The total solar eclipse of 1991 July 11, was photographed from Mauna Loa, Hawaii, by a research team from the High Altitude Observatory of the National Center for Atmospheric Research, Boulder, Colorado and Rhodes College, Memphis, Tennesee. The NCAR is sponsored by the National Science Foundation. The photograph of the solar corona was taken with a camera system developed by Gordon A. Newkirk, Jr. This specialized instrument photographs the corona in red light, 6500 A -- through a radially graded filter that suppresses the bright inner corona in order to show the much fainter streamers of the outer corona in the same photograph. Credit: High Altitude Observatory and Rhodes College. Technical Information for image: WLCC91 Time: 17:31:11 UT Pangle: 1.60 degrees Heliocentric north is 1.6 degrees counter clockwise of vertical. Vertical (top) is geocentric north. Left, (9 o'clock) is east. To assist in orientation, the darkest region is to the NORTH (top). There is a bright "hook" prominence in the NORTHWEST (upper right) and a barely visible prominence in the SOUTHWEST (lower right). There are several dots of prominences just slightly SOUTH of EAST (left, and just a little down). Objective aperture 11.4 cm Focal length 178 cm Focal ratio f/15 Film Kodak Technical Pan / 2415 Development D19 - 5 minutes (Film was developed at Sacramento Peak Observatory by Lou Gilliam) Wavelength isolation filer - Schott OG-3 Effective wavelength - 6500 A Exposure 27 seconds Radial filter range - 10^4 in transmission. Note: There are round dark circular artifacts in the image. These are the result of out of focus dust within the telescope. ftp instructions follow: ftp 128.117.16.39 or ftp puu.hao.ucar.edu anonymous enter some identification, such as your email address cd mk3/pub/eclipse91/WLCC get data_descrip_WLCC91 binary get WLCC91.gif quit ~