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Here are the most popular observations, as measured by the number of downloads.
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257287 matches
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XRT: Synoptic Q90 2x2 18UT
2008-05-01T17:35:00 to 2008-05-01T19:11:02
Science Goal: Synoptic
Program: XOB:14DF; STOP and Synoptic - G-band(64) + Ti/poly(1024/11571) + dark cal(8192) + Al/poly(512/11571)
Target: FS
Pointing: xcen=-681 ycen=0,
saaIntervals hiIntervals
wavelengthcadenceFOVx,yimages
Open+Gband81,585,2,11413
XRT: G-Band monitoring of CCD
2008-04-18T17:31:42 to 2008-04-18T17:31:59
Science Goal: One-Week Campaign #4: Quiet Sun (to occur on disk, near center), WHI ToO #1: Active Regions, WHI ToO #2: Equatorial Coronal Hole Study, WHI ToO #3: Activity in Filaments and Filament Channels
Program: Spot_monitor_1
Target: QR
Pointing: xcen=-0 ycen=-0,
saaIntervals hiIntervals
wavelengthcadenceFOVx,yimages
Open+Be_thick0.081,053,1,0532
Open+Gband0.091,057,1,0572
EIS: Active region loop velocity
2008-04-01T11:28:18 to 2008-04-01T11:30:55
Science Goal: Very narrow context raster with 1" slit
Program:
Target:
Pointing: xcen=670 ycen=-81,
saaIntervals hiIntervals
wavelengthcadenceFOVx,yimages
OVI5,240null
FeXIII5,240null
FeX5,240null
CaXVII5,240null
FeXI5,240null
FeXV5,240null
FeXVII5,240null
MgVII5,240null
MgV5,240null
HeII5,240null
CaXV5,240null
FeXII5,240null
FeXIV5,240null
SOTSP: WHI Campaign
2008-03-24T14:36:05 to 2008-03-24T14:59:21
Science Goal: WHI One-Week Campaign #1: Linking the Corona to the Solar Wind at Ulysses (to occur at the NE limb of the Sun)
Program: Fast map, 60 arcsec, 4 cycle, 1-side CCD, no repeat
Target: Coronal Hole
Pointing: xcen=-7 ycen=-923,
saaIntervals hiIntervals
wavelengthcadenceFOVx,yimages
6302A Continuum Intensity063,162200
6302A Velocity 6301.5A063,162200
6302A Transverse Flux Density063,162200
6302A Longitudinal Flux Density063,162200
XRT: WHI South pole
2008-03-21T14:38:24 to 2008-03-21T17:12:27
Science Goal: WHI One-Week Campaign #1: Linking the Corona to the Solar Wind at Ulysses (to occur at the NE limb of the Sun), WHI ToO #1: Active Regions, WHI ToO #2: Equatorial Coronal Hole Study, WHI ToO #3: Activity in Filaments and Filament Channels
Program: WHI_South_Pole
Target: QR
Pointing: xcen=0 ycen=-930,
saaIntervals hiIntervals
wavelengthcadenceFOVx,yimages
Al_poly+Open56.02527,5272
XRT: Synoptic
2008-03-07T11:03:30 to 2008-03-07T18:22:26
Science Goal:
Program: Long_exp_synoptic_QS
Target: FS
Pointing: xcen=0 ycen=-1042,
saaIntervals hiIntervals
wavelengthcadenceFOVx,yimages
Be_thin+Open10.03527,52744
Open+Gband105528,5285
Al_poly+Open21527,52721
SOTSP: HOP 63 at S Pole
2008-01-29T07:36:06 to 2008-01-29T07:51:53
Science Goal: Magneto-acoustic shocks in the chromosphere and UV variability+Hinode Observations in Support of MOTH-II South Pole Observations
Program: fast map half ht 82"
Target: S Pole
Pointing: xcen=-5 ycen=-938,
saaIntervals hiIntervals
wavelengthcadenceFOVx,yimages
6302A Continuum Intensity079,81250
6302A Velocity 6301.5A079,81250
6302A Transverse Flux Density079,81250
6302A Longitudinal Flux Density079,81250
SOTSP: HOP 63 at E Limb
2008-01-27T14:05:37 to 2008-01-27T14:21:23
Science Goal: Magneto-acoustic shocks in the chromosphere and UV variability+Hinode Observations in Support of MOTH-II South Pole Observations
Program: HOP 63: Na D Doppler, Ca H, 16 sec cadence
Target: E Limb
Pointing: xcen=-950 ycen=7,
saaIntervals hiIntervals
wavelengthcadenceFOVx,yimages
6302A Continuum Intensity079,81250
6302A Velocity 6301.5A079,81250
6302A Transverse Flux Density079,81250
6302A Longitudinal Flux Density079,81250
SOTSP: HOP 58 coronal loop upflows
2008-01-15T10:32:05 to 2008-01-15T11:37:30
Science Goal: CORE/TOO: Measuring coronal outflows in coronal loops
Program: Fast map cyc 4 180x123 arcsec
Target: Active Region
Pointing: xcen=896 ycen=-72,
saaIntervals hiIntervals
wavelengthcadenceFOVx,yimages
6302A Continuum Intensity0178,122562
6302A Velocity 6301.5A0178,122562
6302A Transverse Flux Density0178,122562
6302A Longitudinal Flux Density0178,122562
SOTSP: HOP 58 coronal loop upflows
2008-01-15T07:07:04 to 2008-01-15T08:12:29
Science Goal: CORE/TOO: Measuring coronal outflows in coronal loops
Program: Fast map cyc 4 180x123 arcsec
Target: Active Region
Pointing: xcen=884 ycen=-70,
saaIntervals hiIntervals
wavelengthcadenceFOVx,yimages
6302A Continuum Intensity0178,122562
6302A Velocity 6301.5A0178,122562
6302A Transverse Flux Density0178,122562
6302A Longitudinal Flux Density0178,122562
SOTSP: HOP58 outflows in coronal loops
2008-01-10T16:04:58 to 2008-01-10T16:23:40
Science Goal: CORE/TOO: Measuring coronal outflows in coronal loops
Program: Fast map cyc4 180x164 arcsec
Target: Active Region
Pointing: xcen=9 ycen=-33,
saaIntervals hiIntervals
wavelengthcadenceFOVx,yimages
6302A Continuum Intensity047,162158
6302A Velocity 6301.5A047,162158
6302A Transverse Flux Density047,162158
6302A Longitudinal Flux Density047,162158
SOTSP: HOP57 penumbra dynamics, AR10981
2008-01-08T04:40:04 to 2008-01-08T05:23:31
Science Goal: Observation of dynamical activities in sunspot penumbrae
Program: Normal map 512x512
Target: Active Region
Pointing: xcen=306 ycen=527,
saaIntervals hiIntervals
wavelengthcadenceFOVx,yimages
6302A Continuum Intensity-181,81512
6302A Velocity 6301.5A-181,81512
6302A Transverse Flux Density-181,81512
6302A Longitudinal Flux Density-181,81512
SOTSP: transient brightening in AR
2008-01-06T18:39:28 to 2008-01-06T19:06:26
Science Goal: transient brightening in AR
Program: Fast map 164 arcsec
Target: Active Region
Pointing: xcen=-146 ycen=-55,
saaIntervals hiIntervals
wavelengthcadenceFOVx,yimages
6302A Continuum Intensity0135,162427
6302A Velocity 6301.5A0135,162427
6302A Transverse Flux Density0135,162427
6302A Longitudinal Flux Density0135,162427
SOTSP: HOP57 penumbra dynamics
2008-01-04T22:00:05 to 2008-01-04T22:43:32
Science Goal: HOP57 penumbra dynamics, CORE study
Program: Normal map 512x512
Target: Active Region
Pointing: xcen=-547 ycen=-87,
saaIntervals hiIntervals
wavelengthcadenceFOVx,yimages
6302A Continuum Intensity-181,81512
6302A Velocity 6301.5A-181,81512
6302A Transverse Flux Density-181,81512
6302A Longitudinal Flux Density-181,81512
XRT:
2007-12-30T07:28:11 to 2007-12-30T08:58:51
Science Goal: CORE: SOT continuous magnetic field observations for investigating mechanisms responsible for XBPs and QS dynamics
Program: TI_just_after_OP_Upload
Target:
Pointing: xcen=71 ycen=1,
saaIntervals hiIntervals
wavelengthcadenceFOVx,yimages
Ti_poly9.07527,52711

257287 matches
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