... 5146 UV Observations of Globular Clusters 5330 High Resolution Mapping of Pluto's Albedo Distribution 5440 Spectro Imaging of the Jovian Aurora 5301 Structure and Populations of Globular Clusters . ...
... REPORT #1143 PERIOD COVERED: 0700 EST Daily Status Report as of 140/1200Z. 1.0 ACTIVITIES SCHEDULED AND ACCOMPLISHED: 1.1 Completed WF/PC-2 5217 (Jupiter's Aurora and Airglow) The WF/PC-2 was used to make observations of Jupiter's north Auroral region ...
... Regions in M31 5301 Structure and Populations of Globular Clusters 5341 High Resolution Imaging of Saturn's UV Aurora 5469 Externally Illuminated ProtoStellar Disks and Naked Jets 5751 Understanding the Geminga(1E0630+178) Optical Counterpart Calibration ...
... 9.6.4 Example 4: SBC imaging of Jupiter?s Aurora at Lyman-alpha . ... 9.6.4 . Example 4: SBC imaging of Jupiter?s Aurora at Lyman-alpha . ... is reached in a one orbit exposure (2000 seconds) observing Jupiter?s aurora in Ly ...
... 9.6.4 Example 4: SBC imaging of Jupiter?s Aurora at Lyman-alpha . ... 9.6.4 . Example 4: SBC imaging of Jupiter?s Aurora at Lyman-alpha . ... is reached in a one orbit exposure (2000 seconds) observing Jupiter?s aurora in Ly ...
... in order to get both faces of the planet (Jupiter's rotation period is 10 hours), with the north aurora best viewed on one images and the south aurora best viewed on the other (tilted magnetic axis) and during each orbit, we take one 11-minute image of ...
... 1.14 Completed WF/PC-2 6662 (Observation of Short Timescale Variability of the Jovian UV Aurora) The WF/PC-2 was used to make observations of the aurora on the planet Jupiter in order to study its short timescale variability. ...
... 9.6.3 Example 3: WFC VIS Polarimetry of the Jet of M87 . 9.6.4 Example 4: SBC imaging of Jupiter?s Aurora at Lyman-alpha . ... What signal-to-noise ratio is reached in a one orbit exposure (2000 seconds) observing Jupiter?s aurora in Ly- ? ...