Zobrazeno 1 - 10
of 31
pro vyhledávání: '"Louise, Harra"'
Autor:
Stephanie L. Yardley, Christopher J. Owen, David M. Long, Deborah Baker, David H. Brooks, Vanessa Polito, Lucie M. Green, Sarah Matthews, Mathew Owens, Mike Lockwood, David Stansby, Alexander W. James, Gherardo Valori, Alessandra Giunta, Miho Janvier, Nawin Ngampoopun, Teodora Mihailescu, Andy S. H. To, Lidia van Driel-Gesztelyi, Pascal Démoulin, Raffaella D’Amicis, Ryan J. French, Gabriel H. H. Suen, Alexis P. Rouillard, Rui F. Pinto, Victor Réville, Christopher J. Watson, Andrew P. Walsh, Anik De Groof, David R. Williams, Ioannis Zouganelis, Daniel Müller, David Berghmans, Frédéric Auchère, Louise Harra, Udo Schuehle, Krysztof Barczynski, Éric Buchlin, Regina Aznar Cuadrado, Emil Kraaikamp, Sudip Mandal, Susanna Parenti, Hardi Peter, Luciano Rodriguez, Conrad Schwanitz, Phil Smith, Luca Teriaca, Cis Verbeeck, Andrei N. Zhukov, Bart De Pontieu, Tim Horbury, Sami K. Solanki, Jose Carlos del Toro Iniesta, Joachim Woch, Achim Gandorfer, Johann Hirzberger, David Orozco Súarez, Thierry Appourchaux, Daniele Calchetti, Jonas Sinjan, Fatima Kahil, Kinga Albert, Reiner Volkmer, Mats Carlsson, Andrzej Fludra, Don Hassler, Martin Caldwell, Terje Fredvik, Tim Grundy, Steve Guest, Margit Haberreiter, Sarah Leeks, Gabriel Pelouze, Joseph Plowman, Werner Schmutz, Sunil Sidher, William T. Thompson, Philippe Louarn, Andrei Federov
Publikováno v:
The Astrophysical Journal Supplement Series, Vol 267, Iss 1, p 11 (2023)
The Slow Solar Wind Connection Solar Orbiter Observing Plan (Slow Wind SOOP) was developed to utilize the extensive suite of remote-sensing and in situ instruments on board the ESA/NASA Solar Orbiter mission to answer significant outstanding question
Externí odkaz:
https://doaj.org/article/0066ae64811043d48a0175ce81e45182
Autor:
Louise Harra, Cristina Mandrini
Upflows in the corona are of importance as they may contribute to the solar wind. Because of this, there has been interestin the analysis of upflows at the edges of active regions (ARs). The coronal upflows that are seen at the edges of ARs have coro
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::fb7d93d5e2ec442bf568132753f3d9e1
https://doi.org/10.5194/egusphere-egu23-3094
https://doi.org/10.5194/egusphere-egu23-3094
In this work the analysis of the SOL2022-03-30 X1.4 GOES class flare is presented. This flare was observed by Solar Orbiter during perihelion as well as from Earth based observatories including SDO’s AIA and the Extended Owens Valley Solar Array (E
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::692f4374f0b90a040220f6d6a7f4b01a
https://doi.org/10.5194/egusphere-egu23-11801
https://doi.org/10.5194/egusphere-egu23-11801
Autor:
Krzysztof Barczynski, Louise Harra, Conrad Schwanitz, Nils Janitzek, David Berghmans, Frédéric Auchère, Regina Aznar Cuadrado, Éric Buchlin, Emil Kraaikamp, David M. Long, Sudip Mandal, Susanna Parenti, Hardi Peter, Luciano Rodriguez, Udo Schühle, Phil Smith, Luca Teriaca, Cis Verbeeck, Andrei N. Zhukov
Publikováno v:
Astronomy & Astrophysics, 673
Context. The origin of the slow solar wind is still an open issue. One possibility that has been suggested is that upflows at the edge of an active region can contribute to the slow solar wind. Aims. We aim to explain how the plasma upflows are gener
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cce9f01bd1ef2c6582ad3380c8dd2ae0
https://hdl.handle.net/20.500.11850/615086
https://hdl.handle.net/20.500.11850/615086
Autor:
Andrea Francesco Battaglia, Wen Wang, Jonas Saqri, Tatiana Podladchikova, Astrid M. Veronig, Hannah Collier, Ewan C. M. Dickson, Olena Podladchikova, Christian Monstein, Alexander Warmuth, Frédéric Schuller, Louise Harra, Säm Krucker
Publikováno v:
Astronomy & Astrophysics, 670
Context. One of the main science questions of the Solar Orbiter and Parker Solar Probe missions deals with understanding how electrons in the lower solar corona are accelerated and how they subsequently access interplanetary space. Aims. We aim to in
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::779ea39ef2ed4b85ea3550c82165f219
https://hdl.handle.net/20.500.11850/598928
https://hdl.handle.net/20.500.11850/598928
Autor:
Muriel Zoë Stiefel, Andrea Francesco Battaglia, Krzysztof Barczynski, Hannah Collier, Anna Volpara, Paolo Massa, Conrad Schwanitz, Sofia Tynelius, Louise Harra, Säm Krucker
Publikováno v:
Astronomy & Astrophysics, 670
Context. We present an analysis of a GOES M1.8 flare with excellent observational coverage in UV, extreme-UV (EUV), and X-ray, including observations from the Interface Region Imaging Spectrograph (IRIS), from the Solar Dynamics Observatory (SDO) wit
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::29c0c25f2e76cb02fa9828118eafc01a
https://hdl.handle.net/20.500.11850/599394
https://hdl.handle.net/20.500.11850/599394
Autor:
Sudip Mandal, Hardi Peter, Lakshmi Pradeep Chitta, Regina Aznar Cuadrado, Udo Schühle, Luca Teriaca, Sami K. Solanki, Louise Harra, David Berghmans, Frédéric Auchère, Susanna Parenti, Andrei N. Zhukov, Éric Buchlin, Cis Verbeeck, Emil Kraaikamp, Luciano Rodriguez, David M. Long, Conrad Schwanitz, Krzysztof Barczynski, Gabriel Pelouze, Philip J. Smith, Wei Liu, Mark C. Cheung
Publikováno v:
Astronomy & Astrophysics, 670
The solar chromosphere hosts a wide variety of transients, including dynamic fibrils (DFs) that are characterised as elongated, jet-like features seen in active regions, often through Hα diagnostics. So far, these features have been difficult to ide
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e8ac531ddfb0209046802cf69f74ecd5
https://hdl.handle.net/20.500.11850/597508
https://hdl.handle.net/20.500.11850/597508
Autor:
Louise Harra, Andrea F. Battaglia, Krzysztof Barczynski, Hannah Collier, Säm Krucker, Katharine K. Reeves, George Doschek
Publikováno v:
Solar Physics, 298 (1)
The temperature reached by solar flares is a key parameter to understanding the physical process that causes the energy release. In this work, we analysed data from a Hinode Observing Programme that focused on high cadence measurement of the flaring
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::53a4a43eea5c6f112dc82d84181999c3
Autor:
David H. Brooks, Miho Janvier, Deborah Baker, Harry P. Warren, Frédéric Auchère, Mats Carlsson, Andrzej Fludra, Don Hassler, Hardi Peter, Daniel Müller, David Williams, Regina Aznar Cuadrado, Krzysztof Barczynski, Eric Buchlin, Martin Caldwell, Terje Fredvik, Alessandra Giunta, Tim Grundy, Steve Guest, Margit Haberreiter, Louise Harra, Sarah Leeks, Susanna Parenti, Gabriel Pelouze, Joseph Plowman, Werner Schmutz, Udo Schuehle, Sunil Sidher, Luca Teriaca, William T. Thompson, Peter R. Young
Publikováno v:
The Astrophysical Journal, 940 (1)
The Astrophysical Journal
The Astrophysical Journal
A key goal of the Solar Orbiter mission is to connect elemental abundance measurements of the solar wind enveloping the spacecraft with extreme-UV (EUV) spectroscopic observations of their solar sources, but this is not an easy exercise. Observations
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b988b018d9b5bd43c31f9f2737237208
https://hdl.handle.net/20.500.11850/586185
https://hdl.handle.net/20.500.11850/586185
Autor:
Nour Raouafi, Guillero Stenborg, Daniel Seaton, Haimin Wang, Jiasheng Wang, Craig DeForest, Stuart Bale, James Drake, Vadim Uritsky, Judy Karpen, C. Richard DeVore, Lakshmi Pradeep Chitta, Timothy Horbury, Louise Harra, Sofiane Bourouaine, Justin Kasper, Pankaj Kumar, Tai Phan, Alphonse Sterling, Marco Velli
Solar and stellar winds are ubiquitous flows of charged particles (i.e., electrons, protons, and heavier ions) permeating the astral spheres1. Through these winds, stars lose angular momentum, slow down their rotation as they age, shape planetary sys
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a059302c73d4ab2d0226c97fde919aac
https://doi.org/10.21203/rs.3.rs-2221227/v1
https://doi.org/10.21203/rs.3.rs-2221227/v1