The Heating and Activity of the Solar Corona:
1. Boundary Shearing of an Initially Homogeneous Magnetic Field
(9 Mb) (JGR, 101, 13445-13460, 1996)
The Heating and Activity of the Solar Corona:
2. Kink Instability in a Flux Tube
(27 Mb) (JGR, 102, 219-230, 1997)
The Heating and Activity of the Solar Corona:
3. Dynamics of a Low Beta Plasma with 3D Null Points
(24 Mb) (JGR, 102, 231-248, 1997)
Investigation of Numerical Avalanches in a 3D Vector Field
(A&A, 315, 312-318, 1996)
A 3D MHD Code for Parallel Computers
Energy Release Sites in Magnetic Fields
Containing Single or Multiple Nulls (11 Mb) (SP, 176, 229-325, 1997)
Are Prominences Formed by Flux
Convergence ? (In the proceedings of IAU colloquium
167, New Perspectives on Solar Prominences)
Visualization of three dimensional
datasets, Solar Physics, 181, 87-90 1998
Formation of Prominences by Flux
Convergence ApJ, 510, 444, 1999.
On the visualization of three dimensional
datasets Solar Physics, 183, 445-448, 1998
On the Location of Energy Release and
Temperature Profiles along Coronal Loops,Solar Physics,
189, 95-108, 1999.
Dynamical Investigation of 3D Reconnection in
Quasi-Separatrix Layers in a Boundary-Driven Magnetic Field,
JGR, 105, 5119, 2000.
Three-dimensional Separator Reconnection
- How Does It Occur?,
Solar Physics, 193, 1, 2000 (Monterey conference august 1999).
How Accurately Can We Determine the
Coronal Heating Mechanism in the Large-Scale Solar Corona ?,
Solar Physics, 193, 93, 2000 (Monterey conference august 1999).
Elementary Heating Events - Magnetic
Interactions Between Two Flux Sources, A&A, 2000, 362 p383-394
Evolution of a Density Enhancement in
a Stratified Atmosphere with Uniform Vertical Magnetic Field
, Solar Physics, 2001, 198, 289-312,
Modelling of Explosive Events in a 2D Environment:
Part I. General Reconnection Jet Dynamics, A&A, 2001, 370, 298
Modelling of Explosive Events in a 2D Environment:
Part II. Various MHD Experiments, A&A 2001, 375, 228-242
Modelling of Explosive Events in a 2D Environment:
Part III. Line Synthesis, A&A, 2001, 380, 719
Physical Consequences of the Inclusion of
Anomalous Resistivity in the Dynamics of 2D Magnetic Reconnection
, A&A, 2002, 382, 639-649
Magnetic reconnection in 2D stratified atmospheres:
Part I. Dynamical consequences, A&A, 2002, 383, 685
Magnetic reconnection in 2D stratified atmospheres:
Part II. Observable consequences, A&A, 2002, 383, 697
Magnetic flux interaction in a non-balanced double
source system., A&A, 2002, submitted April.
Coronal Heating by Flux Braiding
(7.4 Mb), "Solar and Astronomical Magnetohydrodynamic Flows"
Crete, Greece, June 1995 (Astro. Lett. and Communications, Vol. 34,
p 175, 1996).
Dynamical Properties of Single and Double
3D Null Points
(1.8 Mb), "Observations of Magnetic Reconnection in the Solar
Atmosphere", Bath, England, March 1996.
Double Null Points and Magnetic
Reconnection
(2.6 Mb), COSPAR 1996, Birmingham, England.
Coronal Heating by Shuffling of Foot points
(19 Mb) Mini conference in Oslo, Norway, June 1996.
Topology and MHD Interaction of 3D
Magnetic Fields
(8.5 Mb) Invited paper at the ``Themis'' meeting in Paris, France,
November 1996
3D Magnetic Reconnection
(10. Mb) Invited paper at the ``High Resolution Solar Atmospheric
Dynamics'' conference in Gloucester, MA, USA, June 1997 Never to
be published!, they have given up. February 2001
Sun Block'99: Young scientists Investigate the sun
Proceedings of the 8th SOHO Workshop "Plasma Dynamic and Diagnostics
in the solar transition region and Corona", Paris, France, 22-25 June
1999 (ESA SP-446, October 1999)
Solar magnetic fields}
NATO ASI summer school, Bucharest, August, 1999 (Invited contribution)
A Numerical Investigation of a Simple 3D
Magnetic Flux Interaction Event, Cool Star 12,
July 30th - August 3rd, 2001, Boulder, Colorado , USA
Flux Braiding In A Stratified Atmosphere,
Magnetic Coupling of the Solar Atmosphere, 11-15/6/02, Santorini, Greece,
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Last updated 10.06.02