We will be having a multiwavelength campaign (with 3-4 X-ray and UV satellites) to study the disk and boundary layer changes throughout the supercycle of V1159 Ori that will begin Feb 8 and run through March 28. Optical magnitudes to delineate where we are in the cycle would be greatly appreciated (as well as any spectra with Balmer lines, especially Hbeta or Halpha). Any immediate attention to this object would also be very helpful to define what should be the start of the superoutburst phase. Further info can be obtained from Paula Szkody at: szkody@astro.washington.edu