Artículo

Nuevo, F.A.; Vásquez, A.M.; Frazin, R.A.; Huang, Z.; Manchester IV, W.B.; Mandrini C.H.; Webb D.F. "The 3D solar corona Cycle 24 rising phase from SDO/AIA tomography" (2011) Proceedings of the International Astronomical Union. 7(S286):238-241
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Abstract:

We recently extended the differential emission measure tomography (DEMT) technique to be applied to the six iron bands of the Atmospheric Imaging Assembly (AIA) instrument aboard the Solar Dynamics Observatory (SDO). DEMT products are the 3D reconstruction of the coronal emissivity in the instrument's bands, and the 3D distribution of the local differential emission measure, in the height range 1.0 to 1.25 R⊙. We show here derived maps of the electron density and temperature of the inner solar corona during the rising phase of solar Cycle 24. We discuss the distribution of our results in the context of open/closed magnetic regions, as derived from a global potential field source surface (PFSS) model of the same period. We also compare the results derived with SDO/AIA to those derived with the Extreme UltraViolet Imager (EUVI) instrument aboard the Solar TErrestrial RElations Observatory (STEREO). © 2012 International Astronomical Union.

Registro:

Documento: Artículo
Título:The 3D solar corona Cycle 24 rising phase from SDO/AIA tomography
Autor:Nuevo, F.A.; Vásquez, A.M.; Frazin, R.A.; Huang, Z.; Manchester IV, W.B.; Mandrini C.H.; Webb D.F.
Filiación:Instituto de Astronomía y Física Del Espacio (CONICET-UBA), CC 67 - Suc 28, (C1428ZAA) Ciudad de Buenos Aires, Argentina
Facultad de Cs. Exactas y Naturales, Universidad de Buenos Aires, Argentina
Department of Atmospheric, Oceanic and Space Sciences, University of Michigan, Ann Arbor, MI 48109, United States
Palabras clave:methods: data analysis; Sun: corona; Sun: fundamental parameters
Año:2011
Volumen:7
Número:S286
Página de inicio:238
Página de fin:241
DOI: http://dx.doi.org/10.1017/S1743921312004905
Título revista:Proceedings of the International Astronomical Union
Título revista abreviado:Proc. Int. Astron. Union
ISSN:17439213
Registro:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_17439213_v7_nS286_p238_Nuevo

Referencias:

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  • V́asquez, A.M., Frazin, R.A., Huang, Z., Manchester, I.V.W.B., Shearer, P., (2012), this volume

Citas:

---------- APA ----------
Nuevo, F.A., Vásquez, A.M., Frazin, R.A., Huang, Z., Manchester IV, W.B., Mandrini C.H. & Webb D.F. (2011) . The 3D solar corona Cycle 24 rising phase from SDO/AIA tomography. Proceedings of the International Astronomical Union, 7(S286), 238-241.
http://dx.doi.org/10.1017/S1743921312004905
---------- CHICAGO ----------
Nuevo, F.A., Vásquez, A.M., Frazin, R.A., Huang, Z., Manchester IV, W.B., Mandrini C.H., et al. "The 3D solar corona Cycle 24 rising phase from SDO/AIA tomography" . Proceedings of the International Astronomical Union 7, no. S286 (2011) : 238-241.
http://dx.doi.org/10.1017/S1743921312004905
---------- MLA ----------
Nuevo, F.A., Vásquez, A.M., Frazin, R.A., Huang, Z., Manchester IV, W.B., Mandrini C.H., et al. "The 3D solar corona Cycle 24 rising phase from SDO/AIA tomography" . Proceedings of the International Astronomical Union, vol. 7, no. S286, 2011, pp. 238-241.
http://dx.doi.org/10.1017/S1743921312004905
---------- VANCOUVER ----------
Nuevo, F.A., Vásquez, A.M., Frazin, R.A., Huang, Z., Manchester IV, W.B., Mandrini C.H., et al. The 3D solar corona Cycle 24 rising phase from SDO/AIA tomography. Proc. Int. Astron. Union. 2011;7(S286):238-241.
http://dx.doi.org/10.1017/S1743921312004905