Zobrazeno 1 - 10
of 551
pro vyhledávání: '"Tsuneta, S."'
Autor:
Bueno, J. Trujillo, Štěpán, J., Belluzzi, L., Ramos, A. Asensio, Sainz, R. Manso, Alemán, T. del Pino, Casini, R., Ishikawa, R., Kano, R., Winebarger, A., Auchère, F., Narukage, N., Kobayashi, K., Bando, T., Katsukawa, Y., Kubo, M., Ishikawa, S., Giono, G., Hara, H., Suematsu, Y., Shimizu, T., Sakao, T., Tsuneta, S., Ichimoto, K., Cirtain, J., Champey, P., De Pontieu, B., Carlsson, M.
The Chromospheric Lyman-Alpha Spectro-Polarimeter (CLASP) is a suborbital rocket experiment that on 3rd September 2015 measured the linear polarization produced by scattering processes in the hydrogen Ly-$\alpha$ line of the solar disk radiation, who
Externí odkaz:
http://arxiv.org/abs/1809.08865
Autor:
Stepan, J., Bueno, J. Trujillo, Belluzzi, L., Ramos, A. Asensio, Sainz, R. Manso, Aleman, T. del Pino, Casini, R., Kano, R., Winebarger, A., Auchere, F., Ishikawa, R., Narukage, N., Kobayashi, K., Bando, T., Katsukawa, Y., Kubo, M., Ishikawa, S., Giono, G., Hara, H., Suematsu, Y., Shimizu, T., Sakao, T., Tsuneta, S., Ichimoto, K., Cirtain, J., Champey, P., De Pontieu, B., Carlsson, M.
On 3rd September 2015, the Chromospheric Lyman-Alpha SpectroPolarimeter (CLASP) successfully measured the linear polarization produced by scattering processes in the hydrogen Lyman-$\alpha$ line of the solar disk radiation, revealing conspicuous spat
Externí odkaz:
http://arxiv.org/abs/1808.02725
Discovery of Scattering Polarization in the Hydrogen Lyman-$\alpha$ Line of the Solar Disk Radiation
Autor:
Kano, R., Bueno, J. Trujillo, Winebarger, A., Auchère, F., Narukage, N., Ishikawa, R., Kobayashi, K., Bando, T., Katsukawa, Y., Kubo, M., Ishikawa, S., Giono, G., Hara, H., Suematsu, Y., Shimizu, T., Sakao, T., Tsuneta, S., Ichimoto, K., Goto, M., Belluzzi, L., Štěpán, J., Ramos, A. Asensio, Sainz, R. Manso, Champey, P., Cirtain, J., De Pontieu, B., Casini, R., Carlsson, M.
Publikováno v:
The Astrophysical Journal Letters, Volume 839, Number 1, L10, 2017
There is a thin transition region (TR) in the solar atmosphere where the temperature rises from 10,000 K in the chromosphere to millions of degrees in the corona. Little is known about the mechanisms that dominate this enigmatic region other than the
Externí odkaz:
http://arxiv.org/abs/1704.03228
We investigated the role of photospheric plasma motions in the formation and evolution of polar magnetic patches using time-sequence observations with high spatial resolution. The observations were obtained with the spectropolarimeter on board the Hi
Externí odkaz:
http://arxiv.org/abs/1412.8023
Autor:
Watanabe, H., Narukage, N., Kubo, M., Ishikawa, R., Bando, T., Kano, R., Tsuneta, S., Kobayashi, K., Ichimoto, K., Trujillo-Bueno, J.
Publikováno v:
Proc. SPIE 8148, Solar Physics and Space Weather Instrumentation IV, 81480T (7 October 2011)
A sounding-rocket program called the Chromospheric Lyman-Alpha Spectro-Polarimeter (CLASP) is proposed to be launched in the summer of 2014. CLASP will observe the solar chromosphere in Ly-alpha (121.567 nm), aiming to detect the linear polarization
Externí odkaz:
http://arxiv.org/abs/1407.4577
Autor:
Ishikawa, R., Ramos, A. Asensio, Belluzzi, L., Sainz, R. Manso, Stepan, J., Bueno, J. Trujillo, Goto, M., Tsuneta, S.
Magnetic field measurements in the upper chromosphere and above, where the gas-to-magnetic pressure ratio $\beta$ is lower than unity, are essential for understanding the thermal structure and dynamical activity of the solar atmosphere. Recent develo
Externí odkaz:
http://arxiv.org/abs/1404.0786
Publikováno v:
The Astrophysical Journal, 776:122 (6pp), 2013 October 20
The magnetic properties of the Sun's polar faculae are investigated with spectropolarimetric observations of the north polar region obtained by the Hinode satellite in 2007 September. Polar faculae are embedded in nearly all magnetic patches with flu
Externí odkaz:
http://arxiv.org/abs/1311.0980
We have been monitoring yearly variation in the Sun's polar magnetic fields with the Solar Optical Telescope aboard {\it Hinode} to record their evolution and expected reversal near the solar maximum. All magnetic patches in the magnetic flux maps ar
Externí odkaz:
http://arxiv.org/abs/1205.2154
Publikováno v:
4th Hinode Science Meeting: Unsolved Problems and New Insights, edited by L.R. Bellot Rubio, F. Reale, and M. Carlsson, ASP Conference Series, Vol. 455 (2012)
The heating of the solar corona is one of the big questions in astrophysics. Rapid pulses called nanoflares are among the best candidate mechanisms. The analysis of the time variability of coronal X-ray emission is potentially a very useful tool to d
Externí odkaz:
http://arxiv.org/abs/1201.5482
We infer the 3D magnetic structure of a transient horizontal magnetic field (THMF) during its evolution through the photosphere using SIRGAUS inversion code. The SIRGAUS code is a modified version of SIR (Stokes Inversion based on Response function),
Externí odkaz:
http://arxiv.org/abs/1003.1376