Keyser

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61paul collaer Archives Managed by Annette Boucneau Introduction by Ignace De Keyser, Head of the Ethnomusicology Section Inventory of the paul

paul collaer Archives Managed by Annette Boucneau Introduction by Ignace De Keyser, Head of the Ethnomusicology Section Inventory of the paul

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Source URL: www.africamuseum.be

Language: English - Date: 2010-04-28 21:37:14
62REISELIVSSTATISTIKK FOR SVALBARD 2013 Forside: Ekspedisjonscruiseskip, guideskuter og hundekjøring Foto: Elin Lien, Margrete Keyser og Torunn Mellison/ Sysselmannen på Svalbard

REISELIVSSTATISTIKK FOR SVALBARD 2013 Forside: Ekspedisjonscruiseskip, guideskuter og hundekjøring Foto: Elin Lien, Margrete Keyser og Torunn Mellison/ Sysselmannen på Svalbard

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Source URL: www.sysselmannen.no

Language: Norwegian - Date: 2014-04-08 03:27:41
    63The 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
    64Coronal 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

    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

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    Source URL: www.aeronomy.be

    Language: English - Date: 2011-04-18 04:10:25
    65Coupling with the ionosphere By J. De Keyser While the motion of the outer regions of the magnetosphere is prescribed by the solar-wind magnetosphere interaction, the motion of the inner regions of the magnetosphere is d

    Coupling with the ionosphere By J. De Keyser While the motion of the outer regions of the magnetosphere is prescribed by the solar-wind magnetosphere interaction, the motion of the inner regions of the magnetosphere is d

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    Source URL: www.aeronomy.be

    Language: English - Date: 2011-04-18 04:38:40
    66Structure of the Magnetosphere By J. De Keyser The complex structure of the magnetosphere is the result of the interplay between the charged particles originating in the upper layers of the terrestrial atmosphere, whose

    Structure of the Magnetosphere By J. De Keyser The complex structure of the magnetosphere is the result of the interplay between the charged particles originating in the upper layers of the terrestrial atmosphere, whose

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    Source URL: www.aeronomy.be

    Language: English - Date: 2011-04-18 04:38:40
    67Magazine AutumnThese are a few of my favourite things... Richard Keyser

    Magazine AutumnThese are a few of my favourite things... Richard Keyser

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    Source URL: www.savetherhino.org

    Language: English - Date: 2015-03-06 09:54:29
    68The Sun By J. De Keyser and V. Pierrard The Sun is a large ball of plasma. This means: a collection of moving electrically charged elements. It is difficult to speak of the

    The Sun By J. De Keyser and V. Pierrard The Sun is a large ball of plasma. This means: a collection of moving electrically charged elements. It is difficult to speak of the "solar surface", because this giant ball is gas

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    Source URL: www.aeronomy.be

    Language: English - Date: 2011-04-18 04:10:24
    69Why do we study the solar wind? By J. De Keyser The solar wind is an important research topic for astronomers. There are indeed a large number of phenomena, which they do not (or only partially) understand. For example,

    Why do we study the solar wind? By J. De Keyser The solar wind is an important research topic for astronomers. There are indeed a large number of phenomena, which they do not (or only partially) understand. For example,

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    Source URL: www.aeronomy.be

    Language: English - Date: 2011-04-18 04:10:24
    70Fast 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