Heliophysics Events Knowledgebase Coverage Registry (HCR)
Observation Details
Overview Where Groups: Mode, FOV, # spectra in map Data Links
2018-09-10 10:15:06-13:08:49
HOP 336 N Hemisphere
Cycle 25 Bright Points
x,y:-33",490"
Max FOV:319"x81"
Target:Quiet Sun
Nearby Events
6302A Continuum Intensity319"x81"2029 spectra
6302A Longitudinal Flux Density319"x81"2029 spectra
6302A Transverse Flux Density319"x81"2029 spectra
6302A Velocity 6301.5A319"x81"2029 spectra

Level 1 Summary
Level 2 Summary
Level 1 Monthly
Level 2 Monthly
SOTSP: HOP 336 N Hemisphere
2018-09-10T10:15:06 to 2018-09-10T13:08:49
Science Goal: Cycle 25 Bright Points
Program: Normal 320"x82", 1 side, Q75
Target: Quiet Sun
xcen=-33 ycen=490
Instrument: SOTSP
HOP/JOP: 336
Description: Main Objective: To find the magnetic and chromospheric signatures of the onset of cycle 25. Scientific Justification: Small magnetic features and coronal bright points have been shown to indicate the bands of activity associated with the solar cycle. The precise location of these bands is important for predicting the timing of solar minimum and, more generally, the long-term variability of the Sun. request to SOT (Updated: 10-May-2018) ---------- brief instruction (general) ----------- ID: 0x1ce (Normal 320"x82") One full resolution, full width, half slit (512 px), normal map centered at longitude 0W and latitude 40N for the northern hemisphere (after correcting for the SOT offset). One full resolution, full width, half slit (512 px), normal map centered at longitude 0W and latitude 45S for the southern hemisphere (after correcting for the SOT offset). NOTE TO COs: Although tracking curves are preferred for these observations, if there are not enough available, then either or both maps should be run with fixed pointing.

Main Objective: To find the magnetic and chromospheric signatures of the onset of cycle 25. Scientific Justification: Small magnetic features and coronal bright points have been shown to indicate the bands of activity associated with the solar cycle. The precise location of these bands is important for predicting the timing of solar minimum and, more generally, the long-term variability of the Sun. request to SOT (Updated: 10-May-2018) ---------- brief instruction (general) ----------- ID: 0x1ce (Normal 320"x82") One full resolution, full width, half slit (512 px), normal map centered at longitude 0W and latitude 40N for the northern hemisphere (after correcting for the SOT offset). One full resolution, full width, half slit (512 px), normal map centered at longitude 0W and latitude 45S for the southern hemisphere (after correcting for the SOT offset). NOTE TO COs: Although tracking curves are preferred for these observations, if there are not enough available, then either or both maps should be run with fixed pointing.

Annotations:
Hits: 64
Chief Observer
Cruz (RCO)
Related Links
Cites: HOP 336 N Hemisphere     
Timeline: gif use
See also
Datasets
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saaIntervals hiIntervals

wavelength: 6302A Continuum Intensity cadence: -1 min fov: 319,81 images: 2029 JavaScript Landing Page
wavelength: 6302A Velocity 6301.5A cadence: -1 min fov: 319,81 images: 2029 JavaScript Landing Page
wavelength: 6302A Transverse Flux Density cadence: -1 min fov: 319,81 images: 2029 JavaScript Landing Page
wavelength: 6302A Longitudinal Flux Density cadence: -1 min fov: 319,81 images: 2029 JavaScript Landing Page