http://chineseinput.net/에서 pinyin(병음)방식으로 중국어를 변환할 수 있습니다.
변환된 중국어를 복사하여 사용하시면 됩니다.
Inference of magnetic fields in the very quiet Sun
Martí,nez Gonzá,lez, M. J.,Pastor Yabar, A.,Lagg, A.,Asensio Ramos, A.,Collados, M.,Solanki, S. K.,Balthasar, H.,Berkefeld, T.,Denker, C.,Doerr, H. P.,Feller, A.,Franz, M.,Gonzá,lez EDP Sciences 2016 Astronomy and astrophysics Vol.596 No.-
UNNOTICED MAGNETIC FIELD OSCILLATIONS IN THE VERY QUIET SUN REVEALED BY SUNRISE/IMaX
Martí,nez Gonzá,lez, M. J.,Asensio Ramos, A.,Manso Sainz, R.,Khomenko, E.,Martí,nez Pillet, V.,Solanki, S. K.,Ló,pez Ariste, A.,Schmidt, W.,Barthol, P.,Gandorfer, A. IOP Publishing 2011 ASTROPHYSICAL JOURNAL LETTERS - Vol.730 No.2
<P>We present observational evidence for oscillations of magnetic flux density in the quiet areas of the Sun. The majority of magnetic fields on the solar surface have strengths of the order of or lower than the equipartition field (300-500 G). This results in a myriad of magnetic fields whose evolution is largely determined by the turbulent plasma motions. When granules evolve they squash the magnetic field lines together or pull them apart. Here, we report on the periodic deformation of the shapes of features in circular polarization observed at high resolution with SUNRISE. In particular, we note that the area of patches with a constant magnetic flux oscillates with time, which implies that the apparent magnetic field intensity oscillates in antiphase. The periods associated with this oscillatory pattern are compatible with the granular lifetime and change abruptly, which suggests that these oscillations might not correspond to characteristic oscillatory modes of magnetic structures, but to the forcing by granular motions. In one particular case, we find three patches around the same granule oscillating in phase, which means that the spatial coherence of these oscillations can reach 1600 km. Interestingly, the same kind of oscillatory phenomenon is also found in the upper photosphere.</P>
Anel Perales-Martí,nez, I.,Rodrí,guez-Gonzá,lez, Vicente,Lee, Soo-Wohn Elsevier 2014 Materials letters Vol.123 No.-
Nanosized cuboid-like TiO2 with anatase-rutile structure was synthesized by using a microwave-assisted hydrothermal method. Silver nanoparticles, which were photoreduced on TiO2 P25 (STiO2), or TiO2 P25 was used as the precursor and HF was the source of F- ions, which played the role of capping agents. The synthesis was performed at pH 2 and 190 degrees C for 5 h. Fluorine species (HF) are important as stabilizing and shape-controlling agents which lead to the formation of TiO2 square-shaped plate nanoparticles. (C) 2014 Elsevier B.V. All rights reserved.
SURFACE WAVES IN SOLAR GRANULATION OBSERVED WITH SUNRISE
Roth, M.,Franz, M.,Bello Gonzá,lez, N.,Martí,nez Pillet, V.,Bonet, J. A.,Gandorfer, A.,Barthol, P.,Solanki, S. K.,Berkefeld, T.,Schmidt, W.,del Toro Iniesta, J. C.,Domingo, V.,Knö,lker IOP Publishing 2010 ASTROPHYSICAL JOURNAL LETTERS - Vol.723 No.2
Stewart, S. J.,Marco, J. F.,Crespo, P.,Romero, J. J.,Martí,nez, A.,Hernando, A.,Palomares, F. J.,Gonzá,lez, J. M. American Scientific Publishers 2007 Journal of Nanoscience and Nanotechnology Vol.7 No.11
<P>We report on the temperature dependencies of the Mössbauer spectra and the AC magnetic susceptibility measured in Cu-rich, FeMnCu samples prepared by mechanically alloying, using, on the one side, Cu and prealloyed FeMn powders and, on the other, pure element Cu, Mn, and Fe powders. From the correlation of the Mössbauer and susceptibility data we conclude about the basic characteristics of the phase distributions present in the different studied samples. Those distributions are a consequence of both the nanostructure induced upon milling and of the different signs of the Mn/Cu (negative) and Fe/Cu (positive) enthalpies of mixing. The proposed phase distributions are significantly different in the samples prepared from different precursors and this fact is analyzed in terms of the disproportion of the precursor FeMn alloy and in those of the favoured Mn/Cu interdiffusion and the hindered Fe/Cu one.</P>
Probing deep photospheric layers of the quiet Sun with high magnetic sensitivity
Lagg, A.,Solanki, S. K.,Doerr, H.-P.,Martí,nez Gonzá,lez, M. J.,Riethmü,ller, T.,Collados Vera, M.,Schlichenmaier, R.,Orozco Suá,rez, D.,Franz, M.,Feller, A.,Kuckein, C.,Schmidt, EDP Sciences 2016 Astronomy and astrophysics Vol.596 No.-