Zobrazeno 1 - 10
of 46
pro vyhledávání: '"Bain, Hazel"'
Autor:
Moreland, Kimberly, Dayeh, Maher, Bain, Hazel M., Chatterjee, Subhamoy, Munoz-Jaramillo, Andres, Hart, Samuel
We introduce a new multivariate data set that utilizes multiple spacecraft collecting in-situ and remote sensing heliospheric measurements shown to be linked to physical processes responsible for generating solar energetic particles (SEPs). Using the
Externí odkaz:
http://arxiv.org/abs/2310.15390
Autor:
Chatterjee, Subhamoy, Dayeh, Maher, Muñoz-Jaramillo, Andrés, Bain, Hazel M., Moreland, Kimberly, Hart, Samuel
The Sun continuously affects the interplanetary environment through a host of interconnected and dynamic physical processes. Solar flares, Coronal Mass Ejections (CMEs), and Solar Energetic Particles (SEPs) are among the key drivers of space weather
Externí odkaz:
http://arxiv.org/abs/2309.14570
Autor:
Dayeh, Maher A., Chatterjee, Subhamoy, Munoz-Jaramillo, Andres, Moreland, Kimberly, Bain, Hazel M., Hart, Samuel
Solar Energetic Particles (SEPs) form a critical component of Space Weather. The complex, intertwined dynamics of SEP sources, acceleration, and transport make their forecasting very challenging. Yet, information about SEP arrival and their propertie
Externí odkaz:
http://arxiv.org/abs/2309.14503
Autor:
Guo, Jingnan, Wang, Bingbing, Whitman, Kathryn, Plainaki, Christina, Zhao, Lingling, Bain, Hazel M., Cohen, Christina, Dalla, Silvia, Dumbovic, Mateja, Janvier, Miho, Jun, Insoo, Luhmann, Janet, Malandraki, Olga E., Mays, M. Leila, Rankin, Jamie S., Wang, Linghua, Zheng, Yihua
Space weather is a multidisciplinary research area connecting scientists from across heliophysics domains seeking a coherent understanding of our space environment that can also serve modern life and society's needs. COSPAR's ISWAT (International Spa
Externí odkaz:
http://arxiv.org/abs/2308.11926
Autor:
Chatterjee, Subhamoy, Muñoz-Jaramillo, Andrés, Dayeh, Maher, Bain, Hazel M., Moreland, Kimberly
Extreme Ultraviolet images of the Sun are becoming an integral part of space weather prediction tasks. However, having different surveys requires the development of instrument-specific prediction algorithms. As an alternative, it is possible to combi
Externí odkaz:
http://arxiv.org/abs/2308.10322
Autor:
Guo, Jingnan, Wang, Bingbing, Whitman, Kathryn, Plainaki, Christina, Zhao, Lingling, Bain, Hazel M., Cohen, Christina, Dalla, Silvia, Dumbovic, Mateja, Janvier, Miho, Jun, Insoo, Luhmann, Janet, Malandraki, Olga E., Leila Mays, M., Rankin, Jamie S., Wang, Linghua, Zheng, Yihua
Publikováno v:
In Advances in Space Research March 2024
Autor:
Whitman, Kathryn, Egeland, Ricky, Richardson, Ian G., Allison, Clayton, Quinn, Philip, Barzilla, Janet, Kitiashvili, Irina, Sadykov, Viacheslav, Bain, Hazel M., Dierckxsens, Mark, Mays, M. Leila, Tadesse, Tilaye, Lee, Kerry T., Semones, Edward, Luhmann, Janet G., Núñez, Marlon, White, Stephen M., Kahler, Stephen W., Ling, Alan G., Smart, Don F., Shea, Margaret A., Tenishev, Valeriy, Boubrahimi, Soukaina F., Aydin, Berkay, Martens, Petrus, Angryk, Rafal, Marsh, Michael S., Dalla, Silvia, Crosby, Norma, Schwadron, Nathan A., Kozarev, Kamen, Gorby, Matthew, Young, Matthew A., Laurenza, Monica, Cliver, Edward W., Alberti, Tommaso, Stumpo, Mirko, Benella, Simone, Papaioannou, Athanasios, Anastasiadis, Anastasios, Sandberg, Ingmar, Georgoulis, Manolis K., Ji, Anli, Kempton, Dustin, Pandey, Chetraj, Li, Gang, Hu, Junxiang, Zank, Gary P., Lavasa, Eleni, Giannopoulos, Giorgos, Falconer, David, Kadadi, Yash, Fernandes, Ian, Dayeh, Maher A., Muñoz-Jaramillo, Andrés, Chatterjee, Subhamoy, Moreland, Kimberly D., Sokolov, Igor V., Roussev, Ilia I., Taktakishvili, Aleksandre, Effenberger, Frederic, Gombosi, Tamas, Huang, Zhenguang, Zhao, Lulu, Wijsen, Nicolas, Aran, Angels, Poedts, Stefaan, Kouloumvakos, Athanasios, Paassilta, Miikka, Vainio, Rami, Belov, Anatoly, Eroshenko, Eugenia A., Abunina, Maria A., Abunin, Artem A., Balch, Christopher C., Malandraki, Olga, Karavolos, Michalis, Heber, Bernd, Labrenz, Johannes, Kühl, Patrick, Kosovichev, Alexander G., Oria, Vincent, Nita, Gelu M., Illarionov, Egor, O’Keefe, Patrick M., Jiang, Yucheng, Fereira, Sheldon H., Ali, Aatiya, Paouris, Evangelos, Aminalragia-Giamini, Sigiava, Jiggens, Piers, Jin, Meng, Lee, Christina O., Palmerio, Erika, Bruno, Alessandro, Kasapis, Spiridon, Wang, Xiantong, Chen, Yang, Sanahuja, Blai, Lario, David, Jacobs, Carla, Strauss, Du Toit, Steyn, Ruhann, van den Berg, Jabus, Swalwell, Bill, Waterfall, Charlotte, Nedal, Mohamed, Miteva, Rositsa, Dechev, Momchil, Zucca, Pietro, Engell, Alec, Maze, Brianna, Farmer, Harold, Kerber, Thuha, Barnett, Ben, Loomis, Jeremy, Grey, Nathan, Thompson, Barbara J., Linker, Jon A., Caplan, Ronald M., Downs, Cooper, Török, Tibor, Lionello, Roberto, Titov, Viacheslav, Zhang, Ming, Hosseinzadeh, Pouya
Publikováno v:
In Advances in Space Research 15 December 2023 72(12):5161-5242
Autor:
Hughes, J. Marcus, Hsu, Vicki W., Seaton, Daniel B., Bain, Hazel M., Darnel, Jonathan M., Krista, Larisza
In order to utilize solar imagery for real-time feature identification and large-scale data science investigations of solar structures, we need maps of the Sun where phenomena, or themes, are labeled. Since solar imagers produce observations every fe
Externí odkaz:
http://arxiv.org/abs/1910.00144
Autor:
Bastian, Tim, Bain, Hazel, Chen, Bin, Gary, Dale, Fleishman, Gregory, Glesener, Lindsay, Saint-Hilaire, Pascal, Lonsdale, Colin, White, Stephen
The Sun is an active star that can have a direct impact on the Earth, its magnetosphere, and the technological infrastructure on which modern society depends. Among the phenomena that drive "space weather" are fast solar wind streams and co-rotating
Externí odkaz:
http://arxiv.org/abs/1904.05817
Autor:
Pillet, Valentin Martinez, Hill, Frank, Hammel, Heidi, de Wijn, Alfred G., Gosain, Sanjay, Burkepile, Joan, Henney, Carl J., McAteer, James R. T., Bain, Hazel M., Manchester IV, Ward B., Lin, Haosheng, Roth, Markus, Ichimoto, Kiyoshi, Suematsu, Yoshinori
Ground-based solar observations provide key contextual data (i.e., the 'big picture') to produce a complete description of the only astrosphere we can study in situ: our Sun's heliosphere. The next decade will see the beginning of operations of the D
Externí odkaz:
http://arxiv.org/abs/1903.06944