Zobrazeno 1 - 10
of 14
pro vyhledávání: '"Allred, Joel"'
Autor:
Tristan, Isaiah I., Notsu, Yuta, Kowalski, Adam F., Brown, Alexander, Vrijmoet, Eliot H., Allred, Joel C., Carter, Brad D., Grady, Carol A., Henry, Todd J., Hinojosa, Rodrigo H., Jao, Wei-Chun, Lomax, Jamie R., Neff, James E., Osten, Rachel A., Paredes, Leonardo A., Schneider, Glenn H., Soutter, Jack, White, Graeme L., Wisniewski, John P.
M dwarfs are considered one of the most likely places to find extraterrestrial life in part due to their large numbers in the nearby solar neighborhood. However, they have much more intense flaring events than stars like our Sun, which could negative
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9ffcdc969caefaede3ad3e30cb09856c
Autor:
Kerr, Graham S., Xu, Yan, Allred, Joel C., Polito, Vanessa, Sadykov, Viacheslav M., Huang, Nengyi, Wang, Haimin
While solar flares are predominantly characterised by an intense broadband enhancement to the solar radiative output, certain spectral lines and continua will, in theory, exhibit flare-induced dimmings. Observations of transitions of orthohelium He I
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::2dd11eacfd4b2442a86c3edab9a33e92
Autor:
Kerr, Graham S., Alaoui, Meriem, Allred, Joel C., Bian, Nicholas H., Dennis, Brian R., Emslie, A. Gordon, Fletcher, Lyndsay, Guidoni, Silvina, Hayes, Laura A., Holman, Gordon D., Hudson, Hugh S., Karpen, Judith T., Kowalski, Adam F., Milligan, Ryan O., Polito, Vanessa, Qiu, Jiong, Ryan, Daniel F.
Solar flares are a fundamental component of solar eruptive events (SEEs; along with solar energetic particles, SEPs, and coronal mass ejections, CMEs). Flares are the first component of the SEE to impact our atmosphere, which can set the stage for th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2c63a0e9e1a217c44006559a57611686
Solar Flare Energy Partitioning and Transport -- the Gradual Phase (a Heliophysics 2050 White Paper)
Autor:
Kerr, Graham S., Alaoui, Meriem, Allred, Joel C., Bian, Nicholas H., Dennis, Brian R., Emslie, A. Gordon, Fletcher, Lyndsay, Guidoni, Silvina, Hayes, Laura A., Holman, Gordon D., Hudson, Hugh S., Karpen, Judith T., Kowalski, Adam F., Milligan, Ryan O., Polito, Vanessa, Qiu, Jiong, Ryan, Daniel F.
Solar flares are a fundamental component of solar eruptive events (SEEs; along with solar energetic particles, SEPs, and coronal mass ejections, CMEs). Flares are the first component of the SEE to impact our atmosphere, which can set the stage for th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d6fd659774e59f7584c3da40362441df
Autor:
Youngblood, Allison, Drake, Jeremy, Mason, James, Osten, Rachel, Jin, Meng, Kowalski, Adam, France, Kevin, Fleming, Brian, Allred, Joel, Amerstorfer, Ute, Berta-Thompson, Zachory, Bourrier, Vincent, Fossati, Luca, Froning, Cynthia, Garraffo, Cecilia, Gronoff, Guillaume, Koskinen, Tommi, Lichtenegger, Herbert
The EUV (100-912 {\AA}) is a spectral region notoriously difficult to observe due to attenuation by neutral hydrogen gas in the interstellar medium. Despite this, hundreds to thousands of nearby stars of different spectral types and magnetic activity
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bb846569cdafbcb3e16c63b2ab662e41
Autor:
Youngblood, Allison, France, Kevin, Koskinen, Tommi, Fossati, Luca, Amerstorfer, Ute, Lichtenegger, Herbert, Drake, Jeremy, Mason, James, Fleming, Brian, Allred, Joel, Berta-Thompson, Zachory, Bourrier, Vincent, Froning, Cynthia, Garraffo, Cecilia, Gronoff, Guillaume, Jin, Meng, Kowalski, Adam, Osten, Rachel
The planetary effective surface temperature alone is insufficient to characterize exoplanet atmospheres and their stability or evolution. Considering the star-planet system as a whole is necessary, and a critical component of the system is the photoi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c6f3814da4bddabf6293871aceba3461
Autor:
Procházka, Ondřej, Reid, Aaron, Milligan, Ryan O., Simões, Paulo J.A., Allred, Joel C., Mathioudakis, Mihalis
Publikováno v:
Reid, A, Milligan, R O, Procházka, O, Simoes, P J A, Allred, J C & Mathioudakis, M 2018, ' Reproducing Type II White-Light Solar Flare Observations with Electron and Proton Beam Simulations ', The Astrophysical Journal, vol. 862, no. 76, 76 . https://doi.org/10.3847/1538-4357/aaca37
We investigate the cause of the suppressed Balmer series and the origin of the white-light continuum emission in the X1.0 class solar flare on 2014 June 11. We use radiative hydrodynamic simulations to model the response of the flaring atmosphere to
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::728a5aa90cbbeb9d08f5c1490843f947
https://pure.qub.ac.uk/en/publications/reproducing-type-ii-whitelight-solar-flare-observations-with-electron-and-proton-beam-simulations(05f5f529-bb71-48b9-8fcb-6a53deeba811).html
https://pure.qub.ac.uk/en/publications/reproducing-type-ii-whitelight-solar-flare-observations-with-electron-and-proton-beam-simulations(05f5f529-bb71-48b9-8fcb-6a53deeba811).html
The Extreme Ultraviolet Normal Incidence Spectrograph (EUNIS) and the Hinode/ EUV Imaging Spectrometer (EIS) observed AR 11726 on 2013 April 23. We present intensity images in numerous atomic lines constructed from these observations. These lines are
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8a908f5f5b98b9605bce34f109e79e5f
Autor:
Christe, Steven, Krucker, Samuel, Glesener, Lindsay, Shih, Albert, Saint-Hilaire, Pascal, Caspi, Amir, Allred, Joel, Battaglia, Marina, Chen, Bin, Drake, James, Dennis, Brian, Gary, Dale, Gburek, Szymon, Goetz, Keith, Grefenstette, Brian, Gubarev, Mikhail, Hannah, Iain, Holman, Gordon, Hudson, Hugh, Inglis, Andrew, Ireland, Jack, Ishikawa, Shinosuke, Klimchuk, James, Kontar, Eduard, Kowalski, Adam, Longcope, Dana, Massone, Anna-Maria, Musset, Sophie, Piana, Michele, Ramsey, Brian, Ryan, Daniel, Schwartz, Richard, St����licki, Marek, Turin, Paul, Warmuth, Alexander, Wilson-Hodge, Colleen, White, Stephen, Veronig, Astrid, Vilmer, Nicole, Woods, Tom
How impulsive magnetic energy release leads to solar eruptions and how those eruptions are energized and evolve are vital unsolved problems in Heliophysics. The standard model for solar eruptions summarizes our current understanding of these events.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::caae90603ba29a68faeaf4f9cba4cef5
http://arxiv.org/abs/1701.00792
http://arxiv.org/abs/1701.00792
Autor:
Christe, Steven, Bandler, Simon, DeLuca, Edward, Caspi, Amir, Golub, Leon, Smith, Randall, Allred, Joel, Brosius, Jeffrey W., Dennis, Brian, Klimchuk, James
Even in the absence of resolved flares, the corona is heated to several million degrees. However, despite its importance for the structure, dynamics, and evolution of the solar atmosphere, the origin of this heating remains poorly understood. Several
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::008b2c66573972bd15a76d59b140bcff