Image of the Solar Corona at the 26 February 1998 Eclipse POISE98 Caption from the HAO expedition to Curacao, Netherlands Antilles Image of the solar corona made at the total solar eclipse on 26 February 1998 in Curacao with the HAO Polarimetric Instrument for the Solar Eclipse 1998 (POISE98). This image shows both the plumes at the solar poles and the coronal streamers nearer the Sun's equator at onset of Solar Cycle 23. The POISE has an aperture of 80 mm, an effective focal length of 1000 mm, and a field of view of 6.56X6.56 solar radii on a Loral CCD with 2034X2034 pixels. The pixel size is 3.1X3.1 arc seconds. The spectral band of the image is set by an Andover filter with a central wavelength of 620 nm and a bandwidth of 10 nm. The CCD camera is a Pixel Vision Spectra Video camera with 16 bit digitization, an electron well depth of 95,000 electrons, and a read noise 20 electrons. The polarization analyzer contains fixed linear and quarter wave polarizers together with a Meadowlark Optics liquid crystal variable retarder. This image was recorded with a 1.0 second exposure time. The POISE98 images are processed numerically to remove the radial gradient due to the rapid outward decrease in the coronal density. This numerical 'flattening' replaces the radially gradiated optical filter used in the photographic Newkirk camera. In order to improve visibility of plumes near the poles and the brighter coronal streamers at lower latitudes, the image was also multiplied with a sine^4.0 function in apparent latitude to equalize the plume and streamer brightness in this image. The HAO expedition team for the '98 eclipse is Alice Lecinski, Kim Streander, David Elmore, Greg Card, Bruce Lites, and Steve Tomczyk. The High Altitude Observatory is a division of the U.S. National Center for Atmospheric Research, which is operated by the University Corporation for Atmospheric Research under contract with U.S. National Science Foundation. Caption written by Oran R. White, 4/30/98