Zobrazeno 1 - 10
of 95
pro vyhledávání: '"A. Seripienlert"'
Autor:
Sonsrettee, Wirin, Chuychai, Piyanate, Seripienlert, Achara, Tooprakai, Paisan, Sáiz, Alejandro, Ruffolo, David, Matthaeus, William H., Chhiber, Rohit
Modeling of time profiles of solar energetic particle (SEP) observations often considers transport along a large-scale magnetic field with a fixed path length from the source to the observer. Here we point out that variability in the turbulent field
Externí odkaz:
http://arxiv.org/abs/2404.14718
Autor:
Poopakun, K., Nuntiyakul, W., Khamphakdee, S., Seripienlert, A., Ruffolo, D., Evenson, P., Jiang, P., Chuanraksasat, P., Munakata, K., Duldig, M. L., Humble, J. E., Madsen, J., Soonthornthum, B., Komonjinda, S.
The Galactic cosmic ray spectrum manifests pronounced variations over the 11-year sunspot cycle and more subtle variations over the 22-year solar magnetic cycle. An important tool to study these variations is repeated latitude surveys with neutron mo
Externí odkaz:
http://arxiv.org/abs/2310.14460
Autor:
Chhiber, R., Matthaeus, W. H., Cohen, C. M. S., Ruffolo, D., Sonsrettee, W., Tooprakai, P., Seripienlert, A., Chuychai, P., Usmanov, A. V., Goldstein, M. L., McComas, D. J., Leske, R. A., Christian, E. R., Mewaldt, R. A., Labrador, A. W., Szalay, J. R., Joyce, C. J., Giacalone, J., Schwadron, N. A., Mitchell, D. G., Hill, M. E., Wiedenbeck, M. E., McNutt Jr., R. L., Desai, M. I.
Publikováno v:
A&A 650, A26 (2021)
Context:In 2020 May-June, six solar energetic ion events were observed by the Parker Solar Probe/ISoIS instrument suite at 0.35 AU from the Sun. From standard velocity-dispersion analysis, the apparent ion path length is 0.625 AU at the onset of each
Externí odkaz:
http://arxiv.org/abs/2011.08329
Autor:
Wirin Sonsrettee, Piyanate Chuychai, Achara Seripienlert, Paisan Tooprakai, Alejandro Sáiz, David Ruffolo, William H. Matthaeus, Rohit Chhiber
Publikováno v:
The Astrophysical Journal, Vol 967, Iss 2, p 97 (2024)
Modeling of time profiles of solar energetic particle (SEP) observations often considers transport along a large-scale magnetic field with a fixed path length from the source to the observer. Here, we point out that variability in the turbulent field
Externí odkaz:
https://doaj.org/article/a0041c946c124a96a4dd19fcf3cbf2c2
Autor:
K. Poopakun, W. Nuntiyakul, S. Khamphakdee, A. Seripienlert, D. Ruffolo, P. Evenson, P. Jiang, P. Chuanraksasat, K. Munakata, M. L. Duldig, J. E. Humble, J. Madsen, B. Soonthornthum, S. Komonjinda
Publikováno v:
The Astrophysical Journal, Vol 958, Iss 1, p 80 (2023)
The Galactic cosmic-ray spectrum manifests pronounced variations over the 11 yr sunspot cycle and more subtle variations over the 22 yr solar magnetic cycle. An important tool to study these variations is repeated latitude surveys with neutron monito
Externí odkaz:
https://doaj.org/article/f5e15617a9be4f3ebe33e532f17e21ca
Akademický článek
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Autor:
Maburee, J, Mitthumsiri, W, Nuntiyakul, W, Pattarakijwanich, P, Ruffolo, D, Sáiz, A, Seripienlert, A
Publikováno v:
Journal of Physics: Conference Series; Nov2023, Vol. 2653 Issue 1, p1-7, 7p
Publikováno v:
Journal of Physics: Conference Series; Nov2023, Vol. 2653 Issue 1, p1-8, 8p
Autor:
Yakum, P, Khamphakdee, S, Nuntiyakul, W, Sáiz, A, Ruffolo, D, Evenson, P, Bangliang, C, Seripienlert, A, Jiang, P, Chuanraksasat, P, Munakata, K, Madsen, J, Soonthornthum, B, Komonjinda, S
Publikováno v:
Journal of Physics: Conference Series; Nov2023, Vol. 2653 Issue 1, p1-6, 6p
Autor:
Duangjai, B, Nuntiyakul, W, Seripienlert, A, Pagwhan, A, Chaiwongkhot, K, Sáiz, A, Ruffolo, D, Evenson, P
Publikováno v:
Journal of Physics: Conference Series; Nov2023, Vol. 2653 Issue 1, p1-7, 7p