Zobrazeno 1 - 10
of 5 303
pro vyhledávání: '"Yashiro S"'
Intense geomagnetic storms are characterized by a minimum value of the Dst index at or below -100 nT. It is well known that these storms are caused by the southward magnetic fields in coronal mass ejections (CMEs) and corotating interaction regions (
Externí odkaz:
http://arxiv.org/abs/2401.03524
The sustained gamma-ray emission (SGRE) from the Sun is a prolonged enhancement of >100 MeV gamma-ray emission that extends beyond the flare impulsive phase.The origin of the >300 MeV protons resulting in SGRE is debated, both flares and shocks drive
Externí odkaz:
http://arxiv.org/abs/2307.05585
Autor:
Gopalswamy, N., Christe, S., Fung, S. F., Gong, Q., Gruesbeck, J. R., Jian, L. K., Kanekal, S. G., Kay, C., Kucera, T. A., Leake, J. E., Li, L., Makela, P., Nikulla, P., Reginald, N. L., Shih, A., Tadikonda, S. K., Viall, N., Wilson III, L. B., Yashiro, S., Golub, L., DeLuca, E., Reeves, K., Sterling, A. C., Winebarger, A. R., DeForest, C., Hassler, D. M., Seaton, D. B., Desai, M. I., Mokashi, P. S., Lazio, J., Jensen, E. A., Manchester, W. B., Sachdeva, N., Wood, B., Kooi, J., Hess, P., Wexler, D. B., Bale, S. D., Krucker, S., Hurlburt, N., DeRosa, M., Gosain, S., Jain, K., Kholikov, S., Petrie, G. J. D., Pevtsov, A., Tripathy, S. C., Zhao, J., Scherrer, P. H., Rajaguru, S. P., Woods, T., Kenney, M., Zhang, J., Scolini, C., Cho, K. S., Park, Y. D., Jackson, B. V.
We report on a study of the Multiview Observatory for Solar Terrestrial Science (MOST) mission that will provide comprehensive imagery and time series data needed to understand the magnetic connection between the solar interior and the solar atmosphe
Externí odkaz:
http://arxiv.org/abs/2303.02895
We report on the solar and interplanetary (IP) causes of the third largest geomagnetic storm (2018 August 26) in solar cycle 24. The underlying coronal mass ejection (CME) originating from a quiescent filament region becomes a 440 km/s magnetic cloud
Externí odkaz:
http://arxiv.org/abs/2207.11630
We report on the 2015 June 25 sustained gamma-ray emission (SGRE) event associated with a halo coronal mass ejection and a type II radio burst in the decameter-hectometric (DH) wavelengths. The duration and ending frequency of the type II burst are l
Externí odkaz:
http://arxiv.org/abs/2105.01212
We report on the first detection of nonthermal radio emission associated with a polar coronal mass ejection. We call the radio emission as diffuse interplanetary radio emission (DIRE), which occurs in the decameter-hectometric wavelengths. The radio
Externí odkaz:
http://arxiv.org/abs/2105.01216
We report that the number of > 500 MeV protons (Ng) inferred from sustained gamma ray emission (SGRE) from the Sun is significantly correlated with that of protons propagating into space (NSEP) as solar energetic particles (SEPs). Under the shock par
Externí odkaz:
http://arxiv.org/abs/2105.01206
Autor:
Gopalswamy, N., Christe, S., Fung, S.F., Gong, Q., Gruesbeck, J.R., Jian, L.K., Kanekal, S.G., Kay, C., Kucera, T.A., Leake, J.E., Li, L., Mӓkelӓ, P., Nikulla, P., Reginald, N.L., Shih, A., Tadikonda, S.K., Viall, N., Wilson, L.B., III, Yashiro, S., Golub, L., DeLuca, E., Reeves, K., Sterling, A.C., Winebarger, A.R., DeForest, C., Hassler, D.M., Seaton, D.B., Desai, M.I., Mokashi, P.S., Lazio, J., Jensen, E.A., Manchester, W.B., Sachdeva, N., Wood, B., Kooi, J., Hess, P., Wexler, D.B., Bale, S.D., Krucker, S., Hurlburt, N., DeRosa, M., Gosain, S., Jain, K., Kholikov, S., Petrie, G.J.D., Pevtsov, A., Tripathy, S.C., Zhao, J., Scherrer, P.H., Rajaguru, S.P., Woods, T., Kenney, M., Zhang, J., Scolini, C., Cho, K.-S., Park, Y.-D., Jackson, B.V.
Publikováno v:
In Journal of Atmospheric and Solar-Terrestrial Physics January 2024 254
Autor:
Gopalswamy, N., Newmark, J., Yashiro, S., Mäkelä, P., Reginald, N., Thakur, N., Gong, Q., Kim, Y-H., Cho, K-S., Choi, S-H., Baek, J-H., Bong, S-C., Yang, H-S., Park, J-Y., Kim, J-H., Park, Y-D., Lee, J. -O., Kim, R. -S., Lim, E. -K.
We report on the Balloonborne Investigation of Temperature and Speed of Electrons in the corona (BITSE) mission launched recently to observe the solar corona from about 3 Rs to 15 Rs at four wavelengths (393.5, 405.0, 398.7, and 423.4 nm). The BITSE
Externí odkaz:
http://arxiv.org/abs/2011.06111
Solar cycle (SC) 24 has come to an end by the end of 2019, providing information on two full cycles to understand the manifestations of SC 24, the smallest cycle in the Space Age that has resulted in a weak heliospheric state indicated by the reduced
Externí odkaz:
http://arxiv.org/abs/2007.08291