Zobrazeno 1 - 10
of 14 068
pro vyhledávání: '"A. Polito"'
Autor:
G. Dowse, E.J. Perkins, H.M. Stein, G. Chidini, O. Danhaive, Y.N. Elsayed, W.B. Carvalho, N. AlNaqeeb, S. Rooze, M. Cetinkaya, S. Vetter-Laracy, F.J. Pilar-Orive, P. Torpiano, W.A. Gonçalves Ferri, D. Buonsenso, B. Rogdo, A. Medina, A. Polito, C.N.M. Brouwer, M.C.J. Kneyber, D. De Luca, D.G. Tingay, Y. Elsayed, A. MedinaVillanueva, J. Shoemaker, B. Piersigilli, O. Bekkouch, A.A. Oliveira, R. Morello, V. Krebs, P. Valentini, N. Al-Naqeeb, S.M.H. Sabbour, A.E.A. Hegazi, P. Sammut, D. Pace, M. Roldán, B. Yasa, E. Letamendia-Richard, G. Regiroli, A. Vivanti, R. Centorrino, N.F. Oliveira, M.H.M. Dittrich, R. Felgueira, C. Neves, P. Tissieres, A. Amigoni, M. Daverio, A. Tosoni, M.C. Andre, B. Wagner, T. Riedel, P. Rimensberger, A.-S. Ramelet, M.-H. Perez, M. Marston, V. Chanez, D. Longchamp, J. Natterer, T. Ferry, B. Brotschi
Publikováno v:
EClinicalMedicine, Vol 56, Iss , Pp 101822- (2023)
Summary: Background: The benefits of facilitating breastmilk feeding and close contact between mother and neonate (family-centred care; FCC) in the perinatal period are well-established. The aim of this study was to determine how the delivery of FCC
Externí odkaz:
https://doaj.org/article/4e0f301c4b5741b5ab27f96ded9091e4
Autor:
Collier, Hannah, Hayes, Laura A., Purkhart, Stefan, Krucker, Säm, Ryan, Daniel F., Polito, Vanessa, Veronig, Astrid M., Harra, Louise K., Berghmans, David, Kraaikamp, Emil, Dominique, Marie, Dolla, Laurent R., Verbeeck, Cis
Aims: This paper aims to demonstrate the importance of short-exposure extreme ultraviolet (EUV) observations of solar flares in the study of particle acceleration, heating and energy partition in flares. This work highlights the observations now avai
Externí odkaz:
http://arxiv.org/abs/2411.09319
Autor:
Herde, Vicki L., Bose, Souvik, Chamberlin, Phillip C., Schmit, Don, Daw, Adrian, Polito, Vanessa, Gonzalez, Gabriella
The Sun's chromosphere is a critical region to understand when considering energy and mass deposition into the transition region and corona, but many of the smaller, faster events which transport a portion of this mass and energy are still difficult
Externí odkaz:
http://arxiv.org/abs/2411.08801
The definition of generalized random processes in Gel'fand sense allows to extend well-known stochastic models, such as the fractional Brownian motion, and study the related fractional pde's, as well as stochastic differential equations in distributi
Externí odkaz:
http://arxiv.org/abs/2410.22880
We consider a discrete-time Markovian random walk with resets on a connected undirected network. The resets, in which the walker is relocated to randomly chosen nodes, are governed by an independent discrete-time renewal process. Some nodes of the ne
Externí odkaz:
http://arxiv.org/abs/2409.08394
Real-time robot actuation is one of the main challenges to overcome in human-robot interaction. Most visual sensors are either too slow or their data are too complex to provide meaningful information and low latency input to a robotic system. Data ou
Externí odkaz:
http://arxiv.org/abs/2407.11560
The excess broadening of high-temperature spectral lines, long observed near the tops of flare arcades, is widely considered to result from magnetohydrodynamic (MHD) turbulence. According to different theories, plasma turbulence is also believed to b
Externí odkaz:
http://arxiv.org/abs/2407.12174
Autor:
Herde, Vicki L., Chamberlin, Phillip C., Schmit, Don, Daw, Adrian, Milligan, Ryan O., Polito, Vanessa, Bose, Souvik, Boyajian, Spencer, Buedel, Paris, Edgar, Will, Gebben, Alex, Gong, Qian, Jacobsen, Ross, Nell, Nicholas, Schwab, Bennet, Sims, Alan, Summers, David, Turner, Zachary, Valade, Trace, Wallace, Joseph
The Solar eruptioN Integral Field Spectrograph (SNIFS) is a solar-gazing spectrograph scheduled to fly in the summer of 2025 on a NASA sounding rocket. Its goal is to view the solar chromosphere and transition region at a high cadence (1s) both spati
Externí odkaz:
http://arxiv.org/abs/2407.08834
The recent detection of gravitational waves (GWs) by pulsar timing array (PTA) collaborations spurred a variety of questions regarding the origin of the signal and the properties of its sources. The amplitude of a GW background produced by inspiralli
Externí odkaz:
http://arxiv.org/abs/2406.17010
Solar flare ribbon fronts appear ahead of the bright structures that normally characterise solar flares, and can persist for an extended period of time in spatially localised patches before transitioning to `regular' bright ribbons. They likely repre
Externí odkaz:
http://arxiv.org/abs/2405.02799