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This special page shows all uploaded files.
Date | Name | Thumbnail | Size | User | Description | Versions |
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20:44, 4 August 2016 | 20150622 TP-bl0-bl11.png (file) | 490 KB | Dgary | Total Power and baseline cross-correlation data for flare of 2015 June 22 | 1 | |
00:44, 5 August 2016 | RSTN.png (file) | 40 KB | Dgary | Figure 1 of EOVSA Total Power Calibration document | 1 | |
00:56, 5 August 2016 | Eovsa1.png (file) | 45 KB | Bchen | EOVSA photo from array center | 1 | |
01:10, 5 August 2016 | X2.png (file) | 90 KB | Dgary | Figure 4 of Total Power Calibration document | 1 | |
01:10, 5 August 2016 | Y2.png (file) | 93 KB | Dgary | Figure 5 of Total Power Calibration document | 1 | |
01:22, 5 August 2016 | Eovsa gain controls.png (file) | 103 KB | Bchen | Summary of EOVSA gain control "knobs" | 1 | |
01:23, 5 August 2016 | Eovsa correlator block.png (file) | 131 KB | Bchen | block diagram of digital correlator | 1 | |
01:24, 5 August 2016 | Eovsa down converter block.png (file) | 40 KB | Bchen | Block diagram of down-converter system | 1 | |
14:03, 5 August 2016 | Calib 20160116.png (file) | 106 KB | Dgary | Figure 6 of Total Power Calibration document | 1 | |
14:10, 5 August 2016 | X3.png (file) | 85 KB | Dgary | Figure 2 for Total Power Calibration document | 1 | |
14:10, 5 August 2016 | Y3.png (file) | 85 KB | Dgary | Figure 3 for Total Power Calibration document | 1 | |
15:11, 15 August 2016 | EOVSA 27-m Receiver Block Diagram.JPG (file) | 83 KB | Dgary | 1 | ||
15:46, 15 August 2016 | Starburst LO DCM Block Diagram.pdf (file) | 89 KB | Dgary | Ryan Monroe's block diagram for Starburst | 1 | |
15:47, 15 August 2016 | Starburst system diagram.pdf (file) | 159 KB | Dgary | James Lamb's version of the starburst block diagram | 1 | |
15:48, 15 August 2016 | Starburst fengine packet format.pdf (file) | 70 KB | Dgary | Starburst F-Engine packet format | 1 | |
15:48, 15 August 2016 | Starburst xengine packet format.pdf (file) | 120 KB | Dgary | Starburst X-Engine packet format | 1 | |
20:43, 18 September 2016 | Ant8 PvsV.png (file) | 36 KB | Dgary | Plot of Power vs. Voltage for the Ant8 front end | 1 | |
18:15, 21 September 2016 | Del centr f1.png (file) | 38 KB | Gfleishman | 1 | ||
18:15, 21 September 2016 | Del centr f2.png (file) | 131 KB | Gfleishman | 1 | ||
18:15, 21 September 2016 | Del centr f3.png (file) | 198 KB | Gfleishman | 1 | ||
14:53, 24 September 2016 | Eovsa calib sources.jpg (file) | 134 KB | Bchen | 1 | ||
20:47, 24 September 2016 | Figure1.jpg (file) | 104 KB | Ztwang | 1 | ||
21:00, 24 September 2016 | Linear to Circular Conversion Figure2.jpg (file) | 82 KB | Ztwang | 1 | ||
21:04, 24 September 2016 | Linear to Circular Conversion Figure3.jpg (file) | 118 KB | Ztwang | 1 | ||
21:04, 24 September 2016 | Linear to Circular Conversion Figure4.jpg (file) | 141 KB | Ztwang | 1 | ||
21:05, 24 September 2016 | Linear to Circular Conversion Figure5.jpg (file) | 138 KB | Ztwang | 1 | ||
17:56, 25 September 2016 | Image1.png (file) | 82 KB | Ychai | Schematic representation of frequency tuning for EOVSA, showing tuning to four of the 34 RF bands. From top to bottom they are: 1.5-2 GHz, 3.5-4 GHz, 7.5-8 GHz, and 17.5-18 GHz. | 1 | |
18:29, 25 September 2016 | Image7.png (file) | 338 KB | Ychai | Figure 6: Direct (not normalized) spectrum for 140 MHz around the strongest RFI in Figure 5(a). The details of the RFI match the strong Sprint PCS RFI near 1.925 GHz, so that it can confidently be identified as second-harmonic distortion from that sou... | 1 | |
18:40, 25 September 2016 | Image8.png (file) | 297 KB | Ychai | Figure 7: Direct (not normalized) spectrum for roughly the same region as in Figure 6, but now with the optical link supposedly centered on its linear range. The second-harmonic distortion is now much reduced, but certainly not eliminated. We can do... | 1 | |
18:43, 25 September 2016 | Image5.png (file) | 694 KB | Ychai | 1 | ||
18:50, 25 September 2016 | Image6.png (file) | 569 KB | Ychai | 1 | ||
18:52, 25 September 2016 | Image2.png (file) | 46 KB | Ychai | 1 | ||
18:52, 25 September 2016 | Image3.png (file) | 41 KB | Ychai | 1 | ||
18:53, 25 September 2016 | Image4.png (file) | 34 KB | Ychai | 1 | ||
00:50, 26 September 2016 | 4.pdf (file) | 149 KB | Schhabra | 1 | ||
01:00, 26 September 2016 | 1.png (file) | 277 KB | Schhabra | 1 | ||
03:45, 27 September 2016 | Figure 1.png (file) | 127 KB | Yjluo | 4 | ||
04:01, 27 September 2016 | Figure 2.png (file) | 57 KB | Yjluo | 1 | ||
04:20, 27 September 2016 | Spectrogram.png (file) | 164 KB | Sshaik | 1 | ||
14:56, 27 September 2016 | 2.png (file) | 15 KB | Schhabra | 1 | ||
14:56, 27 September 2016 | 3.png (file) | 72 KB | Schhabra | 1 | ||
14:57, 27 September 2016 | 4.png (file) | 32 KB | Schhabra | 1 | ||
15:23, 27 September 2016 | 5.png (file) | 19 KB | Schhabra | 1 | ||
15:23, 27 September 2016 | 6.png (file) | 20 KB | Schhabra | 1 | ||
15:24, 27 September 2016 | 7.png (file) | 15 KB | Schhabra | 1 | ||
01:19, 28 September 2016 | New telescope mount.png (file) | 4.24 MB | Sjyu | Figure 1: The new mount for the optical telescope, to be put in place of the radio front-end receiver. This should greatly reduce vibrations that lead to non-circular stars. | 1 | |
02:48, 16 October 2016 | DownConversionDiagram 1120MHz.png (file) | 41 KB | Dgary | Bandpass if we use an 1120 MHz ADC clock speed | 1 | |
13:53, 20 October 2016 | 3C84 chi-rotation.png (file) | 148 KB | Dgary | Observation and simulation of 3C84 feed-rotation effect, applying 2*chi | 1 | |
13:54, 20 October 2016 | 3C84 abs-chi-rotation.png (file) | 148 KB | Dgary | Observation and simulation of 3C84, applying 2*abs(chi) rotation | 1 | |
13:54, 20 October 2016 | 3C273 abs-chi-rotation.png (file) | 66 KB | Dgary | Observation and simulation of 3C273, applying 2*abs(chi) rotation | 1 |