Heliophysics Events Knowledgebase Coverage Registry (HCR)
Observation Details
Overview Where Groups: Mode, FOV, # spectra in map Data Links
2016-12-16 12:30:27-15:59:32
HOP 328 QS w/ALMA Part 1
Quiet Sun Observations
x,y:218",221"
Max FOV:27"x81"
Target:Quiet Sun
Nearby Events
6302A Continuum Intensity27"x81"3105 spectra
6302A Longitudinal Flux Density27"x81"3105 spectra
6302A Transverse Flux Density27"x81"3105 spectra
6302A Velocity 6301.5A27"x81"3105 spectra

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SP Cubes 27 MB
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SP Movies (MP4)
SOTSP: HOP 328 QS w/ALMA Part 1
2016-12-16T12:30:27 to 2016-12-16T15:59:32
Science Goal: Quiet Sun Observations
Program: Fast map, 25x82", repeat, Q75, 1-side
Target: Quiet Sun
xcen=218 ycen=221
Instrument: SOTSP
HOP/JOP: 328
Description: Support for ALMA Cycle 4 Observations (generic) abstract of observational proposal Main Objective: A HOP to support ALMA observations in cycle 4 for those proposers that do not have their own specific HOP request. Scientific Justification: The Atacama Large Millimeter/Submillimeter Array (ALMA) has recently accepted 15 proposals to observe the Sun in Band 3 and Band 6 during cycle 4 (observing from ~September 2016 ~ September 2017). These observations will provide high-resolution (~1-2", 2s cadence) observations of the solar chromosphere. The observations will cover an array of different science topics encompassing this region, where ALMA can serve as a sort of linear thermometer to probe these regions. Here we propose a set of generic observations for those studies, which do not make specific requests to Hinode. request to SOT (primary) SP fast maps 60"x60" FOV --- 11.25 minute/map ~225 MBits/hr

Support for ALMA Cycle 4 Observations (generic) abstract of observational proposal Main Objective: A HOP to support ALMA observations in cycle 4 for those proposers that do not have their own specific HOP request. Scientific Justification: The Atacama Large Millimeter/Submillimeter Array (ALMA) has recently accepted 15 proposals to observe the Sun in Band 3 and Band 6 during cycle 4 (observing from ~September 2016 ~ September 2017). These observations will provide high-resolution (~1-2", 2s cadence) observations of the solar chromosphere. The observations will cover an array of different science topics encompassing this region, where ALMA can serve as a sort of linear thermometer to probe these regions. Here we propose a set of generic observations for those studies, which do not make specific requests to Hinode. request to SOT (primary) SP fast maps 60"x60" FOV --- 11.25 minute/map ~225 MBits/hr

Annotations:
Hits: 61
Chief Observer
Cruz (RCO) --> R.Ishikawa
Related Links
Cites: HOP 328 QS w/ALMA Part 1     
Timeline: gif use
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Datasets
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saaIntervals hiIntervals

wavelength: 6302A Continuum Intensity cadence: 0 min fov: 27,81 images: 3105 JavaScript Landing Page
wavelength: 6302A Velocity 6301.5A cadence: 0 min fov: 27,81 images: 3105 JavaScript Landing Page
wavelength: 6302A Transverse Flux Density cadence: 0 min fov: 27,81 images: 3105 JavaScript Landing Page
wavelength: 6302A Longitudinal Flux Density cadence: 0 min fov: 27,81 images: 3105 JavaScript Landing Page
Time Series (SP Datacubes)
JavaScript MP4