2007-05-22T08:19:47.000Z 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 Kano Sterling, A. Ishibashi, B 0 Synoptic FS FS, SYN 15 -5.938 -0.024 2090.72 2090.72 2007-05-20T17:16:07.000Z 2007-05-20T20:46:17.000Z -5.938 -0.024 CDS/UVCS + Ulysses Campaign Synoptic_7_multi_filters_FW1/FW2_1 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). ivo://sot.lmsal.com/VOEvent#2007-05-20T17:14:00Z