Heliophysics Events Knowledgebase Coverage Registry (HCR)
Observation Details
Overview Where Groups: Mode, FOV, # spectra in map Data Links
2010-05-12 22:58:59-23:32:21
HOP 146 South CH
Solar Wind Source Regions During Solar Minimum Conditions
x,y:-106",-812"
Max FOV:61"x162"
Target:Coronal Hole
Nearby Events
6302A Continuum Intensity61"x162"196 spectra
6302A Longitudinal Flux Density61"x162"196 spectra
6302A Transverse Flux Density61"x162"196 spectra
6302A Velocity 6301.5A61"x162"196 spectra
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SP Cubes 3 MB
SOTSP: HOP 146 South CH
2010-05-12T22:58:59 to 2010-05-12T23:32:21
Science Goal: Solar Wind Source Regions During Solar Minimum Conditions
Program: Fast deep mode, 2048 slit position
Target: Coronal Hole
xcen=-106 ycen=-812
Instrument: SOTSP
HOP/JOP: 146
Description: Request to SOT HOP Number 0146 SOT/NFI NaID, Stokes IV: full FOV, low cadence (~5min) but high sensitvity (long exposure times!) Reminder: program using Na D V/I is OK for on disc pointing only. Use Na D IV for if limb is visible in the field of view. SOT/SP: Stokes IQUV repeated large SP maps also with long exposure times. Other Instruments: Scientific Objectives: 1) Objectives: Characterize solar wind source regions during solar minimum conditions, and relate to properties in the solar wind measured at 1 AU to investigate the formation of the solar wind 2) Scientific background: During solar minimum conditions, the solar wind measured in-situ at 1 AU mostly originates from the two polar coronal holes, especially, the polar coronal hole boundary for the slow solar wind. The Ulysses solar wind ion composition data from the last solar minimum indicates that the coronal temperature in the fast wind is different between the solar wind originating from the south and north CH. There are also variations with time and possibly latitude in both the fast and slow wind. This HOP proposes to monitor the corresponding solar wind source regions for several solar rotations at the two polar CH boundaries that can be directly related to the solar wind data measured at 1 AU to understand the cause of variations and the solar wind formation.

Annotations:
Hits: 65
Chief Observer
Cruz (RCO)
Related Links
Cites: HOP 146 South CH     
Timeline: gif use
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wavelength: 6302A Continuum Intensity cadence: 0 min fov: 61,162 images: 196 JavaScript Landing Page
wavelength: 6302A Velocity 6301.5A cadence: 0 min fov: 61,162 images: 196 JavaScript Landing Page
wavelength: 6302A Transverse Flux Density cadence: 0 min fov: 61,162 images: 196 JavaScript Landing Page
wavelength: 6302A Longitudinal Flux Density cadence: 0 min fov: 61,162 images: 196 JavaScript Landing Page
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