Solar Flares and Active Regions
Reconstructing the 3D Reality

Models gallery

SOL2001-08-25T16:23

SOL2002-04-12

This video shows time evolution of the cloud of nonthermal electrons trapped in the flaring loop found by minimizing residuals between the model and observed radio spectrum. The spectral sequence and residuals are shown in separate panels as well as the microwave dynamic spectrum shown for the reference.

SOL2015-06-22

AR 11236

In the the following figures the modeled data are denoted by colour, the observed data are marked with contour lines.

2011-06-17
2011-06-18
2011-06-19
2011-06-20
2011-06-21
2011-06-22
2011-06-23
2011-06-24

AR 11476

In the the following figures the modeled data are denoted by colour, the observed data are marked with contour lines.

2012-05-08
2012-05-09
2012-05-10
2012-05-11
2012-05-12
2012-05-13
2012-05-14
2012-05-15

AR 11515

In the the following figures the modeled data are denoted by colour, the observed data are marked with contour lines.

2012-06-30
2012-07-01
2012-07-02
2012-07-03
2012-07-04
2012-07-05
2012-07-06
2012-07-07

AR 11520

In the the following figures the modeled data are denoted by colour, the observed data are marked with contour lines.

2012-07-09
2012-07-10
2012-07-11
2012-07-12
2012-07-13
2012-07-14
2012-07-15
2012-07-16

AR 11809

AR11809 EUV AIA convolved 1 2
AR11809 radio convolved 50
AR11809 radio V convolved 50

AR 12158 (2014-09-10)

EUV AR12158 with chromo Corona EBTEL
EUV AR12158 with chromo Corona SteadyHeating
Radio AR12158 with chromo Corona SteadyHeating
Radio P AR12158 with chromo Corona EBTEL
Radio TI AR12158 with chromo Corona EBTEL
AR12158 EUV 94 EBTEL
AR12158 EUV 94 steady
AR12158 Radio 110GHz EBTEL
AR12158 Radio 110GHz steady
Website supervisor: Anastasia Tsvetkova
Page last updated: 21 Apr 2020