Results 61 to 70 of about 5,529 (192)

Current Status and Future Prospects of the SNO+ Experiment

Advances in High Energy Physics, Volume 2016, Issue 1, 2016., 2016
SNO+ is a large liquid scintillator‐based experiment located 2 km underground at SNOLAB, Sudbury, Canada. It reuses the Sudbury Neutrino Observatory detector, consisting of a 12 m diameter acrylic vessel which will be filled with about 780 tonnes of ultra‐pure liquid scintillator. Designed as a multipurpose neutrino experiment, the primary goal of SNO+
S. Andringa, E. Arushanova, S. Asahi, M. Askins, D. J. Auty, A. R. Back, Z. Barnard, N. Barros, E. W. Beier, A. Bialek, S. D. Biller, E. Blucher, R. Bonventre, D. Braid, E. Caden, E. Callaghan, J. Caravaca, J. Carvalho, L. Cavalli, D. Chauhan, M. Chen, O. Chkvorets, K. Clark, B. Cleveland, I. T. Coulter, D. Cressy, X. Dai, C. Darrach, B. Davis-Purcell, R. Deen, M. M. Depatie, F. Descamps, F. Di Lodovico, N. Duhaime, F. Duncan, J. Dunger, E. Falk, N. Fatemighomi, R. Ford, P. Gorel, C. Grant, S. Grullon, E. Guillian, A. L. Hallin, D. Hallman, S. Hans, J. Hartnell, P. Harvey, M. Hedayatipour, W. J. Heintzelman, R. L. Helmer, B. Hreljac, J. Hu, T. Iida, C. M. Jackson, N. A. Jelley, C. Jillings, C. Jones, P. G. Jones, K. Kamdin, T. Kaptanoglu, J. Kaspar, P. Keener, P. Khaghani, L. Kippenbrock, J. R. Klein, R. Knapik, J. N. Kofron, L. L. Kormos, S. Korte, C. Kraus, C. B. Krauss, K. Labe, I. Lam, C. Lan, B. J. Land, S. Langrock, A. LaTorre, I. Lawson, G. M. Lefeuvre, E. J. Leming, J. Lidgard, X. Liu, Y. Liu, V. Lozza, S. Maguire, A. Maio, K. Majumdar, S. Manecki, J. Maneira, E. Marzec, A. Mastbaum, N. McCauley, A. B. McDonald, J. E. McMillan, P. Mekarski, C. Miller, Y. Mohan, E. Mony, M. J. Mottram, V. Novikov, H. M. O’Keeffe, E. O’Sullivan, G. D. Orebi Gann, M. J. Parnell, S. J. M. Peeters, T. Pershing, Z. Petriw, G. Prior, J. C. Prouty, S. Quirk, A. Reichold, A. Robertson, J. Rose, R. Rosero, P. M. Rost, J. Rumleskie, M. A. Schumaker, M. H. Schwendener, D. Scislowski, J. Secrest, M. Seddighin, L. Segui, S. Seibert, T. Shantz, T. M. Shokair, L. Sibley, J. R. Sinclair, K. Singh, P. Skensved, A. Sörensen, T. Sonley, R. Stainforth, M. Strait, M. I. Stringer, R. Svoboda, J. Tatar, L. Tian, N. Tolich, J. Tseng, H. W. C. Tseung, R. Van Berg, E. Vázquez-Jáuregui, C. Virtue, B. von Krosigk, J. M. G. Walker, M. Walker, O. Wasalski, J. Waterfield, R. F. White, J. R. Wilson, T. J. Winchester, A. Wright, M. Yeh, T. Zhao, K. Zuber, Vincenzo Flaminio   +156 more
wiley   +1 more source

Observational Evidence of Shallow Origins for the Magnetic Fields of Solar Cycles

Frontiers in Astronomy and Space Sciences, 2018
Observational evidence for the origin of active region magnetic fields has been sought from published information on extended solar cycles, statistical distributions of active regions and ephemeral regions, helioseismology results, positional ...
Sara F. Martin
doaj   +1 more source

Inferring the Solar Meridional Circulation Flow Profile by Applying Bayesian Methods to Time–Distance Helioseismology

The Astrophysical Journal, 2023
Mapping the large-scale subsurface plasma flow profile within the Sun has been attempted using various methods for several decades. One such flow in particular is the meridional circulation, for which numerous studies have been published.
Aleczander Herczeg, Jason Jackiewicz
doaj   +1 more source

Solar Dynamics, Rotation, Convection and Overshoot

, 2015
We discuss recent observational, theoretical and modeling progress made in understanding the Sun's internal dynamics, including its rotation, meridional flow, convection and overshoot.
Hanasoge, S., Miesch, M. S., Roth, M., Schou, J., Schuessler, M., Thompson, M. J.   +5 more
core   +1 more source

Initial Helioseismic Observations by Hinode/SOT [PDF]

, 2007
Results from initial helioseismic observations by Solar Optical Telescope onboard Hinode are reported. It has been demonstrated that intensity oscillation data from Broadband Filter Imager can be used for various helioseismic analyses.
Berger, Thomas E., Ichimoto, Kiyoshi, Katsukawa, Yukio, Kosovichev, Alexander G., Lites, Bruce W., Nagata, Shin'ichi, Sekii, Takashi, Shibahashi, Hiromoto, Shimizu, Toshifumi, Shine, Richard A., Suematsu, Yoshinori, Tarbell, Theodore D., Title, Alan M., Tsuneta, Saku, Zhao, Junwei   +14 more
core   +1 more source

Estimation of Spectral Solar Irradiance in the Ecliptic Plane Using Synthetic Solar Surface Magnetograms

Journal of Geophysical Research: Space Physics, Volume 129, Issue 5, May 2024.
Abstract The primary external energy input to planetary atmospheres comes from solar radiation. Accurate estimates of solar irradiance are needed in order to understand atmospheric conditions at other planets. Many studies have interpolated Earth‐based irradiance measurements at other planets, disregarding the evolution of solar features, which are ...
I. de Oliveira, K. Sowmya, N.‐E. Nèmec, A. I. Shapiro   +3 more
wiley   +1 more source

Probable Value for the Next Sunspot Minimum

Advances in Astronomy, Volume 2014, Issue 1, 2014., 2014
Gumbel’s first distribution is applied to smoothed monthly mean sunspot numbers for solar cycles 10 to 24. According to that, the next minimum for solar cycle 24‐25 transition would be the deepest solar minimum of the last 150 years. This study provides an additional insight about changes in the Sun which are currently happening.
Virginia Mabel Silbergleit, Gary Wegner
wiley   +1 more source

Global helioseismology (WP4.1): From the Sun to the stars & solar analogs

EPJ Web of Conferences, 2017
Sun-as-a star observations put our star as a reference for stellar observations. Here, I review the activities in which the SPACEINN global seismology team (Working Package WP4.1) has worked during the past 3 years. In particular, we will explain the new
García Rafael A.
doaj   +1 more source

Time--Distance Helioseismology Data Analysis Pipeline for Helioseismic and Magnetic Imager onboard Solar Dynamics Observatory (SDO/HMI) and Its Initial Results [PDF]

, 2011
The Helioseismic and Magnetic Imager onboard the Solar Dynamics Observatory (SDO/HMI) provides continuous full-disk observations of solar oscillations.
A. C. Birch, A. G. Kosovichev, A.C. Birch, A.C. Birch, A.C. Birch, A.G. Kosovichev, A.G. Kosovichev, A.G. Kosovichev, A.G. Kosovichev, B.H. Jacobsen, C. Lindsey, C. Lindsey, C. Lindsey, D. Georgobiani, D.-Y. Chou, D.A. Haber, H. Schunker, H.B. Snodgrass, I.N. Kitiashvili, J. G. Beck, J. Jackiewicz, J. Zhao, J. Zhao, J. Zhao, J. Zhao, J. Zhao, J. Zhao, J. Zhao, J. Zhao, J.G. Beck, J.M. Jensen, J.M. Jensen, J.M. Jensen, K. V. Parchevsky, K.V. Parchevsky, L. Gizon, L. Gizon, L. Gizon, L. Zhao, M. Rempel, P. H. Scherrer, P.H. Scherrer, P.M. Giles, R. Komm, R. Nigam, R. S. Bogart, R.F. Stein, S. Couvidat, S. Couvidat, S. Couvidat, S. Couvidat, S. Couvidat, S. Ilonidis, S. Zharkov, S.M. Hanasoge, S.P. Rajaguru, T. L. Duvall, T. Sekii, T.L. Duvall Jr., T.L. Duvall Jr., T.L. Duvall Jr., T.L. Duvall Jr.   +61 more
core   +3 more sources

Solar Cycle Variations of Rotation and Asphericity in the Near-Surface Shear Layer

, 2018
The precise shape of the Sun is sensitive to the influence of gravity, differential rotation, local turbulence and magnetic fields. It has been previously shown that the solar shape exhibits asphericity that evolves with the 11-year cycle.
Kosovichev, A. G., Rozelot, J. -P.
core   +3 more sources