2007-06-04T12:05:45.000Z http://sot.lmsal.com Ed DeLuca SAO http://hea-www.harvard.edu MS 58, 60 Garden St, Cambridge, MA 02138 +1-617-496-7725 edeluca@cfa.harvard.edu Hinode XRT Suematsu, Y. Okamoto, T. Kotoku,Jun'ichi 12 0 null Active region tracking across disk for HIda campaign AR, FS, SS, XBP 10956 AR 0 5.2 -0.1 0 0 2007-05-28T21:59:54.000Z 2007-05-29T00:09:54.000Z 5.2 -0.1 Cooperative Observations between Hida Observatory and; Hinode Satellite - 1. Emerging Flux Regions 2. Cool Jets 3. Ellerman Bombs Plage_for_Hida_CMPN 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 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