COSMO K-Coronagraph (K-Cor) White Light Polarization Brightness Images
K-Cor provides polarization brightness (pB) images of the Sun's white light corona over a full field-of-view from 1.05 to 3 solar radii. Images are 16-bit 1024x1024, with 5.6 arcsec pixels at a 15 second time cadence. Data are available on the MLSO web page ~15 minutes after acquisition and can be used to identify coronal mass ejections (CMEs) in near realtime.
dataset
eng
https://www2.hao.ucar.edu/mlso/instruments/mlso-kcor-coronagraph
Dataset
publication
2017-08-01
EARTH SCIENCE > SUN-EARTH INTERACTIONS > SOLAR ACTIVITY > CORONA
EARTH SCIENCE > SUN-EARTH INTERACTIONS > SOLAR ACTIVITY > CORONA HOLES
EARTH SCIENCE > SUN-EARTH INTERACTIONS > SOLAR ACTIVITY > CORONAL MASS EJECTIONS
revision
2017-07-14
2013-09-30T19:42:39
publication
2013-09-30
GIF
The user is granted the right to use Mauna Loa Solar observations for non-commercial, non-profit research, or educational purposes only, without any fee or cost. The user is responsible to meet the Terms of Use and Copyright Issues furnished on the UCAR web site. Please credit all use of Mauna Loa data as: 'Courtesy Mauna Loa Solar Observatory, operated by the High Altitude Observatory, National Center for Atmospheric Research (NCAR), and supported by the National Science Foundation.' [http://www2.ucar.edu/terms-of-use]
None
UCAR/NCAR - HAO/Mauna Loa Solar Observatory
pointOfContact
MLSO Data Requests
pointOfContact
2023-02-27T15:41:28