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The Hinode(Solar-B)Mission: An Overview

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TLDR
The Hinode satellite as discussed by the authors is the successor to the Yohkoh mission, which aims to understand how magnetic energy gets transferred from the photosphere to the upper atmosphere and results in explosive energy releases.
Abstract
The Hinode satellite (formerly Solar-B) of the Japan Aerospace Exploration Agency’s Institute of Space and Astronautical Science (ISAS/JAXA) was successfully launched in September 2006. As the successor to the Yohkoh mission, it aims to understand how magnetic energy gets transferred from the photosphere to the upper atmosphere and results in explosive energy releases. Hinode is an observatory style mission, with all the instruments being designed and built to work together to address the science aims. There are three instruments onboard: the Solar Optical Telescope (SOT), the EUV Imaging Spectrometer (EIS), and the X-Ray Telescope (XRT). This paper provides an overview of the mission, detailing the satellite, the scientific payload, and operations. It will conclude with discussions on how the international science community can participate in the analysis of the mission data.

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The Three-dimensional Analysis of Hinode Polar Jets using Images from LASCO C2, the Stereo COR2 Coronagraphs, and SMEI

TL;DR: In this article, the X-ray Telescope on board the Hinode spacecraft is used to provide high-cadence observations of solar jetting activity, and a selection of the brightest of these polar jets shows a positive correlation with high-speed responses traced into the interplanetary medium.
Journal ArticleDOI

Reappraising Transition Region Line Widths in Light of Recent Alfvén Wave Discoveries

TL;DR: In this article, a new interpretation of ultraviolet transition region emission line widths observed by the SUMER instrument on the Solar and Heliospheric Observatory (SOHO) was provided.
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Successive Two-sided Loop Jets Caused by Magnetic Reconnection between Two Adjacent Filamentary Threads

TL;DR: In this paper, the two successive two-sided loop jets observed by the ground-based New Vacuum Solar Telescope and the space-borne Solar Dynamics Observatory were associated with the interaction of two small-scale adjacent filamentary threads, magnetic emerging, and cancellation processes at the jet's source region.
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Transverse Wave Induced Kelvin-Helmholtz Rolls in Spicules

TL;DR: In this article, the role of transverse MHD waves and associated instabilities in spicule-like features was analyzed and it was shown that transverse wave induced TWIKH rolls lead to coherence of strand-like structure in imaging and spectral maps, as seen in some observations.
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3D Whole-Prominence Fine Structure Modeling

TL;DR: In this paper, the authors presented the first 3D whole-prominence fine structure model, which combines a 3D magnetic field configuration of an entire prominence obtained from nonlinear force-free field simulations, with a detailed description of the prominence plasma.
References
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Journal ArticleDOI

A loop-top hard X-ray source in a compact solar flare as evidence for magnetic reconnection

TL;DR: In this paper, the authors identify the reconnection region as the site of particle acceleration, suggesting that the basic physics of the magnetic reconnection process may be common to both types of flares.
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Sigmoidal morphology and eruptive solar activity

TL;DR: In this paper, the authors studied the Yohkoh Soft X-Ray Telescope video movie for 1993 and 1997 and found that regions are significantly more likely to be eruptive if they are either sigmoidal or large.
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Hot-Plasma Ejections Associated with Compact-Loop Solar Flares

TL;DR: In this article, the authors search for plasma ejections in eight impulsive compact-loop flares near the limb, which are selected in an unbiased manner and include also the Masuda flare, 1992 January 13 flare.
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Statistical Study of Solar X-Ray Jets Observed with the YOHKOH Soft X-Ray Telescope

TL;DR: In this article, a statistical study of 100 X-ray jets, found from the database of full Sun images taken with the Soft X-Ray Telescope (SXT) aboard Yohkoh during the period between November 1991 and April 1992, was conducted.
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