The EUV Imaging Spectrometer for Hinode

By J. Culhane, L. Harra, A. James, K. Al-Janabi, L. Bradley, R. Chaudry, K. Rees, J. Tandy, P. Thomas, M. C. R. Whillock and 29 more. 2007

898 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/191101d377d3854e6d57e87d53989916f49d0de7

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In Astronomy and Astrophysics

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Citations in the corpus

• OBSERVING THE ROOTS OF SOLAR CORONAL HEATING—IN THE CHROMOSPHERE (2009, methodology): “To study the thermal evolution of these spicules, we use simultaneous observations of Ca ii H emission (with SOT) and EUV spectral lines formed in the corona at temperatures of several million K from the Extreme-ultraviolet Imaging Spectrometer (EIS; Culhane et al. 2007).”
• GLOBAL ENERGETICS OF THIRTY-EIGHT LARGE SOLAR ERUPTIVE EVENTS (2012, methodology): “For example, the detailed differential emission measure analysis now possible using data from the EUV Imaging Spectrometer (EIS; Culhane et al. 2007) on Hinode, and from the Atmospheric Imaging Assembly (AIA; Lemen et al. 2012) and the Extreme Ultraviolet Variability Experiment (EVE; Woods et al.…”
• TIME–DISTANCE SEISMOLOGY OF THE SOLAR CORONA WITH CoMP (2009, methodology): “Recent analysis of spectra from the EIS instrument (Culhane et al. 2007) on Hinode (Kosugi et al. 2007) show a portion of the corona oscillating at a period very near 5 minutes with a peak-to-peak amplitude of 2 km/s (Van Doorsselaere et al. 2008), indicating that these ubiquitous waves may be…”
• SDO/AIA response to coronal hole, quiet Sun, active region, and flare plasma (2010, methodology): “The AR DEM (O’Dwyer et al. 2010) was obtained from AR intensities measured by the EUV Imaging Spectrometer (EIS; Culhane et al. 2007) on Hinode.”
• Flows and Nonthermal Velocities in Solar Active Regions Observed with the EUV Imaging Spectrometer on Hinode: A Tracer of Active Region Sources of Heliospheric Magnetic Fields? (2008, methodology): “THE EIS ON HINODE The EIS is described in detail by Culhane et al. (2007) and Korendyke et al. (2006).”
• A SYSTEMATIC SURVEY OF HIGH-TEMPERATURE EMISSION IN SOLAR ACTIVE REGIONS (2012, background): “For each region we compute the differential emission measure (DEM) in the active region core using observations from the EUV Imaging Spectrograph (EIS) and the Atmospheric Imaging Assembly (AIA).”
• VELOCITY CHARACTERISTICS OF EVAPORATED PLASMA USING HINODE/EUV IMAGING SPECTROMETER (2009, methodology): “With the launch of Hinode (Kosugi et al. 2007) in September 2006, it is now possible to investigate the process of chromospheric evaporation by observing several high-temperature lines simultaneously with the EUV Imaging Spectrometer (EIS; Culhane et al. 2007).”
• High-precision density measurements in the solar corona I. Analysis methods and results for Fe XII and Fe XIII (2008, methodology): “A key factor is the high sensitivity of the instrument which is enabled by a simple optical design that incorporates multilayer coatings (Culhane et al. 2007).”
• An Observational Overview of Solar Flares (2011, background): “The improved spatial, spectral and temporal capabilities of the Extreme Ultraviolet Imaging Spectrometer (EIS) onboardHinode has also been used to study chromospheric evaporation using emission lines formed over a broad range of temperatures (Milligan & Dennis 2009).”
• The FIP and Inverse FIP Effects in Solar and Stellar Coronae (2015, background): “However, Hinode/EIS does offer imaging spectroscopy sensitive to the FIP effect, as demonstrated by Baker et al. (2013).”
• Observations of Turbulent Magnetic Reconnection within a Solar Current Sheet (2018, background): “The X-Ray Telescope (XRT; Golub et al. 2007) and EUV Imaging Spectrometer (EIS; Culhane et al. 2007) on board Hinode (Kosugi et al. 2007) provide the X-ray images and EUV spectra in the wavelength ranges of 170–210 Å (short) and 250–290 Å (long) with a spectral resolution of 0.0223 Å pixel−1,…”
• Differential Emission Measures from the Regularized Inversion of Hinode and SDO data (2012, methodology): “Using the information given we use CHIANTI to calculate the contribution functions for the 24 EIS lines, and with the Hinode/XRT temperature response function for the Al-thick filter (Golub et al. 2007), and the quoted intensities and errors we calculate the zeroth-order regularized solutions and α ”
• Advances in Observing Various Coronal EUV Waves in the SDO Era and Their Seismological Applications (Invited Review) (2014, neutral): “…wave in a narrow slit, e.g. with the SOHO/Coronal Diagnostic Spectrometer (CDS: Harrison et al., 1995) and the Hinode/EUV Imaging Spectrometer (EIS: Culhane et al., 2007), such studies have been performed for only a few events (Harra and Sterling, 2003; Chen and Ding, 2010; West et al., 2011;…”
• The Solar Optical Telescope of Solar-B (Hinode): The Optical Telescope Assembly (2008, background): “…between the photosphere and the upper layers to understand the mechanism of dynamics and heating with the help of the coordinated observations from the X-Ray Telescope (Golub et al., 2007; Kano et al., 2008) and EUV Imaging Spectrometer (Culhane et al., 2007) flown on Hinode (Kosugi et al., 2007).”