Observation

Observation Details

Overview

Where

Groups: Mode, FOV, # spectra in map

Data Links

2015-09-03 18:26:37-19:15:36

HOP290 (CLASP)

Coordinated observation with CLASP sounding rocket

x,y:	443",-638"
Max FOV:	243"x122"
Target:	Quiet Sun
Nearby Events

6302A Continuum Intensity	243"x122"	770 spectra
6302A Longitudinal Flux Density	243"x122"	770 spectra
6302A Transverse Flux Density	243"x122"	770 spectra
6302A Velocity 6301.5A	243"x122"	770 spectra

Level 1 Summary
Level 2 Summary
Level 1 Monthly
Level 2 Monthly
SP Cubes 9 MB

SOTSP: HOP290 (CLASP)

2015-09-03T18:26:37 to 2015-09-03T19:15:36

Science Goal: Coordinated observation with CLASP sounding rocket

Program: Fast map, BFI Full FOV, Q65, 1-side CCD

Target: Quiet Sun

xcen=443 ycen=-638

Instrument: SOTSP

HOP/JOP: 290

Description: The Chromospheric Lyman-Alpha Spectro-Polarimeter (CLASP) sounding rocket is a high precision spectro-polarimeter designed to measure the Lyman-alpha Stokes profiles (I, Q, and U), and aims at inferring the magnetic field vector of the upper chromosphere and the transition region. CLASP team requests observing support from Hinode and IRIS to uncover the magnetic structure and dynamical state from the photosphere to the corona. The launch date is scheduled for Sept. 3, 2015, and the current launch window is 17:16 - 18:16 UT. The CLASP will avoid the time periods when both Hinode and IRIS pass though the SAA, and the resulting launch window is tentatively 17:30 - 18:15 UT based on the current SAA prediction (this will be updated based on new orbit information before the launch). The flight time is about 5 minutes. The target will be a quiet region near the solar limb. The 400-arcsec-long slit is set to perpendicular to the solar limb. The exact coordinates and the launch time will be informed before the planning.

The Chromospheric Lyman-Alpha Spectro-Polarimeter (CLASP) sounding rocket is a high precision spectro-polarimeter designed to measure the Lyman-alpha Stokes profiles (I, Q, and U), and aims at inferring the magnetic field vector of the upper chromosphere and the transition region. CLASP team requests observing support from Hinode and IRIS to uncover the magnetic structure and dynamical state from the photosphere to the corona. The launch date is scheduled for Sept. 3, 2015, and the current launch window is 17:16 - 18:16 UT. The CLASP will avoid the time periods when both Hinode and IRIS pass though the SAA, and the resulting launch window is tentatively 17:30 - 18:15 UT based on the current SAA prediction (this will be updated based on new orbit information before the launch). The flight time is about 5 minutes. The target will be a quiet region near the solar limb. The 400-arcsec-long slit is set to perpendicular to the solar limb. The exact coordinates and the launch time will be informed before the planning.

Annotations:

Chief Observer

DeRosa (RCO) -> Yasuda