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The Light of the Sun
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121	2012 LWS Heliophysics Summer School Problem Set on the Three Solar Wind 1 Estimating coronal temperatures using Parker model In the lecture we saw that the speed of the solar wind near Earth at 1 AU ranges from about 27 Add to Reading List Source URL: www.vsp.ucar.edu Language: English - Date: 2012-06-04 12:37:41 Astrophysics Astronomy Sun Light sources Corona Solar wind Plasma Wind Alfvén wave Space plasmas Physics Plasma physics
122	Detection of Low-Level Activities in Solar-Analog Stars from the Emission Strengths of Ca II 3934 Line TAKEDA, Yoichi, TAJITSU, Akito, KAWANOMOTO, Satoshi, ANDO, Hiroyasu, SAKURAI, Takashi (NAOJ) HONDA, Satoshi Add to Reading List Source URL: www.nao.ac.jp Language: English - Date: 2014-01-28 00:54:36 Star Stellar astronomy Honda Stellar classification Sun Astronomy Transport Light sources Plasma physics Economy of Japan
123	Measurements of Coronal and Chromospheric Magnetic Fields Using Polarization Observations by the Nobeyama Radioheliograph IWAI, Kazumasa, SHIBASAKI, Kiyoto (NAOJ) The magnetic fields of the corona and the Add to Reading List Source URL: www.nao.ac.jp Language: English - Date: 2015-03-23 03:19:20 Space plasmas Sun Light sources Astrophysics Corona Circular polarization Sunspot Polarization Solar variation Physics Plasma physics Electromagnetism
124	“Ground-based observation of the solar activity by Continuous H-Alpha Imaging Network (CHAIN) and outline of the analysis of solar flares and shock waves” Satoru UeNo, K.Shibata, A.Asai, S.Morita, R.Kitai, T.Ishii, K Add to Reading List Source URL: www.kwasan.kyoto-u.ac.jp Language: English - Date: 2012-02-12 19:17:00 Physics Astrophysics Sun Light sources Coronal mass ejection Moreton wave Corona Solar flare Solar wind Space plasmas Plasma physics Astronomy
125	Coronal mass ejections and magnetized clouds By J. De Keyser It is known that large structures can exist within the corona, that may catapult plasma into space with a speed of 1000 km/s. Such an event is called a coronal Add to Reading List Source URL: www.aeronomy.be Language: English - Date: 2011-04-18 04:10:25 Astrophysics Plasma physics Sun Light sources Jets Coronal mass ejection Corona Solar wind Magnetosphere Space plasmas Physics Astronomy
126	Appendix Appendix A: A.1 Exploration of α-effect and turbulent diffusion While it is generally accepted that differential rotation is the main player transforming poloidal into toroidal field the details of the processe Add to Reading List Source URL: hinode.nao.ac.jp Language: English - Date: 2011-04-28 05:40:05 Plasma physics Light sources Space plasmas Physical quantities Tachocline Helioseismology Io Magnetic helicity Magnetic field Physics Astronomy Sun
127	THE POWER OF LIGHT A Bright Future Light. It is all around us. It is a natural and powerful resource. Light is the brightness of the sun and the heat that comes from it. Imagine, just for a second, a Add to Reading List Source URL: www.osa.org Language: English - Date: 2014-10-14 10:24:31 Acronyms Laser Photonics Optics Light Telescope European Southern Observatory Optical fiber Transparency and translucency Science Technology Physics
128	Chromospheres in Metal-Poor Stars Revealed from the He I 10830 Å Line (Tokai University) that two types of chromospheres exist: ——(1) The rotation-dependent chromospheric activity (seen in less-aged population I s Add to Reading List Source URL: www.nao.ac.jp Language: English - Date: 2012-07-25 04:23:18 Space plasmas Sun Physics Astrophysics Stellar astronomy Star Chromosphere Light sources Astronomy Plasma physics
129	Detailed Density and Velocity Structures of the Protostellar Core B335 KURONO, Yasutaka, SAITO, Masao, KAMAZAKI, Takeshi, MORITA, Koh-Ichiro, KAWABE, Ryohei (NAOJ) In order to understand physical processes of lowmass sta Add to Reading List Source URL: www.nao.ac.jp Language: English - Date: 2014-01-28 00:54:38 Star formation Light sources Astrophysics Star types Star Protostar Sun Mass European Southern Observatory Astronomy Physics Stellar astronomy
130	Vector Tomography for the Reconstruction of the Coronal Magnetic Field as kind of an Inverse Problem Add to Reading List Source URL: stereo-ssc.nascom.nasa.gov Language: English - Date: 2008-04-30 14:34:06 Light sources Sun Isosurface Corona Electron Physics Plasma physics Space plasmas

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