Chromosphere

Results: 123



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21

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Source URL: www.lesia.obspm.fr

Language: English - Date: 2009-05-27 05:36:13
22

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Source URL: www.hao.ucar.edu

Language: English - Date: 2008-10-20 15:57:36
23

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Source URL: hinode.nao.ac.jp

Language: English - Date: 2010-01-31 21:12:24
24

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Source URL: www.spaceweathercenter.org

Language: English - Date: 2009-06-18 18:34:24
25The	
  Active	
  Sun[1]	
   	
     Comment	
  [1]	
   This	
  lab	
  is	
  aimed	
  at	
  students	
  in	
  an	
  observational	
  astronomy	
  course	
  or	
  similar	
  setting.	
  It	
  presumes

The  Active  Sun[1]       Comment  [1]   This  lab  is  aimed  at  students  in  an  observational  astronomy  course  or  similar  setting.  It  presumes

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Source URL: www.vsp.ucar.edu

Language: English - Date: 2015-01-22 15:53:39
26

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Source URL: www.spaceweathercenter.org

Language: English - Date: 2009-06-18 18:34:25
27Braiding and twist in a coronal active-region magnetic field J. K. Thalmann1 , S. K. Tiwari2 & T. Wiegelmann3 1 Institute of Physics/IGAM, University of Graz, Universit¨ atsplatz 5/II, 8010 Graz, Austria 2 NASA/MSFC, 32

Braiding and twist in a coronal active-region magnetic field J. K. Thalmann1 , S. K. Tiwari2 & T. Wiegelmann3 1 Institute of Physics/IGAM, University of Graz, Universit¨ atsplatz 5/II, 8010 Graz, Austria 2 NASA/MSFC, 32

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Source URL: www.tcd.ie

Language: English - Date: 2014-09-11 03:20:46
28Astronomy & Astrophysics A&A 569, L7DOI:

Astronomy & Astrophysics A&A 569, L7DOI:

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Source URL: www.aanda.org

Language: English
29Chromospheres 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

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

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Source URL: www.nao.ac.jp

Language: English - Date: 2012-07-25 04:23:18
30Polarization / Hanle effect / Physical phenomena / Magnetic field / Stokes parameters / Magnet / Zeeman effect / Polarization in astronomy / Magnetogram / Physics / Electromagnetism / Magnetism

The Polarization of the Mg II h & k Lines for Probing the Solar Chromosphere Luca Belluzzi and Javier Trujillo Bueno (IAC, Tenerife, Spain) Negative of a spectroheliogram at the line center of the Ca II K-line (Courtesy

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Source URL: hinode.nao.ac.jp

Language: English - Date: 2012-08-17 08:22:53