spatial resolution.
The NCAR Mauna Loa Solar Observatory benefits from clean air and clear skies year-round.
Other changes are in the offing. By late 2012, a new coronagraph, part of the forthcoming COronal Solar Magnetism Observatory (COSMO), will replace the current K-coronameter, which has been in place since 1980. The new instrument will provide significantly better temporal resolution and signal-to-noise ratio, plus more uniform spatial resolution. These qualities will allow for better monitoring of coronal mass ejections (CMEs), a primary driver of space weather. The new instrument can also collect data from lower coronal altitudes than before, which will help spot the onset of CMEs.
For more on the CoMP replacement, see the news story on the HAO website.
The University Corporation for Atmospheric Research manages the National Center for Atmospheric Research under sponsorship by the National Science Foundation. Any opinions, findings and conclusions, or recommendations expressed in this publication are those of the author(s) and do not necessarily reflect the views of the National Science Foundation.