Heliophysics Events Knowledgebase Coverage Registry (HCR)
Observation Details
Overview Where Groups: Mode, FOV, # spectra in map Data Links
2007-09-26 08:15:29-10:06:34
HOP14 convective collapse
Hinode/Canary Islands Campaign
x,y:2",7"
Max FOV:3"x41"
Target:Quiet Sun
Nearby Events
6302A Continuum Intensity3"x41"3348 spectra
6302A Longitudinal Flux Density3"x41"3348 spectra
6302A Transverse Flux Density3"x41"3348 spectra
6302A Velocity 6301.5A3"x41"3348 spectra
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SOTSP: HOP14 convective collapse
2007-09-26T08:15:29 to 2007-09-26T10:06:34
Science Goal: Hinode/Canary Islands Campaign
Program: 30 s, 2.9", 0.16" convective collapse
Target: Quiet Sun
xcen=2 ycen=7
Instrument: SOTSP
HOP/JOP: 14
Description: HOP 14 Program (Quiet Sun SP Map): starting at (0, 149), tracking solar rotation 25 Sep 10:35 - 11:59 FG now observing in Fe I 6301 (not 6302.5) HOP 14 Alignment Program: fixed at (0, 0) 25 Sep 12:06 - 12:39 HOP 14 Alignment Program (continued): starting at (-21, 0), tracking solar rotation 25 Sep 12:44 ??? 16:00 HOP 14 Convective Collapse, starting at (-12, 0), tracking solar rotation 26 Sep 08:15 ??? 10:06 Request to SOT HOP Number 0014 Quiet Sun magnetic fields SOT/FG: G-band and Ca II H filtergrams for studying connections between internetwork fields and chromospheric structure SOT/SP: Sequence of short scans in Fe I 630.2nm Scientific Objectives: We are planning to carry out two kinds of study in this unique opportunity: characterization of quiet Sun magnetic fields including their evolution, and the study of moving magnetic features and flux cancellation events in sunspots.

HOP 14 Program (Quiet Sun SP Map): starting at (0, 149), tracking solar rotation 25 Sep 10:35 - 11:59 FG now observing in Fe I 6301 (not 6302.5) HOP 14 Alignment Program: fixed at (0, 0) 25 Sep 12:06 - 12:39 HOP 14 Alignment Program (continued): starting at (-21, 0), tracking solar rotation 25 Sep 12:44 ??? 16:00 HOP 14 Convective Collapse, starting at (-12, 0), tracking solar rotation 26 Sep 08:15 ??? 10:06 Request to SOT HOP Number 0014 Quiet Sun magnetic fields SOT/FG: G-band and Ca II H filtergrams for studying connections between internetwork fields and chromospheric structure SOT/SP: Sequence of short scans in Fe I 630.2nm Scientific Objectives: We are planning to carry out two kinds of study in this unique opportunity: characterization of quiet Sun magnetic fields including their evolution, and the study of moving magnetic features and flux cancellation events in sunspots.

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Chief Observer
Tarbell
Related Links
Cites: HOP14 convective collapse     
Timeline: gif use
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wavelength: 6302A Continuum Intensity cadence: 0.03 min fov: 3,41 images: 3348 JavaScript Landing Page
wavelength: 6302A Velocity 6301.5A cadence: 0.03 min fov: 3,41 images: 3348 JavaScript Landing Page
wavelength: 6302A Transverse Flux Density cadence: 0.03 min fov: 3,41 images: 3348 JavaScript Landing Page
wavelength: 6302A Longitudinal Flux Density cadence: 0.03 min fov: 3,41 images: 3348 JavaScript Landing Page
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