A DETAILED COMPARISON BETWEEN THE OBSERVED AND SYNTHESIZED PROPERTIES OF A SIMULATED TYPE II SPICULE

We have performed a three-dimensional radiative MHD simulation of the solar atmosphere. Observational results suggest they may contribute significantly in supplying the corona with hot plasma. We perform a detailed comparison of the properties of the simulated jet with those of type II spicules (obs...

Ausführliche Beschreibung

Gespeichert in:

Bibliographische Detailangaben
Veröffentlicht in:	The Astrophysical journal 2013-07, Vol.771 (1), p.1-25
Hauptverfasser:	Martinez-Sykora, Juan, DE PONTIEU, BART, LEENAARTS, JORRIT, Pereira, Tiago M D, Carlsson, Mats, Hansteen, Viggo, Stern, Julie V, Tian, Hui, McIntosh, Scott W, VAN DER VOORT, LUC ROUPPE
Format:	Artikel
Sprache:	eng
Schlagworte:	ABSORPTION ASTROPHYSICS, COSMOLOGY AND ASTRONOMY ASYMMETRY CHROMOSPHERE COMPARATIVE EVALUATIONS Coronas DENSITY DOPPLER EFFECT Dynamic tests EMISSION HOT PLASMA LIFETIME LINE WIDTHS MAGNETOHYDRODYNAMICS MASS MHD OPACITY RADIANT HEAT TRANSFER SIMULATION SOLAR PROMINENCES Spicules SUN Supplying TELESCOPES THREE-DIMENSIONAL CALCULATIONS
Online-Zugang:	Volltext
Tags:	Tag hinzufügen Keine Tags, Fügen Sie den ersten Tag hinzu!

Schreiben Sie den ersten Kommentar!