D. Biesecker, D. Alexander, R.C. Altrock, C. DeForest, A. Fludra, B. Forsyth, T. Galvin, S. Gibson, D. Hassler, T.W. Henry, J.T. Hoeksema, C. Korendyke, A. Lazarus, A. Lecinski, R. Lepping, A. Panasyuk, P. Riley, J. Steinberg, L. Strachan, B. Thompson, T. Summanen and A. Szabo
The Whole Sun Month campaign uses a coordinated set of observations made by SOHO and other space--based and ground--based instruments. The observations were centered on the conditions of the near--solar--minimum, low altitude corona between August 10 and September 8, 1996. The goal of the analysis of these observations is to quantify the large--scale physical properties ({\it e.g.} densities, temperatures, velocities, and magnetic field) in the solar minimum corona between 1 and 3 solar radii. The connection between low coronal structures and in-situ observations of the solar wind are being studied as well. In this poster we present an overview of the observations, including data taken from the following instruments: SOHO/UVCS, SOHO/LASCO, SOHO/EIT, SOHO/SUMER, SOHO/CDS, SOHO/MDI, SOHO/CELIAS, SOHO/SWAN, WIND/SWE, WIND/MFI, Ulysses/SWOOPS, Ulysses magnetometer, Wilcox Solar Observatory, Mauna Loa MkIII Coronagraph, and NSO/Sacramento Peak.