Heliophysics Events Knowledgebase Coverage Registry (HCR)
 
Planned Observations
Here are observations that are scheduled to run in the next 24 hours. The resulting data may take a few days to appear in our system.

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208581 matches
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more detail
AIA,HMI: data
2016-06-08T17:03:00 to 2016-06-08T17:53:00
Science Goal: ssw_service_161206_022038_27897(SSW)
Program:
Target:
Pointing: xcen=480 ycen=250,
saaIntervals hiIntervals
wavelengthcadenceFOVx,yimages
more detail
SOTSP: HOP 311 w/DST Near Disk Center
2016-06-08T15:31:30 to 2016-06-08T16:35:00
Science Goal: Magnetic Flux Cancellation
Program: Fast Map, 20"x82", Q75 2-side CCD, repeat
Target: Quiet Sun
Pointing: xcen=324 ycen=182,
saaIntervals hiIntervals
wavelengthcadenceFOVx,yimages
more detail
SOTSP: HOP 311 w/DST Near Disk Center
2016-06-08T14:18:00 to 2016-06-08T14:57:00
Science Goal: Magnetic Flux Cancellation
Program: Fast Map, 20"x82", Q75 2-side CCD, repeat
Target: Quiet Sun
Pointing: xcen=324 ycen=182,
saaIntervals hiIntervals
wavelengthcadenceFOVx,yimages
more detail
SOTSP: HOP 311 w/DST Near Disk Center
2016-06-08T14:04:00 to 2016-06-08T14:18:00
Science Goal: Magnetic Flux Cancellation
Program: Fast Map, 50"x122", Q75 1-side CCD, Repeat 1
Target: Quiet Sun
Pointing: xcen=324 ycen=182,
saaIntervals hiIntervals
wavelengthcadenceFOVx,yimages
more detail
XRT: HOP311 2
2016-06-08T13:59:54 to 2016-06-08T17:56:24
Science Goal: AR_observation
Program: XOB:1B3C; AR - Standard Core - (Filter-Ratio with Al/poly and thin-Be long/short pairs) with PFB, 384x384 at 1064 1048, thin-Be, and Al/poly context, with G-band (3ms/3ms VLS=CLS), 60 cad-2 (1AFF)
Target: AR
Pointing: xcen=466 ycen=175,
saaIntervals hiIntervals
wavelengthcadenceFOVx,yimages
more detail
IRIS: IHOP 311: DST coordination (flux cancellation)
2016-06-08T13:59:15 to 2016-06-08T16:53:56
Science Goal: Large coarse 4-step raster 6x120 4s Si IV Mg II h/k Mg II w s Deep x 2 Spatial x 2, Spectral x 2
Program: IHOP 311: DST coordination (flux cancellation)
Target: EF
Pointing: xcen=331 ycen=238,
saaIntervals hiIntervals
wavelengthcadenceFOVx,yimages
more detail
IRIS: 400-step dense raster AR
2016-06-08T12:39:11 to 2016-06-08T13:40:33
Science Goal: Very large dense 400-step raster 131.7x175 400s Deep x 8 Spatial x 2, Spectral x 2
Program: 400-step dense raster AR
Target: AR
Pointing: xcen=-247 ycen=-376,
saaIntervals hiIntervals
wavelengthcadenceFOVx,yimages
more detail
SOTSP: Active Area Observations
2016-06-08T10:35:00 to 2016-06-08T11:40:00
Science Goal: Active Area Observations
Program: Normal 100"x122" Q75 one side
Target: disk center
Pointing: xcen=464 ycen=175,
saaIntervals hiIntervals
wavelengthcadenceFOVx,yimages
more detail
XRT: HOP300 2 woAUTO
2016-06-08T09:59:54 to 2016-06-08T13:59:54
Science Goal: AR_observation
Program: XOB:1AE7; AR - Standard Core - (Filter-Ratio with thin-Be and Med-Be long/short pairs) with PFB, 384x384 at 1064 1048, thin-Be, and Med-Be context, with G-band (3ms/3ms VLS=CLS), 90 cad (1B21)
Target: AR
Pointing: xcen=-293 ycen=357,
saaIntervals hiIntervals
wavelengthcadenceFOVx,yimages
more detail
IRIS: IHOP 300: SST coordination (small AR)
2016-06-08T09:47:32 to 2016-06-08T12:06:35
Science Goal: Large sparse 64-step raster 63x120 64s Si IV Mg II h/k Mg II w s Deep x 8 FUV spectrally rebinned x 2
Program: IHOP 300: SST coordination (small AR)
Target: AR
Pointing: xcen=-458 ycen=189,
saaIntervals hiIntervals
wavelengthcadenceFOVx,yimages
more detail
SOTSP: Coronal loop magnetic field determination and evolution through coronal rain tracing
2016-06-08T08:56:30 to 2016-06-08T09:59:35
Science Goal: Coronal loop magnetic field determination and evolution through coronal rain tracing
Program: Fast map, 123"x123", 1-side CCD
Target: disk center
Pointing: xcen=-292 ycen=356,
saaIntervals hiIntervals
wavelengthcadenceFOVx,yimages
more detail
AIA,HMI: Filaments304
2016-06-08T07:53:00 to 2016-06-10T07:52:00
Science Goal: ssw_service_180922_192803_19483(SSW)
Program:
Target:
Pointing: xcen=576 ycen=250,
saaIntervals hiIntervals
wavelengthcadenceFOVx,yimages
more detail
SOTSP: Coronal loop magnetic field determination and evolution through coronal rain tracing
2016-06-08T07:44:00 to 2016-06-08T08:23:30
Science Goal: Coronal loop magnetic field determination and evolution through coronal rain tracing
Program: Fast map, 123"x123", 1-side CCD
Target: disk center
Pointing: xcen=-292 ycen=356,
saaIntervals hiIntervals
wavelengthcadenceFOVx,yimages
more detail
XRT: HOP300 1
2016-06-08T07:39:54 to 2016-06-08T09:59:54
Science Goal: AR_observation
Program: XOB:1AFF; AR - Standard Core - (Filter-Ratio with thin-Be and Med-Be long/short pairs) with PFB, 384x384 at 1064 1048, thin-Be, and Med-Be context, with G-band (3ms/3ms VLS=CLS), 90 cad (1B21)
Target: AR
Pointing: xcen=0 ycen=0,
saaIntervals hiIntervals
wavelengthcadenceFOVx,yimages
more detail
XRT: Synoptic 1
2016-06-08T07:29:54 to 2016-06-08T07:39:54
Science Goal: Synoptic
Program: XOB:1B35; Synoptic Q95 2x2 - Al/mesh(12/181/1024) + Dark cal(2x2 4x4 8x8 512 Q98) + Dark cal(1x1 512x2048 - 1x1 2048x512) + Al-poly(24/362/1443) + Thin_Be(88/1024/5795ms) + G-band (VLS open 3ms closed 3ms Q95) (1B0A)
Target: FS
Pointing: xcen=-970 ycen=0,
saaIntervals hiIntervals
wavelengthcadenceFOVx,yimages

208581 matches
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