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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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Light bridge in a developing active region. ii. numerical simulation of flux emergence and light bridge formation

TL;DR: In this paper, the authors investigated the detailed magnetic and velocity structures and the formation mechanism of light bridges and found that a weakly magnetized plasma upflow in the near-surface layers of the convection zone is entrained between the emerging magnetic bundles that appear as pores at the solar surface.
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Intensity contrast of solar network and faculae

TL;DR: In this article, the spectral line changes were found to be a significant driver of facular contribution to variation in solar irradiance, and the discrepancy between the continuum contrast reported here and in the literature was shown to arise mainly from the treatment of magnetic signals adjacent to sunspots and pores.
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Inferring the magnetic field vector in the quiet Sun - I. Photon noise and selection criteria

TL;DR: In this paper, the authors investigated whether it is possible to accurately retrieve the magnetic field vector in regions with very low polarization signals (e.g. internetwork), employing the FeI line pair at 6300 A.
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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