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Dynamics in Restructuring Active Regions Observed During Soho/Yohkoh/Gbo Campaigns
(Elsevier, 2000-01)
JOP17 and JOP 33 are SOHO Joint Observing Programs in collaboration with Yohkoh/SXT and ground based observatories (GBO's), dedicated to observe dynamical events through the atmosphere. During runs of these programs we ...
Analysis of the impulsive phase of a solar flare at submillimeter wavelengths
(SpringerDordrechtHolanda, 2004)
The long-term evolution of AR 7978: Testing coronal heating models
(IOP Publishing, 2003-12)
We derive the dependence of the mean coronal heating rate on the magnetic flux density. Our results are based on a previous study of the plasma parameters and the magnetic flux density (B) in the active region NOAA 7978 ...
The long-term evolution of AR 7978: The scalings of the coronal plasma parameters with the mean photospheric magnetic field
(IOP Publishing, 2003-03-20)
We analyze the evolution of the fluxes observed in X-rays and correlate them with the magnetic flux density in active region (AR) NOAA 7978 from its birth throughout its decay, for five solar rotations. We use Solar and ...
The 3B/X3 solar flare of 27 February 1992
(Instituto de Geofísica UNAM, 2000-01)
Analizamos la evolución de la región activa (AR) NOAA 7070 y la relacionamos con una fulguración 3B/X3, ocurrida el 27 de febrero de 1992. Las observaciones en rayos X blandos fueron obtenidas por el SXT (Soft X-ray ...
The 3B/X3 solar flare of 27 February 1992The 3B/X3 solar flare of 27 February 1992
(Instituto de Geofísica, 2012)
On the relationship between magnetic field strength and loop lengths in solar coronal active regions
(Edp Sciences, 2006-12)
By assuming that coronal active regions are made up of many loops, we investigate the relationship between the average magnetic field strength and loop length for a sample of active regions observed by the Soft X-ray ...
Multiwavelength observations of the 5 January 1992 flare
(Kluwer Academic PublDordrechtHolanda, 1998)