Heliophysics Events Knowledgebase Coverage Registry (HCR)
 
Popular Observations
Here are the most popular observations, as measured by the number of downloads.
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249801 matches
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IRIS: 16 step raster, ephemeral region
2014-07-18T12:00:00 to 2014-07-18T16:11:55
Science Goal: Very large coarse 16-step raster 30x175 16s Si IV Mg II h/k Mg II w s Deep x 4 FUV spectrally rebinned x 2
Program: 16 step raster, ephemeral region
Target: AR
Pointing: xcen=-579 ycen=-328,
saaIntervals hiIntervals
wavelengthcadenceFOVx,yimages
28320.7199,182361
14000.23199,1821082
27960.17199,1821442
IRIS: Wobble Test At -45
2014-05-17T20:42:21 to 2014-05-18T00:02:21
Science Goal: SJI MgIIw (10s exp) and SiIV (6s exp), 20s cad, for wobble calibration
Program: Wobble Test At -45
Target: (NONE)
Pointing: xcen=662 ycen=665,
saaIntervals hiIntervals
wavelengthcadenceFOVx,yimages
28320.33174,182599
14000.33174,182600
IRIS: IHOP 254, prominence dynamics
2014-04-26T01:00:36 to 2014-04-26T03:48:14
Science Goal: Large sparse 4-step raster 3x120 4s Si IV Mg II h/k Deep x 4 FUV spectrally rebinned x 2
Program: IHOP 254, prominence dynamics
Target: FI
Pointing: xcen=854 ycen=451,
saaIntervals hiIntervals
wavelengthcadenceFOVx,yimages
14000.18124,129939
27960.18124,129940
IRIS: Flare watch at AR 11990
2014-02-28T17:09:29 to 2014-02-28T22:12:06
Science Goal: Medium sparse 16-step raster 15x60 16s C II Si IV Deep x 15 Spatial x 2, Spectral x 2
Program: Flare watch at AR 11990
Target: AR
Pointing: xcen=-435 ycen=-107,
saaIntervals hiIntervals
wavelengthcadenceFOVx,yimages
13300.5475,69560
14000.5475,69559
IRIS: AR11934 raster scan: HINODE coordination
2013-12-27T22:38:08 to 2013-12-27T23:11:59
Science Goal: Very large dense raster 131.7x175 400s Si IV Mg II h/k Deep x 4 FUV spectrally rebinned x 2
Program: AR11934 raster scan: HINODE coordination
Target: AR
Pointing: xcen=338 ycen=-267,
saaIntervals hiIntervals
wavelengthcadenceFOVx,yimages
14000.17308,182200
27960.17308,182200
IRIS: Coronal Hole Boundary near limb
2013-12-16T00:06:29 to 2013-12-16T01:00:09
Science Goal: Very large sit-and-stare 0.3x175 1s C II Si IV Mg II h/k Mg II w s Deep x 8 FUV spectrally rebinned x 2
Program: Coronal Hole Boundary near limb
Target: CH
Pointing: xcen=806 ycen=352,
saaIntervals hiIntervals
wavelengthcadenceFOVx,yimages
13300.54169,182100
28322.68169,18220
14000.45169,182119
27960.45169,182120
IRIS: NS Fan in Plage (no #)
2013-12-05T13:41:38 to 2013-12-05T14:35:50
Science Goal: Large sit-and-stare 0.3x120 1s C II Si IV Mg II h/k Mg II w s Deep x 8 FUV spectrally rebinned x 2
Program: NS Fan in Plage (no #)
Target: FA
Pointing: xcen=87 ycen=-267,
saaIntervals hiIntervals
wavelengthcadenceFOVx,yimages
13300.54121,129100
28322.71121,12920
14000.45121,129120
27960.45121,129120
IRIS: Shock wave study above AR
2013-10-16T13:20:00 to 2013-10-16T15:24:37
Science Goal: Very large sit-and-stare 0.3x175 1s C II Si IV Mg II h/k Deep x 15 FUV spectrally rebinned x 2
Program: Shock wave study above AR
Target: AR
Pointing: xcen=990 ycen=152,
saaIntervals hiIntervals
wavelengthcadenceFOVx,yimages
13300.83169,182150
14000.83169,182150
27960.83169,182150
IRIS: throughput monitoring, N of disk center due to plage
2013-08-30T04:40:14 to 2013-08-30T04:57:20
Science Goal: Large coarse raster 126"x120" 64s C II Si IV Mg II h/k Mg II w s Deep x 15 SJI cadence 0.5x faster
Program: throughput monitoring, N of disk center due to plage
Target: (NONE)
Pointing: xcen=27 ycen=266,
saaIntervals hiIntervals
wavelengthcadenceFOVx,yimages
13301.07251,12816
28324.27251,1283
14001.14251,12815
27961.14251,12815
IRIS: Very large sparse raster 127"x175" 128s C II Si IV Mg II h/k Mg II w s Deep x 30 FUV spectrally rebinned x 4
2013-08-17T07:39:04 to 2013-08-17T08:45:00
Science Goal: Very large sparse raster 127"x175" 128s C II Si IV Mg II h/k Mg II w s Deep x 30 FUV spectrally rebinned x 4
Program: AR11817, AEC test 2, AF, FF
Target: (NONE)
Pointing: xcen=667 ycen=-397,
saaIntervals hiIntervals
wavelengthcadenceFOVx,yimages
13302.06299,18232
28328.24299,1828
14002.06299,18232
27962.06299,18232
IRIS: Very large dense raster 132"x175" 400s C II Si IV Mg II h/k Mg II w s Deep x 4 FUV spectrally rebinned x 2
2013-08-10T17:12:34 to 2013-08-10T17:45:51
Science Goal: Very large dense raster 132"x175" 400s C II Si IV Mg II h/k Mg II w s Deep x 4 FUV spectrally rebinned x 2
Program: AR 11809 near limb
Target: (NONE)
Pointing: xcen=787 ycen=176,
saaIntervals hiIntervals
wavelengthcadenceFOVx,yimages
13300.35312,18296
28322.09312,18216
14000.35312,18296
27960.35312,18296
IRIS: HOP 307 at AR 12941
2022-02-11T17:36:21 to 2022-02-11T18:25:18
Science Goal: Very large dense 320-step raster 105.3x175 320s Deep x 8 Spatial x 2, Spectral x 2
Program: HOP 307 at AR 12941
Target: AR
Pointing: xcen=366 ycen=489,
saaIntervals hiIntervals
wavelengthcadenceFOVx,yimages
13300.61281,18280
28320.61281,18280
14000.61281,18280
27960.61281,18280
IRIS: BBSO Coord: Flares and Small-scale Events
2021-04-19T17:00:00 to 2021-04-19T23:00:30
Science Goal: Large coarse 8-step raster 14x120 8s C II Si IV Mg II h/k Mg II w s Deep x 4 Spatial x 2, Spectral x 2 FUV spectrally rebinned x 4 SJI cadence 0.5x faster
Program: BBSO Coord: Flares and Small-scale Events
Target: AR
Pointing: xcen=-348 ycen=-284,
saaIntervals hiIntervals
wavelengthcadenceFOVx,yimages
13300.34137,1291068
28322.03137,129178
14000.34137,1291068
27960.34137,1291068
IRIS: Mercury Transit #9/9
2019-11-11T17:37:17 to 2019-11-11T18:12:15
Science Goal: Very large sit-and-stare 0.3x175 1s Si IV Mg II h/k Deep x 4 FUV spectrally rebinned x 4 SJI cadence 10x faster Lossless compression
Program: Mercury Transit #9/9
Target: (NONE)
Pointing: xcen=958 ycen=112,
saaIntervals hiIntervals
wavelengthcadenceFOVx,yimages
14000.17169,182200
27960.17169,182200
IRIS: Nes AR in East, like HOP 307
2017-07-20T01:39:50 to 2017-07-20T03:08:32
Science Goal: Very large dense 320-step raster 105.3x175 320s Deep x 15
Program: Nes AR in East, like HOP 307
Target: AR
Pointing: xcen=-763 ycen=17,
saaIntervals hiIntervals
wavelengthcadenceFOVx,yimages
13301.11281,18280
28321.11281,18280
14001.11281,18280
27961.11281,18280

249801 matches
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