This viewgraph presentation determines the Differential Emission Measure (DEM) from the EUV Imaging Spectrometer (EIS), X Ray Telescope (XRT), and Atmospheric Imaging Array (AIA). Common observations with Fe, Si, and Ca EIS lines are shown along with observations with Al-mesh, Ti-poly Al-thick and Be-thick XRT filters. Results from these observations are shown to determine what lines and filters are important to better constrain the hot component
The differential emission measure (DEM) of a solar active region is derived from SERTS-89 rocket dat...
Aims. We present a thorough investigation of the cool and hot temperature components in four recurri...
Aims. In previous studies, a very hot plasma component has been diagnosed in solar active ...
The Atmospheric Imaging Assembly (AIA) on board the Solar Dynamic Observatory (SDO) has been providi...
The Atmospheric Imaging Assembly (AIA) telescope on board the Solar Dynamics Observatory provides co...
We have performed a differential emission measure (DEM) analysis for a polar coronal hole observed d...
We analyze coordinated Hinode X-ray Telescope (XRT) and Extreme Ultraviolet Imaging Spectrometer (EI...
Aims: In previous studies, a very hot plasma component has been diagnosed in solar active regions th...
Aims. We investigate the possibility of modeling the active region coronal emission in the...
Aims. To demonstrate the capabilities of regularized inversion to recover differential emission meas...
We have investigated differential emission measure (DEM) distribution of hot flare plasma (T>10 MK) ...
Extreme ultraviolet (EUV) images of the optically-thin solar corona in multiple spectral channels gi...
The X-Ray Telescope (XRT) on the Japanese/USA/UK Hinode (Solar-B) spacecraft has detected emission f...
Aims. We present a study of a recurring jet observed on October 31, 2011 by the Atmosphereic Imaging...
Context. The non-Maxwellian κ-distributions have been detected in the solar wind and can explain int...
The differential emission measure (DEM) of a solar active region is derived from SERTS-89 rocket dat...
Aims. We present a thorough investigation of the cool and hot temperature components in four recurri...
Aims. In previous studies, a very hot plasma component has been diagnosed in solar active ...
The Atmospheric Imaging Assembly (AIA) on board the Solar Dynamic Observatory (SDO) has been providi...
The Atmospheric Imaging Assembly (AIA) telescope on board the Solar Dynamics Observatory provides co...
We have performed a differential emission measure (DEM) analysis for a polar coronal hole observed d...
We analyze coordinated Hinode X-ray Telescope (XRT) and Extreme Ultraviolet Imaging Spectrometer (EI...
Aims: In previous studies, a very hot plasma component has been diagnosed in solar active regions th...
Aims. We investigate the possibility of modeling the active region coronal emission in the...
Aims. To demonstrate the capabilities of regularized inversion to recover differential emission meas...
We have investigated differential emission measure (DEM) distribution of hot flare plasma (T>10 MK) ...
Extreme ultraviolet (EUV) images of the optically-thin solar corona in multiple spectral channels gi...
The X-Ray Telescope (XRT) on the Japanese/USA/UK Hinode (Solar-B) spacecraft has detected emission f...
Aims. We present a study of a recurring jet observed on October 31, 2011 by the Atmosphereic Imaging...
Context. The non-Maxwellian κ-distributions have been detected in the solar wind and can explain int...
The differential emission measure (DEM) of a solar active region is derived from SERTS-89 rocket dat...
Aims. We present a thorough investigation of the cool and hot temperature components in four recurri...
Aims. In previous studies, a very hot plasma component has been diagnosed in solar active ...