[3] The mission was extended to the end of 2020 with a likely extension lasting until 2022.[4]. At the SOT focal plane, the Focal Plane Package (FPP) built by the Lockheed Martin Solar and Astrophysics Laboratory in Palo Alto, California consists of three optical instruments: the Broadband Filter Imager (BFI) which produces images of the solar photosphere and chromosphere in six wide-band interference filters; the Narrowband Filter Imager (NFI) which is a tunable Lyot-type birefringent filter capable of producing magnetogram and dopplergram images of the solar surface; and the Spectropolarimeter (SP) which produces the most sensitive vector magnetograph maps of the photosphere to date. [5] Spatial resolution is around 2 arcsec, and the field of view is up to 560 x 512 arcsec2. Hinode was planned as a three-year mission to explore the magnetic fields of the Sun. Hinode (/ˈhiːnoʊdeɪ/; Japanese: ひので, IPA: [çinode], Sunrise), formerly Solar-B, is a Japan Aerospace Exploration Agency Solar mission with United States and United Kingdom collaboration. JAXA and the National Astronomical Observatory of Japan worked on the telescope optics and the U.S. National Aeronautics and Space Administration (NASA) developed the focal-plane package (FPP). Launched on a Japanese M-V rocket out of Kagoshima, Japan, on September 23, 2006, Hinode is led by the Japan Aerospace Exploration Agency, or JAXA. また、極端紫外線撮像分光装置は、彩層より上部の構造から放射される輝線を分光観測し、コロナの加熱領域から流れ出す高速のフローをとらえた。可視光望遠鏡とX線望遠鏡は日米協力、極端紫外線撮像分光装置は日英米の国際協力により開発された。 Artist's impression of the Hinode spacecraft (then known as Solar-B) in orbit, EIS (Extreme-Ultraviolet Imaging Spectrometer), Lockheed Martin Solar and Astrophysics Laboratory, "Solar observatory launched to space by Japanese rocket", National Astronomical Observatory of Japan, HINODE (SOLAR-B) SOT-FPP Education/Public Outreach, https://en.wikipedia.org/w/index.php?title=Hinode_(satellite)&oldid=984356865, Articles containing Japanese-language text, Creative Commons Attribution-ShareAlike License, Superscripts indicate joint development with, This page was last edited on 19 October 2020, at 18:01. On 28 October 2006, the probe's instruments captured their first images. It consists of a coordinated set of optical, extreme ultraviolet (EUV), and x-ray instruments to investigate the interaction between the Sun's magnetic field and its corona. HINODE will carry a coordinated set of optical, X-ray, and EUV instruments that will perform highly accurate measurements of magnetic fields, electrical currents and velocity fields in the solar atmosphere and corona. Hinode is the third Japanese Solar astronomical satellite (following Hinotori and Yohkoh) launched on September 23, 2006 by the M-V rocket. The HINODE (SOLAR-B), which is the successor to the orbiting solar observatory YOHKOH (SOLAR-A), was launched at 6:36 a.m. on September 23, 2006 (JST) by the M-V Launch Vehicle No.7 from the Uchinoura Space Center. if(document.charset!="utf-8"){ A 0.5 meter Gregorian optical telescope with an angular resolution of about 0.2 arcsecond over the field of view of about 400 x 400 arcsec. }); window.dataLayer = window.dataLayer || []; Then the satellite maneuvered to the quasi-circular sun-synchronous orbit over the day/night ter… The Hinode mission is a collaboration between the space agencies of Japan, the United States, the United Kingdom and Europe. HINODE will operate for at least three years. The result will be an improved understanding of the mechanisms of solar explosions, which will in turn greatly help us predict how solar events affect Earth. 6000度の太陽光球の外層にあるコロナがどのように100万度まで加熱されているかの解明を目的として、宇宙科学研究所（ISAS）により開発された太陽観測衛星。第22号科学衛星でコードネームはSOLAR-B。2006年9月23日に内之浦宇宙空間観測所よりM-Vロケット7号機により打ち上げられた後、「ひので」と名づけられた。 The telescope has an imaging field of view of 34 arcminutes. Initial orbit was perigee height 280 km, apogee height 686 km, inclination 98.3 degrees. 1 Overview of “Hinode” 2 Characteristics of the Advanced Telescopes 3 -Want to The satellite systems were developed by JAXA and Mitsubishi Electric Corporation. The telescope was designed and built by Smithsonian Astrophysical Observatory (SAO), which, with the Harvard College Observatory (HCO) form the Harvard-Smithsonian Center for Astrophysics (CfA). These magnetic fields are much smaller and have shorter lifetimes than sunspots. It is the follow-up to the Yohkoh (Solar-A) mission and it was launched on the final flight of the M-V rocket from Uchinoura Space Center, Japan on 22 September 2006 at 21:36 UTC (23 September, 06:36 JST). The camera was developed by NAOJ and JAXA. Each party had the following responsibilities. A modified Wolter I telescope design that uses grazing incidence optics to image the solar corona's hottest components (0.5 to 10 Million K) with an angular resolution consistent with 1 arcsec pixels at the CCD.