Observation

Observation Details

Overview

Where

Groups: Mode, FOV, # spectra in map

Data Links

2009-01-10 16:20:43-16:33:21

HOP 94 - Driving mechanism(s) of small scale transient brightenings in the solar atmosphere

Driving mechanism(s) of small scale transient brightenings in the solar atmosphere

x,y:	22",7"
Max FOV:	59"x162"
Target:	Disk Center
Nearby Events

6302A Continuum Intensity	59"x162"	198 spectra
6302A Longitudinal Flux Density	59"x162"	198 spectra
6302A Transverse Flux Density	59"x162"	198 spectra
6302A Velocity 6301.5A	59"x162"	198 spectra

Level 1 Summary
Level 2 Summary
Level 1 Monthly
Level 2 Monthly

SOTSP: HOP 94 - Driving mechanism(s) of small scale transient brightenings in the solar atmosphere

2009-01-10T16:20:43 to 2009-01-10T16:33:21

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=22 ycen=7

Instrument: SOTSP

HOP/JOP: 0

Description: 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.

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.

Annotations:

Chief Observer

Shine

Timeline: gif use