Time Period of Proposed Observation:
One day in October is preferred since neither Hinode nor IRIS are in eclipse season.
Time window in day, if required:
6 hours continuous overlap observations required with SOT and IRIS on a single day, any time window is acceptable. Observation should fit between synoptics.
Target(s) of interest:
Quiet Sun, disk center (0,0), with Hinode tracking (solar rotation compensation)
Comments:
HOP 182 (2011) and other SOT-only observations have been supported.
Recent resulting publications:
Malherbe, J.-M., Roudier, T., Frank, Z., and Rieutord, M.: 2015, "Families of Granules, Flows, and Acoustic Events in the Solar Atmosphere from Hinode Observations," Solar Physics 290, 321
Roudier, T., Rieutord, M., Prat, V., Malherbe, J. M., Renon, N., Frank, Z., Švanda, M., Berger, T., Burston, R., and Gizon, L.: 2013, "Comparison of solar horizontal velocity fields from SDO/HMI and Hinode data," A&A 552, A113
Malherbe, J.-M., Roudier, T., Rieutord, M., Berger, T., and Franck, Z.: 2012, "Acoustic Events in the Solar Atmosphere from Hinode/SOT NFI Observations," Solar Physics 278, 241
Roudier, T., Malherbe, J., Rieutord, M., Berger, T., Frank, Z., Prat, V., Renon, N., Gizon, L., and Svanda, M.: 2012a, "Some Dynamic Analysis of the Photosphere from Hinode/SOT and SDO/HMI Observations," in L. Golub, I. De Moortel, and T. Shimizu (Eds.), Fifth Hinode Science Meeting, Vol. 456 of Astronomical Society of the Pacific Conference Series, 65
Roudier, T., Rieutord, M., Rincon, F., Malherbe, J.-M., Brito, D., Berger, T., Frank, Z., Parés, L., Bourrec, E., and Beigbeder, F.: 2012b, "The Power Spectrum of the Solar Surface Flows from Hinode Data and First Observations with MOF/CALAS Pic-du-Midi," in T. Sekii, T. Watanabe, and T. Sakurai (Eds.), Hinode-3: The 3rd Hinode Science Meeting, Vol. 454 of Astronomical Society
of the Pacific Conference Series, 47
Malherbe, J.-M., Roudier, T., Berger, T., and Frank, Z.: 2011, "Acoustic Events in the Solar Atmosphere," IEEE Transactions on Plasma Science 39, 2706 |
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