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    PR # 32042                                                                   
     During outburst, the infrared through X-ray spectra of dwarf novae un       
     dergo dramatic changes due to the changing rate of accretion through        
     the disk and boundary layer. To study                       these cha       
     nges at high signal-to-noise ratio and high spectral resolution, we p       
     ropose to obtain near-simultaneous {\it ASCA\/}, {\it EUVE\/}, and {\       
     it HUT\/} observations of a dwarf nova $\sim $ once per day over an i       
     nterval of 4--5 days during the transition from quiescence to outburs       
     t or outburst to quiescence. {\it HUT\/} ($\lambda\lambda = 830$--185       
     0~\AA ) observing time is guaranteed. {\it EUVE\/} ($\lambda\lambda =       
      70$--700~\AA ) observing time is almost guaranteed. We seek approval       
      for {\it ASCA\/} observations to complete the coverage of the waveba       
    nds crucial to the study of th                                               
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