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C. H. Mandrini
C. H. Mandrini
Instituto de Astronomia y Fisica del Espacio
Verifierad e-postadress på iafe.uba.ar
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Quasi-Separatrix layers in solar flares. I. Method.
P Demoulin, JC Henoux, ER Priest, CH Mandrini
Astronomy and Astrophysics, v. 308, p. 643-655 308, 643-655, 1996
4541996
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
3352015
Quasi-separatrix layers in solar flares. II. Observed magnetic configurations.
P Demoulin, LG Bagala, CH Mandrini, JC Henoux, MG Rovira
Astronomy and Astrophysics, v. 325, p. 305-317 325, 305-317, 1997
3331997
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
2532002
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
2452000
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
2082006
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 676 (2), L147, 2008
2072008
Evidence for the interaction of large scale magnetic structures in solar flares
CH Mandrini, P Démoulin, JC Hénoux, ME Machado
Astronomy and Astrophysics (ISSN 0004-6361), vol. 250, no. 2, Oct. 1991, p …, 1991
1821991
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
1682005
Progressive transformation of a flux rope to an ICME: Comparative analysis using the direct and fitted expansion methods
S Dasso, MS Nakwacki, P Démoulin, CH Mandrini
Solar Physics 244, 115-137, 2007
1552007
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
1472002
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
1432004
The magnetic helicity budget of a CME-prolific active region
LM Green, MC Lopez Fuentes, CH Mandrini, P Démoulin, ...
Solar Physics 208, 43-68, 2002
1322002
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
1202009
Using the Evolution of Coronal Dimming Regions to Probe the Global Magnetic Field Topology: “Unidentical Twins”: A New Interpretation of the 12 May 1997 Event
G Attrill, MS Nakwacki, LK Harra, L van Driel-Gesztelyi, CH Mandrini, ...
Solar Physics 238, 117-139, 2006
1192006
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, 127-148, 2010
1172010
Are magnetic null points important in solar flares?
P Démoulin, JC Hénoux, CH Mandrini
Astronomy and Astrophysics, Vol. 285, p. 1023-1037 (1994) 285, 1023-1037, 1994
1161994
The magnetic helicity injected by shearing motions
P Démoulin, CH Mandrini, L van Driel-Gesztelyi, MC Lopez Fuentes, ...
Solar Physics 207, 87-110, 2002
1132002
Twisted flux tube emergence evidenced in longitudinal magnetograms: magnetic tongues
ML Luoni, P Démoulin, CH Mandrini, L van Driel-Gesztelyi
Solar Physics 270, 45-74, 2011
1072011
3D magnetic reconnection at an X-ray bright point
CH Mandrini, P Démoulin, L van Driel-Gesztelyi, B Schmieder, G Cauzzi, ...
Solar Physics 168, 115-133, 1996
1051996
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