Observation

Observation Details

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Where

Groups: Mode, FOV, # spectra in map

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2009-08-28 22:04:22-03:59:58 +1d

HOP 124 XBPs (SP)

Time-varying Doppler velocity diagnosis of X-ray Bright Points

x,y:	-65",7"
Max FOV:	41"x122"
Target:	disk center, Quiet Sun
Nearby Events

6302A Continuum Intensity	41"x122"	5281 spectra
6302A Longitudinal Flux Density	41"x122"	5281 spectra
6302A Transverse Flux Density	41"x122"	5281 spectra
6302A Velocity 6301.5A	41"x122"	5281 spectra

Level 1 Summary
Level 2 Summary
Level 1 Monthly
Level 2 Monthly
SP Cubes 67 MB
SP Movies (Javascript)
SP Movies (MP4)

SOTSP: HOP 124 XBPs (SP)

2009-08-28T22:04:22 to 2009-08-29T03:59:58

Science Goal: Time-varying Doppler velocity diagnosis of X-ray Bright Points

Program: Fast map, 41"x123", Q65, 1-side CCD

Target: disk center, Quiet Sun

xcen=-65 ycen=7

Instrument: SOTSP

HOP/JOP: 124

Description: We intend to carry out a thorough investigation on the magnetic field, density and Doppler velocity of XBPs using HINODE observations in order to clarify the working mechanism of XBPs and solve the big puzzle. ?????? 3 days and
#8211
NFI: Stokes I/V Na 589.6 nm FOV: 164"???~164", 0.16" pix Cadence: 64 seconds Telemetry: 255Mbits/hr, 1530Mbits/6hours ?????? Another 3 days and
#8211
SP: Stokes I, Q, U, V FOV: 41"???~123" Cadence: 8 min (Fast Map Mode) Telemetry:57Mbits/map,one map/10minutes,342Mbits/hr,2052Mbits/6hours Other Instruments: Hida Observatory Domeless Solar Telescope (DST): * Ca-line (K or H) spectro-heliograph: Slit length: 145 arcsec Scan width: about 120 arcsec Time cadence: about 15 sec * H-alpha 5 or 7 wavelengths filtergraph: Wavelength: -0.8, -0.5, (-0.25,) 0.0, (+0.25,) +0.5, +0.8 A Time cadence: about 15 sec FOV: 300 x 300 arcsec Solar Magnetic Activity Research Telescope (SMART): * H-alpha 5 wavelengths full-disk filtergraph Wavelength: -0.8, -0.5, 0.0, +0.5, +0.8 A Time cadence: 2 min

We intend to carry out a thorough investigation on the magnetic field, density and Doppler velocity of XBPs using HINODE observations in order to clarify the working mechanism of XBPs and solve the big puzzle. ?????? 3 days and
#8211
NFI: Stokes I/V Na 589.6 nm FOV: 164"???~164", 0.16" pix Cadence: 64 seconds Telemetry: 255Mbits/hr, 1530Mbits/6hours ?????? Another 3 days and
#8211
SP: Stokes I, Q, U, V FOV: 41"???~123" Cadence: 8 min (Fast Map Mode) Telemetry:57Mbits/map,one map/10minutes,342Mbits/hr,2052Mbits/6hours Other Instruments: Hida Observatory Domeless Solar Telescope (DST): * Ca-line (K or H) spectro-heliograph: Slit length: 145 arcsec Scan width: about 120 arcsec Time cadence: about 15 sec * H-alpha 5 or 7 wavelengths filtergraph: Wavelength: -0.8, -0.5, (-0.25,) 0.0, (+0.25,) +0.5, +0.8 A Time cadence: about 15 sec FOV: 300 x 300 arcsec Solar Magnetic Activity Research Telescope (SMART): * H-alpha 5 wavelengths full-disk filtergraph Wavelength: -0.8, -0.5, 0.0, +0.5, +0.8 A Time cadence: 2 min

Annotations:

Chief Observer

Frank(RCO)