Doc Greiner Research Observatory
By
Matt Mills
The Solar and Heliospheric
Observatory (SOHO) was launched on December 2nd, 1995 to study the Sun. It is currently the main source of near-real
time solar data for space weather prediction.
The Large Angle and Spectrometric Coronagraph (LASCO) aboard SOHO
consist of three coronagraphs: C1, C2, and C3.
Coronagraphs C2 and C3 are both useful for observing the outer solar
atmosphere (corona) from near the solar limb to a distance of 21 million
kilometers. LASCO blocks direct light
from the surface of the Sun with an occulting disk, creating an artificial
eclipse, 24 hours a day, 7 days a week.
LASCO has also become SOHO’s principal comet finder.
The Kreutz, Meyer, Marsden
and Kracht Sungrazers are families of comets characterized by orbits taking
them extremely close to the Sun at perihelion. Many hundreds of smaller members
of the families, some only a few meters across, have been discovered since the
launch of the SOHO satellite in 1995.
None have survived their perihelion passage. More than 75% of the SOHO Sungrazers have
been detected by amateur astronomers analyzing SOHO's observations via the
Internet.
Our streamlined method has
been developed to search for Sungrazers using LASCO C2 and C3 images for the
internet using IrfanView and MaxIM DL
software programs.

Note: Use the Set advanced
options in IrfanView to convert to
grayscale for better comet definition.


Check the Loop box.