Chromosphere

Results: 123



#Item
41Formation and sensitivity of SUVIT lines in a dynamic atmosphere Mats Carlsson Institute of Theoretical Astrophysics, University of Oslo StAndrews, August

Formation and sensitivity of SUVIT lines in a dynamic atmosphere Mats Carlsson Institute of Theoretical Astrophysics, University of Oslo StAndrews, August

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Source URL: hinode.nao.ac.jp

Language: English - Date: 2012-08-17 08:22:56
42Space plasmas / Light sources / Plasma physics / Astrophysics / Corona / Chromosphere / Solar cycle / Convection zone / Solar wind / Sun / Physics / Astronomy

Sun’s rap song by Mary Hogan and Wei Lee 1. Class, today if you will listen, This is about the star of our Solar System. It’s not Elvis, Madonna or Elton John,

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Source URL: www.haverford.edu

Language: English - Date: 2002-08-20 10:34:21
43Sun’s rap song by Mary Hogan and Wei Lee 1. Class, today if you will listen, This is about the star of our Solar System. It’s not Elvis, Madonna or Elton John, Because our star is big, bright, hot and called the Sun.

Sun’s rap song by Mary Hogan and Wei Lee 1. Class, today if you will listen, This is about the star of our Solar System. It’s not Elvis, Madonna or Elton John, Because our star is big, bright, hot and called the Sun.

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Source URL: www.haverford.edu

Language: English - Date: 2002-08-20 10:31:52
44Magnetic TRAnsition region Probe (MTRAP) Science Objectives: • Discover, measure, and understand the 3D structure and dynamics of the magnetic transition region between the photosphere and upper chromosphere. • Conne

Magnetic TRAnsition region Probe (MTRAP) Science Objectives: • Discover, measure, and understand the 3D structure and dynamics of the magnetic transition region between the photosphere and upper chromosphere. • Conne

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Source URL: sec.gsfc.nasa.gov

Language: English - Date: 2002-03-14 11:26:08
45Plan-B: Summary and discussionsT.Shimizu and Y.Katsukawa  Key items to be addressed in the meeting

Plan-B: Summary and discussionsT.Shimizu and Y.Katsukawa Key items to be addressed in the meeting

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Source URL: hinode.nao.ac.jp

Language: English - Date: 2010-09-30 00:26:40
46Astronomy & Astrophysics A&A 532, L9DOI:

Astronomy & Astrophysics A&A 532, L9DOI:

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Source URL: www.aanda.org

Language: English
47Microsoft PowerPoint - hinode2_081001.ppt [Read-Only]

Microsoft PowerPoint - hinode2_081001.ppt [Read-Only]

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Source URL: www.hao.ucar.edu

Language: English - Date: 2008-10-20 16:01:56
48Are solar chromospheric fibrils tracing the magnetic field?

Are solar chromospheric fibrils tracing the magnetic field?

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Source URL: www.aanda.org

Language: English
49LWS TR&T Focus Team: Exploring the Magnetic Connection Between the Photosphere and Low Corona Team Progress Report: Year 1, December 2009 Proposal Number: 07-LWSTRT07-0066 Team Chair:

LWS TR&T Focus Team: Exploring the Magnetic Connection Between the Photosphere and Low Corona Team Progress Report: Year 1, December 2009 Proposal Number: 07-LWSTRT07-0066 Team Chair:

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Source URL: lws-trt.gsfc.nasa.gov

Language: English - Date: 2012-09-12 17:54:38
50WHY ARE CORONAL HOLES INDISTINGUISHABLE FROM THE QUIET SUN IN TRANSITION REGION RADIATION? Thomas Wiegelmann and Sami K. Solanki Max-Planck-Institut f¨ur Sonnensystemforschung, 37191 Katlenburg-Lindau, Germany ABSTRACT

WHY ARE CORONAL HOLES INDISTINGUISHABLE FROM THE QUIET SUN IN TRANSITION REGION RADIATION? Thomas Wiegelmann and Sami K. Solanki Max-Planck-Institut f¨ur Sonnensystemforschung, 37191 Katlenburg-Lindau, Germany ABSTRACT

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Source URL: star.mpae.gwdg.de

Language: English - Date: 2004-09-29 09:19:51