2007-05-31T04:23:54.000Z http://sot.lmsal.com Mr. Sam Freeland Lockheed Martin Solar and Astrophysics Laboratory (LMSAL) http://www.lmsal.com Lockheed Martin Advanced Tech Center, 3251 Hanover Rd, O/ADBS, B/252, Palo Alto, CA 94304 null null Hinode XRT Suematsu, Y. Okamoto, T. Kotoku,Jun'ichi 0 Disk center (QS) tracking for Sac Peak Campaign and the full Sun context QR CH, FS, QS, XBP 13 -23.419 0.192 2090.72 2090.72 2007-05-28T15:27:06.000Z 2007-05-28T21:59:10.000Z -23.419 0.192 Cooperative Observations between Hida Observatory and; Hinode Satellite - 1. Emerging Flux Regions 2. Cool Jets 3. Ellerman Bombs QS-CH_and_full_Sun_disk Tim File-OBS_DEC: AR - MHD waves - Ti/Poly (512FOV) - Al/Mesh context - AEC3 ,supperting for Hida Campaign; Daily Note: No need to edit H/W timer, because the AOCS ground software has been updated to fix the bug. Sac Peak CMPN continues (until 30 May). XRT: Weekly focus recalibration included in this timeline. andnbsp; EIS: (QR study, maybe do this today.) After disappearance of AR 10956, limb quiet Sun studies for: a. Absolute wavelength calibration (3.5 hours each at east and west limbs on same day or neighbouring days) b. Line-broadening from just inside the limb to well above (minimum of 7 hours) Hida CMPN, EFR et al. study from 5/28 to 6/3 (Isobe and Kamio santachi are Hinode POCs); 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: No need to edit H/W timer, because the AOCS ground software has been updated to fix the bug. Sac Peak CMPN continues (until 30 May). XRT: Weekly focus recalibration included in this timeline. andnbsp; EIS: (QR study, maybe do this today.) After disappearance of AR 10956, limb quiet Sun studies for: a. Absolute wavelength calibration (3.5 hours each at east and west limbs on same day or neighbouring days) b. Line-broadening from just inside the limb to well above (minimum of 7 hours) Hida CMPN, EFR et al. study from 5/28 to 6/3 (Isobe and Kamio santachi are Hinode POCs); 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: No need to edit H/W timer, because the AOCS ground software has been updated to fix the bug. Sac Peak CMPN continues (until 30 May). XRT: Weekly focus recalibration included in this timeline. andnbsp; EIS: (QR study, maybe do this today.) After disappearance of AR 10956, limb quiet Sun studies for: a. Absolute wavelength calibration (3.5 hours each at east and west limbs on same day or neighbouring days) b. Line-broadening from just inside the limb to well above (minimum of 7 hours) Hida CMPN, EFR et al. study from 5/28 to 6/3 (Isobe and Kamio santachi are Hinode POCs); 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: No need to edit H/W timer, because the AOCS ground software has been updated to fix the bug. Sac Peak CMPN continues (until 30 May). XRT: Weekly focus recalibration included in this timeline. andnbsp; EIS: (QR study, maybe do this today.) After disappearance of AR 10956, limb quiet Sun studies for: a. Absolute wavelength calibration (3.5 hours each at east and west limbs on same day or neighbouring days) b. Line-broadening from just inside the limb to well above (minimum of 7 hours) Hida CMPN, EFR et al. study from 5/28 to 6/3 (Isobe and Kamio santachi are Hinode POCs); 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 ivo://sot.lmsal.com/VOEvent#2007-05-28T15:24:54Z