9910( 1) - 04/04/03 10:12 - [ 1] PROPOSAL FOR HUBBLE SPACE TELESCOPE OBSERVATIONS ST ScI Use Only ID: 9910 Version: 1 Check-in Date: 04-Apr-2003 10:11:58 1.Proposal Title: Turbulent Variability of Disk Accretion in Cataclysmic Variables ------------------------------------------------------------------------------------ 2. Proposal For 3. Cycle AR 11 ------------------------------------------------------------------------------------ 4. Investigators Contact? PI: Philip Armitage JILA CoI: Dr. Keith Horne University of St. Andrews N ------------------------------------------------------------------------------------ 5. Abstract HST observations of WZ Sagittae by Knigge et al. (2002) detect prominent oscillations in the ultraviolet lightcurve following outburst. The oscillations probably arise in or near the boundary layer between the accretion disk and the white dwarf, and are a particularly clear example of the quasi- periodic variability seen in many accreting systems. We propose to investigate theoretically the origin and predicted properties of this variability. To do this we will run global magnetohydrodynamic simulations of the inner accretion disk and boundary layer, from which we will calculate predicted lightcurves using a range of assumptions as to how energy is dissipated and radiated from the disk. The temporal power spectrum of the predicted emission will be calculated and used as the primary point of comparison with observations. If we are able to reproduce the observations successfully, the investigation will provide a sound basis for using the observed variability of cataclysmic variables in the UV to constrain the physical properties of the white dwarf and inner accretion flow. ------------------------------------------------------------------------------------ 9910( 1) - 04/04/03 10:12 - [ 2] Summary Form for Proposal 9910 Item Used in this proposal ------------------------------------------------------------------------------------------------------------------------------------ Proposal Category AR ------------------------------------------------------------------------------------------------------------------------------------