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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250264 matches
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IRIS: Large dense 320-step raster for continuous monitoring of AR 12641

2017-03-05T00:52:21 to 2017-03-05T01:47:25

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

Program: Large dense 320-step raster for continuous monitoring of AR 12641

Target: AR

Pointing: xcen=334 ycen=364,

saaIntervals hiIntervals

wavelength	cadence	FOVx,y	images
1330	0.34	234,129	160
2832	0.34	234,129	160
1400	0.34	234,129	160
2796	0.34	234,129	160

IRIS: Large dense 320-step raster for continuous monitoring of AR 12641

2017-03-02T07:43:03 to 2017-03-02T08:38:07

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

Program: Large dense 320-step raster for continuous monitoring of AR 12641

Target: AR

Pointing: xcen=-224 ycen=370,

saaIntervals hiIntervals

wavelength	cadence	FOVx,y	images
1330	0.34	234,129	160
2832	0.34	234,129	160
1400	0.34	234,129	160
2796	0.34	234,129	160

IRIS: B2: QS tracking from limb to limb

2017-02-21T07:40:32 to 2017-02-21T07:50:07

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

Program: B2: QS tracking from limb to limb

Target: QS

Pointing: xcen=-51 ycen=-368,

saaIntervals hiIntervals

wavelength	cadence	FOVx,y	images
1330	3.2	204,182	3
2832	3.2	204,182	3
1400	3.2	204,182	3
2796	3.2	204,182	3

IRIS: C1: South Pole

2017-02-18T07:34:32 to 2017-02-18T08:08:42

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

Program: C1: South Pole

Target: CH

Pointing: xcen=6 ycen=-958,

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: IHOP 306 on AR12634 (IRIS only)

2017-02-10T21:23:43 to 2017-02-10T22:32:14

Science Goal: Large coarse 32-step raster 62x120 32s Deep x 4 FUV spectrally rebinned x 2

Program: IHOP 306 on AR12634 (IRIS only)

Target: AR

Pointing: xcen=-98 ycen=179,

saaIntervals hiIntervals

wavelength	cadence	FOVx,y	images
1330	0.36	183,129	192
2832	0.36	183,129	192
1400	0.36	183,129	192
2796	0.36	183,129	192

IRIS: High S/N sit and stare AR12630

2017-02-09T16:10:44 to 2017-02-09T17:19:09

Science Goal: Very large sit-and-stare 0.3x175 1s C II Si IV Mg II h/k Deep x 60 Lossless compression

Program: High S/N sit and stare AR12630

Target: AR

Pointing: xcen=950 ycen=230,

saaIntervals hiIntervals

wavelength	cadence	FOVx,y	images
1330	3.11	169,182	22
1400	3.11	169,182	22
2796	3.11	169,182	22

IRIS: AR 12630, deep exposures

2017-02-03T10:48:31 to 2017-02-03T11:47:36

Science Goal: Very large sit-and-stare 0.3x175 1s C II Si IV Mg II h/k Deep x 60 Lossless compression

Program: AR 12630, deep exposures

Target: AR

Pointing: xcen=-102 ycen=351,

saaIntervals hiIntervals

wavelength	cadence	FOVx,y	images
1330	3.11	169,182	19
1400	3.11	169,182	19
2796	3.11	169,182	19

IRIS: Rapid QS SJI

2017-01-20T04:19:20 to 2017-01-20T04:46:32

Science Goal: Very large coarse 2-step raster 2x175 2s Mg II h/k Mg II w Deep x 2 Spatial x 2, Spectral x 2 SJI cadence 10x faster

Program: Rapid QS SJI

Target: QS

Pointing: xcen=57 ycen=-201,

saaIntervals hiIntervals

wavelength	cadence	FOVx,y	images
2832	0.11	171,182	250
2796	0.11	171,182	250

IRIS: Prominence NE limb

2017-01-19T10:02:35 to 2017-01-19T11:01:24

Science Goal: Large coarse 16-step raster 30x120 16s Si IV Mg II h/k Deep x 30 FUV spectrally rebinned x 2

Program: Prominence NE limb

Target: FI

Pointing: xcen=-827 ycen=565,

saaIntervals hiIntervals

wavelength	cadence	FOVx,y	images
1400	1.05	151,130	56
2796	1.05	151,130	56

IRIS: Short term AR evolution (coordination with Hinode)

2017-01-14T14:52:27 to 2017-01-14T15:49:33

Science Goal: Large coarse 32-step raster 62x120 32s Deep x 4 FUV spectrally rebinned x 2

Program: Short term AR evolution (coordination with Hinode)

Target: AR

Pointing: xcen=-846 ycen=197,

saaIntervals hiIntervals

wavelength	cadence	FOVx,y	images
1330	0.36	183,130	160
2832	0.36	183,130	160
1400	0.36	183,130	160
2796	0.36	183,130	160

IRIS: A1: QS monitoring

2017-01-07T04:19:18 to 2017-01-07T04:37:22

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=41 ycen=-50,

saaIntervals hiIntervals

wavelength	cadence	FOVx,y	images
1330	1.13	247,130	16
2832	4.52	247,130	4
1400	1.13	247,130	16
2796	1.13	247,130	16

IRIS: Flare watch on AR12615

2016-12-01T06:54:32 to 2016-12-01T07:54:07

Science Goal: Medium coarse 8-step raster 14x60 8s C II Mg II h/k Mg II w Spatial x 2, Spectral x 2

Program: Flare watch on AR12615

Target: AR

Pointing: xcen=-545 ycen=-132,

saaIntervals hiIntervals

wavelength	cadence	FOVx,y	images
1330	0.29	71,68	209
2832	0.29	71,68	209
2796	0.29	71,68	209

IRIS: AR 12611 (HOP 306), high rate ver

2016-11-24T12:27:04 to 2016-11-24T13:20:37

Science Goal: Very large sparse 64-step raster 63x175 64s Deep x 15 Lossless compression

Program: AR 12611 (HOP 306), high rate ver

Target: AR

Pointing: xcen=532 ycen=22,

saaIntervals hiIntervals

wavelength	cadence	FOVx,y	images
1330	1.12	232,182	48
2832	1.12	232,182	48
1400	1.12	232,182	48
2796	1.12	232,182	48

IRIS: HOP 306, AR 12606

2016-11-06T09:01:49 to 2016-11-06T10:11:08

Science Goal: Large sparse 64-step raster 63x120 64s Deep x 15

Program: HOP 306, AR 12606

Target: AR

Pointing: xcen=-515 ycen=147,

saaIntervals hiIntervals

wavelength	cadence	FOVx,y	images
1330	1.08	184,128	64
2832	1.08	184,128	64
1400	1.08	184,128	64
2796	1.08	184,128	64

IRIS: Wobble calibration roll=90 deg, 300 rpts, pointing #1

2016-08-19T11:43:21 to 2016-08-19T13:23:21

Science Goal: SJI MgII w, 1x1, 10s exp, 20s cadence, for wobble calibration

Program: Wobble calibration roll=90 deg, 300 rpts, pointing #1

Target: (NONE)

Pointing: xcen=-918 ycen=-7,

saaIntervals hiIntervals

wavelength	cadence	FOVx,y	images
2832	0.33	173,182	300

250264 matches
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