Zobrazeno 1 - 10
of 23
pro vyhledávání: '"Simone Di Matteo"'
Autor:
Martin O. Archer, Xueling Shi, Maria-Theresia Walach, Michael D. Hartinger, D. Megan Gillies, Simone Di Matteo, Frances Staples, Katariina Nykyri
Publikováno v:
Frontiers in Astronomy and Space Sciences, Vol 11 (2024)
The dynamics of Earth’s magnetopause, driven by several different external/internal physical processes, plays a major role in the geospace energy budget. Given magnetopause motion couples across many space plasma regions, numerous forms of observat
Externí odkaz:
https://doaj.org/article/c632af0cf62948f2870de261a0f0f86d
Publikováno v:
The Astrophysical Journal, Vol 969, Iss 1, p 67 (2024)
Periodic density structures (PDSs) are quasiperiodic variations of solar wind density ranging from a few minutes to a few hours. PDSs advect with the solar wind and have radial length scales ( L _x ) of tens to several thousand megameters, thus belon
Externí odkaz:
https://doaj.org/article/d0efd7420bbb407b968c9ea0bc7f7e88
Autor:
Katariina Nykyri, Xuanye Ma, Brandon Burkholder, Yu-Lun Liou, Roberto Cuéllar, Shiva Kavosi, Joseph E. Borovsky, Jeff Parker, Mitchell Rosen, Lauren De Moudt, Robert Wilkes Ebert, Keiichi Ogasawara, Merav Opher, David Gary Sibeck, Simone Di Matteo, Nicholeen Viall, Samantha Wallace, Therese M. Jorgensen, Michael Hesse, Matthew J. West, Laxman Adhikari, Matthew R. Argall, Jan Egedal, Frederick Wilder, Jeffrey Broll, Gangkai Poh, Simon Wing, Christopher Russell
Publikováno v:
Frontiers in Astronomy and Space Sciences, Vol 10 (2023)
This paper summarizes the Seven Sisters solar wind mission concept and the outstanding science questions motivating the mission science objectives. The Seven Sisters mission includes seven individual spacecraft designed to uncover fundamental physica
Externí odkaz:
https://doaj.org/article/7455b9825bb848868c43111f3f241538
Autor:
Nathalia Alzate, Simone Di Matteo, Huw Morgan, Daniel B. Seaton, Mari Paz Miralles, Laura Balmaceda, Michael S. Kirk, Matthew West, Craig DeForest, Angelos Vourlidas
Publikováno v:
Frontiers in Astronomy and Space Sciences, Vol 10 (2023)
Establishing the Sun-Earth connection requires overcoming the challenges of exploring the data from past and current missions and leveraging tools and models (data mining) to create an efficient system treatment of the Sun and heliosphere. However, s
Externí odkaz:
https://doaj.org/article/0a43b6409dc54406a1c294a2df319198
Autor:
Simone Di Matteo, Nithin Sivadas
Publikováno v:
Frontiers in Astronomy and Space Sciences, Vol 9 (2022)
Many studies of solar-wind coupling with the magnetosphere depend on the properties of the solar wind impacting the magnetosphere. Our ability to estimate these properties relies heavily on spacecraft measurements at the first Lagrangian point (L1),
Externí odkaz:
https://doaj.org/article/ef3883a862d24c8aa80daa87300c46d6
Publikováno v:
The Astrophysical Journal, Vol 945, Iss 2, p 116 (2023)
Understanding the solar corona requires knowledge of its dynamics through its various layers and subsequent connectivity to the heliosphere. This requires understanding the nature of the outflows and the physical transitions through the middle corona
Externí odkaz:
https://doaj.org/article/5c628dfced654d74acdb3f12a6866a87
Autor:
Michael Pezzopane, Afredo Del Corpo, Mirko Piersanti, Claudio Cesaroni, Alessio Pignalberi, Simone Di Matteo, Luca Spogli, Massimo Vellante, Balazs Heilig
Publikováno v:
Earth, Planets and Space, Vol 71, Iss 1, Pp 1-21 (2019)
Abstract This paper presents how the magnetosphere–plasmasphere–ionosphere system was affected as a whole during the geomagnetic storm peaking on 27 May 2017. The interplanetary conditions, the magnetospheric response in terms of the magnetopause
Externí odkaz:
https://doaj.org/article/dc6ccf1913dd4f12ac65ab74366f316e
Autor:
Simone Di Matteo, Larry Kepko, Nicholeen Viall, Aaron Breneman, Alexa Halford, Umberto Villante
In the solar wind density, we often observe periodic fluctuations on time scales ranging from a few minutes to a few hours which we refer to as Periodic Density Structures (PDSs). The PDSs belong to the class of “meso-scale structures” with radia
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::3d48b7a470ce690c4490a7a562a0562b
https://doi.org/10.5194/egusphere-egu23-10258
https://doi.org/10.5194/egusphere-egu23-10258
Understanding the source of the variability in the slow solar wind is a key part of Space Weather research because it can lead to an understanding of the physical processes that drive solar activity, heat the corona and accelerate the solar wind. Ach
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::1f506a34c6141a25d5e59cb887adba73
https://doi.org/10.5194/egusphere-egu23-10248
https://doi.org/10.5194/egusphere-egu23-10248
Understanding the solar corona requires knowledge of its dynamics through its various layers and subsequent connectivity to the heliosphere. This requires understanding the nature of the outflows and the physical transitions through the middle corona
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d0163efc5442b087ce19f45f6f7b6574