Heliophysics Events Knowledgebase Coverage Registry (HCR)
Observation Details
Overview Where Groups: Mode, FOV, # spectra in map Data Links
2021-05-06 13:02:15-13:59:30
HOP 416
A holistic view on coronal holes - temporal evolution
x,y:-19",-281"
Max FOV:2"x162"
Target:Coronal Hole
Nearby Events
6302A Continuum Intensity2"x162"506 spectra
6302A Longitudinal Flux Density2"x162"506 spectra
6302A Transverse Flux Density2"x162"506 spectra
6302A Velocity 6301.5A2"x162"506 spectra

Level 1 Summary
Level 2 Summary
Level 1 Monthly
Level 2 Monthly
SOTSP: HOP 416
2021-05-06T13:02:15 to 2021-05-06T13:59:30
Science Goal: A holistic view on coronal holes - temporal evolution
Program: Normal Map (8 cycles), 1.6"x164", repeats, 1-side, not summed
Target: Coronal Hole
xcen=-19 ycen=-281
Instrument: SOTSP
HOP/JOP: 416
Description: request to SOT SOT/SP shall perform the following sequence outside SAAS: SAA - n1 x 1.5?x164? normal - SSA - n2 x 60?x164? fast - SAA - n3 x 60?x164? fast - SAA. During the first observing slot outside SAAs, repeat 1.5?x164? SP normal scans as often as possible. Suitable cadences are - 1 minute resulting in 0.5 Gbit/hour (e.g., SP 0x232, margin factor 0.95) - 30 seconds resulting in 0.75 Gbits/hour (e.g., SP 0x231, margin factor 0.75), - 20 seconds resulting in estimated 1.5 Gbits/hour Note that SP 0x231 and 0x232 cannot be in the same table (they use the same SEQ and PAR slots). We will leave it to the discretion of the planner to choose the cadence which best fits to the available telemetry. The 1.5?x164? scans shall be coordinated with EIS and IRIS, to have roughly the same center position. Note that in case of insufficient telemetry, we can skip the SOT observations in this observing slot on some days. During the observing slots two and three outside SAAs, repeat 60?x164? fast maps as often as possible. The cadence of a single 60?x164? scan is 13min26s. The amount of data is 0.7 Gbit/hour. In case of telemetry issues, these observing slots shall be given priority over the observing slot one (1.5?x164?).

request to SOT SOT/SP shall perform the following sequence outside SAAS: SAA - n1 x 1.5?x164? normal - SSA - n2 x 60?x164? fast - SAA - n3 x 60?x164? fast - SAA. During the first observing slot outside SAAs, repeat 1.5?x164? SP normal scans as often as possible. Suitable cadences are - 1 minute resulting in 0.5 Gbit/hour (e.g., SP 0x232, margin factor 0.95) - 30 seconds resulting in 0.75 Gbits/hour (e.g., SP 0x231, margin factor 0.75), - 20 seconds resulting in estimated 1.5 Gbits/hour Note that SP 0x231 and 0x232 cannot be in the same table (they use the same SEQ and PAR slots). We will leave it to the discretion of the planner to choose the cadence which best fits to the available telemetry. The 1.5?x164? scans shall be coordinated with EIS and IRIS, to have roughly the same center position. Note that in case of insufficient telemetry, we can skip the SOT observations in this observing slot on some days. During the observing slots two and three outside SAAs, repeat 60?x164? fast maps as often as possible. The cadence of a single 60?x164? scan is 13min26s. The amount of data is 0.7 Gbit/hour. In case of telemetry issues, these observing slots shall be given priority over the observing slot one (1.5?x164?).

Annotations:
Hits: 125
Chief Observer
Cruz (RCO) --> Katsukawa
Related Links
Cites: HOP 416     
Timeline: gif use
See also
Datasets
Get All Data
saaIntervals hiIntervals

wavelength: 6302A Continuum Intensity cadence: 0.01 min fov: 2,162 images: 506 JavaScript Landing Page
wavelength: 6302A Velocity 6301.5A cadence: 0.01 min fov: 2,162 images: 506 JavaScript Landing Page
wavelength: 6302A Transverse Flux Density cadence: 0.01 min fov: 2,162 images: 506 JavaScript Landing Page
wavelength: 6302A Longitudinal Flux Density cadence: 0.01 min fov: 2,162 images: 506 JavaScript Landing Page