Search Publications
The Solar Optical Telescope for the Hinode Mission: An Overview
Ichimoto, K.; Tsuneta, S.; Suematsu, Y. +22 more
The Solar Optical Telescope (SOT) aboard the Hinode satellite (formerly called Solar-B) consists of the Optical Telescope Assembly (OTA) and the Focal Plane Package (FPP). The OTA is a 50-cm diffraction-limited Gregorian telescope, and the FPP includes the narrowband filtergraph (NFI) and the broadband filtergraph (BFI), plus the Stokes Spectro-Po…
The Solar Optical Telescope of Solar-B ( Hinode): The Optical Telescope Assembly
Kubo, M.; Ichimoto, K.; Tsuneta, S. +18 more
The Solar Optical Telescope (SOT) aboard the Solar-B satellite (Hinode) is designed to perform high-precision photometric and polarimetric observations of the Sun in visible light spectra (388 - 668 nm) with a spatial resolution of 0.2 - 0.3 arcsec. The SOT consists of two optically separable components: the Optical Telescope Assembly (OTA), consi…
Polarization Calibration of the Solar Optical Telescope onboard Hinode
Ichimoto, K.; Tsuneta, S.; Suematsu, Y. +17 more
The Solar Optical Telescope (SOT) onboard Hinode aims to obtain vector magnetic fields on the Sun through precise spectropolarimetry of solar spectral lines with a spatial resolution of 0.2 - 0.3 arcsec. A photometric accuracy of 10−3 is achieved and, after the polarization calibration, any artificial polarization from crosstalk among S…
Image Stabilization System for Hinode (Solar-B) Solar Optical Telescope
Ichimoto, K.; Kobayashi, K.; Tsuneta, S. +16 more
The Hinode Solar Optical Telescope (SOT) is the first space-borne visible-light telescope that enables us to observe magnetic-field dynamics in the solar lower atmosphere with 0.2 - 0.3 arcsec spatial resolution under extremely stable (seeing-free) conditions. To achieve precise measurements of the polarization with diffraction-limited images, sta…
The Hinode X-Ray Telescope (XRT): Camera Design, Performance and Operations
Weber, M.; Golub, L.; Kano, R. +15 more
The X-ray Telescope (XRT) aboard the Hinode satellite is a grazing incidence X-ray imager equipped with a 2048×2048 CCD. The XRT has 1 arcsec pixels with a wide field of view of 34×34 arcmin. It is sensitive to plasmas with a wide temperature range from < 1 to 30 MK, allowing us to obtain TRACE-like low-temperature images as well as Yohkoh/SXT-…
Dynamics of Sunspot Light Bridges as Revealed by High-Resolution Images from Hinode
Venkatakrishnan, P.; Mathew, Shibu K.; Louis, Rohan E. +1 more
We present G-band and Ca II H filtergrams of two sunspot light bridges in NOAA AR 10953 taken from the 50-cm Solar Optical Telescope onboard the Japanese space satellite Hinode on 1 May 2007. The two light bridges differ in structure, with one of them resembling the filamentary penumbra and the other possessing a dark central lane running along th…
Solar Radio Spikes in 2.6 - 3.8 GHz during the 13 December 2006 Event
Zhang, Y.; Yan, Y. H.; Liu, Y. Y. +3 more
On 13 December 2006, some unusual radio bursts in the range 2.6 - 3.8 GHz were observed during an X3.4 flare/CME event from 02:30 to 04:30 UT in active region NOAA 10930 (S06W27) with the digital spectrometers of the National Astronomical Observatories of China (NAOC). During this event many spikes were detected with the high temporal resolution o…
Lorentz Force: A Possible Driving Force for Sunspot Rotation
Zhang, Hongqi; Liu, Yu; Li, Hui +5 more
Zhao and Kosovichev (Astrophys. J.591, 446, 2003) found two opposite sub-photospheric vortical flows in the depth range of 0 - 12 Mm around a fast rotating sunspot. So far there is no theoretical model explaining such flow motions. In this paper, we try to explain this phenomenon from the point of view of magnetic flux tubes interacting with large…
EIS/ Hinode Observations of Doppler Flow Seen through the 40-Arcsec Wide-Slit
Madjarska, M. S.; Innes, D. E.; Hara, H. +1 more
The Extreme ultraviolet Imaging Spectrometer (EIS) onboard Hinode is the first solar telescope to obtain wide-slit spectral images that can be used for detecting Doppler flows in transition region and coronal lines on the Sun and to relate them to their surrounding small-scale dynamics. We select EIS lines covering the temperature range 6×104…