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Combined display of all available logs of EOVSA Wiki. You can narrow down the view by selecting a log type, the username (case-sensitive), or the affected page (also case-sensitive).
(newest | oldest) View (newer 20 | older 20) (20 | 50 | 100 | 250 | 500)- 15:23, 27 September 2016 Schhabra talk contribs uploaded File:6.png
- 15:23, 27 September 2016 Schhabra talk contribs uploaded File:5.png
- 14:57, 27 September 2016 Schhabra talk contribs uploaded File:4.png
- 14:56, 27 September 2016 Schhabra talk contribs uploaded File:3.png
- 14:56, 27 September 2016 Schhabra talk contribs uploaded File:2.png
- 04:20, 27 September 2016 Sshaik talk contribs uploaded File:Spectrogram.png
- 04:01, 27 September 2016 Yjluo talk contribs uploaded File:Figure 2.png
- 03:45, 27 September 2016 Yjluo talk contribs uploaded a new version of File:Figure 1.png
- 03:38, 27 September 2016 Yjluo talk contribs uploaded a new version of File:Figure 1.png
- 03:38, 27 September 2016 Yjluo talk contribs uploaded a new version of File:Figure 1.png
- 02:36, 27 September 2016 Yjluo talk contribs uploaded File:Figure 1.png (Figure 1: Summary of EOVSA computers, labeled with their function, and network hostname in parentheses. All hostnames are on solar.pvt except the Gateway computer (the web server, which has two aliases, ovsa.njit.edu and ovsa.solar.ovro.caltech.edu)....)
- 01:00, 26 September 2016 Schhabra talk contribs uploaded File:1.png
- 00:50, 26 September 2016 Schhabra talk contribs uploaded File:4.pdf
- 18:53, 25 September 2016 Ychai talk contribs uploaded File:Image4.png
- 18:52, 25 September 2016 Ychai talk contribs uploaded File:Image3.png
- 18:52, 25 September 2016 Ychai talk contribs uploaded File:Image2.png
- 18:50, 25 September 2016 Ychai talk contribs uploaded File:Image6.png
- 18:43, 25 September 2016 Ychai talk contribs uploaded File:Image5.png
- 18:40, 25 September 2016 Ychai talk contribs uploaded File:Image8.png (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...)
- 18:29, 25 September 2016 Ychai talk contribs uploaded File:Image7.png (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...)