YEAR: 2010

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StartStopStudyX-cenY-cenObs. Title
01:36:4101:41:48VHH_HI_BRT_SCAN 869.1 -324.8Chromosphere corona connection, line asymmetry due to spicule type
01:41:5101:46:57VHH_HI_BRT_SCAN 869.0 -324.9Chromosphere corona connection, line asymmetry due to spicule type
01:47:0001:52:07VHH_HI_BRT_SCAN 869.1 -324.9Chromosphere corona connection, line asymmetry due to spicule type
01:52:1001:57:17VHH_HI_BRT_SCAN 869.0 -324.9Chromosphere corona connection, line asymmetry due to spicule type
01:57:2002:00:24VHH_HI_BRT_SCAN 869.0 -324.8Chromosphere corona connection, line asymmetry due to spicule type
02:31:2402:33:26VHH_HI_BRT_SCAN 866.3 -336.0Chromosphere corona connection, line asymmetry due to spicule type
03:14:4404:22:49VHH_SlowAR_1h12_V2 868.3 -324.9Chromosphere-corona conection, line asymmetries due to spicule type
04:56:5105:01:34VHH_SlowAR_5m_V2 856.1 -325.1Chromosphere-corona connection, line asymmetries due to type II spi
06:49:3107:48:05Atlas_60 177.7 210.6EIS Spectral Atlas Synoptic Program
08:55:2609:00:10VHH_SlowAR_5m_V2 394.7 243.5Chromosphere-corona connection, line asymmetries due to type II spi
09:49:1010:57:15VHH_SlowAR_1h12_V2 409.1 243.6Chromosphere-corona conection, line asymmetries due to spicule type
11:27:4011:32:47VHH_HI_BRT_SCAN 408.6 243.4Chromosphere corona connection, line asymmetry due to spicule type
11:32:5011:37:57VHH_HI_BRT_SCAN 408.6 243.5Chromosphere corona connection, line asymmetry due to spicule type
11:38:0011:43:07VHH_HI_BRT_SCAN 408.6 243.4Chromosphere corona connection, line asymmetry due to spicule type
11:43:1011:48:16VHH_HI_BRT_SCAN 408.5 243.4Chromosphere corona connection, line asymmetry due to spicule type
11:48:1911:53:26VHH_HI_BRT_SCAN 408.4 243.6Chromosphere corona connection, line asymmetry due to spicule type
11:53:2911:58:36VHH_HI_BRT_SCAN 408.4 243.5Chromosphere corona connection, line asymmetry due to spicule type
11:58:3912:03:46VHH_HI_BRT_SCAN 408.4 243.4Chromosphere corona connection, line asymmetry due to spicule type
12:03:4912:08:56VHH_HI_BRT_SCAN 408.4 243.4Chromosphere corona connection, line asymmetry due to spicule type
12:08:5912:14:06VHH_HI_BRT_SCAN 408.3 243.4Chromosphere corona connection, line asymmetry due to spicule type
12:14:0912:19:16VHH_HI_BRT_SCAN 408.3 243.3Chromosphere corona connection, line asymmetry due to spicule type
12:19:1912:24:26VHH_HI_BRT_SCAN 408.3 243.3Chromosphere corona connection, line asymmetry due to spicule type
12:24:2912:29:35VHH_HI_BRT_SCAN 408.2 243.4Chromosphere corona connection, line asymmetry due to spicule type
13:06:1014:14:15VHH_SlowAR_1h12_V2 407.6 243.3Chromosphere-corona conection, line asymmetries due to spicule type
14:50:1315:58:17VHH_SlowAR_1h12_V2 407.0 243.2Chromosphere-corona conection, line asymmetries due to spicule type
16:38:4316:43:49VHH_HI_BRT_SCAN 406.5 243.0Chromosphere corona connection, line asymmetry due to spicule type
16:43:5216:48:59VHH_HI_BRT_SCAN 406.5 243.0Chromosphere corona connection, line asymmetry due to spicule type
16:49:0216:54:09VHH_HI_BRT_SCAN 406.4 243.0Chromosphere corona connection, line asymmetry due to spicule type
16:54:1216:59:19VHH_HI_BRT_SCAN 406.3 243.1Chromosphere corona connection, line asymmetry due to spicule type
16:59:2217:04:29VHH_HI_BRT_SCAN 406.3 242.9Chromosphere corona connection, line asymmetry due to spicule type
17:04:3217:09:38VHH_HI_BRT_SCAN 406.2 242.9Chromosphere corona connection, line asymmetry due to spicule type
17:09:4117:14:48VHH_HI_BRT_SCAN 406.2 243.0Chromosphere corona connection, line asymmetry due to spicule type
17:14:5117:19:58VHH_HI_BRT_SCAN 406.2 243.0Chromosphere corona connection, line asymmetry due to spicule type
18:15:3318:17:03SYNOP005_A -81.3 10.9Synoptic 005
18:17:1418:18:44SYNOP005_A -62.2 6.8Synoptic 005
18:49:4018:54:24VHH_SlowAR_5m_V2 389.8 242.8Chromosphere-corona connection, line asymmetries due to type II spi
19:52:4021:00:45VHH_SlowAR_1h12_V2 404.8 242.7Chromosphere-corona conection, line asymmetries due to spicule type
22:10:4022:15:24VHH_SlowAR_5m_V2 388.0 242.7Chromosphere-corona connection, line asymmetries due to type II spi
22:57:4000:05:44VHH_SlowAR_1h12_V2 403.7 242.5Chromosphere-corona conection, line asymmetries due to spicule type