Astronomy at the University of Maryland

Maryland Solar Radio Physics Group

The Solar Radio Physics Group currently has one professorial faculty and several research scientists. Mukul Kundu is a solar radio astronomer who does solar research using large interferometers at meter, centimeter and millimeter wavelengths such as the Very Large Array (VLA), Berkeley-Illinois-Maryland Millimeter Array (BIMA), Nobeyama Radio Heliograph (NoRH), and Nancay (France) Radio Heliograph (NRH). His primary research interests are studies of quiet sun phenomena, solar active regions including sunspots, prominences and their magnetic fields, and explosive energy releases on the Sun -- solar flares and other weak coronal transients in practically all radio spectral domains from millimeter and centimeter to meter and decameter wavelengths along with spacecraft observations in X-rays, extreme ultraviolet, and ground-based H-alpha and magnetometer data.These studies are related to solar coronal heating, solar flare energy release and particle acceleration.

Gyroresonant layers in Solar corona
A figure showing the gyroresonant layers at three different frequencies, corresponding to surfaces of constant magnetic field in the corona, for an active region.
X-ray jets observed by Yohkoh telescope
Three X-ray jets observed by Yohkoh Soft X-ray telescope along with type III burst positions on the extensions of the jets marked by crosses at three frequencies.


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Mukul Kundu

Stephen White

Vladimir Garaimov

Victor Grechnev



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Department of Astronomy, University of Maryland College Park, MD 20742-2421
Phone: (301) 405-3001    FAX: (301) 314-9067

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Page updated on: 01-Sep-2006.