152 citations · 319 across the 7 of their papers we have counts for
7 papers
Ten Years of the Solar Radiospectrograph ARTEMIS-IV
C. Caroubalos, C. E. Alissandrakis, A. Hillaris +10
The Solar Radiospectrograph of the University of Athens (ARTEMIS-IV) is in operation at the Thermopylae Satellite Communication Station since 1996. The observations extend from the…
ARTEMIS IV Radio Observations of the 14 July 2000 Large Solar Event
C. Caroubalos, C. E. Alissandrakis, A. Hillaris +13
In this report we present a complex metric burst, associated with the 14 July 2000 major solar event, recorded by the ARTEMIS-IV radio spectrograph at Thermopylae. Additional space…
Solar flares with and without SOHO/LASCO coronal mass ejections and type II shocks
A. Hillaris, V. Petousis, E. Mitsakou +10
We analyse of a set of radio rich (accompanied by type IV or II bursts) solar flares and their association with SOHO/LASCO Coronal Mass Ejections in the period 1998 2000. The inten…
Interplanetary shocks lacking type II radio bursts
N. Gopalswamy, H. Xie, P. Makela +5
We report on the radio-emission characteristics of 222 interplanetary (IP) shocks. A surprisingly large fraction of the IP shocks (~34%) is radio quiet (i.e., the shocks lacked typ…
On the Brightness and Waiting-time Distributions of a Type III Radio Storm observed by STEREO/WAVES
J. P. Eastwood, M. S. Wheatland, H. S. Hudson +5
Type III solar radio storms, observed at frequencies below approximately 16 MHz by space borne radio experiments, correspond to the quasi-continuous, bursty emission of electron be…
Dust detection by the wave instrument on STEREO: nanoparticles picked up by the solar wind?
N. Meyer-Vernet, M. Maksimovic, A. Czechowski +7
The STEREO/WAVES instrument has detected a very large number of intense voltage pulses. We suggest that these events are produced by impact ionisation of nanoparticles striking the…
Space VLBI at Low Frequencies
D. Jones, R. Allen, J. Basart +25
At sufficiently low frequencies, no ground-based radio array will be able to produce high resolution images while looking through the ionosphere. A space-based array will be needed…