Heliophysics Events Knowledgebase Coverage Registry (HCR)
Observation Details
Overview Where Groups: Mode, FOV, # spectra in map Data Links
2022-07-30 01:33:42-02:36:54
HOP 393 Cycle 24/25 Equatorial
Cycle 24/25 equatorial transition
x,y:9",-210"
Max FOV:316"x162"
Target:Active Region
Nearby Events
6302A Continuum Intensity316"x162"1000 spectra
6302A Longitudinal Flux Density316"x162"1000 spectra
6302A Transverse Flux Density316"x162"1000 spectra
6302A Velocity 6301.5A316"x162"1000 spectra
Level 1 Summary
Level 2 Summary
Level 1 Monthly
Level 2 Monthly
SP Cubes 17 MB
SOTSP: HOP 393 Cycle 24/25 Equatorial
2022-07-30T01:33:42 to 2022-07-30T02:36:54
Science Goal: Cycle 24/25 equatorial transition
Program: Fast Map, Full FOV 1 side CCD Q75
Target: Active Region
xcen=9 ycen=-210
Instrument: SOTSP
HOP/JOP: 393
Description: request to SOT SOT requests: ---------- brief instruction (general) ----------- ID: 0x1ce (Normal 320"x82") One full resolution, full width, half slit (512 px), normal map centered on the central meridian and the solar equator (latitude 0N). The SSW command hel2arcmin may be used to convert from 0N degrees latitude to arcsec (divide by 60). Corrections should be made for the SOT offset. NOTE TO COs: Run once per week, at a cadence equivalent to HOP 336. Simultaneous observations with HOP 336 are not required. Although tracking curves are preferred for these observations, if there are not enough available, this map should be run with fixed pointing. ---------- additional instruction (in eclipse season) ----------- ID: 0x12c (Fast Map, Full FOV) During eclipse season, please run a full width, full height fast map at the same pointing, instead of the normal maps. Each of these should run twice, in 2 consecutive orbits, for redundancy. Full height is requested because SOT offsets in Y are large and slightly uncertain during eclipse season.

request to SOT SOT requests: ---------- brief instruction (general) ----------- ID: 0x1ce (Normal 320"x82") One full resolution, full width, half slit (512 px), normal map centered on the central meridian and the solar equator (latitude 0N). The SSW command hel2arcmin may be used to convert from 0N degrees latitude to arcsec (divide by 60). Corrections should be made for the SOT offset. NOTE TO COs: Run once per week, at a cadence equivalent to HOP 336. Simultaneous observations with HOP 336 are not required. Although tracking curves are preferred for these observations, if there are not enough available, this map should be run with fixed pointing. ---------- additional instruction (in eclipse season) ----------- ID: 0x12c (Fast Map, Full FOV) During eclipse season, please run a full width, full height fast map at the same pointing, instead of the normal maps. Each of these should run twice, in 2 consecutive orbits, for redundancy. Full height is requested because SOT offsets in Y are large and slightly uncertain during eclipse season.

Annotations:
Hits: 45
Chief Observer
Cruz (RCO) --> Okamoto
Related Links
Cites: HOP 393 Cycle 24/25 Equatorial     
Timeline: gif use
See also
Datasets
Order AIA Data Cutout
Get All Data
saaIntervals hiIntervals

wavelength: 6302A Continuum Intensity cadence: 0 min fov: 316,162 images: 1000 JavaScript Landing Page
wavelength: 6302A Velocity 6301.5A cadence: 0 min fov: 316,162 images: 1000 JavaScript Landing Page
wavelength: 6302A Transverse Flux Density cadence: 0 min fov: 316,162 images: 1000 JavaScript Landing Page
wavelength: 6302A Longitudinal Flux Density cadence: 0 min fov: 316,162 images: 1000 JavaScript Landing Page
Time Series (SP Datacubes)
VOEvent XML Planning Event