! File: 1512C.PROP ! Database: PEPDB ! Date: 16-FEB-1994:21:23:23 coverpage: title_1: FOC AIRGLOW AND PARTICLE BACKGROUND proposal_for: SV/FOC pi_title: DR. pi_fname: F. pi_lname: PARESCE pi_inst: SPACE TELESCOPE SCIENCE INSTITUTE pi_country: USA pi_phone: 301-338-4823 ! end of coverpage abstract: line_1: The FOC background due to high energy particles in the earth's upper atmosphere line_3: will be measured. The main objectives are to assess the contributions of this line_4: source of noise to the FOC's deep survey capabilities and to its performance line_5: in daylight conditions and in the vicinity of the SAA. line_7: Measurements of the SAA induced noise will determine the line_8: operational constraints to be adopted for the FOC in the SAA. ! ! end of abstract general_form_proposers: lname: PARESCE fname: F. title: DR. inst: SPACE TELESCOPE SCIENCE INSTITUTE country: USA ! ! end of general_form_proposers block general_form_text: question: 3 section: 1 line_1: In order to compute a S/N ratio for an observation, the instrument line_2: background as a function of position in the orbit and target location need to line_3: be known as accurately as possible. Furthermore, if count rates in the SAA line_4: exceed certain limits, the instrument may have to be turned off. The line_5: boundaries of this region need to be carefully explored. line_9: 1. HIGH ENERGY PARTICLE BACKGROUND. With shutters closed, LEDs off, 512 x 512 line_10: format, F/48 and F/96 cameras, about 9-10 consecutive 10 minute exposures line_11: per orbit for 10 consecutive orbits through the SAA. Total time = 2 x 9.5 line_12: x 10 x 10 = 1600 minutes = 26.7 hours. line_13: Note that all these exposures should be obtained in parallel. line_14: If possible, parallel HSP dark count measurements should also be made. ! question: 3 section: 2 line_1: For the high-energy particle background the ST pointing is not important. ! question: 5 section: 1 line_1: To be scheduled as early as possible in the mission after FOC turn on. line_4: NOTES TO SCHEDULER: In this activity, an optimum OTA focus is not required. line_5: Both parts can be executed without requiring test FOC-i1 (1505-FOC Stability line_6: Test) or FOC-03 (1507-FOC Optical Focus) to have been performed. line_7: In these observations the FOC will be left exposing with the line_8: shutter closed, the attitude of the SC is not a concern. line_9: The particle background observations are to be executed in parallel with any line_10: other instrument. line_11: The HSP should be run in parallel, in response to the STScI request for line_12: supporting data for the HSP Radiation Monitoring OLT. If those parallel line_13: measures present scheduling problems, or are not possible at the time of line_14: execution, the HSP measurements should be dropped. ! !end of general form text general_form_address: lname: PARESCE fname: F. title: DR. inst: SPACE TELESCOPE SCIENCE INSTITUTE addr_1: 3700 SAN MARTIN DRIVE city: BALTIMORE state: MD zip: 21218 country: USA phone: 301-338-4823 telex: 684-9101-STSCI ! ! end of general_form_address records ! No fixed target records found ! No solar system records found ! No generic target records found exposure_logsheet: linenum: 1.000 targname: DARK config: FOC/96 opmode: IMAGE aperture: 512X512 sp_element: CLEAR num_exp: 15 time_per_exp: 600S priority: 1 req_1: PAR; req_2: CYCLE 0 /1-2; comment_1: SAA PEAK SHOULD BE SCHEDULED TO OCCUR comment_2: AT EXPOSURE #7 +/- 1. ! linenum: 2.000 targname: DARK config: FOC/48 opmode: IMAGE aperture: 512X512 sp_element: CLEAR num_exp: 15 time_per_exp: 600S priority: 1 req_1: PAR; comment_1: SAA PEAK SHOULD BE SCHEDULED TO OCCUR comment_2: AT EXPOSURE #7 +/- 1. ! ! end of exposure logsheet ! No scan data records found