Convective blueshifts in the solar atmosphere
暂无分享,去创建一个
[1] Xavier Dumusque,et al. Measuring precise radial velocities on individual spectral lines , 2018, Astronomy & Astrophysics.
[2] T. Steinmetz,et al. Convective blueshifts in the solar atmosphere-II. High-accuracy observations of the Fe I 6173.3 Å line and deviations of full-disk Dopplergrams , 2019 .
[3] R. Haywood,et al. Stellar Surface Magneto-convection as a Source of Astrophysical Noise. II. Center-to-limb Parameterization of Absorption Line Profiles and Comparison to Observations , 2018, The Astrophysical Journal.
[4] Absolute velocity measurements in sunspot umbrae , 2018, Astronomy & Astrophysics.
[5] F. Bauer,et al. The influence of convective blueshift on radial velocities of F, G, and K stars , 2018 .
[6] W. Schmidt,et al. Convective blueshifts in the solar atmosphere, I. Absolute measurements with LARS of the spectral lines at 6302 {\AA} , 2017, 1712.07059.
[7] W. Schmidt,et al. LARS: An Absolute Reference Spectrograph for solar observations Upgrade from a prototype to a turn-key system , 2017, 1707.01573.
[8] L. Rachmeler. The Sun: An Introduction , 2017 .
[9] W. Schmidt,et al. Daniel K. Inouye Solar Telescope: High‐resolution observing of the dynamic Sun , 2016 .
[10] A. Collier Cameron,et al. The Sun as a planet-host star: proxies from SDO images for HARPS radial-velocity variations , 2016, 1601.05651.
[11] S. Antiochos,et al. ACHIEVING CONSISTENT DOPPLER MEASUREMENTS FROM SDO/HMI VECTOR FIELD INVERSIONS , 2015, 1511.06500.
[12] Nicolas Buchschacher,et al. HARPS-N OBSERVES THE SUN AS A STAR , 2015, 1511.02267.
[13] J. Bailey. Measuring the surface magnetic fields of magnetic stars with unresolved Zeeman splitting , 2014, 1407.7847.
[14] M. Riva,et al. ESPRESSO: The next European exoplanet hunter , 2014, 1401.5918.
[15] K. Puschmann,et al. GREGOR Fabry-Pérot interferometer and its companion the blue imaging solar spectrometer , 2013, 1302.7157.
[16] Yukio Katsukawa,et al. The Hinode Spectro-Polarimeter , 2013 .
[17] R. Schlichenmaier,et al. Correlations between sunspots and their moat flows , 2013, 1301.2434.
[18] Antonio Manescau,et al. Astronomical Spectrograph Calibration at the Exo-Earth Detection Limit , 2012 .
[19] P. Scherrer,et al. Line-of-Sight Observables Algorithms for the Helioseismic and Magnetic Imager (HMI) Instrument Tested with Interferometric Bidimensional Spectrometer (IBIS) Observations , 2012 .
[20] C. J. Wolfson,et al. Design and Ground Calibration of the Helioseismic and Magnetic Imager (HMI) Instrument on the Solar Dynamics Observatory (SDO) , 2012 .
[21] Jesper Schou,et al. Wavelength Dependence of the Helioseismic and Magnetic Imager (HMI) Instrument onboard the Solar Dynamics Observatory (SDO) , 2012 .
[22] Alexandra Tritschler,et al. The second ATST-EAST meeting : magnetic fields from the photosphere to the corona , 2012 .
[23] G. Scharmer,et al. Detection of Convective Downflows in a Sunspot Penumbra , 2011, Science.
[24] S. Solanki,et al. CONVECTIVE NATURE OF SUNSPOT PENUMBRAL FILAMENTS: DISCOVERY OF DOWNFLOWS IN THE DEEP PHOTOSPHERE , 2011, 1105.1877.
[25] D. Kiselman,et al. Solar velocity references from 3D HD photospheric models , 2011, 1101.2671.
[26] Christophe Lovis,et al. Planetary detection limits taking into account stellar noise - I. Observational strategies to reduce stellar oscillation and granulation effects , 2010, 1010.2616.
[27] A. Álvarez-Herrero,et al. The Sunrise Mission , 2010, 1009.2689.
[28] J. C. del Toro Iniesta,et al. The Imaging Magnetograph eXperiment (IMaX) for the Sunrise Balloon-Borne Solar Observatory , 2010, 1009.1095.
[29] A.-M. Lagrange,et al. Using the Sun to estimate Earth-like planets detection capabilities II. Impact of plages , 2010, 1001.1638.
[30] K. Reardon,et al. THE QUIET SOLAR ATMOSPHERE OBSERVED AND SIMULATED IN Na i D1 , 2009, 0912.2206.
[31] Michael Wegner,et al. Ground-based and Airborne Instrumentation for Astronomy III , 2010 .
[32] Jan Swevers,et al. Ground-based and airborne instrumentation for astronomy , 2010 .
[33] F. Kneer,et al. Acoustic waves in the solar atmosphere at high spatial resolution , 2009 .
[34] R. Rutten,et al. Explanation of the activity sensitivity of Mn I 5394.7 Å , 2008, 0811.3555.
[35] T. Hänsch,et al. Laser Frequency Combs for Astronomical Observations , 2008, Science.
[36] The origin of the reversed granulation in the solar photosphere , 2006, astro-ph/0612464.
[37] F. Cavallini. IBIS: A New Post-Focus Instrument for Solar Imaging Spectroscopy , 2006 .
[38] G. Scharmer. Comments on the optimization of high resolution Fabry-Pérot filtergraphs , 2006 .
[39] R. Schlichenmaier,et al. Multi-line spectroscopy of dark-cored penumbral filaments , 2005 .
[40] M. Asplund,et al. New light on stellar abundance analyses: Departures from LTE and homogeneity. , 2005 .
[41] D. C. Solana,et al. Sensitivity of spectral lines to temperature, velocity, and magnetic field , 2005 .
[42] F. Kneer,et al. Polarimetry in Sunspot Penumbrae at High Spatial Resolution , 2005 .
[43] R. Schlichenmaier,et al. Two-dimensional spectroscopy of a sunspot - I. Properties of the penumbral fine structure , 2004 .
[44] R. Schlichenmaier,et al. Two-dimensional spectroscopy of a sunspot II. Penumbral line asymmetries , 2004 .
[45] Jean-Luis Lizon,et al. Setting New Standards with HARPS , 2003 .
[46] Investigation of temperature and velocity fluctuations through the solar photosphere with the Na I D lines , 2001 .
[47] P. Hauschildt,et al. Solar Mn I 5432/5395 A line formation explained , 2001 .
[48] R. Muller,et al. The Solar Granulation , 1999 .
[49] D. F. Gray,et al. Monitoring the Solar Temperature: Empirical Calibration of the Temperature Sensitivity of C I λ5380 , 1997 .
[50] C. H. Acton,et al. Ancillary data services of NASA's Navigation and Ancillary Information Facility , 1996 .
[51] S. Johansson,et al. A New Multiplet Table for Fe , 1994, astro-ph/9404049.
[52] B. Lites. The polarization properties of Feii 614.9 nm , 1993 .
[53] Herschel B. Snodgrass,et al. Rotation of Doppler Features in the Solar Photosphere , 1990 .
[54] H. Balthasar. On the contribution of horizontal granular motions to observed limb-effect curves , 1985 .
[55] B. N. Andersen,et al. Limb effect of solar absorption lines , 1984 .
[56] H. Balthasar. Asymmetries and wavelengths of solar spectral lines and the solar rotation determined from Fourier-transform spectra , 1984 .
[57] Dainis Dravins,et al. Photospheric Spectrum Line Asymmetries and Wavelength Shifts , 1982 .
[58] P. Brandt,et al. On the centre-to-limb variation and latitude dependence of the asymmetry and wavelength shift of the solar line λ 5576 , 1982 .
[59] J. Beckers,et al. Some comments on the limb shift of solar lines , 1978 .
[60] J. Beckers. Material motions in sunspot umbrae. , 1977 .
[61] P. Ibbetson,et al. The Solar Limb Effect: Observations of Line Contours and Line Shifts , 1976 .
[62] S. P. Worden,et al. Heights of formation of non-magnetic solar lines suitable for velocity studies , 1975 .
[63] T. Margrave. The solar manganese abundance , 1972 .
[64] I. Appenzeller,et al. Center-to-limb variations of the intensity and the wavelength of several Fraunhofer lines along the sun's polar and equatorial diameter. , 1967 .
[65] R. Loughhead,et al. The Solar Granulation , 1967 .
[66] J. Halm. Über eine bisher unbekannte Verschiebung der Fraunhoferschen Linien des Sonnenspektrums , 1906 .