
Helicity of the Solar Magnetic Field - An application to predicting the severity of solar flares - signiertes Exemplar
2010, ISBN: 9783838397719
Taschenbuch
[ED: Taschenbuch / Paperback], [PU: LAP Lambert Academic Publishing], Magnetic helicity is a physical quantity that measures the complexity in the field lines. It is given by a volume integral over scalar product of magnetic field and its vector potential. Direct computation of magnetic helicity in the solar atmosphere is not possible in want of observations to compute the volume integral. We have clarified the physical meaning of and its relation with the magnetic helicity. An analytical bipole was generated to study the effect of polarimetric noise on the estimation of various magnetic parameters. We then examined the fine structures of sunspots in terms of local current and . The concept of signed shear angle (SSA) has been introduced. Spatially averaged SSA (SASSA) gives actual twist present in a sunspot at an observed height irrespective of force-free nature and shape of sunspots. We find that there is no net current in the sunspots even in the presence of significant twist which is consistent with fibril-bundle structure of sunspot magnetic fields. The SASSA holds promise to be very useful in predicting the severity of solar flares. A good correlation has been found among the signs of helicity at different heights in the solar atmosphere., DE, [SC: 0.00], Neuware, gewerbliches Angebot, 212, [GW: 294g], Selbstabholung und Barzahlung, PayPal, Offene Rechnung, Banküberweisung, Internationaler Versand
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ISBN: 9783838397719
Taschenbuch
[ED: Taschenbuch], [PU: LAP Lambert Academic Publishing], Neuware - Magnetic helicity is a physical quantity that measures the complexity in the field lines. It is given by a volume integral over scalar product of magnetic field and its vector potential. Direct computation of magnetic helicity in the solar atmosphere is not possible in want of observations to compute the volume integral. We have clarified the physical meaning of and its relation with the magnetic helicity. An analytical bipole was generated to study the effect of polarimetric noise on the estimation of various magnetic parameters. We then examined the fine structures of sunspots in terms of local current and . The concept of signed shear angle (SSA) has been introduced. Spatially averaged SSA (SASSA) gives actual twist present in a sunspot at an observed height irrespective of force-free nature and shape of sunspots. We find that there is no net current in the sunspots even in the presence of significant twist which is consistent with fibril-bundle structure of sunspot magnetic fields. The SASSA holds promise to be very useful in predicting the severity of solar flares. A good correlation has been found among the signs of helicity at different heights in the solar atmosphere., DE, [SC: 0.00], Neuware, gewerbliches Angebot, 220x150x13 mm, 212, [GW: 294g], PayPal, Offene Rechnung, Banküberweisung, Sofortüberweisung, Internationaler Versand
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2010, ISBN: 3838397711
Taschenbuch
[EAN: 9783838397719], New book, [SC: 8.88], [PU: LAP Lambert Acad. Publ. Aug 2010], Neuware - Magnetic helicity is a physical quantity that measures the complexity in the field lines. It is given by a volume integral over scalar product of magnetic field and its vector potential. Direct computation of magnetic helicity in the solar atmosphere is not possible in want of observations to compute the volume integral. We have clarified the physical meaning of and its relation with the magnetic helicity. An analytical bipole was generated to study the effect of polarimetric noise on the estimation of various magnetic parameters. We then examined the fine structures of sunspots in terms of local current and . The concept of signed shear angle (SSA) has been introduced. Spatially averaged SSA (SASSA) gives actual twist present in a sunspot at an observed height irrespective of force-free nature and shape of sunspots. We find that there is no net current in the sunspots even in the presence of significant twist which is consistent with fibril-bundle structure of sunspot magnetic fields. The SASSA holds promise to be very useful in predicting the severity of solar flares. A good correlation has been found among the signs of helicity at different heights in the solar atmosphere. 212 pp. Englisch
AbeBooks.co.uk BuchWeltWeit Inh. Ludwig Meier e.K., Bergisch Gladbach, Germany [57449362] [Rating: 5 (of 5)] NEW BOOK. Versandkosten: EUR 8.88 Details... |
ISBN: 9783838397719
Magnetic helicity is a physical quantity that measures the complexity in the field lines. It is given by a volume integral over scalar product of magnetic field and its vector potential. Direct computation of magnetic helicity in the solar atmosphere is not possible in want of observations to compute the volume integral. We have clarified the physical meaning of and its relation with the magnetic helicity. An analytical bipole was generated to study the effect of polarimetric noise on the estimation of various magnetic parameters. We then examined the fine structures of sunspots in terms of local current and . The concept of signed shear angle (SSA) has been introduced. Spatially averaged SSA (SASSA) gives actual twist present in a sunspot at an observed height irrespective of force-free nature and shape of sunspots. We find that there is no net current in the sunspots even in the presence of significant twist which is consistent with fibril-bundle structure of sunspot magnetic fields. The SASSA holds promise to be very useful in predicting the severity of solar flares. A good correlation has been found among the signs of helicity at different heights in the solar atmosphere. Bücher, Hörbücher & Kalender / Bücher / Sachbuch / Naturwissenschaften / Physik
Dodax.de Nr. GPUEKS6IPT4. Versandkosten:, Lieferzeit: 5 Tage, DE. (EUR 0.00) Details... |

Helicity of the Solar Magnetic Field: An application to predicting the severity of solar flares - Taschenbuch
2010, ISBN: 9783838397719
LAP LAMBERT Academic Publishing, 2010-08-27. Paperback. Good., LAP LAMBERT Academic Publishing, 2010-08-27
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Helicity of the Solar Magnetic Field - An application to predicting the severity of solar flares - signiertes Exemplar
2010, ISBN: 9783838397719
Taschenbuch
[ED: Taschenbuch / Paperback], [PU: LAP Lambert Academic Publishing], Magnetic helicity is a physical quantity that measures the complexity in the field lines. It is given by a volume int… Mehr…
Versandkosten:Versandkostenfrei, Versand nach Deutschland. (EUR 0.00)
ISBN: 9783838397719
Taschenbuch
[ED: Taschenbuch], [PU: LAP Lambert Academic Publishing], Neuware - Magnetic helicity is a physical quantity that measures the complexity in the field lines. It is given by a volume integ… Mehr…
Versandkosten:Versandkostenfrei, Versand nach Deutschland. (EUR 0.00)
2010
ISBN: 3838397711
Taschenbuch
[EAN: 9783838397719], New book, [SC: 8.88], [PU: LAP Lambert Acad. Publ. Aug 2010], Neuware - Magnetic helicity is a physical quantity that measures the complexity in the field lines. It … Mehr…
NEW BOOK. Versandkosten: EUR 8.88
ISBN: 9783838397719
Magnetic helicity is a physical quantity that measures the complexity in the field lines. It is given by a volume integral over scalar product of magnetic field and its vector potential. … Mehr…
Nr. GPUEKS6IPT4. Versandkosten:, Lieferzeit: 5 Tage, DE. (EUR 0.00)
Helicity of the Solar Magnetic Field: An application to predicting the severity of solar flares - Taschenbuch
2010, ISBN: 9783838397719
LAP LAMBERT Academic Publishing, 2010-08-27. Paperback. Good., LAP LAMBERT Academic Publishing, 2010-08-27
Versandkosten: EUR 11.44
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Detailangaben zum Buch - Helicity of the Solar Magnetic Field
EAN (ISBN-13): 9783838397719
ISBN (ISBN-10): 3838397711
Taschenbuch
Erscheinungsjahr: 2010
Herausgeber: LAP Lambert Acad. Publ.
212 Seiten
Gewicht: 0,331 kg
Sprache: eng/Englisch
Buch in der Datenbank seit 2012-11-03T03:19:36+01:00 (Berlin)
Detailseite zuletzt geändert am 2021-01-12T09:59:37+01:00 (Berlin)
ISBN/EAN: 9783838397719
ISBN - alternative Schreibweisen:
3-8383-9771-1, 978-3-8383-9771-9
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