Heliophysics Events Knowledgebase Coverage Registry (HCR)
Observation Details
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2009-01-13 15:00:06-15:12:43
HOP 94
Driving mechanism(s) of small scale transient brightenings in the solar atmosphere
x,y:9",7"
Max FOV:63"x162"
Target:disk center
Nearby Events
6302A Continuum Intensity63"x162"198 spectra
6302A Longitudinal Flux Density63"x162"198 spectra
6302A Transverse Flux Density63"x162"198 spectra
6302A Velocity 6301.5A63"x162"198 spectra

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SP Cubes 3 MB
SOTSP: HOP 94
2009-01-13T15:00:06 to 2009-01-13T15:12:43
Science Goal: Driving mechanism(s) of small scale transient brightenings in the solar atmosphere
Program: Fast map, 60 arcsec FOV, 1-side CCD, no repeat
Target: disk center
xcen=9 ycen=7
Instrument: SOTSP
HOP/JOP: 94
Description: The aim of this study is to determine the driving mechanism(s) behind these events as well as to study their coronal responses. For this, it is crucial to obtain the plasma parameters of these events and their magnetic topology. From EIS data, we can derive the densities, temperatures and Doppler shifts of the associated plasma. Highly coordinated observations such as magnetograms and Halpha images from SOT along with XRT will give a clue on the unification of classified transients for instance like blinkers and spicules/macro-spicules/jets along with CDS/SoHO, the later of which is necessary in the identification of the already known blinkers. We will also review the coronal response of the features named blinkers, by using simultaneous CDS and EIS observations. Request to SOT HOP Number 0094 NaI 5896 FGIV magnetograms - 1/min H-alpha 6563/SOT - 1/min

The aim of this study is to determine the driving mechanism(s) behind these events as well as to study their coronal responses. For this, it is crucial to obtain the plasma parameters of these events and their magnetic topology. From EIS data, we can derive the densities, temperatures and Doppler shifts of the associated plasma. Highly coordinated observations such as magnetograms and Halpha images from SOT along with XRT will give a clue on the unification of classified transients for instance like blinkers and spicules/macro-spicules/jets along with CDS/SoHO, the later of which is necessary in the identification of the already known blinkers. We will also review the coronal response of the features named blinkers, by using simultaneous CDS and EIS observations. Request to SOT HOP Number 0094 NaI 5896 FGIV magnetograms - 1/min H-alpha 6563/SOT - 1/min

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Cites: HOP 94     
Timeline: gif use
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wavelength: 6302A Continuum Intensity cadence: 0 min fov: 63,162 images: 198 JavaScript Landing Page
wavelength: 6302A Velocity 6301.5A cadence: 0 min fov: 63,162 images: 198 JavaScript Landing Page
wavelength: 6302A Transverse Flux Density cadence: 0 min fov: 63,162 images: 198 JavaScript Landing Page
wavelength: 6302A Longitudinal Flux Density cadence: 0 min fov: 63,162 images: 198 JavaScript Landing Page
Time Series (SP Datacubes)