Titlebook: Meditation – Neuroscientific Approaches and Philosophical Implications; Stefan Schmidt,Harald Walach Book 2014 The Editor(s) (if applicabl

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foreign

TOXIC

Wendy Hasenkamp Ph.D. altitudes of . ? 20 Mm (§ 3.8–3.9). Also stellar differential emission measure distributions are sensitive to the heating function (§ 3.10). Of course, a large number of coronal loops are found to be not in hydrostatic equilibrium, but nearly hydrostatic loops have been found preferentially in the quiet corona and in older dipolar active regions.

無畏

Stefan Schmidt,Harald Walach contain information on the motion of chromospheric evaporation fronts (§ 16.3.4). The forth stage of postflare loop cooling is now understood to be dominated by thermal conduction initially, and by radiative cooling later on (§ 16.4). However, spatio-temporal temperature modeling of flare plasmas is still in its infancy.

ARC

Conflagration

陶瓷

of ? 20 keV, the propagation time to the flare loop footpoints may exceed the collisional deflection time, and thus they are stopped in the coronal part of the flare loop. Particle kinematics is a novel key tool for the interpretation of nonthermal hard X-ray, .-ray, and radio emission.

Senescent

Shawn S. Clausen M.D., M.PH.,Cindy C. Crawford,John A. Ives

進(jìn)取心

Fynn-Mathis Trautwein,José Raúl Naranjo,Stefan Schmidt

STIT

Michael D. Mrazek,Benjamin W. Mooneyham,Jonathan W. Schooler