XRT: COALIGNMENT North Pole
2007-05-14T11:19:36 to 2007-05-14T13:18:03
Science Goal: CDS/UVCS + Ulysses Campaign
Program: Co-alignment_N_limb
Target: FS
xcen=264 ycen=930
Instrument: XRT
HOP/JOP: 0
Description:
Tim File-OBS_DEC: AR - Microflares and Topology - Ti/Poly, Thick-Al, Thick-Be pairs, G-band - contexts + 512 - high cadence
Daily Note: Plan to upload orbital elements on Tuesday, not on Monday. This is because an expert is required to manually edit AOCS orl file after completing poiting plan. Shimizu/Bando are out of office on Monday. EIS: Would like to run a variety of active region programs. XRT: Ditto
also request co-alignment program to be included in this upload. SOT: Ditto STEREO CMPN continues (but currently this is a passive cmpn vis-a-vis Hinode). Co-alignment program (2hr each for N and E limbs) to be run today.
Request to XRT HOP Number 0007:
Other Instruments: SoHO/CDS, UVCS
SoHO keyhole starts 17-May (26m dish) and 21-May (34m dish) STEREO/SECCHI Ulysses will be ending the quadrature with SOHO. Ulysses will be at a latitude of 55 deg (south-west), in the plane of the sky. Hence any active region say between 45 and 65 degree south that might be near the limb would contribute to the solar wind measured in-situ by Ulysses. Scintillation measurement (G. Poletto)
Scientific Objectives: The main aim is to measure chemical abundances in active regions as a function of height for 1.0 andlt
R(Sun) andlt
1.6 using SOHO/CDS, Hinode/EIS, SOHO/UVCS, and to link them with in-situ measurements by Ulysses. A secondary aim is to measure electron temperatures, densities, and ionization state of the plasma as function of height from 1.0 to 1.6 solar radii using SOHO/CDS and Hinode/EIS. There have been no previous spectroscopic observations in the range 1.2 and
#8211
1.6 R(Sun).Daily Note: Plan to upload orbital elements on Tuesday, not on Monday. This is because an expert is required to manually edit AOCS orl file after completing poiting plan. Shimizu/Bando are out of office on Monday. EIS: Would like to run a variety of active region programs. XRT: Ditto
also request co-alignment program to be included in this upload. SOT: Ditto STEREO CMPN continues (but currently this is a passive cmpn vis-a-vis Hinode). Co-alignment program (2hr each for N and E limbs) to be run today.
Request to XRT HOP Number 0007:
Other Instruments: SoHO/CDS, UVCS
SoHO keyhole starts 17-May (26m dish) and 21-May (34m dish) STEREO/SECCHI Ulysses will be ending the quadrature with SOHO. Ulysses will be at a latitude of 55 deg (south-west), in the plane of the sky. Hence any active region say between 45 and 65 degree south that might be near the limb would contribute to the solar wind measured in-situ by Ulysses. Scintillation measurement (G. Poletto)
Scientific Objectives: The main aim is to measure chemical abundances in active regions as a function of height for 1.0 andlt
R(Sun) andlt
1.6 using SOHO/CDS, Hinode/EIS, SOHO/UVCS, and to link them with in-situ measurements by Ulysses. A secondary aim is to measure electron temperatures, densities, and ionization state of the plasma as function of height from 1.0 to 1.6 solar radii using SOHO/CDS and Hinode/EIS. There have been no previous spectroscopic observations in the range 1.2 and
#8211
1.6 R(Sun).Daily Note: Plan to upload orbital elements on Tuesday, not on Monday. This is because an expert is required to manually edit AOCS orl file after completing poiting plan. Shimizu/Bando are out of office on Monday. EIS: Would like to run a variety of active region programs. XRT: Ditto
also request co-alignment program to be included in this upload. SOT: Ditto STEREO CMPN continues (but currently this is a passive cmpn vis-a-vis Hinode). Co-alignment program (2hr each for N and E limbs) to be run today.
Request to XRT HOP Number 0007:
Other Instruments: SoHO/CDS, UVCS
SoHO keyhole starts 17-May (26m dish) and 21-May (34m dish) STEREO/SECCHI Ulysses will be ending the quadrature with SOHO. Ulysses will be at a latitude of 55 deg (south-west), in the plane of the sky. Hence any active region say between 45 and 65 degree south that might be near the limb would contribute to the solar wind measured in-situ by Ulysses. Scintillation measurement (G. Poletto)
Scientific Objectives: The main aim is to measure chemical abundances in active regions as a function of height for 1.0 andlt
R(Sun) andlt
1.6 using SOHO/CDS, Hinode/EIS, SOHO/UVCS, and to link them with in-situ measurements by Ulysses. A secondary aim is to measure electron temperatures, densities, and ionization state of the plasma as function of height from 1.0 to 1.6 solar radii using SOHO/CDS and Hinode/EIS. There have been no previous spectroscopic observations in the range 1.2 and
#8211
1.6 R(Sun).
wavelength: Ti_poly cadence: 6.62 min fov: 1585,2114 images: 18 JavaScript Landing Page
