Observation

Observation Details

XRT: Active region tracking across disk

2007-05-21T00:12:06 to 2007-05-21T11:00:33

Science Goal: CDS/UVCS + Ulysses Campaign

Program: AR_on_disk_7

Target: AR

xcen=363 ycen=47

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: none EIS: 3.6 hours quiet Sun andnbsp
for instrument sensitivity monitoring andnbsp
in saturday's upload plan (already discussed yesterday). Co-alignment program (2hr each for N and E limbs) may run once every a few days, depending on the satellite temperatures and science programs.
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: none EIS: 3.6 hours quiet Sun andnbsp
for instrument sensitivity monitoring andnbsp
in saturday's upload plan (already discussed yesterday). Co-alignment program (2hr each for N and E limbs) may run once every a few days, depending on the satellite temperatures and science programs.
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: none EIS: 3.6 hours quiet Sun andnbsp
for instrument sensitivity monitoring andnbsp
in saturday's upload plan (already discussed yesterday). Co-alignment program (2hr each for N and E limbs) may run once every a few days, depending on the satellite temperatures and science programs.
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: none EIS: 3.6 hours quiet Sun andnbsp
for instrument sensitivity monitoring andnbsp
in saturday's upload plan (already discussed yesterday). Co-alignment program (2hr each for N and E limbs) may run once every a few days, depending on the satellite temperatures and science programs.
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: none EIS: 3.6 hours quiet Sun andnbsp
for instrument sensitivity monitoring andnbsp
in saturday's upload plan (already discussed yesterday). Co-alignment program (2hr each for N and E limbs) may run once every a few days, depending on the satellite temperatures and science programs.
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: none EIS: 3.6 hours quiet Sun andnbsp
for instrument sensitivity monitoring andnbsp
in saturday's upload plan (already discussed yesterday). Co-alignment program (2hr each for N and E limbs) may run once every a few days, depending on the satellite temperatures and science programs.
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: none EIS: 3.6 hours quiet Sun andnbsp
for instrument sensitivity monitoring andnbsp
in saturday's upload plan (already discussed yesterday). Co-alignment program (2hr each for N and E limbs) may run once every a few days, depending on the satellite temperatures and science programs.
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: none EIS: 3.6 hours quiet Sun andnbsp
for instrument sensitivity monitoring andnbsp
in saturday's upload plan (already discussed yesterday). Co-alignment program (2hr each for N and E limbs) may run once every a few days, depending on the satellite temperatures and science programs.
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: none EIS: 3.6 hours quiet Sun andnbsp
for instrument sensitivity monitoring andnbsp
in saturday's upload plan (already discussed yesterday). Co-alignment program (2hr each for N and E limbs) may run once every a few days, depending on the satellite temperatures and science programs.
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: none EIS: 3.6 hours quiet Sun andnbsp
for instrument sensitivity monitoring andnbsp
in saturday's upload plan (already discussed yesterday). Co-alignment program (2hr each for N and E limbs) may run once every a few days, depending on the satellite temperatures and science programs.
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: none EIS: 3.6 hours quiet Sun andnbsp
for instrument sensitivity monitoring andnbsp
in saturday's upload plan (already discussed yesterday). Co-alignment program (2hr each for N and E limbs) may run once every a few days, depending on the satellite temperatures and science programs.
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: none EIS: 3.6 hours quiet Sun andnbsp
for instrument sensitivity monitoring andnbsp
in saturday's upload plan (already discussed yesterday). Co-alignment program (2hr each for N and E limbs) may run once every a few days, depending on the satellite temperatures and science programs.
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: none EIS: 3.6 hours quiet Sun andnbsp
for instrument sensitivity monitoring andnbsp
in saturday's upload plan (already discussed yesterday). Co-alignment program (2hr each for N and E limbs) may run once every a few days, depending on the satellite temperatures and science programs.
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: none EIS: 3.6 hours quiet Sun andnbsp
for instrument sensitivity monitoring andnbsp
in saturday's upload plan (already discussed yesterday). Co-alignment program (2hr each for N and E limbs) may run once every a few days, depending on the satellite temperatures and science programs.
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).

Annotations:

Chief Observer

Ishibashi, B

Related Links
Cites: Active region tracking across disk

Timeline: gif use