Heliophysics Events Knowledgebase Coverage Registry (HCR)
Observation Details
Overview Where Groups: Mode, FOV, # spectra in map Data Links
2011-06-11 08:18:23-09:19:52
HOP 126
CORE: Chromospheric Jets
x,y:-2",-33"
Max FOV:10"x81"
Target:disk center, Quiet Sun, Spicule and Jets
Nearby Events
6302A Continuum Intensity10"x81"1526 spectra
6302A Longitudinal Flux Density10"x81"1526 spectra
6302A Transverse Flux Density10"x81"1526 spectra
6302A Velocity 6301.5A10"x81"1526 spectra
Level 1 Summary
Level 2 Summary
Level 1 Monthly
Level 2 Monthly
SP Cubes 13 MB
SP Movies (Javascript)
SP Movies (MP4)
SOTSP: HOP 126
2011-06-11T08:18:23 to 2011-06-11T09:19:52
Science Goal: CORE: Chromospheric Jets
Program: Dynamics, 9.6"x82", repeat
Target: disk center, Quiet Sun, Spicule and Jets
xcen=-2 ycen=-33
Instrument: SOTSP
HOP/JOP: 126
Description: SP: fast map large enough to cover the AR, perhaps 123x123 or 164x164 arcsec, avoiding SAA NFI: Program 0x3b4 AR mode case2 (Large), G-band 120min, Na IV 5min, Ca H 5min, during the SP map High-cadence programs: NFI: Program 03bd H-alpha sequence: H-alpha at -2.1A, at -1.28A and -0.87A, 112"x112", 2x2 summed, at 13 s cadence, and Na D IVDG every 5 minutes, same FOV SP : Program 0xed fast raster (dynamics), 4.8"x60" at 1 min cadence The NFI high cadence program should run for the prime observing time in La Palma, 2-3 hours depending on telemetry. The SP high cadence should run for 30 minutes in the middle of this period (avoiding SAA). The context programs should run once before the high cadence observing begins and again once after it ends. The CT should cycle off/on before the start of each of the SP programs. Other Instruments: SST: Ca-H, Ca 8542, H alpha

SP: fast map large enough to cover the AR, perhaps 123x123 or 164x164 arcsec, avoiding SAA NFI: Program 0x3b4 AR mode case2 (Large), G-band 120min, Na IV 5min, Ca H 5min, during the SP map High-cadence programs: NFI: Program 03bd H-alpha sequence: H-alpha at -2.1A, at -1.28A and -0.87A, 112"x112", 2x2 summed, at 13 s cadence, and Na D IVDG every 5 minutes, same FOV SP : Program 0xed fast raster (dynamics), 4.8"x60" at 1 min cadence The NFI high cadence program should run for the prime observing time in La Palma, 2-3 hours depending on telemetry. The SP high cadence should run for 30 minutes in the middle of this period (avoiding SAA). The context programs should run once before the high cadence observing begins and again once after it ends. The CT should cycle off/on before the start of each of the SP programs. Other Instruments: SST: Ca-H, Ca 8542, H alpha

Annotations:
Hits: 70
Chief Observer
Zoe (RCO) -> Sekii
Related Links
Cites: HOP 126     
Timeline: gif use
See also
Datasets
Order AIA Data Cutout
Get All Data
saaIntervals hiIntervals

wavelength: 6302A Continuum Intensity cadence: 0.01 min fov: 10,81 images: 1526 JavaScript Landing Page
wavelength: 6302A Velocity 6301.5A cadence: 0.01 min fov: 10,81 images: 1526 JavaScript Landing Page
wavelength: 6302A Transverse Flux Density cadence: 0.01 min fov: 10,81 images: 1526 JavaScript Landing Page
wavelength: 6302A Longitudinal Flux Density cadence: 0.01 min fov: 10,81 images: 1526 JavaScript Landing Page
Time Series (SP Datacubes)
JavaScript MP4
VOEvent XML Planning Event