Heliophysics Events Knowledgebase Coverage Registry (HCR)
Observation Details
Overview Where Groups: Mode, FOV, # spectra in map Data Links
2007-08-12 22:06:14-22:25:10
Emerging Flux -- SP
Cooperative Observations between Hida Observatory and; Hinode Satellite - 1. Emerging Flux Regions 2. Cool Jets 3. Ellerman Bombs
x,y:683",-160"
Max FOV:95"x162"
Target:Active Region
Nearby Events
6302A Continuum Intensity95"x162"300 spectra
6302A Longitudinal Flux Density95"x162"300 spectra
6302A Transverse Flux Density95"x162"300 spectra
6302A Velocity 6301.5A95"x162"300 spectra
Level 1 Summary
Level 2 Summary
Level 1 Monthly
Level 2 Monthly
SP Cubes 5 MB
SOTSP: Emerging Flux -- SP
2007-08-12T22:06:14 to 2007-08-12T22:25:10
Science Goal: Cooperative Observations between Hida Observatory and; Hinode Satellite - 1. Emerging Flux Regions 2. Cool Jets 3. Ellerman Bombs
Program: Fast map 100 arcsec repeat
Target: Active Region
xcen=683 ycen=-160
Instrument: SOTSP
HOP/JOP: 12
Description: Daily Note and User Entry: SOT will be doing normal observing, using old s/w (installation of new s/w postponed). EIS: Sensitivity calibration for 3.5 hours in this weekend andnbsp
plan HOP29, filament, prominence, cavities (18 -22 UT). HOP26 (4 or more hrs, between 11 - 18 UT). HOP12 (22 - 3 UT, can be extended to 6 UT if no conflict). XRT: CCD Bakeout Alignment offset pointing over weekend.
Request to SOT: 1a.


* G-band Filtergraph: ???@



Observation of the arch-filaments on the photosphere, ???@



measurement of the horizontal flow (by LCT) around EFR/AFS. ???@




Time cadence: 15 sec ???@




Duration: as long as possible ???@

* Ca Filtergraph: ???@



Observation of the arch-filaments in the chromosphere ???@




Time cadence: about 30 sec ???@




Duration: as long as possible ???@

* SP: ???@



Measurement of the time-evolution of magnetic flux and Doppler ???@



velocity around the EFR/AFS. ???@




Time cadence: 180 sec ???@




Scan step: 0.3 - 0.6 arcsec/step ???@




Scan width: 20 - 60 arcsec (wider than the size of EFR) ???@




Duration: as long as possible 1b. ???@

* Ca Filtergraph: ???@


Observation of the chromospheric gas motion on the footpoint of ???@


magnetic filament. ???@



Time cadence: 8 sec ???@

* G-band Filtergraph: ???@


Detection of the photospheric bright point (G-band bright point). ???@



Time cadence: 8 sec ???@

* SP: ???@


Distinction of the footpoint of magnetic filament. ???@




Time cadence: 30 sec ???@




Scan step: 0.3 - 0.6 arcsec/step ???@




Scan width: about 20 - 30 arcsec 1c. ???@

* G-band Filtergraph: ???@


Detection and distinction of the footpoint of magnetic flux tube, ???@


measurement of the horizontal flow on the photosphere ???@



Time cadence: 8 sec ???@ ???@

* Ca Filtergraph: ???@


Observation of the chromospheric gas motion on the footpoint of ???@


magnetic flux tube ???@



Time cadence: 8 sec ???@ ???@

* SP: ???@


Measurement of the time-evolution of magnetic flux and Doppler ???@


velocity around/in the flux tube. ???@



Time cadence: <
30 sec ???@



Scan step: 0.3 - 0.6 arcsec ???@



Scan width: as wide as possible 2. ???@



Ca and
G-band Filtergraph: ???@




Detection of jets around the photosphere and chromosphere ???@




Time cadence: 10 sec (respectively) ???@



SP: ???@




Observation of the photospheric magnetic field configurations around the jets ???@




Time cadence: 60 sec ???@




Scan step: 0.3 - 0.6 arcsec ???@




Scan width: as wide as possible 3. ???@


* SP: ???@




Obtaining photospheric magnetic field and Doppler velocity ???@




around/at Ellerman bomb ???@




Time cadence: 60 sec ???@




Scan step: 0.3 - 0.6 arcsec ???@




Scan width: as wide as possible ???@


* Ca H Filtergram: ???@




Observing shape and time evolution of the Ellerman bomb ???@




Time cadence: 8 sec
Scientific Objectives: 1a. Rise velocity of emerging loops 1b. Shock waves just below the arch filaments in emerging flux regions 1c. Evolution of magnetic element at the footpoint of emerging flux region 2. Detection of Alfven wave generation 3. Observation of reconnection jets and X-ray signatures in the corona
Other Instruments:

Daily Note and User Entry: SOT will be doing normal observing, using old s/w (installation of new s/w postponed). EIS: Sensitivity calibration for 3.5 hours in this weekend andnbsp
plan HOP29, filament, prominence, cavities (18 -22 UT). HOP26 (4 or more hrs, between 11 - 18 UT). HOP12 (22 - 3 UT, can be extended to 6 UT if no conflict). XRT: CCD Bakeout Alignment offset pointing over weekend.
Request to SOT: 1a.


* G-band Filtergraph: ???@



Observation of the arch-filaments on the photosphere, ???@



measurement of the horizontal flow (by LCT) around EFR/AFS. ???@




Time cadence: 15 sec ???@




Duration: as long as possible ???@

* Ca Filtergraph: ???@



Observation of the arch-filaments in the chromosphere ???@




Time cadence: about 30 sec ???@




Duration: as long as possible ???@

* SP: ???@



Measurement of the time-evolution of magnetic flux and Doppler ???@



velocity around the EFR/AFS. ???@




Time cadence: 180 sec ???@




Scan step: 0.3 - 0.6 arcsec/step ???@




Scan width: 20 - 60 arcsec (wider than the size of EFR) ???@




Duration: as long as possible 1b. ???@

* Ca Filtergraph: ???@


Observation of the chromospheric gas motion on the footpoint of ???@


magnetic filament. ???@



Time cadence: 8 sec ???@

* G-band Filtergraph: ???@


Detection of the photospheric bright point (G-band bright point). ???@



Time cadence: 8 sec ???@

* SP: ???@


Distinction of the footpoint of magnetic filament. ???@




Time cadence: 30 sec ???@




Scan step: 0.3 - 0.6 arcsec/step ???@




Scan width: about 20 - 30 arcsec 1c. ???@

* G-band Filtergraph: ???@


Detection and distinction of the footpoint of magnetic flux tube, ???@


measurement of the horizontal flow on the photosphere ???@



Time cadence: 8 sec ???@ ???@

* Ca Filtergraph: ???@


Observation of the chromospheric gas motion on the footpoint of ???@


magnetic flux tube ???@



Time cadence: 8 sec ???@ ???@

* SP: ???@


Measurement of the time-evolution of magnetic flux and Doppler ???@


velocity around/in the flux tube. ???@



Time cadence: <
30 sec ???@



Scan step: 0.3 - 0.6 arcsec ???@



Scan width: as wide as possible 2. ???@



Ca and
G-band Filtergraph: ???@




Detection of jets around the photosphere and chromosphere ???@




Time cadence: 10 sec (respectively) ???@



SP: ???@




Observation of the photospheric magnetic field configurations around the jets ???@




Time cadence: 60 sec ???@




Scan step: 0.3 - 0.6 arcsec ???@




Scan width: as wide as possible 3. ???@


* SP: ???@




Obtaining photospheric magnetic field and Doppler velocity ???@




around/at Ellerman bomb ???@




Time cadence: 60 sec ???@




Scan step: 0.3 - 0.6 arcsec ???@




Scan width: as wide as possible ???@


* Ca H Filtergram: ???@




Observing shape and time evolution of the Ellerman bomb ???@




Time cadence: 8 sec
Scientific Objectives: 1a. Rise velocity of emerging loops 1b. Shock waves just below the arch filaments in emerging flux regions 1c. Evolution of magnetic element at the footpoint of emerging flux region 2. Detection of Alfven wave generation 3. Observation of reconnection jets and X-ray signatures in the corona
Other Instruments:

Annotations:
Hits: 75
Chief Observer
Nagata, Tarbell
Related Links
Cites: Emerging Flux -- SP     
Timeline: gif use
See also
Datasets
Order AIA Data Cutout
Get All Data
saaIntervals hiIntervals

wavelength: 6302A Continuum Intensity cadence: 0 min fov: 95,162 images: 300 JavaScript Landing Page
wavelength: 6302A Velocity 6301.5A cadence: 0 min fov: 95,162 images: 300 JavaScript Landing Page
wavelength: 6302A Transverse Flux Density cadence: 0 min fov: 95,162 images: 300 JavaScript Landing Page
wavelength: 6302A Longitudinal Flux Density cadence: 0 min fov: 95,162 images: 300 JavaScript Landing Page
Time Series (SP Datacubes)
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