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Pappa Kalaivani, P., Umapathy, S., Shanmugaraju, A., Prakash, O. (2010) Characteristics of coronal mass ejection associated with DH type II radio bursts (All and Limb events). Astrophysics and Space Science, 330 (2). 237-242 doi:10.1007/s10509-010-0405-z

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Reference TypeJournal (article/letter/editorial)
TitleCharacteristics of coronal mass ejection associated with DH type II radio bursts (All and Limb events)
JournalAstrophysics and Space Science
AuthorsPappa Kalaivani, P.Author
Umapathy, S.Author
Shanmugaraju, A.Author
Prakash, O.Author
Year2010 (December)Volume330
Issue2
PublisherSpringer Science and Business Media LLC
DOIdoi:10.1007/s10509-010-0405-zSearch in ResearchGate
Generate Citation Formats
Mindat Ref. ID3534189Long-form Identifiermindat:1:5:3534189:7
GUID0
Full ReferencePappa Kalaivani, P., Umapathy, S., Shanmugaraju, A., Prakash, O. (2010) Characteristics of coronal mass ejection associated with DH type II radio bursts (All and Limb events). Astrophysics and Space Science, 330 (2). 237-242 doi:10.1007/s10509-010-0405-z
Plain TextPappa Kalaivani, P., Umapathy, S., Shanmugaraju, A., Prakash, O. (2010) Characteristics of coronal mass ejection associated with DH type II radio bursts (All and Limb events). Astrophysics and Space Science, 330 (2). 237-242 doi:10.1007/s10509-010-0405-z
In(2010, December) Astrophysics and Space Science Vol. 330 (2) Springer Science and Business Media LLC

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Prakash, O., Umapathy, S., Shanmugaraju, A., Pappa kalaivani, P., Vršnak, Bojan (2012) Characteristics of DH type II bursts, CMEs and flares with respect to the acceleration of CMEs. Astrophysics and Space Science, 337 (1). 47-64 doi:10.1007/s10509-011-0817-4
Prakash, O., Feng, Li, Michalek, G., Gan, Weiqun, Lu, Lei, Shanmugaraju, A., Umapathy, S. (2017) Characteristics of events with metric-to-decahectometric type II radio bursts associated with CMEs and flares in relation to SEP events. Astrophysics and Space Science, 362 (3). doi:10.1007/s10509-017-3034-y
Prakash, O., Umapathy, S., Shanmugaraju, A., Pappa kalaivani, P., Vršnak, Bojan (2010) Type-II Bursts in Meter and Deca – Hectometer Wavelengths and Their Relation to Flares and CMEs: II. Solar Physics, 266 (1). 135-147 doi:10.1007/s11207-010-9604-6
Prakash, O., Umapathy, S., Shanmugaraju, A. (2012) Distinctions between the characteristics of before and after DH CMEs associated flares. Astrophysics and Space Science, 340 (1). 1-8 doi:10.1007/s10509-012-1034-5
Kalaivani, P. Pappa, Shanmugaraju, A., Prakash, O., Kim, R.-S. (2020) Statistical Characteristics on SEPs, Radio-Loud CMEs, Low Frequency Type II and Type III Radio Bursts Associated with Impulsive and Gradual Flares. Earth, Moon, and Planets, 123 (3) 61-85 doi:10.1007/s11038-020-09533-9
Lakshmi, M. Anna, Umapathy, S. (2012) Characteristics of CMEs associated with solar flares and DH type II radio bursts based on source position. Astrophysics and Space Science, 338 (2). 227-231 doi:10.1007/s10509-011-0949-6
Prasanna Subramanian, S., Shanmugaraju, A. (2013) Study of interacting CMEs and DH type II radio bursts. Astrophysics and Space Science, 344 (2). 305-312 doi:10.1007/s10509-012-1347-4
Pappa Kalaivani, P., Prakash, O., Shanmugaraju, A., Michalek, G., Selvarani, G. (2022) Kinematic Study of Radio-Loud CMEs Associated with Solar Flares and DH Type-II Radio Emissions During Solar Cycles 23 and 24. Solar Physics, 297 (5) doi:10.1007/s11207-022-01985-8
Shanmugaraju, A., Suresh, K., Vasanth, V., Selvarani, G., Umapathy, S. (2018) Interplanetary type II radio bursts and their association with CMEs and flares. Astrophysics and Space Science, 363 (6). doi:10.1007/s10509-018-3345-7
Prakash, O., Vijayalakshmi, P., Shanmugaraju, A., Pappa Kalaivani, P., Ravishankar, A., Moon, Y.-J., Park, J. (2023) Solar source longitudinal dependence of SEPs and their association with solar flares and radio-loud CMEs. Astrophysics and Space Science, 368 (10) doi:10.1007/s10509-023-04238-7
Vasanth, V., Umapathy, S. (2013) A Statistical Study on CMEs Associated with DH-Type-II Radio Bursts Based on Their Source Location (Limb and Disk Events). Solar Physics, 282 (1). 239-247 doi:10.1007/s11207-012-0126-2
 
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