1998
DOI: 10.1023/a:1005075003370
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Cited by 107 publications
(61 citation statements)
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“…They concluded based on a coronal density measurement that the type II bursts might be generated at the interface of the CME flank and the streamer. Ramesh et al (2010) inspected the seven near-limb type II burst obtained by the Gauribidanur radioheliograph (GRH, Ramesh et al 1998Ramesh et al ) between 1997Ramesh et al and 2005 and reported that the type II associated CMEs are largely accelerated before the type II bursts start. They noted that the present spatial resolution of the GRH is insufficient to precisely locate the type II bursts in low corona.…”
Section: Introductionmentioning
confidence: 99%
“…They concluded based on a coronal density measurement that the type II bursts might be generated at the interface of the CME flank and the streamer. Ramesh et al (2010) inspected the seven near-limb type II burst obtained by the Gauribidanur radioheliograph (GRH, Ramesh et al 1998Ramesh et al ) between 1997Ramesh et al and 2005 and reported that the type II associated CMEs are largely accelerated before the type II bursts start. They noted that the present spatial resolution of the GRH is insufficient to precisely locate the type II bursts in low corona.…”
Section: Introductionmentioning
confidence: 99%
“…The radio data reported in the present work were obtained on 2012 January 16, 23, and 26 at 80 MHz with the Gauribidanur RAdioheliograPH (GRAPH; Ramesh et al 1998;Ramesh et al 1999aRamesh et al , 2006b in the imaging mode, and over the 85-35 MHz band with the Gauribidanur LOw frequency Solar Spectrograph (GLOSS; Ebenezer et al 2001;Ebenezer et al 2007) in the spectral mode. Both of the above instruments are located in the Gauribidanur radio observatory, 4 about 100 km north of Bangalore in India (Ramesh 2011).…”
Section: Observationsmentioning
confidence: 96%
“…The radio data were obtained with the Gauribidanur RAdioheliograPH (GRAPH; Ramesh et al (1998);Ramesh (2011)) at 80 MHz during the local meridian transit of the Crab nebula. The GRAPH is a T-shaped interferometer array with baselines ranging from ≈ 80 to ≈ 2600 meters.…”
Section: Observations: Scatter-broadened Images Of the Crab Nebulamentioning
confidence: 99%