Zobrazeno 1 - 10
of 244
pro vyhledávání: '"GLESENER, Lindsay"'
Autor:
Chen, Bin, Kong, Xiangliang, Yu, Sijie, Shen, Chengcai, Li, Xiaocan, Guo, Fan, Zhang, Yixian, Glesener, Lindsay, Krucker, Säm
Where and how flares efficiently accelerate charged particles remains an unresolved question. Recent studies revealed that a "magnetic bottle" structure, which forms near the bottom of a large-scale reconnection current sheet above the flare arcade,
Externí odkaz:
http://arxiv.org/abs/2406.00109
Autor:
Christe, Steven, Glesener, Lindsay, Buitrago-Casas, Camilo, Ishikawa, Shin-Nosuke, Ramsey, Brian, Gubarev, Mikhail, Kilaru, Kiranmayee, Kolodziejczak, Jeffery J., Watanabe, Shin, Takahashi, Tadayuki, Tajima, Hiroyasu, Turin, Paul, Shourt, Van, Foster, Natalie, Krucker, Sam
Publikováno v:
Journal of Astronomical Instrumentation, 2016, Volume 05, Number 01, 1640005
The Focusing Optics X-ray Solar Imager (FOXSI) sounding rocket payload flew for the second time on 2014 December 11. To enable direct Hard X-Ray (HXR) imaging spectroscopy, FOXSI makes use of grazing-incidence replicated focusing optics combined with
Externí odkaz:
http://arxiv.org/abs/2403.07610
When and where the magnetic field energy is released and converted in eruptive solar flares remains an outstanding topic in solar physics. To shed light on this question, here we report multi-wavelength observations of a C9.4-class eruptive limb flar
Externí odkaz:
http://arxiv.org/abs/2403.00985
Microflares are energetically smaller versions of solar flares, demonstrating the same processes of plasma heating and particle acceleration. However, it remains unclear down to what energy scales this impulsive energy release continues, which has im
Externí odkaz:
http://arxiv.org/abs/2402.05426
Autor:
Duncan, Jessie, Masek, Reed B., Shih, Albert Y., Glesener, Lindsay, Barnes, Will, Reeves, Katharine K., Zhang, Yixian, Hannah, Iain G., Grefenstette, Brian W.
Solar active regions contain a broad range of temperatures, with the thermal plasma distribution often observed to peak in the few millions of kelvin. Differential emission measure (DEM) analysis can allow instruments with diverse temperature respons
Externí odkaz:
http://arxiv.org/abs/2312.05109
Autor:
Allred, Joel C., Kerr, Graham S., Alaoui, Meriem, Buitrago-Casas, Juan Camilo, Caspi, Amir, Chen, Bin, Chen, Thomas Y., Glesener, Lindsay, Guidoni, Silvina E., Guo, Fan, Karpen, Judith T., Musset, Sophie, Reeves, Katharine K., Shih, Albert Y.
Publikováno v:
Bulletin of the AAS, Vol. 55, Issue 3, Whitepaper #010 (10pp); 2023 July 31
Solar flares and coronal mass ejections are interrelated phenomena that together are known as solar eruptive events. These are the main drivers of space weather and understanding their origins is a primary goal of Heliophysics. In this white paper, w
Externí odkaz:
http://arxiv.org/abs/2307.14946
Autor:
Christe, Steven, Alaoui, Meriem, Allred, Joel, Battaglia, Marina, Baumgartner, Wayne, Buitrago-Casas, Juan Camilo, Caspi, Amir, Chen, Bin, Chen, Thomas, Dennis, Brian, Drake, James, Glesener, Lindsay, Hannah, Iain, Hayes, Laura A., Hudson, Hugh, Inglis, Andrew, Ireland, Jack, Klimchuk, James, Kowalski, Adam, Krucker, Säm, Massone, Anna Maria, Musset, Sophie, Piana, Michele, Ryan, Daniel, Shih, Albert Y., Veronig, Astrid, Vilmer, Nicole, Warmuth, Alexander, White, Stephen
Publikováno v:
Bulletin of the AAS, Vol. 55, Issue 3, Whitepaper #065 (13pp); 2023 July 31
FOXSI is a direct-imaging, hard X-ray (HXR) telescope optimized for solar flare observations. It detects hot plasma and energetic electrons in and near energy release sites in the solar corona via bremsstrahlung emission, measuring both spatial struc
Externí odkaz:
http://arxiv.org/abs/2306.15071
Autor:
Shih, Albert Y., Glesener, Lindsay, Krucker, Säm, Guidoni, Silvina, Christe, Steven, Reeves, Katharine K., Gburek, Szymon, Caspi, Amir, Alaoui, Meriem, Allred, Joel, Battaglia, Marina, Baumgartner, Wayne, Dennis, Brian, Drake, James, Goetz, Keith, Golub, Leon, Hannah, Iain, Hayes, Laura, Holman, Gordon, Inglis, Andrew, Ireland, Jack, Kerr, Graham, Klimchuk, James, McKenzie, David, Moore, Christopher S., Musset, Sophie, Reep, Jeffrey, Ryan, Daniel, Saint-Hilaire, Pascal, Savage, Sabrina, Seaton, Daniel B., Stęślicki, Marek, Woods, Thomas N.
Publikováno v:
Bulletin of the AAS, Vol. 55, Issue 3, Whitepaper #364 (5pp); 2023 July 31
It is essential that there be coordinated and co-optimized observations in X-rays, gamma-rays, and EUV during the peak of solar cycle 26 (~2036) to significantly advance our understanding of impulsive energy release in the corona. The open questions
Externí odkaz:
http://arxiv.org/abs/2306.11777
Autor:
Shih, Albert Y., Caspi, Amir, Duncan, Jessie, Glesener, Lindsay, Guidoni, Silvina E., Reeves, Katharine K.
Publikováno v:
Bulletin of the AAS, Vol. 55, Issue 3, Whitepaper #363 (4pp); 2023 July 31
Research efforts that require observations of high solar activity, such as multiwavelength studies of large solar flares and CMEs, must contend with the 11-year solar cycle to a degree unparalleled by other segments of heliophysics. While the "fallow
Externí odkaz:
http://arxiv.org/abs/2306.11776
Autor:
Glesener, Lindsay, Shih, Albert Y., Caspi, Amir, Milligan, Ryan, Hudson, Hugh, Oka, Mitsuo, Buitrago-Casas, Juan Camilo, Guo, Fan, Ryan, Dan, Kontar, Eduard, Veronig, Astrid, Hayes, Laura A., Inglis, Andrew, Golub, Leon, Vilmer, Nicole, Gary, Dale, Reid, Hamish, Hannah, Iain, Kerr, Graham S., Reeves, Katharine K., Allred, Joel, Guidoni, Silvina, Yu, Sijie, Christe, Steven, Musset, Sophie, Dennis, Brian, Oliveros, Juan Carlos Martínez, Athiray, P. S., Vievering, Juliana, White, Stephen, Winebarger, Amy, Drake, James, Jeffrey, Natasha, Antiochos, Spiro, Duncan, Jessie, Zhang, Yixian, Alaoui, Meriem, Simões, Paulo J. A., Battaglia, Marina, Setterberg, William, Masek, Reed, Chen, Thomas Y., Peterson, Marianne, Krucker, Säm, Temmer, Manuela, Saint-Hilaire, Pascal, Petrosian, Vahe, Knuth, Trevor, Moore, Christopher S.
Publikováno v:
Bulletin of the AAS, Vol. 55, Issue 3, Whitepaper #129 (14pp); 2023 July 31
Understanding the nature of energetic particles in the solar atmosphere is one of the most important outstanding problems in heliophysics. Flare-accelerated particles compose a huge fraction of the flare energy budget; they have large influences on h
Externí odkaz:
http://arxiv.org/abs/2306.05447