Mark Weber

TL;DR: The X-ray Telescope (XRT) of the Hinode mission as mentioned in this paper provides an unprecedented combination of spatial and temporal resolution in solar coronal studies, and the high sensitivity and broad dynamic range of XRT, coupled with the spacecraft's onboard memory capacity and the planned downlink capability, will permit a broad range of solar studies over an extended period of time for targets ranging from quiet Sun to X-flares.

TL;DR: In this article, the authors examined the contribution of spectral lines and continuum emission to the EUV channels of the Atmospheric Imaging Assembly (AIA) on the Solar Dynamics Observatory (SDO) in different regions of the solar atmosphere.

TL;DR: The most extensive study of polar jet formation and evolution from within both the north and south polar coronal holes so far was performed by Shimojo et al. as discussed by the authors, who measured the apparent outward velocity, the height, the width and the lifetime of the jets.

TL;DR: In this paper, the authors presented the first results of sunspot oscillations from observations by the Interface Region Imaging Spectrograph (IRIS) and identified a strongly nonlinear oscillation in both the slit-jaw images and the spectra of several emission lines formed in the transition region and chromosphere.

TL;DR: Soft x-ray observations of fast bidirectional motions of coronal loops, observed by the Hinode spacecraft, support the existence of this slipping magnetic reconnection regime in the Sun's corona.