Titlebook: Energy Storage and Release through the Solar Activity Cycle; Models Meet Radio Ob Christophe Marqué,Alexander Nindos Book 2012 Springer Sci

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,Coronal Shock Waves, EUV Waves, and Their Relation to CMEs. I. Reconciliation of “EIT Waves”, Type ned into shocks and freely propagated afterwards like decelerating blast waves that showed up as Moreton waves and EUV waves. We propose a simple quantitative description for such shock waves to reconcile their observed propagation with drift rates of metric type II bursts and kinematics of leading

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Coronal Shock Waves, EUV Waves, and Their Relation to CMEs. III. Shock-Associated CME/EUV Wave in ay connected off-limb and on-disk signatures. Veronig .. (.., L57, .) concluded that the dome was formed by a weak shock wave. We have revealed two EUV components, one of which corresponded to this transient. All of its properties found from EUV, white light, and a metric type II burst match expectat

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The 17 January 2005 Complex Solar Radio Event Associated with Interacting Fast Coronal Mass Ejectioanied by metre-to-kilometre type-III groups tracing energetic electrons that escape into the interplanetary space and by decametre-to-hectometre type-II bursts attributed to CME-driven shock waves. A peculiar type-III burst group was observed below 600 kHz 1.5 hours after the second type-III group.

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The Connection of Solar Wind Parameters with Radio and UV Emission from Coronal Holes,MHz, from NoRH, SSRT and Nançay radioheliographs), and solar wind parameters, from ACE spacecraft data over the period 12 March – 31 May 2007. The increase in the solar wind velocity up to ∼ 600 km s. was found to correlate with a decrease in the UV flux in the central parts of the solar disk. A con

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978-1-4899-9309-0Springer Science+Business Media New York 2012

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,Gehirnakrobatik? – Sich selbst überlisten?,mpulsive phase and can last for a few tens of minutes to more than one hour. The few examples discussed in the literature indicate that such long-lasting submillimeter emission is most likely thermal bremsstrahlung. We present a detailed analysis of the time-extended phase of the 27 October 2003 (M6