Zobrazeno 1 - 10
of 53
pro vyhledávání: '"Sarah E, Gibson"'
Autor:
Jie Zhao, Fu Yu, Sarah E. Gibson, Yuhong Fan, Yang Su, Ying Li, Jun Dai, Hui Li, Chuan Li, Pengfei Chen, Ming-De Ding, Cheng Fang
Publikováno v:
The Astrophysical Journal Letters, Vol 965, Iss 2, p L16 (2024)
Active regions are the brightest structures seen in the solar corona, so their physical properties hold important clues to the physical mechanisms underlying coronal heating. In this work, we present a comprehensive study for a filament-embedding act
Externí odkaz:
https://doaj.org/article/00e46940918f4f7f92c264779070447d
Autor:
Elena Provornikova, Viacheslav G. Merkin, Angelos Vourlidas, Anna Malanushenko, Sarah E. Gibson, Eric Winter, Charles N. Arge
Publikováno v:
The Astrophysical Journal, Vol 977, Iss 1, p 106 (2024)
Variations of the magnetic field within a solar coronal mass ejection (CME) in the heliosphere depend on the CME’s magnetic structure as it leaves the solar corona and its interplanetary evolution. To account for this evolution, we developed a new
Externí odkaz:
https://doaj.org/article/2663af7982ce48d181dd52543900db9c
Autor:
Shaheda Begum Shaik, Mark G. Linton, Sarah E. Gibson, Phillip Hess, Robin C. Colaninno, Guillermo Stenborg, Carlos R. Braga, Erika Palmerio
Publikováno v:
The Astrophysical Journal, Vol 976, Iss 2, p 179 (2024)
Despite the significance of coronal mass ejections (CMEs) in space weather, a comprehensive understanding of their interior morphology remains a scientific challenge, particularly with the advent of many state-of-the-art solar missions such as Parker
Externí odkaz:
https://doaj.org/article/32a5a70ff3934973892110b7d9110ece
Autor:
Valmir P. Moraes Filho, Vadim M. Uritsky, Barbara J. Thompson, Sarah E. Gibson, Craig E. DeForest
Publikováno v:
The Astrophysical Journal, Vol 975, Iss 2, p 294 (2024)
The Synthetic Corona Outflow Model (SynCOM), an empirical model, simulates the solar corona’s dynamics to match high-resolution observations, providing a useful resource for testing velocity measurement algorithms. SynCOM generates synthetic images
Externí odkaz:
https://doaj.org/article/88e37ad7a7cd4353894db070b7da627a
Publikováno v:
The Astrophysical Journal, Vol 971, Iss 1, p 27 (2024)
Magnetic fields are the primary driver of the plasma thermodynamics in the upper solar atmosphere, especially in the corona. However, magnetic field measurements in the solar corona are sporadic, thereby limiting us from the complete understanding of
Externí odkaz:
https://doaj.org/article/31f0bc0b5b144a518aff652e13922dfc
Autor:
Enrico Landi, Sarah E. Gibson, Steven Tomczyk, Joan Burkepile, Giuliana de Toma, Jie Zhang, Tom Schad, Therese A. Kucera, Katharine K. Reeves, Hebe Cremades
Publikováno v:
Frontiers in Astronomy and Space Sciences, Vol 9 (2022)
The Need: Understanding and predicting the major phenomena taking place in the solar corona, such as flares and Coronal Mass Ejections (CMEs), the heating and evolution of the solar atmosphere, and the acceleration of the solar wind, are fundamental
Externí odkaz:
https://doaj.org/article/358f4c2c225549478e27cfe10de69b7f
Autor:
Tristan Loveday, Gerben Duns, Lisa M. Rimsza, Karen L. Rech, James R. Cook, Ryan S. Robetorye, Allison C. Rosenthal, Colleen A. Ramsower, Tameson K. Yip, Catherine L. McKinney, Steven H. Swerdlow, Shweta Bhavsar, Christian Steidl, Sarah E. Gibson
Publikováno v:
Blood Advances. 7:893-899
We investigated the clinicopathologic features of 5 follicular lymphomas (FLs) that transformed (tFL) morphologically to diffuse large B-cell lymphomas (DLBCLs) and had a primary mediastinal large B-cell lymphoma (PMBL)–like gene expression profile
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b074d5769f94e14f345db1d24ec3af63
https://doi.org/10.1182/bloodadvances.2022007360
https://doi.org/10.1182/bloodadvances.2022007360
Autor:
Sarah E. Gibson
Publikováno v:
Living Reviews in Solar Physics, Vol 15, Iss 1, Pp 1-39 (2018)
Abstract Magnetic fields suspend the relatively cool material of solar prominences in an otherwise hot corona. A comprehensive understanding of solar prominences ultimately requires complex and dynamic models, constrained and validated by observation
Externí odkaz:
https://doaj.org/article/48c804a1bb5b4a85a594e749aa040fa0
Autor:
Bryan Rea, Yen-Chun Liu, Alanna Maguire, Lorinda A. Soma, Chris M. Bacon, Michael G. Bayerl, Molly H. Smith, Michael T. Barrett, Steven H. Swerdlow, Sarah E. Gibson
Publikováno v:
Modern Pathology. 35:938-945
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::096765798b2380506c4c2e9d31e11e88
https://doi.org/10.1038/s41379-021-01002-6
https://doi.org/10.1038/s41379-021-01002-6
Autor:
Sarah E. Gibson, Angelos Vourlidas, Donald M. Hassler, Laurel A. Rachmeler, Michael J. Thompson, Jeffrey Newmark, Marco Velli, Alan Title, Scott W. McIntosh
Publikováno v:
Frontiers in Astronomy and Space Sciences, Vol 5 (2018)
We explore new opportunities for solar physics that could be realized by future missions providing sustained observations from vantage points away from the Sun-Earth line. These include observations from the far side of the Sun, at high latitudes inc
Externí odkaz:
https://doaj.org/article/32e1d0fd5ed74cd788ad4f3ad2eee861