Hinode (was Solar-B) was launched at 6:36 a.m. on September 23, 2006 (Japan Standard Time).
New XPOW: Full Disk Focus Mode
New XPOW: Overlapogram
New XPOW: The West Limb
Press Release: Searing Sun Seen in X-rays Visit NASA or The Royal Astronomical Society to read about an observation campaign that combined Hinode XRT images with high-energy X-rays from the NuSTAR satellite.
New XPOW: A Solar Facelift
Big News! Hinode gets excellent ratings in 2015 NASA Senior Review. The Hinode team has received the results from the NASA Senior Review panel for the heliophysics missions. Our science, as well as our role in the NASA heliophysics fleet, were highly regarded in their report. (Science value was "excellent", "future contributions promise to be compelling".) The budget recommendations were also about as good as could be hoped for. The XRT community is well-positioned to move forward with another two years of discovery and science!
New XPOW: A Long, Bright Flare
New XPOW: Four Active Regions
New XPOW: Swept Away
New XPOW: Looking Through the Atmosphere
New XPOW: A Sympathetic Flare
Big News! Hinode Scientist Patrick McCauley was awarded the Fulbright Scholarship. Patrick will begin a Ph.D. in solar physics at the University of Sydney next year. Congratulations from the Hinode/XRT Team Patrick! We will miss you but look forward to calling you Dr. McCauley.
New XPOW: Three Years in the Life of XRT
New XPOW: Prominence Eruption
See the XRT News page for older XRT news items.
The Hinode X-Ray Telescope (XRT) is a high-resolution grazing-incidence telescope, which is a successor to the highly successful Yohkoh Soft X-Ray Telescope (SXT). A primary purpose of the Hinode XRT is to observe the generation, transport, and emergence of solar magnetic fields, as well as the ultimate dissipation of magnetic energy in forms such as flares and pico-flares, coronal heating, and coronal mass ejections. The XRT aboard Hinode observes the dissipation part of the life-cycle story of solar magnetic fields. High-resolution soft X-ray images reveal magnetic field configuration and its evolution, allowing us to observe the energy buildup, storage and release process in the corona for any transient event. One of the unique features of XRT is its wide temperature coverage to see all the coronal features that are not seen with any normal incidence telescope.
The XRT consists of the X-ray and visible light optics, focal plane mechanisms (filters and shutter), and the 2k x 2k CCD camera. The Mission Data Processor (MDP) also plays a vital role for XRT.
The XRT was designed and developed by the Japan-US collaboration between Smithsonian Astrophysical Observatory (SAO), NASA MSFC, JAXA, and NAOJ. The XRT telescope was tested and calibrated at the XRCF at MSFC, and the CCD camera was tested and calibrated in X-rays at the ATC of the NAOJ with JAXA.
If XRT data is used in a published article or report, please give a proper Acknowledgement:
"Hinode is a Japanese mission developed and launched by ISAS/JAXA, with NAOJ as domestic partner and NASA and STFC (UK) as international partners. It is operated by these agencies in co-operation with ESA and the NSC (Norway)."
If an XRT image is displayed in a popular article, on a website, et cetera, then please acknowledge the contributing institutions:
"(SAO, NASA, JAXA, NAOJ)"
You may find a list of the XRT instrument papers and other important references that should be considered for inclusion in your XRT science paper HERE.