JOP098 -- SOHO Joint Observation Programme. submitted by: Neale Ranns e-mail; ndrr@mssl.ucl.ac.uk CDS/EIT/MDI/TRACE/YOHKOH 03-Feb-1999 Multi-Wavelength Observations of Solar Flares. The principle aim of this Joint Observation Programme is to examine the morphological and temporal relationships between flare loop footpoint emissions in Hard X-ray and Extreme Ultraviolet radiation. Flare loop footpoint emission has been observed up to thirty minutes before a flare (Cheng,84) and during the impulsive phase (Cheng,81). The impulsive phase emission was observed to spatially correlate with the HXR emission and the preflare emission in some examples originated from future flare kernels. To accomplish our aim this observing program will incorporate TRACE, Yohkoh and SOHO-CDS-EIT-MDI in a combined continuous observation of an active region as it traverses the solar disk. This will ensure the acquisition of preflare data. Using the wide temporal coverage and high time resolution of the TRACE instrument we aim to observe EUV brightenings from Transition region or Chromospheric lines, during the preflare and impulsive phases of a solar flare and use Yohkoh-HXT to determine the location of the HXR source. Our intention is to determine the nature of the preflare burst i.e. whether they are the cause or a consequence of the X-ray flare. Using the improved spatial resolution of both instruments we will study the morphological relationships between the EUV and HXR sources and investigate any relationships between the intensity of the two photon energy domains. HXT will enable us to accomplish this in a higher energy band ($53-93keV$) than previously available. The further employment of SOHO-CDS/NIS, Yohkoh-SXT and SOHO-EIT will provide information on the densities and temperatures involved within the flare loops, and with CDS we can measure the velocities of the flare plasma. Inclusion of the MDI will allow the association of flare kernels with photospheric magnetic features, and aid with the determination of loop orientation. Yohkoh Continuous tracking of a single active region. TRACE Continuous tracking of a single active region. Cycle through filters, $1550\AA$, $1600\AA$, $WL$ and $171\AA$ to gain high time resolution CIV and FeIX images. CDS Continuous tracking of a single active region. Imaging in FeXVI, FeXIV, OV and HeI lines. EIT Tracking of a single active region, all filters. MDI Normal synoptic imaging.