Heliospheric current sheet

Results: 18



#Item
1Dramatic  Changes  in  the   Heliospheric  Current  Sheet:   Cycles  21-­‐24   J  Todd  Hoeksema   Wilcox  Solar  Observatory   Stanford  University  

Dramatic  Changes  in  the   Heliospheric  Current  Sheet:   Cycles  21-­‐24   J  Todd  Hoeksema   Wilcox  Solar  Observatory   Stanford  University  

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Source URL: sun.stanford.edu

Language: English - Date: 2015-08-20 18:05:42
    2Microsoft PowerPoint - MSSL Seminar Jan2010.ppt

    Microsoft PowerPoint - MSSL Seminar Jan2010.ppt

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    Source URL: www.mssl.ucl.ac.uk

    Language: English - Date: 2010-11-08 06:38:44
    3Multiple-spacecraft observation of current sheets in solar wind University of Science and Technology of China Dawei Guo 郭大伟 xi’an

    Multiple-spacecraft observation of current sheets in solar wind University of Science and Technology of China Dawei Guo 郭大伟 xi’an

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    Source URL: scostep.apps01.yorku.ca

    Language: English - Date: 2016-04-11 16:47:08
    4The interplanetary magnetic field By J. De Keyser The Sun possesses a magnetic field. There are not only strong local magnetic fields (for example near sunspots), but a global magnetic field exists as well. In a first ap

    The interplanetary magnetic field By J. De Keyser The Sun possesses a magnetic field. There are not only strong local magnetic fields (for example near sunspots), but a global magnetic field exists as well. In a first ap

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    Source URL: www.aeronomy.be

    Language: English - Date: 2011-04-18 04:10:24
    5Fast and slow solar wind By J. De Keyser The solar wind escaping from the coronal holes has a speed of about 800km/s. Near the heliospheric current sheet (HCS), the contact area between the solar wind coming from the nor

    Fast and slow solar wind By J. De Keyser The solar wind escaping from the coronal holes has a speed of about 800km/s. Near the heliospheric current sheet (HCS), the contact area between the solar wind coming from the nor

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    Source URL: www.aeronomy.be

    - Date: 2011-04-18 04:10:24
      6The interplanetary magnetic field By J. De Keyser The Sun possesses a magnetic field. There are not only strong local magnetic fields (for example near sunspots), but a global magnetic field exists as well. In a first ap

      The interplanetary magnetic field By J. De Keyser The Sun possesses a magnetic field. There are not only strong local magnetic fields (for example near sunspots), but a global magnetic field exists as well. In a first ap

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      Source URL: www.bira-iasb.be

      Language: English - Date: 2011-04-18 04:10:24
      7Global Simulations of the Solar Corona and Inner Heliosphere: Solar Wind Prediction Pete Riley, Jon Linker, Zoran Mikic, and Roberto Lionello

      Global Simulations of the Solar Corona and Inner Heliosphere: Solar Wind Prediction Pete Riley, Jon Linker, Zoran Mikic, and Roberto Lionello

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      Source URL: hmi.stanford.edu

      Language: English - Date: 2006-04-19 14:58:27
      8Fast and slow solar wind By J. De Keyser The solar wind escaping from the coronal holes has a speed of about 800km/s. Near the heliospheric current sheet (HCS), the contact area between the solar wind coming from the nor

      Fast and slow solar wind By J. De Keyser The solar wind escaping from the coronal holes has a speed of about 800km/s. Near the heliospheric current sheet (HCS), the contact area between the solar wind coming from the nor

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      Source URL: www.bira-iasb.be

      - Date: 2011-04-18 04:10:24
        9The interplanetary magnetic field By J. De Keyser The Sun possesses a magnetic field. There are not only strong local magnetic fields (for example near sunspots), but a global magnetic field exists as well. In a first ap

        The interplanetary magnetic field By J. De Keyser The Sun possesses a magnetic field. There are not only strong local magnetic fields (for example near sunspots), but a global magnetic field exists as well. In a first ap

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        Source URL: www.aeronomie.be

        Language: English - Date: 2011-04-18 04:10:24
        10Magnetic connectivity associated with SW reconnection events: STEREO/SWEA Benoit Lavraud,1 Andrea Opitz,1 Jack Gosling,2 J.-A. Sauvaud,1 and the IMPACT team1,3,4,5 1: CESR/CNRS, Toulouse, France

        Magnetic connectivity associated with SW reconnection events: STEREO/SWEA Benoit Lavraud,1 Andrea Opitz,1 Jack Gosling,2 J.-A. Sauvaud,1 and the IMPACT team1,3,4,5 1: CESR/CNRS, Toulouse, France

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        Source URL: stereo-ssc.nascom.nasa.gov

        Language: English - Date: 2008-04-30 13:46:50