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Date Name Thumbnail descSize User Description Versions
08:14, 13 September 2018 2110.gif (file) 6.41 MB Yjluo   1
23:36, 13 September 2018 2008ty3.gif (file) 4.58 MB Yjluo   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
06:46, 13 September 2018 1943.gif (file) 3.87 MB Yjluo   2
17:40, 8 August 2018 2047spw7.png (file) 1.64 MB Yjluo   1
21:12, 11 January 2017 EOVSA Status Jan 2017.pptx (file) 1.52 MB Dgary Report of X-Y delay issues at EOVSA 1
12:09, 21 September 2018 190703.gif (file) 1.49 MB SJaniak   4
04:05, 19 July 2017 Overview image.png (file) 1.38 MB Yjluo   1
04:23, 24 July 2018 191718.gif (file) 1.32 MB SJaniak   2
04:23, 24 July 2018 194100.gif (file) 1.09 MB SJaniak   2
17:39, 8 August 2018 2047spw6.png (file) 1.07 MB Yjluo   1
20:57, 23 November 2017 Svplot.png (file) 1.06 MB Yjluo   1
15:41, 5 October 2018 VLA Pband 20181002.png (file) 983 KB Bchen Cross-power dynamic spectrum for VLA P band test observation on 2018 Oct 2. 1
03:52, 24 July 2018 184450.gif (file) 837 KB SJaniak Reverted to version as of 03:46, 24 July 2018 5
14:02, 11 April 2018 1943.png (file) 782 KB Yjluo   1
18:40, 15 May 2019 Fig-browser.png (file) 725 KB Bchen Screenshot for viewing EOVSA all-day summary plot in RHESSI browser 1
15:28, 19 July 2019 Fig-tp calqual.png (file) 711 KB Bchen Quality of total-power calibration 1
18:43, 25 September 2016 Image5.png (file) 694 KB Ychai   1
21:06, 31 July 2018 2008gs.png (file) 684 KB Yjluo   1
04:11, 5 June 2018 2158 2201.png (file) 674 KB SJaniak   1
04:10, 5 June 2018 1844 1848.png (file) 667 KB SJaniak   1
04:10, 5 June 2018 1942 1949.png (file) 663 KB SJaniak   1
22:57, 19 May 2019 Fig-specmovie.png (file) 660 KB Sjyu   2
17:46, 25 April 2018 2008ty3.png (file) 654 KB Yjluo   2
04:09, 5 June 2018 1807 1810.png (file) 581 KB SJaniak   1
15:54, 11 April 2018 2110.png (file) 578 KB Yjluo   6
15:42, 13 February 2019 VLA Pband 20190125.png (file) 573 KB Sjyu   2
18:50, 25 September 2016 Image6.png (file) 569 KB Ychai   1
15:06, 13 February 2019 VLA Pband 20190104 1.png (file) 563 KB Sjyu   2
13:21, 3 July 2018 1906 1910.png (file) 558 KB SJaniak   1
13:22, 3 July 2018 1917 1921.png (file) 557 KB SJaniak   1
17:46, 14 February 2019 VLA Pband 20181207.png (file) 554 KB Sjyu   1
13:20, 3 July 2018 1843 1846.png (file) 543 KB SJaniak   1
13:40, 24 May 2019 Fig-qlookplot1.png (file) 529 KB Bchen EOVSA quicklook imaging at selected time range and frequency range. Background shows SDO/AIA 171 angstrom image at the closest time. 1
04:11, 5 June 2018 2028 2031.png (file) 527 KB SJaniak   1
13:22, 3 July 2018 1939 1943.png (file) 526 KB SJaniak   1
15:05, 13 February 2019 VLA Pband 20190104 2.png (file) 509 KB Sjyu   1
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
18:28, 20 September 2017 Details2.png (file) 488 KB Yjluo   1
19:54, 16 November 2016 Cal src vis.png (file) 484 KB Nkuroda Produced by dg_src_visibility for 2016-10-14, minflux = 4.0 and for 24 hours. 1
00:09, 19 May 2019 Fig-qlookplot mbds.png (file) 479 KB Sjyu   2
00:08, 19 May 2019 Fig-qlookplot2.png (file) 470 KB Sjyu   2
12:48, 20 May 2019 Fig-qlookplot3.png (file) 463 KB Bchen Fix GOES plot date. 2
02:31, 12 February 2019 VLA Pband 20181118 2.png (file) 453 KB Sjyu   1
16:10, 11 November 2018 Slf t0 n0.png (file) 451 KB Dgary   1
16:10, 11 November 2018 Slf t0 n2.png (file) 402 KB Dgary   1
18:18, 20 September 2017 Details1.PNG (file) 376 KB Yjluo   3
18:26, 20 September 2017 Details1.png (file) 376 KB Yjluo   1
06:36, 18 May 2017 2017-04-05 1430-1900 selfcal White AIA171.png (file) 356 KB Nkuroda   2
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

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