2007-10-06T23:11:07.000Z 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 ARIKAWA,Yusuke STERLING,Alphonse MATSUMOTO,Takuma 14 0 null CH OBS NEAR DISK CENTER AR AR 0 0 0 0 0 2007-10-04T05:58:24.000Z 2007-10-05T10:39:00.000Z 0 0 Hinode/Canary Islands Campaign AR_FOV384_3_filters_7 Daily Note: none; Request to XRT HOP Number 0014: Quiet Sun magnetic fields: high cadence observation covering SOT FOV, with low temperature sensitive filters Active region magnetism: high cadence observation covering the active region ; Other Instruments: VTT TIP: Stokes profiles in FeI 1.56 micron and MnI 1.52 micron TESOS+VIP: 2D Spectropolarimetry in Fe I 630nm THEMIS Fe I 630nm and Ca II IR triplet lines DOT: filtergrams in H alpha, CaII H, and G-band SST: magnetogram and G-band filtergram; Scientific Objectives: We are planning to carry out two kinds of study in this unique opportunity: characterization of quiet Sun magnetic fields including their evolution, and the study of moving magnetic features and flux cancellation events in sunspots. The two problems will be investigated using coordinated observations of Hinode and four solar telescopes in Canary Islands. SOT onboard Hinode and solar telescopes in Canary Islands (SST, VTT, THEMIS, and DOT) will allow us to perform perform high precision spectro-polarimetric measurements in different spectral ranges (in the photosphere and the chromosphere), and imaging observations at the highest spatial resolution possible. All layers of the solar atmosphere will be covered from the photosphere to the corona, by means of XRT and EIS onboard Hinode.Daily Note: none; Request to XRT HOP Number 0014: Quiet Sun magnetic fields: high cadence observation covering SOT FOV, with low temperature sensitive filters Active region magnetism: high cadence observation covering the active region ; Other Instruments: VTT TIP: Stokes profiles in FeI 1.56 micron and MnI 1.52 micron TESOS+VIP: 2D Spectropolarimetry in Fe I 630nm THEMIS Fe I 630nm and Ca II IR triplet lines DOT: filtergrams in H alpha, CaII H, and G-band SST: magnetogram and G-band filtergram; Scientific Objectives: We are planning to carry out two kinds of study in this unique opportunity: characterization of quiet Sun magnetic fields including their evolution, and the study of moving magnetic features and flux cancellation events in sunspots. The two problems will be investigated using coordinated observations of Hinode and four solar telescopes in Canary Islands. SOT onboard Hinode and solar telescopes in Canary Islands (SST, VTT, THEMIS, and DOT) will allow us to perform perform high precision spectro-polarimetric measurements in different spectral ranges (in the photosphere and the chromosphere), and imaging observations at the highest spatial resolution possible. All layers of the solar atmosphere will be covered from the photosphere to the corona, by means of XRT and EIS onboard Hinode.Daily Note: none; Request to XRT HOP Number 0014: Quiet Sun magnetic fields: high cadence observation covering SOT FOV, with low temperature sensitive filters Active region magnetism: high cadence observation covering the active region ; Other Instruments: VTT TIP: Stokes profiles in FeI 1.56 micron and MnI 1.52 micron TESOS+VIP: 2D Spectropolarimetry in Fe I 630nm THEMIS Fe I 630nm and Ca II IR triplet lines DOT: filtergrams in H alpha, CaII H, and G-band SST: magnetogram and G-band filtergram; Scientific Objectives: We are planning to carry out two kinds of study in this unique opportunity: characterization of quiet Sun magnetic fields including their evolution, and the study of moving magnetic features and flux cancellation events in sunspots. The two problems will be investigated using coordinated observations of Hinode and four solar telescopes in Canary Islands. SOT onboard Hinode and solar telescopes in Canary Islands (SST, VTT, THEMIS, and DOT) will allow us to perform perform high precision spectro-polarimetric measurements in different spectral ranges (in the photosphere and the chromosphere), and imaging observations at the highest spatial resolution possible. All layers of the solar atmosphere will be covered from the photosphere to the corona, by means of XRT and EIS onboard Hinode.Daily Note: none; Request to XRT HOP Number 0014: Quiet Sun magnetic fields: high cadence observation covering SOT FOV, with low temperature sensitive filters Active region magnetism: high cadence observation covering the active region ; Other Instruments: VTT TIP: Stokes profiles in FeI 1.56 micron and MnI 1.52 micron TESOS+VIP: 2D Spectropolarimetry in Fe I 630nm THEMIS Fe I 630nm and Ca II IR triplet lines DOT: filtergrams in H alpha, CaII H, and G-band SST: magnetogram and G-band filtergram; Scientific Objectives: We are planning to carry out two kinds of study in this unique opportunity: characterization of quiet Sun magnetic fields including their evolution, and the study of moving magnetic features and flux cancellation events in sunspots. The two problems will be investigated using coordinated observations of Hinode and four solar telescopes in Canary Islands. SOT onboard Hinode and solar telescopes in Canary Islands (SST, VTT, THEMIS, and DOT) will allow us to perform perform high precision spectro-polarimetric measurements in different spectral ranges (in the photosphere and the chromosphere), and imaging observations at the highest spatial resolution possible. All layers of the solar atmosphere will be covered from the photosphere to the corona, by means of XRT and EIS onboard Hinode.Daily Note: none; Request to XRT HOP Number 0014: Quiet Sun magnetic fields: high cadence observation covering SOT FOV, with low temperature sensitive filters Active region magnetism: high cadence observation covering the active region ; Other Instruments: VTT TIP: Stokes profiles in FeI 1.56 micron and MnI 1.52 micron TESOS+VIP: 2D Spectropolarimetry in Fe I 630nm THEMIS Fe I 630nm and Ca II IR triplet lines DOT: filtergrams in H alpha, CaII H, and G-band SST: magnetogram and G-band filtergram; Scientific Objectives: We are planning to carry out two kinds of study in this unique opportunity: characterization of quiet Sun magnetic fields including their evolution, and the study of moving magnetic features and flux cancellation events in sunspots. The two problems will be investigated using coordinated observations of Hinode and four solar telescopes in Canary Islands. SOT onboard Hinode and solar telescopes in Canary Islands (SST, VTT, THEMIS, and DOT) will allow us to perform perform high precision spectro-polarimetric measurements in different spectral ranges (in the photosphere and the chromosphere), and imaging observations at the highest spatial resolution possible. All layers of the solar atmosphere will be covered from the photosphere to the corona, by means of XRT and EIS onboard Hinode.Daily Note: none; Request to XRT HOP Number 0014: Quiet Sun magnetic fields: high cadence observation covering SOT FOV, with low temperature sensitive filters Active region magnetism: high cadence observation covering the active region ; Other Instruments: VTT TIP: Stokes profiles in FeI 1.56 micron and MnI 1.52 micron TESOS+VIP: 2D Spectropolarimetry in Fe I 630nm THEMIS Fe I 630nm and Ca II IR triplet lines DOT: filtergrams in H alpha, CaII H, and G-band SST: magnetogram and G-band filtergram; Scientific Objectives: We are planning to carry out two kinds of study in this unique opportunity: characterization of quiet Sun magnetic fields including their evolution, and the study of moving magnetic features and flux cancellation events in sunspots. The two problems will be investigated using coordinated observations of Hinode and four solar telescopes in Canary Islands. SOT onboard Hinode and solar telescopes in Canary Islands (SST, VTT, THEMIS, and DOT) will allow us to perform perform high precision spectro-polarimetric measurements in different spectral ranges (in the photosphere and the chromosphere), and imaging observations at the highest spatial resolution possible. All layers of the solar atmosphere will be covered from the photosphere to the corona, by means of XRT and EIS onboard Hinode.Daily Note: none; Request to XRT HOP Number 0014: Quiet Sun magnetic fields: high cadence observation covering SOT FOV, with low temperature sensitive filters Active region magnetism: high cadence observation covering the active region ; Other Instruments: VTT TIP: Stokes profiles in FeI 1.56 micron and MnI 1.52 micron TESOS+VIP: 2D Spectropolarimetry in Fe I 630nm THEMIS Fe I 630nm and Ca II IR triplet lines DOT: filtergrams in H alpha, CaII H, and G-band SST: magnetogram and G-band filtergram; Scientific Objectives: We are planning to carry out two kinds of study in this unique opportunity: characterization of quiet Sun magnetic fields including their evolution, and the study of moving magnetic features and flux cancellation events in sunspots. The two problems will be investigated using coordinated observations of Hinode and four solar telescopes in Canary Islands. SOT onboard Hinode and solar telescopes in Canary Islands (SST, VTT, THEMIS, and DOT) will allow us to perform perform high precision spectro-polarimetric measurements in different spectral ranges (in the photosphere and the chromosphere), and imaging observations at the highest spatial resolution possible. All layers of the solar atmosphere will be covered from the photosphere to the corona, by means of XRT and EIS onboard Hinode.Daily Note: none; Request to XRT HOP Number 0014: Quiet Sun magnetic fields: high cadence observation covering SOT FOV, with low temperature sensitive filters Active region magnetism: high cadence observation covering the active region ; Other Instruments: VTT TIP: Stokes profiles in FeI 1.56 micron and MnI 1.52 micron TESOS+VIP: 2D Spectropolarimetry in Fe I 630nm THEMIS Fe I 630nm and Ca II IR triplet lines DOT: filtergrams in H alpha, CaII H, and G-band SST: magnetogram and G-band filtergram; Scientific Objectives: We are planning to carry out two kinds of study in this unique opportunity: characterization of quiet Sun magnetic fields including their evolution, and the study of moving magnetic features and flux cancellation events in sunspots. The two problems will be investigated using coordinated observations of Hinode and four solar telescopes in Canary Islands. SOT onboard Hinode and solar telescopes in Canary Islands (SST, VTT, THEMIS, and DOT) will allow us to perform perform high precision spectro-polarimetric measurements in different spectral ranges (in the photosphere and the chromosphere), and imaging observations at the highest spatial resolution possible. All layers of the solar atmosphere will be covered from the photosphere to the corona, by means of XRT and EIS onboard Hinode.Daily Note: none; Request to XRT HOP Number 0014: Quiet Sun magnetic fields: high cadence observation covering SOT FOV, with low temperature sensitive filters Active region magnetism: high cadence observation covering the active region ; Other Instruments: VTT TIP: Stokes profiles in FeI 1.56 micron and MnI 1.52 micron TESOS+VIP: 2D Spectropolarimetry in Fe I 630nm THEMIS Fe I 630nm and Ca II IR triplet lines DOT: filtergrams in H alpha, CaII H, and G-band SST: magnetogram and G-band filtergram; Scientific Objectives: We are planning to carry out two kinds of study in this unique opportunity: characterization of quiet Sun magnetic fields including their evolution, and the study of moving magnetic features and flux cancellation events in sunspots. The two problems will be investigated using coordinated observations of Hinode and four solar telescopes in Canary Islands. SOT onboard Hinode and solar telescopes in Canary Islands (SST, VTT, THEMIS, and DOT) will allow us to perform perform high precision spectro-polarimetric measurements in different spectral ranges (in the photosphere and the chromosphere), and imaging observations at the highest spatial resolution possible. All layers of the solar atmosphere will be covered from the photosphere to the corona, by means of XRT and EIS onboard Hinode.Daily Note: none; Request to XRT HOP Number 0014: Quiet Sun magnetic fields: high cadence observation covering SOT FOV, with low temperature sensitive filters Active region magnetism: high cadence observation covering the active region ; Other Instruments: VTT TIP: Stokes profiles in FeI 1.56 micron and MnI 1.52 micron TESOS+VIP: 2D Spectropolarimetry in Fe I 630nm THEMIS Fe I 630nm and Ca II IR triplet lines DOT: filtergrams in H alpha, CaII H, and G-band SST: magnetogram and G-band filtergram; Scientific Objectives: We are planning to carry out two kinds of study in this unique opportunity: characterization of quiet Sun magnetic fields including their evolution, and the study of moving magnetic features and flux cancellation events in sunspots. The two problems will be investigated using coordinated observations of Hinode and four solar telescopes in Canary Islands. SOT onboard Hinode and solar telescopes in Canary Islands (SST, VTT, THEMIS, and DOT) will allow us to perform perform high precision spectro-polarimetric measurements in different spectral ranges (in the photosphere and the chromosphere), and imaging observations at the highest spatial resolution possible. All layers of the solar atmosphere will be covered from the photosphere to the corona, by means of XRT and EIS onboard Hinode.Daily Note: none; Request to XRT HOP Number 0014: Quiet Sun magnetic fields: high cadence observation covering SOT FOV, with low temperature sensitive filters Active region magnetism: high cadence observation covering the active region ; Other Instruments: VTT TIP: Stokes profiles in FeI 1.56 micron and MnI 1.52 micron TESOS+VIP: 2D Spectropolarimetry in Fe I 630nm THEMIS Fe I 630nm and Ca II IR triplet lines DOT: filtergrams in H alpha, CaII H, and G-band SST: magnetogram and G-band filtergram; Scientific Objectives: We are planning to carry out two kinds of study in this unique opportunity: characterization of quiet Sun magnetic fields including their evolution, and the study of moving magnetic features and flux cancellation events in sunspots. The two problems will be investigated using coordinated observations of Hinode and four solar telescopes in Canary Islands. SOT onboard Hinode and solar telescopes in Canary Islands (SST, VTT, THEMIS, and DOT) will allow us to perform perform high precision spectro-polarimetric measurements in different spectral ranges (in the photosphere and the chromosphere), and imaging observations at the highest spatial resolution possible. All layers of the solar atmosphere will be covered from the photosphere to the corona, by means of XRT and EIS onboard Hinode.Daily Note: none; Request to XRT HOP Number 0014: Quiet Sun magnetic fields: high cadence observation covering SOT FOV, with low temperature sensitive filters Active region magnetism: high cadence observation covering the active region ; Other Instruments: VTT TIP: Stokes profiles in FeI 1.56 micron and MnI 1.52 micron TESOS+VIP: 2D Spectropolarimetry in Fe I 630nm THEMIS Fe I 630nm and Ca II IR triplet lines DOT: filtergrams in H alpha, CaII H, and G-band SST: magnetogram and G-band filtergram; Scientific Objectives: We are planning to carry out two kinds of study in this unique opportunity: characterization of quiet Sun magnetic fields including their evolution, and the study of moving magnetic features and flux cancellation events in sunspots. The two problems will be investigated using coordinated observations of Hinode and four solar telescopes in Canary Islands. SOT onboard Hinode and solar telescopes in Canary Islands (SST, VTT, THEMIS, and DOT) will allow us to perform perform high precision spectro-polarimetric measurements in different spectral ranges (in the photosphere and the chromosphere), and imaging observations at the highest spatial resolution possible. All layers of the solar atmosphere will be covered from the photosphere to the corona, by means of XRT and EIS onboard Hinode.Daily Note: none; Request to XRT HOP Number 0014: Quiet Sun magnetic fields: high cadence observation covering SOT FOV, with low temperature sensitive filters Active region magnetism: high cadence observation covering the active region ; Other Instruments: VTT TIP: Stokes profiles in FeI 1.56 micron and MnI 1.52 micron TESOS+VIP: 2D Spectropolarimetry in Fe I 630nm THEMIS Fe I 630nm and Ca II IR triplet lines DOT: filtergrams in H alpha, CaII H, and G-band SST: magnetogram and G-band filtergram; Scientific Objectives: We are planning to carry out two kinds of study in this unique opportunity: characterization of quiet Sun magnetic fields including their evolution, and the study of moving magnetic features and flux cancellation events in sunspots. The two problems will be investigated using coordinated observations of Hinode and four solar telescopes in Canary Islands. SOT onboard Hinode and solar telescopes in Canary Islands (SST, VTT, THEMIS, and DOT) will allow us to perform perform high precision spectro-polarimetric measurements in different spectral ranges (in the photosphere and the chromosphere), and imaging observations at the highest spatial resolution possible. All layers of the solar atmosphere will be covered from the photosphere to the corona, by means of XRT and EIS onboard Hinode.