Chromospheric/coronal spectroheliograph
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Troy W. Barbee | Arthur B. C. Walker | Dennis S. Martinez-Galarce | Richard B. Hoover | Paul F. X. Boerner | R. Hoover | D. Martínez-Galarce | T. Barbee | P. Boerner | A. Walker
[1] R. Hoover,et al. Observation and modeling of soft x-ray bright points. I. Initial results , 1996 .
[2] Arthur B. C. Walker,et al. Astronomical observations with normal incidence multilayer optics IV: selection of spectral lines , 1994, Optics & Photonics.
[3] R. H. O'Neal,et al. Multi-Spectral Solar Telescope Array , 1990 .
[4] E. M. Reeves,et al. The extreme-ultraviolet spectrum of a solar active region. , 1973 .
[5] Troy W. Barbee,et al. Design and performance of thin foil XUV filters for the Multi-Spectral Solar Telescope Array II , 1995, Optics & Photonics.
[6] Troy W. Barbee,et al. High Resolution Thermally Differentiated Images of the Chromosphere and Corona , 1993 .
[7] Troy W. Barbee,et al. CHROMOSPHERIC AND CORONAL STRUCTURE OF POLAR PLUMES – I. Magnetic Structure and Radiative Energy Balance , 1997 .
[8] Spiro K. Antiochos,et al. Numerical modeling of quasi-static coronal loops. I - Uniform energy input , 1979 .
[9] P. Lemaire,et al. High resolution profiles of the MG II H and MG II K lines. , 1995 .
[10] Spiro K. Antiochos,et al. The Structure of the Static Corona and Transition Region , 1986 .
[11] Arthur B. C. Walker,et al. Solar observations with the multispectral solar telescope array , 1992, Optics & Photonics.
[12] Richard B. Hoover,et al. Thermal and density structure of polar plumes , 1993 .
[13] Leon Golub,et al. Normal incidence soft x-ray telescopes , 1991 .
[14] D. Hathaway,et al. Network Coronal Bright Points: Coronal Heating Concentrations Found in the Solar Magnetic Network , 1998 .
[15] Troy W. Barbee,et al. Multi-spectral solar telescope array V; Temperature diagnostic response to the optically thin solar plasma , 1991 .
[16] Troy W. Barbee,et al. Calibration of the multispectral solar telescope array multilayer mirrors and XUV filters , 1993, Optics & Photonics.
[17] Juan M. Fontenla,et al. Energy Balance in the Solar Transition Region. II. Effects of Pressure and Energy Input on Hydrostatic Models , 1991 .
[18] P. Cally,et al. Stability, structure, and evolution of cool loops , 1991 .
[19] W. Neupert,et al. EIT: Extreme-ultraviolet Imaging Telescope for the SOHO mission , 1995 .
[20] Troy W. Barbee,et al. Performance of the multilayer-coated mirrors for the MultiSpectral Solar Telescope Array , 1994, Optics & Photonics.
[21] Craig E. Deforest,et al. Multi-Spectral Solar Telescope Array IX: quantitative measurements of the solar corona , 1995, Optics & Photonics.
[22] L. Malinovský,et al. An Analysis of the Solar Extreme-Ultraviolet Between 50 and 300 A , 1973 .
[23] E. Avrett,et al. Energy balance in the solar transition region. I - Hydrostatic thermal models with ambipolar diffusion , 1990 .
[24] C. J. Wolfson,et al. Trace — The transition region and coronal explorer , 1994 .
[25] R. Hoover,et al. Soft X-ray Images of the Solar Corona with a Normal-Incidence Cassegrain Multilayer Telescope , 1988, Science.
[26] Y.-M. Wang,et al. The high‐latitude solar wind near sunspot Maximum , 1997 .
[27] Arthur B. C. Walker,et al. Performance of the Multi-Spectral Solar Telescope Array III: optical characteristics of the Ritchey-Chretien and Cassegrain Telescopes , 1991, Optics & Photonics.
[28] A. Walker,et al. Relative coronal abundances derived from X-ray observations 3: The effect of cascades on the relative intensity of Fe (XVII) line fluxes, and a revised iron abundance , 1974 .