DIOGENESS and RESIK Database

This page provides access to high resolution spectra obtained from

Diogeness and RESIK X-ray spectrometers flown on CORONAS-F satellite

 

Diogeness

Diogeness was a flat crystal scanning spectrometer and photometer. The  scanning range

of   the   spectrometer  covered  140  arcmin. The   instrument   had   four  measurement

channels. Details concerning the  crystal  used and  wavelength ranges covered are given

in Table 1.

Table 1: Diogeness crystals characteristics

 

During intense flare  spectra were  sampled about twice faster than normally (0.4 s). Two

identical  quartz crystals   were  mounted  in  the   so-called dopplerometer  configuration.

Such  arrangement  of  the  crystals   allowed  to  precisely measure expected flare related

Doppler shifts of X-ray lines. For  the  source plasma being at  rest,  the  maxima  of  lines 

scanned  in opposite  directions  would be measured  nearly simultaneously. If  any  radial 

motions  were  present,  the lines  were  off-set in time. The relative off-set can be directly

translated to the solar plasma velocities.

 

Diogeness spectrometer as seen from the crystal assembly side.

ACCESS TO Diogeness DATA ARCHIVE

RESIK

RESIK was  a bent  crystal  spectrometer designed to observe solar spectra in wavelength

range   below  6 Å.  RESIK   was   aimed  at  measuring   line  and  continuum   fluxes  for

many  lines  belonging  to  ions  with  atomic  numbers  between 14 and 30. Thin large area

crystals  wafers  (0.5 mm and 1 mm)  of  silicon  and  quartz  monocrystals  were  used  as

dispersive elements (Table 2).

 

Table 2: RESIK crystal characteristics

 http://www.cbk.pan.wroc.pl/body/publikacje/2001/Neapol/table2.gif

The wavelength  channels  of  RESIK spread over  ten  different spectral bands (including

higher order reflections). The  crystals were bent to a convex cylindrical profiles ­ since  this

geometry allows  to reduce the  overall size of  the  crystal­-detector  assembly.  There   are

 no moving  parts  (except  for the stepper motors   used   for  calibration    purposes  (Fe55)

and   no   collimator   was   used,   so   the  X-ray  radiation   of  the  entire  solar  corona

contributed to the spectra.

 

Acknowledgement. The research leading to these results has received funding from the

European Commission's Seventh Framework Programme (FP7/2007-2013) under the

 grant agreement eHeroes (project n° 284461, www.eheroes.eu).

 

 

 

 

 

RESIK spectrometer as seen from the crystal assembly side.

ACCESS TO RESIK DATA ARCHIVE