Popular

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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246630 matches
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IRIS: SST coordination: quiet sun

2019-06-09T07:14:30 to 2019-06-09T12:29:50

Science Goal: Large dense 4-step raster 1x120 4s Si IV Mg II h/k Deep x 4 Spatial x 2, Spectral x 2 SJI cadence 3x faster Lossless compression

Program: SST coordination: quiet sun

Target: QS

Pointing: xcen=0 ycen=-600,

saaIntervals hiIntervals

wavelength	cadence	FOVx,y	images
1400	0.17	123,129	1840
2796	0.17	123,129	1840

IRIS: HOP 336, South Pointing 3/3

2019-05-20T05:01:53 to 2019-05-20T05:50:45

Science Goal: Large dense 320-step raster 105.3x120 320s Deep x 8 Spatial x 2, Spectral x 2

Program: HOP 336, South Pointing 3/3

Target: QS

Pointing: xcen=101 ycen=-575,

saaIntervals hiIntervals

wavelength	cadence	FOVx,y	images
1330	0.61	234,129	80
2832	0.61	234,129	80
1400	0.61	234,129	80
2796	0.61	234,129	80

IRIS: HOP 307 (IRIS only), AR 12741

2019-05-13T00:24:50 to 2019-05-13T01:51:15

Science Goal: Very large dense 320-step raster 105.3x175 320s Deep x 15 Spatial x 2, Spectral x 2

Program: HOP 307 (IRIS only), AR 12741

Target: AR

Pointing: xcen=2 ycen=131,

saaIntervals hiIntervals

wavelength	cadence	FOVx,y	images
1330	1.08	281,182	80
2832	1.08	281,182	80
1400	1.08	281,182	80
2796	1.08	281,182	80

IRIS: SST coordination, AR 12740

2019-05-08T07:29:24 to 2019-05-08T12:00:56

Science Goal: Medium dense 64-step raster 20.8x60 64s Mg II h/k Mg II w s Deep x 2 FUV spectrally rebinned x 4 Lossless compression

Program: SST coordination, AR 12740

Target: AR

Pointing: xcen=-382 ycen=201,

saaIntervals hiIntervals

wavelength	cadence	FOVx,y	images
2832	0.83	82,65	328
2796	0.21	82,65	1311

IRIS: A1: QS monitoring

2019-05-04T04:42:06 to 2019-05-04T05:00:10

Science Goal: Large coarse 64-step raster 126x120 64s C II Si IV Mg II h/k Mg II w s Deep x 15 SJI cadence 0.5x faster

Program: A1: QS monitoring

Target: QS

Pointing: xcen=-2 ycen=1,

saaIntervals hiIntervals

wavelength	cadence	FOVx,y	images
1330	1.13	247,129	16
2832	4.52	247,129	4
1400	1.13	247,129	16
2796	1.13	247,129	16

IRIS: A1: QS monitoring

2019-04-28T04:25:07 to 2019-04-28T04:43:10

Science Goal: Large coarse 64-step raster 126x120 64s C II Si IV Mg II h/k Mg II w s Deep x 15 SJI cadence 0.5x faster

Program: A1: QS monitoring

Target: QS

Pointing: xcen=-2 ycen=0,

saaIntervals hiIntervals

wavelength	cadence	FOVx,y	images
1330	1.13	247,129	16
2832	4.52	247,129	4
1400	1.13	247,129	16
2796	1.13	247,129	16

IRIS: B2: QS tracking from limb to limb (AR12739)

2019-04-21T05:30:52 to 2019-04-21T05:40:27

Science Goal: Coarse synoptic raster 34x175 18s Deep x 30 SJI cadence 3x faster Lossless compression

Program: B2: QS tracking from limb to limb (AR12739)

Target: QS

Pointing: xcen=861 ycen=-97,

saaIntervals hiIntervals

wavelength	cadence	FOVx,y	images
1330	3.2	203,182	3
2832	3.2	203,182	3
1400	3.2	203,182	3
2796	3.2	203,182	3

IRIS: Filament tracking

2019-04-18T18:00:43 to 2019-04-18T22:38:31

Science Goal: Large dense 320-step raster 105.3x120 320s Deep x 2 Spatial x 2, Spectral x 2 FUV spectrally rebinned x 4

Program: Filament tracking

Target: FI

Pointing: xcen=317 ycen=473,

saaIntervals hiIntervals

wavelength	cadence	FOVx,y	images
1330	0.2	234,128	1360
2832	0.2	234,128	1360
1400	0.2	234,128	1360
2796	0.2	234,128	1360

IRIS: C1: South Pole

2019-04-06T05:59:12 to 2019-04-06T06:33:23

Science Goal: Very large coarse 64-step raster 126x175 64s Deep x 30

Program: C1: South Pole

Target: CH

Pointing: xcen=6 ycen=-950,

saaIntervals hiIntervals

wavelength	cadence	FOVx,y	images
1330	2.14	295,182	16
2832	2.14	295,182	16
1400	2.14	295,182	16
2796	2.14	295,182	16

IRIS: HOP 366: PSP coordination (SP)

2019-04-04T11:05:09 to 2019-04-04T11:25:26

Science Goal: Very large coarse 2-step raster 2x175 2s Si IV Mg II h/k Deep x 8 Spatial x 2, Spectral x 2

Program: HOP 366: PSP coordination (SP)

Target: QS

Pointing: xcen=-275 ycen=-918,

saaIntervals hiIntervals

wavelength	cadence	FOVx,y	images
1400	0.31	171,182	65
2796	0.31	171,182	65

IRIS: HOP 369: Polar jet studies

2019-04-03T09:44:20 to 2019-04-03T11:02:51

Science Goal: Large sparse 64-step raster 63x120 64s Si IV Mg II h/k Deep x 8 Spatial x 2, Spectral x 2

Program: HOP 369: Polar jet studies

Target: CH

Pointing: xcen=40 ycen=-846,

saaIntervals hiIntervals

wavelength	cadence	FOVx,y	images
1400	0.31	185,129	256
2796	0.31	185,129	256

IRIS: Plume region at the North Pole

2019-03-09T06:27:19 to 2019-03-09T12:13:35

Science Goal: Very large dense 320-step raster 105.3x175 320s Deep x 15 Spatial x 2, Spectral x 2

Program: Plume region at the North Pole

Target: CH

Pointing: xcen=-4 ycen=935,

saaIntervals hiIntervals

wavelength	cadence	FOVx,y	images
1330	1.08	281,182	320
2832	1.08	281,182	320
1400	1.08	281,182	320
2796	1.08	281,182	320

IRIS: HOP 307: Long-term AR evolution, day 2

2019-03-08T04:48:23 to 2019-03-08T06:17:04

Science Goal: Very large dense 320-step raster 105.3x175 320s Deep x 15 Lossless compression

Program: HOP 307: Long-term AR evolution, day 2

Target: AR

Pointing: xcen=42 ycen=287,

saaIntervals hiIntervals

wavelength	cadence	FOVx,y	images
1330	1.11	281,182	80
2832	1.11	281,182	80
1400	1.11	281,182	80
2796	1.11	281,182	80

IRIS: HOP 269, Filament tracking

2019-02-26T04:19:20 to 2019-02-26T08:51:01

Science Goal: Very large dense 400-step raster 131.7x175 400s Deep x 4 Spatial x 2, Spectral x 2

Program: HOP 269, Filament tracking

Target: FI

Pointing: xcen=955 ycen=200,

saaIntervals hiIntervals

wavelength	cadence	FOVx,y	images
1330	0.34	309,182	800
2832	0.34	309,182	800
1400	0.34	309,182	800
2796	0.34	309,182	800

IRIS: F1: HOP 336, pointing #3

2019-02-11T14:38:01 to 2019-02-11T15:27:54

Science Goal: Large dense 320-step raster 105.3x120 320s Deep x 8 FUV spectrally rebinned x 2

Program: F1: HOP 336, pointing #3

Target: QS

Pointing: xcen=97 ycen=718,

saaIntervals hiIntervals

wavelength	cadence	FOVx,y	images
1330	0.62	233,129	80
2832	0.62	233,129	80
1400	0.62	233,129	80
2796	0.62	233,129	80

246630 matches
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