XRT: Active region tracking across disk for HIda campaign
2007-06-03T00:06:05 to 2007-06-03T08:59:47
Science Goal: Cooperative Observations between Hida Observatory and; Hinode Satellite - 1. Emerging Flux Regions 2. Cool Jets 3. Ellerman Bombs
Program: AR_for_Hida_CMPN_2
Target: AR
xcen=-838 ycen=-102
Instrument: XRT
HOP/JOP: 0
Description:
Tim File-OBS_DEC: AR - Microflares and Topology - Al/mesh, Ti/Poly, Thick-Al, G-band (512FOV) - Ti-poly context (8s_Q92-35p compression) - AEC123
Daily Note: EIS: Sensitivity monitoring SYNOP002 (3.5 hours) should be run on quiet Sun near disc centre during the two-day plan. Co-alignment program (2hr each for N and E limbs) to be included today. OK to perform in next day if any conflict with science observarions.
Request to XRT HOP Number 0012:
Other Instruments:
Scientific Objectives: 1a. Rise velocity of emerging loops 1b. Shock waves just below the arch filaments in emerging flux regions 1c. Evolution of magnetic element at the footpoint of emerging flux region 2. Detection of Alfven wave generation 3. Observation of reconnection jets and X-ray signatures in the coronaDaily Note: EIS: Sensitivity monitoring SYNOP002 (3.5 hours) should be run on quiet Sun near disc centre during the two-day plan. Co-alignment program (2hr each for N and E limbs) to be included today. OK to perform in next day if any conflict with science observarions.
Request to XRT HOP Number 0012:
Other Instruments:
Scientific Objectives: 1a. Rise velocity of emerging loops 1b. Shock waves just below the arch filaments in emerging flux regions 1c. Evolution of magnetic element at the footpoint of emerging flux region 2. Detection of Alfven wave generation 3. Observation of reconnection jets and X-ray signatures in the coronaDaily Note: EIS: Sensitivity monitoring SYNOP002 (3.5 hours) should be run on quiet Sun near disc centre during the two-day plan. Co-alignment program (2hr each for N and E limbs) to be included today. OK to perform in next day if any conflict with science observarions.
Request to XRT HOP Number 0012:
Other Instruments:
Scientific Objectives: 1a. Rise velocity of emerging loops 1b. Shock waves just below the arch filaments in emerging flux regions 1c. Evolution of magnetic element at the footpoint of emerging flux region 2. Detection of Alfven wave generation 3. Observation of reconnection jets and X-ray signatures in the coronaDaily Note: EIS: Sensitivity monitoring SYNOP002 (3.5 hours) should be run on quiet Sun near disc centre during the two-day plan. Co-alignment program (2hr each for N and E limbs) to be included today. OK to perform in next day if any conflict with science observarions.
Request to XRT HOP Number 0012:
Other Instruments:
Scientific Objectives: 1a. Rise velocity of emerging loops 1b. Shock waves just below the arch filaments in emerging flux regions 1c. Evolution of magnetic element at the footpoint of emerging flux region 2. Detection of Alfven wave generation 3. Observation of reconnection jets and X-ray signatures in the coronaDaily Note: EIS: Sensitivity monitoring SYNOP002 (3.5 hours) should be run on quiet Sun near disc centre during the two-day plan. Co-alignment program (2hr each for N and E limbs) to be included today. OK to perform in next day if any conflict with science observarions.
Request to XRT HOP Number 0012:
Other Instruments:
Scientific Objectives: 1a. Rise velocity of emerging loops 1b. Shock waves just below the arch filaments in emerging flux regions 1c. Evolution of magnetic element at the footpoint of emerging flux region 2. Detection of Alfven wave generation 3. Observation of reconnection jets and X-ray signatures in the coronaDaily Note: EIS: Sensitivity monitoring SYNOP002 (3.5 hours) should be run on quiet Sun near disc centre during the two-day plan. Co-alignment program (2hr each for N and E limbs) to be included today. OK to perform in next day if any conflict with science observarions.
Request to XRT HOP Number 0012:
Other Instruments:
Scientific Objectives: 1a. Rise velocity of emerging loops 1b. Shock waves just below the arch filaments in emerging flux regions 1c. Evolution of magnetic element at the footpoint of emerging flux region 2. Detection of Alfven wave generation 3. Observation of reconnection jets and X-ray signatures in the corona
wavelength: Ti_poly cadence: 14.53 min fov: 2091,2091 images: 26 JavaScript Landing Page
