C. H. Mandrini
C. H. Mandrini
Instituto de Astronomia y Fisica del Espacio
Verified email at iafe.uba.ar
Cited by
Cited by
Quasi-Separatrix layers in solar flares. I. Method.
P Demoulin, JC Henoux, ER Priest, CH Mandrini
Astronomy and Astrophysics 308, 643-655, 1996
A companion to AB Pic at the planet/brown dwarf boundary
G Chauvin, AM Lagrange, B Zuckerman, C Dumas, D Mouillet, I Song, ...
Astronomy & Astrophysics 438 (3), L29-L32, 2005
Quasi-separatrix layers in solar flares. II. Observed magnetic configurations.
P Demoulin, LG Bagala, CH Mandrini, JC Henoux, MG Rovira
Astronomy and Astrophysics 325, 305-317, 1997
What is the source of the magnetic helicity shed by CMEs? The long-term helicity budget of AR 7978
P Démoulin, CH Mandrini, L van Driel-Gesztelyi, BJ Thompson, S Plunkett, ...
Astronomy & Astrophysics 382 (2), 650-665, 2002
The SOHO mission
B Fleck
Coronal Magnetic Energy Releases, 233-244, 1995
Magnetic field and plasma scaling laws: their implications for coronal heating models
CH Mandrini, P Démoulin, JA Klimchuk
The Astrophysical Journal 530 (2), 999, 2000
Evidence for the interaction of large scale magnetic structures in solar flares
CH Mandrini, P Démoulin, JC Hénoux, ME Machado
Astronomy and Astrophysics 250, 541-547, 1991
Understanding space weather to shield society: A global road map for 2015–2025 commissioned by COSPAR and ILWS
CJ Schrijver, K Kauristie, AD Aylward, CM Denardini, SE Gibson, A Glover, ...
Advances in Space Research 55 (12), 2745-2807, 2015
Outflows at the edges of active regions: contribution to solar wind formation?
LK Harra, T Sakao, CH Mandrini, H Hara, S Imada, PR Young, ...
The Astrophysical Journal Letters 676 (2), L147, 2008
Interplanetary flux rope ejected from an X-ray bright point-The smallest magnetic cloud source-region ever observed
CH Mandrini, S Pohjolainen, S Dasso, LM Green, P Démoulin, ...
Astronomy & Astrophysics 434 (2), 725-740, 2005
A new model-independent method to compute magnetic helicity in magnetic clouds
S Dasso, CH Mandrini, P Démoulin, ML Luoni
Astronomy & Astrophysics 455 (1), 349-359, 2006
Observational consequences of a magnetic flux rope emerging into the corona
SE Gibson, Y Fan, C Mandrini, G Fisher, P Démoulin
The Astrophysical Journal 617 (1), 600, 2004
The structure and evolution of a sigmoidal active region
SE Gibson, L Fletcher, G Del Zanna, CD Pike, HE Mason, CH Mandrini, ...
The Astrophysical Journal 574 (2), 1021, 2002
Progressive transformation of a flux rope to an ICME
S Dasso, MS Nakwacki, P Démoulin, CH Mandrini
Solar Physics 244 (1-2), 115-137, 2007
Are magnetic null points important in solar flares?
P Démoulin, JC Hénoux, CH Mandrini
Astronomy and Astrophysics 285, 1023-1037, 1994
How can a negative magnetic helicity active region generate a positive helicity magnetic cloud?
R Chandra, E Pariat, B Schmieder, CH Mandrini, W Uddin
Solar Physics 261 (1), 127-148, 2010
The magnetic helicity budget of a CME-prolific active region
LM Green, CH Mandrini, P Démoulin, L Van Driel-Gesztelyi, JL Culhane
Solar Physics 208 (1), 43-68, 2002
Using the evolution of coronal dimming regions to probe the global magnetic field topology
G Attrill, MS Nakwacki, LK Harra, L Van Driel-Gesztelyi, CH Mandrini, ...
Solar Physics 238 (1), 117-139, 2006
The magnetic helicity injected by shearing motions
P Démoulin, CH Mandrini, L Van Driel-Gesztelyi, MCL Fuentes, ...
Solar Physics 207 (1), 87-110, 2002
Magnetic reconnection along quasi-separatrix layers as a driver of ubiquitous active region outflows
D Baker, L van Driel-Gesztelyi, CH Mandrini, P Démoulin, MJ Murray
The Astrophysical Journal 705 (1), 926, 2009
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