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Analysis of Type II and Type III Radio Bursts Associated with SEPs from Non-Interacting/Interacting Radio-Loud CMEs
DOI: 10.1007/s10511-021-09693-0 Bibcode: 2021Ap.....64..327K

Feng, Li; Prakash, O.; Shanmugaraju, A. +4 more

We analyze radio bursts observed in events with interacting/non-interacting CMEs that produced major SEPs (Ip > 10 MeV) from April 1997 to December 2014. We compare properties of meter (m), decahectometer (DH) type II and DH type III bursts, and time lags for interacting-CME-associated (IC) events and non-interacting-CME-associated (…

2021 Astrophysics
SOHO 4
Interrelationships between Halo-Type Coronal Mass Ejections and Solar Flares Based on Observations in the 23rd and 24th Cycles
DOI: 10.1007/s10511-021-09668-1 Bibcode: 2021Ap.....64...61B

Bruevich, E. A.; Burov, V. A.; Arakelov, A. S. +1 more

Solar activity of an explosive character during the 23rd and 24th cycles is analyzed. X-ray observations from the GOES-15 satellite during flares and observations during coronal mass ejections (CME) with the SOHO/LASCO coronagraph are used. The delay intervals between the onset of a flare and the onset of a Halo-type CME associated the same active…

2021 Astrophysics
SOHO 0
Fluctuations in the Intensity of Radiation Emerging from a Multicomponent Stochastic Atmosphere. II
DOI: 10.1007/s10511-005-0024-5 Bibcode: 2005Ap.....48..253N

Nikoghossian, A. G.; Aboudarham, J.; Mouradian, Z.

This part of a series of papers examines the more general problem in which it is assumed that the fluctuations in the intensity of radiation emerging from a medium are caused by random variations in both the optical thickness of the structural elements and the power of the energy sources contained in them. The frequency dependence of the relative …

2005 Astrophysics
SOHO 0