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Kai, Keizo, Kosugi, Takeo, Nakajima, Hiroshi (1982) Differences of observed characteristics between impulsive bursts and post-burst increases. Solar Physics, 75 (1). 331-339 doi:10.1007/bf00153480

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Reference TypeJournal (article/letter/editorial)
TitleDifferences of observed characteristics between impulsive bursts and post-burst increases
JournalSolar Physics
AuthorsKai, KeizoAuthor
Kosugi, TakeoAuthor
Nakajima, HiroshiAuthor
Year1982 (January)Volume75
Issue1
PublisherSpringer Science and Business Media LLC
DOIdoi:10.1007/bf00153480Search in ResearchGate
Generate Citation Formats
Mindat Ref. ID8917166Long-form Identifiermindat:1:5:8917166:2
GUID0
Full ReferenceKai, Keizo, Kosugi, Takeo, Nakajima, Hiroshi (1982) Differences of observed characteristics between impulsive bursts and post-burst increases. Solar Physics, 75 (1). 331-339 doi:10.1007/bf00153480
Plain TextKai, Keizo, Kosugi, Takeo, Nakajima, Hiroshi (1982) Differences of observed characteristics between impulsive bursts and post-burst increases. Solar Physics, 75 (1). 331-339 doi:10.1007/bf00153480
In(1982, January) Solar Physics Vol. 75 (1) Springer Science and Business Media LLC

See Also

These are possibly similar items as determined by title/reference text matching only.

Kosugi, Takeo, Kai, Keizo, Suzuki, Takashi (1983) Source characteristics of main and post-burst-increase phases of solar bursts at 17 GHz. Solar Physics, 87 (2). doi:10.1007/bf00224847
Kosugi, Takeo (1981) Radio and X-ray observations of a multiple impulsive solar burst with high time resolution. Solar Physics, 71 (1). 91-105 doi:10.1007/bf00153609
Kosugi, Takeo (1982) A long-enduring multi-source burst at 17 GHz and its relation to a type IVm-dm burst with spectral fine features. Solar Physics, 75 (1). 293-304 doi:10.1007/bf00153478
Kai, K., Kosugi, T., Nakajima, H. (1982) Source structure of gradual rise and fall bursts at 17 GHz. Solar Physics, 78 (2). 243-252 doi:10.1007/bf00151607
Kosugi, Takeo, Dennis, Brian R., Kai, Keizo (1988) Energetic electrons in impulsive and extended solar flares as deduced from flux correlations between hard X-rays and microwaves. The Astrophysical Journal, 324. 1118pp. doi:10.1086/165967
Kosugi, Takeo, Tsuneta, Saku (1983) Time variations of hard X-ray bursts observed with the Solar X-ray Telescope aboard Hinotori (with a movie). Solar Physics, 86 (1). 333-338 doi:10.1007/bf00157206
Kosugi, Takeo (1976) Type II?IV radio bursts and compact and diffuse white-light clouds in the outer corona of December 14, 1971. Solar Physics, 48 (2). 339-356 doi:10.1007/bf00152000
Kaufmann, Pierre (1969) Unpolarized impulsive solar bursts observed at 7 GHz. Solar Physics, 9 (1). 166-172 doi:10.1007/bf00145737
Nishio, Masanori, Yaji, Kentaro, Kosugi, Takeo, Nakajima, Hiroshi, Sakurai, Takashi (1997) Magnetic Field Configuration in Impulsive Solar Flares Inferred from Coaligned Microwave/X‐Ray Images. The Astrophysical Journal, 489 (2). 976-991 doi:10.1086/304793
Kai, Keizo (1978) Relation between circular polarization of moving type IV bursts and polarity of photospheric magnetic fields. Solar Physics, 56 (2). doi:10.1007/bf00152481
Kosugi, Takeo (1987) Solar flares observed in microwaves: Recent results from solar radio groups in Japan. Solar Physics, 113 (1). 327-332 doi:10.1007/bf00147719
 
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