| Start | Stop | Study | X-cen | Y-cen | Obs. Title |
| 01:36:41 | 01:41:48 | VHH_HI_BRT_SCAN | 869.1 | -324.8 | Chromosphere corona connection, line asymmetry due to spicule type |
| 01:41:51 | 01:46:57 | VHH_HI_BRT_SCAN | 869.0 | -324.9 | Chromosphere corona connection, line asymmetry due to spicule type |
| 01:47:00 | 01:52:07 | VHH_HI_BRT_SCAN | 869.1 | -324.9 | Chromosphere corona connection, line asymmetry due to spicule type |
| 01:52:10 | 01:57:17 | VHH_HI_BRT_SCAN | 869.0 | -324.9 | Chromosphere corona connection, line asymmetry due to spicule type |
| 01:57:20 | 02:00:24 | VHH_HI_BRT_SCAN | 869.0 | -324.8 | Chromosphere corona connection, line asymmetry due to spicule type |
| 02:31:24 | 02:33:26 | VHH_HI_BRT_SCAN | 866.3 | -336.0 | Chromosphere corona connection, line asymmetry due to spicule type |
| 03:14:44 | 04:22:49 | VHH_SlowAR_1h12_V2 | 868.3 | -324.9 | Chromosphere-corona conection, line asymmetries due to spicule type |
| 04:56:51 | 05:01:34 | VHH_SlowAR_5m_V2 | 856.1 | -325.1 | Chromosphere-corona connection, line asymmetries due to type II spi |
| 06:49:31 | 07:48:05 | Atlas_60 | 177.7 | 210.6 | EIS Spectral Atlas Synoptic Program |
| 08:55:26 | 09:00:10 | VHH_SlowAR_5m_V2 | 394.7 | 243.5 | Chromosphere-corona connection, line asymmetries due to type II spi |
| 09:49:10 | 10:57:15 | VHH_SlowAR_1h12_V2 | 409.1 | 243.6 | Chromosphere-corona conection, line asymmetries due to spicule type |
| 11:27:40 | 11:32:47 | VHH_HI_BRT_SCAN | 408.6 | 243.4 | Chromosphere corona connection, line asymmetry due to spicule type |
| 11:32:50 | 11:37:57 | VHH_HI_BRT_SCAN | 408.6 | 243.5 | Chromosphere corona connection, line asymmetry due to spicule type |
| 11:38:00 | 11:43:07 | VHH_HI_BRT_SCAN | 408.6 | 243.4 | Chromosphere corona connection, line asymmetry due to spicule type |
| 11:43:10 | 11:48:16 | VHH_HI_BRT_SCAN | 408.5 | 243.4 | Chromosphere corona connection, line asymmetry due to spicule type |
| 11:48:19 | 11:53:26 | VHH_HI_BRT_SCAN | 408.4 | 243.6 | Chromosphere corona connection, line asymmetry due to spicule type |
| 11:53:29 | 11:58:36 | VHH_HI_BRT_SCAN | 408.4 | 243.5 | Chromosphere corona connection, line asymmetry due to spicule type |
| 11:58:39 | 12:03:46 | VHH_HI_BRT_SCAN | 408.4 | 243.4 | Chromosphere corona connection, line asymmetry due to spicule type |
| 12:03:49 | 12:08:56 | VHH_HI_BRT_SCAN | 408.4 | 243.4 | Chromosphere corona connection, line asymmetry due to spicule type |
| 12:08:59 | 12:14:06 | VHH_HI_BRT_SCAN | 408.3 | 243.4 | Chromosphere corona connection, line asymmetry due to spicule type |
| 12:14:09 | 12:19:16 | VHH_HI_BRT_SCAN | 408.3 | 243.3 | Chromosphere corona connection, line asymmetry due to spicule type |
| 12:19:19 | 12:24:26 | VHH_HI_BRT_SCAN | 408.3 | 243.3 | Chromosphere corona connection, line asymmetry due to spicule type |
| 12:24:29 | 12:29:35 | VHH_HI_BRT_SCAN | 408.2 | 243.4 | Chromosphere corona connection, line asymmetry due to spicule type |
| 13:06:10 | 14:14:15 | VHH_SlowAR_1h12_V2 | 407.6 | 243.3 | Chromosphere-corona conection, line asymmetries due to spicule type |
| 14:50:13 | 15:58:17 | VHH_SlowAR_1h12_V2 | 407.0 | 243.2 | Chromosphere-corona conection, line asymmetries due to spicule type |
| 16:38:43 | 16:43:49 | VHH_HI_BRT_SCAN | 406.5 | 243.0 | Chromosphere corona connection, line asymmetry due to spicule type |
| 16:43:52 | 16:48:59 | VHH_HI_BRT_SCAN | 406.5 | 243.0 | Chromosphere corona connection, line asymmetry due to spicule type |
| 16:49:02 | 16:54:09 | VHH_HI_BRT_SCAN | 406.4 | 243.0 | Chromosphere corona connection, line asymmetry due to spicule type |
| 16:54:12 | 16:59:19 | VHH_HI_BRT_SCAN | 406.3 | 243.1 | Chromosphere corona connection, line asymmetry due to spicule type |
| 16:59:22 | 17:04:29 | VHH_HI_BRT_SCAN | 406.3 | 242.9 | Chromosphere corona connection, line asymmetry due to spicule type |
| 17:04:32 | 17:09:38 | VHH_HI_BRT_SCAN | 406.2 | 242.9 | Chromosphere corona connection, line asymmetry due to spicule type |
| 17:09:41 | 17:14:48 | VHH_HI_BRT_SCAN | 406.2 | 243.0 | Chromosphere corona connection, line asymmetry due to spicule type |
| 17:14:51 | 17:19:58 | VHH_HI_BRT_SCAN | 406.2 | 243.0 | Chromosphere corona connection, line asymmetry due to spicule type |
| 18:15:33 | 18:17:03 | SYNOP005_A | -81.3 | 10.9 | Synoptic 005 |
| 18:17:14 | 18:18:44 | SYNOP005_A | -62.2 | 6.8 | Synoptic 005 |
| 18:49:40 | 18:54:24 | VHH_SlowAR_5m_V2 | 389.8 | 242.8 | Chromosphere-corona connection, line asymmetries due to type II spi |
| 19:52:40 | 21:00:45 | VHH_SlowAR_1h12_V2 | 404.8 | 242.7 | Chromosphere-corona conection, line asymmetries due to spicule type |
| 22:10:40 | 22:15:24 | VHH_SlowAR_5m_V2 | 388.0 | 242.7 | Chromosphere-corona connection, line asymmetries due to type II spi |
| 22:57:40 | 00:05:44 | VHH_SlowAR_1h12_V2 | 403.7 | 242.5 | Chromosphere-corona conection, line asymmetries due to spicule type |