Zobrazeno 1 - 10
of 229
pro vyhledávání: '"Barthol, P."'
Autor:
Chaouche, L. Yelles, Cameron, R. H., Solanki, S. K., Riethmüller, T. L., Anusha, L. S., Witzke, V., Shapiro, A. I., Barthol, P., Gandorfer, A., Gizon, L., Hirzberger, J., van Noort, M., Rodríguez, J. Blanco, Iniesta, J. C. Del Toro, Suárez, D. Orozco, Schmidt, W., Pillet, V. Martínez, Knölker, M.
Publikováno v:
A&A 644, A44 (2020)
The solar photosphere provides us with a laboratory for understanding turbulence in a layer where the fundamental processes of transport vary rapidly and a strongly superadiabatic region lies very closely to a subadiabatic layer. Our tools for probin
Externí odkaz:
http://arxiv.org/abs/2010.09037
Autor:
Barry A. Whaley, Jonathan G. Martinis, Giuseppe F. Pagano, Sara Barthol, Jessica Senzer, Pamela R. Williamson, Peter D. Blanck
Publikováno v:
Laws, Vol 13, Iss 1, p 5 (2024)
Since the passage of the landmark Americans with Disabilities Act of 1990, the United States federal government, states, and localities have passed laws and created policies intended to ensure that people with disabilities had full and equal access t
Externí odkaz:
https://doaj.org/article/a7aba6669af6469bbe37c878ce2362b4
Autor:
Gorobets, A. Y., Berdyugina, S. V., Riethmüller, T. L., Rodríguez, J. Blanco, Solanki, S. K., Barthol, P., Gandorfer, A., Gizon, L., Hirzberger, J., van Noort, M., Iniesta, J. C. Del Toro, Suárez, D. Orozco, Schmidt, W., Pillet, V. Martínez, Knölker, M.
Publikováno v:
2017 ApJS 233 5
The observed magnetic field on the solar surface is characterized by a very complex spatial and temporal behavior. Although feature-tracking algorithms have allowed us to deepen our understanding of this behavior, subjectivity plays an important role
Externí odkaz:
http://arxiv.org/abs/1710.08361
Autor:
Gafeira, R., Jafarzadeh, S., Solanki, S. K., Lagg, A., Van Noort, M., Barthol, P., RodrÍguez, J. Blanco, Iniesta, J. C. Del Toro, Gandorfer, A., Gizon, L., Hirzberger, J., KnÖlker, M., SuÁrez, D. Orozco, RiethmÜller, T. L., Schmidt, W.
We report the detection of oscillations in slender Ca II H fibrils (SCFs) from high-resolution observations acquired with the Sunrise balloon-borne solar observatory. The SCFs show obvious oscillations in their intensity, but also their width. The os
Externí odkaz:
http://arxiv.org/abs/1701.02801
Autor:
Solanki, S. K., Riethmüller, T. L., Barthol, P., Danilovic, S., Deutsch, W., Doerr, H. P., Feller, A., Gandorfer, A., Germerott, D., Gizon, L., Grauf, B., Heerlein, K., Hirzberger, J., Kolleck, M., Lagg, A., Meller, R., Tomasch, G., van Noort, M., Rodríguez, J. Blanco, Blesa, J. L. Gasent, Jiménez, M. Balaguer, Iniesta, J. C. Del Toro, Jiménez, A. C. López, Suárez, D. Orozco, Berkefeld, T., Halbgewachs, C., Schmidt, W., Álvarez-Herrero, A., Sabau-Graziati, L., Grande, I. Pérez, Pillet, V. Martínez, Card, G., Centeno, R., Knölker, M., Lecinski, A.
The SUNRISE balloon-borne solar observatory, consisting of a 1~m aperture telescope that provided a stabilized image to a UV filter imager and an imaging vector polarimeter, carried out its second science flight in June 2013. It provided observations
Externí odkaz:
http://arxiv.org/abs/1701.01555
Magneto-static modelling from SUNRISE/IMaX: Application to an active region observed with SUNRISE II
Autor:
Wiegelmann, T., Neukirch, T., Nickeler, D. H., Solanki, S. K., Barthol, P., Gandorfer, A., Gizon, L., Hirzberger, J., Riethmüller, T. L., van Noort, M., Rodríguez, J. Blanco, Iniesta, J. C. Del Toro, Suárez, D. Orozco, Schmidt, W., Pillet, V. Martínez, Knölker, M.
Magneto-static models may overcome some of the issues facing force-free magnetic field extrapolations. So far they have seen limited use and have faced problems when applied to quiet-Sun data. Here we present a first application to an active region.
Externí odkaz:
http://arxiv.org/abs/1701.01458
Autor:
Gafeira, R., Lagg, A., Solanki, Sami K, Jafarzadeh, Shahin, Van Noort, M., Barthol, P., Rodriguez, J. Blanco, Iniesta, J. C. del Toro, Gandorfer, A., Gizon, L., Hirzberger, J., Knolker, M., Suarez, D. Orozco, Riethmüller, T. L., Schmidt, W.
We use seeing-free high spatial resolution Ca II H data obtained by the SUNRISE observatory to determine properties of slender fibrils in the lower solar chromosphere. In this work we use intensity images taken with the SUFI instrument in the Ca II H
Externí odkaz:
http://arxiv.org/abs/1612.00319
Autor:
Requerey, Iker S., Cobo, B. Ruiz, Iniesta, J. C. Del Toro, Suárez, D. Orozco, Rodríguez, J. Blanco, Solanki, S. K., Barthol, P., Gandorfer, A., Gizon, L., Hirzberger, J., Riethmüller, T. L., van Noort, M., Schmidt, W., Pillet, V. Martínez, Knölker, M.
We study the dynamics and topology of an emerging magnetic flux concentration using high spatial resolution spectropolarimetric data acquired with the Imaging Magnetograph eXperiment on board the Sunrise balloon-borne solar observatory. We obtain the
Externí odkaz:
http://arxiv.org/abs/1611.06732
Autor:
Riethmüller, T. L., Solanki, S. K., Barthol, P., Gandorfer, A., Gizon, L., Hirzberger, J., van Noort, M., Rodríguez, J. Blanco, Iniesta, J. C. Del Toro, Suárez, D. Orozco, Schmidt, W., Pillet, V. Martínez, Knölker, M.
We present a new method of Stokes inversion of spectropolarimetric data and evaluate it by taking the example of a SUNRISE/IMaX observation. An archive of synthetic Stokes profiles is obtained by the spectral synthesis of state-of-the-art magnetohydr
Externí odkaz:
http://arxiv.org/abs/1611.05175
Autor:
Chitta, L. P., Peter, H., Solanki, S. K., Barthol, P., Gandorfer, A., Gizon, L., Hirzberger, J., Riethmueller, T. L., van Noort, M., Rodriguez, J. Blanco, Iniesta, J. C. Del Toro, Suarez, D. Orozco, Schmidt, W., Pillet, V. Martinez, Knoelker, M.
Publikováno v:
2017, ApJS, 229, 4
How and where are coronal loops rooted in the solar lower atmosphere? The details of the magnetic environment and its evolution at the footpoints of coronal loops are crucial to understanding the processes of mass and energy supply to the solar coron
Externí odkaz:
http://arxiv.org/abs/1610.07484