| Overview | Where | Groups: Mode, FOV, # spectra in map | Data Links |
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2016-12-16 19:20:05-19:36:15
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HOP 328 QS w/ALMA Part 2 Quiet Sun Observations |
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| 6302A Continuum Intensity | 81"x81" | 256 spectra | | 6302A Longitudinal Flux Density | 81"x81" | 256 spectra | | 6302A Transverse Flux Density | 81"x81" | 256 spectra | | 6302A Velocity 6301.5A | 81"x81" | 256 spectra |
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Level 1 Summary
Level 2 Summary
Level 1 Monthly
Level 2 Monthly
SP Cubes 2 MB |
SOTSP: HOP 328 QS w/ALMA Part 2
2016-12-16T19:20:05 to 2016-12-16T19:36:15
Science Goal: Quiet Sun Observations
Program: Fast map 82x82", 1 side Q65
Target: Quiet Sun
xcen=0 ycen=-26
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: 60
Chief Observer
Cruz (RCO) --> R.Ishikawa
See also
Get All Data
saaIntervals
hiIntervals
Time Series (SP Datacubes)
wavelength: 6302A Continuum Intensity cadence: 0 min fov: 81,81 images: 256 JavaScript Landing Page
