@article{BalthasarGoemoeryGonzalezManriqueetal.2016,
  author    = {Balthasar, H. and G{\"o}m{\"o}ry, P. and Gonz{\´a}lez Manrique, Sergio Javier and Kuckein, Christoph and Kavka, J. and Kucera, A. and Schwartz, P. and Vaskova, R. and Berkefeld, T. and Collados Vera, M. and Denker, Carsten and Feller, A. and Hofmann, A. and Lagg, A. and Nicklas, H. and Suarez, D. and Pastor Yabar, A. and Rezaei, R. and Schlichenmaier, R. and Schmidt, D. and Schmidt, W. and Sigwarth, M. and Sobotka, M. and Solanki, S. K. and Soltau, D. and Staude, J. and Strassmeier, Klaus G. and Volkmer, R. and von der L{\"u}he, O. and Waldmann, T.},
  title     = {Spectropolarimetric observations of an arch filament system with the GREGOR solar telescope},
  series = {Astronomische Nachrichten = Astronomical notes},
  volume    = {337},
  journal   = {Astronomische Nachrichten = Astronomical notes},
  publisher = {Wiley-VCH},
  address   = {Weinheim},
  issn      = {0004-6337},
  doi       = {10.1002/asna.201612432},
  pages     = {1050 -- 1056},
  year      = {2016},
  abstract  = {Arch filament systems occur in active sunspot groups, where a fibril structure connects areas of opposite magnetic polarity, in contrast to active region filaments that follow the polarity inversion line. We used the GREGOR Infrared Spectrograph (GRIS) to obtain the full Stokes vector in the spectral lines SiI lambda 1082.7 nm, He I lambda 1083.0 nm, and Ca I lambda 1083.9 nm. We focus on the near-infrared calcium line to investigate the photospheric magnetic field and velocities, and use the line core intensities and velocities of the helium line to study the chromospheric plasma. The individual fibrils of the arch filament system connect the sunspot with patches of magnetic polarity opposite to that of the spot. These patches do not necessarily coincide with pores, where the magnetic field is strongest. Instead, areas are preferred not far from the polarity inversion line. These areas exhibit photospheric downflows of moderate velocity, but significantly higher downflows of up to 30 km s(-1) in the chromospheric helium line. Our findings can be explained with new emerging flux where the matter flows downward along the field lines of rising flux tubes, in agreement with earlier results. (C) 2016 WILEY-VCH Verlag GmbH\& Co. KGaA, Weinheim},
  language  = {en}
}
@article{KimSchwartzPerreiraetal.2018,
  author    = {Kim, Su Yeong and Schwartz, Seth J. and Perreira, Krista M. and Juang, Linda P.},
  title     = {Culture's Influence on Stressors, Parental Socialization, and Developmental Processes in the Mental Health of Children of Immigrants},
  series = {Annual Review of clinical psychologgy},
  volume    = {14},
  journal   = {Annual Review of clinical psychologgy},
  publisher = {Annual Reviews},
  address   = {Palo Alto},
  issn      = {1548-5943},
  doi       = {10.1146/annurev-clinpsy-050817-084925},
  pages     = {343 -- 370},
  year      = {2018},
  abstract  = {Children of immigrants represent one in four children in the United States and will represent one in three children by 2050. Children of Asian and Latino immigrants together represent the majority of children of immigrants in the United States. Children of immigrants may be immigrants themselves, or they may have been born in the United States to foreign-born parents; their status may be legal or undocumented. We review transcultural and culture-specific factors that influence the various ways in which stressors are experienced; we also discuss the ways in which parental socialization and developmental processes function as risk factors or protective factors in their influence on the mental health of children of immigrants. Children of immigrants with elevated risk for mental health problems are more likely to be undocumented immigrants, refugees, or unaccompanied minors. We describe interventions and policies that show promise for reducing mental health problems among children of immigrants in the United States.},
  language  = {en}
}