HUBBLE SPACE TELESCOPE DAILY REPORT #1625 PERIOD COVERED: 0000Z (UTC) 05/01/96 - 0000Z (UTC) 05/02/96 Daily Status Report as of 123/0000Z 1.0 ACTIVITIES SCHEDULED AND ACCOMPLISHED: 1.1 Completed GHRS/2 6072 (The First Multiple Layer Doppler Imaging of = an Active Binary) The High Resolution Spectrograph (Side Two) was used to make the = first rapid mode multiple layer Doppler imaging of the active binary = system HD155555 (aka, V824). This target was observed in wavelengths of = Mg II and C IV in order to construct a 2-Dimensional map of the uneven = heating distribution in the choromosphere. A wavelength calibration = image was also taken. The observations were executed as scheduled, and = no anomalies were noted. 1.2 Completed FOS/BL 6242 (Binaries in Globular Clusters (FOS 37): = Time-Resolved Spectra) The Faint Object Spectrograph (Blue Side) was used to make rapid = mode spectrographic observations of the X-ray burst binary source located = in the globular cluster NGC-6624. Simultaneously X-ray observations will = be obtained using the XTE satellite. The orbital period of the X-ray = binary system is thought to be eleven minutes. The observations were = executed as scheduled, and no anomalies were noted. 1.3 Completed WF/P-2 6254 (GTO Pure Parallel Program - Cycle 5) The WF/PC-2 was use to make random long exposures of high galactic = fields taken in parallel with the prime science observations to obtain a = random sample of galaxies. The observations were executed as scheduled, = and no anomalies were noted. 1.4 Completed Two Sets of GHRS/1 6171 (CRIMP1: Cycle 5 = Condensed-Regimen Integrated Monitoring Program) The High Resolution Spectrograph (Side One) was used to obtain = darks, internal flats (in photoscan mode), wavelength calibrations and = observations of standard star BD+28D4211. This includes detector = calibration, sensitivity monitoring, and wavelength monitoring. The = observations were executed as scheduled, and no anomalies were noted. 1.5 Completed WF/PC-2 6561 (Ages of Extreme Metallicity Inner Galaxy = Globular Clusters) The WF/PC-2 was used to make photometric observations of the stars = in the globular cluster NGC-6387. This cluster has a very low = metallicity, and is relatively close to the galactic center. The = objective is to determine the age of the cluster, and compare it with the = ages of low-metallicity clusters at large galactocentric distances. The = observations were executed as scheduled, and no anomalies were noted. 2.0 FLIGHT OPERATIONS SUMMARY: 2.1 Guide Star Acquisitions: Scheduled Acquisitions : 5 Successful : 5 Scheduled Reacquisitions : 10 Successful : 10 2.2 FHST Updates: Scheduled : 9 Successful : 9 2.3 Operations Notes: HST operations transferred to the SAMS back-up facility at approxim= ately 123/0530Z in preparation for the simulation activities which will = take place in the SMOR/MOR area today. 3.0 SIGNIFICANT FORTHCOMING EVENTS: GSFC Internal Simulation #4 (EVA #2 - FGS/OCEK/ESTR2) will occur = today from approximately 8:00 a.m. until 6:00 p.m. /DMH