Zobrazeno 1 - 3
of 3
pro vyhledávání: '"Sakanoi, T. (T.)"'
Autor:
Miyoshi, Y. (Y.), Saito, S. (S.), Kurita, S. (S.), Asamura, K. (K.), Hosokawa, K. (K.), Sakanoi, T. (T.), Mitani, T. (T.), Ogawa, Y. (Y.), Oyama, S. (S.), Tsuchiya, F. (F.), Jones, S. L. (S. L.), Jaynes, A. N. (A. N.), Blake, J. B. (J. B.)
Publikováno v:
Geophysical Research Letters. 47(21)
In this study, by simulating the wave‐particle interactions, we show that subrelativistic/relativistic electron microbursts form the high‐energy tail of pulsating aurora (PsA). Whistler‐mode chorus waves that propagate along the magnetic field
Autor:
Fukizawa, M. (M.), Sakanoi, T. (T.), Miyoshi, Y. (Y.), Hosokawa, K. (K.), Shiokawa, K. (K.), Katoh, Y. (Y.), Kazama, Y. (Y.), Kumamoto, A. (A.), Tsuchiya, F. (F.), Miyashita, Y. (Y.), Tanaka, Y. -. (Y. -M.), Kasahara, Y. (Y.), Ozaki, M. (M.), Matsuoka, A. (A.), Matsuda, S. (S.), Hikishima, M. (M.), Oyama, S. (S.), Ogawa, Y. (Y.), Kurita, S. (S.), Fujii, R. (R.)
Pulsating auroras (PsAs) are thought to be generated by precipitating electrons scattered by lower‐band chorus (LBC) waves near the magnetic equator. One‐to‐one correlation between the LBC intensity and the PsA intensity has been reported. Elec
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______2423::6b16a2c832543e2e96522c05a7d21f57
http://urn.fi/urn:nbn:fi-fe201903128683
http://urn.fi/urn:nbn:fi-fe201903128683
Autor:
Shiokawa, K. (K.), Ozaki, M. (M.), Kadokura, A. (A.), Endo, Y. (Y.), Sakanoi, T. (T.), Kurita, S. (S.), Miyoshi, Y. (Y.), Oyama, S. -. (S. -I.), Connors, M. (M.), Schofield, I. (I.), Ruohoniemi, J. M. (J. M.), Nose, M. (M.), Nagatsuma, T. (T.), Sakaguchi, K. (K.), Baishev, D. G. (D. G.), Pashinin, A. (A.), Rakhmatulin, R. (R.), Shevtsov, B. (B.), Poddelsky, I. (I.), Engebretson, M. (M.), Raita, T. (Tero), Tanaka, Y. -. (Y. -M.), Shinohara, M. (M.), Teramoto, M. (M.), Nomura, R. (R.), Fujimoto, A. (A.), Matsuoka, A. (A.), Higashio, N. (N.), Takashima, T. (T.), Shinohara, I. (I.), Albert, J. M. (Jay M.)
Publikováno v:
Geophysical Research Letters. 45(20):10-10,828
This paper reports two unique auroral features: postmidnight purple auroral rays and global Pc1 geomagnetic pulsations, observed before the onset of the corotating interaction region (CIR) storm of 21 March 2017, at the beginning of the first campaig