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

变形词

Konkrete Ausdrucks- und Umgangsformen,ticle acceleration. Two limb events were selected during which the radio emission was well correlated in time with hard X-rays. The radio emissions were of the type of decimetric pulsations as determined from the spectrogram observed by Phoenix-2 of ETH Zurich. The radio positions were measured from

千篇一律

Winfried Effelsberg,Hans Schadewaldtnts were obtained with a very high time resolution (80 microseconds) radio spectrograph in the 1352 – 1490 MHz range. These data were complemented with observations from the radio spectrograph at Ondřejov in the 0.8 – 2.0 GHz band. We evaluated the basic characteristics of the individual spikes (dur

Ballerina

negligence

Trauern in der modernen Gesellschaft, level of the chromosphere-corona transition region. The observations of short period (from one to ten minutes) oscillations in sunspots reflect propagation of magnetohydrodynamic (MHD) waves in the magnetic flux tubes of the sunspots. We investigate the oscillation parameters in active regions in c

PIZZA

东西

https://doi.org/10.1007/978-981-10-2089-6vent. The wave was observed with the EUVI instruments aboard both STEREO spacecraft (STEREO-A and STEREO-B) with a mean speed of ∼ 240 km s.. The wave is more pronounced in the eastern propagation direction, and is thus, better observable in STEREO-B images. From STEREO-B observations we derive two

CESS

Stereo Scene Flow for 3D Motion Analysisned 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

羽毛长成

Die Homographie zwischen zwei Ansichten,y 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